Package 'RandomFields'

Title: Simulation and Analysis of Random Fields
Description: Methods for the inference on and the simulation of Gaussian fields are provided. Furthermore, methods for the simulation of extreme value random fields are provided. Main geostatistical parts are based among others on the books by Christian Lantuejoul <doi:10.1007/978-3-662-04808-5>.
Authors: Martin Schlather [aut, cre], Alexander Malinowski [aut], Marco Oesting [aut], Daphne Boecker [aut], Kirstin Strokorb [aut], Sebastian Engelke [aut], Johannes Martini [aut], Felix Ballani [aut], Olga Moreva [aut], Jonas Auel[ctr], Peter Menck [ctr], Sebastian Gross [ctr], Ulrike Ober [ctb], Paulo Ribeiro [ctb], Brian D. Ripley [ctb], Richard Singleton [ctb], Ben Pfaff [ctb], R Core Team [ctb]
Maintainer: Martin Schlather <[email protected]>
License: GPL (>= 3)
Version: 3.3.14
Built: 2024-12-05 04:57:24 UTC
Source: https://github.com/cran/RandomFields

Help Index


Simulation and Analysis of Random Fields

Description

The package RandomFields offers various tools for

  1. model estimation (ML) and inference (tests) for regionalized variables and data analysis,

  2. simulation of different kinds of random fields, including

    • multivariate, spatial, spatio-temporal, and non-stationary Gaussian random fields,

    • Poisson fields, binary fields, Chi2 fields, t fields and

    • max-stable fields.

    It can also deal with non-stationarity and anisotropy of these processes and conditional simulation (for Gaussian random fields, currently).

See https://www.wim.uni-mannheim.de/schlather/publications/software for intermediate updates.

Details

The following features are provided by the package:

  1. Bayesian Modelling

  2. Coordinate systems

  3. Data and example studies: Some data sets and published code are provided to illustrate the syntax and structure of the package functions.

    • soil : soil physical data

    • weather : UWME weather data

    • papers : code used in the papers published by the author(s)

  4. Estimation of parameters (for second-order random fields)

    • RFfit : general function for estimating parameters; (for Gaussian random fields)

    • RFhurst : estimation of the Hurst parameter

    • RFfractaldim : estimation of the fractal dimension

    • RFvariogram : calculates the empirical variogram

    • RFcov : calculates the empirical (auto-)covariance function

  5. Graphics

    • Fitting a covariance function manually RFgui

    • the generic function plot

    • global graphical parameters with RFpar

  6. Inference (for Gaussian random fields)

  7. Models

    • For an introduction and general properties, see RMmodels.

    • For an overview over classes of covariance and variogram models –e.g. for geostatistical purposes– see RM. More sophisticated models and covariance function operators are included.

    • RFformula reports a new style of passing a model since version 3.3.

    • definite models are evaluated by RFcov, RFvariogram and RFcovmatrix. For a quick impression use plot(model).

    • non-definite models are evaluated by RFfctn and RFcalc

    • RFlinearpart returns the linear part of a model

    • RFboxcox deals explicitly with Box-Cox transformations. In many cases it is performed implicitly.

  8. Prediction (for second-order random fields)

  9. Simulation

    • RFsimulate: Simulation of random fields, including conditional simulation. For a list of all covariance functions and variogram models see RM. Use plot for visualisation of the result.

  10. S3 and S4 objects

    • The functions return S4 objects based on the package sp, if spConform=TRUE. This is the default.

      If spConform=FALSE, simple objects as in version 2 are returned. These simple objects are frequently provided with an S3 class. This option makes the returning procedure much faster, but currently does not allow for the comfortable use of plot.

    • plot, print, summary, sometimes also str recognise these S3 and S4 objects

    • use sp2RF for an explicit transformation of sp objects to S4 objects of RandomFields.

    • Further generic functions are available for fitted models, see ‘Inference’ above.

  11. Xtended features, especially for package programmers

    • might decide on a large variety of arguments of the simulation and estimation procedures using the function RFoptions

    • may use ‘./configure –with-tcl-config=/usr/lib/tcl8.5/tclConfig.sh –with-tk-config=/usr/lib/tk8.5/tkConfig.sh’ to configure R

Changings

A list of major changings from Version 2 to Version 3 can be found in MajorRevisions.

Changings lists some further changings, in particular of argument and argument names.

RandomFields should be rather stable when running it with parallel. However RandomFields might crash severely if an error occurs when running in parallel. When used with parallel, you might set RFoptions(cores = 1). Note that RFoptions(cores = ...) with more than 1 core uses another level of parallelism which will be in competetions with parallel during runtime.

Update

Current updates are available through https://www.wim.uni-mannheim.de/schlather/publications/software.

Contributions

  • Contributions to version 3.0 and following:
    Felix Ballani (TU Bergakademie Freiberg; Poisson Polygons, 2014)
    Daphne Boecker (Univ. Goettingen; RFgui, 2011)
    Katharina Burmeister (Univ. Goettingen; testing, 2012)
    Sebastian Engelke (Univ. Goettingen; RFvariogram, 2011-12)
    Sebastian Gross (Univ. Goettingen; tilde formulae, 2011)
    Alexander Malinowski (Univ. Mannheim; S3, S4 classes 2011-13)
    Juliane Manitz (Univ. Goettingen; testing, 2012)
    Johannes Martini (Univ. Goettingen; RFvariogram, 2011-12)
    Ulrike Ober (Univ. Goettingen; help pages, testing, 2011-12)
    Marco Oesting (Univ. Mannheim; Brown-Resnick processes, Kriging, Trend, 2011-13)
    Paulo Ribeiro (Unversidade Federal do Parana; code adopted from geoR, 2014)
    Kirstin Strokorb (Univ. Mannheim; help pages, 2011-13)

  • Contributions to version 2.0 and following:
    Peter Menck (Univ. Goettingen; multivariate circulant embedding)
    R Core Team, Richard Singleton (fft.c and advice)

  • Contributions to version 1 and following:
    Ben Pfaff, 12167 Airport Rd, DeWitt MI 48820, USA making available an algorithm for AVL trees (avltr*)

Thanks

Patrick Brown : comments on Version 3
Paulo Ribeiro : comments on Version 1
Martin Maechler : advice for Version 1

Financial support

  • V3.0 has been financially supported by the German Science Foundation (DFG) through the Research Training Group 1953 ‘Statistical Modeling of Complex Systems and Processes — Advanced Nonparametric Approaches’ (2013-2018).

  • V3.0 has been financially supported by Volkswagen Stiftung within the project ‘WEX-MOP’ (2011-2014).

  • Alpha versions for V3.0 have been financially supported by the German Science Foundation (DFG) through the Research Training Groups 1644 ‘Scaling problems in Statistics’ and 1023 ‘Identification in Mathematical Models’ (2008-13).

  • V1.0 has been financially supported by the German Federal Ministry of Research and Technology (BMFT) grant PT BEO 51-0339476C during 2000-03.

  • V1.0 has been financially supported by the EU TMR network ERB-FMRX-CT96-0095 on “Computational and statistical methods for the analysis of spatial data” in 1999.

Note

The following packages enable further choices for the optimizer (instead of optim) in RandomFields: optimx, soma, GenSA, minqa, pso, DEoptim, nloptr, RColorBrewer, colorspace

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Singleton, R.C. (1979). In Programs for Digital Signal Processing Ed.: Digital Signal Processing Committee and IEEE Acoustics, Speech, and Signal Processing Committe (1979) IEEE press.

  • Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’

  • see also the corresponding vignette.

See Also

See also RF, RM, RP, RR, RC, R.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

# simulate some data first (Gaussian random field with exponential
# covariance; 6 realisations)
model <- RMexp()
x <- seq(0, 10, 0.1)
z <- RFsimulate(model, x, x, n=6)

## select some data from the simulated data
xy <- coordinates(z)
pts <- sample(nrow(xy), min(100, nrow(xy) / 2))
dta <- matrix(nrow=nrow(xy), as.vector(z))[pts, ]
dta <- cbind(xy[pts, ], dta)
plot(z, dta)


## re-estimate the parameter (true values are 1)
estmodel <- RMexp(var=NA, scale=NA)
(fit <- RFfit(estmodel, data=dta))

## show a kriged field based on the estimated parameters
kriged <- RFinterpolate(fit, x, x, data=dta)
plot(kriged, dta)

Simulation methods for Brown-Resnick processes

Description

These models define particular ways to simulate Brown-Resnick processes.

Usage

RPbrmixed(phi, tcf, xi, mu, s, meshsize, vertnumber, optim_mixed,
          optim_mixed_tol,lambda, areamat, variobound) 

RPbrorig(phi, tcf, xi, mu, s)

RPbrshifted(phi, tcf, xi, mu, s)

RPloggaussnormed(variogram, prob, optimize_p, nth, burn.in, rejection)

Arguments

phi, variogram

object of class RMmodel; specifies the covariance model to be simulated.

tcf

the extremal correlation function; either phi or tcf must be given.

xi, mu, s

the shape parameter, the location parameter and the scale parameter, respectively, of the generalized extreme value distribution. See Details.

lambda

positive constant factor in the intensity of the Poisson point process used in the M3 representation, cf. Thm. 6 and Remark 7 in Oesting et. al (2012); can be estimated by setting optim_mixed if unknown. Default value is 1.

areamat

vector of values in [0,1][0,1]. The value of the kkth component represents the portion of processes whose maximum is located at a distance dd with k1d<kk-1 \leq d < k from the origin taken into account for the simulation of the shape function in the M3 representation. areamat can be used for isotropic models only; can be optimized by setting optim_mixed if unknown. Default value is 1.

meshsize, vertnumber, optim_mixed, optim_mixed_tol, variobound

further arguments for simulation via the mixed moving maxima (M3) representation; see RFoptions.

prob

to do

optimize_p

to do

nth

to do

burn.in

to do

rejection

to do

Details

The argument xi is always a number, i.e. ξ\xi is constant in space. In contrast, μ\mu and ss might be constant numerical values or given an RMmodel, in particular by an RMtrend model.

The functions RPbrorig, RPbrshifted and RPbrmixed simulate a Brown-Resnick process, which is defined by

Z(x)=maxi=1Xiexp(Wi(x)γ),Z(x) = \max_{i=1}^\infty X_i \exp(W_i(x) - \gamma),

where the XiX_i are the points of a Poisson point process on the positive real half-axis with intensity x2dxx^{-2} dx, WiWW_i \sim W are iid centered Gaussian processes with stationary increments and variogram γ\gamma given by model. The functions correspond to the following ways of simulation:

RPbrorig

simulation using the original definition (method 0 in Oesting et al., 2012)

RPbrshifted

simulation using a random shift (similar to method 1 and 2)

RPbrmixed

simulation using M3 representation (method 4)

Value

The functions return an object of class RMmodel.

Note

Advanced options for RPbroriginal and RPbrshifted are maxpoints and max_gauss, see RFoptions.

Author(s)

Marco Oesting, [email protected], https://www.isa.uni-stuttgart.de/institut/team/Oesting/; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Oesting, M., Kabluchko, Z. and Schlather M. (2012) Simulation of Brown-Resnick Processes, Extremes, 15, 89-107.

See Also

RPbrownresnick, RMmodel, RPgauss, maxstable, maxstableAdvanced.

Examples

#
RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## currently does not work

Brown-Resnick process

Description

RPbrownresnick defines a Brown-Resnick process.

Usage

RPbrownresnick(phi, tcf, xi, mu, s)

Arguments

phi

specifies the covariance model or variogram, see RMmodel and RMmodelsAdvanced.

tcf

the extremal correlation function; either phi or tcf must be given.

xi, mu, s

the extreme value index, the location parameter and the scale parameter, respectively, of the generalized extreme value distribution. See Details.

Details

The argument xi is always a number, i.e. ξ\xi is constant in space. In contrast, μ\mu and ss might be constant numerical values or (in future!) be given by an RMmodel, in particular by an RMtrend model.
For xi=0xi=0, the default values of mumu and ss are 00 and 11, respectively. For xi0xi\not=0, the default values of mumu and ss are 11 and ξ|\xi|, respectively, so that it defaults to the standard Frechet case if ξ>0\xi > 0.

The functions RPbrorig, RPbrshifted and RPbrmixed perform the simulation of a Brown-Resnick process, which is defined by

Z(x)=maxi=1Xiexp(Wi(x)γ2),Z(x) = \max_{i=1}^\infty X_i \exp(W_i(x) - \gamma^2),

where the XiX_i are the points of a Poisson point process on the positive real half-axis with intensity x2dxx^{-2} dx, WiWW_i \sim W are iid centered Gaussian processes with stationary increments and variogram γ\gamma given by phi.

For simulation, internally, one of the methods RPbrorig, RPbrshifted and RPbrmixed is chosen automatically.

Note

Advanced options are maxpoints and max_gauss, see RFoptions.

Further advanced options related to the simulation methods RPbrorig, RPbrshifted and RPbrmixed can be found in the paragraph ‘Specific method options for Brown-Resnick Fields’ in RFoptions.

Author(s)

Marco Oesting, [email protected], https://www.isa.uni-stuttgart.de/institut/team/Oesting/; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Brown, B.M. and Resnick, S.I. (1977). Extreme values of independent stochastic processes. J. Appl. Probab. 14, 732-739.

  • Buishand, T., de Haan , L. and Zhou, C. (2008). On spatial extremes: With application to a rainfall problem. Ann. Appl. Stat. 2, 624-642.

  • Kabluchko, Z., Schlather, M. and de Haan, L (2009) Stationary max-stable random fields associated to negative definite functions Ann. Probab. 37, 2042-2065.

  • Oesting, M., Kabluchko, Z. and Schlather M. (2012) Simulation of Brown-Resnick Processes, Extremes, 15, 89-107.

See Also

RPbrorig, RPbrshifted, RPbrmixed, RMmodel, RPgauss, maxstable, maxstableAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


## for some more sophisticated models see 'maxstableAdvanced'

Calcium content in soil samples

Description

This data set contains the calcium content measured in soil samples taken from the 0-20cm layer at 178 locations within a certain study area divided in three sub-areas. The elevation at each location was also recorded.

The first region is typically flooded during the rain season and not used as an experimental area. The calcium levels would represent the natural content in the region. The second region has received fertilisers a while ago and is typically occupied by rice fields. The third region has received fertilisers recently and is frequently used as an experimental area.

Usage

data(ca20)

Format

The object ca20 belongs to the class geodata and is a list with the following elements:

coords

a matrix with the coordinates of the soil samples.

data

calcium content measured in mmolc/dm3mmol_c/dm^3.

covariate

a data-frame with the covariates

altitude

a vector with the elevation of each sampling location, in meters (mm).

area

a factor indicating the sub area to which the locations belongs.

borders

a matrix with the coordinates defining the borders of the area.

reg1

a matrix with the coordinates of the limits of the sub-area 1.

reg1

a matrix with the coordinates of the limits of the sub-area 2.

reg1

a matrix with the coordinates of the limits of the sub-area 3.

Source

The data was collected by researchers from PESAGRO and EMBRAPA-Solos, Rio de Janeiro, Brasil and provided by Dra. Maria Cristina Neves de Oliveira.

Capeche, C.L.; Macedo, J.R.; Manzatto, H.R.H.; Silva, E.F. (1997) Caracterização pedológica da fazenda Angra - PESAGRO/RIO - Estação experimental de Campos (RJ). (compact disc). In: Congresso BRASILEIRO de Ciência do Solo. 26., Informação, globalização, uso do solo; Rio de Janeiro, 1997. trabalhos. Rio de Janeiro: Embrapa/SBCS.

References

Oliveira, M.C.N. (2003) Métodos de estimação de parâmetros em modelos geoestatísticos com diferentes estruturas de covariâncias: uma aplicação ao teor de cálcio no solo. Tese de Doutorado, ESALQ/USP/Brasil.

Further information on the package geoR can be found at:
http://www.leg.ufpr.br/geoR/.


Documentation of some further changings

Description

  • Version 3.3

    • RFempiricalvariogram, RFempiricalcovariance and RFempiricalmadogram became obsolete. Use RFvariogram, RFcov, RFmadogram instead.

    • RFoptions(grDefault=FALSE) returns to the old style of graphical device handling. Otherwise there is no handling.

    • C code is started to be parallelized.

    • Some new Multivariate RMmodels

    • New way of passing models, see RFformula, which allows connections (formulae) between parameters, e.g. one parameter value might be twice as large as another parameter value. Also dummy variables can be RMdeclared.

  • Options getting obsolete (Version 3 and older)

    • oldstyle is becoming warn_oldstyle

    • newstyle is becoming warn_newstyle

    • newAniso is becoming warn_newAniso

    • ambiguous is becoming warn_ambiguous

    • normal_mode is becoming warn_normal_mode

    • colour_palette is becoming warn_colour_palette

  • Changings in option names

    • several changes in RFoptions()$graphics in version 3.1.11

    • pdfnumber became in version 3.0.42 filenumber

    • pdfonefile became in version 3.0.42 onefile

    • pdffile became in version 3.0.42 file

    • tbmdim became in version 3.0.41 reduceddim

    • coord_units became in version 3.0.39 coordunits

    • new_coord_units became in version 3.0.39 new_coordunits

    • variab_units became in version 3.0.39 varunits

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

MajorRevisions, RandomFields.

Examples

## no examples given

Circulant Embedding methods

Description

Circulant embedding is a fast simulation method for stationary (possibly anisotropic) Gaussian random fields on regular grids based on Fourier transformations. It is guaranteed to be an exact method for covariance functions with finite support, e.g. the spherical model. The method is admissible for any dimension apart from memory restrictions.
The simulation is performed on a torus which represents the bended grid. To remove wrong dependencies occuring at different borders of the grid which would be close on the torus, the simulation area is multiplied by a natural number. There is also a multivariate version of circulant embedding.

Cut-off embedding is a fast simulation method for stationary, isotropic Gaussian random fields on square lattices based on the standard RPcirculant method, so that exact simulation is garantueed for further covariance models, e.g. the RMwhittle model.

In fact, the circulant embedding is called with the cutoff hypermodel, see RMcutoff. Cutoff halfens the maximum number of elements models used to define the covariance function of interest (from 10 to 5).

Here, multiplicative models are not allowed (yet).
For details see RMcutoff.

Intrinsic embedding is a fast simulation method for intrinsically stationary, isotropic Gaussian random fields on square lattices based on the standard RPcirculant method, for further variogram models, e.g. RMfbm.

Note that the simulated random field is always non-stationary. In fact, the circulant embedding is called with the Intrinsic hypermodel, see RMintrinsic.

Here, multiplicative models are not allowed (yet).
For details see RMintrinsic.

Usage

RPcirculant(phi, boxcox, force, mmin, strategy,
 maxGB, maxmem,  tolIm, tolRe, trials, useprimes, dependent,
 approx_step, approx_maxgrid)

RPcutoff(phi, boxcox, force, mmin, strategy,
 maxGB, maxmem, tolIm, tolRe, trials, useprimes, dependent,
 approx_step, approx_maxgrid, diameter, a) 
 

RPintrinsic(phi, boxcox, force, mmin, strategy,
 maxGB, maxmem, tolIm, tolRe, trials, useprimes, dependent,
 approx_step, approx_maxgrid, diameter, rawR)

Arguments

phi

See RPgauss.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

force

Logical. Circulant embedding does not work if the constructed circulant matrix has negative eigenvalues. Sometimes it is convenient to replace all the negative eigenvalues by zero (force=TRUE) after trials number of trials. Default: FALSE.

mmin

Scalar or vector, integer if positive. CE.mmin determines the initial size of the circulant matrix. If CE.mmin=0 the minimal starting size is determined automatically according to the dimensions of the grid. If CE.mmin>0 then the absolute starting size is given. If CE.mmin<0 then the automatically determined matrix size is multiplied by CE.mmin|\code{CE.mmin}|; here, CE.mmin must be smaller than -1; the value -1 takes over the minimal starting size.
Note: in any cases, the initial size might be increased according to CE.useprimes.
Default: 0.

strategy

Logical. 0: If the circulant matrix has negative eigenvalues then the size in each direction is doubled;
1: The size is enhanced only in one direction, namely that one where the covariance function has the largest value at the end point of the grid — note that the default value of trials is probably too small in that case.

In some cases strategy=0 works better, in other cases strategy=1. Just try. Clearly, if the field is isotropic and a square grid should be simulated, then strategy=0 is the better choice.

Default: 0.

maxGB

Maximal memory used for the circulant matrix in units of GB. If this argument is set then maxmem is set to MAXINT.

Default: 1.

maxmem

Integer. maximal number of entries in a row of the circulant matrix. The total amount of memory needed for the internal calculations is 32 (= 4 * sizeof(double)) time as large (factor 2 is needed as complex numbers must be considered for calculating the fft of the covariance matrix; another factor 2 is needed for storing the simulated result).

The value of maxmem must be at least 2d2^d times as large as the number of points to be simulated. Here, dd is the space dimension. In some cases even much larger.

Note that maxmem can be used to control the automatic choice of the simulation algorithm. Namely, in case of huge circulant matrices, other simulation methods (TBM) might be faster and might be preferred by the user.

If this argument is set then maxGB is set to Inf.

Default: MAXINT.

tolIm

If the modulus of the imaginary part is less than tolIm then the eigenvalue is always considered as real (independently of the value of force).

Default: 1E-3.

tolRe

Eigenvalues between tolRe and 0 are always considered as 0 and set 0 (independently of the value of force).

Default: -1E-7.

trials

Integer. A larger circulant matrix is likely to make more eigenvalues non-negative. If at least one of the thresholds tolRe and tolIm are missed then the matrix size is doubled according to strategy, and the matrix is checked again. This procedure is repeated up to trials - 1 times. If there are still negative eigenvalues, the simulation method fails if force=FALSE.

Default: 3.

useprimes

Logical. If FALSE the columns of the circulant matrix have length 2k2^k for some kk. Otherwise the algorithm tries to find a nicely factorizable number close to the size of the given matrix.

Default: TRUE.

dependent

Logical. If FALSE then independent random fields are created. If TRUE then at least 4 non-overlapping rectangles are taken out of the the expanded grid defined by the circulant matrix. These simulations are dependent. See RFoptionsAdvanced for an example. See trials for some more information on the circulant matrix.

Default: FALSE.

approx_step

Real value. It gives the grid size of the approximating grid in case circulant embedding is used although the points do not lie on a grid.

If NA then approx_step is chosen such that approx_maxgrid is nearly reached.

Default: NA.

approx_maxgrid

It defaults to maxmem.

diameter

See RMcutoff or RMintrinsic.

a

See RMcutoff.

rawR

See RMintrinsic.

Details

Here, the algorithms by Dietrich and Newsam are implemented.

Value

An object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Circulant Embedding

  • Chan, G. and Wood, A.T.A. (1997) An Algorithm for Simulating Stationary Gaussian Random Fields. Journal of the Royal Statistical Society: Series C (Applied Statistics), 46, 171–181.

  • Dietrich, C. R. and G. N. Newsam (1993) A fast and exact method for multidimensional gaussian stochastic simulations. Water Resour. Res. 29(8), 2861–2869.

  • Dietrich, C. R. and G. N. Newsam (1996) A fast and exact method for multidimensional Gaussian stochastic simulations: Extension to realizations conditioned on direct and indirect measurements Water Resour. Res. 32(6), 1643–1652.

  • Dietrich, C. R. and Newsam, G. N. (1997) Fast and Exact Simulation of Stationary Gaussian Processes through Circulant Embedding of the Covariance Matrix. SIAM J. Sci. Comput. 18, 1088–1107.

  • Wood, A. T. A. and Chan, G. (1994) Simulation of Stationary Gaussian Processes in [0,1]d[0, 1]^d. Journal of Computational and Graphical Statistics 3, 409–432.

Cutoff and Intrinsic

  • Gneiting, T., Sevecikova, H, Percival, D.B., Schlather M., Jiang Y. (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in $R^2$: Exploring the Limits. J. Comput. Graph. Stat. 15, 483–501.

  • Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599

See Also

Gaussian, RP

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMstable(s=1, alpha=1.8)
x <- seq(-3,3,0.1)

z <- RFsimulate(model=RPcirculant(model), x=x, y=x, n=1)
plot(z)

model <- RMexp(var=10, s=2)
z <- RFsimulate(model=RPcirculant(model), 1:10)
plot(z)

model <- RMfbm(Aniso=diag(c(1,2)), alpha=1.5)
z <- RFsimulate(model, x=1:10, y=1:10)
plot(z)

Random coin method

Description

The random coin method (or dilution method) is a simulation method for stationary Gaussian random fields. It is based on the following procedure: For a stationary Poisson point process on Rd{\bf R}^d consider the random field

Y(y)=xXf(yx)Y(y) = \sum_{x\in X} f(y-x)

for a function ff. The covariance of YY is proportional to the convolution

C(h)=f(x)f(x+h)dxC(h) = \int f(x)f(x+h) dx

If the intensity of the Poisson point process increases, the random field YY approaches a Gaussian random field with covariance function CC.

Usage

RPcoins(phi, shape, boxcox, intensity, method) 

RPaverage(phi, shape, boxcox, intensity, method)

Arguments

phi

object of class RMmodel; specifies the covariance function of the Poisson process; either phi or shape must be given.

shape

object of class RMmodel; specifies the function which is attached to the Poisson points; note that this is not the covariance function of the simulated random field.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

intensity

positive number, intensity of the underlying Poisson point process.

method

integer. Default is the value 0 which addresses the current standard procedure. There might be further methods implemented mainly for internal purposes.

Value

RPcoins returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Lantuejoul, C. (2002) Geostatistical Simulation: Models and Algorithms. Springer.

See Also

Gaussian, RP, RPhyperplane, RPspectral, RPtbm.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Constants used in RandomFields (RC constants)

Description

Several constants are provided that might make the use of some functions easier, e.g. RFgetModelNames.

Value

RC_TYPE_NAMES = c( "tail correlation", "positive definite", "variogram", "negative definite", "point-shape function", "shape function", "trend", "distribution or shape", "of manifold type", "process", "method for Gauss process", "normed process (non-negative values with maximum value being 0 or 1)", "method for Brown-Resnick process", "Smith", "Schlather", "Poisson", "PoissonGauss", "distribution family", "interface", "mathematical operator", "other type")

RC_DOMAIN_NAMES = c("single variable", "kernel", "framework dependent", "submodel dependent", "parameter dependent", "<keep copy>", "mismatch")

RC_ISO_NAMES = c("isotropic", "space-isotropic", "vector-isotropic", "symmetric", "cartesian system", "gnomonic projection", "orthographic projection", "spherical isotropic", "spherical symmetric", "spherical system", "earth isotropic", "earth symmetric", "earth system", "cylinder system", "non-dimension-reducing", "framework dependent", "submodel dependent", "parameter dependent", "<internal keep copy>", "<mismatch>")

RC_MONOTONE_NAMES = c( "not set", "mismatch in monotonicity", "submodel dependent monotonicity", "previous model dependent monotonicity", "parameter dependent monotonicity", "not monotone", "monotone", "Gneiting-Schaback class", "normal mixture", "completely monotone", "Bernstein")

RC_ISOTROPIC gives the numerical code for option "isotropic"

RC_DOUBLEISOTROPIC gives the numerical code for option "space-isotropic"

RC_CARTESIAN_COORD gives the numerical code for option "cartesian system"

RC_GNOMONIC_PROJ gives the numerical code for the gnomonic projection, see also zenit in RFoptions.

RC_ORTHOGRAPHIC_PROJ gives the numerical code for the orthographic projection, see also zenit in RFoptions.

RC_EARTH_COORDS gives the numerical code for option "earth coordinates"

RC_EARTH_ISOTROPIC gives the numerical code for option "earth isotropic"

RC_SPHERICAL_COORDS gives the numerical code for option "earth coordinates"

RC_OPTIMISER_NAMES and RC_NLOPTR_NAMES give the names for the options optimiser and algorithm, respectively, RFfitoptimiser.

RC_LIKELIHOOD_NAMES = c("auto", "full", "composite", "tesselation") gives the names of the ML variants: (i) internal choice according to the number of data, (ii) full likelihood, (iii) (pairwise) composite likelihood, and (iv) composite likelihood based on a tessellation of the space.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RF, RM, RP, RR, R., RFgetModelNames, RMmodelgenerator-class, RMtrafo.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RC_ISO_NAMES
RC_ISO_NAMES[RC_ISOTROPIC:RC_CARTESIAN_COORD + 1]
## Not run: 
RFgetModelNames(isotropy=RC_ISO_NAMES[RC_ISOTROPIC:RC_CARTESIAN_COORD +
1])

## End(Not run)

Coercion to class 'RFsp' objects

Description

Generate an object of class RFsp from conventional objects.

Usage

conventional2RFspDataFrame(data, coords=NULL, gridTopology=NULL, n=1,
                           vdim=1, T=NULL, vdim_close_together)

Arguments

data

array; of dimension c(vdim, space-time-dim, n); contains the values of the random field

coords

matrix of coordinates

gridTopology

3-row-matrix or of class GridTopology; specifies the grid vectors; either coords or gridTopology must be NULL

n

number of iid copies of the random field, default is 1

vdim

number of dimensions of the values of the random field, default is 1

T

time component if any. The length of the temporal grid is needed by as.array if the spatial locations are randomly scattered.

vdim_close_together

logical. Currently, only vdim_close_together=FALSE is coded. In this case the dimensions of the data follow the order “locations, multivariate, repeated”. Otherwise “multivariate, locations, repeated”.

Value

Object of class RFspatialGridDataFrame, RFspatialPointsDataFrame, RFgridDataFrame or RFpointsDataFrame.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
x <- 1:20
z <- RFsimulate(RMexp(), x, spConform=FALSE)
z2 <- conventional2RFspDataFrame(z, coord=x)
Print(z, z2)

Coordinate systems

Description

Implemented Coordinate Systems.

Implemented coordinate systems

  • Cartesian coordinate system

  • Earth coordinate systems
    The earth is considered as an ellipsoid; The first angle takes values in [0,360)[0, 360), the second angle takes values in [90,90][-90, 90].

  • Spherical coordinate systems
    The earth is considered as an ellipsoid; The first angle takes values in [0,2π)[0, 2\pi), the second angle takes values in [π/2,π/2][-\pi/2, \pi/2].

Transformations between the system

  • Earth to cartesian
    The 3-dimensional resulting coordinates are either given in ‘km’ or in ‘miles’.

  • Gnomonic and orthographic projections
    The 2-dimensional resulting coordinates are either given in ‘km’ or in ‘miles’. The projection direction is given by the zenit.

  • Earth to spherical
    In this case the Earth is considered as a ball.

Cartesian systems cannot be transformed to earth or spherical coordinate systems, nor a spherical system to earth coordinates.

Options

coord_system

character. One of the values "auto", "cartesian", "earth"

If "auto", then the coordinates are considered as "cartesian" except the names of the given coordinates indicate a different system. Currently, only "longitude" and "latidute" (or abbreviations of them) are excepted as names for given coordinates and indicate an earth coordinate systems. See the examples below.

Default: "auto"

coordidx

integer vector of column numbers of the variables in the data frame. varidx can be set alternatively to coordnames. This parameter gives the coordinate columns in a data frame by starting column and ending column or the sequence. An NA in the second component means ‘until the end’.

coordnames

vector of characters that can be set alternatively to coordidx. This parameter gives the coordinate columns in a data frame by names. If it is "NA", then, depending on the context, either an error message is returned or it is assumed that the first columns give the coordinates.

coordunits

any string. If coordinate_system = "earth" and longitude and latitude are transformed to 3d cartesian coordinates, coordunits determines whether the radius is given in kilometers ("km") or miles ("miles"). If empty, then "km" is chosen.

Default: ""

new_coord_system

One of the values "keep", "cartesian", "earth", "plane".

  1. "keep"
    The coord_system is kept (except an explicit transformation is given, see RMtrafo.

    Note that some classes of models, e.g. completely monotone functions and compactly supported covariance models with range less than π\pi are valid models on a sphere. In this case the models are considered as models on the sphere. See spherical models for lists.

  2. "cartesian"
    If coord_system is "earth" the coordinates are transformed to cartesian coordinates before any model is considered.

  3. "orthographic", "genomic"
    If coord_system is "earth" the locations are projected to a plane before any model is considered.

Default: "keep"

new_coordunits

internal and should not be set by the user.

Default: ""

polar_coord

logical. If FALSE the spherical coordinates agree with the earth coordinate parametrization, except that radians are used for spherical coordinates instead of degrees for the earth coordinates.

If TRUE the spherical coordinates signify polar coordinates.

Default : FALSE

varidx

integer vector of length 2. varidx can be set alternatively to varnames. This parameter gives the data columns in a data frame, either by starting column and ending column. An NA in the second component means ‘until the end’.

varnames

vector of characters that can be set alternatively to varidx. This parameter gives the data columns in a data frame by names.

if varnames equals "NA" then for keywords ‘data’, ‘value’ and ‘variable’ will be searched for keywords. If none of them are found, depending on the context, either an error message is returned or it is assumed that the last columns give the data.

varunits

vector of characters. The default units of the variables.

Default: ""

xyz_notation

logical or NA. Used by RMuser only.

NA : automatic choice (if possible)

FALSE : notation (x, y) should not be understood as kernel definition, not as xyz notation

TRUE: xyz notation used

zenit

two angles of the central projection direction for the gnomonic projection (https://en.wikipedia.org/wiki/Gnomonic_projection, https://de.wikipedia.org/wiki/Gnomonische_Projektion) and the orthographic projection, (https://en.wikipedia.org/wiki/Orthographic_projection_in_cartography, https://de.wikipedia.org/wiki/Orthografische_Azimutalprojektion).

If any(is.na(zenit)) then either the value of either of the components may not be NA, whose value will be denoted by pp.

If p=1p=1 then the mean of the locations is calculated; if p=Infp=Inf then the mean of the range is calculated.

Default: c(1, NA)

References

Covariance models in a cartesian system

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

Covariance models on a sphere

  • Gneiting, T. (2013) Strictly and non-strictly positive definite functions on spheres. Bernoulli, 19, 1327-1349.

Tail correlation function

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMtrafo, RFearth2cartesian, RPdirect, models valid on a sphere, RFoptions.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

z <- 1:4
x <- cbind(z, 0)
y <- cbind(0, z)
model <- RMwhittle(nu=0.5)
RFcov(model, x, y, grid=FALSE) ##  standard is (cartesian) model


## same as above, but explicit:
RFcov(model, x, y, grid=FALSE, coord_sys="cartesian") 


## model is not valid on a sphere; x,y coordinates are
## transformed from earth coordinates to spherical coordinates
RFcov(model, x, y, grid=FALSE, coord_sys="earth")


## now the scale is chosen such that the covariance
## values are comparable to those in the cartesian case
RFcov(RMS(model, s= 1 / 180 * pi), x, y, grid=FALSE,
      coord_sys="earth")


## projection onto a plane first. Then the scale is interpreted
## in the usual, i.e. cartesian, sense, i.e. the model does not
## really make sense
RFoptions(zenit = c(2.5, 2.5))
RFcov(model, x, y, grid=FALSE,
      coord_sys="earth", new_coord_sys="orthographic")


## again, here the scale is chosen to be comparable to the cartesian case
## here the (standard) units are [km]
(z1 <- RFcov(RMS(model, s= 6350 / 180 * pi), x, y, grid=FALSE,
             coord_sys="earth", new_coord_sys="orthographic"))


## as above, but in miles
(z2 <- RFcov(RMS(model, s= 6350 / 1.609344 / 180 * pi), x, y, grid=FALSE,
             coord_sys="earth", new_coord_sys="orthographic",
             new_coordunits="miles"))
stopifnot(all.equal(z1, z2))


## again, projection onto a plane first, but now using the
## gnomonic projection
## here the (standard) units are [km]
(z1 <- RFcov(RMS(model, s= 6350 / 180 * pi), x, y, grid=FALSE,
             coord_sys="earth", new_coord_sys="gnomonic"))

## as above, but in miles
(z2 <- RFcov(RMS(model, s= 6350 / 1.609344 / 180 * pi), x, y, grid=FALSE,
             coord_sys="earth", new_coord_sys="gnomonic",
             new_coordunits="miles"))
stopifnot(all.equal(z1, z2, tol=1e-5))

Distribution families (RR commands)

Description

Distribution families to specify random parameters in the model definition.

Details

See Bayesian Modelling for a less technical introduction to hierarchical modelling.

When simulating Gaussian random fields, the random parameters are drawn only once at the very beginning. So, if the argument n in RFsimulate is greater than 1 then n simulations conditional on a single realization of the random parameters are performed. See the examples below.

There are (simple) multivariate versions and additional versions to the distributions families implemented. Further, any distribution family defined in R can be used, see the examples below.

These functions will allow for Bayesian modelling. (Future project).

Implemented models

RRdeterm no scattering
RRdistr families of distributions transferred from R
RRgauss a (multivariate) Gaussian random variable
RRloc modification of location and scale
RRspheric random scale for the RMball to simulate RMspheric, etc.
RRunif a (multivariate) uniform random variable

Note

The allowance of random parameters is a very recent, developing feature of RandomFields.

Future changings of the behaviour are not unlikely.

Note

A further random element is RMsign, which is an operator on shape functions. As an exception its name starts with RM and not with RR.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RC, RF, RM, RP, Other models, RFdistr, RMmodelgenerator, R.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## here, the scale is given by an exponential variable:
model <- RMgauss(scale=exp())
for (i in 1:4) {
  RFoptions(seed = i)
  # each leads to a simulation with a different scale parameter
  plot(model) ## random
  plot(RFsimulate(model, x=seq(0,10,0.1)))
  readline("press return")
}

# but here, all 4 simulations have the same (but random) scale:
plot(RFsimulate(model, x=seq(0,10,0.1), n=4)) 


## hierarchical models are also possible:
## here, the scale is given by an exponential variable whose
## rate is given by a uniform variable
model <- RMgauss(scale=exp(rate=unif()))
plot(model)
plot(RFsimulate(model, x=seq(0,10,0.1)))


## HOWEVER, the next model is deterministic with scale \code{e=2.718282}.
model <- RMgauss(scale=exp(1))
plot(model)
plot(RFsimulate(model, x=seq(0,10,0.1)))

Extremal t process

Description

RPopitz defines an extremal t process.

Usage

RPopitz(phi, xi, mu, s, alpha)

Arguments

phi

an RMmodel; covariance model for a standardized Gaussian random field, or the field itself.

xi, mu, s

the extreme value index, the location parameter and the scale parameter, respectively, of the generalized extreme value distribution. See Details.

alpha

originally referred to the α\alpha-Frechet marginal distribution, see the original literature for details.

Details

The argument xi is always a number, i.e. ξ\xi is constant in space. In contrast, μ\mu and ss might be constant numerical values or (in future!) be given by an RMmodel, in particular by an RMtrend model.
For xi=0xi=0, the default values of mumu and ss are 00 and 11, respectively. For xi0xi\not=0, the default values of mumu and ss are 11 and ξ|\xi|, respectively, so that it defaults to the standard Frechet case if ξ>0\xi > 0.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Davison, A.C., Padoan, S., Ribatet, M. (2012). Statistical modelling of spatial extremes. Stat. Science 27, 161-186.

  • Opitz, T. (2012) A spectral construction of the extremal t process. arxiv 1207.2296.

See Also

RMmodel, RPgauss, maxstable, maxstableAdvanced.

Examples

## sorry, does not work savely yet

Extremal Gaussian process

Description

RPschlather defines an extremal Gaussian process.

Usage

RPschlather(phi, tcf, xi, mu, s)

Arguments

phi

an RMmodel, see Details.

tcf

an RMmodel specifying the extremal correlation function; either phi or tcf must be given.

xi, mu, s

the extreme value index, the location parameter and the scale parameter, respectively, of the generalized extreme value distribution. See Details.

Details

The argument xi is always a number, i.e. ξ\xi is constant in space. In contrast, μ\mu and ss might be constant numerical values or (in future!) be given by an RMmodel, in particular by an RMtrend model.
For xi=0xi=0, the default values of mumu and ss are 00 and 11, respectively. For xi0xi\not=0, the default values of mumu and ss are 11 and ξ|\xi|, respectively, so that it defaults to the standard Frechet case if ξ>0\xi > 0.

The argument phi can be any random field for which the expectation of the positive part is known at the origin.

It simulates an Extremal Gaussian process ZZ (also called “Schlather model”), which is defined by

Z(x)=maxi=1Ximax(0,Yi(x)),Z(x) = \max_{i=1}^\infty X_i \max(0, Y_i(x)),

where the XiX_i are the points of a Poisson point process on the positive real half-axis with intensity cx2dxc x^{-2} dx, YiYY_i \sim Y are iid stationary Gaussian processes with a covariance function given by phi, and cc is chosen such that ZZ has standard Frechet margins. phi must represent a stationary covariance model.

Note

Advanced options are maxpoints and max_gauss, see RFoptions.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RPgauss, maxstable, maxstableAdvanced.

Examples

RFoptions(seed=0, xi=0)
## seed=0: *ANY* simulation will have the random seed 0; set
##         RFoptions(seed=NA) to make them all random again

## xi=0: any simulated max-stable random field has extreme value index 0
x <- seq(0, 2,0.01)

## standard use of RPschlather (i.e. a standardized Gaussian field)
model <- RMgauss()
z1 <- RFsimulate(RPschlather(model), x)
plot(z1, type="l")

## the following refers to the generalized use of RPschlather, where
## any random field can be used. Note that 'z1' and 'z2' have the same
## margins and the same .Random.seed (and the same simulation method),
## hence the same values
model <- RPgauss(RMgauss(var=2))
z2 <- RFsimulate(RPschlather(model), x)
plot(z2, type="l")
all.equal(z1, z2) # true

## Note that the following definition is incorrect
try(RFsimulate(model=RPschlather(RMgauss(var=2)), x=x))


## check whether the marginal distribution (Gumbel) is indeed correct:
model <- RMgauss()
z <- RFsimulate(RPschlather(model, xi=0), x, n=100)
plot(z)
hist(unlist(z@data), 50, freq=FALSE)
curve(exp(-x) * exp(-exp(-x)), from=-3, to=8, add=TRUE)

Details on fitting Gaussian random fields, including Box-Cox transformation

Description

Here, some details of RFfit are given concerning the fitting of models for Gaussian random fields.

This documentation is far from being complete.

Maximum likelihood

The application of the usual maximum likelihood method and reporting the result is the default.

Least squares

The weighted least squares methods minimize

iwi(γ^(hi)γ(hi))2\sum_{i} w_i (\hat \gamma(h_i) - \gamma(h_i))^2

over all parametrized models of γ\gamma. Here, ii runs over all NN bins of the binned variogram γ^\hat \gamma and hih_i is the centre of bin ii.

The following variants of the least squares methods, passed as sub.methods in RFfit are implemented:

'self'

wi=(γ(hi))2w_i = (\gamma(h_i))^{-2}

'plain'

wi=1w_i = 1 for all ii.

'sqrt.nr'

wi2w_i^2 equals the number of points nin_i in bin ii.

'sd.inv'

1/wi1 / w_i equals the standard deviation of the variogram cloud within bin ii.

'internal'

Three subvariants are implemented:

'internal1'

wi2=(Ni+1)niw_i^2 = (N-i+1) n_i

'internal2'

wi=Ni+1w_i = N-i+1

'internal3'

wi2=Ni+1w_i^2 = N-i+1

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFfit, RFfit-class.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
## See 'RFfit'.

Methods for Gaussian Random Fields

Description

Here, all the methods (models) for simulating Gaussian random fields are listed.

Implemented models

RPcirculant simulation by circulant embedding
RPcutoff simulation by a variant of circulant embedding
RPcoins simulation by random coin / shot noise
RPdirect through the square root of the covariance matrix
RPgauss generic model that chooses automatically among the specific methods
RPhyperplane simulation by hyperplane tessellation
RPintrinsic simulation by a variant of circulant embedding
RPnugget simulation of (anisotropic) nugget effects
RPsequential sequential method
RPspecific model specific methods (very advanced)
RPspectral spectral method
RPtbm turning bands

Computing demand for simulations

Assume at nn locations in dd dimensions a vv-variate field has to be simulated. Let

f(n,d)=2dnlog(n)f(n, d) = 2^d n \log(n)

The following table gives in particular the time and memory needed for the specific simulation method.

grid vv dd time memory comments
RPcirculant yes any 13\le 13 O(v3f(n,d))O(v^3f(n, d)) O(v2f(n,d))O(v^2f(n, d))
no any 13\le 13 O(v3f(k,d))O(v^3 f(k, d)) O(v2f(k,d))O(v^2f(k, d)) kk \simapprox_stepd{}^{-d}
RPcutoff see RPcirculant above
RPcoins yes 11 4\le 4 O(kn)O(k n) O(n)O(n) kk \sim(latticespacing)d(lattice spacing)^{-d}
no 11 4\le 4 O(kn)O(k n) O(n)O(n) kk depends on the geometry
RPdirect any any any O(1)..O(v2n2)O(1)..O(v^2 n^2) O(v2n2)O(v^2 n^2) effort to investigate the covariance matrix, if matrix_methods is not specified (default)
O(vn)O(v n) O(vn)O(v n) covariance matrix is diagonal
see spam O(z+vn)O(z + v n) covariance matrix is sparse matrix with zz non-zeros
O(v3n3)O(v^3 n^3) O(v2n2)O(v^2 n^2) arbitrary covariance matrix (preparation)
O(v2n2)O(v^2 n^2) O(v2n2)O(v^2 n^2) arbitrary covariance matrix (simulation)
RPgauss any any any O(1)O(v3n3)O(1) \ldots O(v^3n^3) O(1)O(n2)O(1)\ldots O(n^2) only the selection process; O(1)O(1) if first method tried is successful
RPhyperplane any 11 22 O(n/sd)O(n / s^d) O(n/sd)O(n / s^d) s=s =scale
RPintrinsic see RPcirculant above
RPnugget any any any O(vn)O(v n) O(vn)O(v n)
RPsequential any 11 any O(S3b3)O(S^3 b^3) O(S2b2)O(S^2 b^2) n=STn=ST; SS and TT the number of spatial and temporal locations, respectively; b=b =back_steps (preparation)
O(nSb2)O(n S b^2) O(S2b2)+O(n)O(S^2 b^2) + O(n) (simulation)
RPspectral any 11 2\le 2 O(C(d)n)O(C(d) n) O(n)O(n) C(d)C(d) : large constant increasing in dd
RPtbm any 11 4\le 4 O(C(d)(n+L)O(C(d) (n + L) O(n+L)O(n + L) C(d)C(d) : large constant increasing in dd; LL is the effort needed to simulate on a line (or plane)
RPspecific only the specific part
* * RMplus any any any O(v n) O(v n)
* * RMS any any any O(1) O(v n)
* * RMmult any any any O(v n) O(v n)

Computing demand for interpolation

Assume vv-variate data are given at nn locations in dd dimensions. To interpolate at kk locations RandomFields needs

grid vv dd time memory comments
any any any O(1)..O(v2n2)O(1)..O(v^2 n^2) O(v2n2)O(v^2 n^2) effort to investigate the covariance matrix, if matrix_methods is not specified (default)
O(v2nk)O(v ^2 n k) O(v(n+k))O(v (n + k)) covariance matrix is diagonal
see spam+ O(v^2nk) O(z+v(n+k))O(z + v (n + k)) covariance matrix is sparse matrix with zz non-zeros
O(v3n3+v2nk)O(v^3 n^3 + v^2nk) O(v2n2+vk)O(v^2 n^2 + v*k) arbitrary covariance matrix

Computing demand for conditional simulation

Assume vv-variate data are given at nn locations x1,,xnx_1,\ldots, x_n in dd dimensions. To conditionally simulate at kk locations y1,,yky_1,\ldots, y_k, the computing demand equals the sum of the demand for interpolating and the demand for simulating on the k+nk+n locations. (Grid algorithms for simulating will apply if the kk locations y1,,yky_1,\ldots, y_k are defined by a grid and the nn locations x1,,xnx_1,\ldots, x_n are a subset of y1,,yky_1,\ldots, y_k, a situation typical in image analysis.)

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

  • Yaglom, A.M. (1987) Correlation Theory of Stationary and Related Random Functions I, Basic Results. New York: Springer.

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3nd edition.

See Also

RP, Other models, RMmodel, RFgetMethodNames, RFsimulateAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

set.seed(1)
x <- runif(90, 0, 500)
z <- RFsimulate(RMspheric(), x)
z <- RFsimulate(RMspheric(), x, max_variab=10000)

Fast and Exact Simulation of Large Gaussian Lattice Systems in R2

Description

Here, the code of the paper on ‘Fast and Exact Simulation of Large Gaussian Lattice Systems in R2’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Sevcikova, H., Percival, D.B., Schlather, M., Jiang, Y. (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in R2: Exploring the Limits. J. Comput. Graph. Stat., 15, 483-501.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Figure 1 (pretty time consuming)
stabletest <- function(alpha, theta, size=512) {
  RFoptions(trials=1, tolIm = 1e-8, tolRe=0, force = FALSE,
            useprimes=TRUE, strategy=0, skipchecks=!FALSE,
             storing=TRUE)
  model <- RMcutoff(diameter=theta, a=1, RMstable(alpha=alpha))
  RFcov(dist=0, model=model, dim=2, seed=0)
  r <- RFgetModelInfo(modelname="RMcutoff", level=3)$storage$R_theor
  x <- seq(0, r, by= r / (size - 1)) * theta
  err <- try(RFsimulate(x, x, model=RPcirculant(model), n=0))
  return(if (class(err) == "try-error") NA else r)
}

alphas <- seq(1.52, 2.0, 0.02) 
thetas <- seq(0.05, 3.5, 0.05)

m <- matrix(NA, nrow=length(thetas), ncol=length(alphas))
for (it in 1:length(thetas)) {
  theta <- thetas[it]
  for (ia in 1:length(alphas)) {
  alpha <- alphas[ia]
  cat("alpha=", alpha, "theta=", theta,"\n")
  m[it, ia] <- stabletest(alpha=alpha, theta=theta)
  if (is.na(m[it, ia])) break
  }
  if (any(is.finite(m))) image(thetas, alphas, m, col=rainbow(100))
}

Bayesian Spatial Modelling

Description

RandomFields provides Bayesian modelling to some extend: (i) simulation of hierarchical models at arbitrary depth; (ii) estimation of the parameters of a hierarchical model of depth 1 by means of maximizing the likelihood.

Details

A Bayesian approach can be taken for scalar, real valued model parameters, e.g. the shape parameter nu in the RMmatern model. A random parameter can be passed through a distribution of an existing family, e.g. (dnorm, pnorm, qnorm, rnorm) or self-defined. It is passed without the leading letter d, p, q, r, but as a function call e.g norm(). This function call may contain arguments that must be named, e.g. norm(mean=3, sd=5).

Usage:

  • exp() denotes the exponential distribution family with rate 1,

  • exp(3) is just the scalar e3e^3 and

  • exp(rate=3) is the exponential distribution family with rate 33.

The family can be passed in three ways:

  • implicitly, e.g. RMwhittle(nu=exp()) or

  • explicitly through RRdistr, e.g. RMwhittle(nu=RRdistr(exp())).

  • by use of RRmodels of the package.

The first is more convenient, the second more flexible and slightly safer.

Note

  • While simulating any depth of hierarchical modelling is possible, estimation is currently restricted to one level of hierarchy.

  • The effect of the distribution family varies between the different processes:

    • in max-stable fields and RPpoisson, a new realization of the prior distribution(s) is drawn for each shape function

    • in all other cases: a realization of the prior(s) is only drawn once. This effects, in particular, Gaussian fields with argument n>1, where all realizations are based on the same realization out of the prior distribution(s).

    Note that checking the validity of the arguments is rather limited for such complicated models, in general.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodelsAdvanced. For hierarchical modelling see RR.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
## See 'RRmodels' for hierarchical models

## the following model defines the argument nu of the Whittle-Matern
## model to be an exponential random variable with rate 5.
model <- ~ 1 + RMwhittle(scale=NA, var=NA, nu=exp(rate=5)) + RMnugget(var=NA)

data(soil)
fit <- RFfit(model, x=soil$x, y=soil$y, data=soil$moisture, modus="careless")
print(fit)

Hyperplane method

Description

The Hyperplane method is a simulation method for stationary, isotropic random fields with exponential covariance function. It is based on a tessellation of the space by hyperplanes. Each cell takes a spatially constant value of an i.i.d. random variable. The superposition of several such random fields yields approximatively a Gaussian random field.

Usage

RPhyperplane(phi, boxcox, superpos, maxlines, mar_distr, mar_param ,additive)

Arguments

phi

object of class RMmodel; specifies the covariance function to be simulated; only exponential covariance functions and scale mixtures of it are allowed.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

superpos

integer. number of superposed hyperplane tessellations. Default: 300.

maxlines

integer. Maximum number of allowed lines.

Default: 1000.

mar_distr

integer. code for the marginal distribution used in the simulation:

0

uniform distribution

1

Frechet distribution with form parameter mar_param

2

Bernoulli distribution (Binomial with n=1n=1) with argument mar_param

This argument should not be changed yet.

Default: 0.

mar_param

Argument used for the marginal distribution. The argument should not be changed yet.

Default: NA.

additive

logical. If TRUE independent realizations are added, else the maximum is taken.

Default: TRUE.

Value

RPhyperplane returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Lantuejoul, C. (2002) Geostatistical Simulation: Models and Algorithms. Springer.

See Also

Gaussian, RP.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RPhyperplane(RMexp(s=2), superpos=1)
x <- seq(0, 3, 0.04)
z <- RFsimulate(x=x, x, model=model, n=1)
plot(z)

Method to simulate the Nugget effect

Description

Method to simulate the Nugget effect. (Only for advanced users)

Usage

RPnugget(phi, boxcox, tol, vdim)

Arguments

phi

object of class RMmodel; specifies the covariance model to be simulated. The only possible model for phi is RMnugget.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

tol

points at a distance less than or equal to nugget.tol are considered as being identical. This strategy applies to the simulation method and the covariance function itself. Hence, the covariance function is only positive definite if nugget.tol=0.0. However, if the anisotropy matrix does not have full rank and nugget.tol=0.0, then the simulations are likely to be odd. The value of nugget.tol should be of order 101510^{-15}.

Default: 0.0

vdim

positive integer; the model is treated vdim-variate, vdim=1 (default) corresponds to a univariate random field. Mostly, the value of vdim is set automatically.

Default is that it takes the value of the submodel phi.

Details

General

This method only allows RMnugget as a submodel.

Anisotropy

The method also allows for zonal nugget effects. Only there the argument tol becomes important. For the zonal nugget effect, the anisotropy matrix Aniso should be given in RMnugget. There, only the kernel of the matrix is important.

Points close together

The locations at a distance less than or equal to the RFoptions nugget.tol are considered as being identical. This strategy applies to the simulation method and the covariance function itself. Hence, the covariance function is only positive definite if nugget.tol=0.0. However, if the anisotropy matrix does not have full rank and nugget.tol=0.0, then the simulations are likely to be odd. The value of nugget.tol should be of order 101510^{-15}.

Repeated measurements

Measurement errors are mathematically not distinguishable from spatial nugget effects as long as measurements are not repeated at the very same space-time location. So there is no need to distinguish the spatial nugget effect from a measurement error. This is the default, see allow_duplicated_locations in RFoptions.

In case several measurement have been taken in single space-time locations, measurement errors can be separated from spatial noise. In this case RMnugget() models the measurement error (which corresponds to a non-stationary model in an abstract space) by default and the measurement error model cannot be extended beyond the given locations. On the other hand RMnugget(Ansio=something) and RMnugget(proj=something) model the spatial nugget effect (with and without zonal anisotropy in case Aniso has low and full rank respectively).

Role of RPnugget

Even for advanced users, there is no need to call RPnugget directly, as this is done internally when the RMnugget is involved in the covariance model.

Value

RPnugget returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

See Also

Gaussian, RP, RPcoins, RPhyperplane, RPspectral, RPtbm.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


x <- y <- 1:2
xy <- as.matrix(expand.grid(x, y)) ## we get 4 locations
## Standard use of the nugget effect
model <- RMnugget(var = 100)
RFcovmatrix(model, x=xy)
as.vector(RFsimulate(model, x=x, y=x, tol=1e-10))

## zonal nugget effect, which is not along the axes
model <- RMnugget(Aniso=matrix(1, nr=2, nc=2))
RFcovmatrix(model, x=xy)
as.vector(RFsimulate(model, x=x, y=x, tol=1e-10))


## All the following examples refer to repeated measurements
RFoptions(allow_duplicated_locations = TRUE) 
(xy <- rbind(xy, xy)) ## now, the 4 locations are repeated twice 

## standard situation: the nugget is interpreted as measurement error:
model <- RMnugget()
RFcovmatrix(model, x=xy)
as.matrix(RFsimulate(model, x=xy)) 

## any anisotropy matrix with full rank: spatial nugget effect
model <- RMnugget(Aniso=diag(2))
RFcovmatrix(model, x=xy)
as.matrix(RFsimulate(model, x=xy))

## anisotropy matrix with lower rank: zonal nugget effect
model <- RMnugget(Aniso=matrix(c(1, 0, 0, 0), nc=2))
RFcovmatrix(model, x=xy)
as.matrix(RFsimulate(model, x=xy))

## same as before: zonal nugget effect
model <- RMnugget(Aniso=t(c(1,0)))
RFcovmatrix(model, x=xy)
as.matrix(RFsimulate(model, x=xy))

Internal functions

Description

These functions are internal and should not be used.

Usage

rfGenerateModels(package = "RandomFields", assigning,
                 RFpath ="~/svn/RandomFields/RandomFields",
                 RMmodels.file=paste(RFpath, "R/RMmodels.R", sep="/"),
                 PL = RFoptions()$basic$printlevel)

rfGenerateConstants(package="RandomFields", aux.package = "RandomFieldsUtils",
	   RFpath = paste0("~/svn/",package, "/", package),
           RCauto.file = paste(RFpath, "R/aaa_auto.R", sep="/"),
	   header.source =
	   c(if (length(aux.package) > 0) paste0("../../", aux.package,"/",
				 aux.package, "/src/Auto", aux.package, ".h"),
	     paste0("src/Auto",package,".h")),
	   c.source = paste0("src/Auto", package, ".cc"))

rfGenerateTest(package = "RandomFields", files = NULL,
               RFpath = paste0("~/svn/", package, "/", package))

rfGenerateMaths(package = "RandomFields",
			    files = "/usr/include/tgmath.h",
			    do.cfile = FALSE,
                            ## copy also in ../private/lit
                            Cfile = "QMath",
                            Rfile = "RQmodels",
                            RFpath = paste0("~/svn/",package,"/", package))


checkExamples(exclude = NULL, include=1:length(.fct.list),
               ask=FALSE, echo=TRUE, halt=FALSE, ignore.all = FALSE,
               path=package, package = "RandomFields", 
               read.rd.files=TRUE, local = TRUE, libpath = NULL,
               single.runs = FALSE)

ScreenDevice(height, width)

FinalizeExample()
StartExample(reduced = TRUE, save.seed = TRUE)
showManpages(path="/home/schlather/svn/RandomFields/RandomFields/man")

plotWithCircles(data, factor=1.0,
                xlim=range(data[,1])+c(-maxr,maxr),
                ylim=range(data[,2])+c(-maxr,maxr),
                col=1, fill=0, ...)

maintainers.machine()

Arguments

package, assigning, RFpath, RMmodels.file, PL

internal

aux.package, RCauto.file, header.source, c.source

internal

files

internal

Cfile, Rfile, do.cfile

internal

exclude, include, ask, echo, halt, ignore.all, path, read.rd.files, libpath, single.runs

internal; ignore.all refers to the ‘all’ export statement in the namespace – whether this should be ignored. If read.rf.files is TRUE or a path to the Rd files, then the man pages are analysed to get all examples; ignore.all is then ignored. If FALSE only examples of functions (which are searched in the environments) are run.

height, width

window sizes

data, factor, xlim, ylim, col, fill, ...

internal

reduced, save.seed, local

internal

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## internal functions: no examples given


# for (i in dep.packages) cat(maintainer(i), "\n")

Covariance models for multivariate and vector-valued fields

Description

Here, the code of the paper on ‘Analysis, simulation and prediction of multivariate random fields with package RandomFields’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’

See Also

weather, SS12, S10.

Examples

## Not run: 
               ###########################################
               ##  SECTION 4: UNCONDITIONAL SIMULATION  ##
               ###########################################

RFoptions(seed = 0, height = 4)
## seed=0:  *ANY* simulation will have the random seed 0; set
##          RFoptions(seed=NA) to make them all random again
## height : height of X11
## always_close_device=FALSE: the pictures are kept on the screen


## Fig. 1: linear model of coregionalization
M1 <- c(0.9, 0.6)
M2 <- c(sqrt(0.19), 0.8)
model <- RMmatrix(M = M1, RMwhittle(nu = 0.3)) + 
         RMmatrix(M = M2, RMwhittle(nu = 2))
x <- y <- seq(-10, 10,  0.2)
simu <- RFsimulate(model, x, y)
plot(simu)


## Fig. 2: Wackernagel's delay model
model <- RMdelay(RMstable(alpha = 1.9, scale = 2), s = c(4, 4))
simu <- RFsimulate(model, x, y)
plot(simu, zlim = 'joint')

## Fig. 3: extended Wackernagel's delay model
model <- RMdelay(RMstable(alpha = 1.9, scale = 2), s = c(0, 4)) + 
         RMdelay(RMstable(alpha = 1.9, scale = 2), s = c(4, 0))
simu <- RFsimulate(model, x, y)
plot(simu, zlim = 'joint')
plot(model, dim = 2, xlim = c(-5, 5), main = "Covariance function", 
     cex = 1.5, col = "brown")

## Fig. 4: latent dimension model
## MARGIN.slices has the effect of choosing the third dimension
##               as latent dimension
## n.slices has the effect of choosing a bivariate model
model <- RMgencauchy(alpha = 1.5, beta = 3)
simu <- RFsimulate(model, x, y, z = c(0,1))
plot(simu, MARGIN.slices = 3, n.slices = 2)


## Fig. 5: Gneiting's bivariate Whittle-Matern model
model <- RMbiwm(nudiag = c(1, 2), nured = 1, rhored = 1, cdiag = c(1, 5), 
                s = c(1, 1, 2))
simu <- RFsimulate(model, x, y)
plot(simu)


## Fig. 6: anisotropic linear model of coregionalization
M1 <- c(0.9, 0.6)
M2 <- c(sqrt(0.19), 0.8)
A1 <- RMangle(angle = pi/4, diag = c(0.1, 0.5))
A2 <- RMangle(angle = 0, diag = c(0.1, 0.5))
model <- RMmatrix(M = M1, RMgengneiting(kappa = 0, mu = 2, Aniso = A1)) +
         RMmatrix(M = M2, RMgengneiting(kappa = 3, mu = 2, Aniso = A2))
simu <- RFsimulate(model, x, y)
plot(simu)


## Fig. 7: random vector field whose paths are curl free
## A 4-variate field is simulated, where the first component
## refers to the potential field, the second and third component
## to the curl free vector field and the forth component to the
## field of sinks and sources
model <- RMcurlfree(RMmatern(nu = 5), scale = 4)
simu <- RFsimulate(model, x, y)
plot(simu, select.variables = list(1, 2 : 3, 4))
plot(model, dim = 2, xlim = c(-3, 3), main = "", cex = 2.3, col="brown") 


## Fig. 8: Kolmogorov's model of turbulence
## See the physical literature for its derivation and details
x <- y <- seq(-2, 2, len = 20)
model <- RMkolmogorov()
simu <- RFsimulate(model, x, y, z = 1)
plot(simu, select.variables = list(1 : 2), col = c("red"))
plot(model, dim = 3, xlim = c(-3, 3), MARGIN = 1 : 2, cex = 2.3,
     fixed.MARGIN = 1.0, main = "", col = "brown")



               ###########################################
               ## SECTION 5: DATA ANALYSIS              ##
               ###########################################

## get the data     
data("weather")
PT <- weather[ , 1 : 2]  ## full data set takes more than 
##                                     half an hour to be analysed
## transformation of earth coordinates to Euclidean coordinates
Dist.mat <- as.vector(RFearth2dist(weather[ , 3 : 4]))
All <- TRUE
\dontshow{if(RFoptions()$internal$examples_reduced){warning("reduced data set")
All <- 1:10
PT <- weather[All , 1 : 2] 
Dist.mat <- as.vector(RFearth2dist(weather[All , 3 : 4]))
}}



#################################
## model definition            ##
#################################
## bivariate pure nugget effect:
nug <- RMmatrix(M = matrix(nc = 2, c(NA, 0, 0, NA)), RMnugget())
## parsimonious bivariate Matern model
pars.model <- nug + RMbiwm(nudiag = c(NA, NA), scale = NA, cdiag = c(NA, NA),
                           rhored = NA)
## whole bivariate Matern model
whole.model <- nug + RMbiwm(nudiag = c(NA, NA), nured = NA, s = rep(NA, 3),
                            cdiag = c(NA, NA), rhored = NA)



#################################
## model fitting and testing   ## 
#################################
## 'parsimonious model'
## fitting takes a while ( > 10 min)
pars <- RFfit(pars.model, distances = Dist.mat, dim = 3, data = PT)
print(pars)
print(pars, full=TRUE)
RFratiotest(pars)
#RFcrossvalidate(pars, x = weather[All , 3 : 4], data = PT, full = TRUE)

## 'whole model'
## fitting takes a while ( > 10 min)
whole <- RFfit(whole.model, distances = Dist.mat, dim = 3, data = PT)
print(whole, full=TRUE)
RFratiotest(whole)
#RFcrossvalidate(whole, x = weather[All , 3 : 4], data = PT, full = TRUE)

## compare parsimonious and whole
RFratiotest(nullmodel = pars, alternative = whole)


#################################
## kriging                     ##
#################################
## First, the coordinates are projected on a plane
a <- colMeans(weather[All , 3 : 4]) * pi / 180
P <- cbind(c(-sin(a[1]), cos(a[1]), 0),
           c(-cos(a[1]) * sin(a[2]), -sin(a[1]) * sin(a[2]), cos(a[2])),
           c(cos(a[1]) * cos(a[2]), sin(a[1]) * cos(a[2]), sin(a[2])))
x <- RFearth2cartesian(weather[All , 3 : 4])
plane <- (t(x) %*%P)[ , 1 : 2]

## here, kriging is performed on a rectangular that covers
## the projected points above. The rectangular is approximated
## by a grid of length 200 in each direction.
n <- 200 
r <- apply(plane, 2, range)
dta <- cbind(plane, weather[All , 1 : 2])
z <- RFinterpolate(pars, data = dta, dim = 2,
                   x = seq(r[1, 1], r[2, 1], length = n),
                   y = seq(r[1, 2], r[2, 2], length = n),
                   varunits = c("Pa", "K"), spConform = TRUE)
plot(z)

## End(Not run)

Documentation of major changings

Description

This man page documents some major changings in RandomFields.

Changes done in 3.1.0 (Summer 2015)

  • full (univariate) trend modelling

  • error in particular in RFfit corrected

  • RFfit runs much faster now

  • effects of modus operandi changed for estimating

Corrections done in 3.0.56 (Jan 2015)

  • log Gauss field corrected (has been a log log Gauss field)

  • RMconstant is now called RMfixcov

Corrections done in 3.0.55 (Jan 2015)

  • Conditional simulation: several severe typos corrected.

Major Revision: changings from Version 2 to Version 3 (Jan 2014)

  • S4 objects

    • RandomFields is now based on S4 objects using the package sp. The functions accept both sp objects and simple objects as used in version 2. See also above.

  • Documentation

    • each model has now its own man page;

    • classes of models and functions are bundled in several pages: Covariance models start with RM, distribution families with RR, processes with RP, user functions with RF

    • the man pages of several functions are split into two parts:

      (i) a beginners man page which includes a link to

      (ii) man pages for advanced users

  • Interfaces

    • The interfaces become simpler, at the same time more powerful than the functions in version 2. E.g., RFsimulate can perform unconditional simulation, conditional simulation and random imputing.

    • Only those arguments are kept in the functions that are considered as being absolutely necessary. All the other arguments can be included as options.

    • RFgui is an instructive interface based on tcl/tk, replacing the former ShowModels

  • Inference for Gaussian random fields

    • RFfit has undergone a major revision. E.g.:

      (i) estimation of random effect models with spatial covariance structure

      (ii) automatic estimation of 10 and more arguments in multivariate and/or space-time models

    • RFvariogram is now based on an fft algorithm if the data are on a grid, even allowing for missing values.

    • RFratiotest has been added.

  • Processes

  • Models

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## S4 vs S3
x <- seq(0, 10, 0.1)
model <- RMexp()
plot(RFsimulate(model, x)) ## S4
plot(RFsimulate(model, x, spConform=FALSE)) ## no class

Transformation of coordinate systems

Description

The functions provide mathematical c functions as RMmodels

Usage

RFcalc(model, params, ...)
R.minus(x, y, factor)
R.plus(x, y, factor)
R.div(x, y, factor)
R.mult(x, y, factor)
R.const(x)
R.c(a, b, c, d, e, f, g, h, i, j, l, m, n, o, p, q, ncol, factor)
R.p(proj, new, factor)
R.is(x, is, y)
R.lon()
R.lat()
R.gamma(x)
R.acos(x)
R.asin(x)
R.atan(x)
R.atan2(y, x)
R.cos(x)
R.sin(x)
R.tan(x)
R.acosh(x)
R.asinh(x)
R.atanh(x)
R.cosh(x)
R.sinh(x)
R.tanh(x)
R.exp(x)
R.log(x)
R.expm1(x)
R.log1p(x)
R.exp2(x)
R.log2(x)
R.pow(x, y)
R.sqrt(x)
R.hypot(x, y)
R.cbrt(x)
R.ceil(x)
R.fabs(x)
R.floor(x)
R.fmod(x, y)
R.round(x)
R.trunc(x)
R.erf(x)
R.erfc(x)
R.lgamma(x)
R.remainder(x, y)
R.fdim(x, y)
R.fmax(x, y)
R.fmin(x, y)

## S4 method for signature 'ANY,RMmodel'
e1 %% e2
## S4 method for signature 'RMmodel,ANY'
e1 %% e2
## S4 method for signature 'RMmodel,character'
e1 * e2
## S4 method for signature 'character,RMmodel'
e1 * e2
## S4 method for signature 'RMmodel,character'
e1 + e2
## S4 method for signature 'RMmodel,factor'
e1 + e2
## S4 method for signature 'RMmodel,list'
e1 + e2
## S4 method for signature 'character,RMmodel'
e1 + e2
## S4 method for signature 'data.frame,RMmodel'
e1 + e2
## S4 method for signature 'factor,RMmodel'
e1 + e2
## S4 method for signature 'RMmodel,character'
e1 - e2
## S4 method for signature 'character,RMmodel'
e1 - e2
## S4 method for signature 'RMmodel,character'
e1 / e2
## S4 method for signature 'character,RMmodel'
e1 / e2
## S4 method for signature 'ANY,RMmodel'
e1 ^ e2
## S4 method for signature 'RMmodel,ANY'
e1 ^ e2
## S4 method for signature 'RMmodel,character'
e1 ^ e2
## S4 method for signature 'character,RMmodel'
e1 ^ e2
## S4 method for signature 'RMmodel'
abs(x)
## S4 method for signature 'RMmodel'
acosh(x)
## S4 method for signature 'RMmodel'
asin(x)
## S4 method for signature 'RMmodel'
asinh(x)
## S4 method for signature 'ANY,RMmodel'
atan2(y,x)
## S4 method for signature 'RMmodel,ANY'
atan2(y,x)
## S4 method for signature 'RMmodel'
atan(x)
## S4 method for signature 'RMmodel'
atanh(x)
## S4 method for signature 'RMmodel'
ceiling(x)
## S4 method for signature 'RMmodel'
cos(x)
## S4 method for signature 'RMmodel'
cosh(x)
## S4 method for signature 'RMmodel'
exp(x)
## S4 method for signature 'RMmodel'
expm1(x)
## S4 method for signature 'RMmodel'
floor(x)
## S4 method for signature 'RMmodel'
lgamma(x)
## S4 method for signature 'RMmodel'
log1p(x)
## S4 method for signature 'RMmodel'
log2(x)
## S4 method for signature 'RMmodel'
log(x)
## S4 method for signature 'RMmodel,missing'
round(x,digits)
## S4 method for signature 'RMmodel'
sin(x)
## S4 method for signature 'RMmodel'
sinh(x)
## S4 method for signature 'RMmodel'
sqrt(x)
## S4 method for signature 'RMmodel'
tan(x)
## S4 method for signature 'RMmodel'
tanh(x)
## S4 method for signature 'RMmodel'
trunc(x)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula. model is usually a R.model given here.

e1, e2, x, y, a, b, c, d, e, f, g, h, i, j, l, m, n, o, p, q

constant or object of class RMmodel, in particular R.model

ncol

in contrast to c, R.c also allows for defining matrices; ncol gives the number of columns

factor

constant factor multiplied with the function. This is useful when linear models are built

is

one of "==", "!=", "<=", "<", ">=", ">"

proj

selection of a component of the vector giving the location. Default value is 1.

new

coordinate system or other kind of isotropy which is supposed to be present at this model. It shold always be given if the coordinates are not cartesian.

digits

number of digits. Does not work with a RMmodel

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

R.plus

adds two values

R.minus

substracts two values

R.mult

multiplies two values

R.div

devides two values

R.const

defines a constant

R.c

builds a vector

R.is

evaluates equalities and inequalities; note that TRUE is returned if the equality or inequality holds up to a tolerance given by RFoptions()$nugget$tol

R.p

takes a component out of the vector giving the location

R.lon, R.lat

longitudinal and latitudinal coordinate, given in the spherical system, i.e. in radians. (earth system is in degrees).

R.round

Note that R.round rounds away from zero.

For the remaining models see the corresponding C functions for their return value. (For any ‘R.model’ type ‘man model’ under Linux.)

Value

Formally, the functions return an object of class RMmodel, except for RFcalc that returns a scalar. Neither vectors nor parentheses are allowed.

Note

Instead of R.model the standard function can be used in case there is no ambiguity, i.e., c(...),asin(x), atan(x), atan2(y, x), cos(x), sin(x), tan(x), acosh(x), asinh(x), atanh(x), cosh(x), sinh(x), tanh(x), exp(x), log(x), expm1(x), log2(x), log1p(x), exp2(x), ^, sqrt(x), hypot(a,b), cbrt(x), ceiling(x), abs(x), floor(x), round(x), trunc(x), erf(x), erfc(x), lgamma(x). See the examples below.

The function RFcalc is intended for simple calculations only and it is not excessively tested. Especially, binary operators should be used with caution.

Note that all the functions here are NOT recognized as being positive definite (or negative definite), e.g. cos in R1R^1:

  1. please use the functions given in RMmodels for definite functions (for cos see RMbessel)

  2. Using uncapsulated substraction to build up a covariance function is ambiguous, see the example in RMtrend

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFfctn, RMtrend

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


## simple calculation
RFcalc(3 + R.sin(pi/4))

## calculation performed on a field
RFfctn(R.p(1) + R.p(2), 1:3, 1:3) 
RFfctn(10 + R.p(2), 1:3, 1:3) 

## calculate the distances between two vectors
print(RFfctn(R.p(new="iso"), 1:10, 1:10))

## simulation of a non-stationary field where
## anisotropy by a transform the coordinates (x_1^2, x_2^1.5)
x <- seq(0.1, 6, 0.12)
Aniso <- R.c(R.p(1)^2, R.p(2)^1.5)
z <- RFsimulate(RMexp(Aniso=Aniso), x, x)


## calculating norms can be abbreviated:
x <- seq(-5, 5, 5) #0.1)
z2 <- RFsimulate(RMexp() + -40 + exp(0.5 * R.p(new="isotropic")), x, x)
z1 <- RFsimulate(RMexp() + -40 + exp(0.5 * sqrt(R.p(1)^2 + R.p(2)^2)), x, x)
stopifnot(all.equal(z1, z2))
plot(z1)

Simulation of Max-Stable Random Fields

Description

Here, a list of models and methods for simulating max-stable random fields is given.

See also maxstableAdvanced for more advanced examples.

Implemented models and methods

Models

RPbrownresnick Brown-Resnick process using an automatic choice of the 3 RPbr* methods below
RPopitz extremal t process
RPschlather extremal Gaussian process
RPsmith M3 processes

Methods

RPbrmixed simulation of Brown-Resnick processes using M3 representation
RPbrorig simulation of Brown-Resnick processes using the original definition
RPbrshifted simulation of Brown-Resnick processes using a random shift

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Kabluchko, Z., Schlather, M. & de Haan, L (2009) Stationary max-stable random fields associated to negative definite functions Ann. Probab. 37, 2042-2065.

  • Schlather, M. (2002) Models for stationary max-stable random fields. Extremes 5, 33-44.

  • Smith, R.L. (1990) Max-stable processes and spatial extremes Unpublished Manuscript.

See Also

RP, RMmodel, RPgauss, RPbernoulli, maxstableAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

### currently not programmed



## Not run: \dontshow{
## to do : seq(0, 10, 0.02) oben ist furchtbar langsam. Warum?
}
## End(Not run)

## Not run: \dontshow{
model <- RMball()
x <- seq(0, 10, 5) # nice for   x <- seq(0, 10, 0.02)
z <- RFsimulate(RPsmith(model, xi=0), x, n=1000, every=1000)
plot(z)
hist(unlist(z@data), 150, freq=FALSE) #not correct; to do; sqrt(2) wrong
curve(exp(-x) * exp(-exp(-x)), from=-3, to=8, add=TRUE, col=3)
}
## End(Not run)

model <- RMgauss()
x <- seq(0, 10, 0.05)
z <- RFsimulate(RPschlather(model, xi=0), x, n=1000)
plot(z)
hist(unlist(z@data), 50, freq=FALSE)
curve(exp(-x) * exp(-exp(-x)), from=-3, to=8, add=TRUE)


## for some more sophisticated models see maxstableAdvanced

Simulation examples of advanced Max-Stable Random Fields

Description

Here, an advanced example is given used to test whether the algorithms work correctly.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Strokorb, K. (2013) Ph.D. thesis.

See Also

RPmaxstable

Examples


Obsolete functions Version 2

Description

This part gives the obsolete functions of RandomFields Version 2 that are not maintained anymore.

Usage

Covariance(x, y = NULL, model, param = NULL, dim = NULL,
 Distances, fctcall = c("Cov", "Variogram", "CovMatrix"))
CovarianceFct(x, y = NULL, model, param = NULL, dim =NULL,
 Distances, fctcall = c("Cov", "Variogram", "CovMatrix"))
CovMatrix(x, y = NULL, model, param = NULL, dim = NULL, Distances)
DeleteAllRegisters()
DeleteRegister(nr=0)
DoSimulateRF(n = 1, register = 0, paired=FALSE, trend=NULL) 
InitSimulateRF(x, y = NULL, z = NULL, T=NULL, grid=!missing(gridtriple),
 model, param, trend, method = NULL, register = 0,
 gridtriple, distribution=NA)
InitGaussRF(x, y = NULL, z = NULL, T=NULL, grid=!missing(gridtriple),
 model, param, trend=NULL, method = NULL, register = 0, gridtriple) 
GaussRF(x, y = NULL, z = NULL, T=NULL, grid=!missing(gridtriple), model,
 param, trend=NULL, method = NULL, n = 1, register = 0, gridtriple,
 paired=FALSE, PrintLevel=1, Storing=TRUE, ...) 
Variogram(x, model, param = NULL, dim = NULL, Distances)
InitMaxStableRF(x, y = NULL, z = NULL, grid=NULL, model, param, maxstable,
 method = NULL, register = 0, gridtriple = FALSE)
MaxStableRF(x, y = NULL, z = NULL, grid=NULL, model, param, maxstable,
 method = NULL, n = 1, register = 0, gridtriple = FALSE, ...)
EmpiricalVariogram(x, y = NULL, z = NULL, T=NULL, data, grid=NULL, bin,
 gridtriple = FALSE, phi, theta, deltaT)
Kriging(krige.method, x, y=NULL, z=NULL, T=NULL, grid=NULL, gridtriple=FALSE,
 model, param, given, data, trend=NULL,pch=".", return.variance=FALSE,
 allowdistanceZero = FALSE, cholesky=FALSE) 
CondSimu(krige.method, x, y=NULL, z=NULL, T=NULL, grid=NULL, gridtriple=FALSE,
 model, param, method=NULL, given, data, trend=NULL, n=1, register=0, 
 err.model=NULL, err.param=NULL, err.method=NULL, err.register=1, 
 tol=1E-5, pch=".", paired=FALSE, na.rm=FALSE) 
RFparameters(...)
hurst(x, y = NULL, z = NULL, data, gridtriple = FALSE, sort=TRUE,
 block.sequ = unique(round(exp(seq(log(min(3000, dim[1] / 5)),
 log(dim[1]), len=min(100, dim[1]))))),
 fft.m = c(1, min(1000, (fft.len - 1) / 10)),
 fft.max.length = Inf, 
 method=c("dfa", "fft", "var"), mode=c("plot", "interactive"),
 pch=16, cex=0.2, cex.main=0.85,
 PrintLevel=RFoptions()$basic$printlevel,height=3.5, ...)
fractal.dim(x, y = NULL, z = NULL, data, grid=TRUE, gridtriple = FALSE,
 bin, vario.n=5, sort=TRUE, fft.m = c(65, 86), fft.max.length=Inf,
 fft.max.regr=150000, fft.shift = 50, method=c("variogram", "fft"),
 mode=c("plot", "interactive"), pch=16, cex=0.2, cex.main=0.85,
 PrintLevel = RFoptions()$basic$printlevel, height=3.5, ...)
fitvario(x, y=NULL, z=NULL, T=NULL, data, model, param, lower=NULL,
 upper=NULL, sill=NA, grid=!missing(gridtriple), gridtriple=FALSE, ...)

Arguments

x, y, model, param, dim, Distances, fctcall, n, register, paired, trend, z, T, grid, method, gridtriple, distribution, PrintLevel, Storing, ..., maxstable, data, bin, phi, theta, deltaT, krige.method, pch, return.variance, allowdistanceZero, cholesky, given, err.model, err.param, err.method, err.register, tol, na.rm, sort, block.sequ, fft.m, fft.max.length, mode, cex, cex.main, height, vario.n, fft.max.regr, fft.shift, lower, upper, sill, nr

As the functions are obsolete, all these arguments are not documented anymore.

Value

See ‘version2’ for details on these obsolete commands.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

The functions that should be used instead are, for instance, RFcov, RFcovmatrix, RFvariogram, RFsimulate, RFinterpolate, RFvariogram, RFfit, RFoptions, RFhurst, RFfractaldim

See ‘version2’ for details on the obsolete commands.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again




## no examples given, as command is obsolete

Obsolete functions Version 3

Description

Some functions of RandomFields Version 3 have been replaced by more powerful functions

Usage

RFempiricalvariogram(...)
RFempiricalcovariance(...)
RFempiricalmadogram(...)

Arguments

...

See for the recent functions given in the Details

Details

RFempiricalvariogram

see RFvariogram

RFempiricalcovariance

see RFcov

RFempiricalmadogram

see RFmadogram

Strokorb's M3/M4 functions

are called RMm2r, RMm3b, RMmps

Value

see the respective recent function

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFcov, RFcovmatrix, RFvariogram. RFpseudovariogram, RFmadogram, RFpseudomadogram

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again




## no examples given, as command is obsolete

Auxiliary and other Models

Description

Here, auxiliary models are given that are not covariance functions or variograms, but which might be used within the definition of a model.

Implemented models

Distribution families See RR.

Evaluation operators See RF.

Random Fields / Random Processes See RP.

Mathematical functions See R.

Shape functions

Besides any of the covariance functions the following functions can be used as shape functions.

RMangle defines an anisotropy matrix by angle and a diagonal matrix
RMball Indicator of a ball of radius 1/21/2
RMm2r spectral function belonging to a tail correlation function of the Gneiting class HnH_n
RMm3b spectral function belonging to a tail correlation function of the Gneiting class HnH_n
RMmppplus operator to define mixed moving maxima (M3) processes
RMmps spectral functions belonging to a tail correlation function of the Gneiting class HnH_n
RMpolygon Indicator of a typical Poisson polygon
RMrational shape function used in the Bernoulli paper given in the references
RMrotat shape function used in the Bernoulli paper given in the references
RMsign random sign
RMtruncsupport truncates the support of a shape in a Poisson based model

Special transformations

RMeaxxa shape function used in the Bernoulli paper given in the references
RMetaxxa shape function used in the Bernoulli paper given in the references
RMidmodel model identity
RMid identity but interpretation turns from a coordinate to a model value
RMtrafo allows to model the identity within the set of coordinates
RMrotation shape function used in the Bernoulli paper given in the references

Other models

RMuser User defined covariance model

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RM

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
RFgetModelNames()

Papers involving RandomFields and co-authored by M. Schlather

Description

Here, an overview is given over the papers co-authored by M. Schlather that involve RandomFields.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Kleiber, W. and Schlather, M. (2010) Matern cross-covariance functions for multivariate random fields J. Amer. Statist. Assoc. 105, 1167-1177.

    See GKS11 for the code.

  • Gneiting, T., Sevcikova, H., Percival, D.B., Schlather, M., Jiang, Y. (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in R2: Exploring the Limits. J. Comput. Graph. Stat., 15, 483-501.

    See GSPSJ06 for the code.

  • Scheuerer, M. and Schlather, M. (2012) Covariance Models for Random Vector Fields. Stochastic Models, 82, 433-451.

    See SS12 for the code.

  • Schlather, M. (2002) Models for stationary max-stable random fields. Extremes 5, 33-44.

    See S02 for the code.

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

    See S10 for the code.

  • Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’,

    See ‘multivariate_jss’ for the vignette.

  • Strokorb, K., Ballani, F. and Schlather, M. (2014) In Preparation.

    See SBS14 for the code.

See Also

weather, GSPSJ06, SS12, S02, S10, jss14.

Examples

# For examples, see the specific papers.

Methods for function plot in package RandomFields

Description

Plot methods are implemented for simulated random fields (objects of class RFsp), explicit covariance models (objects of class RMmodel), empirical variograms (objects of class RFempVariog) and fitted models (objects of class RFfit).

The plot methods not described here are described together with the class itself, for instance, RFfit, RFempVariog RMmodel.

Usage

RFplotSimulation(x, y, MARGIN=c(1,2), MARGIN.slices=NULL,
 n.slices = if (is.null(MARGIN.slices)) 1 else 10, nmax=6, 
 plot.variance = !is.null(x@.RFparams$has.variance) && x@.RFparams$has.variance,
 select.variables, zlim, legend=TRUE,
 MARGIN.movie = NULL, file=NULL, speed = 0.3,
 height.pixel=300, width.pixel=height.pixel,
 ..., plotmethod="image")

RFplotSimulation1D(x, y, nmax=6,
  plot.variance=!is.null(x@.RFparams$has.variance) && x@.RFparams$has.variance,
  legend=TRUE, ...)

## S4 method for signature 'RFgridDataFrame,missing'
plot(x, y, ...)
## S4 method for signature 'RFpointsDataFrame,missing'
plot(x, y, ...)
## S4 method for signature 'RFspatialGridDataFrame,missing'
plot(x, y, ...)
## S4 method for signature 'RFspatialPointsDataFrame,missing'
plot(x, y, ...)

## S4 method for signature 'RFgridDataFrame,matrix'
plot(x, y, ...)
## S4 method for signature 'RFpointsDataFrame,matrix'
plot(x, y, ...)
## S4 method for signature 'RFspatialGridDataFrame,matrix'
plot(x, y, ...)
## S4 method for signature 'RFspatialPointsDataFrame,matrix'
plot(x, y, ...)

## S4 method for signature 'RFgridDataFrame,data.frame'
plot(x, y, ...)
## S4 method for signature 'RFpointsDataFrame,data.frame'
plot(x, y, ...)
## S4 method for signature 'RFspatialGridDataFrame,data.frame'
plot(x, y, ...)
## S4 method for signature 'RFspatialPointsDataFrame,data.frame'
plot(x, y, ...)

## S4 method for signature 'RFgridDataFrame,RFgridDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFgridDataFrame,RFpointsDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFpointsDataFrame,RFgridDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFpointsDataFrame,RFpointsDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFspatialGridDataFrame,RFspatialGridDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFspatialGridDataFrame,RFspatialPointsDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFspatialPointsDataFrame,RFspatialGridDataFrame'
plot(x, y, ...)
## S4 method for signature 'RFspatialPointsDataFrame,RFspatialPointsDataFrame'
plot(x, y, ...)

## S4 method for signature 'RFspatialGridDataFrame'
persp(x, ..., zlab="")
## S3 method for class 'RFspatialGridDataFrame'
contour(x, ...)

Arguments

x

object of class RFsp or RMmodel; in the latter case, x can be any sophisticated model but it must be either stationary or a variogram model

y

ignored in most methods; in case of RFplotSimulation data might be given

MARGIN

vector of two; two integer values giving the coordinate dimensions w.r.t. whether the field or the covariance model is to be plotted; in all other directions, the first index is taken

MARGIN.slices

integer value; if [spacetimedimension>2][space-time-dimension>2], MARGIN.slices can specify a third dimension w.r.t. which a sequence of slices is plotted. Currently only works for grids.

n.slices

integer value. The number of slices to be plotted; if n.slices>1, nmax is set to 1. Or n.slices is a vector of 3 elements: start, end, length. Currently only works for grids.

nmax

the maximal number of the [email protected]$n iid copies of the field that are to be plotted

MARGIN.movie

integer. If given a sequence of figures is shown for this direction. This option is in an experimental stage. It works only for grids.

file, speed, height.pixel, width.pixel

In case MARGIN.movie and file is given an 'avi' movie is stored using the mencoder command with speed argument speed. As temporary files file__###.png of size width.pixel x height.pixel are created.

...

arguments to be passed to methods; mainly graphical arguments, or further models in case of class CLASS_CLIST, see Details.

plot.variance

logical, whether variances should be plotted if available

select.variables

vector of integers or list of vectors. The argument is only of interest for multivariate models. Here, length(select.variables) gives the number of pictures shown (excluding the plot for the variances, if applicable). If select.variables is a vector of integers then exactly these components are shown. If select.variables is a list, each element should be a vector up to length l3l\le 3:

  • l=1l=1
    the component is shown in the usual way

  • l=2l=2
    the two components are interpreted as vector and arrows are plotted

  • l=3l=3
    the first component is shown as single component; the remaining two component are interpreted as a vector and plotted into the picture of the first component

legend

logical, whether a legend should be plotted

zlim

vector of length 2 with the usual meaning. In case of multivariate random fields, zlim can also be a character with the value ‘joint’ indicating that all plotted components shall have the same zlim OR a matrix with two rows, where the i-th column gives the zlim of the i-th variable OR a list with entries named data and var if a separate zlim for the Kriging variance is to be used.

plotmethod

string or function. Internal.

zlab

character. See persp

Details

Internally, ... are passed to image and plot.default, respectively; if, by default, multiple colors, xlabs or ylabs are used, also vectors of suitable length can be passed as col, xlab and ylab, respectively.

One exception is the use of ... in plot for class CLASS_CLIST. Here, further models might be passed. All models must have names starting with model. If '.' is following in the name, the part of the name after the dot is shown in the legend. Otherwise the name is ignored and a standardized name derived from the model definition is shown in the legend. Note that for the first argument a name cannot be specified.

Methods

signature(x = "RFspatialGridDataFrame", y = "missing")

Generates nice image plots of simulation results for simulation on a grid and space-time-dimension 2\ge 2. If space-time-dimension 3\ge 3, plots are on 2-dimensional subspaces. Handles multivariate random fields (.RFparams$vdim>1) as well as repeated iid simulations (.RFparams$vdim>n).

signature(x = "RFspatialGridDataFrame", y = "RFspatialPointsDataFrame")

Similar to method for y="missing", but additionally adds the points of y. Requires MARGIN.slices=NULL and all.equal([email protected], [email protected]).

signature(x = "RFspatialGridDataFrame", y = "matrix")

Similar to method for y="missing", but additionally adds the points of y. Requires MARGIN.slices=NULL and all.equal([email protected], [email protected]).

signature(x = "RFspatialPointsDataFrame", y = "RFspatialGridDataFrame")

Throws an error. Probably x and y have been interchanged.

signature(x = "RFspatialPointsDataFrame", y = "missing")

Similar to method for class RFspatialGridDataFrame, but for non-gridded simulation results. Instead of a grid, only existing points are plotted with colors indicating the value of the random field at the respective location. Handles multivariate random fields (.RFparams$vdim>1) as well as repeated iid simulations (.RFparams$vdim>n).

signature(x = "RFspatialPointsDataFrame", y = "RFspatialPointsDataFrame")

Similar to method for y="missing", but additionally adds the points of y. Requires all.equal([email protected], [email protected]).

signature(x = "RFgridDataFrame", y = "missing")

Generates plots of simulation results for space-time-dimension =1=1. Handles different values for the number of repetitions as well as multivariate responses.

signature(x = "RFpointsDataFrame", y = "missing")

Similar to method for class RFgridDataFrame, but for non-gridded data.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFpar.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## define the model:
model <- RMtrend(mean=0.5) + # mean
         RMstable(alpha=1, var=4, scale=10) + # see help("RMstable")
                                        ## for additional arguments
         RMnugget(var=1) # nugget


#############################################################
## Plot of covariance structure


plot(model)
plot(model, xlim=c(0, 30))
plot(model, xlim=c(0, 30), fct.type="Variogram")
plot(model, xlim=c(-10, 20), fct.type="Variogram", dim=2)
image(model, xlim=c(-10, 20), fct.type="Variogram")
persp(model, xlim=c(-10, 20), fct.type="Variogram")

#############################################################
## Plot of simulation results

## define the locations:
from <- 0
step <- .1 
len <- 50  # nicer if len=100 %ok
 
x1D <- GridTopology(from, step, len)
x2D <- GridTopology(rep(from, 2), rep(step, 2), rep(len, 2))
x3D <- GridTopology(rep(from, 3), rep(step, 3), rep(len, 3))

## 1-dimensional
sim1D <- RFsimulate(model = model, x=x1D, n=6) 
plot(sim1D, nmax=4)

## 2-dimensional
sim2D <- RFsimulate(model = model, x=x2D, n=6) 
plot(sim2D, nmax=4)
plot(sim2D, nmax=4, col=terrain.colors(64),
main="My simulation", xlab="my_xlab")

## 3-dimensional
model <- RMmatern(nu=1.5, var=4, scale=2)
sim3D <- RFsimulate(model = model, x=x3D) 
plot(sim3D, MARGIN=c(2,3), MARGIN.slices=1, n.slices=4)

 
#############################################################
## empirical variogram plots

x <- seq(0, 10, 0.05)
bin <- seq(from=0, by=.2, to=3)

model <- RMexp()
X <- RFsimulate(model, x=cbind(x))
ev1 <- RFvariogram(data=X, bin=bin)
plot(ev1)

model <- RMexp(Aniso = cbind(c(10,0), c(0,1)))
X <- RFsimulate(model, x=cbind(x,x))
ev2 <- RFvariogram(data=X, bin=bin, phi=3)
plot(ev2, model=list(exp = model))




#############################################################
## plot Kriging results 
model <- RMwhittle(nu=1.2, scale=2)
n <- 200
x <- runif(n, max=step*len/2) 
y <- runif(n, max=step*len/2) # 200 points in 2 dimensional space
sim <- RFsimulate(model, x=x, y=y)

interpolate <- RFinterpolate(model, x=x2D, data=sim)
plot(interpolate)
plot(interpolate, sim)


#############################################################
## plotting vector-valued results
model <- RMdivfree(RMgauss(), scale=4)
x <- y <- seq(-10,10, 0.5)
simulated <- RFsimulate(model, x=x, y=y, n=1)
plot(simulated)
plot(simulated, select.variables=list(1, 1:3, 4))



#############################################################
## options for the zlim argument
model <- RMdelay(RMstable(alpha=1.9, scale=2), s=c(0, 4)) +
         RMdelay(RMstable(alpha=1.9, scale=2), s=c(4, 0))
simu <- RFsimulate(model, x, y)

plot(simu, zlim=list(data=cbind(c(-6,2), c(-2,1)), var=c(5,6)))
plot(simu, zlim=cbind(c(-6,2), c(-2,1)))
plot(simu, zlim=c(-6,2))
plot(simu, zlim="joint")

Information about the implemented covariance models

Description

PrintModelList prints the list of currently implemented models including the corresponding simulation methods.

Usage

PrintModelList(operators=FALSE, internal=FALSE, newstyle=TRUE)

Arguments

operators

logical. Flag whether operators should also be considered.

internal

logical. Flag whether internal models should also be considered. In case of PrintModelList and internal=2, variants of internal models are also printed.

newstyle

logical. If FALSE then only the old style model names (Version 2 and earlier) are shown. These names can still be used in the list definition of models, see RMmodelsAdvanced. If TRUE then the standard names will also be shown.

Details

See RMmodel for a description of the models and their use.

Value

PrintModelList prints a table of the currently implemented covariance functions and the matching methods. PrintModelList returns NULL.

Note

From version 3.0 on, the command PrintModelList() is replaced by the call RFgetModelNames(internal=FALSE).

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFgetModelNames

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
PrintModelList()

Linear part of RMmodel

Description

RFboxcox performs the Box-Cox transformation: (x+μ)λ1λ\frac{(x+\mu)^\lambda-1}{\lambda}

Usage

RFboxcox(data, boxcox, vdim = 1, inverse=FALSE, ignore.na=FALSE)

Arguments

data

matrix or list of matrices.

boxcox

the one or two parameters (λ,μ)(\lambda, \mu) of the box cox transformation, in the univariate case; if μ\mu is not given, then μ\mu is set to 00. If not given, the globally defined parameters are used, see Details. In the mm-variate case boxcox should be a 2×m2 \times m matrix. If λ=\lambda =\infty then no transformation is performed.

vdim

the multivariate dimensionality of the field;

inverse

logical. Whether the inverse transformation should be performed.

ignore.na

logical. If FALSE an error message is returned if any value of boxcox is NA. Otherwise the data are returned without being transformed.

Details

The Box-Cox transfomation boxcox can be set globally through RFoptions. If it is set globally the transformation applies in the Gaussian case to RFfit, RFsimulate, RFinterpolate, RFvariogram. Always first, the Box-Cox transformation is applied to the data. Then the command is performed. The result is back-transformed before returned.

If the first value of the transformation is Inf no transformation is performed (and is identical to boxcox = c(1,0)). If boxcox has length 1, then the transformation parameter μ\mu is set to 00, which is the standard case.

Value

RFboxcox returns a list of three components, Y, X, vdim returning the deterministic trend, the design matrix, and the multivariability, respectively. If set is positive, Y and X contain the values for the set-th set of coordinates. Else, Y and X are both lists containing the values for all the sets.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

For the likelihood correction see

  • Konishi, S., and Kitagawa, G. (2008) Information criteria and statistical modeling. Springer Science & Business Media. Section 4.9.

See Also

Bayesian, RMmodel, RFsimulate, RFlikelihood.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

data(soil)
str(soil)
soil <- RFspatialPointsDataFrame(
 coords = soil[ , c("x.coord", "y.coord")],
 data = soil[ , c("moisture", "NO3.N", "Total.N", "NH4.N", "DOC", "N20N")],
 RFparams=list(vdim=6, n=1)
)
dta <- soil["moisture"]


model <- ~1 + RMplus(RMwhittle(scale=NA, var=NA, nu=NA), RMnugget(var=NA))



## main Parameter in the Box Cox transformation to be estimated
print(fit <- RFfit(model, data=dta, boxcox=NA))

(Cross-)Covariance function

Description

Calculates both the empirical and the theoretical (cross-)covariance function.

Usage

RFcov(model, x, y = NULL, z = NULL, T=NULL, grid, params, distances, dim, ...,
      data, bin=NULL, phi=NULL, theta = NULL, deltaT = NULL, vdim=NULL)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

bin

a vector giving the borders of the bins; If not specified an array describing the empirical (pseudo-)(cross-) covariance function in every direction is returned.

phi

an integer defining the number of sectors one half of the X/Y plane shall be divided into. If not specified, either an array is returned (if bin missing) or isotropy is assumed (if bin specified).

theta

an integer defining the number of sectors one half of the X/Z plane shall be divided into. Use only for dimension d=3d=3 if phi is already specified.

deltaT

vector of length 2, specifying the temporal bins. The internal bin vector becomes seq(from=0, to=deltaT[1], by=deltaT[2])

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

vdim

the number of variables of a multivariate data set. If not given and data is an RFsp object created by RandomFields, the information there is taken from there. Otherwise vdim is assumed to be one. NOTE: still the argument vdim is an experimental stage.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

RFcov computes the empirical cross-covariance function for given (multivariate) spatial data.

The empirical (cross-)covariance function of two random fields XX and YY is given by

γ(r):=1N(r)(ti,tj)ti,j=r(X(ti)Y(tj))mXmY\gamma(r):=\frac{1}{N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} (X(t_{i})Y(t_{j})) - m_{X} m_{Y}

where ti,j:=titjt_{i,j}:=t_{i}-t_{j}, N(r)N(r) denotes the number of pairs of data points with distancevector ti,j=rt_{i,j}=r and where mX:=1N(r)(ti,tj)ti,j=rXtim_{X} := \frac{1}{N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} X_{t_{i}} and mY:=1N(r)(ti,tj)ti,j=rYtim_{Y} := \frac{1}{N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} Y_{t_{i}} denotes the mean of data points with distancevector ti,j=rt_{i,j}=r.

The spatial coordinates x, y, z should be vectors. For random fields of spatial dimension d>3d > 3 write all vectors as columns of matrix x. In this case do neither use y, nor z and write the columns in gridtriple notation.

If the data is spatially located on a grid a fast algorithm based on the fast Fourier transformed (fft) will be used. As advanced option the calculation method can also be changed for grid data (see RFoptions.)

It is also possible to use RFcov to calculate the pseudocovariance function (see RFoptions).

Value

RFcov returns objects of class RFempVariog.

Author(s)

Jonas Auel; Sebastian Engelke; Johannes Martini; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RFvariogram, RFmadogram, RMstable, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

n <- 1 ## use n <- 2 for better results

## isotropic model
model <- RMexp()
x <- seq(0, 10, 0.02)
z <- RFsimulate(model, x=x, n=n)
emp.vario <- RFcov(data=z)
plot(emp.vario, model=model)


## anisotropic model
model <- RMexp(Aniso=cbind(c(2,1), c(1,1)))
x <- seq(0, 10, 0.05)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFcov(data=z, phi=4)
plot(emp.vario, model=model)


## space-time model
model <- RMnsst(phi=RMexp(), psi=RMfbm(alpha=1), delta=2)
x <- seq(0, 10, 0.05)
T <- c(0, 0.1, 100)
z <- RFsimulate(x=x, T=T, model=model, n=n)
emp.vario <- RFcov(data=z, deltaT=c(10, 1))
plot(emp.vario, model=model, nmax.T=3)


## multivariate model
model <- RMbiwm(nudiag=c(1, 2), nured=1, rhored=1, cdiag=c(1, 5), 
                s=c(1, 1, 2))
x <- seq(0, 20, 0.1)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFcov(data=z)
plot(emp.vario, model=model)


## multivariate and anisotropic model
model <- RMbiwm(A=matrix(c(1,1,1,2), nc=2),
                nudiag=c(0.5,2), s=c(3, 1, 2), c=c(1, 0, 1))
x <- seq(0, 20, 0.1)
dta <- RFsimulate(model, x, x, n=n)
ev <- RFcov(data=dta, phi=4)
plot(ev, model=model, boundaries=FALSE)

Covariance matrix

Description

RFcovmatrix returns the covariance matrix for a set of points;

Usage

RFcovmatrix(model, x, y = NULL, z = NULL, T = NULL, grid, params,
            distances, dim,...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

RFcovmatrix returns a covariance matrix. Here, a matrix of coordinates (x) or a vector or a matrix of distances is expected.

RFcovmatrix also allows for variogram models. Then the negative of the variogram matrix is returned.

Value

RFcovmatrix returns a covariance matrix.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFsimulate, RFfit, RFfctn, RFcalc, RFcov, RFpseudovariogram, RFvariogram.

Examples

##################################################
# Example: get covariance matrix C(x_i,x_j)    
# at given locations x_i, i=1,...,n 
#
# here for an isotropic stationary covariance model
# yields a 4 times 4 covariance matrix of the form
# C(0)   C(5)   C(3)   C(2.5)
# C(5)   C(0)   C(4)   C(2.5)
# C(3)   C(4)   C(0)   C(2.5)
# C(2.5) C(2.5) C(2.5) C(0)

model <- RMexp() # the covariance function C(x,y)=C(r) of this model
#                  depends only on the distance r between x and y
RFcovmatrix(model=model, distances=c(5,3,2.5,4,2.5,2.5), dim=4)

Fitting model parameters to spatial data (regionalised variables) and to linear (mixed) models

Description

The function estimates arbitrary parameters of a random field specification with various methods. Currently, the models to be fitted can be

The fitting of max-stable random fields and others has not been implemented yet.

Usage

RFcrossvalidate(model, x, y=NULL, z=NULL, T=NULL, grid=NULL, data,
                params, lower=NULL, upper=NULL, method="ml",
                users.guess=NULL, distances=NULL, dim, optim.control=NULL,
                transform=NULL, full = FALSE, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

lower

list or vector. Lower bounds for the parameters. If lower is a vector, lower has to be a vector as well and its length must equal the number of parameters to be estimated. The order of lower has to be maintained. A component being NA means that no manual lower bound for the corresponding parameter is set.
If lower is a list, lower has to be of (exactly) the same structure of the model.

upper

list or vector. Upper bounds for the parameters. See lower.

method

Single method to be used for estimating, either one of the methods or one of the sub.methods see RFfit

users.guess

User's guess of the parameters. All the parameters must be given using the same rules as for lower (except that no NA's should be contained).

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

optim.control

control list for optim, which uses ‘L-BFGS-B’. However parscale may not be given.

transform

obsolete for users; use param instead. transform=list() will return structural information to set up the correct function.

full

logical. If TRUE then cross-validation is also performed for intermediate models used in RFfit (if any).

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Value

An object of the class "RFcrossvalidate" which is a list with the following components, cf. xvalid in the package geoR :

data

the original data.

predicted

the values predicted by cross-validation.

krige.var

the cross-validation prediction variance.

error

the differences data - predicted value.

std.error

the errors divided by the square root of the prediction variances.

p

In contrast to geoR the p-value is returned, i.e. the probability that a difference with absolute value larger than the absolute value of the actual difference is observed.

A method for summary returns summary statistics for the errors and standard errors similar to geoR.

If cross_refit = TRUE and detailed_output = TRUE the returned object also contains a fitted which is a list of fitted models.

Methods

print

prints the summary

summary

gives a summary

Note

An important option is cross_refit that determines whether the model is refitted for each location left out. Default is FALSE. See also RFoptions.

Note

This function does not depend on the value of RFoptions()$PracticalRange. The function RFcrossvalidate always uses the standard specification of the covariance model as given in RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Ribeiro, P.J., Jr. and Diggle, P.J (2014) R package geoR.

  • Burnham, K. P. and Anderson, D. R. (2002) Model selection and Multi-Model Inference: A Practical Information-Theoretic Approach. 2nd edition. New York: Springer.

See Also

RFratiotest RFfit RMmodel, RandomFields, weather.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


## currently disabled!

Evaluating distribution families

Description

Through RRdistr distribution families can be passed to RandomFields to create distributions available in the RMmodel definitions.

Usage

RFddistr(model, x, params, dim=1, ...)
RFpdistr(model, q, params, dim=1, ...)
RFqdistr(model, p, params, dim=1, ...)
RFrdistr(model, n, params, dim=1, ...)
RFdistr(model, x, q, p, n, params, dim=1, ...)

Arguments

model, params

an RRmodel.

x

the location where the density is evaluated

q

the location where the probability function is evaluated

p

the value where the quantile function is evaluated

n

the number of random values to be drawn

dim

the dimension of the vector to be drawn

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions

Details

RFdistr is the generic function for the 4 functions belonging to a distribution.

Value

as described in the arguments

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RRgauss, RR

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## a very toy example to understand the use
model <- RRdistr(norm())
v <- 0.5
Print(RFdistr(model=model, x=v), dnorm(x=v)) 
Print(RFdistr(model=model, q=v), pnorm(q=v))
Print(RFdistr(model=model, p=v), qnorm(p=v))

n <- 10
r <- RFdistr(model=model, n=n, seed=0)
set.seed(0); Print(r, rnorm(n=n))


## note that a conditional covariance function given the
## random parameters is given here:
model <- RMgauss(scale=exp())
for (i in 1:3) {
  RFoptions(seed = i + 10)
  readline(paste("Model no.", i, ": press return", sep=""))
  plot(model)
  readline(paste("Simulation no.", i, ": press return", sep=""))  
  plot(RFsimulate(model, x=seq(0,10,0.1)))
}

Class RFempVariog

Description

Class for RandomFields' representation of empirical variograms

Usage

RFplotEmpVariogram(x, model = NULL, nmax.phi = NA, nmax.theta = NA,
                    nmax.T = NA,
                     plot.nbin = TRUE, plot.sd=FALSE, method = "ml",
                     variogram=TRUE,
                               boundaries = TRUE,
                               ...)
## S4 method for signature 'RFempVariog,missing'
plot(x, y, ...)
## S4 method for signature 'RFempVariog'
persp(x, ...)

Arguments

x

object of class RFempVariog

y

unused

model

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.. Or a list of such models. Tit gives the covariance or variogram models that are to be plotted into the same plot as the empirical variogram (and the fitted models)

nmax.phi

even integer; only for class(x)=="RFempVariog"; the number of bins of angle phi that are to be plotted

.

nmax.theta

integer; only for class(x)=="RFempVariog"; the number of bins of angle theta that are to be plotted

nmax.T

integer; only for class(x)=="RFempVariog"; the maximal number of different time bins that are to be plotted

plot.nbin

logical; only for class(x)=="RFempVariog"; indicates whether the number of pairs per bin are to be plotted

plot.sd

logical; only for class(x)=="RFempVariog"; indicates whether the calculated standard deviation (x@sd) is to be plotted (in form of arrows of length +-1*sd)

method

character. Currently restricted to "ml" for maximum-likelihood method.

variogram

logical; This argument should currently not be set by the user. If TRUE then the empirical variogram is plotted, else an estimate for the covariance function.

boundaries

logical; only for class(x)=="RFempVariog" and the anisotropic case where model is given. As the empirical variogram is calculated on a sector of angles, no exact variogram curve corresponds to the mean values in this sector. If boundaries=TRUE the values of the variogram on the sector boundaries are plotted. If FALSE some kind of mean model values are plotted. Neither the boundaries may contain the values of empirical variogram nor does the mean values need to be close the empirical variogram.

...

arguments to be passed to methods; mainly graphical arguments.

Slots

centers:

the bin centres of the spatial distances

empirical:

value of the empirical variogram

var:

the empirical (overall) variance in the data

sd:

standard deviation of the variogram cloud within each bin

n.bin:

number of bins

phi.centers:

centres of the bins with respect to the (first) angle (for anisotropic empirical variograms only)

theta.centers:

centres of the bins with respect to the second angle (for anisotropic empirical variograms in 3D only)

T:

the bin centres of the time axis

vdim:

the multivariate dimension

coordunits:

string giving the units of the coordinates, see also option coordunits of RFoptions.

varunits:

string giving the units of the variables, see also option varunits of RFoptions.

call:

language object; the function call by which the object was generated

method:

integer; variogram (0), covariance (2), madogram (4)

Methods

plot

signature(x = "RFempVariog"): gives a plot of the empirical variogram, for more details see plot-method.

plot

signature(x = "RFempVariog", y = "missing")

Gives nice plots of the empirical variogram; handles binning in up to three space-dimensions and a time-dimension, where the empirical variogram is plotted along lines which are directed according to the angle-centers given in [email protected] and [email protected]; arbitrary theoretical model curves can be added to the plot by using the argument model. If no bins are given, i.e. (x@bin=NULL), image-plots are generated.

as

signature(x = "RFempVariog"): converts into other formats, only implemented for target class list.

show

signature(x = "RFfit"): returns the structure of x

persp

signature(obj = "RFempVariog"): generates nice persp plots

print

signature(x = "RFfit"): identical with show-method

summary

provides a summary

Details

print returns also an invisible list that is convenient to access.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFvariogram, plot-method

Examples

#  see 'RFvariogram'

Evaluate Covariance and Variogram Functions

Description

RFfctn returns the values of a shape function.

Usage

RFfctn(model, x, y = NULL, z = NULL, T = NULL, grid, params, distances, dim,...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

RFcovmatrix also allows for variogram models. Then the negative of the variogram matrix is returned.

Value

RFfctn returns a vector.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFsimulate, RFfit, RFcalc, RFcov, RFcovmatrix, RFpseudovariogram, RFvariogram.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp() - 1
RFfctn(model, 1:10)

Fitting model parameters to spatial data (regionalised variables) and to linear (mixed) models

Description

The function estimates arbitrary parameters of a random field specification with various methods. Currently, the models to be fitted can be

The fitting of max-stable random fields and others has not been implemented yet.

Usage

RFfit(model, x, y = NULL, z = NULL, T = NULL, grid=NULL, data,
      lower = NULL, upper = NULL, methods,
      sub.methods, optim.control = NULL, users.guess = NULL,
      distances = NULL, dim, transform = NULL, params=NULL, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

All parameters that are set to NA will be estimated; see the examples below.

Type RFgetModelNames(type="variogram") to get all options for model.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

lower

list or vector. Lower bounds for the parameters. If lower is a vector, lower has to be a vector as well and its length must equal the number of parameters to be estimated. The order of lower has to be maintained. A component being NA means that no manual lower bound for the corresponding parameter is set.
If lower is a list, lower has to be of (exactly) the same structure of the model.

upper

list or vector. Upper bounds for the parameters. See lower.

methods

Main methods to be used for estimating. If several methods are given, estimation will be performed with each method and the results reported.

sub.methods

variants of the least squares fit of the variogram. variants of the maximum likelihood fit of the covariance function.. See Details.

users.guess

User's guess of the parameters. All the parameters must be given using the same rules as for lower (except that no NA's should be contained).

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

optim.control

control list for optim, which uses ‘L-BFGS-B’. However parscale may not be given.

transform

obsolete for users; use param instead. transform=list() will return structural information to set up the correct function.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

For details on the simulation methods see

If x-coordinates are not given, the function will check data for NAs and will perform imputing.

The function has many more options to tune the optimizer, see RFoptions for details.

If the model defines a Gaussian random field, the options for methods and submethods are currently "ml" and c("self", "plain", "sqrt.nr", "sd.inv", "internal"), respectively.

Value

The result depends on the logical value of spConform. If TRUE, an S4 object is created. In case the model indicates a Gaussian random field, an RFfit object is created.

If spConform=FALSE, a list is returned. In case the model indicates a Gaussian random field, the details are given in fitgauss.

Note

  • An important optional argument is boxcox which indicates a Box-Cox transformation; see boxcox in RFoptions and RFboxcox for details.

  • Instead of optim, other optimisers can be used, see RFfitOptimiser.

  • Several advanced options can be found in sections ‘General options’ and ‘fit’ of RFoptions.

  • In particular, boxcox, boxcox_lb, boxcox_ub allow Box-Cox transformation.

  • This function does not depend on the value of RFoptions()$PracticalRange. The function RFfit always uses the standard specification of the covariance model as given in RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Burnham, K. P. and Anderson, D. R. (2002) Model selection and Multi-Model Inference: A Practical Information-Theoretic Approach. 2nd edition. New York: Springer.

See Also

RFfitOptimiser, RFlikelihood, RFratiotest, RMmodel, RandomFields, weather.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions(modus_operandi="sloppy")


#########################################################
## simulate some data first                            ## 
points <- 100
x <- runif(points, 0, 3)
y <- runif(points, 0, 3) ## random points in square [0, 3]^2
model <- RMgencauchy(alpha=1, beta=2)
d <- RFsimulate(model, x=x, y=y, grid=FALSE, n=100) #1000


#########################################################
## estimation; 'NA' means: "to be estimated"           ##
estmodel <- RMgencauchy(var=NA, scale=NA, alpha=NA, beta=2) +
            RMtrend(mean=NA)
RFfit(estmodel, data=d)


#########################################################
## coupling alpha and beta                             ##
estmodel <- RMgencauchy(var=NA, scale=NA, alpha=NA, beta=NA) + 
            RMtrend(NA)
RFfit(estmodel, data=d, transform = NA) ## just for information
trafo <- function(a) c(a[1], rep(a[2], 2))
fit <- RFfit(estmodel, data=d,
             transform = list(c(TRUE, TRUE, FALSE), trafo))
print(fit)
print(fit, full=TRUE)

Class RFfit

Description

Class for RandomFields' representation of model estimation results

Usage

## S4 method for signature 'RFfit'
residuals(object, ..., method="ml", full=FALSE)
## S4 method for signature 'RFfit'
summary(object, ..., method="ml")
## S4 method for signature 'RFfit,missing'
plot(x, y, ...) 

## S3 method for class 'RFfit'
contour(x, ...) 
## S3 method for class 'RFempVariog'
contour(x, ...)

RFhessian(model)

Arguments

object

see the generic function;

...
  • plot: arguments to be passed to methods; mainly graphical arguments, or further models in case of class CLASS_CLIST, see Details.

  • summary: see the generic function

  • contour : see RFplotEmpVariogram

method

character; only for class(x)=="RFfit"; a vector of slot names for which the fitted covariance or variogram model is to be plotted; should be a subset of slotNames(x) for which the corresponding slots are of class CLASS_FIT; by default, the maximum likelihood fit ("ml") will be plotted

full

logical. if TRUE submodels are reported as well (if available).

x

object of class RFsp or RFempVariog or RFfit or RMmodel; in the latter case, x can be any sophisticated model but it must be either stationary or a variogram model

y

unused

model

class(x)=="RF_fit" or class(x)=="RFfit", obtained from RFfit

Details

for the definition of plot see RFplotEmpVariogram.

Creating Objects

Objects are created by the function RFfit

Slots

autostart:

RMmodelFit; contains the estimation results for the method 'autostart' including a likelihood value, a constant trend and the residuals

boxcox:

logical; whether the parameter of a Box Cox tranformation has been estimated

coordunits:

string giving the units of the coordinates, see also option coordunits of RFoptions.

deleted:

integer vector. Positions of the parameters that have been deleted to get the set of variables, used in the optimization.

ev:

list; list of objects of class RFempVariog, contains the empirical variogram estimates of the data

fixed:

list of two vectors. The fist gives the position where the parameters are set to zero. The second gives the position where the parameters are set to one.

internal1:

RMmodelFit; analog to slot 'autostart'

internal2:

RMmodelFit; analog to slot 'autostart'

internal3:

RMmodelFit; analog to slot 'autostart'

lowerbounds:

RMmodel; covariance model in which each parameter value gives the lower bound for the respective parameter

ml:

RMmodelFit; analog to slot 'autostart'

modelinfo:

table with information on the parameters: name, boundaries, type of parameter

n.covariates:

number of covariates

n.param:

number of parameters (given by the user)

n.variab:

number of variables (used internally); n.variab is always less than or equal to n.param

number.of.data:

the number of data values passed to RFfit that are not NA or NaN

number.of.parameters:

total number of parameters of the model that had to be estimated including variances, scales, co-variables, etc.

p.proj:

vector of integers. The original position of those parameters that are used in the submodel

plain:

RMmodelFit; analog to slot 'autostart'

report:

If not empty, it indicates that this model should be reported and gives a standard name of the model.

Various functions, e.g. print.RMmodelFit, use this information if their argument full equals TRUE.

self:

RMmodelFit; analog to slot 'autostart'

sd.inv:

RMmodelFit; analog to slot 'autostart'

sqrt.nr:

RMmodelFit; analog to slot 'autostart'

submodels:

list. Sequence (in some cases even nested sequence) of models that is used to determine an initial value in

table:

matrix; summary of estimation results of different methods

transform:

function;

true.tsdim:

time space dimension of the (original!) data, even for submodels that consider parts of separable models.

true.vdim:

multivariability of the (original!) data, even for submodels that consider independent models for the multivariate components.

upperbounds:

RMmodel; see slot 'lowerbounds'

users.guess:

RMmodelFit; analog to slot 'autostart'

ml:

RMmodelFit; analog to slot 'autostart'; with maximum likelihood method

v.proj:

vector of integers. The components selected in one of the submodels

varunits:

string giving the units of the variables, see also option varunits of RFoptions.

x.proj:

logical or integer. If logical, it means that no separable model is considered there. If integer, then it gives the considered directions of a separable model.

Z:

standardized list of information on the data

Methods

plot

signature(x = "RFfit"): gives a plot of the empirical variogram together with the fitted model, for more details see plot-method.

show

signature(x = "RFfit"): returns the structure of x

persp

signature(obj = "RFfit"): generates persp plots

print

signature(x = "RFfit"): identical with show-method, additional argument is max.level

[

signature(x = "RFfit"): enables accessing the slots via the "["-operator, e.g. x["ml"]

as

signature(x = "RFfit"): converts into other formats, only implemented for target class RFempVariog

anova

performs a likelihood ratio test base on a chisq approximation

summary

provides a summary

logLik

provides an object of class "logLik"

AIC,BIC

provides the AIC and BIC information, respectively

signature(x = "RFfit", y = "missing")

Combines the plot of the empirical variogram with the estimated covariance or variogram model (theoretical) curves; further models can be added via the argument model.

Further 'methods'

AICc.RFfit(object, ..., method="ml", full=FALSE)

AICc.RF_fit(object, ..., method="ml", full=TRUE)

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

AICc:

  • Hurvich, C.M. and Tsai, C.-L. (1989) Regression and Time Series Model Selection in Small Samples Biometrika, 76, 297-307.

See Also

RFfit, RFvariogram, RMmodel-class, RMmodelFit-class, plot-method.

Examples

# see RFfit

Optimisers for fitting model parameters to spatial data

Description

See RFfit for a detailed description of the fitting procedure.

Details

Two parameters, see also RFoptions can be passed to RFfit that allow for choosing an optimiser different from optim:

optimiser takes one of the values "optim", "optimx", "soma", "nloptr", "GenSA", "minqa", "pso" or "DEoptim", see the corresponding packages for a description.

If optimiser="nloptr", then the additional parameter algorithm must be given which takes the values "NLOPT_GN_DIRECT", "NLOPT_GN_DIRECT_L", "NLOPT_GN_DIRECT_L_RAND", "NLOPT_GN_DIRECT_NOSCAL", "NLOPT_GN_DIRECT_L_NOSCAL", "NLOPT_GN_DIRECT_L_RAND_NOSCAL", "NLOPT_GN_ORIG_DIRECT", "NLOPT_GN_ORIG_DIRECT_L", "NLOPT_LN_PRAXIS", "NLOPT_GN_CRS2_LM", "NLOPT_LN_COBYLA", "NLOPT_LN_NELDERMEAD", "NLOPT_LN_SBPLX", "NLOPT_LN_BOBYQA", "NLOPT_GN_ISRES", see nloptr for a description.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFfit, RFoptions

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Not run: 
## Here some alternative optimisers to 'optim' are considered.
## All but the \pkg{nloptr} algorithms are largely slower than 'optim'.
## Only a few of them return results as good as 'optim'.

data(soil)
str(soil)
soil <- RFspatialPointsDataFrame(
 coords = soil[ , c("x.coord", "y.coord")],
 data = soil[ , c("moisture", "NO3.N", "Total.N", "NH4.N", "DOC", "N20N")],
 RFparams=list(vdim=6, n=1)
)
dta <- soil["moisture"]
\dontshow{if (RFoptions()$internal$examples_red) {
  warning("data have been reduced !")
  All <- 1:7 
  rm(soil)
  data(soil)
  soil <- RFspatialPointsDataFrame(
     coords = soil[All, c("x.coord", "y.coord")],
     data = soil[All, c("moisture", "NO3.N", "Total.N",
      "NH4.N", "DOC", "N20N")],
      RFparams=list(vdim=6, n=1)
  )
  dta <- soil["moisture"]
}}

model <- ~1 + RMwhittle(scale=NA, var=NA, nu=NA) + RMnugget(var=NA)
\dontshow{if (RFoptions()$internal$examples_red){model<-~1+RMwhittle(scale=NA,var=NA,nu=1/2)}}
## standard optimiser 'optim'
print(system.time(fit <- RFfit(model, data=dta)))
print(fit)

opt <- "optimx" #  30 sec; better result
print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt))))
print(fit2)

\dontshow{\dontrun{ 
opt <- "soma" #  450 sec 
print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt))))
print(fit2)
}}

opt <- "minqa" # 330 sec 
print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt))))
print(fit2)


opt <- "nloptr"
algorithm <- RC_NLOPTR_NAMES
\dontshow{if(!interactive()) algorithm <- RC_NLOPTR_NAMES[1]}
for (i in 1:length(algorithm)) { 
  print(algorithm[i])
  print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt,
                                    algorithm=algorithm[i]))))
  print(fit2)
}



if (interactive()) {
## the following two optimisers are too slow to be run on CRAN.

opt <- "pso" # 600 sec
print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt))))
print(fit2)

opt <- "GenSA" #  10^4 sec
print(system.time(fit2 <- try(RFfit(model, data=dta, optimiser=opt))))
print(fit2)
}

## End(Not run)

RFformula - syntax to design random field models with trend or linear mixed models

Description

It is described how to create a formula, which, for example, can be used as an argument of RFsimulate and RFfit to simulate and to fit data according to the model described by the formula.

In general, the created formula serves two purposes:

  • to describe models in the “Linear Mixed Models”-framework

  • to define models for random fields including trend surfaces from a geostatistical point of view.

Thereby, fixed effects and trend surfaces can be adressed via the expression RMfixed and the function RMtrend. In simple cases, the trend can also be given in a very simple, see the examples below. The covariance structures of the zero-mean multivariate normally distributed random field components are adressed by objects of class RMmodel, which allow for a very flexible covariance specification.

See RFformulaAdvanced for rather complicated model definitions.

Details

The formula should be of the type

response fixedeffects+errortermresponse ~ fixed effects %+ random effects + error term

or

response trend+zeromeanrandomfield+nuggeteffect,response ~ trend + zero-mean random field + nugget effect,

respectively.

Thereby:

  • response
    optional; name of response variable

  • fixed effects/trend:
    optional, should be a sum (using +) of components either of the form X@RMfixed(beta) or RMtrend(...) with XX being a design matrix and β\beta being a vector of coefficients (see RMfixed and RMtrend).
    Note that a fixed effect of the form XX is interpreted as X@RMfixed(beta=NA) by default (and β\beta is estimated provided that the formula is used in RFfit).

  • error term/nugget effect
    optional, should be of the form RMnugget(...). RMnugget describes a vector of iid Gaussian random variables.

IMPORTANT

Note that in formula constants are interpreted as part of a linear model, i.e. the corresponding parameter has to be estimated (e.g. ~ 1 + ...) whereas in models not given as formula the parameters to be estimated must be given explicitly.

Note

(additional) argument names should always start with a capital letter. Small initial letters are reserved for RFoptions.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and P. Delfiner (1999) Geostatistics. Modeling Spatial Uncertainty. New York, Chichester: John Wiley & Sons.

  • McCulloch, C. E., Searle, S. R. and Neuhaus, J. M. (2008) Generalized, linear, and mixed models. Hoboken, NJ: John Wiley & Sons.

  • Ruppert, D. and Wand, M. P. and Carroll, R. J. (2003) Semiparametric regression. Cambridge: Cambridge University Press.

See Also

RMmodel, RFsimulate, RFfit, RandomFields.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions(modus_operandi="sloppy")

##############################################################
#
# Example  : Simulation and fitting of a two-dimensional
# Gaussian random field with exponential covariance function
#
###############################################################

V <- 10
S <- 0.3
M <- 3
model <- RMexp(var=V, scale=S) + M
x <- y <- seq(1, 3, 0.1)

simulated <- RFsimulate(model = model, x=x, y=y)
plot(simulated)


# an alternative code to the above code:
model <- ~ Mean + RMexp(var=Var, scale=Sc)
simulated2 <- RFsimulate(model = model,x=x, y=y, Var=V, Sc=S, Mean=M)
plot(simulated2)


# a third way of specifying the model using the argument 'param'
# the initials of the variables do not be captical letters
model <- ~ M + RMexp(var=var, scale=sc)
simulated3 <- RFsimulate(model = model,x=x, y=y,
                         param=list(var=V, sc=S, M=M))
plot(simulated3)


# Estimate parameters of underlying covariance function via
# maximum likelihood
model.na <- ~ NA + RMexp(var=NA, scale=NA)
fitted <- RFfit(model=model.na, data=simulated)

# compare sample mean of data with ML estimate, which is very similar:
mean(simulated@data[,1]) 
fitted

Advanced RFformula

Description

Here examples for much more advanced formula are given

Note

NaN, in contrast to NA, signifies a unknown parameter that can be calculated from other (unknown) parameters.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

#################################################################
### the following definitions are needed in all the examples  ###
#################################################################
V <- 10
S <- 0.3
M <- 3
x <- y <- seq(1, 3, 0.1)


#################################################################
###       Example 1: simple example                          ###
#################################################################

## the following to definitions of a model and call of RFsimulate
## give the same result:
model <- RMexp(var=V, scale=S) + M
z1 <- RFsimulate(model = model, x=x, y=y)
plot(z1)


model <- ~ M + RMexp(var=var, scale=sc)
p <- list(var=V, sc=S, M=M)
z2 <- RFsimulate(model = model,x=x, y=y, param=p)
plot(z2)



#################################################################
###       Example 2: formulae within the parameter list       ###
#################################################################

## free parameters (above 'var' and 'sc') can be used
## even within the definition of the list of 'param'eters
model <- ~ RMexp(var=var, sc=sc) + RMnugget(var=nugg)
p <- list(var=V, nugg= ~ var * abs(cos(sc)), sc=S) ## ordering does not matter!
z1 <- RFsimulate(model, x, y, params=p)
plot(z1)
RFgetModel(RFsimulate) ## note that V * abs(cos(S) equals  9.553365

## so the above is equivalent to
model <- ~ RMexp(var=var, sc=sc) + RMnugget(var=var * abs(cos(sc)))
z2 <- RFsimulate(model, x, y, params=list(var=V, sc=S))
plot(z2)



#################################################################
###     Example 3: formulae for fitting (i.e. including NAs)  ###
#################################################################
## first generate some data
model <- ~ RMexp(var=var, sc=sc) + RMnugget(var=nugg)
p <- list(var=V, nugg= ~ var * abs(cos(sc)), sc=S) 
z <- RFsimulate(model, x, y, params=p, n=10)

## estimate the parameters
p.fit <- list(sc = NA, var=NA, nugg=NA)
print(f <- RFfit(model, data=z, params=p.fit))

## estimation with a given boundaries for the scale
p.fit <- list(sc = NA, var=NA, nugg=NA)
lower <- list(sc=0.01)
upper <- list(sc=0.02)
print(f <- RFfit(model, data=z, params=p.fit, lower = lower, upper = upper))




#################################################################
###   Example 4 (cont'd Ex 3): formulae with dummy variables  ###
#################################################################
V <- 10
S <- 0.3
M <- 3
x <- y <- seq(1, 3, 0.1)

model <- ~  RMexp(sc=sc1, var=var) + RMgauss(var=var2, sc=sc2) +
            RMdeclare(u) ## introduces dummy variable 'u'
p.fit <- list(sc1 = NA, var=NA, var2=~2 * u, sc2 = NA, u=NA)
lower <- list(sc1=20, u=5)
upper <- list(sc2=1.5, sc1=100, u=15)
print(f <- RFfit(model, data=z, params=p.fit, lower = lower, upper = upper
                 ))

RFfractaldimension

Description

The function estimates the fractal dimension of a process

Usage

RFfractaldim(x, y = NULL, z = NULL, data, grid, 
 bin=NULL,
 vario.n=5,
 sort=TRUE,
 fft.m = c(65, 86), ## in % of range of l.lambda
 fft.max.length=Inf,
 fft.max.regr=150000,
 fft.shift = 50, # in %; 50:WOSA; 100: no overlapping
 method=c("variogram", "fft"), 
 mode = if (interactive ()) c("plot", "interactive") else "nographics", 
 pch=16, cex=0.2, cex.main=0.85,
 printlevel = RFoptions()$basic$printlevel,
 height=3.5,
 ...)

Arguments

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced. If x is not given and data is not an sp object, a grid with unit grid length is assumed

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

data

the values measured; it can also be an sp object

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

bin

sequence of bin boundaries for the empirical variogram

vario.n

first vario.n values of the empirical variogram are used for the regression fit that are not NA.

sort

If TRUE then the coordinates are permuted such that the largest grid length is in x-direction; this is of interest for algorithms that slice higher dimensional fields into one-dimensional sections.

fft.m

numeric vector of two components; interval of frequencies for which the regression should be calculated; the interval is given in percent of the range of the frequencies in log scale.

fft.max.length

The first dimension of the data is cut into pieces of length fft.max.length. For each piece the FFT is calculated and then the average for all pieces is taken. The pieces may overlap, see the argument fft.shift.

fft.max.regr

If the fft.m is too large, parts of the regression fit will take a very long time. Therefore, the regression fit is calculated only if the number points given by fft.m is less than fft.max.regr.

fft.shift

This argument is given in percent [of fft.max.length] and defines the overlap of the pieces defined by fft.max.length. If fft.shift=50 the WOSA estimator is given; if fft.shift=100 no overlap exists.

method

list of implemented methods to calculate the fractal dimension; see Details

mode

character. A vector with components 'nographics', 'plot' or 'interactive':

'nographics'

no graphical output

'plot'

the regression line is plotted

'interactive'

the regression domain can be chosen interactively

Usually only one mode is given. Two modes may make sense in the combination c("plot", "interactive"). In this case, all the results are plotted first, and then the interactive mode is called. In the interactive mode, the regression domain is chosen by two mouse clicks with the left mouse; a right mouse click leaves the plot.

pch

vector or scalar; sign by which data are plotted.

cex

vector or scalar; size of pch.

cex.main

The size of the title in the regression plots.

printlevel

integer. If printlevel is 0 nothing is printed. If printlevel=1 error messages are printed. If printlevel=2 warnings and the regression results are given. If printlevel>2 tracing information is given.

height

height of the graphics window

...

graphical arguments

Details

The function calculates the fractal dimension by various methods:

  • variogram method

  • Fourier transform

Value

The function returns a list with elements vario, fft corresponding to the 2 methods given in the Details.

Each of the elements is itself a list that contains the following elements.

x

the x-coordinates used for the regression fit

y

the y-coordinates used for the regression fit

regr

the return list of the lm.

sm

smoothed curve through the (x,y) points

x.u

NULL or the restricted x-coordinates given by the user in the interactive plot

y.u

NULL or y-coordinates according to x.u

regr.u

NULL or the return list of lm for x.u and y.u

D

the fractal dimension

D.u

NULL or the fractal dimension corresponding to the user's regression line

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

variogram method

  • Constantine, A.G. and Hall, P. (1994) Characterizing surface smoothness via estimation of effective fractal dimension. J. R. Statist. Soc. Ser. B 56, 97-113.

fft

  • Chan, Hall and Poskitt (1995)

See Also

RMmodel, RFhurst

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0, 10, 0.001)
z <- RFsimulate(RMexp(), x)
RFfractaldim(data=z)

Evaluation operators (RF commands)

Description

Here, all the RF_name_ commands are listed.

Functionals of RMmodels

The user's RMmodel is supplemented internally by operators that are tacitely assumed, e.g. RPgauss.

Further completions of the user's model determine what should be done with the model, e.g. calculation of the covariance (RFcov). The following list gives those RFfunctions that have an internal representation as completion to the user's model.

RFcalc performs some simple calculations based on R.models
RFcov assigns to a covariance model the covariance values at given locations
RFcovmatrix assigns to a covariance model the matrix of covariance values at given locations
RFdistr generic function assigning to a distribution family various values of the distribution
RFfctn assigns to a model the value of the function at given locations. In case of a covariance model RFfctn is identical to RFcov.
RFlikelihood assigns to a model and a dataset the (log)likelihood value.
RFlinearpart assigns to a model and a set of coordinates the linear part of the model, i.e. the deterministic trend and the design matrix.
RFpseudovariogram assigns to a model the values of the pseudo variogram at given locations
RFsimulate assigns to a model a realisation of the corresponding random field
RFvariogram assigns to a model the values of the (cross-)variogram at given locations

Estimation and Inference

RFcrossvalidate cross validation for Gaussian fields
RFvariogram empirical variogram
RFfit (maximum likelihood) fitting of the parameters
RFinterpolate 'kriging' and 'imputing'
RFratiotest likelihood ratio test for Gaussian fields

Graphics for Gaussian fields

RFgui educational tool for
* manual selection of a covariance model
* manual fitting to the empirical variogram
RFfractaldim determination of the fractal dimension
RFhurst determination of the Hurst effect (long range dependence)

Coordinate transformations

RFearth2cartesian transformation of earth coordinates to cartesian coordinates
RFearth2dist transformation of earth coordinates to Euclidean distances

Information from and to RandomFields

RFgetMethodNames currently implemented list of simulation methods
RFgetModel returns the model used in a RFfunction, with some more details
RFgetModelInfo similar to RFgetModel, but with detailed information on the implementation
RFgetModelNames lists the implemented models
RFoptions options of package RandomFields

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RC, RM, RP, RR, R., RMmodelgenerator

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

z <- RFsimulate(model=RMexp(), 1:10)
RFgetModel(RFsimulate, show.call = TRUE)  # user's definition
RFgetModel(RFsimulate, show.call = FALSE) # main internal part

Simulation Techniques

Description

RFgetMethodNames prints and returns a list of currently implemented methods for simulating Gaussian random fields and max stable random fields

Usage

RFgetMethodNames()

Details

By default, RFsimulate automatically chooses an appropriate method for simulation. The method can also be set explicitly by the user via RFoptions, in particular by passing gauss.method=_a valid method string_ as an additional argument to RFsimulate or by globally changing the options via RFoptions(gauss.method=_a valid method string_). The following methods are available:

  • (random spatial) Averages
    – details soon

  • Boolean functions.
    See marked point processes.

  • circulant embedding.
    Introduced by Dietrich & Newsam (1993) and Wood and Chan (1994).

    Circulant embedding is a fast simulation method based on Fourier transformations. It is garantueed to be an exact method for covariance functions with finite support, e.g. the spherical model.

    See also cutoff embedding and intrinsic embedding for variants of the method.

  • cutoff embedding.
    Modified circulant embedding method so that exact simulation is guaranteed for further covariance models, e.g. the whittle matern model. In fact, the circulant embedding is called with the cutoff hypermodel, see RMmodel, and A=BA=B there. cutoff embedding halfens the maximum number of elements models used to define the covariance function of interest (from 10 to 5).

    Here, multiplicative models are not allowed (yet).

  • direct matrix decomposition.
    This method is based on the well-known method for simulating any multivariate Gaussian distribution, using the square root of the covariance matrix. The method is pretty slow and limited to about 8000 points, i.e. a 20x20x20 grid in three dimensions. This implementation can use the Cholesky decomposition and the singular value decomposition. It allows for arbitrary points and arbitrary grids.

  • hyperplane method.
    The method is based on a tessellation of the space by hyperplanes. Each cell takes a spatially constant value of an i.i.d. random variables. The superposition of several such random fields yields approximatively a Gaussian random field.

  • intrinsic embedding.
    Modified circulant embedding so that exact simulation is guaranteed for further variogram models, e.g. the fractal brownian one. Note that the simulated random field is always non-stationary. In fact, the circulant embedding is called with the Stein hypermodel, see RMmodel, and A=BA=B there.

    Here, multiplicative models are not allowed (yet).

  • Marked point processes.
    Some methods are based on marked point process Π=[xi,mi]\Pi=\bigcup [x_i,m_i] where the marks mim_i are deterministic or i.i.d. random functions on RdR^d.

    • add.MPP (Random coins).
      Here the functions are elements of the intersection L1L2L_1 \cap L_2 of the Hilbert spaces L1L_1 and L2L_2. A random field Z is obtained by adding the marks:

      Z()=[xi,mi]Πmi(xi)Z(\cdot) = \sum_{[x_i,m_i] \in \Pi} m_i(\cdot - x_i)

      In this package, only stationary Poisson point fields are allowed as underlying unmarked point processes. Thus, if the marks mim_i are all indicator functions, we obtain a Poisson random field. If the intensity of the Poisson process is high we obtain an approximative Gaussian random field by the central limit theorem - this is the add.mpp method.

    • max.MPP (Boolean functions).
      If the random functions are multiplied by suitable, independent random values, and then the maximum is taken, a max-stable random field with unit Frechet margins is obtained - this is the max.mpp method.

  • nugget.
    The method allows for generating a random field of independent Gaussian random variables. This method is called automatically if the nugget effect is positive except the method "circulant embedding" or "direct" has been explicitly chosen.

    The method has been extended to zonal anisotropies, see also argument nugget.tol in RFoptions.

  • particular method
    – details missing –

  • Random coins.
    See marked point processes.

  • sequential This method is programmed for spatio-temporal models where the field is modelled sequentially in the time direction conditioned on the previous kk instances. For k=5k=5 the method has its limits for about 1000 spatial points. It is an approximative method. The larger kk the better. It also works for certain grids where the last dimension should contain the highest number of grid points.

  • spectral TBM (Spectral turning bands).
    The principle of spectral TBM does not differ from the other turning bands methods. However, line simulations are performed by a spectral technique (Mantoglou and Wilson, 1982).

    The standard method allows for the simulation of 2-dimensional random fields defined on arbitrary points or arbitrary grids. Here, a realisation is given as the cosine with random amplitude and random phase.

  • TBM2, TBM3 (Turning bands methods; turning layers).
    It is generally difficult to use the turning bands method (TBM2) directly in the 2-dimensional space. Instead, 2-dimensional random fields are frequently obtained by simulating a 3-dimensional random field (using TBM3) and taking a 2-dimensional cross-section. TBM3 allows for multiplicative models; in case of anisotropy the anisotropy matrices must be multiples of the first matrix or the anisotropy matrix consists of a time component only (i.e. all components are zero except the very last one).
    TBM2 and TBM3 allow for arbitrary points, and arbitrary grids (arbitrary number of points in each direction, arbitrary grid length for each direction).

    Note: Both the precision and the simulation time depend heavily on TBM*.linesimustep and TBM*.linesimufactor that can be set by RFoptions. For covariance models with larger values of the scale parameter, TBM*.linesimufactor=2 is too small.

    The turning layers are used for the simulations with time component. Here, if the model is a multiplicative covariance function then the product may contain matrices with pure time component. All the other matrices must be equal up to a factor and the temporal part of the anisotropy matrix (right column) may contain only zeros, except the very last entry.

Value

an invisible string vector of the Gaussian methods.

Automatic selection algorithm

— details coming soon —

Note

Most methods possess additional arguments, see RFoptions() that control the precision of the result. The default arguments are chosen such that the simulations are fine for many models and their parameters. The example in RFvariogram() shows a way of checking the precision.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gneiting, T. and Schlather, M. (2004) Statistical modeling with covariance functions. In preparation.

Lantuejoul, Ch. (2002) Geostatistical simulation. New York: Springer.

Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

Original work:

  • Circulant embedding:

    Chan, G. and Wood, A.T.A. (1997) An algorithm for simulating stationary Gaussian random fields. J. R. Stat. Soc., Ser. C 46, 171-181.

    Dietrich, C.R. and Newsam, G.N. (1993) A fast and exact method for multidimensional Gaussian stochastic simulations. Water Resour. Res. 29, 2861-2869.

    Dietrich, C.R. and Newsam, G.N. (1996) A fast and exact method for multidimensional Gaussian stochastic simulations: Extensions to realizations conditioned on direct and indirect measurement Water Resour. Res. 32, 1643-1652.

    Wood, A.T.A. and Chan, G. (1994) Simulation of stationary Gaussian processes in [0,1]d[0,1]^d J. Comput. Graph. Stat. 3, 409-432.

    The code used in RandomFields is based on Dietrich and Newsam (1996).

  • Intrinsic embedding and Cutoff embedding:

    Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599.

    Gneiting, T., Sevcikova, H., Percival, D.B., Schlather, M. and Jiang, Y. (2005) Fast and Exact Simulation of Large Gaussian Lattice Systems in R2R^2: Exploring the Limits J. Comput. Graph. Statist. Submitted.

  • Markov Gaussian Random Field:

    Rue, H. (2001) Fast sampling of Gaussian Markov random fields. J. R. Statist. Soc., Ser. B, 63 (2), 325-338.

    Rue, H., Held, L. (2005) Gaussian Markov Random Fields: Theory and Applications. Monographs on Statistics and Applied Probability, no 104, Chapman \& Hall.

  • Turning bands method (TBM), turning layers:

    Dietrich, C.R. (1995) A simple and efficient space domain implementation of the turning bands method. Water Resour. Res. 31, 147-156.

    Mantoglou, A. and Wilson, J.L. (1982) The turning bands method for simulation of random fields using line generation by a spectral method. Water. Resour. Res. 18, 1379-1394.

    Matheron, G. (1973) The intrinsic random functions and their applications. Adv. Appl. Probab. 5, 439-468.

    Schlather, M. (2004) Turning layers: A space-time extension of turning bands. Submitted

  • Random coins:

    Matheron, G. (1967) Elements pour une Theorie des Milieux Poreux. Paris: Masson.

See Also

RMmodel, RFsimulate, RandomFields.

Examples

RFgetMethodNames()

Internally stored model

Description

The function returns the stored model.

Usage

RFgetModel(register, explicite.natscale, show.call=FALSE,
           origin="original")

Arguments

register

0,...,210,...,21 or an evaluating function, e.g. RFsimulate. Place where intermediate calculations are stored. See also section Registers in RFoptions.

explicite.natscale

logical. Advanced option. If missing, then the model is returned as stored. If FALSE then any RMnatsc is ignored. If TRUE then any RMnatsc is tried to be combined with leading RMS, or returned as such.

show.call

logical or character. If FALSE then the model is shown as interpreted. If TRUE then the user's input including the calling function is returned. See example below.

If show.call is a character it behaves as which.submodels.

origin

character; one of "original", "MLE conform", "all". This argument determines the parameters that are returned.

Details

Whereas RFgetModel returns a model that can be re-used by the user, RFgetModelInfo can return detailed information.

Value

The stored model is returned in list format.

Note

Put Storing=TRUE, see RFoptions, if you like to have (more) internal information in case of failure of an initialization of a random field simulation.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFgetModelInfo, RFsimulate.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMexp(scale=4, var=2) + RMnugget(var=3) + RMtrend(mean=1)
z <- RFsimulate(model, 1:4)
RFgetModel(show.call=FALSE)
RFgetModel(show.call=TRUE)

Information on RMmodels

Description

The function returns information about an RMmodel, either internal information when used in simulations, for instance, or general information

Usage

RFgetModelInfo(...) 

RFgetModelInfo_register(register, level = 1, spConform =
                 RFoptions()$general$spConform, which.submodels =
                 c("user", "internal", "call+user", "call+internal",
                 "user.but.once", "internal.but.once",
                 "user.but.once+jump", "internal.but.once+jump", "all"),
                 modelname = NULL, origin = "original")

RFgetModelInfo_model(model, params, dim = 1, Time = FALSE,
                     kernel = FALSE, exclude_trend = TRUE, ...)

Arguments

...

See the argument of RFgetModelInfo_register and RFgetModelInfo_model; RFgetModelInfo is an abbreviation for the other two functions.

register

0,...,210,...,21 or an evaluating function, e.g. RFsimulate. Place where intermediate calculations are stored. See also section Registers in RFoptions.

level

integer [0...5]; level of details, i.e. the higher the number the more details are given.

spConform

see RFoptions

which.submodels

Internally, the sub-models are represented in two different ways: ‘internal’ and ‘user’. The latter is very close to the model defined by the user.

Most models have a leading internal model. The values "call+user" and "call+internal" also return this leading model if existent.

The values "user.but.once", "internal.but.once" "user.but.once" returns the user path of the internal model following the leading model. "internal.but.once" would return the internal path of the user model following the leading model, but this path should never exist. So as all the other options if a certain direction does not exist, the alternative path is taken.

The values "user.but.once+jump", "internal.but.once+jump" same as "user.but.once" and "internal.but.once", except that the first submodel below the leading model is not given.

The value "all" returns the whole tree of models (very advanced).

modelname

string. If modelname is given then it returns the first appearance of the covariance model with name modelname. If meth is given then the model within the method is returned.

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula. Here, NAs should be placed where information on the parameters is desired..

dim

positive integer. Spatial dimension.

Time

logical. Should time be considered, too?

kernel

logical. Should the model be considered as a kernel?

exclude_trend

logical. Currently, only TRUE is available.

origin

character; one of "original", "MLE conform", "all". This argument determines the parameters that are returned.

Details

RFgetModelInfo branches either into RFgetModelInfo_register or RFgetModelInfo_model, depending on the type of the first argument. The latter two are usually not called by the user.

RFgetModelInfo has three standard usages:

  • RFgetModelInfo() returns internal information on the last call of an RF function.

  • RFgetModelInfo(RFfunction) returns internal information on the last call of RFfunction.

  • RFgetModelInfo(RMmodel) returns general information on RMmodel

Whereas RFgetModelInfo() can return detailed internal information, RFgetModel returns a model that can be re-used by the user.

Value

If RFgetModelInfo(model) is called a list is returned with the following elements:

  • trans.inv : logical. Whether the model is translation invariant (stationary)

  • isotropic : logical. Whether the model is rotation invariant (stationary)

  • NAs : in case of an additive model it gives the number of NAs in each submodel

  • minmax : a data frame containing information on all arguments set to NAs

    • pmin, pmax : lower and upper endpoint of the parameter values usually found in practice

    • type : integer; recognized particularities of a parameter; an explanation of the values is given after the table, if printed.

    • NAN : the number of NANs found

    • min, max : mathematically valid lower and upper endpoints of the parameter values

    • omin, omax : logical. If FALSE the respective mathematical endpoint is included

    • col, row : the dimension of the parameter. If the parameter is a scalar then col = row = 1. If it is a vector then col = 1.

    • bayes : currently not used (always FALSE)

Else a list of internal structure is returned.

Note

Put Storing=TRUE, see RFoptions if you like to have more internal information in case of failure of an initialisation of a random field simulation.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

commandRFgetModel, RFsimulate

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp(scale=4, var=2) + RMnugget(var=3) + RMtrend(mean=1)
z <- RFsimulate(model, 1:4, storing=TRUE)
RFgetModelInfo()

model <-  RMwhittle(scale=NA, var=NA, nu=NA) + RMnugget(var=NA)
RFgetModelInfo(model)

Names of implemented covariance and variogram models

Description

Displays the names of covariance and variogram models (see RMmodel) and returns them as a list. The user may specify and group the models according to the following properties:

  • type of function ("positive definite", "variogram", etc.)

  • whether the function depends on two arguments ("kernel") or on one argument only ("single variable")

  • types of isotropy

  • whether the model is an operator

  • whether the model is a normal scale mixture

  • whether the model has a finite range covariance

  • validity in certain dimensions of the coordinate space

  • maximal possible dimension of the coordinate space

  • uni- or multivariety

See Details for an explanation and RMmodelgenerator for possible states (values) of these properties.

Usage

RFgetModelNames(type = RC_TYPE_NAMES, domain = RC_DOMAIN_NAMES,
                isotropy = RC_ISO_NAMES, operator = c(TRUE, FALSE),
                monotone = RC_MONOTONE_NAMES,
                implied_monotonicities = length(monotone) == 1,
                finiterange = c(TRUE, FALSE, NA),
                valid.in.dim = c(1, Inf), 
                vdim = c(1, 5),
                group.by,
                exact.match = !missing(group.by),
                simpleArguments = FALSE,
                internal, newnames)

Arguments

type, domain, isotropy, operator, monotone, finiterange, vdim

see constants for the definition of RC_TYPE_NAMES, RC_DOMAIN_NAMES, etc. See also RMmodelgenerator.

implied_monotonicities

logical. If TRUE then all the models with a stronger monotonocity than the required one are also shown.

valid.in.dim

an optional integer indicating the dimension of the space where the model is valid

group.by

an optional character string or NULL; must be one of 'type', 'domain', 'isotropy', 'operator', 'monotone', 'finiterange','maxdim','vdim'. If group.by is not given, the result is grouped by 'type' if more than one type is given.

exact.match

logical. If not TRUE, then all categories that are subclasses or might match are show as well.

simpleArguments

logical. If TRUE, only models are considered whose arguments are all integer or real valued.

internal, newnames

both logical; internal might be also integer valued. If any of them are given, RFgetModelNames behaves very differently. See the Notes below.

Details

The plain call RFgetModelNames() simply gives back a vector of the names of all implemented covariance and variogram models and operators, i.e. members of the class RMmodelgenerator.

The following arguments can be specified. In general, only exact matches are returned. One exception exists: If the length of type equals 1 and if group.by is not given, then types included in type are also returned. E.g. if type="variogram" and group.by is not given then only models are returned that are negative definite. However, also positive definite functions and tail correlaton functions are returned if "type" is included in group.by.

type

specifies the class of functions; for the meaning of the possible values see RMmodelgenerator

stationarity

specifies the type of stationarity; for the meaning of the possible values see RMmodelgenerator

isotropy

specifies the type of isotropy; for the meaning of the possible values see RMmodelgenerator

operator

indicates whether the model is an operator, i.e. it requires at least one submodel, e.g. + or RMdelay are operators; see RMmodelgenerator

monotone

indicates what kind of monotonicity is known, e.g., whether the model is a normal scale mixture, the latter including RMexp or RMcauchy; see RMmodelgenerator

finiterange

indicates whether the covariance of the model has finite range, e.g. RMcircular or RMnugget have covariances with finite range; see RMmodelgenerator. NA is used if the finiteness depends on the submodel.

valid.in.dim

If valid.in.dim=n is passed, all models which are valid in dimension nn are displayed. Otherwise valid.in.dim should be a bivariate vector giving the range of requested dimensions.

maxdim

if a positive integer, it specifies the maximal possible dimension of the coordinate space; note that a model which is valid in dimension nn is also valid in dimension n1n-1; maxdim=-1 means that the maximal possible dimension depends on the parameters of the RMmodel object; maxdim=-2 means that the maximal possible dimension is adopted from the called submodels; see also RMmodelgenerator

vdim

if a positive integer, vdim specifies, whether the model is vdimvdim-variate; vdim=-1 means that being multivariate in a certain dimension depends on the parameters of the RMmodel object; vdim=-2 means that being multivariate in a certain dimension is adopted from the called submodels; see also RMmodelgenerator

If vdim is bivariate then a range is given.

group.by

If group.by="propertyname" is passed, the displayed models are grouped according to propertyname.

All arguments allow also for vectors of values. In case of valid.in.dim the smallest value is taken. The interpretation is canonical.

Note that the arguments stationarity, isotropy, operator, monotone, finiterange, maxdim, vdim are also slots (attributes) of the SP4-class RMmodelgenerator.

Value

Either a vector of model names if the argument group.by is not used; or a list of vectors of model names if the argument group.by is used (with list elements specified by the categories of the grouping argument).

In case internal or newnames is given, RFgetModelNames prints a table of the currently implemented covariance functions and the matching methods. RFgetModelNames returns NULL.

Note

In case internal or newnames is given, only the values of internal, newnames and operator are considered. All the other arguments are ignored and RFgetModelNames prints a table of the currently implemented covariance functions and the matching methods:

  • internal:
    if TRUE also RMmodels are listed that are internal, hence invisible to the user. Default: FALSE.

  • newnames:
    The model names of version 2 of RandomFields and earlier can still be used in the model definitions. Namely when the list notation is chosen; see Advanced RMmodels for the latter. If internal or newnames is given, then these old names are shown; if newnames=TRUE then also the usual names are shown. Default: FALSE.

    In fact, both internal and public models can have different variants implemented. These variants are also shown if internal has a value greater than or equal to 2,

  • operator:
    see above.

Here, also an indication is given, which method for simulating Gaussian random fields matches the model.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

constants, RMmodelgenerator, RMmodel, RandomFields, RC_DOMAIN_NAMES, RC_ISO_NAMES

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

# get list of names of all functions
RFgetModelNames()

# any kind of positive definite functions
RFgetModelNames(type="positive definite", exact.match=TRUE)
## Not run: RFgetModelNames(type="positive definite")

# get a list of names of all stationary models
RFgetModelNames(type="positive definite", domain="single variable",
                 exact.match=TRUE)
## Not run: RFgetModelNames(type="positive definite", domain="single variable")

# get a vector of all model names
RFgetModelNames(group.by=NULL)

Class RFgridDataFrame

Description

Class for attributes in one-dimensional space.

Usage

## S4 method for signature 'RFgridDataFrame'
RFspDataFrame2conventional(obj, data.frame=FALSE)

Arguments

obj

an RFgridDataFrame object

data.frame

logical. If TRUE a data.frame is returned.

Creating Objects

Objects can be created by using the functions RFgridDataFrame or conventional2RFspDataFrame or by calls of the form as(x, "RFgridDataFrame"), where x is of class RFgridDataFrame.

Slots

.RFparams:

list of up to 5 elements;

  • n is the number of repetitions of the random field contained in the data slot

  • vdim gives the dimension of the values of the random field, equals 1 in most cases

  • has.variance indicates whether information on the variance is available,

  • coordunits gives the names of the units for the coordinates

  • varunits gives the names of the units for the variables

data:

object of class data.frame, containing attribute data

grid:

object of class GridTopology.

Methods

plot

signature(obj = "RFgridDataFrame"): generates nice plots of the random field; if spacetimedim2space-time-dim2, a two-dimensional subspace can be selected using the argument MARGIN; to get different slices in a third direction, the argument MARGIN.slices can be used; for more details see plot-method or type method?plot("RFgridDataFrame")

show

signature(x = "RFgridDataFrame"): uses the show-method for class SpatialGridDataFrame.

print

signature(x = "RFgridDataFrame"): identical to show-method

RFspDataFrame2conventional

signature(obj = "RFgridDataFrame"): conversion to a list of non-sp-package based objects; the data-slot is converted to an array of dimension [1(vdim>1)+spacetimedimension+1(n>1)][1*(vdim>1) + space-time-dimension + 1*(n>1)]

coordinates

signature(x = "RFgridDataFrame"): returns the coordinates

[

signature(x = "RFgridDataFrame"): selects columns of data-slot; returns an object of class RFgridDataFrame.

[<-

signature(x = "RFgridDataFrame"): replaces columns of data-slot; returns an object of class RFgridDataFrame.

as

signature(x = "RFgridDataFrame"): converts into other formats, only implemented for target class RFpointsDataFrame

cbind

signature(...): if arguments have identical topology, combine their attribute values

range

signature(x = "RFgridDataFrame"): returns the range

hist

signature(x = "RFgridDataFrame"): plots histogram

as.matrix

signature(x = "RFgridDataFrame"): converts data-slot to matrix

as.array

signature(x = "RFgridDataFrame"): converts data-slot to array

as.vector

signature(x = "RFgridDataFrame"): converts data-slot to vector

as.data.frame

signature(x = "RFgridDataFrame"): converts data-slot and coordinates to a data.frame

Details

Methods summary and dimensions are defined for the “parent”-class RFsp.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFspatialGridDataFrame, which is for point locations in higher dimensional spaces, RFpointsDataFrame-class which is for one-dimensional arbitrary locations, RFsp

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,10,length=100)
f <- RFsimulate(model=RMgauss(), x=x, n=3)

str(f)
str(RFspDataFrame2conventional(f))
head(coordinates(f))
str(f[2]) ## selects second column of data-slot
all.equal(f, cbind(f,f)[1:3]) ## TRUE

plot(f, nmax=2)

Graphical User Interface For Fitting Covariance Models And Variograms

Description

This is a nice instructive graphical tool useful in particular for teaching classes

Usage

RFgui(data, x, y, same.algorithm = TRUE, ev, bin = NULL, xcov, ycov,
      sim_only1dim=FALSE, wait = 0, ...)

Arguments

data

See RFvariogram. If data is given, the empirical variogram is shown.

x

a sequence of the locations of the simulated process; if not given, x is determined by data and if data is not given by default values

y

a sequence of numbers if a simulation on RdR^d is performed. Default is y = x; see x for details.

same.algorithm

Force the picture being simulated with the same algorithm so that the pictures are always directly comparable. The disadvantage is that some models are simulated only (very) approximatively.

ev

instead of the data, the empirical variogram itself might be passed

bin

only considered if data is given. See RFvariogram for details.

xcov

sequence of the locations where the covariance function is plotted

ycov

Only for anisotropic models. sequence of the locations where the covariance function is also plotted

sim_only1dim

Logical. The argument determines whether a process should be simulated on the line or on the plane

wait

integer. See details.

...

further options and control arguments for the simulation that are passed to and processed by RFoptions.

Details

If wait is negative the xterm does not wait for the tkltk-window to be finished. Further the variable RFgui.model is created in the environment .GlobalEnv and contains the currently chosen variable in the gui. RFgui always returns NULL.

If wait is non-negative the xterm waits for the tkltk-window to be finished. RFgui returns invisibly the last chosen model (or NULL if no model has been chosen). RFgui idles a lot when wait=0. It idles less for higher values by sleeping about wait microseconds. Of course the handling in the tkltk window gets slower as well. Reasonable values for wait are within [0,1000].

same.alg = TRUE is equivalent to setting circulant.trials=1, circulant.simu_method = "RPcirculant", circulant.force=TRUE, circulant.mmin=-2.

Value

If wait < 0 the function returns NULL else it returns the last chosen RMmodel.

If wait < 0, a side effect of RFgui is the creation of the variable RFgui.model on .GlobalEnv.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Author(s) of the code

Daphne Boecker; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

soil for a further example

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
RFgui()

Hurst coefficient

Description

The function estimates the Hurst coefficient of a process

Usage

RFhurst(x, y = NULL, z = NULL, data, sort = TRUE,
 block.sequ = unique(round(exp(seq(log(min(3000, dimen[1]/5)),
 log(dimen[1]),
 len = min(100, dimen[1]))))),
 fft.m = c(1, min(1000, (fft.len - 1)/10)),
 fft.max.length = Inf, method = c("dfa", "fft", "var"),
 mode = if (interactive ()) c("plot", "interactive") else "nographics", 
 pch = 16, cex = 0.2, cex.main = 0.85,
 printlevel = RFoptions()$basic$printlevel, height = 3.5,
 ...)

Arguments

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

data

the data

sort

logical. If TRUE then the coordinates are permuted such that the largest grid length is in x-direction; this is of interest for algorithms that slice higher dimensional fields into one-dimensional sections.

block.sequ

ascending sequences of block lengths for which the detrended fluctuation analysis and the variance method are performed.

fft.m

vector of 2 integers; lower and upper endpoint of indices for the frequency which are used in the calculation of the regression line for the periodogram near the origin.

fft.max.length

if the number of points in x-direction is larger than fft.max.length then the segments of length fft.max.length are considered, shifted by fft.max.length/2 (WOSA-estimator).

method

list of implemented methods to calculate the Hurst parameter; see Details

mode

character. A vector with components 'nographics', 'plot' or 'interactive':

'nographics'

no graphical output

'plot'

the regression line is plotted

'interactive'

the regression domain can be chosen interactively

Usually only one mode is given. Two modes may make sense in the combination c("plot", "interactive") in which case all the results are plotted first, and then the interactive mode is called. In the interactive mode, the regression domain is chosen by two mouse clicks with the left mouse; a right mouse click leaves the plot.

pch

vector or scalar; sign by which data are plotted.

cex

vector or scalar; size of pch.

cex.main

font size for title in regression plot; only used if mode includes 'plot' or 'interactive'

printlevel

integer. If printlevel is 0 or 1 nothing is printed. If printlevel=2 warnings and the regression results are given. If printlevel>2 tracing information is given.

height

height of the graphics window

...

graphical arguments

Details

The function is still in development. Several functionalities do not exist - see the code itself for the current stage.

The function calculates the Hurst coefficient by various methods:

  • detrended fluctuation analysis (dfa)

  • aggregated variation (var)

  • periodogram or WOSA estimator (fft)

Value

The function returns a list with elements dfa, varmeth, fft corresponding to the three methods given in the Details.

Each of the elements is itself a list that contains the following elements.

x

the x-coordinates used for the regression fit

y

the y-coordinates used for the regression fit

regr

the coefficients of the lm.

sm

smoothed curve through the (x,y) points

x.u

NULL or the restricted x-coordinates given by the user in the interactive plot

y.u

NULL or y-coordinates according to x.u

regr.u

NULL or the coefficients of lm for x.u and y.u

H

the Hurst coefficient

H.u

NULL or the Hurst coefficient corresponding to the user's regression line

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

detrended fluctuation analysis

  • Peng, C.K., Buldyrev, S.V., Havlin, S., Simons, M., Stanley, H.E. and Goldberger, A.L. (1994) Mosaic organization of DNA nucleotides Phys. Rev. E 49, 1685-1689

aggregated variation

  • Taqqu, M.S. and Teverovsky, V. (1998) On estimating the intensity of long range dependence in finite and infinite variance time series. In: Adler, R.J., Feldman, R.E., and Taqqu, M.S. A Practical Guide to Heavy Tails, Statistical Techniques an Applications. Boston: Birkhaeuser

  • Taqqu, M.S. and Teverovsky, V. and Willinger, W. (1995) Estimators for long-range dependence: an empirical study. Fractals 3, 785-798

periodogram

  • Percival, D.B. and Walden, A.T. (1993) Spectral Analysis for Physical Applications: Multitaper and Conventional Univariate Techniques, Cambridge: Cambridge University Press.

  • Welch, P.D. (1967) The use of Fast Fourier Transform for the estimation of power spectra: a method based on time averaging over short, modified periodograms IEEE Trans. Audio Electroacoustics 15, 70-73.

See Also

RMmodel, RFfractaldim

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


x <- runif(1000)
h <- RFhurst(1:length(x), data=x)

Interpolation methods

Description

The function allows for different methods of interpolation. Currently, only various kinds of kriging are installed.

Usage

RFinterpolate(model, x, y = NULL, z = NULL, T = NULL, grid=NULL,
              distances, dim, data, given=NULL, params, err.model, err.params,
              ignore.trend = FALSE, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest. If given is not given and data is a matrix or data is a data.frame, RandomFields tries to identify where the data and the coordinates are, e.g. by names in formulae or by fixed names, see Coordinate systems. See also RFsimulateAdvanced. If all fails, the first columns are interpreted as coordinate vectors, and the last column(s) as (multiple) measurement(s) of the field. Notes that also lists of data can be passed.

If the argument x is missing, data may contain NAs, which are then replaced through imputing.

given

optional, matrix or list. If given matrix then the coordinates can be given separately, namely by given where, in each row, a single location is given.
If given is a list, it may consist of x, y, z, T, grid.
If given is provided, data must be a matrix or an array containing the data only.

err.model, err.params

For conditional simulation and random imputing only.
In case of (assumed) error-free measurements (which is mostly the case in geostatistics) the argument err.model is not given. In case of measurement errors we have err.model=RMnugget(var=var).
err.param plays the same role as params for model.

ignore.trend

logical. If TRUE only the covariance model of the given model is considered, without the trend part.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

In case of repeated data, they are kriged separately; if the argument x is missing, data may contain NAs, which are then replaced by the kriged values (imputing);

In case of intrinsic cokriging (intrinsic kriging for multivariate random fields) the pseudo-cross-variogram is used (cf. Ver Hoef and Cressie, 1991).

Value

The value depends on the additional argument variance.return, see RFoptions.

If variance.return=FALSE (default), Kriging returns a vector or matrix of kriged values corresponding to the specification of x, y, z, and grid, and data.

data: a vector or matrix with one column
* grid=FALSE. A vector of simulated values is returned (independent of the dimension of the random field)
* grid=TRUE. An array of the dimension of the random field is returned (according to the specification of x, y, and z).

data: a matrix with at least two columns
* grid=FALSE. A matrix with the ncol(data) columns is returned.
* grid=TRUE. An array of dimension d+1d+1, where dd is the dimension of the random field, is returned (according to the specification of x, y, and z). The last dimension contains the realisations.

If variance.return=TRUE, a list of two elements, estim and var, i.e. the kriged field and the kriging variances, is returned. The format of estim is the same as described above. The format of var is accordingly.

Note

Important options are

  • method (overwriting the automatically detected variant of kriging)

  • return_variance (returning also the kriging variance)

  • locmaxm (maximum number of conditional values before neighbourhood kriging is performed)

  • fillall imputing estimates location by default

  • varnames and coordnames in case data.frames are used to tell which column contains the data and the coordinates, respectively.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/; Marco Oesting, [email protected], https://www.isa.uni-stuttgart.de/institut/team/Oesting/

Author(s) of the code:

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/; Alexander Malinowski; Marco Oesting, [email protected], https://www.isa.uni-stuttgart.de/institut/team/Oesting/

References

Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

Cressie, N.A.C. (1993) Statistics for Spatial Data. New York: Wiley.

Goovaerts, P. (1997) Geostatistics for Natural Resources Evaluation. New York: Oxford University Press.

Ver Hoef, J.M. and Cressie, N.A.C. (1993) Multivariate Spatial Prediction. Mathematical Geology 25(2), 219-240.

Wackernagel, H. (1998) Multivariate Geostatistics. Berlin: Springer, 2nd edition.

See Also

RMmodel, RFvariogram, RandomFields,

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Preparation of graphics
dev.new(height=7, width=16) 

## creating random variables first
## here, a grid is chosen, but does not matter
p <- 3:8
points <- as.matrix(expand.grid(p,p))
model <- RMexp() + RMtrend(mean=1)
dta <- RFsimulate(model, x=points)
plot(dta)
x <- seq(0, 9, 0.25)


## Simple kriging with the exponential covariance model
model <- RMexp()
z <- RFinterpolate(model, x=x, y=x, data=dta)
plot(z, dta)

## Simple kriging with mean=4 and scaled covariance
model <- RMexp(scale=2) + RMtrend(mean=4)
z <- RFinterpolate(model, x=x, y=x, data=dta)
plot(z, dta)

## Ordinary kriging
model <- RMexp() + RMtrend(mean=NA)
z <- RFinterpolate(model, x=x, y=x, data=dta)
plot(z, dta)



## Co-Kriging
n <- 100
x <- runif(n=n, min=1, max=50)
y <- runif(n=n, min=1, max=50)



rho <- matrix(nc=2, c(1, -0.8, -0.8, 1))
model <- RMparswmX(nudiag=c(0.5, 0.5), rho=rho)

## generation of artifical data
data <- RFsimulate(model = model, x=x, y=y, grid=FALSE)
## introducing some NAs ...
print(data)
len <- length(data)
data@data$variable1[1:(len / 10)] <- NA
data@data$variable2[len - (0:len / 100)] <- NA
print(data)
plot(data)

## co-kriging
x <- y <- seq(0, 50, 1)

k <- RFinterpolate(model, x=x, y=y, data= data)
plot(k, data)

## conditional simulation
z <- RFsimulate(model, x=x, y=y, data= data) ## takes some time
plot(z, data)







close.screen(all = TRUE)

Linear part of RMmodel

Description

RFlinearpart returns the linear part of a model

Usage

RFlinearpart(model, x, y = NULL, z = NULL, T = NULL, grid=NULL,
                data, params, distances, dim, set=0, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

set

integer. See section Value for details.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Value

RFlinearpart returns a list of three components, Y, X, vdim returning the deterministic trend, the design matrix, and the multivariability, respectively. If set is positive, Y and X contain the values for the set-th set of coordinates. Else, Y and X are both lists containing the values for all the sets.

Note

In the linear part of the model specification the parameters that are NA must be the first model part. I.e. NA * sin(R.p(new="isotropic")) + NA + R.p(new="isotropic") is OK, but not sin(R.p(new="isotropic")) * NA + NA + R.p(new="isotropic")

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

Bayesian, RMmodel, RFsimulate, RFlikelihood.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


x <- seq(0, pi, len=10)
trend <- 2 * sin(R.p(new="isotropic")) + 3
model <- RMexp(var=2, scale=1) + trend
print(RFlinearpart(model, x=x))  ## only a deterministic part

trend <- NA * sin(R.p(new="isotropic")) + NA + R.p(new="isotropic") / pi
model <- RMexp(var=NA, scale=NA) + trend
print(RFlinearpart(model, x=x))

Likelihood and estimation of linear models

Description

RFloglikelihood returns the log likelihood for Gaussian random fields. In case NAs are given that refer to linear modeling, the ML of the linear model is returned.

Usage

RFlikelihood(model, x, y = NULL, z = NULL, T = NULL, grid = NULL,
                data, params, distances, dim, likelihood,
                estimate_variance =NA, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

likelihood

Not programmed yet. Character. Choice of kind of likelihood ("full", "composite", etc.), see also likelihood for RFfit in RFoptions.

estimate_variance

logical or NA. See Details.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

The function calculates the likelihood for data of a Gaussian process with given covariance structure. The covariance structure may not have NA values in the parameters except for a global variance. In this case the variance is returned that maximizes the likelihood. Additional to the covariance structure the model may include a trend. The latter may contain unknown linear parameters. In this case again, the unknown parameters are estimated, and returned.

Value

RFloglikelihood returns a list containing the likelihood, the log likelihood, and the global variance (if estimated – see details).

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

Bayesian, RMmodel, RFfit, RFsimulate, RFlinearpart.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


requireNamespace("mvtnorm")

pts <- 4
repet <- 3
model <- RMexp()
x <- runif(n=pts, min=-1, max=1)
y <- runif(n=pts, min=-1, max=1)
dta <- as.matrix(RFsimulate(model, x=x, y=y, n=repet, spC = FALSE))
print(cbind(x, y, dta))
print(system.time(likeli <- RFlikelihood(model, x, y, data=dta)))
str(likeli, digits=8)

L <- 0
C <- RFcovmatrix(model, x, y)
for (i in 1:ncol(dta)) {
  print(system.time(dn <- mvtnorm::dmvnorm(dta[,i], mean=rep(0, nrow(dta)),
sigma=C, log=TRUE)))
  L <- L + dn
}
print(L)
stopifnot(all.equal(likeli$log, L))





pts <- 4
repet <- 1
trend <- 2 * sin(R.p(new="isotropic")) + 3
#trend <- RMtrend(mean=0)
model <- 2 * RMexp() + trend
x <- seq(0, pi, len=pts)
dta <- as.matrix(RFsimulate(model, x=x, n=repet, spC = FALSE))
print(cbind(x, dta))

print(system.time(likeli <- RFlikelihood(model, x, data=dta)))
str(likeli, digits=8)

L <- 0
tr <- RFfctn(trend, x=x, spC = FALSE)
C <- RFcovmatrix(model, x)
for (i in 1:ncol(dta)) {
  print(system.time(dn <- mvtnorm::dmvnorm(dta[,i], mean=tr, sigma=C,log=TRUE)))
  L <- L + dn
}
print(L)

stopifnot(all.equal(likeli$log, L))






pts <- c(3, 4)
repet <- c(2, 3)
trend <- 2 * sin(R.p(new="isotropic")) + 3
model <- 2 * RMexp() + trend
x <- y <- dta <- list()
for (i in 1:length(pts)) {
  x[[i]] <- list(x = runif(n=pts[i], min=-1, max=1),
                 y = runif(n=pts[i], min=-1, max=1))
  dta[[i]] <- as.matrix(RFsimulate(model, x=x[[i]]$x, y=x[[i]]$y,
                                    n=repet[i], spC = FALSE))
}

print(system.time(likeli <- RFlikelihood(model, x, data=dta)))
str(likeli, digits=8)

L <- 0
for (p in 1:length(pts)) {
  tr <- RFfctn(trend, x=x[[p]]$x, y=x[[p]]$y,spC = FALSE)
  C <- RFcovmatrix(model, x=x[[p]]$x, y=x[[p]]$y)
  for (i in 1:ncol(dta[[p]])) {
    print(system.time(dn <- mvtnorm::dmvnorm(dta[[p]][,i], mean=tr, sigma=C,
                                    log=TRUE)))
    L <- L + dn
  }
}
print(L)
stopifnot(all.equal(likeli$log, L))

Empirical (Cross-)Madogram

Description

Calculates the empirical (cross-)madogram. The empirical (cross-)madogram of two random fields XX and YY is given by

γ(r):=1N(r)(ti,tj)ti,j=r(X(ti)X(tj))(Y(ti)Y(tj))\gamma(r):=\frac{1}{N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} |(X(t_{i})-X(t_{j}))||(Y(t_{i})-Y(t_{j}))|

where ti,j:=titjt_{i,j}:=t_{i}-t_{j}, and where N(r)N(r) denotes the number of pairs of data points with distancevector ti,j=rt_{i,j}=r.

Usage

RFmadogram(model, x, y=NULL, z=NULL, T=NULL, grid, params, distances,
           dim, ..., data, bin=NULL, phi=NULL, theta = NULL,
           deltaT = NULL, vdim=NULL)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

bin

a vector giving the borders of the bins; If not specified an array describing the empirical (pseudo-)(cross-) covariance function in every direction is returned.

phi

an integer defining the number of sectors one half of the X/Y plane shall be divided into. If not specified, either an array is returned (if bin missing) or isotropy is assumed (if bin specified).

theta

an integer defining the number of sectors one half of the X/Z plane shall be divided into. Use only for dimension d=3d=3 if phi is already specified.

deltaT

vector of length 2, specifying the temporal bins. The internal bin vector becomes seq(from=0, to=deltaT[1], by=deltaT[2])

vdim

the number of variables of a multivariate data set. If not given and data is an RFsp object created by RandomFields, the information there is taken from there. Otherwise vdim is assumed to be one. NOTE: still the argument vdim is an experimental stage.

Details

RFmadogram computes the empirical cross-madogram for given (multivariate) spatial data.

The spatial coordinates x, y, z should be vectors. For random fields of spatial dimension d>3d > 3 write all vectors as columns of matrix x. In this case do neither use y, nor z and write the columns in gridtriple notation.

If the data is spatially located on a grid a fast algorithm based on the fast Fourier transformed (fft) will be used. As advanced option the calculation method can also be changed for grid data (see RFoptions.)

It is also possible to use RFmadogram to calculate the pseudomadogram (see RFoptions).

Value

RFmadogram returns objects of class RFempVariog.

Author(s)

Jonas Auel; Sebastian Engelke; Johannes Martini; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RMstable, RMmodel, RFsimulate, RFfit, RFcov, RFpseudomadogram. RFvariogram.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

n <- 1 ## use n <- 2 for better results

## isotropic model
model <- RMexp()
x <- seq(0, 10, 0.02)
z <- RFsimulate(model, x=x, n=n)
emp.vario <- RFmadogram(data=z)
plot(emp.vario)


## anisotropic model
model <- RMexp(Aniso=cbind(c(2,1), c(1,1)))
x <- seq(0, 10, 0.05)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFmadogram(data=z, phi=4)
plot(emp.vario)


## space-time model
model <- RMnsst(phi=RMexp(), psi=RMfbm(alpha=1), delta=2)
x <- seq(0, 10, 0.05)
T <- c(0, 0.1, 100)
z <- RFsimulate(x=x, T=T, model=model, n=n)
emp.vario <- RFmadogram(data=z, deltaT=c(10, 1))
plot(emp.vario, nmax.T=3)


## multivariate model
model <- RMbiwm(nudiag=c(1, 2), nured=1, rhored=1, cdiag=c(1, 5), 
                s=c(1, 1, 2))
x <- seq(0, 20, 0.1)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFmadogram(data=z)
plot(emp.vario)


## multivariate and anisotropic model
model <- RMbiwm(A=matrix(c(1,1,1,2), nc=2),
                nudiag=c(0.5,2), s=c(3, 1, 2), c=c(1, 0, 1))
x <- seq(0, 20, 0.1)
dta <- RFsimulate(model, x, x, n=n)
ev <- RFmadogram(data=dta, phi=4)
plot(ev, boundaries=FALSE)

RFoldstyle

Description

This function is written only for package writers who have based their code on RandomFields version 2.

It avoids warnings if the old style is used, and sets spConform = FALSE.

Usage

RFoldstyle(old=TRUE)

Arguments

old

logical

Value

NULL

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

See ‘version2’ for details on the commands of version 2.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

GaussRF(x=1:10, model="exp", param=c(0,1,0,1), grid=TRUE)

RFoldstyle()
GaussRF(x=1:10, model="exp", param=c(0,1,0,1), grid=TRUE)

Setting control arguments

Description

RFoptions sets and returns control arguments for the analysis and the simulation of random fields. It expands the functionality of RFoptions.

Usage

RFoptions(...)

Arguments

...

arguments in tag = value form, or a list of tagged values.

Details

The subsections below comment on
0. basic: See RFoptions
1. general: General options
2. br: Options for Brown-Resnick Fields
3. circulant: Options for circulant embedding methods RPcirculant
4. coords: Options for coordinates and units, see coordinate systems
5. direct: Options for simulating by simple matrix decomposition
6. distr: Options for distributions, in particular RRrectangular
7. empvario: Options for calculating the empirical variogram
8. fit: Options for RFfit, RFratiotest, and RFcrossvalidate
9. gauss: Options for simulating Gaussian random fields
10. graphics: Options for graphical output
11. gui: Options for RFgui
12. hyper: Options for simulating hyperplane tessellations
13. krige: Options for Kriging
14. maxstable: Options for simulating max-stable random fields
15. mpp: Options for the random coins (shot noise) methods
16. nugget: Options for the nugget effect
17. registers: Register numbers
18. sequ: Options for the sequential method
19. solve: Options for solving linear systems
20. special: Options for some special methods
21. spectral: Options for the spectral (turning bands) method
22. tbm: Options for the turning bands method
23. internal: Internal


1. General options

allowdistanceZero

boolean. Only used in RFinterpolate and in RFfit. If true, then multiple observations or identical locations are allowed within a single data set. In this case, the coordinates are slightly scattered, so that the points have some tiny distances.

Default: FALSE.

cPrintlevel

cPrintlevel is automatically set to printlevel when printlevel is changed. Standard users will never use a value higher than 3.

0 : no messages
1 : messages and warnings when the user's input looks odd
2 : messages (and internal errors) documenting the choice of the simulation method
3 : further user relevant informations
4 : information on recursive function calls
5 : function flow information of central functions
6 : errors that are internally treated
7 : details on building up the covariance structure
8 : details on taking the square root of the covariance matrix
9 : details on intermediate calculations
10 : further details on intermediate calculations

Note that printlevel works on the R level whereas cPrintlevel works on the C level.

Default: 1

detailed_output

logical. if TRUE some function, e.g. RFcrossvalidate will return additional information.

every

integer. if greater than zero, then every everyth iteration is printed if simulated by TBM or random coin method. The value zero means that nothing is printed.

Default: 0

exactness

logical or NA. Currently only used when simulating Gaussian random fields.

  • TRUE: RPcoins, RPhyperplane, RPsequential, RPspectral and RPtbm and approximative circulant embedding are excluded. If the circulant embedding method is considered as badly behaved, then the matrix decomposition methods are preferred.

  • FALSE: all the methods are allowed. If the circulant embedding method is considered as badly behaved or the number of points to be simulated is large, the turning bands methods are rather preferred.

  • NA: Similar to FALSE, but some inexact algorithms get less preference.

Default: NA .

expected_number_simu

positive integer which is usally set internally as the value of the argument n in RFsimulate. The argument expected_number_simu should be set only by an advanced users and only if RFsimulate will be called with argument n alone.

gridtolerance

used in RFsimulate to see if the coordinates build a grid for x, y, z, T-values. This argument is also used in case of conditional simulation where the data locations might ly on a grid.

Default: 1e-6

asList

logical. Lists of arguments are treated slightly different from non-lists. If asList=FALSE they are treated the same way as non-lists. This options being set to FALSE after calling RFoptions it should be set as first element of a list.

Default: TRUE

modus_operandi

character. One of the values "careless", "sloppy", "easygoing", "normal", "precise", "pedantic", "neurotic" . This argument is in an experimental stage and its definition and effects will change very likely in near future. This argument sets a lot of argument at once related to estimation and simulation. "careless" prefers rather fast algorithms, but the results might be very rough approximations. By way of contrast, "neurotic" will try very hard to return exact result at the cost of hugh computing times.

Default: "normal"

na_rm_lines

logical. If TRUE then a line of the data that contains a NA value is deleted. Otherwise it is tried to deal with the NA value at higher costs of computing time. (Only used for kriging – estimation can fully deal with NAs.)

Default: FALSE.

output

character. one of the values "sp" (if and only if spConform=TRUE), "RandomFields" (if and only if spConform=FALSE), "geoR".

The output mode geoR currently adds some attributes such as the call of the function.

NOTE: output is in an experimental stage, whose effects might change in future. Currently, output changes the values of reportcoord, returncall and spConform.

pch

character. RFfit: shown before evaluating any method; if pch!="" then one or two additional steps in the MLE methods are marked by “+” and “#”.

Simulation:

The character is printed after each performed simulation if more than one simulation is performed at once. If pch='!' then an absolute counter is shown instead of the character. If pch='%' then a counter of percentages is shown instead of the character. Note that also ‘^\mbox{\textasciicircum}H’s are printed in the last two cases, which may have undesirable interactions with some few other R functions, e.g. Sweave.

Default: '*'.

practicalrange

logical or integer. If not FALSE the range of primitive covariance functions is adjusted so that cov(1) is zero for models with finite range. (Operators are too complex to be adjusted; for anisotropic covariance the practical range is not well defined.)

The value of cov(1) is about 0.05 (for scale=1) for models without range. See RMmodel or type
RFgetModelNames(type="positive definite", domain="single variable", isotropy="isotropic", operator=FALSE, vdim=1)
for the list of primitive models.

  • FALSE : the practical range ajustment is not used.

  • TRUE : practicalrange is applicable only if the value is known exactly, or, at least, can be approximated by a closed formula.

  • 2 : if the practical range is not known exactly it is approximated numerically.

Default: FALSE .

printlevel

If printlevel0\le0 there is not any output on the screen. The higher the number the more tracing information is given. Standard users will never use a value higher than 3.

0 : no messages
1 : important (error) messages and warnings
2 : less important messages
3 : details, but still for the user
4 : recursive call tracing (only used within RFfit)
5 : function flow information of large functions
6 : errors that are internally treated
7 : details on intermediate calculations
8 : further details on intermediate calculations

Default: 1

reportcoord

character. Current values are "always", "important", "warn", "never",

Both "warn" and "important" have any effect only if the coordinate system is changed internally. In this case "warn" yields a displayed warning message whereas "important" adds an attribute to the result as in the case "always".

If "always" or "important" the reports are added as attribute to the results. Note that in this case the class of the result may change (e.g. from "numeric" to "atomic").

Default: "warn"

returncall

logical. If TRUE then the call is returned as an attribute

Default: TRUE

seed

integer. If NULL or NA set.seed is not called. Otherwise, set.seed(seed) is set before simulations are performed, e.g. by RFsimulate or RFdistr.

If the argument is set locally, i.e., within a function, it has the usual local effect. If it is set globally, i.e. by RFoptions the seed is fixed for all subsequent calls.

If the number of simulations n is greater than one and if RFoptions(seed=seed) is set, the iith simulation is started with the seed ‘seed+i1+i-1’.

Note also that RFratiotest has its own argument seed with a slightly different meaning.

seed_incr, seed_sub_incr

(does not work yet) This argument is important iff RFsimulate is used within a function from package parallel. The value of seed_incr should be set only locally, i.e. not by RFoptions().

If seed_incr != 0 (or the number of simulations n is greater than 1) and !is.na(seed) then the seed for each simulation is calculated as

seed +(k1)+ (k-1) * seed_sub_incr ++ seed_incr n* n

where kk runs from 1 to n.

Default: 0

set

integer. Certain models (e.g. RMfixcov and RMcovariate) allow for lists as arguments. set selects a certain list element. If necessary the list is recycled.

spConform

logical. spConform=TRUE might be used by a standard user as this allows the comfortable use of plot, for instance, while spConform=FALSE is much faster and and consumes much less memory, hence might be used by programmers or advanced users.

Details: if spConform=TRUE then RFsimulate and many other functions return an sp-object (which is an S4 object). Otherwise, matrices or lists are returned as defined in RandomFields 2.0, see the manuals for the specific functions. Frequently, the latter have now a class attribute to make the output nicer.

Note: for large data sets (to be generated), spConform=TRUE should not be used.

See also output.

Default: TRUE

skipchecks

logical. If TRUE, several checks whether the given parameter values and the dimension are within the allowed range is skipped. Do not change the value of this variable except you really know what you do.

Default: FALSE $

storing

Logical. If FALSE then the intermediate results are destroyed after the simulation of the random field(s) or if an error had occured. If storing=TRUE, then additional simulations can be performed by calling RFsimulate with at most the argument n. This call can then be much faster, but the a rather large amount of memory could be kept.

When storing turned from TRUE to FALSE by global call then all registers are deleted. Advanced: With RFoptions(storing=list(FALSE, register, model_register)) single registers can be deleted.

Default: FALSE

Ttriple

Logical or NA. If TRUE, then triple for the time argument T is expected, containing start, step (by), length. If FALSE a sequence on a grid is expected. If NA then the decision is automatic, but will lead to an error if ambiguous.

vdim_close_together

logical. Used especially in functions that create covariance matrices. If the model is multivariate, then two ways of ordering the matrix exist. To consider first all variables at a certain location (vdim_close_together=TRUE) or to consider first all locations keeping the variable fixed (vdim_close_together=FALSE). Note that several simulation methods rely on the value FALSE, so that these methods will not work anymore if vdim_close_together=FALSE.

Default: FALSE.

2. Options for Brown-Resnick Fields

deltaAM

integer; only used for simulation of BR processes via RPbrmixed with optim_mixed=2. In this case, deltaAM is the number of additionally simulated Gaussian processes used for an update of areamat in the optimization pricedure.

Default: 300

maxtrendmem

integer; the maximal number of real valued variables used for intermediate storage:

  • RPbrshifted: trends for shifted locations that may be stored at the same time when simulating BR processes.

  • RPbrnormed: Let nn be the number of locations. Then a n×nn\times n (covariance) matrix has to be evaluated at random columns.

if maxtrendmem is large (and nn small, n104n\le 10^4), multiple evaluations can be avoided.

Default: 1e7 .

meshsize

positive; width of the grid on which the shape functions in the M3 representation of BR processes are simulated; only used for simulation of BR processes via RPbrmixed.

Default: 0.1 .

optim_mixed

0, 1, 2; only used for simulation of BR processes via RPbrmixed.
If optim_mixed=0, the arguments lambda and areamat of RPbrmixed are used for the simulation.
If optim_mixed=1, lambda is estimated for areamat=1.
If optim_mixed=2, areamat is optimized and lambda is estimated.

Default: 1 .

optim_mixed_tol

value in [0,1][0,1]; only used for simulation of BR processes via RPbrmixed with optim_mixed=2. In this case, areamat is optimized under the constraint that the probability of drawing the shape function incorrectly is bounded by optim_mixed_tol (cf. Oesting et al., 2012).

Default: 0.01 .

variobound

positive; the shape functions in the mixed moving maxima representation are cut off where the variogram belonging to phi exceeds variobound.

Default: 8.0 .

vertnumber

positive integer; for an efficient simulation of the shape functions in the M3 representation of BR processes, the component EE from of the domain [x0,]×E[x_0, \infty] \times E of the underlying Poisson point process is sub-dividedinto cubes (cf. Oesting et al., 2012); vertical is the number of vertical breaks of EE; only used for simulation of BR processes via RPbrmixed with optim_mixed=2.

Default: 7 .

3. circulant: Options for circulant embedding methods, cf. RPcirculant
These options influence the standard circulant embedding method, cutoff circulant embedding intrinsic circulant embedding. It can also influence RPtbm if the line is simulated with any circulant embedding method.

approx_maxgrid

See RPcirculant

approx_step

See RPcirculant

dependent

See RPcirculant

force

See RPcirculant

maxGB

See RPcirculant

maxmem

See RPcirculant

mmin

See RPcirculant

strategy

See RPcirculant

tolIm

See RPcirculant

tolRe

See RPcirculant

trials

See RPcirculant

useprimes

See RPcirculant

4. coords: Options for coordinates and units

coord_system

character. See coordinate systems

coordunits

See coordinate systems

coordnames

See coordinate systems

new_coord_system

See coordinate systems

new_coordunits

See coordinate systems

polar_coord

See coordinate systems

varnames

See coordinate systems

varunits

See coordinate systems

xyz_notation

See coordinate systems

zenit

See coordinate systems

5. direct: Options for simulating by simple matrix decomposition

max_variab

Maximal size of the covariance matrix.

Default: 12000

6. distr: Options for distributions, in particular RRrectangular

innermin

Default value to simulate from the RRrectangular distribution. The minimal length of the interval where the Taylor expansion shall be valid.

Default: 1e-20 .

maxit

Default value to simulate from the RRrectangular distribution.

The number of iterative steps where the the constant of the Taylor development is increased, to find an upper bound for the given function.

Default: 20 .

maxsteps

Default value to simulate from the RRrectangular distribution.

maxsteps is usually the number of steps in the middle part of the approximation. From this value and the length between the determined endpoints for the approximation at the origin and in the tail, the step length is calculated. If the step length is less than minsteplen the number of steps is reduced.

Default: 1000 .

mcmc_n

In case of the use of MCMC it leaves out n1n-1 member of the Markov chain bevor the nn member is returned. See also maxsteps.

Default: 15 .

minsteplen

Default value to simulate from the RRrectangular distribution. The minimal step length for the middle part of approximation, which is a step function,

Default: 0 (i.e. not used as a criterion.)

outermax

Default value to simulate from the RRrectangular distribution. The largest possible endpoint for the middle part that approximates the function by a step function. See also innermax.

Default: 20.

parts

Default value to simulate from the RRrectangular distribution.

parts determines the number of tests that are performed to check whether a proposed power function is an upper bound for the given function, at the origin and the tail.

Default: 8 .

repetitions

Minimal number of realisations to determine a quantity of the distribution by MCMC. E.g. to determine the integral value cc in the paper of Oesting, Schlather, Zhou.

Default: 1000.

safety

Default value to simulate from the RRrectangular distribution.

First, at the origin, the first power function of the Taylor expansion is taken as potential upper function. The constant of the power function are increased by factor 1+1 +safety and the exponent of the function similarly decreased. A number of test evaluations is performed to check whether this modified function is indeed a upper bound. If not, the considered interval at the origin is reduced iteratively, the constants of the power function further increased and the exponent decreased. If maxit iteration have been performed without success, the search for an upper bound fails. The search at the origin also fails if the interval around the origin has become less than innermin.

Similar procedure is performed for the tail.

Default: 0.08 .

7. empvario: Options for calculating the empirical variogram

fft

Logical. Determines whether FFT should be used for data on a grid Default: TRUE.

phi0

numeric. In case of anisotropic fields directional cones are considered. The argument phi0 determines the starting angle.

Default: 0.

pseudovariogram

logical. Only in the multivariate case. Whether the pseudovariogram or the crossvariogram should be calculated.

Default: FALSE.

theta0

numeric. In case of anisotropic fields directional cones are considered. The argument theta0 determines one of the boundaries, hence all boundaries for a given fixed number of cones. The argument theta0 determines the starting value of the second anglue in polar coordinate representation in 3 dimensions.

Default: 0.

tol0

numeric. Estimated values of the empirical variogram below tol0 times the grid step in the third dimension are considered to be zero. Hence the respective values are set to zero.

Default: 1e-13.

8. fit: Options for RFfit, RFratiotest, and RFcrossvalidate

algorithm

See RFfitOptimiser.

Default: NULL

approximate_functioncalls

In case the parameter vector is too close to the given bounds, the ML target function is evaluated on a grid to get a new initial value for the ML estimation. The number of points of the grid is approximately approximate_functioncalls.

Default: 50

boxcox_lb

lower bound for the Box-Cox transformation

Default: -10.

boxcox_ub

upper bound for the Box-Cox transformation

Default: 10.

bin_dist_factor

numeric. The empirical variogram is calculated up the distance bin_dist_factor times (maximum distance among any pair of locations)

Default: 0.5.

bins

vector of explicit boundaries for the bins or the number of bins for the empirical variogram (used in the LSQ target function, which is described at the beginning of the Details). Note that for anisotropic models, the value of bins might be enlarged.

Default: 20.

critical

logical or signed integer.

If critical=FALSE and if the result of any maximum likelihood method is on a borderline, then the optimisation is redone in a modified way (which takes about double extra time)

If critical=TRUE and if the result of any maximum likelihood method is on a borderline, then a kind of profile likelihood optimization is done (which takes about 10 times extra time)

If critical>=2 then a kind of profile likelihood optimization is always done (which takes about n_crit times extra time) for an automatically chosen selection of the model parameters.

If critical>=3 then a kind of profile likelihood optimization is always done (which takes about n_crit times extra time) for all the parameters.

If critical<0 then none of the refined methods are performed.

Default: TRUE.

cross_refit

logical. For each of the subset of the cross-validation method the parameters have to be fitted to the given model. If cross_refit is TRUE, this is done, but takes a huge amount of time. If FALSE, the model is fitted only once to the data and the value at each point is predicted with the same model given the values of the other points.

Default: FALSE.

estimate_variance

see RFlikelihood.

factr, factr_recall

See the argument control in optim. factr_recall is used for intermediate calculations.

likelihood

character – not programmed yet. types of likelihood are "auto", "full", "composite", "tesselation";

Default: "auto"

lowerbound_scale_factor

The lower bound for the scale is determined as

(minimum distance between different pairs of points) /
lowerbound_scale_factor.

Default: 3.

lowerbound_scale_ls_factor

For the LSQ target function a different lower bound for the scale is used. It is determined as

(minimum distance between different pairs of points) /
lowerbound_scale_ls_factor.

Default: 5.

lowerbound_var_factor

The lower bound for the nugget and the variance is determined as var(data) / lowerbound_var_factor. If a standard model definition is given and either the nugget or the variance is fixed, the parameter to be estimated must also be greater than lowerbound_sill.

Default: 10000.

maxmixedvar

OBSOLETE. upper bound for variance in a mixed model; so, the covariance model for mixed model part might be calibrated appropriately

max_neighbours

integer. Maximum number of locations (with depending values) that are allowed.

Default: 5000.

minbounddistance

If any value of the parameter vector returned from the ML estimation is closer than minbounddistance to any of the bounds or if any value has a relative distance smaller than minboundreldist, then it is assumed that the MLE algorithm has dropped into a local minimum, and it will be continued with evaluating the ML target function on a grid, cf. the beginning paragraphs of the Details.

Default: 0.001.

minboundreldist

relative distance to the bounds below which a part of the algorithm is considered as having failed. See minbounddistance.

Default: 0.02.

min_diag

Minimal value of any estimated diagonal matrix element.

Default: 1e-7.

n_crit

integer. The approximate profiles that are considered.

Default: 10.

nphi

scalar or vector of 2 components. If it is a vector then the first component gives the first angle of the xy plane and the second one gives the number of directions on the half circle. If scalar then the first angle is assumed to be zero. Note that a good estimation of the variogramm by LSQ with a anisotropic model a large value for ntheta might be needed (about 20).

Default: 1.

ntheta

scalar or vector of 2 components. If it is a vector then the first component gives the first angle in the third direction and the second one gives the number of directions on the half circle. If scalar then the first angle is assumed to be zero.

Note that a good estimation of the variogramm by LSQ with a anisotropic model a large value for ntheta might be needed (about 20).

Default: 1.

ntime

scalar or vector of 2 components. if ntimes is a vector, then the first component are the maximum time distance (in units of the grid length T[3]) and the second component gives the step size (in units of the grid length T[3]). If scalar then the step size is assumed to 1 (in units of the grid length T[3]).

Default: 20.

only_users

boolean. If true then only users_guess is used as a starting point for the fitting algorithms

Default: FALSE.

optimiser

See RFfitOptimiser.

Default: "optim".

pgtol, pgtol_recall

See the argument control in optim. pgtol_recall is used for intermediate calculations.

refine_onborder

logical. If TRUE and an estimated parameter of the model is close to the boundary, a second search for the optimum is started.

Default: TRUE

minmixedvar

lower bound for variance in a mixed model; so, the covariance model for mixed model part might be calibrated appropriately

Default: 1/1000

ratiotest_approx

logical. if TRUE the approximative formula that twice the difference of the likelihoods follow about a χ2\chi^2 distribution is used. The parameter of freedom equals the number of parameters to be estimated for the covariance function, including those for the covariates.

Default: TRUE

reoptimise

logical. If TRUE && !only_users then at a very last step, the optimisation is redone with currently best parameters and likelihood as scale parameter for optim.

Default: TRUE.

scale_max_relative_factor

If the initial scale value for the ML estimation obtained by the LSQ target function is less than (minimumdistancebetweendifferentpairsofpoints)/(minimum distance between different pairs of points) / scale_max_relative_factor

a warning is given that probably a nugget effect is present. Note: if scale_max_relative_factor is greater than lowerbound_scale_ls_factor then no warning is given as the scale has the lower bound (minimumdistancebetweendifferentpairsofpoints)/(minimum distance between different pairs of points) / lowerbound_scale_ls_factor.

Default: 1000

scale_ratio

RFfit uses parscale and fnscale in the calls of optim. As these arguments should have the magnitude of the estimated values, RFfit checks this by calculating the absolute log ratios. If they are larger than scale_ratio, parscale and fnscale are reset and the optimisation is redone.

Default: 0.1.

shortnamelength

The names of the variables in the returned table are abbreviated by taking the first shortnamelength letters.

Default: 4.

smalldataset

If the number of locations is considered as small, then some more data are kept in the storage to accelerate the estimation algorithm.

Default: 2000.

split

integer. If the number of parameters to be numerically optimised is larger than or equal to split then RFfit checks whether a space-time covariance model or a multivariate covariance model can be split into components, so that certain parameters can be estimated separately.

Default: 4.

cliquesize

integer. RFfit tries to split the data set into parts of size splitn_neighbours[2] or less, but never more than splitn_neighbours[3] and never less than splitn_neighbours[1].

Default: c(200, 1000, 3000).

splitfactor_neighbours

The total number of neighbouring boxes in each direction 1+2splitfactor1 + 2\code{splitfactor}, including the current box itself.

Default: 2.

split_refined

logical. If TRUE then also submodels are fitted if splitted. This takes more time, but anova and RFratiotest, for instance, will give additional information.

Default: TRUE.

upperbound_scale_factor

The upper bound for the scale is determined as

upperbound_scale_factor * (maximum distance between all pairs of points).

Default: 3.

upperbound_var_factor

The upper bound for the variance and the nugget is determined as upperbound_var_factor * var(data)

Default: 10.

use_naturalscaling

logical. Only used if model is given in standard (simple) way. If TRUE then internally, rescaled covariance functions will be used for which cov(1)\approx0.05. use_naturalscaling has the advantage that scale and the form parameters of the model get ‘orthogonal’, but use_naturalscaling does not work for all models.

Note that this argument does not influence the output of RFfit: the parameter vector returned by RFfit refers always to the standard covariance model as given in RMmodel. (In contrast to practicalrange in RFoptions.)
Advantages if use_naturalscaling=TRUE:

  • scale and the shape parameter of a parameterised covariance model can be estimated better if they are estimated simultaneously.

  • The estimated bounds calculated by means of upperbound_scale_factor and lowerbound_scale_factor, etc. might be more realistic.

  • in case of anisotropic models, the inverse of the elements of the anisotropy matrix should be in the above bounds.

Disadvantages if use_naturalscaling=TRUE:

  • For some covariance models with additional parameters, the rescaling factor has to be determined numerically. Then, more time is needed to perform RFfit.

  • note the use_naturalscaling only affects simple models, no operators. Also functions that define a parameter of the model are not changed.

Default: FALSE.

9. gauss: Options for simulating Gaussian random fields

approx_zero

Value below which a correlation is considered to be essentially zero. This argument is used to determine the practical range of covariance function with non-compact support.

Default: 0.05

boxcox

real vector of one or two components. If the first component is Inf then no transformation is performed. Otherwise the BoxCox transformation is performed. Note that Box Cox only works in a Gaussian framework. Note further that either boxcox or loggauss may be given.

Default c(Inf, 0)

direct_bestvar

integer. When searching for an appropriate simuation method the matrix decomposition method (method="direct") is preferred if the number of variables is less than or equal to direct_bestvariables.

Default is 1200.

loggauss

logical. Whether a log-Gauss random fields should be returned. See also boxcox for a generalisation.

paired

(“Antithetic pairs”.) Logical. If TRUE then the second half of the simulations is logical. If TRUE then the second half of the simulations is obtained by only changing the signs of all the standard Gaussian random variables, on which the first half of the simulations is based. Default is FALSE.

stationary_only

See RPgauss

10. graphics: Options for graphical output

always_close_device

logical. If FALSE the current device is kept as it is; otherwise the current device is closed before the next device is opened. If NA it closes the preceding device if the opened device is pdf or jpeg.

Default: NA.

always_open_device

logical. If TRUE a new graphical window is opened for every plot if a standard graphical output is used, trying to respect the aspect ratios for the plots. The devices pdf and jpeg are always opened.

If NA then the value is set to interactive().

Default: TRUE.

close_screen

logical; only relevant if split_screen = TRUE and always_close_screen = FALSE. If FALSE the windows opened by split.screen are left open.

Default: TRUE.

filecharacter; only relevant if split_screen = TRUE. argument file in pdf If "" then no internal naming is performed.

Default: "".

filenumber

integer; only relevant if split_screen = TRUE. Starting number of the file if onefile=FALSE. It is set to 0 whenever file is changed and onefile=FALSE.

Default 0.

grDefault

logical. If FALSE the graphic style up to Version 3.2 is used. Otherwise, the changes of th graphical style are reduced to a minimum.

Default: FALSE

grPrintlevel

integer values 0, 1, 2; only relevant when simulations are plotted. The higher the more text is shown in the plot.

Default: 1.

height

real number; only relevant if a new device is opened, see alwyas_open_screen.

  • height=NA or height is not positive: no device is opened.

  • width = NA If height is greater than zero then it gives the height of a single figure in a plot created by RandomFields; See also close_screen.

    If plots with multiple figures are shown, the height and width of the plot will be increased by a factor up the ones given by increase_upto.

    The width is calculated so that the aspect ratio is correct.

  • width not NA height and width give the size of the whole window.

Default: 6.

increase_upto

See height.

Default: c(3,4).

split_screen

logical. If TRUE split.screen is used to split the screen. Otherwise par(mfcol). When using split_screen then the figures tend to be fancier.

Default: TRUE.

onefile

logical; only relevant if split_screen = TRUE. About the behaviour of argument onefile in pdf

Default: FALSE.

width

real number or NA; only relevant if always_open_screen=TRUE. See height for details.

Default: NA.

11. gui: Options for cRFgui

alwaysSimulate

logical. If TRUE then a new random field is simulated whenever a parameter is changed. Otherwise only the covariance function or the variogram is re-plotted; simulations are performed only when the correponding button is pressed.

Default: TRUE.

simu_method

"RPcirculant", "RPcutoff", "RPintrinsic", "RPtbm", "RPspectral", "RPdirect", "RPsequential", "RPaverage", "RPnugget", "RPcoins", "RPhyperplane", "RPspecific", "any method".

Default: "RPcirculant".

size

vector of 2 components. Grid size of the simulated stochastic processes. The two components of the vector correspond to one-dimensional and two-dimensional processes, respectively.

Default: c(1024, 64).

12. hyper: Options for simulating hyperplane tessellations

mar_distr

integer. This argument should not be changed yet.

It codes the marginal distribution used in the simulation:

0 : uniform distribution
1 : Frechet distribution with form argument mar_param
2 : Bernoulli distribution (Binomial with n=1n=1) with argument mar_param

Default: 0 .

mar_param

Argument used for the marginal distribution. The argument should not be changed yet.

Default: NA .

maxlines

integer. Maximum number of allowed lines.

Default: 1000 .

superpos

integer. number of superposed hyperplane tessellations.

Default: 300 .

13. krige: Options for Kriging

cholesky_R

obsolete

fillall

logical value for imputing. If true all the components are estimated whether they are NA or not.

Default: TRUE.

locmaxn

Kriging is conditions on maximal locmaxn points. If the data contain more points, neighbourhood kriging is performed.

Default: 8000.

locsplitfactor

In case of neighbourhood kriging, the area is split into small boxes. The complete neighbourhood contains (2 * locsplitfactor +1) boxes in each direction.

Default: 2.

locsplitn

vector of 3 components. A box should contain no more than locsplitn[3] points, but never less than locsplitn[1]. If a box had originally less than locsplitn[1] points, then the box is increased until at least locsplitn[2] points are in the box.

Default: c(200, 1000, 5000).

method

obsolete

return.variance

logical. If FALSE the kriged field is returned. If TRUE a list of two elements, estim and var, i.e. the kriged field and the kriging variances, is returned.

Default: FALSE.

14. maxstable: Options for simulating max-stable random fields

check_every

integer. In order to get a precise simulation result, by definition, the maximum must be taken, for each shape function, over alle locations of interest. Clearly, small values will not play a role. To this end, the global minimum has to be determined. The calculation of the global minimum is expensive and therefor should not be done too frequently. On the other hand, rare updates increases the computing times for taking the maximum over a single shape functions. Here, after every check_every considered shape function, the global minimum is calculated. It is expected that a good choice for check_every is in in the interval [10,100][10, 100].

(For ease and for concerns of efficiency, the more adequate, local minimum is not considered.)

Default: 30 .

density_ratio

value in [0,1][0,1]. This argument is considered only if flat=-1 and the simulation is performed on a grid. Then, the ratio between the highest and the lowest value is calculated within the convex hull of the grid. If the value is less than density_ratio then the grid points are considered separately. Else the density is considered to be constant in the convex hull of the grid.

Default: 0.0.

eps_zhou

positive real number, which gives the aimed relative precision when the constant cc in the paper of Oesting, Schlather, Zhou (2018) has to be estimated. E.g. if eps_zhou=0.01 then the first 2 digits should be correct.

Default: 0.01

flathull

NA, FALSE, TRUE. Only used in M3 modelling in the algorithm by Oesting, Schlather, Zhou (2018). The argument is considered only if the simulation is performed on a grid. If flat=TRUE , then the density is considered to be flat in the convex hull of the grid, i.e. the simulation method of Schlather (2002) is used. If flat=NA the choice is done automatically.

Default: FALSE .

max_gauss

The simulation of the max-stable process by the old-fashioned method of Schlather (2002) and by older methods for Brown-Resnick processes uses a stopping rule that necessarily needs a finite upper endpoint of the marginal distribution of the random field. In the case of Brown-Resnick processes, extremal Gaussian fields, and extremal t fields, the upper endpoint is approximated by standardmax.

Default: 3.0 .

max_n_zhou

positive integer. The overall constant cc in the paper of Oesting, Schlather, Zhou (2018) has to be determined by MCMC, if the shape functions are random.

The two arguments, min_n_zhou and max_n_zhou, give the minimal and the maximal number of simulations that are performed. To economize computer time the values of cc is partially estimated when the shape functions are simulated. If the number of shape functions is larger than the number of simulations given by eps_zhou then no further simulation is performed to determine cc. So, it is advantageous to simulate all fields at once by RFsimulate(..., n = ).

Default: 1000 and 10000000, respectively.

maxpoints

positive integer; the maximal number of Poisson points to be simulated for one realization of the max-stable random field. This option will not be considered for most of the users. This option allows the simulation to interrupt after maxpoints shape function have been placed.

Default: 2e9 (never).

mcmc_zhou

positive integer. In case of random shape functions, an MCMC step is required. mcmc_zhou-1 equals the number of members of the MCMC chain that are left out before the next value of the chain is returned.

Default: 20

min_n_zhou

see max_n_zhou

mcmc_zhou

positive integer. In case of random shape functions, an MCMC step is required. mcmc_zhou-1 equals the number of members of the MCMC chain that are left out before the next value of the chain is returned.

Default: 20

min_n_zhou

see max_n_zhou

min_shape_gumbel

To increase speed, the minimum field value is assumed to be min_shape_gumbel for calculation of threshold values for simulation short cuts. During a simulation, its value becomes void as soon as the real (current) minimum of the field being simulated exceeds min_shape_gumbel

Default: -1e15.

scatter_method

logical. If

Default: NA;

xi

Extreme value index. Default: 2e9 . While ξ\xi can be set globally, the shift μ\mu and the scale ss can be given only locally within the process definitions, e.g., RPsmith.

Default: 1.0.

15. mpp: Options for the random coins (shot noise) methods

about_zero

In certain cases (Coins,RMtruncsupport), functions are assumed to zero if the value is less than about_zero.

Default: 0.001 .

n_estim_E

integer. Number of draws from the distribution of the scale to estimate the mean of the distribution. This is used only if the mean of the scale distribution is not explicitely given. Default: 50000 .

scatter_method
scatter_size, scatter_max

Real valued and integer valued, respectively, or NA.

Used in the internal function RMscatter that calculates i=1nf(x+hi)\sum_{i=1}^n f(x + h_i) for some function ff and for some distances hih_i.

Let ε=\varepsilon=about_zero, s=s=scatter_size and m=m=scatter_max. We distinguish 4 cases:

  • scatter_size > 0 and scatter_max >= 0
    Here, nn equals (2m)d(2m)^d. and hiM={(ks,,ks),,(ms,,ms)}h_i \in M = \{ (k s, \ldots, k s),\ldots, (m s, \ldots, m s)\} with k=mk=-m.

  • scatter_size > 0 and scatter_max < 0
    same as the previous case, but mm is chosen such that f(kieisi)εf(k_i e_i s_i) \approx \varepsilon, kiN-k_i\in N, i=1,,di=1,\ldots,d and f(mieisi)εf(m_i e_i s_i) \approx \varepsilon, mNm \in N.

  • scatter_size <= 0 and scatter_max >= 0
    This option is possible only for grids. Here hih_i runs on the given grid i=1,,di=1,\ldots,d, but at most scatter_max steps.

  • scatter_size <= 0 and scatter_max < 0
    this option is possible only for grids. Here, hih_i runs over the whole grid.

shape_power

Shape functions are powered by shape_power before used as intensity function for the point process.

Default: 2.0.

16. nugget: Options for the nugget effect
Simulating a nugget effect is per se trivial. However, it gets complicated and best methods (including direct and circulant embedding!) fail if zonal anisotropies are considered, where sets of points have to be identified that belong to the same subspace of eigenvalue 0 of the anisotropy matrix.

tol

The nugget tolerance influences two different kind of models

See there for more information.

17. registers: Register numbers
Model for different purposes are or can be stored at different places. They are called registers and have non-negative numbers up to 21 (currently). The user can use the registers 0..9.

register

number in 0:9; place where intermediate calculation for random field simulation are stored; the number refers to 10 internal registers 0..9.

Changing the register number only makes sense, when two different random fields, say, are to be simulated alternatingly, several times in a row. Then the simlulation speed can be increased if several registers are used, storing=TRUE and RFsimulate is used with the only argument n.

Default: 0

18. sequ: Options for the sequential method

back_steps

See RPsequential

initial

See RPsequential

max_variables

See RPsequential

19. solve: Options for solving linear systems

det_as_log

See RFoptions

eigen2zero

See RFoptions

max_chol

integer. Maximum number of rows of a matrix in a Cholesky decomposition

Default: 81928192

max_svd

integer. Maximum number of rows of a matrix in a svd decomposition

Default: 65556555

pivot

Type of pivoting for the Cholesky decomposition. Possible values are

PIVOT_NONE

No pivoting.

PIVOT_AUTO

If the matrix has a size greater than 3x3 and Choleskey fails without pivoting, privoting is done. For matrices of size less than 4x4, no pivoting and no checks are performed.

PIVOT_DO

Do alwaoys pivoting. NOTE: privoted Cholesky decomposition yields only very approximately an upper triangular matrix L, but still L^t L = M holds true.

PIVOT_IDX

uses the same pivoting as in the previous pivoted decomposition. This option becomes relevant only when simulations with different parameters or different models shall be performed with the same seed so that also the pivoting must be coupled.

Default: PIVOT_auto

pivot_actual_size

See RFoptions

pivot_check

logical. Only used in pivoted Cholesky decomposition. If TRUE and a numerically zero diagonal element is detected, it is checked whether the offdiagonal elements are numerically zero as well. (See also pivot_max_deviation and pivot_max_reldeviation.) if NA then, in RPdirect, the value is equivent to

FALSE

if the model is positive (semi-)definite.

TRUE

if the model is genuinely negative definite.

Default: NA

pivot_idx

See RFoptions

pivot_relerror

See RFoptions

pivot_max_deviation

See RFoptions

pivot_max_reldeviation

See RFoptions

solve_method

See RFoptions

spam_factor

See RFoptions

spam_min_n

See RFoptions

spam_min_p

See RFoptions

spam_pivot

See RFoptions

spam_sample_n

See RFoptions

spam_tol

See RFoptions

svdtol

See RFoptions

use_spam

See RFoptions

20. special: Options for specific methods

multicopies

Only used by RMmult. The covariance functions are multiplied if the corresponding independent random fields are multiplied. To get an approximative Gaussian random fields with a multiplicative covariance functions the average over multicopies products of random fields is calculated.

21. spectral: Options for the spectral (turning bands) method

ergodic

In case of an additive model and ergodic=FALSE, the additive component are chosen proportional to their variance. In total lines are simulated. If ergodic=TRUE, the components are simulated separately and then added.

Default: FALSE.

prop_factor

see RPspectral

sigma

see RPspectral

sp_grid

see RPspectral

sp_lines

see RPspectral

22. tbm: Options for the turning bands method

center

Scalar or vector. If not NA, the center is used as the center of the turning bands for TBM2 and TBM3. Otherwise the center is determined automatically such that the line length is minimal. See also points and the examples below.

Default: NA .

fulldim

positiv integer. The dimension of the space into which the simulated field is embedded. So, the value fulldim must be at least the dimension of the field.

Default: 3.

grid

Logical. The angle of the lines is random if grid=FALSE, and kπ/k\pi/lines for kk in 1:lines, otherwise.

This option is used by both RPspectral and RPtbm, the latter only when the dimension is 2.

Default: TRUE .

layers

Logical or integer. If TRUE then the turning layers are used whenever a time component is given. If NA the turning layers are used only when the traditional TBM is not applicable. If FALSE then turning layers may never be used.

Default: TRUE .

lines

Number of lines used.

Default: 60 .

linesimustep

If linesimustep is positive the grid on the line has lag linesimustep. See also linesimufactor.

Default: 0.0 .

linesimufactor

linesimufactor or linesimustep must be non-negative; if linesimustep is positive then linesimufactor is ignored. If both arguments are naught then points is used (and must be positive). The grid on the line is linesimufactor-times finer than the smallest distance. See also linesimustep.

Default: 2.0 .

points

integer. If greater than 0, points gives the number of points simulated on the TBM line, hence must be greater than the minimal number of points given by the size of the simulated field and the two paramters TBMx.linesimufactor and TBMx.linesimustep. If points is not positive the number of points is determined automatically. The use of center and points is highlighted in an example below.

Default: 0.

reduceddim

if positiv integer, then the value itself. If negativ, then the value is substracted from fulldim.

Default: -2.

23. internal: Internal options mostly for warnings and messages

All these options should not be changed by the user unless he/she really known what he/she is doing.

Most of the options below change their value in a session without the user's notice.

do_tests

Internal variable. Do not use it. Default: FALSE.

examples_reduced

non-negative integer. If positve, then the design of any simulation in RandomFields is internally reduced in size (roughly downto the given value in each direction). Warnings report this behaviour. This option is necessary to run the examples of RandomFields under the time constraint of CRAN.

stored.init

internally used logical argument. This option is closely related to storing which controls whether intermediate calculations should be stored to have faster repeated simulations.

This user option is internally overwritten if the user calls several simulations at once. This current value is stored in stored.init.

Default: FALSE.

warn_ambiguous

internally used logical argument. Usually, the argument grid in RFsimulate, for instance, can or should be given. If not given, the system takes a default definition. Additionally a message is displayed in this case if ambiguous=TRUE.

Default: FALSE.

warn_aspect_ratio

internally used logical argument. if TRUE then a warning is given not a standard graphical device is used and the package plots try to keep a certain aspect ratio.

Default: TRUE

warn_colour_palette

internally used logical argument. If none of the packages RColorBrewer and colorspace are available and graphics are displayed, a message is displayed.

Default: TRUE.

warn_constant

The definition of RMconstant has changed. A warning is displayed if the command is used. warn_constant will become obsolete in future versions.

Default: TRUE.

warn_coordinates

internally used logical argument. If TRUE then a transformation from earth coordinates to cartesian coordinates is reported.

Default: TRUE.

allow_duplicated_locations

logical. If FALSE duplicated locations are not allowed. If TRUE then the (standard) nugget effect becomes a non-stationary model in an abstract space that cannot be extended outside the given locations. See also RMnugget for the distinction between measurement error and spatial nugget.

Default: FALSE.

warn_missing_zenit

Only for Earth systems: a missing zenit is frequently a cause for errors that are difficult to understand. Therefore, in such cases an additional warning message is displayed.

Default: TRUE

warn_newAniso

obsolete.
internally used logical argument. If newAniso=TRUE and the argument Aniso is used in the model definition, then a message is displayed that the matrix Aniso is multiplied from the right by xx, where up to Version 2.0 the argument aniso was available which was multiplied from the left by xx.

Default: TRUE.

warn_newstyle

internally used logical argument. If TRUE a message is displayed the by the argument spConform=FALSE oldstyle return values are obtained instead of S4 objects.

Default: TRUE.

warn_normal_mode

internally used logical argument. if TRUE then the function RFfit displays the message that other values for the option modus_operandi are available.

Default: TRUE.

warn_oldstyle

internally used logical argument. If TRUE a warning is given if an obsolete function from Version 2 is used.

Default: TRUE.

warn_on_grid

internally used logical argument. If a (one-dimensional) grid is given, but the argument grid=FALSE, e.g. in RFsimulate, this contraction is reported if warn_on_grid=TRUE

Default: TRUE.

warn_scale

internally used logical argument. If warn_scale=TRUE then a scale less than 10 [km] is reported if earth coordinates are transformed to cartesian coordinates.

Default: TRUE.

warn_var

In some cases, RandomFields cannot detect whether the variance is non-negative. If TRUE then a warning is displayed in such a case. Default: TRUE.

Value

NULL if any argument is given, and the full list of arguments, otherwise.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Basic

  • General

    • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

    • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

  • rectangular distribution; eps_zhou

    • Oesting, M., Schlather, M. and Zhou, C. (2013) On the Normalized Spectral Representation of Max-Stable Processes on a compact set. arXiv, 1310.1813

  • shape_power

    • Ballani, F. and Schlather, M. (2015) In preparation.

See Also

RFsimulate, RFoptionsAdvanced, RFoptions, and RFgetMethodNames.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions()


############################################################
##                                                        ## 
## use of exactness                                       ##
##                                                        ##
############################################################
x <- seq(0, 1, 1/30)
model <- RMgauss()

for (exactness in c(NA, FALSE, TRUE)) { 
  readline(paste("\n\nexactness: `", exactness, "'; press return"))
  z <- RFsimulate(model, x, x, exactness=exactness,
                  stationary_only=NA, storing=TRUE)
  print(RFgetModelInfo(which="internal")$internal$name)
}

Setting control arguments of RandomFields – advanced examples

Description

Some more complex examples for the use of RFoptions are given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Examples

#############################################################
 ##                      EXAMPLE 1                          ##
 ## The following gives an example on the advantage of      ##
 ## dependent=TRUE for simulating with RPcirculant if, in a ##
 ## study, most of the time is spent with simulating the    ##
 ## Gaussian random fields. Here, the covariance at a pair  ##
 ## of points is estimated for n independent repetitions    ##
 ## and 2*n locally dependent repetitions.                  ##
 ## To get the precision, the procedure is repeated m times.##
 #############################################################

# In the example below, local.dependent speeds up the simulation
# by about factor 16 at the price of an increased variance of
# factor 1.5

RFoptions(seed=NA)
len <- 10

x <- seq(0, 1, len=len)
y <- seq(0, 1, len=len)
grid.size <- c(length(x), length(y))
meth <- RPcirculant
model <- RMexp(var=1.1, Aniso=matrix(nc=2, c(2,0.1,1.5,1)))

m <- 5 
n <- 100


# using local.dependent=FALSE (which is the default)
c1 <- numeric(m)
time <- system.time(
  for (i in 1:m) {
    cat("", i, "out of", m, "\n")
    z <- RFsimulate(meth(model), x, y, n=n, pch="", 
                    dependent=FALSE, spConform=FALSE, trials=5, force=TRUE)
    c1[i] <- cov(z[1, dim(z)[2], ], z[dim(z)[1], 1, ])
}) # many times slower than with local.dependent=TRUE below

true.cov <- RFcov(model, t(y[c(1, length(y))]), t(x[c(length(x), 1)]))
print(time)
Print(true.cov, mean(c1), sd(c1), empty.lines=1)## true mean is zero

# using local.dependent=TRUE ...
c2 <- numeric(m)
time <- system.time(
  for (i in 1:m) {
    cat("", i)
    z <- RFsimulate(meth(model), x, y, n=2 * n, pch="", 
                    dependent=TRUE, spConform=FALSE, trials=5, force=TRUE)
    c2[i] <- cov(z[1, dim(z)[2], ], z[dim(z)[1], 1, ])
})

print(time)                                      ## 20 times faster
Print(true.cov, mean(c2), sd(c2), empty.lines=1) ## much better results

## the sd is smaller (using more locally dependent realisations)
## but it is (much) faster! Note that for n=n2 instead of n=2 * n, 
## the value of sd(c2) would be larger due to the local dependencies 
## in the realisations.




 #############################################################
 ##                      EXAMPLE 2                          ##
 ## This example shows that the same realisation can be     ##
 ## obtained on different grid geometries (or point         ##
 ## configurations, i.e. grid, non-grid) using TBM          ##
 #############################################################

RFoptions(seed=0)
step <- 1
x1 <- seq(-150,150,step)
y1 <- seq(-15, 15, step)
x2 <- seq(-50, 50, step)
model <- RPtbm(RMexp(scale=10))


RFoptions(storing=TRUE)
mar <- c(2.2, 2.2, 0.1, 0.1)
points <- 700

###### simulation of a random field on long thin stripe
z1 <- RFsimulate(model, x1, y1, center=0, seed=0,
                 points=points, storing=TRUE, spConform=FALSE)
ScreenDevice(height=1.55, width=12)
par(mar=mar)
image(x1, y1, z1, col=rainbow(100))
polygon(range(x2)[c(1,2,2,1)], range(y1)[c(1,1,2,2)],
        border="red", lwd=3)


###### definition of a random field on a square of shorter diagonal
z2 <- RFsimulate(model, x2, x2, register=1, seed=0,
                 center=0, points=points, spConform=FALSE)
ScreenDevice(height=4.3, width=4.3)
par(mar=mar)
image(x2, x2, z2, zlim=range(z1), col=rainbow(100))
polygon(range(x2)[c(1,2,2,1)], range(y1)[c(1,1,2,2)],
        border="red", lwd=3)
tbm.points <- RFgetModelInfo(level=3)$loc$totpts
Print(tbm.points, empty.lines=0) # number of points on the line

Graphical parameters for plots

Description

This function sets globally graphical parameters for plots of RMmodels, simulations and estimations.

Usage

RFpar(...)

Arguments

...

see par

Value

If RFpar is called without arguments, the current list is returned.

If RFpar is called with NULL only, the current list is deleted.

Otherwise the arguments are stored for global use in RandomFields.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

plot-method

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFpar(col="red")
plot(RMexp())

Class RFpointsDataFrame

Description

Class for attributes in one-dimensional space that are not on a grid.

Usage

## S4 method for signature 'RFpointsDataFrame'
RFspDataFrame2conventional(obj)

Arguments

obj

an RFspatialPointsDataFrame object

Creating Objects

Objects can be created by using the functions RFpointsDataFrame or conventional2RFspDataFrame or by calls of the form as(x, "RFpointsDataFrame"), where x is of class RFpointsDataFrame.

Slots

data:

object of class data.frame, containing attribute data

coords:

n-times-1 matrix of coordinates (each row is a point)

.RFparams:

list of 2; .RFparams$n is the number of repetitions of the random field contained in the data slot, .RFparams$vdim gives the dimension of the values of the random field, equals 1 in most cases

Methods

plot

signature(obj = "RFpointsDataFrame"): generates nice plots of the random field; if spacetimedim2space-time-dim2, a two-dimensional subspace can be selected using the argument MARGIN; to get different slices in a third direction, the argument MARGIN.slices can be used; for more details see plot-method or type method?plot("RFpointsDataFrame").

show

signature(x = "RFpointsDataFrame"): uses the show-method for class SpatialPointsDataFrame.

print

signature(x = "RFpointsDataFrame"): identical to show-method

RFspDataFrame2conventional

signature(obj = "RFpointsDataFrame"): conversion to a list of non-sp-package based objects; the data-slot is converted to an array of dimension [1(vdim>1)+spacetimedimension+1(n>1)][1*(vdim>1) + space-time-dimension + 1*(n>1)]

coordinates

signature(x = "RFpointsDataFrame"): returns the coordinates

[

signature(x = "RFpointsDataFrame"): selects columns of data-slot; returns an object of class RFpointsDataFrame.

[<-

signature(x = "RFpointsDataFrame"): replaces columns of data-slot; returns an object of class RFpointsDataFrame.

as

signature(x = "RFpointsDataFrame"): converts into other formats, only implemented for target class RFgridDataFrame

cbind

signature(...): if arguments have identical topology, combine their attribute values

range

signature(x = "RFpointsDataFrame"): returns the range

hist

signature(x = "RFpointsDataFrame"): plots histogram

as.matrix

signature(x = "RFpointsDataFrame"): converts data-slot to matrix

as.array

signature(x = "RFpointsDataFrame"): converts data-slot to array

as.vector

signature(x = "RFpointsDataFrame"): converts data-slot to vector

as.data.frame

signature(x = "RFpointsDataFrame"): converts data-slot and coordinates to a data.frame

Details

Methods summary and dimensions are defined for the “parent”-class RFsp.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFspatialPointsDataFrame, which is for point locations in higher dimensional spaces, RFpointsDataFrame-class which is for one-dimensional locations on a grid, RFsp

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- runif(100)
f <- RFsimulate(model=RMexp(), x=x, n=3)

str(f)
str(RFspDataFrame2conventional(f))
head(coordinates(f))
str(f[2]) ## selects second column of data-slot
all.equal(f, cbind(f,f)[1:3]) ## TRUE

plot(f, nmax=2)

Empirical Pseudomadogram

Description

Calculates the empirical pseudomadogram. The empirical pseudomadogram of two random fields XX and YY is given by

γ(r):=1N(r)(ti,tj)ti,j=r(X(ti)X(tj))(Y(ti)Y(tj))\gamma(r):=\frac{1}{N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} |(X(t_{i})-X(t_{j}))||(Y(t_{i})-Y(t_{j}))|

where ti,j:=titjt_{i,j}:=t_{i}-t_{j}, and where N(r)N(r) denotes the number of pairs of data points with distancevector ti,j=rt_{i,j}=r.

Usage

RFpseudomadogram(model, x, y=NULL, z=NULL, T=NULL, grid, params, distances,
           dim, ..., data, bin=NULL, phi=NULL, theta = NULL,
           deltaT = NULL, vdim=NULL)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

bin

a vector giving the borders of the bins; If not specified an array describing the empirical (pseudo-)(cross-) covariance function in every direction is returned.

phi

an integer defining the number of sectors one half of the X/Y plane shall be divided into. If not specified, either an array is returned (if bin missing) or isotropy is assumed (if bin specified).

theta

an integer defining the number of sectors one half of the X/Z plane shall be divided into. Use only for dimension d=3d=3 if phi is already specified.

deltaT

vector of length 2, specifying the temporal bins. The internal bin vector becomes seq(from=0, to=deltaT[1], by=deltaT[2])

vdim

the number of variables of a multivariate data set. If not given and data is an RFsp object created by RandomFields, the information there is taken from there. Otherwise vdim is assumed to be one. NOTE: still the argument vdim is an experimental stage.

Details

RFpseudomadogram computes the empirical pseudomadogram for given (multivariate) spatial data.

The spatial coordinates x, y, z should be vectors. For random fields of spatial dimension d>3d > 3 write all vectors as columns of matrix x. In this case do neither use y, nor z and write the columns in gridtriple notation.

If the data is spatially located on a grid a fast algorithm based on the fast Fourier transformed (fft) will be used. As advanced option the calculation method can also be changed for grid data (see RFoptions.)

It is also possible to use RFpseudomadogram to calculate the pseudomadogram (see RFoptions).

Value

RFpseudomadogram returns objects of class RFempVariog.

Author(s)

Jonas Auel; Sebastian Engelke; Johannes Martini; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RMstable, RMmodel, RFsimulate, RFfit, RFcov, RFmadogram. RFvariogram.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMbiwm(nudiag=c(1, 2), nured=1, rhored=1, cdiag=c(1, 5), 
                s=c(1, 1, 2))
n <- 2
x <- seq(0, 20, 0.1)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFpseudomadogram(data=z)
plot(emp.vario)

Pseudovariogram

Description

Calculates the theoretical and empirical Pseudovariogram.

Usage

RFpseudovariogram(model, x, y=NULL, z = NULL, T=NULL, grid, params, distances,
            dim, ..., data, bin=NULL, phi=NULL, theta = NULL,
            deltaT = NULL, vdim=NULL)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

bin

a vector giving the borders of the bins; If not specified an array describing the empirical (pseudo-)(cross-) covariance function in every direction is returned.

phi

an integer defining the number of sectors one half of the X/Y plane shall be divided into. If not specified, either an array is returned (if bin missing) or isotropy is assumed (if bin specified).

theta

an integer defining the number of sectors one half of the X/Z plane shall be divided into. Use only for dimension d=3d=3 if phi is already specified.

deltaT

vector of length 2, specifying the temporal bins. The internal bin vector becomes seq(from=0, to=deltaT[1], by=deltaT[2])

vdim

the number of variables of a multivariate data set. If not given and data is an RFsp object created by RandomFields, the information there is taken from there. Otherwise vdim is assumed to be one. NOTE: still the argument vdim is an experimental stage.

Details

RFpseudovariogram computes the empirical pseudovariogram for given (multivariate) spatial data.

The spatial coordinates x, y, z should be vectors. For random fields of spatial dimension d>3d > 3 write all vectors as columns of matrix x. In this case do neither use y, nor z and write the columns in gridtriple notation.

If the data is spatially located on a grid a fast algorithm based on the fast Fourier transformed (fft) will be used. As advanced option the calculation method can also be changed for grid data (see RFoptions.)

Value

an objects of class RFempVariog.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RMstable, RMmodel, RFsimulate, RFfit, RFcov, RFmadogram. RFvariogram,

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


model <- RMbiwm(nudiag=c(1, 2), nured=1, rhored=1, cdiag=c(1, 5), 
                s=c(1, 1, 2))
x <- seq(0, 20, 0.1)
z <- RFsimulate(model, x=x, y=x, n=2)
emp.vario <- RFpseudovariogram(data=z)
plot(emp.vario, model=model)

Likelihood ratio test

Description

The function performs an approximate chi2 test or a Monte Carlo likelihood ratio test based on fitgauss. Currently, it only works for Gaussian random fields.

Usage

RFratiotest(nullmodel, alternative, x, y = NULL, z = NULL, T = NULL,
            grid=NULL, data, alpha, n = 5 / alpha, seed = 0, 
            lower = NULL, upper = NULL, methods,
            sub.methods, optim.control = NULL, users.guess = NULL,
            distances = NULL, dim, transform = NULL, ...)

Arguments

nullmodel, alternative

See Details.

The set of parameters to be estimated for nullmodel should be a subset of the parameters to be estimated for alternative if alternative is given.

alpha

value in [0,1] or missing. Significance level.

n

integer. The test is based on n-1 simulations.

seed

integer. If not NULL and not NA, the .Random.seed is set to seed. Otherwise, set.seed is set to the value of RFoptions{}$basic$seed if the latter is not NA.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

lower

list or vector. Lower bounds for the parameters. If lower is a vector, lower has to be a vector as well and its length must equal the number of parameters to be estimated. The order of lower has to be maintained. A component being NA means that no manual lower bound for the corresponding parameter is set.
If lower is a list, lower has to be of (exactly) the same structure of the model.

upper

list or vector. Upper bounds for the parameters. See lower.

methods

Main methods to be used for estimating. If several methods are given, estimation will be performed with each method and the results reported.

sub.methods

variants of the least squares fit of the variogram. variants of the maximum likelihood fit of the covariance function. See RFfit for details.

users.guess

User's guess of the parameters. All the parameters must be given using the same rules as for lower (except that no NA's should be contained).

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

optim.control

control list for optim, which uses ‘L-BFGS-B’. However parscale may not be given.

transform

obsolete for users; use param instead. transform=list() will return structural information to set up the correct function.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

nullmodel (and the alternative) can be

  • a covariance model, see RMmodel or type RFgetModelNames(type="variogram") to get all options.

    If RFoptions ratiotest_approx is TRUE the chisq approximation is performed. Otherwise a Monte Carlo ratio test is performed.

  • RFfit or RMmodelFit

    Here, a chisq approximative test is always performed on the already fitted models.

RFratiotest tries to detect whether nullmodel is a submodel of alternative. If it fails,

  • a message is printed that says that an automatic detection has not been possible;

  • it is not guaranteed anymore that the alternative model returns a (log) likelihood that is at least as large as that of the nullmodel, even if nullmodel is a submodel of alternative. This is due to numerical optimisation which is never perfect.

Otherwise it is guaranteed that the alternative model has a (log) likelihood that is at least as large as that of the nullmodel.

Value

The test returns a message whether the null hypothesis, i.e. the smaller model is accepted. Invisibly, a list that also contains

  • p, the pp-value

  • n

  • data.ratio the log ratio for the data

  • simu.ratio the log ratio for the simulations

  • data.fit the models fitted to the data

  • msg the message that is also directly returned

It has S3 class "RFratiotest".

Methods

print

prints the summary

summary

gives a summary

Note

An important RFoptions is ratiotest_approx.

Note

Note that the likelihood ratio test may take a huge amount of time.

Note

This function does not depend on the value of RFoptions()$PracticalRange. The function RFratiotest always uses the standard specification of the covariance model as given in RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFfit, RMmodel, RandomFields, weather.

Examples


Simulation of Random Fields

Description

This function simulates unconditional random fields:

It also simulates conditional random fields for

  • univariate and multivariate, spatial and spatio-temporal Gaussian random fields

Here, only the simulation of Gaussian random fields is described. For other kinds of random fields (binary, max-stable, etc.) or more sophisticated approaches see RFsimulateAdvanced.

Usage

RFsimulate(model, x, y=NULL, z=NULL, T=NULL, grid=NULL,
           distances, dim, data, given=NULL, err.model, params,
           err.params, n=1, ...)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

data

For conditional simulation and random imputing only. If data is missing, unconditional simulation is performed.

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest. If given is not given and data is a matrix or data is a data.frame, RandomFields tries to identify where the data and the coordinates are, e.g. by names in formulae or by fixed names, see Coordinate systems. See also RFsimulateAdvanced. If all fails, the first columns are interpreted as coordinate vectors, and the last column(s) as (multiple) measurement(s) of the field. Notes that also lists of data can be passed.

If the argument x is missing, data may contain NAs, which are then replaced by conditionally simulated values (random imputing);

given

optional, matrix or list. If given matrix then the coordinates can be given separately, namely by given where, in each row, a single location is given.
If given is a list, it may consist of x, y, z, T, grid.
If given is provided, data must be a matrix or an array containing the data only.

err.model, err.params

For conditional simulation and random imputing only.
In case of (assumed) error-free measurements (which is mostly the case in geostatistics) the argument err.model is not given. In case of measurement errors we have err.model=RMnugget(var=var).
err.param plays the same role as params for model..

n

number of realizations to generate. For a very advanced feature, see the notes in RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

Details

By default, all Gaussian random fields have zero mean. Simulating with trend can be done by including RMtrend in the model, see the examples below.

If data is passed, conditional simulation based on simple kriging is performed:

  • If of class RFsp, ncol(data@coords) must equal the dimension of the index space. If data@data contains only a single variable, variable names are optional. If data@data contains more than one variable, variables must be named and model must be given in the tilde notation resp ~ ... (see RFformula) and "resp" must be contained in names(data@data).

  • If data is a matrix or a data.frame, either ncol(data) equals (dimensionofindexspace+1)(dimension of index space + 1) and the order of the columns is (x, y, z, T, response) or, if data contains more than one response variable (i.e. ncol(data) > (dimension of index space + 1)), colnames(data) must contain colnames(x) or those of "x", "y", "z", "T" that are not missing. The response variable name is matched with model, which must be given in the tilde notation. If "x", "y", "z", "T" are missing and data contains NAs, colnames(data) must contain an element which starts with ‘data’; the corresponding column and those behind it are interpreted as the given data and those before the corresponding column are interpreted as the coordinates.

  • If x is missing, RFsimulate searches for NAs in the data and performs a conditional simulation for them.

Specification of err.model: In geostatistics we have two different interpretations of a nugget effect: small scale variability and measurement error. The result of conditional simulation usually does not include the measurement error. Hence the measurement error err.model must be given separately. For sake of generality, any model (and not only the nugget effect) is allowed. Consequently, err.model is ignored when unconditional simulation is performed.

Value

By default, an object of the virtual class RFsp; result is of class RMmodel.

  • RFspatialGridDataFrame if the space-time dimension is greater than 1 and the coordinates are on a grid,

  • RFgridDataFrame if the space-time dimension equals 1 and the coordinates are on a grid,

  • RFspatialPointsDataFrame if the space-time dimension is greater than 1 and the coordinates are not on a grid,

  • RFpointsDataFrame if the space-time dimension equals 1 and the coordinates are not on a grid.

In case of a multivariate

If n > 1 the repetitions make the last dimension.

See RFsimulateAdvanced for additional options.

Note

Several advanced options can be found in sections ‘General options’ and ‘coords’ of RFoptions. In particular, option spConform=FALSE leads to a simpler (and faster!) output, see RFoptions for details.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Lantuejoul, Ch. (2002) Geostatistical simulation. New York: Springer.

Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

See RFsimulateAdvanced for more specific literature.

See Also

RFvariogram, RFfit, RFgetModelInfo, RFgui, RMmodel, RFoptions, RFsimulateAdvanced, RFsimulate.more.examples

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

#############################################################
## ##
## ONLY TWO VERY BASIC EXAMPLES ARE GIVEN HERE ##
## see ##
## ?RMsimulate.more.examples ##
## and ##
## ?RFsimulateAdvanced ##
## for more examples ##
## ##
#############################################################

#############################################################
## ##
## Unconditional simulation ## 
## ##
#############################################################

## first let us look at the list of implemented models
RFgetModelNames(type="positive definite", domain="single variable",
                iso="isotropic") 

## our choice is the exponential model;
## the model includes nugget effect and the mean:
model <- RMexp(var=5, scale=10) + # with variance 4 and scale 10
 RMnugget(var=1) + # nugget
 RMtrend(mean=0.5) # and mean
 
## define the locations:
from <- 0
to <- 20
x.seq <- seq(from, to, length=200) 
y.seq <- seq(from, to, length=200)

simu <- RFsimulate(model, x=x.seq, y=y.seq)
plot(simu)



#############################################################
## ##
## Conditional simulation ## 
## ##
#############################################################

# first we simulate some random values at 
# 100 random locations:
n <- 100
x <- runif(n=n, min=-1, max=1)
y <- runif(n=n, min=-1, max=1)
dta <- RFsimulate(model = RMexp(), x=x, y=y, grid=FALSE)
plot(dta)

# let simulate a field conditional on the above data
L <- if (interactive()) 100 else 5
x.seq.cond <- y.seq.cond <- seq(-1.5, 1.5, length=L)
model <- RMexp()
cond <- RFsimulate(model, x=x.seq.cond, y=y.seq.cond, data=dta)
plot(cond, dta)

Further Examples for the Simulation of Random Fields

Description

This man page will give a collection of basic examples for the use of RFsimulate.

For other kinds of random fields (binary, max-stable, etc.) or more sophisticated approaches see RFsimulateAdvanced.

See RFsimulate.sophisticated.examples for further examples.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFsimulate, RFsimulateAdvanced, RFsimulate.sophisticated.examples.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Sophisticated Examples for the Simulation of Random Fields

Description

This man page will give a collection of basic examples for the use of RFsimulate.

For other kinds of random fields (binary, max-stable, etc.) or more sophisticated approaches see RFsimulateAdvanced.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFsimulate, RFsimulateAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Simulation of Random Fields – Advanced

Description

This function simulates unconditional random fields:

It also simulates conditional random fields for

  • univariate and multivariate, spatial and spatio-temporal Gaussian random fields.

For basic simulation of Gaussian random fields, see RFsimulate. See RFsimulate.more.examples and RFsimulate.sophisticated.examples for further examples.

Arguments

model

object of class RMmodel, RFformula or formula; specifies the model to be simulated

  • if of class RMmodel, model specifies

    • the type of random field by using RPfunctions, e.g.,

      • RPgauss: Gaussian random field (default if none of the functions in the list is given)

      • RPsmith: Smith model See RP for an overview.

    • the covariance or variogram model in case of a Gaussian random field (RPgauss) and for fields based on Gaussian fields (e.g. RPbernoulli); type RFgetModelNames(type="variogram") for a list of available models; see also RMmodel.

    • the shape function in case of a shot noise process; type RFgetModelNames(type='shape') for a list of available models.

  • if of class RFformula or formula, submodel specifies a linear mixed model where random effects can be modelled by Gaussian random fields; see RFformula for details on model specification.

x

matrix of coordinates, or vector of x coordinates, or object of class GridTopology or raster; if matrix, ncol(x) is the dimension of the index space; matrix notation is required in case of more than 3 space dimensions; in this case, if grid=FALSE, x_ij is the i-th coordinate in the j-th dimension; otherwise, if grid=TRUE, the columns of x are interpreted as gridtriples (see grid); if of class GridTopology, x is interpreted as grid definition and grid is automatically set to TRUE.

y

optional vector of y coordinates, ignored if x is a matrix

z

optional vector of z coordinates, ignored if x is a matrix

T

optional vector of time coordinates, T must always be an equidistant vector or given in a gridtriple format (see argument grid); for each component of T, the random field is simulated at all location points.

grid

logical; determines whether the vectors x, y, and z or the columns of x should be interpreted as a grid definition (see Details). If grid=TRUE, either x, y, and z must be equidistant vectors in ascending order or the columns of x must be given in the gridtriple format: c(from, stepsize, len).

Note: If grid is not given, RFsimulate tries to guess what is meant.

c(from, stepsize, len) (see Details)

data

matrix, data.frame or object of class RFsp; coordinates and response values of measurements in case that conditional simulation is to be performed; if a matrix or a data.frame, the first columns are interpreted as coordinate vectors, and the last column(s) as (multiple) measurement(s) of the field; if x is missing, data may contain NAs, which are then replaced by conditionally simulated values; if data is missing, unconditional simulation is performed; for details on matching of variable names see Details; if of class RFsp

err.model

same as model; gives the model of the measurement errors for the measured data (which must be given in this case!), see Details. err.model=NULL (default) corresponds to error-free measurements, the most common alternative is err.model=RMnugget(); ignored if data is missing.

distances

object of class dist representing the upper triangular part of the matrix of Euclidean distances between the points at which the field is to be simulated; only applicable for stationary and isotropic models; if not NULL, dim must be given and x, y, z and T must be missing or NULL.

If distances are given, the current value of spConform, see RFoptions, is ignored and instead spConform=FALSE is used. (This fact may change in future.)

dim

integer; space or space-time dimension of the field

n

number of realizations to generate

...

further options and control arguments for the simulation that are passed to and processed by RFoptions

Details

RFsimulate simulates different classes of random fields, controlled by the wrapping model.

If the wrapping function of the model argument is a covariance or variogram model, i.e., one of the list obtained by RFgetModelNames(type="variogram", group.by="type"), by default, a Gaussian field with the corresponding covariance structure is simulated. By default, the simulation method is chosen automatically through internal algorithms. The simulation method can be set explicitly by enclosing the covariance function with a method specification.

If other than Gaussian fields are to be simulated, the model argument must be enclosed by a function specifying the type of the random field.

There are different possibilities of passing the locations at which the field is to be simulated. If grid=FALSE, all coordinate vectors (except for the time component TT) must have the same length and the field is only simulated at the locations given by the rows of xx or of cbind(x, y, z). If TT is not missing, the field is simulated for all combinations (x[i,],T[k])(x[i, ], T[k]) or (x[i],y[i],z[i],T[k])(x[i], y[i], z[i], T[k]), i=1,...,i=1, ...,nrow(x), k=1,...,k=1, ...,length(T), even if model is not explicitly a space-time model.
If grid=TRUE, the vectors x, y, z and T or the columns of x and T are interpreted as a grid definition, i.e. the field is simulated at all locations (xi,yj,zk,Tl)(x_i, y_j, z_k, T_l), as given by expand.grid(x, y, z, T). Here, “grid” means “equidistant in each direction”, i.e. all vectors must be equidistant and in ascending order. In case of more than 3 space dimensions, the coordinates must be given in matrix notation. To enable different grid lengths for each direction in combination with the matrix notation, the “gridtriple” notation c(from, stepsize, len) is used: If x, y, z, T or the columns of x are of length 3, they are internally replaced by seq(from=from, to=from+(len-1)*stepsize, by=stepsize) , i.e. the field is simulated at all locations
expand.grid(seq(x$from, length.out=x$len, by=x$stepsize), seq(y$from, length.out=y$len, by=y$stepsize), seq(z$from, length.out=z$len, by=z$stepsize), seq(T$from, length.out=T$len, by=T$stepsize))

If data is passed, conditional simulation is performed.

  • If of class RFsp, ncol(data@coords) must equal the dimension of the index space. If data@data contains only a single variable, variable names are optional. If data@data contains more than one variable, variables must be named and model must be given in the tilde notation resp ~ ... (see RFformula) and "resp" must be contained in names(data@data).

  • If data is a matrix or a data.frame, either ncol(data) equals (dimensionofindexspace+1)(dimension of index space + 1) and the order of the columns is (x, y, z, T, response) or, if data contains more than one response variable (i.e. ncol(data) > (dimension of index space + 1)), colnames(data) must contain colnames(x) or those of "x", "y", "z", "T" that are not missing. The response variable name is matched with model, which must be given in the tilde notation. If "x", "y", "z", "T" are missing and data contains NAs, colnames(data) must contain an element which starts with ‘data’; the corresponding column and those behind it are interpreted as the given data and those before the corresponding column are interpreted as the coordinates.

  • If x is missing, RFsimulate searches for NAs in the data and performs a conditional simulation for them.

Specification of err.model: In geostatistics we have two different interpretations of a nugget effect: small scale variability and measurement error. The result of conditional simulation usually does not include the measurement error. Hence the measurement error err.model must be given separately. For sake of generality, any model (and not only the nugget effect) is allowed. Consequently, err.model is ignored when unconditional simulation is performed.

Value

By default, an object of the virtual class RFsp; result is of class RFspatialGridDataFrame if [spacetimedimension>1][space-time-dimension > 1] and the coordinates are on a grid, result is of class RFgridDataFrame if [spacetimedimension=1][space-time-dimension = 1] and the coordinates are on a grid, result is of class RFspatialPointsDataFrame if [spacetimedimension>1][space-time-dimension > 1] and the coordinates are not on a grid, result is of class RFpointsDataFrame if [spacetimedimension=1][space-time-dimension = 1] and the coordinates are not on a grid.

The output format can be switched to the "old" array format using RFoptions, either by globally setting RFoptions(spConform=FALSE) or by passing spConform=FALSE in the call of RFsimulate. Then the object returned by RFsimulate depends on the arguments n and grid in the following way:

If vdim > 1 the vdim-variate vector makes the first dimension.

If grid=TRUE an array of the dimension of the random field makes the next dimensions. Here, the dimensions are ordered in the sequence x, y, z, T (if given).

Else if no time component is given, then the values are passed as a single vector. Else if the time component is given the next 2 dimensions give the space and the time, respectively.

If n > 1 the repetitions make the last dimension.

Note: Conversion between the sp format and the conventional format can be done using the method RFspDataFrame2conventional and the function conventional2RFspDataFrame.

InitRFsimulate returns 0 if no error has occurred and a positive value if failed.

Note

Advanced options are

  • spConform (suppressed return of S4 objects)

  • practicalrange (forces range of covariances to be one)

  • exactness (chooses the simulation method by precision)

  • seed (sets .Random.seed locally or globally)

See RFoptions for further options.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

General

  • Lantuejoul, Ch. (2002) Geostatistical simulation. New York: Springer.

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

Original work:

  • Circulant embedding:

    Chan, G. and Wood, A.T.A. (1997) An algorithm for simulating stationary Gaussian random fields. J. R. Stat. Soc., Ser. C 46, 171-181.

    Dietrich, C.R. and Newsam, G.N. (1993) A fast and exact method for multidimensional Gaussian stochastic simulations. Water Resour. Res. 29, 2861-2869.

    Dietrich, C.R. and Newsam, G.N. (1996) A fast and exact method for multidimensional Gaussian stochastic simulations: Extensions to realizations conditioned on direct and indirect measurement Water Resour. Res. 32, 1643-1652.

    Wood, A.T.A. and Chan, G. (1994) Simulation of stationary Gaussian processes in [0,1]d[0,1]^d J. Comput. Graph. Stat. 3, 409-432.

    The code used in RandomFields is based on Dietrich and Newsam (1996).

  • Intrinsic embedding and Cutoff embedding:

    Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599.

    Gneiting, T., Sevcikova, H., Percival, D.B., Schlather, M. and Jiang, Y. (2005) Fast and Exact Simulation of Large Gaussian Lattice Systems in R2R^2: Exploring the Limits J. Comput. Graph. Statist. Submitted.

  • Markov Gaussian Random Field:

    Rue, H. (2001) Fast sampling of Gaussian Markov random fields. J. R. Statist. Soc., Ser. B, 63 (2), 325-338.

    Rue, H., Held, L. (2005) Gaussian Markov Random Fields: Theory and Applications. Monographs on Statistics and Applied Probability, no 104, Chapman \& Hall.

  • Turning bands method (TBM), turning layers:

    Dietrich, C.R. (1995) A simple and efficient space domain implementation of the turning bands method. Water Resour. Res. 31, 147-156.

    Mantoglou, A. and Wilson, J.L. (1982) The turning bands method for simulation of random fields using line generation by a spectral method. Water. Resour. Res. 18, 1379-1394.

    Matheron, G. (1973) The intrinsic random functions and their applications. Adv. Appl. Probab. 5, 439-468.

    Schlather, M. (2004) Turning layers: A space-time extension of turning bands. Submitted

  • Random coins:

    Matheron, G. (1967) Elements pour une Theorie des Milieux Poreux. Paris: Masson.

See Also

RFoptions, RMmodel, RFgui, methods for simulating Gaussian random fields, RFfit, RFvariogram, RFsimulate.more.examples, RFsimulate.sophisticated.examples, RPgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Class RFsp

Description

"RFsp" is a virtual class which contains the four classes RFspatialGridDataFrame (data on a full grid and spacetimedimension2space-time-dimension \ge 2), RFspatialPointsDataFrame (data not on a grid and spacetimedimension2space-time-dimension \ge 2), RFgridDataFrame (data on a full grid and spacetimedimension=1space-time-dimension = 1), RFpointsDataFrame (data not on a grid and spacetimedimension=1space-time-dimension = 1)

The first two subclasses are summarized in "RFspatialDataFrame" whilst the latter two are summarized in "RFdataFrame".

Objects from the Class

are never to be generated; only derived classes can be meaningful.

Methods

summary

signature(obj = "RFsp"): returns a summary of the object; uses or imitates summary method of class Spatial from the sp-package

dimensions

signature(obj = "RFsp"): retrieves the number of spatial or spatio-temporal dimensions spanned

RFspDataFrame2dataArray

signature(obj = "RFsp"): transforms RFsp objects to array

RFspDataFrame2conventional

signature(obj = "RFsp"): transforms RFsp objects to a list with additional information

[

signature(obj = "RFsp"): selects columns of the data-slot, while all other slots are kept unmodified

[<-

signature(obj = "RFsp"): replaces columns of the data-slot, while all other slots are kept unmodified

variance

signature(object = "RFsp"): returns the kriging variance if available

Warning

This class is not useful itself, but the above mentioned classes in this package derived from it.

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFspatialGridDataFrame, RFspatialPointsDataFrame, RFgridDataFrame, RFpointsDataFrame, sp2RF

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Generating an object of class "RFspatialGridDataFrame"
## and one of class "RFspatialPointsDataFrame".

model <- RMcauchy(gamma=4, var=0.1, scale=2)
x <- seq(0,10,len=100)
r <- cbind(runif(100, min=1, max=9),runif(100, min=1, max=9))

z1 <- RFsimulate(model=model, x=x, y=x, n=4)
z2 <- RFsimulate(model=model, x=r, n=2)

## Applying available functions.

class(z1)
class(z2)
summary(z1)
summary(z2)
plot(z1)
plot(z2)

z4 <- RFspDataFrame2conventional(z2)
str(z2)
str(z4)

dta <- data.frame(coords=z4$x,data=z2@data[,1])
z3<-RFinterpolate(model=model, x=x, y=x, data=dta) 
plot(z3,z2)

## Illustrating the warning.

a1 <- new("RFpointsDataFrame")
str(a1)
try(a2 <- new("RFsp")) ## ERROR

Class "RFspatialGridDataFrame"

Description

Class for spatial attributes that have spatial or spatio-temporal locations (at least of dimension 2) on a (full) regular grid. Direct extension of class SpatialGridDataFrame from the sp-package. See sp2RF for an explicit transformation.

Usage

## S4 method for signature 'RFspatialGridDataFrame'
RFspDataFrame2conventional(obj, data.frame=FALSE)

Arguments

obj

an RFspatialGridDataFrame object

data.frame

logical. If TRUE a data.frame is returned.

Creating Objects

Objects can be created by using the functions RFspatialGridDataFrame or conventional2RFspDataFrame or by calls of the form as(x, "RFspatialGridDataFrame"), where x is of class RFspatialGridDataFrame.

Slots

.RFparams:

list of 2; .RFparams$n is the number of repetitions of the random field contained in the data slot; .RFparams$vdim gives the dimension of the values of the random field, equals 1 in most cases

data:

object of class data.frame; containing attribute data

grid:

object of class GridTopology; grid parameters

bbox:

matrix specifying the bounding box

proj4string:

object of class CRS; projection

Extends

Class "SpatialGridDataFrame", directly. Class "SpatialGrid", by class "SpatialGridDataFrame". Class "Spatial", by class "SpatialGrid".

Methods

contour

signature(obj = "RFspatialGridDataFrame"): generates contour plots

plot

signature(obj = "RFspatialGridDataFrame"): generates nice image plots of the random field; if spacetimedim2space-time-dim2, a two-dimensional subspace can be selected using the argument MARGIN; to get different slices in a third direction, the argument MARGIN.slices can be used; for more details see plot-method or type method?plot("RFspatialGridDataFrame")

persp

signature(obj = "RFspatialGridDataFrame"): generates persp plots

show

signature(x = "RFspatialGridDataFrame"): uses the show-method for class SpatialGridDataFrame.

print

signature(x = "RFspatialGridDataFrame"): identical to show-method

RFspDataFrame2conventional

signature(obj = "RFspatialGridDataFrame"): conversion to a list of non-sp-package based objects; the data-slot is converted to an array of dimension [1(vdim>1)+spacetimedimension+1(n>1)][1*(vdim>1) + space-time-dimension + 1*(n>1)]; the grid-slot is converted to a 3-row matrix; the grid definition of a possible time-dimension becomes a separate list element

RFspDataFrame2dataArray

signature(obj = "RFspatialGridDataFrame"): conversion of the data-slot to an array of dimension [spacetimedimension+2][space-time-dimension + 2], where the space-time-dimensions run fastest, and vdimvdim and nn are the last two dimensions

coordinates

signature(x = "RFspatialGridDataFrame"): calculates the coordinates from grid definition

[

signature(x = "RFspatialGridDataFrame"): selects columns of data-slot; returns an object of class RFspatialGridDataFrame.

[<-

signature(x = "RFspatialGridDataFrame"): replaces columns of data-slot; returns an object of class RFspatialGridDataFrame.

as

signature(x = "RFspatialGridDataFrame"): converts into other formats, only implemented for target class RFspatialPointsDataFrame

cbind

signature(...): if arguments have identical topology, combine their attribute values

range

signature(x = "RFspatialGridDataFrame"): returns the range

hist

signature(x = "RFspatialGridDataFrame"): plots histogram

as.matrix

signature(x = "RFspatialGridDataFrame"): converts data-slot to matrix

as.array

signature(x = "RFspatialGridDataFrame"): converts data-slot to array

as.vector

signature(x = "RFspatialGridDataFrame"): converts data-slot to vector

as.data.frame

signature(x = "RFspatialGridDataFrame"): converts data-slot and coordinates to a data.frame

Details

Note that in the data-slot, each column is ordered according to the ordering of coordinates(grid), the first dimension runs fastest and for all BUT the second dimension, coordinate values are in ascending order. In the second dimension, coordinate values run from high to low. Hence, when converting to conventional formats using RFspDataFrame2conventional or RFspDataFrame2dataArray, the data array is re-ordered such that all dimensions are in ascending order. as.matrix does not perform re-ordering.

Methods summary, and dimensions are defined for the “parent”-class RFsp.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFspatialPointsDataFrame-class, which is for point locations that are not on a grid, RFgridDataFrame-class which is for one-dimensional locations, RFsp, sp2RF

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

n <- 3

x <- GridTopology(cellcentre.offset=c(0, 0),
 cellsize=c(1, 0.2),
 cells.dim=c(10, 30))
f <- RFsimulate(model=RMexp(), x=x, n=n)

str(f)
str(RFspDataFrame2conventional(f))
str(RFspDataFrame2dataArray(f))
head(coordinates(f))
str(f[2]) ## selects second column of data-slot
all.equal(f, cbind(f,f)[1:3]) ## TRUE
str(as(f, "RFspatialPointsDataFrame"))

plot(f, nmax=2)

steps <- c(10, 1, 10, 10)

x2 <- rbind(c(0, 0, 0, 0),
 c(1, 0.2, 2, 5),
 steps)
scale <- 10

f2 <- RFsimulate(model=RMwhittle(nu=1.2, scale=scale), x=x2, n=n,
                 grid = TRUE)
plot(f2, MARGIN=c(3,4), MARGIN.slices=1, n.slices=6, nmax=2)

f.sp <- RFsimulate(model=RMexp(), x=x, n=n)
f.old <- RFsimulate(model=RMexp(), x=x, n=n, spConform=FALSE)
all.equal(RFspDataFrame2conventional(f.sp)$data, f.old, check.attributes=FALSE) ## TRUE

Class "RFspatialPointsDataFrame"

Description

Class for spatial attributes that have spatial or spatio-temporal locations (at least of dimension 2) that are not on a grid. Direct extension of class SpatialPointsDataFrame from the sp-package. See sp2RF for an explicit transformation.

Usage

## S4 method for signature 'RFspatialPointsDataFrame'
RFspDataFrame2conventional(obj)

Arguments

obj

an RFspatialPointsDataFrame object

Creating Objects

Objects can be created by using the functions RFspatialPointsDataFrame or conventional2RFspDataFrame or by calls of the form as(x, "RFspatialPointsDataFrame"), where x is of class RFspatialPointsDataFrame.

Slots

.RFparams:

list of 2; .RFparams$n is the number of repetitions of the random field contained in the data slot, .RFparams$vdim gives the dimension of the values of the random field, equals 1 in most cases

data:

object of class data.frame, containing attribute data

coords.nrs:

See SpatialPointsDataFrame.

coords:

matrix of coordinates (each row is a point); in case of SpatialPointsDataFrame an object of class SpatialPoints is also allowed, see SpatialPoints.

bbox:

matrix specifying the bounding box

proj4string:

object of class CRS; projection

Extends

Class SpatialPointsDataFrame, directly. Class SpatialPoints, by class SpatialPointsDataFrame. Class Spatial, by class SpatialPoints.

Methods

plot

signature(obj = "RFspatialPointsDataFrame"): generates nice plots of the random field; if spacetimedim2space-time-dim2, a two-dimensional subspace can be selected using the argument MARGIN; to get different slices in a third direction, the argument MARGIN.slices can be used; for more details see plot-method or type method?plot("RFspatialPointsDataFrame")

show

signature(x = "RFspatialPointsDataFrame"): uses the show-method for class SpatialPointsDataFrame

print

signature(x = "RFspatialPointsDataFrame"): identical to show-method

RFspDataFrame2conventional

signature(obj = "RFspatialPointsDataFrame"): conversion to a list of non-sp-package based objects; the data-slot is converted to an array of dimension [1(vdim>1)+spacetimedimension+1(n>1)][1*(vdim>1) + space-time-dimension + 1*(n>1)]

coordinates

signature(x = "RFspatialPointsDataFrame"): returns the coordinates

[

signature(x = "RFspatialPointsDataFrame"): selects columns of data-slot; returns an object of class RFspatialPointsDataFrame

[<-

signature(x = "RFspatialPointsDataFrame"): replaces columns of data-slot; returns an object of class RFspatialPointsDataFrame

as

signature(x = "RFspatialPointsDataFrame"): converts into other formats, only implemented for target class RFspatialGridDataFrame

cbind

signature(...): if arguments have identical topology, combine their attribute values

range

signature(x = "RFspatialPointsDataFrame"): returns the range

hist

signature(x = "RFspatialPointsDataFrame"): plots histogram

as.matrix

signature(x = "RFspatialPointsDataFrame"): converts data-slot to matrix

as.array

signature(x = "RFspatialPointsDataFrame"): converts data-slot to array

as.vector

signature(x = "RFspatialPointsDataFrame"): converts data-slot to vector

as.data.frame

signature(x = "RFspatialPointsDataFrame"): converts data-slot and coordinates to a data.frame

Details

Note that in the data-slot, each column is ordered according to the ordering of coordinates(grid), the first dimension runs fastest and for all BUT the second dimension, coordinate values are in ascending order. In the second dimension, coordinate values run from high to low. Hence, when converting to conventional formats using RFspDataFrame2conventional or RFspDataFrame2dataArray, the data array is re-ordered such that all dimensions are in ascending order. as.matrix does not perform re-ordering.

Methods summary and dimensions are defined for the “parent”-class RFsp.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFspatialGridDataFrame-class, which is for point locations that are on a grid, RFpointsDataFrame-class which is for one-dimensional locations, RFsp, sp2RF

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- cbind(runif(50), runif(50))
f <- RFsimulate(model=RMexp(), x=x, n=3)

str(f)
str(RFspDataFrame2conventional(f))
head(coordinates(f))
str(f[2]) ## selects second column of data-slot
all.equal(f, cbind(f,f)[1:3]) ## TRUE
try(as(f, "RFspatialGridDataFrame")) # yields error

plot(f, nmax=2)

f2 <- RFsimulate(model=RMwhittle(nu=1.2, scale=10), x=cbind(x,x), n=4)
plot(f2, MARGIN=c(3,4), nmax=2)

f.sp <- RFsimulate(model=RMexp(), x=x, n=3)
f.old <- RFsimulate(model=RMexp(), x=x, n=3, spConform=FALSE)
all.equal(RFspDataFrame2conventional(f.sp)$data, f.old, check.attributes=FALSE) ## TRUE

Empirical (Cross-)Variogram

Description

Calculates empirical (cross-)variogram.

Usage

RFvariogram(model, x, y=NULL, z = NULL, T=NULL, grid,
            params, distances, dim, ...,
	    data, bin=NULL, phi=NULL, theta = NULL,
	    deltaT = NULL, vdim=NULL)

Arguments

model, params

object of class RMmodel, RFformula or formula; best is to consider the examples below, first.
The argument params is a list that specifies free parameters in a formula description, see RMformula.

x

vector of x coordinates, or object of class GridTopology or raster; for more options see RFsimulateAdvanced.

y, z

optional vectors of y (z) coordinates, which should not be given if x is a matrix.

T

optional vector of time coordinates, T must always be an equidistant vector. Instead of T=seq(from=From, by=By, len=Len), one may also write T=c(From, By, Len).

grid

logical; the function finds itself the correct value in nearly all cases, so that usually grid need not be given. See also RFsimulateAdvanced.

distances, dim

another alternative for the argument x to pass the (relative) coordinates, see RFsimulateAdvanced.

...

for advanced use: further options and control arguments for the simulation that are passed to and processed by RFoptions. If params is given, then ... may include also the variables used in params.

data

matrix, data.frame or object of class RFsp;
If a matrix is given the ordering of the colums is the following: space, time, multivariate, repetitions, i.e. the index for the space runs the fastest and that for repetitions the slowest.

bin

a vector giving the borders of the bins; If not specified an array describing the empirical (pseudo-)(cross-) covariance function in every direction is returned.

phi

an integer defining the number of sectors one half of the X/Y plane shall be divided into. If not specified, either an array is returned (if bin missing) or isotropy is assumed (if bin specified).

theta

an integer defining the number of sectors one half of the X/Z plane shall be divided into. Use only for dimension d=3d=3 if phi is already specified.

deltaT

vector of length 2, specifying the temporal bins. The internal bin vector becomes seq(from=0, to=deltaT[1], by=deltaT[2])

vdim

the number of variables of a multivariate data set. If not given and data is an RFsp object created by RandomFields, the information there is taken from there. Otherwise vdim is assumed to be one. NOTE: still the argument vdim is an experimental stage.

Details

RFvariogram computes the empirical cross-variogram for given (multivariate) spatial data.

The empirical (cross-)variogram of two random fields XX and YY is given by

γ(r):=12N(r)(ti,tj)ti,j=r(X(ti)X(tj))(Y(ti)Y(tj))\gamma(r):=\frac{1}{2N(r)} \sum_{(t_{i},t_{j})|t_{i,j}=r} (X(t_{i})-X(t_{j}))(Y(t_{i})-Y(t_{j}))

where ti,j:=titjt_{i,j}:=t_{i}-t_{j}, and where N(r)N(r) denotes the number of pairs of data points with distancevector ti,j=rt_{i,j}=r.

The spatial coordinates x, y, z should be vectors. For random fields of spatial dimension d>3d > 3 write all vectors as columns of matrix x. In this case do neither use y, nor z and write the columns in gridtriple notation.

If the data is spatially located on a grid a fast algorithm based on the fast Fourier transformed (fft) will be used. As advanced option the calculation method can also be changed for grid data (see RFoptions.)

Value

RFvariogram returns objects of class RFempVariog.

Author(s)

Sebastian Engelke; Johannes Martini; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RMstable, RMmodel, RFsimulate, RFfit, RFcov, RFpseudovariogram. RFmadogram.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

n <- 1 ## use n <- 2 for better results

## isotropic model
model <- RMexp()
x <- seq(0, 10, 0.02)
z <- RFsimulate(model, x=x, n=n)
emp.vario <- RFvariogram(data=z)
plot(emp.vario, model=model)


## anisotropic model
model <- RMexp(Aniso=cbind(c(2,1), c(1,1)))
x <- seq(0, 10, 0.05)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFvariogram(data=z, phi=4)
plot(emp.vario, model=model)


## space-time model
model <- RMnsst(phi=RMexp(), psi=RMfbm(alpha=1), delta=2)
x <- seq(0, 10, 0.05)
T <- c(0, 0.1, 100)
z <- RFsimulate(x=x, T=T, model=model, n=n)
emp.vario <- RFvariogram(data=z, deltaT=c(10, 1))
plot(emp.vario, model=model, nmax.T=3)


## multivariate model
model <- RMbiwm(nudiag=c(1, 2), nured=1, rhored=1, cdiag=c(1, 5), 
                s=c(1, 1, 2))
x <- seq(0, 20, 0.1)
z <- RFsimulate(model, x=x, y=x, n=n)
emp.vario <- RFvariogram(data=z)
plot(emp.vario, model=model)


## multivariate and anisotropic model
model <- RMbiwm(A=matrix(c(1,1,1,2), nc=2),
                nudiag=c(0.5,2), s=c(3, 1, 2), c=c(1, 0, 1))
x <- seq(0, 20, 0.1)
dta <- RFsimulate(model, x, x, n=n)
ev <- RFvariogram(data=dta, phi=4)
plot(ev, model=model, boundaries=FALSE)

Anisotropy matrix given by angle

Description

RMangle delivers an anisotropy matrix for the argument Aniso in RMmodel in two dimensions. RMangle requires one or two stretching values, passed by ratio or diag, and an angle.

In two dimensions and with angle equal to aa and diag equal to (d1,d2)(d1, d2) the anisotropy matrix AA is

A = diag(d1, d2) %*% matrix(ncol=2, c(cos(a), sin(a), -sin(a), cos(a)))

In three dimensions and with angle equal to aa, second angle LL and diag equal to (d1,d2,d3)(d1, d2, d3) the anisotropy matrix AA is

A = diag(d1, d2, d3) %*% matrix(ncol=3, c(cos(a) * cos(L), sin(a) * cos(L), sin(L), -sin(a), cos(a), 0, -cos(a) * sin(L), -sin(a) * sin(L), cos(L) )) i.e. AxAx turns a vector x first in the xzx-z plane, then in the xyx-y plane.

Usage

RMangle(angle, lat.angle, ratio, diag)

Arguments

angle

angle a

lat.angle

second angle; in 3 dimensions only

ratio

equivalent to diag=c(1, 1/ratio); in 2 dimensions only

diag

the diagonal components of the matrix

Value

RMangle returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMtrafo, RMmodel

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp(Aniso=RMangle(angle=pi/4, ratio=3))
plot(model, dim=2)

x <- seq(0, 2, 0.05)
z <- RFsimulate(x, x, model=model)
plot(z)


model <- RMexp(Aniso=RMangle(angle=pi/4, lat.angle=pi/8, diag=c(1,2,3)))
x <- seq(0, 2, 0.2)
z <- RFsimulate(x, x, x, model=model)
plot(z, MARGIN.slices=3)


## next model gives an example how to estimate the parameters back
n <- 20
x <- runif(n, 0, 10)
y <- runif(n, 0, 10)
coords <- expand.grid(x, y)
model <- RMexp(Aniso=RMangle(angle=pi/4, diag=c(1/4, 1/12)))
d <- RFsimulate(model, x=coords[, 1], y=coords[, 2], n=10)
estmodel <- RMexp(Aniso=RMangle(angle=NA, diag=c(NA, NA)))
system.time(RFfit(estmodel, data=d, modus_operandi='sloppy'))

Askey model

Description

Askey's model

C(x)=(1x)α1[0,1](x)C(x)= (1-x)^\alpha 1_{[0,1]}(x)

Usage

RMaskey(alpha, var, scale, Aniso, proj)
RMtent(var, scale, Aniso, proj)

Arguments

alpha

a numerical value in the interval [0,1]

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This covariance function is valid for dimension dd if α(d+1)/2\alpha \ge (d+1)/2. For α=1\alpha=1 we get the well-known triangle (or tent) model, which is only valid on the real line.

Value

RMaskey returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Covariance function

  • Askey, R. (1973) Radial characteristic functions. Technical report, Research Center, University of Wisconsin-Madison.

  • Golubov, B. I. (1981) On Abel-Poisson type and Riesz means, Anal. Math. 7, 161-184.

Applications as covariance function

  • Gneiting, T. (1999) Correlation functions for atmospheric data analysis. Quart. J. Roy. Meteor. Soc., 125:2449-2464.

  • Gneiting, T. (2002) Compactly supported correlation functions. J. Multivar. Anal., 83:493-508.

  • Wendland, H. (1994) Ein Beitrag zur Interpolation mit radialen Basisfunktionen. Diplomarbeit, Goettingen.

  • Wendland, H. Piecewise polynomial, positive definite and compactly supported radial functions of minimal degree. Adv. Comput. Math., 4:389-396, 1995.

Tail correlation function (for α[d/2]+1\alpha \ge [d / 2] + 1)

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMmodel, RMbigneiting, RMgengneiting, RMgneiting, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMtent()
x <- seq(0, 10, 0.02) 
plot(model)
plot(RFsimulate(model, x=x))

Space-time moving average model

Description

RMave is a univariate stationary covariance model which depends on a normal scale mixture covariance model phiphi.

The corresponding covariance function only depends on the difference (h,u)Rd(h,u) \in {\bf R}^{d} between two points in the dd-dimensional space and is given by

C(h,u)=E+2AhhtA1/2ϕ((h2/2+(zth+u)2(12htA(E+2AhhtA)1Ah)))C(h, u) = |E + 2Ahh^tA|^{-1/2} \phi(\sqrt(\|h\|^2/ 2 + (z^th + u)^2 (1 - 2h^tA (E+2Ahh^tA)^{-1} Ah)))

where EE is the identity matrix. The spatial dimension is d1d-1 and hh is real-valued.

Usage

RMave(phi, A, z, spacetime, var, scale, Aniso, proj)

Arguments

phi

a covariance model which is a normal mixture, that means an RMmodel whose monotone property equals 'normal mixture', see RFgetModelNames(monotone="normal mixture")

A

a symmetric d1×d1d-1 \times d-1-matrix if the corresponding random field is in the dd-dimensional space

z

a d1d-1 dimensional vector if the corresponding random field is on dd-dimensional space

spacetime

logical. If FALSE then the model is interpreted as if h=0h=0, i.e. the spatial dimension is dd. Default is TRUE.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

See Schlather, M. (2010), Example 13 with l=1.

Value

RMave returns an object of class RMmodel

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2010) Some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RFfit, RFsimulate, RMmodel, RMstp.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Example of an evaluation of the ave2-covariance function
## in three different ways
## ---------------------------------------------------------
## some parameters A and z
A <- matrix(c(2,1,1,2),ncol=2)
z <- c(1,2)
## h for evalutation
h <- c(1,2)
## some abbreviations
E <- matrix(c(1,0,0,1),ncol=2)
B <- A %*% h %*% t(h) %*% A
phi <- function(t){return(RFcov(RMwhittle(1), t))}
## ---------------------------------------------------------
## the following should yield the same value 3 times
## (also for other choices of A,z and h)
z1 <- RFcov( model=RMave(RMwhittle(1),A=A,z=z) , x=t(c(h,0)) )
z2 <- RFcov( model=RMave(RMwhittle(1),A=A,z=z,spacetime=FALSE) , x=t(h) )
z3 <- ( (det(E+2*B))^(-1/2) ) *
 phi( sqrt( sum(h*h)/2 + (t(z) %*% h)^2 *
 ( 1-2*t(h) %*% A %*% solve(E+2*B) %*% A %*% h) ) )
##

## Not run:  stopifnot(abs(z1-z2)<1e-12, abs(z2-z3)<1e-12)

RMball

Description

RMball refers to the indicator function of a ball with radius 1.

Usage

RMball(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMpolygon, RMspheric, RFsimulate, RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,10,len=100)
model <- RMball(var=2,scale=1.5)
plot(model)
z <- RFsimulate(RPpoisson(model),x=x,y=x,intensity=0.1)
plot(z)

Model bridging stationary and intrinsically stationary processes

Description

RMbcw is a variogram model that bridges between some intrinsically stationary isotropic processes and some stationary ones. It reunifies the RMgenfbm ‘b’, RMgencauchy ‘c’ and RMdewijsian ‘w’.

The corresponding centered semi-variogram only depends on the distance r0r \ge 0 between two points and is given by

γ(r)=(rα+1)β/α12β/α1\gamma(r) = \frac{(r^{\alpha}+1)^{\beta/\alpha}-1}{2^{\beta/\alpha} -1}

where α(0,2]\alpha \in (0,2] and β2\beta \le 2.

Usage

RMbcw(alpha, beta, c, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; should be in the interval (0,2].

beta

a numerical value; should be in the interval (-infty,2].

c

only for experts. If given, a not necessarily positive definite function cγ(r)c-\gamma(r) is built.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above variogram remains unmodified.

Details

For β>0\beta >0, β<0\beta<0, β=0\beta=0 we have the generalized fractal Brownian motion RMgenfbm, the generalized Cauchy model RMgencauchy, and the de Wisjian model RMdewijsian, respectively.

Hence its two arguments alpha and beta allow for modelling the smoothness and a wide range of tail behaviour, respectively.

Value

RMbcw returns an object of class RMmodel

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M (2014) A parametric variogram model bridging between stationary and intrinsically stationary processes. arxiv 1412.1914.

See Also

RMlsfbm is equipped with Matheron's constant cc for the fractional brownian motion, RMgenfbm, RMgencauchy, RMdewijsian, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMbcw(alpha=1, beta=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Covariance Model for binary field based on a Gaussian field

Description

RMbernoulli gives the centered correlation function of a binary field, obtained by thresholding a Gaussian field.

Usage

RMbernoulli(phi, threshold, correlation, centred, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel.

threshold

real valued threshold, see RPbernoulli. Currently, only threshold=0.0 is possible.

Default: 0.

correlation

logical. If FALSE the corresponding covariance function is returned.

Default: TRUE.

centred

logical. If FALSE the uncentred covariance is returned.

Default: TRUE.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model yields the covariance function of the field that is returned by RPbernoulli.

Value

RMbernoulli returns an object of class RMmodel.

Note

Previous to version 3.0.33 the covariance function was returned, not the correlation function.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Ballani, Schlather

See Also

RPbernoulli, RMmodel, RFsimulate.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

threshold <- 0
x <- seq(0, 5, 0.02)
GaussModel <- RMgneiting()

n <- 1000
z <- RFsimulate(RPbernoulli(GaussModel, threshold=threshold), x=x, n=n)
plot(z)

model <- RMbernoulli(RMgauss(), threshold=threshold, correlation=FALSE)
plot(model, xlim=c(0,5))
z1 <- as.matrix(z)
estim.cov <- apply(z1, 1, function(x) cov(x, z1[1,]))
points(coordinates(z), estim.cov, col="red")

Bessel Family Covariance Model

Description

RMbessel is a stationary isotropic covariance model belonging to the Bessel family. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=2νΓ(ν+1)rνJν(r)C(r) = 2^\nu \Gamma(\nu+1) r^{-\nu} J_\nu(r)

where νd22\nu \ge \frac{d-2}2, Γ\Gamma denotes the gamma function and JνJ_\nu is a Bessel function of first kind.

Usage

RMbessel(nu, var, scale, Aniso, proj)

Arguments

nu

a numerical value; should be equal to or greater than d22\frac{d-2}2 to provide a valid covariance function for a random field of dimension dd.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This covariance models a hole effect (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 92, cf. Gelfand et al. (2010), p. 26).

An important case is ν=0.5\nu=-0.5 which gives the covariance function

C(r)=cos(r)C(r)=\cos(r)

and which is only valid for d=1d=1. This equals RMdampedcos for λ=0\lambda = 0, there.

A second important case is ν=0.5\nu=0.5 with covariance function

C(r)=sin(r)/rC(r)=\sin(r)/r

which is valid for d3d \le 3. This coincides with RMwave.

Note that all valid continuous stationary isotropic covariance functions for dd-dimensional random fields can be written as scale mixtures of a Bessel type covariance function with ν=d22\nu=\frac{d-2}2 (cf. Gelfand et al., 2010, pp. 21–22).

Value

RMbessel returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

See Also

RMdampedcos, RMwave, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMbessel(nu=1, scale=0.1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Bivariate Cauchy Model

Description

RMbicauchy is a bivariate stationary isotropic covariance model whose corresponding covariance function only depends on the distance r0r \ge 0 between two points.

For constraints on the constants see Details.

Usage

RMbicauchy(alpha, beta, s, rho, var, scale, Aniso, proj)

Arguments

alpha

[to be done]

beta

[to be done]

s

a vector of length 3 of numerical values; each entry positive; the vector (s11,s21,s22)(s_{11},s_{21},s_{22})

rho

[to be done]

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Constraints on the constants: [to be done]

Value

RMbicauchy returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Moreva, O., Schlather, M. (2016) Modelling and simulation of bivariate Gaussian random fields. arXiv 1412.1914

See Also

RMcauchy, Multivariate RMmodels.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## todo

Gneiting-Wendland Covariance Models

Description

RMbigneiting is a bivariate stationary isotropic covariance model family whose elements are specified by seven parameters.

Let

δij=μ+γij+1.\delta_{ij} = \mu + \gamma_{ij} + 1.

Then,

Cn(h)=cij(Cn,δ(h/sij))i,j=1,2C_{n}(h) = c_{ij} (C_{n, \delta} (h / s_{ij}))_{i,j=1,2}

and Cn,δC_{n, \delta} is the generalized Gneiting model with parameters nn and δ\delta, see RMgengneiting, i.e.,

Cκ=0,δ(r)=(1r)β1[0,1](r),β=δ+2κ+1/2;C_{\kappa=0, \delta}(r) = (1-r)^\beta 1_{[0,1]}(r), \qquad \beta=\delta + 2\kappa + 1/2;

Cκ=1,δ(r)=(1+βr)(1r)β1[0,1](r),β=δ+2κ+1/2;C_{\kappa=1, \delta}(r) = \left(1+\beta r \right)(1-r)^{\beta} 1_{[0,1]}(r), \qquad \beta = \delta + 2\kappa + 1/2;

Cκ=2,δ(r)=(1+βr+β213r2)(1r)β1[0,1](r),β=δ+2κ+1/2;C_{\kappa=2, \delta}(r)=\left( 1 + \beta r + \frac{\beta^{2} - 1}{3}r^{2} \right)(1-r)^{\beta} 1_{[0,1]}(r), \qquad \beta=\delta + 2\kappa + 1/2;

Cκ=3,δ(r)=(1+βr+(2β23)5r2+(β24)β15r3)(1r)β1[0,1](r),β=δ+2κ+1/2.C_{\kappa=3, \delta}(r)=\left( 1 + \beta r + \frac{(2\beta^{2}-3)}{5} r^{2}+ \frac{(\beta^2 - 4)\beta}{15} r^{3} \right)(1-r)^\beta 1_{[0,1]}(r), \qquad \beta=\delta+2\kappa+1/2.

Usage

RMbigneiting(kappa, mu, s, sred12, gamma, cdiag, rhored, c, var, scale, Aniso, proj)

Arguments

kappa

argument that chooses between the four different covariance models and may take values 0,,30,\ldots,3. The model is kk times differentiable.

mu

mu has to be greater than or equal to d2\frac{d}{2} where dd is the (arbitrary) dimension of the random field.

s

vector of two elements giving the scale of the models on the diagonal, i.e. the vector (s11,s22)(s_{11}, s_{22}).

sred12

value in [1,1][-1,1]. The scale on the offdiagonals is given by s12=s21=s_{12} = s_{21} = sred12 * min{s11,s22}\min\{s_{11},s_{22}\}.

gamma

a vector of length 3 of numerical values; each entry is positive. The vector gamma equals (γ11,γ21,γ22)(\gamma_{11},\gamma_{21},\gamma_{22}). Note that γ12=γ21\gamma_{12} =\gamma_{21}.

cdiag

a vector of length 2 of numerical values; each entry positive; the vector (c11,c22)(c_{11},c_{22}).

c

a vector of length 3 of numerical values; the vector (c11,c21,c22)(c_{11}, c_{21}, c_{22}). Note that c12=c21c_{12}= c_{21}.

Either rhored and cdiag or c must be given.

rhored

value in [1,1][-1,1]. See also the Details for the corresponding value of c12=c21c_{12}=c_{21}.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

A sufficient condition for the constant cijc_{ij} is

c12=ρredm(c11c22i,j=1,2(Γ(γij+μ+2κ+5/2)bijνij+2κ+1Γ(1+γij)Γ(μ+2κ+3/2))(1)i+j)1/2c_{12} = \rho_{\rm red} \cdot m \cdot \left(c_{11} c_{22} \prod_{i,j=1,2} \left(\frac{\Gamma(\gamma_{ij} + \mu + 2\kappa + 5/2)}{b_{ij}^{\nu_{ij} + 2\kappa + 1} \Gamma(1 + \gamma_{ij}) \Gamma(\mu + 2\kappa + 3/2)} \right)^{(-1)^{i+j}} \right)^{1/2}

where ρred[1,1]\rho_{\rm red} \in [-1,1].

The constant mm in the formula above is obtained as follows:

m=min{1,m1,m+1}m = \min\{1, m_{-1}, m_{+1}\}

Let

a=2γ12γ11γ22a = 2 \gamma_{12} - \gamma_{11} -\gamma_{22}

b=2γ12(s11+s22)+γ11(s12+s22)+γ22(s12+s11)b = -2 \gamma_{12} (s_{11} + s_{22}) + \gamma_{11} (s_{12} + s_{22}) + \gamma_{22} (s_{12} + s_{11})

e=2γ12s11s22γ11s12s22γ22s12s11e = 2 \gamma_{12} s_{11}s_{22} - \gamma_{11}s_{12}s_{22} - \gamma_{22}s_{12}s_{11}

d=b24aed = b^2 - 4ae

tj=b+jd2at_j =\frac{- b + j \sqrt d}{2 a}

If d0d \ge0 and tj∉(0,s12)t_j \not\in (0, s_{12}) then mj=m_j=\infty else

mj=(1tj/s11)γ11(1tj/s22)γ22(1tj/s12)2γ11mj=(1tj/s11)γ11(1tj/s22)γ22/(1tj/s12)2γ11m_j = \frac{(1 - t_j/s_{11})^{\gamma_{11}}(1 - t_j/s_{22})^{\gamma_{22}}}{(1 - t_j/s_{12})^{2 \gamma_{11}} }{ m_j = (1 - t_j/s_{11})^{\gamma_{11}} (1 - t_j/s_{22})^{\gamma_{22}} / (1 - t_j/s_{12})^{2 \gamma_{11}} }

In the function RMbigneiting, either c is passed, then the above condition is checked, or rhored is passed; then c12c_{12} is calculated by the above formula.

Value

RMbigneiting returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Bevilacqua, M., Daley, D.J., Porcu, E., Schlather, M. (2012) Classes of compactly supported correlation functions for multivariate random fields. Technical report.

    RMbigeneiting is based on this original work. D.J. Daley, E. Porcu and M. Bevilacqua have published end of 2014 an article intentionally without clarifying the genuine authorship of RMbigneiting, in particular, neither referring to this original work nor to RandomFields, which has included RMbigneiting since version 3.0.5 (05 Dec 2013).

  • Gneiting, T. (1999) Correlation functions for atmospherical data analysis. Q. J. Roy. Meteor. Soc Part A 125, 2449-2464.

  • Wendland, H. (2005) Scattered Data Approximation. Cambridge Monogr. Appl. Comput. Math.

See Also

RMaskey, RMbiwm, RMgengneiting, RMgneiting, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMbigneiting(kappa=2, mu=0.5, gamma=c(0, 3, 6), rhored=1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Bivariate stable Model

Description

RMbistable is a bivariate stationary isotropic covariance model whose corresponding covariance function only depends on the distance r0r \ge 0 between two points.

For constraints on the constants see Details.

Usage

RMbistable(alpha, s, cdiag, rho, rhored, betared, alphadiag, var, scale, Aniso, proj)

Arguments

alpha, alphadiag

[to be done]

s

a vector of length 3 of numerical values; each entry positive; the vector (s11,s21,s22)(s_{11},s_{21},s_{22})

cdiag

[to be done]

rho, rhored

[to be done]

betared

to do

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Constraints on the constants: [to be done]

Value

RMbistable returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Moreva, O., Schlather, M. (2016) Modelling and simulation of bivariate Gaussian random fields. arXiv 1412.1914

See Also

RMstable, Multivariate RMmodels.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## todo

Full Bivariate Whittle Matern Model

Description

RMbiwm is a bivariate stationary isotropic covariance model whose corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given for i,j{1,2}i,j \in \{1,2\} by

Cij(r)=cijWνij(r/sij).C_{ij}(r)=c_{ij} W_{\nu_{ij}}(r/s_{ij}).

Here WνW_\nu is the covariance of the RMwhittle model. For constraints on the constants see Details.

Usage

RMbiwm(nudiag, nured12, nu, s, cdiag, rhored, c, notinvnu, var,
 scale, Aniso, proj)

Arguments

nudiag

a vector of length 2 of numerical values; each entry positive; the vector (ν11,ν22)(\nu_{11},\nu_{22})

nured12

a numerical value in the interval [1,)[1,\infty); ν21\nu_{21} is calculated as 0.5(ν11+ν22)νred0.5 (\nu_{11} + \nu_{22})*\nu_{red}.

nu

alternative to nudiag and nured12: a vector of length 3 of numerical values; each entry positive; the vector (ν11,ν21,ν22)(\nu_{11},\nu_{21},\nu_{22}). Either nured and nudiag, or nu must be given.

s

a vector of length 3 of numerical values; each entry positive; the vector (s11,s21,s22)(s_{11},s_{21},s_{22}).

cdiag

a vector of length 2 of numerical values; each entry positive; the vector (c11,c22)(c_{11},c_{22}).

rhored

a numerical value; in the interval [1,1][-1,1]. See also the Details for the corresponding value of c12=c21c_{12}=c_{21}.

c

a vector of length 3 of numerical values; the vector (c11,c21,c22)(c_{11},c_{21}, c_{22}). Either rhored and cdiag or c must be given.

notinvnu

logical or NULL. If not given (default) then the formula of the (RMwhittle) model applies. If logical then the formula for the RMmatern model applies. See there for details.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Constraints on the constants: For the diagonal elements we have

νii,sii,cii>0.\nu_{ii}, s_{ii}, c_{ii} > 0.

For the offdiagonal elements we have

s12=s21>0,s_{12}=s_{21} > 0,

ν12=ν21=0.5(ν11+ν22)νred\nu_{12} =\nu_{21} = 0.5 (\nu_{11} + \nu_{22}) * \nu_{red}

for some constant νred[1,)\nu_{red} \in [1,\infty) and

c12=c21=ρredfmc11c22c_{12} =c_{21} = \rho_{red} \sqrt{f m c_{11} c_{22}}

for some constant ρred\rho_{red} in [1,1][-1,1].

The constants ff and mm in the last equation are given as follows:

f=(Γ(ν11+d/2)Γ(ν22+d/2))/(Γ(ν11)Γ(ν22))(Γ(ν12)/Γ(ν12+d/2))2(s122ν12/(s11ν11s22ν22))2f = (\Gamma(\nu_{11} + d/2) \Gamma(\nu_{22} + d/2)) / (\Gamma(\nu_{11}) \Gamma(\nu_{22})) * (\Gamma(\nu_{12}) / \Gamma(\nu_{12}+d/2))^2 * ( s_{12}^{2*\nu_{12}} / (s_{11}^{\nu_{11}} s_{22}^{\nu_{22}}) )^2

where Γ\Gamma is the Gamma function and dd is the dimension of the space. The constant mm is the infimum of the function gg on [0,)[0,\infty) where

g(t)=(1/s122+t2)2ν12+d(1/s112+t2)ν11d/2(1/s222+t2)ν22d/2g(t) = (1/s_{12}^2 +t^2)^{2\nu_{12} + d} (1/s_{11}^2 + t^2)^{-\nu_{11}-d/2} (1/s_{22}^2 + t^2)^{-\nu_{22}-d/2}

(cf. Gneiting, T., Kleiber, W., Schlather, M. (2010), Full Bivariate Matern Model (Section 2.2)).

Value

RMbiwm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Kleiber, W., Schlather, M. (2010) Matern covariance functions for multivariate random fields JASA

See Also

RMparswm, RMwhittle, RMmodel, RFsimulate, RFfit, Multivariate RMmodels.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- y <- seq(-10, 10, 0.2)
model <- RMbiwm(nudiag=c(0.3, 2), nured=1, rhored=1, cdiag=c(1, 1.5), 
                s=c(1, 1, 2))
plot(model)
plot(RFsimulate(model, x, y))

Scale model for a few areas of different scales and/or differentiabilities

Description

Let Z=(Z1,Zk)Z=(Z_1, \ldots Z_k) be an kk-variate random field and A1,,AkA_1,\ldots, A_k a partition of the space. Then

Y(x)=i=1kZi1(xAi)Y(x) = \sum_{i=1}^k Z_i * 1(x \in A_i)

i.e. the model blends the components of ZZ to a new, univariate model YY.

Usage

RMblend(multi, blend, thresholds, var, scale, Aniso, proj)

Arguments

multi

a multivariate covariance function

blend, thresholds

The threshold is a vector of increasing values. If the value of blend is below all thresholds up to the kk-th threshold, then the kk-th component of the field given by multi is taken. If necessary the components are recycled.

Default: threshold = 0.5, useful for blending a bivariate field if blend takes only the values 00 and 1.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMblend returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Bonat, W.H. , Ribeiro, P. Jr. and Schlather, M. (2019) Modelling non-stationarity in scale. In preparation.

  • Genton, Apanovich Biometrika.

See Also

RMSadvanced, RMbubble, RMscale,

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,1, if (interactive()) 0.01 else 0.5)
len <- length(x)
m <- matrix(1:len, nc=len, nr=len)
m <- m > t(m)
image(m) # two areas separated by the first bisector

biwm <- RMbiwm(nudiag=c(0.3, 1), nured=1, rhored=1, cdiag=c(1, 1), 
                s=c(1, 1, 0.5))
model <- RMblend(multi=biwm, blend=RMcovariate(data = as.double(m), raw=TRUE))
plot(z <- RFsimulate(model, x, x)) ## takes a while ...

Transformation from Brown-Resnick to Bernoulli

Description

This function can be used to model a max-stable process based on a binary field, with the same extremal correlation function as a Brown-Resnick process

Cbg(h)=cos(π(2Φ(γ(h)/2)1))C_{bg}(h) = \cos(\pi (2\Phi(\sqrt{\gamma(h) / 2}) -1) )

Here, Φ\Phi is the standard normal distribution function, and γ\gamma is a semi-variogram with sill

4(erf1(1/2))2=2Φ1(3/4)2=1.819746/2=0.90987284(erf^{-1}(1/2))^2 = 2 * { \Phi^{-1}( 3 / 4 ) }^2 = 1.819746 / 2 = 0.9098728

Usage

RMbr2bg(phi, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

RMbr2bg
binary random field RPbernoulli simulated with RMbr2bg(RMmodel()) has a uncentered covariance function that equals

  1. the tail correlation function of the max-stable process constructed with this binary random field

  2. the tail correlation function of Brown-Resnick process with variogram RMmodel.

Note that the reference paper is based on the notion of the (genuine) variogram, whereas the package RandomFields is based on the notion of semi-variogram. So formulae differ by factor 2.

Value

object of class RMmodel

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

maxstableAdvanced, RMbr2eg, RMmodel, RMm2r, RPbernoulli, RPbrownresnick, RPschlather.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp(var=1.62 / 2) 
x <- seq(0, 10, 0.05)
z <- RFsimulate(RPschlather(RMbr2eg(model)), x, x)
plot(z)

Transformation from Brown-Resnick to Gauss

Description

This function can be used to model a max-stable process based on a binary field, with the same extremal correlation function as a Brown-Resnick process

Ceg(h)=12(12Φ(γ(h)/2))2C_{eg}(h) = 1 - 2 (1 - 2 \Phi(\sqrt{\gamma(h) / 2}) )^2

Here, Φ\Phi is the standard normal distribution function, and γ\gamma is a semi-variogram with sill

4(erf1(1/2))2=2[Φ1([1+1/2]/2)]2=4.425098/2=2.2125494(erf^{-1}(1/\sqrt 2))^2 = 2 * [\Phi^{-1}( [1 + 1/\sqrt 2] / 2)]^2 = 4.425098 / 2 = 2.212549

Usage

RMbr2eg(phi, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

RMbr2eg
The extremal Gaussian model RPschlather simulated with RMbr2eg(RMmodel()) has tail correlation function that equals the tail correlation function of Brown-Resnick process with variogram RMmodel.

Note that the reference paper is based on the notion of the (genuine) variogram, whereas the package RandomFields is based on the notion of semi-variogram. So formulae differ by factor 2.

Value

object of class RMmodel

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

maxstableAdvanced, RMbr2bg, RMmodel, RMm2r, RPbernoulli, RPbrownresnick, RPschlather.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp(var=1.62 / 2) 
binary.model <- RPbernoulli(RMbr2bg(model))
x <- seq(0, 10, 0.05)

z <- RFsimulate(RPschlather(binary.model), x, x)
plot(z)

Tail correlation function of the Brown-Resnick process

Description

RMbrownresnick defines the tail correlation function of the Brown-Resnick process.

C(h)=22Φ(γ(h)/2)C(h) = 2 - 2\Phi(\sqrt{\gamma(h)} / 2)

where ϕ\phi is the standard normal distribution function and γ\gamma is the semi-variogram.

Usage

RMbrownresnick(phi, var, scale, Aniso, proj)

Arguments

phi

variogram of class RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

For a given RMmodel the function RMbrownresnick(RMmodel()) 'returns' the tail correlation function of a Brown-Resnick process with variogram RMmodel.

Value

object of class RMmodel

Note

In the paper Kabluchko et al. (2009) the variogram instead of the semi-variogram is considered, so the formulae differ slightly.

In Version 3.0.33 a typo has been corrected.

Here, a definition is used that is consistent with the rest of the package.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Kabluchko, Z., Schlather, M. & de Haan, L (2009) Stationary max-stable random fields associated to negative definite functions Ann. Probab. 37, 2042-2065.

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RFsimulate, RMm2r, RMm3b, RMmps, RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

#plot covariance model of type RMbrownresnick
RMmodel <- RMfbm(alpha=1.5, scale=0.2)
plot(RMbrownresnick(RMmodel))

#simulate and plot corresponding Gaussian random field
x <- seq(-5, 5, 0.05)
z <- RFsimulate(RMbrownresnick(RMmodel), x=x, y=x)
plot(z)

Bubble model for arbitrary areas of scales

Description

A model that allows for arbitray areas of scale applied to an isotropic model, i.e.

C(x,y)=ϕ(xy/s)C(x,y) = \phi(\|x -y \| / s)

as long as sx=sy=ss_x = s_y = s. Here, sxs_x is the scaling at location xx,

The cross-correlations between areas of different scales are given through a modified distance dd. Let zsz_{s} be a finite subset of RdR^d depending on the scale ss. Let wuw_u be a weight for an auxiliary point uzsu\in z_{s} with uzswu=1\sum_{u \in z_s} w_u = 1. Let τx=sx2\tau_x = s_x^{-2}. Then

d2(x,y)=min{τ(x),τ(y)}xy2+ξspan(τ(x),τ(y))uzξ0.5wuxu2Δξd^2(x, y) = \min\{\tau(x), \tau(y)\} \|x - y\|^2 + \sum_{\xi \in_{span(\tau(x), \tau(y))}} \sum_{u \in z_{\xi^{-0.5}}} w_u \|x - u\|^2 \Delta \xi

Here, span(τ(x),τ(y))span(\tau(x), \tau(y)) is the finite set of values s2s^{-2} that are realized on the locations of interest and Δξ\Delta \xi is the difference of two realized and ordered values of the scaling ss.

Usage

RMbubble(phi, scaling, z, weight, minscale, barycentre,
         var, scale, Aniso, proj)

Arguments

phi

isotropic submodel

scaling

model that gives the non-stationary scaling sxs_x

z

matrix of the union of all zsz_s. The number of rows equals the dimension of the field. If not given, the locations with non-vanishing gradient are taken.

weight

vector of weights ww whose length equals the number of columns of z. The points given by z might be weighted.

minscale

vector for partioning zz into classes zsz_s. Its length equals the number of columns of z. The vector values must be descending. See details. If not given then zs=z_s=z for all ss. Else see details.

barycentre

logical. If FALSE and z is not given, the reference locations are those with non-vashing gradient. If TRUE then, for each realized value of the scale, the barycentre of the corresponding reference locations is used instead of the reference locations themselves. This leads to higher correlations, but also to highly non-stationary cross-correlation between the areas of different scale.

The argument has no effect when z is given.

Default: FALSE.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

minscale gives the minimal scale ss value above which the corresponding points z define the set zsz_s. The validity of the set zsz_s ends with the next lower value given.

Let minscale = (10, 10, 10, 7, 7, 7, 0.5). Then for some dd-dimensional vectors z1,,z7z_1,\ldots, z_7 we have

zs={z1,z2,z3},s10z_s = \{ z_1, z_2, z_3 \}, s \ge 10

zs={z4,z5,z5},7s<10z_s = \{ z_4, z_5, z_5 \}, 7 \ge s < 10

zs={z7},s0.5z_s = \{ z_7 \}, s \ge 0.5

Note that, in this case, all realized scaling values must be 0.5\ge 0.5. Note further, that the weights for the subset must sum up to one, i.e.

w1+w2+w3=w4+w5+w6=w7=1.w_1+w_2 +w_3=w_4 + w_5 + w_6 = w_7 = 1.

Value

RMbubble returns an object of class RMmodel.

Note

This model is defined only for grids.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Bonat, W.H. , Ribeiro, P. Jr. and Schlather, M. (2019) Modelling non-stationarity in scale. In preparation.

See Also

RMSadvanced, RMblend, RMscale

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,1, if (interactive()) 0.02 else 0.5)
d <- sqrt(rowSums(as.matrix(expand.grid(x-0.5, x-0.5))^2))
d <- matrix(d < 0.25, nc=length(x))
image(d)

scale <- RMcovariate(data=as.double(d) * 2 + 0.5, raw=TRUE)

## two models:
## the frist uses the standard approach for determining the
##           reference point z, which is based on gradients
## the second takes the centre of the ball
model1 <- RMbubble(RMexp(), scaling=scale)
model2 <- RMbubble(RMexp(), scaling=scale, z=c(0.5, 0.5))
model3 <- RMbubble(RMexp(), scaling=scale, barycentre=TRUE) # approx. of model2

## model2 has slightly higher correlations than model1:
C1 <- RFcovmatrix(model1, x, x)
C2 <- RFcovmatrix(model2, x, x)
C3 <- RFcovmatrix(model3, x, x) 
print(range(C2 - C1))
dev.new(); hist(C2 - C1)
print(range(C3 - C2)) # only small differences to C2
print(mean(C3 - C2))
dev.new(); hist(C3 - C2)

plot(z1 <- RFsimulate(model1, x, x))
plot(z2 <- RFsimulate(model2, x, x))
plot(z3 <- RFsimulate(model3, x, x)) # only tiny differences to z2


## in the following we compare the standard bubble model with
## the models RMblend, RMscale and RMS (so, model2 above
## performs even better)
biwm <- RMbiwm(nudiag=c(0.5, 0.5), nured=1, rhored=1, cdiag=c(1, 1), 
                s=c(0.5, 2.5, 0.5))
blend <- RMblend(multi=biwm, blend=RMcovariate(data = as.double(d), raw=TRUE))
plot(zblend <- RFsimulate(blend, x, x)) ## takes a while ...
Cblend <- RFcovmatrix(blend, x, x)

Mscale <- RMscale(RMexp(), scaling = scale, penalty=RMid() / 2)
plot(zscale <- RFsimulate(Mscale, x, x))
Cscale <- RFcovmatrix(Mscale, x, x)

Mscale2 <- RMscale(RMexp(), scaling = scale, penalty=RMid() / 20000)
plot(zscale2 <- RFsimulate(Mscale2, x, x))
Cscale2 <- RFcovmatrix(Mscale2, x, x)

S <- RMexp(scale = scale)
plot(zS <- RFsimulate(S, x, x))
CS <- RFcovmatrix(S, x, x)

print(range(C1 - CS))
print(range(C1 - Cscale))
print(range(C1 - Cscale2))
print(range(C1 - Cblend))
dev.new(); hist(C1-CS)     ## C1 is better
dev.new(); hist(C1-Cscale) ## C1 is better
dev.new(); hist(C1-Cscale2) ## both are equally good. Maybe C1 slightly better
dev.new(); hist(C1-Cblend) ## C1 is better

Cauchy Family Covariance Model

Description

RMcauchy is a stationary isotropic covariance model belonging to the Cauchy family. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(1+r2)(γ)C(r) = (1 + r^2)^(-\gamma)

where γ>0\gamma > 0. See also RMgencauchy.

Usage

RMcauchy(gamma, var, scale, Aniso, proj)

Arguments

gamma

a numerical value; should be positive to provide a valid covariance function for a random field of any dimension.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The paramater γ\gamma determines the asymptotic power law. The smaller γ\gamma, the longer the long-range dependence. The covariance function is very regular near the origin, because its Taylor expansion only contains even terms and reaches its sill slowly.

Each covariance function of the Cauchy Family is a normal scale mixture.

The generalized Cauchy Family (see RMgencauchy) includes this family for the choice α=2\alpha = 2 and β=2γ\beta = 2 \gamma. The generalized Hyperbolic Family (see RMhyperbolic) includes this family for the choice ξ=0\xi = 0 and γ=ν/2\gamma = -\nu/2; in this case scale=δ\delta.

Value

RMcauchy returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

  • Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

See Also

RMcauchytbm, RMgencauchy, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcauchy(gamma=1)
x <- seq(0, 10, 0.02)
plot(model, xlim=c(-3, 3))
plot(RFsimulate(model, x=x, n=4))

Modifications of the Cauchy Family Covariance Model

Description

RMcauchytbm() is a shortcut of RMtbm(RMgencauchy()) and is given here for downwards compatibility.

Usage

RMcauchytbm(alpha, beta, gamma, var, scale, Aniso, proj)

Arguments

alpha, beta

See RMgencauchy.

gamma

is the same as fulldim in RMtbm.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMcauchytbm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

See Also

RMcauchy, RMgencauchy, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcauchytbm(alpha=1, beta=1, gamma=3)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Schoenberg's representation for the classes psi_d and psipsi_{\infty} in d=2

Description

RMchoquet is an isotropic covariance model. The corresponding covariance function only depends on the angle 0θπ0 \le \theta \le \pi between two points on the sphere and is given for d=2 by

ψ(θ)=n=0bn,2/(n+1)Pn(cos(θ)),\psi(\theta) = \sum_{n=0}^{\infty} b_{n,2}/(n+1)*P_n(cos(\theta)),

where

n=0bn,d=1\sum_{n=0}^{\infty} b_{n,d}=1

and PnP_n is the Legendre Polynomial of integer order n>=0n >= 0.

Usage

RMchoquet(b)

Arguments

b

a numerical vector of weights in (0,1)(0,1), such that sum(b)=1.

Details

By the results (cf. Gneiting, T. (2013), p.1333) of Schoenberg and others like Menegatto, Chen, Sun, Oliveira and Peron, the class psidpsi_d of all real valued funcions on [0,π][0,\pi], with ψ(0)=1\psi(0)=1 and such that the associated isotropic function

h(x,y)=ψ(theta)withcos(θ)=<x,y>h(x,y)=\psi(theta) with cos(\theta)=<x,y>

forx,yinxinRd:x=1for x,y in {x in R^d: ||x|| = 1}

is (strictly) positive definite is represented by this covariance model. The model can be interpreted as Choquet representation in terms of extremal members, which are non-strictly positive definite.

Special cases are the multiquadric family (see RMmultiquad) and the model of the sine power function (see RMsinepower).

Value

RMchoquet returns an object of class RMmodel.

Author(s)

Christoph Berreth; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (2013) Strictly and non-strictly positive definite functions on spheres. Bernoulli, 19(4), 1327-1349.

  • Schoenberg, I.J. (1942) Positive definite functions on spheres. Duke Math.J.,9, 96-108.

  • Menegatto, V.A. (1994) Strictly positive definite kernels on the Hilbert sphere. Appl. Anal., 55, 91-101.

  • Chen, D., Menegatto, V.A., and Sun, X. (2003) A necessary and sufficient condition for strictly positive definite functions on spheres. Proc. Amer. Math. Soc.,131, 2733-2740.

  • Menegatto, V.A., Oliveira, C.P. and Peron, A.P. (2006) Strictly positive definite kernels on subsets of the complex plane. Comput. Math. Appl., 51, 1233-1250.

See Also

RMmodel, RFsimulate, RFfit, spherical models, RMmultiquad, RMsinepower

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## to do

Circular Covariance Model

Description

RMcircular is a stationary isotropic covariance model which is only valid for dimensions d2d \le 2. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=12/π(r(1r2)+arcsin(r))1[0,1](r).C(r) = 1 - 2/\pi (r \sqrt(1-r^2) + arcsin(r)) 1_{[0,1]}(r).

Usage

RMcircular(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimensions d2d \le 2. It is a covariance function with compact support (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 82).

Value

RMcircular returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcircular()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Covariance Matrix Constant in Space

Description

RMconstant defines a spatially constant covariance function.

Usage

RMconstant(M, var)

Arguments

M

a numerical matrix defining the user-defined covariance for a random field; the matrix should be positive definite, symmetric and its dimension should be equal to the length of observation or simulation vector.

var

variance

Value

RMconstant returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMfixcov, RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMconstant(diag(2),var=3)
plot(model)
x <- seq(0,10,length=100)
z <- RFsimulate(model=model,x=x)

Non-stationary covariance model corresponding to a variogram model

Description

This function generalizes the well-known non-stationary covariance function 2min{x,y}2\min\{x,y\} of the Brownian motion with variogram γ(x,y)=xy\gamma(x,y) = |x-y|, x,y0x,y\ge 0 to arbitrary variogram models any spatial processes of any dimension and multivariability.

Furthermore, the standard condition for the Brownian motion WW is that variance equals 00 at the origin, i.e., W(x)=dZ(x)Z(0)W(x) =^d Z(x) -Z(0) for any zero mean Gaussian process ZZ with variogram γ(x,y)=xy\gamma(x,y) = |x-y| is replaced by W(x)=Z(x)i=1naiZ(xi)W(x) = Z(x) -\sum_{i=1}^n a_i Z(x_i) with i=1nai=1\sum_{i=1}^n a_i = 1.

For a given variogram γ\gamma, aia_i and xix_i, the model equals C(x,y)=i=1nai(γ(x,xi)+γ(xi,y))γ(x,y)i=1nj=1naiajγ(xi,yi)C(x, y) = \sum_{i=1}^n a_i (\gamma(x, x_i) + \gamma(x_i, y)) - \gamma(x, y) - \sum_{i=1}^n \sum_{j=1}^n a_i a_j \gamma(x_i, y_i)

Usage

RMcov(gamma, x, y=NULL, z=NULL, T=NULL, grid, a,
       var, scale, Aniso, proj, raw, norm)

Arguments

gamma

a variogram model. Possibly multivariate.

x, y, z, T, grid

The usual arguments as in RFsimulate to define the locations where the covariates are given. Additional x might be set to one of the values "origin", "center", "extremals", or "all". If x is not given, x is set to "origin".

a

vector of weights. The length of a must equal the number of points given by x, y, z and T. The values of a must sum up to 11. If a is not given, equals weights are used.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

raw

logical. If FALSE then the data are interpolated. This approach is always save, but might be slow. If TRUE then the data may be accessed when covariance matrices are calculated. No rescaling or anisotropy definition is allowed in combination with the model. The use is dangerous, but fast.
Default: FALSE.

norm

optional model that gives the norm between locations

Value

RMcov returns an object of class RMmodel

Author(s)

Martin Schlather, [email protected]

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
bm <- RMfbm(alpha=1)
plot(bm)

x <- seq(0, 6, if (interactive()) 0.125 else 3)
plot(RFsimulate(bm, x))

## standardizing with the random variable at the origin
z1 <- RFsimulate(RMcov(bm), x)
plot(z1)
z1 <- as.vector(z1)
zero <- which(abs(x) == 0)
stopifnot(abs(z1[zero]) < 1e-13)

## standardizing with the random variable at the center of the interval
z2 <- RFsimulate(RMcov(bm, "center"), x)
plot(z2)
z2 <- as.vector(z2)
stopifnot(abs(z2[(length(z2) + 1) / 2]) < 1e-13)


## standardizing with the random variables at the end points of the interval
z3 <- RFsimulate(RMcov(bm, "extremals"), x)
plot(z3)
z3 <- as.vector(z3)
stopifnot(abs(z3[1] + z3[length(z3)]) < 1e-13)

Model for covariates

Description

The model makes covariates available.

Usage

RMcovariate(formula=NULL, data, x, y=NULL, z=NULL, T=NULL, grid,
            raw, norm, addNA, factor)

Arguments

formula, data

formula and by which the data should be modelled, similar to lm.

If formula is not given, the the linear model is given by the data themselves.

x, y, z, T, grid

optional. The usual arguments as in RFsimulate to define the locations where the covariates are given.

raw

logical. If FALSE then the data are interpolated. This approach is always save, but might be slow. If TRUE then the data may be accessed when covariance matrices are calculated. No rescaling or anisotropy definition is allowed in combination with the model. The use is dangerous, but fast.
Default: FALSE.

norm

optional model that gives the norm between locations

addNA

If addNA is TRUE, then an additional (linear) factor is estimated in an estimation framework. This parameter must be set in particular when RMcovariate passes several covariates.

factor

real value. From user's point of view very much the same as setting the argument var

.

Details

The function interpolates (nearest neighbour) between the values.

Value

RMcovariate returns an object of class RMmodel.

Note

  • c, x also accept lists of data. However, its use is not in an advanced stage yet.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMfixcov, RMmodel, RMtrend

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

z <- 0.2 + (1:10)
RFfctn(RMcovariate(z), 1:10)
RFfctn(RMcovariate(data=z, x=1:10), c(2, 2.1, 2.5, 3))

Cox Isham Covariance Model

Description

RMcoxisham is a stationary covariance model which depends on a univariate stationary isotropic covariance model C0C_0, which is a normal scale mixture.

The corresponding covariance function only depends on the difference (h,t)Rd+1=Rd×R(h,t) \in {\bf R}^{d+1}={\bf R}^d\times{\bf R} between two points in d+1d+1-dimensional space and is given by

C(h,t)=E+tβD1/2C0([(htμ)T(E+tβD)1(htμ)]1/2)C(h,t)=|E + t^\beta D|^{-1/2} C_0([(h - t \mu)^T (E + t^\beta D)^{-1} (h - t \mu)]^{1/2})

Here μRd\mu \in {\bf R}^d is a vector in dd-dimensional space; EE is the d×dd \times d-identity matrix and DD is a d×dd \times d-correlation matrix with D>0|D| > 0. The parameter β\beta is in (0,2](0,2]. Currently, the implementation is done only for d=2d=2.

Usage

RMcoxisham(phi,mu,D,beta,var, scale, Aniso, proj)

Arguments

phi

a univariate stationary isotropic covariance model for random fields on dd-dimensional space, which is moreover a normal scale mixture, that means an RMmodel whose monotone property equals 'normal mixture', see
RFgetModelNames(monotone="normal mixture")
and whose maxdim is at least 2.

mu

a vector in dd-dimensional space

D

a d×dd \times d-correlation matrix with D>0|D| > 0

beta

numeric in the interval (0,2](0,2]; default value is 2

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model stems from a rainfall model (cf. Cox, D.R., Isham, V.S. (1988)) and equals the following expectation

C(h,t)=EVC0(hVt)C(h,t)=\bold{E}_V C_0(h-Vt)

where the random wind speed vector VV follows a dd-variate normal distribution with expectation mumu and covariance matrix D/2D/2 (cf. Schlather, M. (2010), Example 9).

Value

RMcoxisham returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Cox, D.R., Isham, V.S. (1988) A simple spatial-temporal model of rainfall. Proc. R. Soc. Lond. A, 415, 317-328.

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcoxisham(RMgauss(), mu=1, D=1)
x <- seq(0, 10, 0.3)
plot(model, dim=2)
plot(RFsimulate(model, x=x, y=x))

Cubic Covariance Model

Description

RMcubic is a stationary isotropic covariance model which is only valid for dimensions d3d \le 3. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(17r2+8.75r33.5r5+0.75r7)1[0,1](r).C(r) = (1 - 7r^2 + 8.75 r^3 - 3.5 r^5 + 0.75 r^7) 1_{[0,1]}(r).

Usage

RMcubic(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimensions d3d \le 3. It is a 2 times differentiable covariance function with compact support (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 84).

Value

RMcubic returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcubic()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Curlfree Covariance Model

Description

RMcurlfree is a multivariate covariance model which depends on a univariate stationary covariance model where the covariance function phi(h) is twice differentiable.

The corresponding matrix-valued covariance function C of the model only depends on the difference hh between two points and it is given by the following components:

  • the potential

  • the vector field given by

    C(h)=(h(h)T)C0(h)C(h)=( - \nabla_h (\nabla_h)^T ) C_0(h)

  • the field of sinks and sources

Usage

RMcurlfree(phi, which, var, scale, Aniso, proj)

Arguments

phi

a univariate stationary covariance model (2- or 3-dimensional).

which

vector of integers. If not given all components are returned; otherwise the selected components are returned.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model returns the potential field in the first component, the corresponding curlfree field and field of sources and sinks in the last component.

See also the models RMdivfree and RMvector.

Value

RMcurlfree returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Scheuerer, M. and Schlather, M. (2012) Covariance Models for Divergence-Free and Curl-Free Random Vector Fields. Stochastic Models 28:3.

See Also

RMderiv, RMdivfree, RMvector, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMcurlfree(RMgauss(), scale=4)
plot(model, dim=2)

x.seq <- y.seq <- seq(-10, 10, 0.2)
simulated <- RFsimulate(model=model, x=x.seq, y=y.seq)
plot(simulated, select.variables=list(1, c(1, 2:3), 4))

Gneiting's modification towards finite range

Description

RMcutoff is a functional on univariate stationary isotropic covariance functions ϕ\phi.

The corresponding function CC (which is not necessarily a covariance function, see details) only depends on the distance rr between two points in dd-dimensional space and is given by

C(r)=ϕ(r),0rdC(r)=\phi(r), 0\le r \le d

C(r)=b0((dR)ara)2a,drdRC(r) = b_0 ((dR)^a - r^a)^{2 a}, d \le r \le dR

C(r)=0,dRrC(r) = 0, dR \le r

The parameters RR and b0b_0 are chosen internally such that CC is a smooth function.

Usage

RMcutoff(phi, diameter, a, var, scale, Aniso, proj)

Arguments

phi

a univariate stationary isotropic covariance model. See, for instance,

RFgetModelNames(type="positive definite", domain="single variable", isotropy="isotropic", vdim=1).

diameter

a numerical value; should be greater than 0; the diameter of the domain on which the simulation is done

a

a numerical value; should be greater than 0; has been shown to be optimal for a=1/2a = 1/2 or a=1a =1.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The algorithm that checks the given parameters knows only about some few necessary conditions. Hence it is not ensured that the cutoff-model is a valid covariance function for any choice of ϕ\phi and the parameters.

For certain models ϕ\phi, e.g. RMstable, RMwhittle and RMgencauchy, some sufficient conditions are known (cf. Gneiting et al. (2006)).

Value

RMcutoff returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Sevecikova, H, Percival, D.B., Schlather M., Jiang Y. (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in $R^2$: Exploring the Limits. J. Comput. Graph. Stat. 15, 483–501.

  • Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp()
plot(model, model.cutoff=RMcutoff(model, diameter=1), xlim=c(0, 4))

model <- RMstable(alpha = 0.8)
plot(model, model.cutoff=RMcutoff(model, diameter=2), xlim=c(0, 5))
x <- y <- seq(0, 4, 0.05)
plot(RFsimulate(RMcutoff(model), x=x, y = y))

Dagum Covariance Model Family

Description

RMdagum is a stationary isotropic covariance model. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=1(1+rβ)γβ.C(r) = 1-(1+r^{-\beta})^{\frac{-\gamma}{\beta}}.

The parameters β\beta and γ\gamma can be varied in the intervals (0,1](0,1] and (0,1)(0,1), respectively.

Usage

RMdagum(beta, gamma, var, scale, Aniso, proj)

Arguments

beta

numeric in (0,1](0,1]

gamma

numeric in (0,1)(0,1)

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Like the generalized Cauchy model the Dagum family can be used to model fractal dimension and Hurst effect. For a comparison of these see Berg, C. and Mateau, J. and Porcu, E. (2008). This paper also establishes valid parameter choices for the Dagum family, but be careful because therein the model is parameterized differently.

Value

RMdagum returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Berg, C. and Mateau, J. and Porcu, E. (2008) The dagum family of isotropic correlation functions. Bernoulli 14(4), 1134–1149.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMdagum(beta=0.5, gamma=0.5, scale=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Exponentially Damped Cosine

Description

RMdampedcos is a stationary isotropic covariance model. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=exp(λr)cos(r).C(r) = exp(-\lambda r) \cos(r).

Usage

RMdampedcos(lambda, var, scale, Aniso, proj)

Arguments

lambda

numeric. The range depends on the dimension of the random field (see details).

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is valid for any dimension dd. However, depending on the dimension of the random field the following bound for the argument λ\lambda has to be respected:

λ1/tan(π/(2d)).\lambda \ge 1/{\tan(\pi/(2d))}.

This covariance models a hole effect (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 92).

For λ=0\lambda = 0 we obtain the covariance function

C(r)=cos(r)C(r)=\cos(r)

which is only valid for d=1d=1 and corresponds to RMbessel for ν=0.5\nu=-0.5, there.

Value

RMdampedcos returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

See Also

RMbessel, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMdampedcos(lambda=0.3, scale=0.1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Declaration of dummy variables for statistical inference

Description

The only purpose of this function is the declaration of dummy variables for defining more complex relations between parameters that are to be estimated.

Its value as a covariance model is identically zero, independently of the variables declared.

Usage

RMdeclare(...)

Arguments

...

the names of additional parameters, not in inverted commas. No values should be given.

Value

RMdeclare returns an object of class RMmodel

Note

Only scalars can be defined here, since only scalars can be used within formulae.

Author(s)

Martin Schlather, [email protected]

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## The following two examples illustrate the use of RMdeclare and the
## argument 'params'. The purpose is not to give nice statistical models 

x <- seq(1, 3, 0.1)
## note that there isn't any harm to declare variables ('u')
## RMdeclare that are of no use in a simulation
model <- ~ RMexp(sc=sc1, var=var1) + RMgauss(var=var2, sc=sc2) + RMdeclare(u)
p <- list(sc1=2, var1=3, sc2=4, var2=5)
z <- RFsimulate(model = model, x=x, y=x, params=p)
plot(z)

## note that the model remains the same, only the values in the
## following list change. Here, sc1, var1, sc2 and u are estimated
## and var2 is given by a forula.
p.fit <- list(sc1 = NA, var1=NA, var2=~2 * u, sc2 = NA, u=NA)
lower <- list(sc1=20, u=5)
upper <- list(sc2=1.5, sc1=100, u=15)
f <- RFfit(model, data=z, params=p.fit, lower = lower, upper = upper)
print(f)


## The second example shows that rather complicated constructions are
## possible, i.e., formulae involving several variables, both known ('abc')
## and unknown ones ('sc', 'var'). Note that there are two different
## 'var's a unknown variable and an argument for RMwhittle
## Not run: 
	 
model2 <- ~ RMexp(sc) + RMwhittle(var = g, nu=Nu) + 
  RMnugget(var=nugg) +  RMexp(var=var, Aniso=matrix(A, nc=2)) +
  RMdeclare(CCC, DD)
p.fit <- list(g=~sc^1.5,  nugg=~sc * var * abc, sc=NA, var=~DD, Nu=NA, abc=123,
	      A = ~c(1, 2, DD * CCC, CCC), CCC = NA, DD=NA)
lower <- list(sc=1, CCC=1, DD=1)
upper <- list(sc=100, CCC=100, DD=100)
f2 <- RFfit(model2, data=z, params=p.fit, lower = lower, upper = upper)
print(f2)

## End(Not run)

Bivariate Delay Effect

Description

RMdelay is a (m+1)(m+1)-variate stationary covariance model. which depends on a univariate stationary covariance model C0C_0.

The corresponding covariance function only depends on the difference hRdh \in {\bf R}^d between two points in dd-dimensional space and is given by

C(h)=(C0(hsi+sj))i,j=0,,mC(h)=(C_0(h - s_i +s_j))_{i,j=0,\ldots,m}

where sRd×ms \in {\bf R}^{d\times m} and s0=0s_0=0

Usage

RMdelay(phi,s,var, scale, Aniso, proj)

Arguments

phi

a univariate stationary covariance model, that means an RMmodel whose vdim equals 1.

s

a d×md\times m-dimensional shift matrix, where dd is the dimension of the space, giving the components s=(s1,,sm)s=(s_1,\ldots, s_m) where the sis_i are vectors.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Here, a multivariate random field is obtained from a single univariate random field by shifting it by a fixed value.

Value

RMdelay returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3nd edition.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- y <- seq(-10,10,0.2)
model <- RMdelay(RMstable(alpha=1.9, scale=2), s=c(4,4))
plot(model, dim=2, xlim=c(-6, 6), ylim=c(-6,6))

simu <- RFsimulate(model, x, y)
plot(simu, zlim="joint")

Gradient of a field

Description

RMderiv is a multivariate covariance model which models a field and its gradient.

For an isotropic covariance model varphivarphi, the covariance CC given by RMderiv equals

C11(x,y)=φ(xy)C_{11}(x,y) = \varphi(\| x - y\|)

Cj1(x,y)=C1j(x,y)=φ(xy)/xC_{j1}(x,y) = -C_{1j}(x,y) = \partial \varphi(\|x - y\|) / \partial x

Ci,j(x,y)=2φ(xy)/xyC_{i,j}(x,y) = \partial^2 \varphi(\|x - y\|) / \partial x \partial y

for i,j=2,,di,j = 2,\ldots, d where dd is the dimension of the field.

Usage

RMderiv(phi, which, var, scale, Aniso, proj)

Arguments

phi

a univariate stationary covariance model (in 2 or 3 dimensions).

which

vector of integers. If not given all components are returned; otherwise the selected components are returned.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMderiv returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Matheron

See Also

RMcurlfree, RMdivfree, RMvector

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMderiv(RMgauss(), scale=4)
plot(model, dim=2)

x.seq <- y.seq <- seq(-10, 10, 0.4)
simulated <- RFsimulate(model=model, x=x.seq, y=y.seq)

plot(simulated)

Modified De Wijsian Variogram Model

Description

The modified RMdewijsian model is an intrinsically stationary isotropic variogram model. The corresponding centered semi-variogram only depends on the distance r0r \ge 0 between two points and is given by

γ(r)=log(rα+1)\gamma(r) = \log(r^{\alpha}+1)

where α(0,2]\alpha \in (0,2].

Usage

RMdewijsian(alpha, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; in the interval (0,2].

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above variogram remains unmodified.

Details

Originally, the logarithmic model γ(r)=log(r)\gamma(r) = \log(r) was named after de Wijs and reflects a principle of similarity (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 90). But note that γ(r)=log(r)\gamma(r) = \log(r) is not a valid variogram (γ(0)\gamma(0) does not vanish) and can only be understood as a characteristic of a generalized random field.

The modified RMdewijsian model γ(r)=log(rα+1)\gamma(r) = \log(r^{\alpha}+1) is a valid variogram model (cf. Wackernagel, H. (2003), p. 336).

Value

RMdewijsian returns an object of class RMmodel.

Note

Note that the (non-modified) de Wijsian model equals γ(r)=log(r)\gamma(r) = \log(r).

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3nd edition.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMdewijsian(alpha=1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Divfree Covariance Model

Description

RMdivfree is a multivariate covariance model which depends on a univariate stationary covariance model where the covariance function phi(h) is twice differentiable.

The corresponding matrix-valued covariance function C of the model only depends on the difference hh between two points and it is given by the following components:

  • the potential

  • the vector field given by

    C(h)=(ΔE+T)C0(h)C(h)=( - \Delta E + \nabla \nabla^T ) C_0(h)

  • the curl field

Usage

RMdivfree(phi, which, var, scale, Aniso, proj)

Arguments

phi

a univariate stationary covariance model (in 2 or 3 dimensions).

which

vector of integers. If not given all components are returned; otherwise the selected components are returned.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model returns the potential field in the first component, the corresponding divfree field and the field of curl strength in the last component.

See also the models RMcurlfree and RMvector.

Value

RMdivfree returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Scheuerer, M. and Schlather, M. (2012) Covariance Models for Divergence-Free and Curl-Free Random Vector Fields. Stochastic Models 28:3.

See Also

RMcurlfree, RMderiv, RMvector, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMdivfree(RMgauss(), scale=4)
plot(model, dim=2)

x.seq <- y.seq <- seq(-10, 10, 0.2)
simulated <- RFsimulate(model=model, x=x.seq, y=y.seq)

plot(simulated)
plot(simulated, select.variables=1)
plot(simulated, select.variables=2:3)
plot(simulated, select.variables=list(2:3))
plot(simulated, select.variables=list(1, 2:3, 4))
plot(simulated, select.variables=list(1, c(1, 2:3), 4))

Special models for rotation like fields

Description

RMeaxxa and RMetaxxa define the auxiliary functions

f(h)=hAAh+diag(E)f(h) = h^\top A A^\top h + diag(E)

and

f(h)=hARRAh+diag(E)f(h) = h^\top A R R A^\top h + diag(E)

respectively.

Usage

RMeaxxa(E, A) 
RMetaxxa(E, A, alpha)

Arguments

E

m-variate vector of positive values

A

m×km\times k matrix

alpha

angle for the rotation matrix RR

Details

RMeaxxa is defined in space and returns an m-variate model.

RMetaxxa is a space-time model with two spatial dimensions. The matrix R is a rotation matrix with angle βt\beta t where tt is the time component.

Value

RMeaxxa and RMetaxxa return an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMmodel, S10

Examples

# see S10

Generalized Cauchy Family Covariance Model

Description

RMepscauchy is a stationary isotropic covariance model belonging to the generalized Cauchy family. In contrast to most other models it is not a correlation function. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(ε+rα)(β/α)C(r) = (\varepsilon + r^\alpha)^(-\beta/\alpha)

where ϵ>0\epsilon > 0, α(0,2]\alpha \in (0,2] and β>0\beta > 0. See also RMcauchy.

Usage

RMepscauchy(alpha, beta, eps, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; should be in the interval (0,2] to provide a valid covariance function for a random field of any dimension.

beta

a numerical value; should be positive to provide a valid covariance function for a random field of any dimension.

eps

a positive value

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model has a smoothness parameter α\alpha and a parameter β\beta which determines the asymptotic power law. More precisely, this model admits simulating random fields where fractal dimension D of the Gaussian sample and Hurst coefficient H can be chosen independently (compare also RMlgd): Here, we have

D=d+1α/2,α(0,2]D = d + 1 - \alpha/2, \alpha \in (0,2]

and

H=1β/2,β>0.H = 1 - \beta/2, \beta > 0.

I. e. the smaller β\beta, the longer the long-range dependence.

The covariance function is very regular near the origin, because its Taylor expansion only contains even terms and reaches its sill slowly.

Each covariance function of the Cauchy family is a normal scale mixture.

Note that the Cauchy Family (see RMcauchy) is included in this family for the choice α=2\alpha = 2 and β=2γ\beta = 2 \gamma.

Value

RMepscauchy returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

See Also

RMcauchy, RMcauchytbm, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMepscauchy(alpha=1.5, beta=1.5, scale=0.3, eps=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Exponential Covariance Model

Description

RMexp is a stationary isotropic covariance model whose corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=er.C(r) = e^{-r}.

Usage

RMexp(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model is a special case of the Whittle covariance model (see RMwhittle) if ν=12\nu=\frac{1}{2} and of the symmetric stable family (see RMstable) if ν=1\nu = 1. Moreover, it is the continuous-time analogue of the first order autoregressive time series covariance structure.

The exponential covariance function is a normal scale mixture.

Value

RMexp returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Covariance model

  • Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Tail correlation function

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMwhittle, RMstable, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Exponential operator

Description

RMexponential yields a covariance model from a given variogram or covariance model. The covariance CC is given as

C(h)=exp(ϕ(h))k=0nϕk(h)/k!exp(ϕ(0))k=0nϕk(0)/k!C(h) = \frac{\exp(\phi(h)) -\sum_{k=0}^n \phi^k(h)/k!}{\exp(\phi(0)) -\sum_{k=0}^n \phi^k(0)/k!}

if ϕ\phi is a covariance model, and as

C(h)=exp(ϕ(h))C(h) = \exp(-\phi(h))

if ϕ\phi is a variogram model.

Usage

RMexponential(phi, n, standardised, var, scale, Aniso, proj)

Arguments

phi

a valid RMmodel; either a variogram model or a covariance model

n

integer, see formula above. Default is -1; if the multivariate dimension of the submodel is greater than 1 then only the default value is valid.

standardised

logical. If TRUE then the above formula holds. If FALSE then only the nominator of the above formula is returned. Default value is TRUE.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

If γ\gamma is a variogram, then exp(γ)\exp(-\gamma) is a valid covariance.

Value

RMexponential returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

See, for instance,

  • Berg, C., Christensen, J. P. R., Ressel, P. (1984) Harmonic Analysis on Semigroups. Theory of Positive Definite and Related Functions. Springer, New York.

  • Sasvari, Z. (2013) Multivariate Characteristic and Correlation Functions. de Gruyter, Berlin.

  • Schlather, M. (2010) Some covariance models based on normal scale mixtures, Bernoulli 16, 780-797.

  • Schlather, M. (2012) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J. M., Schlather, M. Advances and Challenges in Space-time Modelling of Natural Events, Springer, New York.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMexponential(RMfbm(alpha=1))  ## identical to RMexp()
plot(RMexp(), model=model, type=c("p", "l"), pch=20)

Variogram Model of Fractal Brownian Motion

Description

RMfbm is an intrinsically stationary isotropic variogram model. The corresponding centered semi-variogram only depends on the distance r0r \ge 0 between two points and is given by

γ(r)=rα\gamma(r) = r^\alpha

where α(0,2]\alpha \in (0,2].
By now, the model is implemented for dimensions up to 3.
For a generalized model see also RMgenfbm.

Usage

RMfbm(alpha, var, scale, Aniso, proj)

Arguments

alpha

numeric in (0,2](0,2]; refers to the fractal dimension of the process

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above variogram remains unmodified.

Details

The variogram is unbounded and belongs to a non-stationary process with stationary increments. For α=1\alpha=1 and scale=2 we get a variogram corresponding to a standard Brownian Motion.

For α(0,2)\alpha \in (0,2) the quantity H=α2H = \frac{\alpha} 2 is called Hurst index and determines the fractal dimension DD of the corresponding Gaussian sample paths

D=d+1HD = d + 1 - H

where dd is the dimension of the random field (see Chiles and Delfiner, 1999, p. 89).

Value

RMfbm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and P. Delfiner (1999) Geostatistics. Modeling Spatial Uncertainty. New York, Chichester: John Wiley & Sons.

  • Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599.

See Also

RMgenfbm, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMfbm(alpha=1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Fixed Covariance Matrix

Description

RMfixcov is a user-defined covariance according to the given covariance matrix.

It extends to the space through a Voronoi tessellation.

Usage

RMfixcov(M, x, y=NULL, z=NULL, T=NULL, grid, var, proj, raw, norm)

Arguments

M

a numerical matrix defining the user-defined covariance for a random field; the matrix should be positive definite, symmetric and its dimension should be equal to the length of observation or simulation vector.

x, y, z, T, grid

optional. The usual arguments as in RFsimulate to define the locations where the covariates are given.

var, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

raw

logical. If FALSE then the data are interpolated. This approach is always save, but might be slow. If TRUE then the data may be accessed when covariance matrices are calculated. No rescaling or anisotropy definition is allowed in combination with the model. The use is dangerous, but fast.
Default: FALSE.

norm

optional model that gives the norm between locations

Details

The covariances passed are implemented for the given locations. Within any Voronoi cell (around a given location) the correlation is assumed to be one.

In particular, it is used in RFfit to define neighbour or network structure in the data.

Value

RMfixcov returns an object of class RMmodel.

Note

Starting with version 3.0.64, the former argument element is replaced by the general option set in RFoptions.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Ober, U., Ayroles, J.F., Stone, E.A., Richards, S., Zhu, D., Gibbs, R.A., Stricker, C., Gianola, D., Schlather, M., Mackay, T.F.C., Simianer, H. (2012): Using Whole Genome Sequence Data to Predict Quantitative Trait Phenotypes in Drosophila melanogaster. PLoS Genet 8(5): e1002685.

See Also

RMcovariate, RMmodel, RFsimulate, RFfit, RMuser.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


## Example 1 showing that the covariance structure is correctly implemented
n <- 10
C <- matrix(runif(n^2), nc=n)
(C <- C %*% t(C))
RFcovmatrix(RMfixcov(C), 1:n)


## Example 2 showing that the covariance structure is interpolated
RFcovmatrix(RMfixcov(C, 1:n), c(2, 2.1, 2.5, 3))


## Example 3 showing the use in a separable space-time model
model <- RMfixcov(C, 1:n, proj="space") * RMexp(s=40, proj="time")
(z <- RFsimulate(model, x = seq(0,12, 0.5), T=1:100))
plot(z)

Fixed Effect Model

Description

Expressions of the form X@RMfixed(beta) can be used within a formula of the type

response fixedeffects+randomeffects+errortermresponse ~ fixed effects + random effects + error term

that specifies the Linear Mixed Model.

Important remark: RMfixed is NOT a function although the parentheses notation is used to specify the vector of coefficients.

The matrix XX is the design matrix and β\beta is a vector of coefficients.

Note that a fixed effect of the form XX is interpreted as X@RMfixed(beta=NA) by default (and β\beta is estimated provided that the formula is used in RFfit). Note that the 1 in an expression 1@RMfixed(beta) is interpreted as the identity matrix.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFformula, RFsimulate.

Examples

## For examples see the help page of 'RFformula'. ##

Variogram Model Similar to Fractal Brownian Motion

Description

RMflatpower is an intrinsically stationary isotropic variogram model. The corresponding centered semi-variogram only depends on the distance r0r \ge 0 between two points and is given by

γ(r)=r2/(1+r2)α\gamma(r) = r^2 / ( 1 + r^2)^\alpha

where α(0,1]\alpha \in (0,1].

For related models see RMgenfbm.

Usage

RMflatpower(alpha, var, scale, Aniso, proj)

Arguments

alpha

numeric in (0,1](0,1]; refers to the fractal dimension of the process

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above variogram remains unmodified.

Details

The model is always smooth at the origin.

The parameter α\alpha only gives the tail behaviour and satisfies α(0,1]\alpha \in (0,1].

The variogram is unbounded and belongs to a non-stationary process with stationary increments.

Value

RMflatpower returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Oesting, M., Schlather, M., and Friederichs, P. (2014) Conditional Modelling of Extreme Wind Gusts by Bivariate Brown-Resnick Processes arxiv 1312.4584.

See Also

RMgenfbm, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMflatpower(alpha=0.5)
x <- seq(0, 10, 0.1)
plot(model)
plot(RFsimulate(model, x=x))

Fractionally Differenced Process Model

Description

RMfractdiff is a stationary isotropic covariance model. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given for integers rNr \in {\bf N} by

C(r)=(1)rΓ(1a/2)2Γ(1a/2+r)Γ(1a/2r)rNC(r) = (-1)^r \frac{ \Gamma(1-a/2)^2 }{ \Gamma(1-a/2+r) \Gamma(1-a/2-r) } r \in {\bf N}

and otherwise linearly interpolated. Here, a[1,1)a \in [-1,1), Γ\Gamma denotes the gamma function. It can only be used for one-dimensional random fields.

Usage

RMfractdiff(a, var, scale, Aniso, proj)

Arguments

a

1a<1-1 \le a < 1

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimension d=1d = 1. It stems from time series modelling where the grid locations are multiples of the scale parameter.

Value

RMfractdiff returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMfractdiff(0.5, scale=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Fractal Gaussian Model Family

Description

RMfractgauss is a stationary isotropic covariance model. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=0.5((r+1)α2rα+r1α)C(r) = 0.5 ((r+1)^{\alpha}-2r^{\alpha}+|r-1|^{\alpha})

with 0<α20 < \alpha \le 2. It can only be used for one-dimensional random fields.

Usage

RMfractgauss(alpha,var, scale, Aniso, proj)

Arguments

alpha

0<α20 < \alpha \le 2

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimension d=1d = 1. It is the covariance function for the fractional Gaussian noise with self-affinity index (Hurst parameter) H=α/2H=\alpha /2 with 0<α20 < \alpha \le 2.

Value

RMfractgauss returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMfractgauss(alpha=0.5, scale=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Gaussian Covariance Model

Description

RMgauss is a stationary isotropic covariance model. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=er2C(r) = e^{-r^2}

Usage

RMgauss(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model is called Gaussian because of the functional similarity of the spectral density of a process with that covariance function to the Gaussian probability density function.

The Gaussian model has an infinitely differentiable covariance function. This smoothness is artificial. Furthermore, this often leads to singular matrices and therefore numerically instable procedures (cf. Stein, M. L. (1999), p. 29).

The Gaussian model is included in the symmetric stable class (see RMstable) for the choice α=2\alpha = 2.

Value

RMgauss returns an object of class RMmodel.

Note

The use of RMgauss is questionable from both a theoretical (analytical paths) and a practical point of view (e.g. speed of algorithms). Instead, RMgneiting should be used.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Stein, M. L. (1999) Interpolation of Spatial Data. New York: Springer-Verlag

See Also

RMstable and RMmatern for generalizations;
RMmodel, RFsimulate, RFfit.

Do not mix up with RPgauss or RRgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMgauss(scale=0.4)
x <- seq(0, 10, 0.02)
plot(model)
lines(RMgauss(), col="red")
plot(RFsimulate(model, x=x))

Generalized Cauchy Family Covariance Model

Description

RMgencauchy is a stationary isotropic covariance model belonging to the generalized Cauchy family. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(1+rα)(β/α)C(r) = (1 + r^\alpha)^(-\beta/\alpha)

where α(0,2]\alpha \in (0,2] and β>0\beta > 0. See also RMcauchy.

Usage

RMgencauchy(alpha, beta, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; should be in the interval (0,2] to provide a valid covariance function for a random field of any dimension.

beta

a numerical value; should be positive to provide a valid covariance function for a random field of any dimension.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model has a smoothness parameter α\alpha and a parameter β\beta which determines the asymptotic power law. More precisely, this model admits simulating random fields where fractal dimension D of the Gaussian sample and Hurst coefficient H can be chosen independently (compare also with RMlgd): Here, we have

D=d+1α/2,α(0,2]D = d + 1 - \alpha/2, \alpha \in (0,2]

and

H=1β/2,β>0.H = 1 - \beta/2, \beta > 0.

I. e. the smaller β\beta, the longer the long-range dependence.

The covariance function is very regular near the origin, because its Taylor expansion only contains even terms and reaches its sill slowly.

Each covariance function of the Cauchy family is a normal scale mixture.

Note that the Cauchy Family (see RMcauchy) is included in this family for the choice α=2\alpha = 2 and β=2γ\beta = 2 \gamma.

Value

RMgencauchy returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Covariance function

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

Tail correlation function (for α(0,1]\alpha \in (0,1])

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMcauchy, RMcauchytbm, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMgencauchy(alpha=1.5, beta=1.5, scale=0.3)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Generalized Fractal Brownian Motion Variogram Model

Description

RMgenfbm is an intrinsically stationary isotropic variogram model. The corresponding centered semi-variogram only depends on the distance r0r \ge 0 between two points and is given by

γ(r)=(rα+1)β/α1\gamma(r) = (r^{\alpha}+1)^{\beta/\alpha}-1

where α(0,2]\alpha \in (0,2] and β(0,2]\beta \in (0,2].
See also RMfbm.

Usage

RMgenfbm(alpha, beta, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; should be in the interval (0,2].

beta

a numerical value; should be in the interval (0,2].

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above variogram remains unmodified.

Details

Here, the variogram of RMfbm is modified by the transformation (γ+1)δ/1(\gamma+1)^{\delta/-1} on variograms γ\gamma for δ(0,1]\delta \in (0,1]. This original modification allows for further generalization, cf. RMbcw.

Value

RMgenfbm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (2002) Nonseparable, stationary covariance functions for space-time data, JASA 97, 590-600.

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMbcw, RMfbm, RMmodel, RMflatpower, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMgenfbm(alpha=1, beta=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Gneiting-Wendland Covariance Models

Description

RMgengneiting is a stationary isotropic covariance model family whose elements are specified by the two parameters κ\kappa and μ\mu with nn being a non-negative integer and μd2\mu \ge \frac{d}{2} with dd denoting the dimension of the random field (the models can be used for any dimension). A corresponding covariance function only depends on the distance r0r \ge 0 between two points. For the case κ=0\kappa = 0 the Gneiting-Wendland model equals the Askey model RMaskey,

C(r)=(1r)β1[0,1](r),β=μ+1/2=μ+2κ+1/2.C(r) = (1-r)^\beta 1_{[0,1]}(r),\qquad\beta = \mu +1/2 = \mu + 2\kappa + 1/2.

For κ=1\kappa = 1 the Gneiting model is given by

C(r)=(1+βr)(1r)β1[0,1](r),β=μ+2κ+1/2.C(r) = \left(1+\beta r \right)(1-r)^{\beta} 1_{[0,1]}(r), \qquad \beta = \mu +2\kappa+1/2.

If κ=2\kappa = 2

C(r)=(1+βr+β213r2)(1r)β1[0,1](r),β=μ+2κ+1/2.C(r) = \left(1 + \beta r + \frac{\beta^{2} - 1}{3}r^{2} \right)(1-r)^{\beta} 1_{[0,1]}(r), \qquad \beta = \mu+2\kappa+1/2.

In the case κ=3\kappa = 3

C(r)=(1+βr+(2β23)5r2+(β24)β15r3)(1r)β1[0,1](r),β=μ+2κ+1/2.C(r) = \left( 1 + \beta r + \frac{(2\beta^{2}-3)}{5} r^{2}+ \frac{(\beta^2 - 4)\beta}{15} r^{3} \right)(1-r)^\beta 1_{[0,1]}(r), \qquad \beta = \mu+2\kappa + 1/2.

A special case of this model is RMgneiting.

Usage

RMgengneiting(kappa, mu, var, scale, Aniso, proj)

Arguments

kappa

0,,30,\ldots,3

; it chooses between the three different covariance models above.

mu

mu has to be greater than or equal to d2\frac{d}{2} where dd is the dimension of the random field.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This isotropic family of covariance functions is valid for any dimension of the random field.

A special case of this family is RMgneiting (with s=1s = 1 there) for the choice κ=3,μ=3/2\kappa = 3, \mu = 3/2.

Value

RMgengneiting returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (1999) Correlation functions for atmospherical data analysis. Q. J. Roy. Meteor. Soc Part A 125, 2449-2464.

  • Wendland, H. (2005) Scattered Data Approximation. Cambridge Monogr. Appl. Comput. Math.

See Also

RMaskey, RMbigneiting, RMgneiting, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMgengneiting(kappa=1, mu=1.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))


## same models:
model2 <- RMgengneiting(kappa=3, mu=1.5, scale= 1 / 0.301187465825)
plot(RMgneiting(), model2=model2, type=c("p", "l"), pch=20)

Non-Separable Space-Time model

Description

RMgennsst is a univariate stationary spaceisotropic covariance model on RdR^d whose corresponding covariance is given by

C(h,u)=ϕ(sqrt(hψ1(u)h))/(det(psi))C(h,u)= \phi( sqrt(h^\top \psi^{-1}(u) h)) / \sqrt(det(psi))

Usage

RMgennsst(phi, psi, dim_u, var, scale, Aniso, proj)

Arguments

phi

is a normal mixture RMmodel, cf.
RFgetModelNames(monotone="normal mixture").

psi

is a dd-variate variogram model RMmodel.

dim_u

the dimension of the component u

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model is used for space-time modelling where the spatial component is isotropic.

Value

RMgennsst returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMnsst, RMmodel, RFsimulate, RFfit.

Examples


Gneiting Covariance Model

Description

RMgneiting is a stationary isotropic covariance model which is only valid up to dimension 3, or 5 (see the argument orig). The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(1+8sr+25s2r2+32s3r3)(1sr)8C(r) = (1 + 8 s r + 25 s^2 r^2 + 32 s^3 r^3)(1-s r)^8

if 0r1s0 \le r \le \frac{1}{s} and

C(r)=0C(r)=0

otherwise. Here, s=0.301187465825s=0.301187465825. For a generalized model see also RMgengneiting.

Usage

RMgneiting(orig, var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

orig

logical. If TRUE the above model is used. Otherwise the RMgengneiting model C(s r) with kappa=3 as above, but with mu = 2.683509 and s=0.2745640815 is used. The latter has the advantage of being closer to the Gaussian model and it is valid up to dimension 5.

Default: TRUE.

Details

This isotropic covariance function is valid only for dimensions less than or equal to 3. It is 6 times differentiable and has compact support.

This model is an alternative to RMgauss as its graph is hardly distinguishable from the graph of the Gaussian model, but possesses neither the mathematical nor the numerical disadvantages of the Gaussian model.

It is a special case of RMgengneiting for the choice κ=3,μ=1.5\kappa=3, \mu=1.5.

Note that, in the original work by Gneiting (1999), a numerical value slightly deviating from the optimal one was used for μ=1.5\mu=1.5: s=10(2)47s=\frac{10 \sqrt(2)}{47}.

Value

RMgneiting returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

For the original version

  • Gneiting, T. (1999) Correlation functions for atmospherical data analysis. Q. J. Roy. Meteor. Soc Part A 125, 2449-2464.

For the version (orig=FALSE)

  • this package RandomFields.

See Also

RMbigneiting, RMgengneiting, RMgauss, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

plot(RMgneiting(), model2=RMgneiting(orig=FALSE), model3=RMgauss(), 
     xlim=c(-3,3), maxchar=100)
plot(RMgneiting(), model2=RMgneiting(orig=FALSE), model3=RMgauss(), 
     xlim=c(1.5,2.5), maxchar=100)

model <- RMgneiting(orig=FALSE, scale=0.4)
x <- seq(0, 10, 0.2) ## nicer with 0.1 instead of 0.2
z <- RFsimulate(model, x=x, y=x, z=x, T=c(1,1,4), maxGB=3)
plot(z, MARGIN.slices=4, MARGIN.movie=3)

Gneiting Covariance Model Used as Tapering Function

Description

RMgneitingdiff is a stationary isotropic covariance model which is only valid up to dimension 3. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(h)=C0(h/t)Wν(h/s)C(h) = C_0(h / t) W_\nu(h / s)

where C0C_0 is Gneiting's model RMgneiting and WνW_\nu is the Whittle model RMwhittle.

Usage

RMgneitingdiff(nu, taper.scale, scale, var, Aniso, proj)

Arguments

nu

see RMwhittle

taper.scale

is the parameter tt in the above formula.

scale

is the parameter ss in the above formula.

var, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model allows to a certain degree the smooth modelling of the differentiability of a covariance function with compact support.

Value

RMgneitingdiff returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (1999) Correlation functions for atmospherical data analysis. Q. J. Roy. Meteor. Soc Part A 125, 2449-2464.

See Also

RMbigneiting, RMgneiting, RMgengneiting, RMgauss, RMmodel, RMwhittle, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMgneitingdiff(nu=2, taper.scale=1, scale=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Generalized Hyperbolic Covariance Model

Description

RMhyperbolic is a stationary isotropic covariance model called “generalized hyperbolic”. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(δ2+r2)ν/2Kν(ξ(δ2+r2)1/2)δνKν(ξδ)C(r) = \frac{(\delta^2+r^2)^{\nu/2} K_\nu(\xi(\delta^2+r^2)^{1/2})}{\delta^\nu K_\nu(\xi \delta)}

where KνK_{\nu} denotes the modified Bessel function of second kind.

Usage

RMhyperbolic(nu, lambda, delta, var, scale, Aniso, proj)

Arguments

nu, lambda, delta

numerical values; should either satisfy
δ0\delta \ge 0, λ>0\lambda > 0 and ν>0\nu > 0, or
δ>0\delta > 0, λ>0\lambda > 0 and ν=0\nu = 0, or
δ>0\delta > 0, λ0\lambda \ge 0 and ν<0\nu < 0.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This class is over-parametrized, i.e. it can be reparametrized by replacing the three parameters λ\lambda, δ\delta and scale by two other parameters. This means that the representation is not unique.

Each generalized hyperbolic covariance function is a normal scale mixture.

The model contains some other classes as special cases; for λ=0\lambda = 0 we get the Cauchy covariance function (see RMcauchy) with γ=ν2\gamma = -\frac{\nu}2 and scale=δ\delta; the choice δ=0\delta = 0 yields a covariance model of type RMwhittle with smoothness parameter ν\nu and scale parameter λ1\lambda^{-1}.

Value

RMhyperbolic returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Shkarofsky, I.P. (1968) Generalized turbulence space-correlation and wave-number spectrum-function pairs. Can. J. Phys. 46, 2133-2153.

  • Barndorff-Nielsen, O. (1978) Hyperbolic distributions and distributions on hyperbolae. Scand. J. Statist. 5, 151-157.

  • Gneiting, T. (1997). Normal scale mixtures and dual probability densities. J. Stat. Comput. Simul. 59, 375-384.

See Also

RMcauchy, RMwhittle, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMhyperbolic(nu=1, lambda=2, delta=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Iaco-Cesare model

Description

The space-time covariance function is

C(r,t)=(1.0+rν+tλ)δC(r,t) = (1.0 + r^\nu + t^\lambda)^\delta

Usage

RMiaco(nu, lambda, delta, var, scale, Aniso, proj)

Arguments

nu, lambda

number in (0,2](0,2]

delta

positive number

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMiaco returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • de Cesare, L., Myers, D.E., and Posa, D. (2002) FORPRAN programs for space-time modeling. Computers \& Geosciences 28, 205-212.

  • de Iaco, S.. Myers, D.E., and Posa, D. (2002) Nonseparable space-time covariance models: some parameteric families. Math. Geol. 34, 23-42.

See Also

RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMiaco(nu=1, lambda=1.5, delta=0.5)
plot(model, dim=2)

x <- seq(0, 10, 0.1)
plot(RFsimulate(model, x=x, y=x))

Identical Model

Description

RMid is the identical function f(x)=xf(x) = x where xx is a vector of coordinates and f(x)f(x) is a model value.

Usage

RMid()

Value

RMid returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel. RMid, RMtrafo, RMprod

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## C(x,y) = < x, y >
RFcov(RMprod(RMid()), as.matrix(1:10), as.matrix(1:10), grid=FALSE)

Identical Model

Description

RMidmodel is the identical operator on models, i.e. for objects of class RMmodel.

Usage

RMidmodel(phi, vdim, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel

vdim

for internal purposes

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMidmodel returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel. RMid, RMtrafo, RMprod

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMexp()
x <- 0:10
z <- RFsimulate(model, x)

model2 <- RMidmodel(model)
z2 <- RFsimulate(model, x)
sum(abs(as.vector(z)- as.vector(z2))) == 0 # TRUE

Internal models

Description

Internal models or model names that may appear in feedbacks from 'RandomFields'. Those endings by ‘Intern’ should appear only in very rare cases.

Details

The following and many more internal models exist:

  • RF__Name__ : internal representation of certain functions RF__name__

  • RO# : model for transforming coordinates within the cartesian system

  • RO> : model for transforming earth coordinates to cartesian coordinates

  • ROmissing : for error messages only

  • RMmixed : internal representation of a mixed model

  • RMselect : will be obsolete in future

  • RMsetparam, RMptsGivenShape, RMstandardShape, RMstatShape : for max-stable processes and Poisson processes: models that combine shape functions with corresponding point processes

  • RP__name__Intern : internal representations of some processes

  • RPS, RPplusp, etc. : specific processes for RMS and RMplus etc. (For those covariance models that have specific simulation processes programmed.)

  • RMS : internal representation of the modifying arguments var, scale, Aniso, proj

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## in the following 'RPplus' appears as internal model
x <- seq(0, 10, 1) 
z <- RFsimulate(RPspecific(RMexp() + RMnugget()), x)
RFgetModelInfo(which="internal", level=0)

Integral exponential operator

Description

RMintexp is a univariate stationary covariance model depending on a univariate variogram model ϕ\phi. The corresponding covariance function only depends on the difference hh between two points and is given by

C(h)=(1exp(ϕ(h)))/ϕ(h)C(h)=(1 - exp(-\phi(h)))/\phi(h)

Usage

RMintexp(phi, var, scale, Aniso, proj)

Arguments

phi

a variogram RMmodel

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMintexp returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2012) Construction of covariance functions and unconditional simulation of random fields. Lecture Notes in Statistics, Proceedings, 207, 25–54.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMintexp(RMfbm(alpha=1.5, scale=0.2))
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Intrinsic Embedding Covariance Model

Description

RMintrinsic is a univariate stationary isotropic covariance model which depends on a univariate stationary isotropic covariance model.

The corresponding covariance function C of the model only depends on the distance r0r \ge 0 between two points and is given by

C(r)=a0+a2r2+ϕ(r),0rdiameterC(r)=a_0 + a_2 r^2 + \phi(r), 0\le r \le diameter

C(r)=b0(rawRDr)3/(r),diameterrrawRdiameterC(r)=b_0 (rawR D - r)^3/(r), diameter \le r \le rawR * diameter

C(r)=0,rawRdiameterrC(r) = 0, rawR * diameter \le r

Usage

RMintrinsic(phi, diameter, rawR, var, scale, Aniso, proj)

Arguments

phi

an RMmodel; has to be stationary and isotropic

diameter

a numerical value; positive; should be the diameter of the domain on which simulation is done

rawR

a numerical value; greater or equal to 1

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The parameters a0a_0, a2a_2 and b0b_0 are chosen internally such that CC becomes a smooth function. See formulas (3.8)-(3.10) in Gneiting et alii (2006). This model corresponds to the method Intrinsic Embedding. See also RPintrinsic.

NOTE: The algorithm that checks the given parameters knows only about some few necessary conditions. Hence it is not ensured that the Stein-model is a valid covariance function for any choice of ϕ\phi and the parameters.

For certain models ϕ\phi, i.e. stable, whittle, gencauchy, and the variogram model fractalB some sufficient conditions are known.

Value

RMintrinsic returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Sevecikova, H, Percival, D.B., Schlather M., Jiang Y. (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in $R^2$: Exploring the Limits. J. Comput. Graph. Stat. 15, 483–501.

  • Stein, M.L. (2002) Fast and exact simulation of fractional Brownian surfaces. J. Comput. Graph. Statist. 11, 587–599

See Also

RPintrinsic, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x.max <- 10
model <- RMintrinsic(RMfbm(alpha=1), diameter=x.max)
x <- seq(0, x.max, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Identical Model

Description

RMkolmogorov corresponds to a vector-valued random field with covariance function

γij(h)=h2/3(43δij13hihjh2)\gamma_{ij}(h) = \|h\|^{2/3}\left(\frac43 \delta_{ij} - \frac13\frac{h_ih_j}{\|h\|^2}\right)

Usage

RMkolmogorov(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMkolmogorov returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

The above formula is from eq. (6.32) of section 6.2 in

Pope, S.B. (2000) Turbulent Flows. Cambridge: Cambridge University Pess.

See Also

RMmodel, RMcurlfree, RMdivfree, RMvector.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- y <- seq(-2, 2, len=20)
model <- RMkolmogorov()
plot(model, dim=3, MARGIN=1:2, fixed.MARGIN=1)

simu <- RFsimulate(model, x, y, z=0)
plot(simu, select.variables=list(c(1,2)), col=c("red"))

Local-Global Distinguisher Family Covariance Model

Description

RMlgd is a stationary isotropic covariance model, which is valid only for dimensions d=1,2d =1,2. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=1β1(α+β)rα1[0,1](r)+α1(α+β)rβ1r>1(r)C(r) =1 - \beta^{-1}(\alpha + \beta)r^{\alpha} 1_{[0,1]}(r) + \alpha^{-1}(\alpha + \beta)r^{-\beta} 1_{r>1}(r)

where β>0\beta >0 and 0<α(3d)/20 < \alpha \le (3-d)/2, with dd denoting the dimension of the random field.

Usage

RMlgd(alpha, beta, var, scale, Aniso, proj)

Arguments

alpha

argument whose range depends on the dimension of the random field: 0<α(3d)/20< \alpha \le (3-d)/2.

beta

positive number

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimension d=1,2d=1,2.

This model admits simulating random fields where fractal dimension D of the Gaussian sample and Hurst coefficient H can be chosen independently (compare also RMgencauchy):

Here, the random field has fractal dimension

D=d+1α/2D = d+1 - \alpha/2

and Hurst coefficient

H=1β/2H = 1-\beta/2

for 0<β10< \beta \le 1.

Value

RMlgd returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. and Schlather, M. (2004) Stochastic models which separate fractal dimension and Hurst effect. SIAM review 46, 269–282.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMlgd(alpha=0.7, beta=4, scale=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Locally Positive Definite Function Given by the Fractal Brownian Motion

Description

RMlsfbm is a positive definite function on the unit ball in RdR^d centred at the origin,

C(r)=crαC(r) = c - r^\alpha

with r=xy[0,1]r = \|x- y\|\in [0,1].

Usage

RMlsfbm(alpha, const, var, scale, Aniso, proj)

Arguments

alpha

numeric in (0,2)(0,2); refers to the fractal dimension of the process.

const

the constant cc is given by the formula

c=2αΓ(d/2+α/2)Γ(1α/2)/Γ(d/2)c = 2^{-\alpha} \Gamma(d / 2 + \alpha/2) \Gamma(1 - \alpha/2) / \Gamma(d / 2)

and should not be changed by the user in order to ensure positive definiteness.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMlsfbm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Martini, J., Schlather, M., Simianer, H. (In preparation.)

See Also

RMbcw generalizes RMlsfbm in case that cc is given, RMfbm, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMlsfbm(alpha=1, scale=10)
x <- seq(0, 10, 0.02)
plot(model, xlim=c(0,10))
plot(RFsimulate(model, x=x))

Ma operator

Description

RMma is a univariate stationary covariance model depending on a univariate stationary covariance model. The corresponding covariance function only depends on the difference hh between two points and is given by

C(h)=(θ/(1(1θ)ϕ(h)))αC(h) = (\theta / (1 - (1-\theta) \phi(h)))^\alpha

Usage

RMma(phi, alpha, theta, var, scale, Aniso, proj)

Arguments

phi

a stationary covariance RMmodel.

alpha

a numerical value; positive

theta

a numerical value; in the interval (0,1)(0,1)

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMma returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Ma, C. (2003) Spatio-temporal covariance functions generated by mixtures. Math. Geol., 34, 965-975.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMma(RMgauss(), alpha=4, theta=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Ma-Stein operator

Description

RMmastein is a univariate stationary covariance model depending on a variogram or covariance model on the real axis. The corresponding covariance function only depends on the difference hh between two points and is given by

C(h,t)=Γ(ν+ϕ(t))Γ(ν+δ)Γ(ν+ϕ(t)+δ)Γ(ν)Wν+ϕ(t)(hVt)C(h, t)=\frac{\Gamma(\nu + \phi(t))\Gamma(\nu + \delta)}{ \Gamma(\nu + \phi(t) + \delta) \Gamma(\nu)} W_{\nu + \phi(t)}(\|h -Vt\|)

if ϕ\phi is a variogram model. It is given by

C(h,t)=Γ(ν+ϕ(0)ϕ(t))Γ(ν+δ)Γ(ν+ϕ(0)ϕ(t)+δ)Γ(ν)Wν+ϕ(t)(hVt)C(h, t)=\frac{\Gamma(\nu + \phi(0)-\phi(t))\Gamma(\nu + \delta)}{ \Gamma(\nu + \phi(0)-\phi(t) + \delta) \Gamma(\nu)} W_{\nu + \phi(t)}(\|h -Vt\|)

if ϕ\phi is a covariance model.

Here Γ\Gamma is the Gamma function; WW is the Whittle-Matern model (RMwhittle).

Usage

RMmastein(phi, nu, delta, var, scale, Aniso, proj)

Arguments

phi

an RMmodel on the real axis

nu

numerical value; positive; smoothness parameter of the Whittle-Matern model (for t=0t=0)

delta

a numerical value; δ\delta must be greater than or equal to half the dimension of hh

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

See Stein (2005), formula (12).

Instead of the velocity parameter VV in the original model description, a preceding anisotropy matrix is chosen appropriately:

(AV01)\left( \begin{array}{cc} A & -V \\ 0 & 1\end{array}\right)

A is a spatial transformation matrix. (I.e. (x,t) is multiplied from the left on the above matrix and the first elements of the obtained vector are interpreted as new spatial components and only these components are used to form the argument in the Whittle-Matern function.) The last component in the new coordinates is the time which is passed to ϕ\phi. (Velocity is assumed to be zero in the new coordinates.)

Note, that for numerical reasons, ν+ϕ+d\nu+\phi+d may not exceed the value 80.0. If exceeded the algorithm fails.

Value

RMmastein returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Ma, C. (2003) Spatio-temporal covariance functions generated by mixtures. Math. Geol., 34, 965-975.

  • Stein, M.L. (2005) Space-time covariance functions. JASA, 100, 310-321.

See Also

RMwhittle, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make plotthem all random again
model <- RMmastein(RMgauss(), nu=1, delta=10)
plot(RMexp(), model.mastein=model, dim=2)

x <- seq(0, 10, 0.1)
plot(RFsimulate(model, x=x, y=x))

Matrix operator

Description

RMmatrix is a multivariate covariance model depending on one multivariate covariance model, or one or several univariate covariance models C0,C0,\ldots. The corresponding covariance function is given by

C(h)=Mϕ(h)MtC(h) = M \phi(h) M^t

if a multivariate case is given. Otherwise it returns a matrix whose diagonal elements are filled with the univarate model(s) C0, C1, etc, and the offdiagonals are all zero.

Usage

RMmatrix(C0, C1,  C2, C3, C4, C5, C6, C7, C8, C9, M, vdim,
         var, scale, Aniso, proj)

Arguments

C0

a k-variate covariance RMmodel or a univariate model or a list of models joined by c

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional univariate models

M

a k times k matrix, which is multiplied from left and right to the given model; MM may depend on the location, hence it is then a matrix-valued function and CC will be non-stationary with

C(x,y)=M(x)ϕ(x,y)M(y)tC(x, y) = M(x) \phi(x, y) M(y)^t

vdim

positive integer. This argument should be given if and only if a multivariate model is created from a single univariate model and M is not given. (In fact, if M is given, vdim must equal the number of columns of M)

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMmatrix returns an object of class RMmodel.

Note

  • RMmatrix also allows variogram models are arguments.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


## Not run: 
## first example: bivariate Linear Model of Coregionalisation
x <- y <- seq(0, 10, 0.2)

model1 <- RMmatrix(M = c(0.9, 0.43), RMwhittle(nu = 0.3)) + 
  RMmatrix(M = c(0.6, 0.8), RMwhittle(nu = 2))
plot(model1)
simu1 <- RFsimulate(RPdirect(model1), x, y)
plot(simu1)


## second, equivalent way of defining the above model
model2 <- RMmatrix(M = matrix(ncol=2, c(0.9, 0.43, 0.6, 0.8)),
                  c(RMwhittle(nu = 0.3), RMwhittle(nu = 2)))
simu2 <- RFsimulate(RPdirect(model2), x, y)
stopifnot(all.equal(as.array(simu1), as.array(simu2)))


## third, equivalent way of defining the above model
model3 <- RMmatrix(M = matrix(ncol=2, c(0.9, 0.43, 0.6, 0.8)),
                   RMwhittle(nu = 0.3), RMwhittle(nu = 2))
simu3 <- RFsimulate(RPdirect(model3), x, y)
stopifnot(all(as.array(simu3) == as.array(simu2)))

## End(Not run)


## second example: bivariate, independent fractional Brownian motion
## on the real axis
x <- seq(0, 10, 0.1) 
modelB <- RMmatrix(c(RMfbm(alpha=0.5), RMfbm(alpha=1.5))) ## see the Note above
print(modelB)
simuB <- RFsimulate(modelB, x)
plot(simuB)


## third example: bivariate non-stationary field with exponential correlation
## function. The variance of the two components is given by the
## variogram of fractional Brownian motions.
## Note that the two components have correlation 1.
x <- seq(0, 10, 0.1)
modelC <- RMmatrix(RMexp(), M=c(RMfbm(alpha=0.5), RMfbm(alpha=1.5))) 
print(modelC)
simuC <- RFsimulate(modelC, x, x, print=1)
#print(as.vector(simuC))
plot(simuC)

Covariance and Variogram Models in RandomFields (RM commands)

Description

Summary of implemented covariance and variogram models

Details

To generate a covariance or variogram model for use within RandomFields, calls of the form

RMname(...,var,scale,Aniso,proj)RM_name_(..., var, scale, Aniso, proj)

can be used, where _name_ has to be replaced by a valid model name.

  • ... can take model specific arguments.

  • var is the optional variance argument vv,

  • scale the optional scale argument ss,

  • Aniso an optional anisotropy matrix AA or given by RMangle, and

  • proj is the optional projection.

With ϕ\phi denoting the original model, the transformed model is C(h)=vϕ(Ah/s)C(h) = v * \phi(A*h/s). See RMS for more details.

RM_name_ must be a function of class RMmodelgenerator. The return value of all functions RM_name_ is of class RMmodel.

The following models are available (cf. RFgetModelNames):

Basic stationary and isotropic models

RMcauchy Cauchy family
RMexp exponential model
RMgencauchy generalized Cauchy family
RMgauss Gaussian model
RMgneiting differentiable model with compact support
RMmatern Whittle-Matern model
RMnugget nugget effect model
RMspheric spherical model
RMstable symmetric stable family or powered exponential model
RMwhittle Whittle-Matern model, alternative parametrization

Variogram models (stationary increments/intrinsically stationary)

RMfbm fractal Brownian motion

Basic Operations

RMmult, * product of covariance models
RMplus, + sum of covariance models or variograms

Others

RMtrend trend
RMangle defines a 2x2 anisotropy matrix by rotation and stretch arguments.

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

  • Yaglom, A.M. (1987) Correlation Theory of Stationary and Related Random Functions I, Basic Results. New York: Springer.

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3nd edition.

See Also

RM for an overview over more advanced classes of models
RC, RF, RP, RR, R., RFcov, RFformula, RMmodelsAdvanced, RMmodelsAuxiliary, trend modelling

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## an example of a simple model
model <- RMexp(var=1.6, scale=0.5) + RMnugget(var=0) #exponential + nugget
plot(model)

Class RMmodel

Description

Class for RandomFields' representation of explicit covariance models

Usage

RFplotModel(x, y, dim=1,
           n.points=if (dim==1 || is.contour) 200 else 100,
           fct.type=NULL, MARGIN, fixed.MARGIN, maxchar=15, ...,
           plotmethod=if (dim==1) "matplot" else "contour")

## S4 method for signature 'RMmodel,missing'
plot(x, y, ...)
## S4 method for signature 'RMmodel'
points(x, ..., type="p")
## S4 method for signature 'RMmodel'
lines(x, ..., type="l")
## S4 method for signature 'RMmodel'
image(x, ..., dim=2)
## S4 method for signature 'RMmodel'
persp(x, ..., dim=2, zlab="")

Arguments

x

object of class RFsp or RFempVario or RFfit or RMmodel; in the latter case, x can be any sophisticated model but it must be either stationary or a variogram model.

y

ignored in most methods

MARGIN

vector of two; two integer values giving the coordinate dimensions w.r.t. whether the field or the covariance model is to be plotted; in all other directions, the first index is taken.

fixed.MARGIN

only for class(x)==CLASS_CLIST and if dim > 2; a vector of length dim-2 with distance values for the coordinates that are not displayed.

maxchar

integer. Maximum number of characters to print the model in the legend.

...

arguments to be passed to methods; mainly graphical arguments, or further models in case of class CLASS_CLIST, see Details.

dim

must equal 1 or 2; only for class(x)==CLASS_CLIST; the covariance function and the variogram are plotted as a function of Rdim\R^\code{dim}.

n.points

integer; only for class(x)==CLASS_CLIST; the number of points at which the model is evaluated (in each dimension); defaults to 200.

fct.type

character; only for class(x)==CLASS_CLIST; must equal NULL, "Cov" or "Variogram"; controls whether the covariance (fct.type="Cov") or the variogram (fct.type="Variogram") is plotted; NULL implies automatic choice, where "Cov" is chosen whenever the model is stationary.

plotmethod

string or function. Internal.

type

character. See points.

zlab

character. See persp.

Value

If RFoptions()$split_screen=TRUE and RFoptions()$close_screen=TRUE then the plot functions return the screen numbers. Else NULL.

Creating Objects

Objects are created by calling a function of class RMmodelgenerator.

Slots

call:

language object; the function call by which the object was generated

name:

character string; nickname of the model, name of the function by which the object was generated

submodels:

list; contains submodels (if existent)

par.model:

list; contains model specific arguments

par.general:

list of 4; contains the four standard arguments var, scale, Aniso and proj that can be given for any model; if not specified by the user, the string "RFdefault" is inserted

Methods

+

signature(x = CLASS_CLIST): allows to sum up covariance models; internally calls RMplus.

-

signature(x = CLASS_CLIST): allows to substract covariance models; internally calls R.minus.

*

signature(x = CLASS_CLIST): allows to multiply covariance models; internally calls R.mult.

/

signature(x = CLASS_CLIST): allows to divide covariance models; internally calls R.div.

c

signature(x = CLASS_CLIST): concatenates covariance functions or variogram models.

plot

signature(x = CLASS_CLIST): gives a plot of the covariance function or of the variogram model; for more details see plot-method.

points

signature(x = CLASS_CLIST): adds a covariance plot to an existing plot; for more details see plot-method.

lines

signature(x = CLASS_CLIST): adds a covariance plot to an existing plot; for more details see plot-method.

str

signature(x = CLASS_CLIST): as the usual str-method for S4 objects but only those entries of the 'par.general'-slot are shown that contain values different from 'RFdefault'.

show

signature(x = CLASS_CLIST): returns the structure of x.

print

signature(x = CLASS_CLIST): identical with show-method, additional argument is max.level.

[

signature(x = CLASS_CLIST): enables accessing the slots via the "["-operator, e.g. x["par.general"].

[<-

signature(x = CLASS_CLIST): enables replacing the slots via the "["-operator.

signature(x = CLASS_CLIST, y = "missing")

Generates covariance function or variogram function plots in one or two dimensions.

Details

All the above arguments apply for all the S3 and S4 functions given here as they call RFplotModel immediately.

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodelgenerator RMmodel

Examples

# see RMmodel for introductory examples


# Compare:
model <- RMexp(scale=2) + RMnugget(var=3)
str(model)  ## S4 object as default in version 3 of RandomFields

model <- summary(model)
str(model)  ## list style as in version 2 of RandomFields
            ## see also 'spConform' in 'RFoptions' to make this style
            ## the default

Class CLASS_FIT

Description

Extension of class RMmodel which additionally contains the likelihood of the data w.r.t. the covariance model represented by the CLASS_CLIST part, the estimated trend of the data if it is a constant trend, and the residuals of the data w.r.t. the model. Objects of this class only occur as slots in the output of "RFfit".

Creating Objects

Objects are only meant to be created by the function RFfit.

Slots

model,formel:

See RMmodel.

variab:

vector of estimated variables. Variables are used in the internal representation and can be a subset of the parameters.

param:

vector of estimated parameters

covariate:

to do

globalvariance:

to do

hessian:

to do

likelihood:

numeric; the likelihood of the data w.r.t. the covariance model

AIC:

the AIC value for the ml estimation

AICc:

the corrected AIC value for the ml estimation

BIC:

the BIC value for the ml estimation

residuals:

array or of class RFsp; residuals of the data w.r.t. the trend model

Extends

Class CLASS_CLIST, directly.

Methods

[

signature(x = CLASS_FIT): enables accessing the slots via the "["-operator, e.g. x["likelihood"]

[<-

signature(x = CLASS_FIT): enables replacing the slots via the "["-operator

show

signature(x = "RFfit"): returns the structure of x

print

signature(x = "RFfit"): identical with show-method

anova

performs a likelihood ratio test base on a chisq approximation

summary

gives a summary

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFfit.

Examples

# see RFfit

Class RMmodelgenerator

Description

Class for all functions of this package with prefix RM, i.e. all functions that generate objects of class RMmodel; direct extension of class function.

Creating Objects

Objects should not be created by the user!

Slots

.Data:

function; the genuine function that generates an object of class RMmodel

type:

character string; specifies the category of RMmodel-function, see Details

domain:

character string; specifies whether the corresponding function(s) depend on 1 or 2 variables, see Details

isotropy:

character string; specifies the type of isotropy of the corresponding covariance model, see Details

operator:

logical; specifies whether the underlying covariance model is an operator, see Details

monotone:

character string; specifies the kind of monotonicity of the model

finiterange:

logical; specifies whether the underlying covariance model has finite range, see Details

simpleArguments:

logical. If TRUE than all the parameters are real valued (or integer valued).

maxdim:

numeric; the maximal dimension, in which the corresponding model is a valid covariance model, see Details

vdim:

numeric; dimension of the value of the random field at a single fixed location, equals 1 in most cases, see Details

Extends

Class function, directly.

Methods

show

signature(x = CLASS_CLIST): returns the structure of x

print

signature(x = CLASS_CLIST): identical with show-method

[

signature(x = CLASS_RM): enables accessing the slots via the "["-operator, e.g. x["maxdim"]

[<-

signature(x = CLASS_RM): enables replacing the slots via the "["-operator

Details

type:

can be one of the following strings:

'tail correlation function':

indicates that the function returns a tail correlation function (a subclass of the set of positive definite functions)

'positive definite':

indicates that the function returns a covariance function (positive definite function)

'negative definite':

indicates that the function returns a variogram model (negative definite function)

'process':

functions of that type determine the class of processes to be simulated

'method for Gauss processes':

methods to simulate Gaussian random fields

'method for Brown-Resnick processes':

methods to simulate Brown-Resnick fields

'point-shape function':

functions of that type determine the distribution of points in space

'distribution family':

e.g. (multivariate) uniform distribution, normal distribution, etc., defined in RandomFields. See RR for a complete list.

'shape function':

functions used in, e.g., M3 processes (RPsmith)

'trend':

RMtrend or a mixed model

'interface':

indicates internal models which are usually not visible for the users. These functions are the internal representations of RFsimulate, RFcov, etc. See RF for a complete list.

'undefined':

some models can take different types, depending on the parameter values and/or the submodels

'other type':

very very special internal functions, not belonging to any of the above types.

domain:

can be one of the following strings:

'single variable':

Function depending on a single variable

'kernel':

model refers to a kernel, e.g. a non-stationary covariance function

'framework dependent':

domain depends on the calling model

'mismatch':

this option is used only internally and should never appear

isotropy:

can be one of the following strings:

'isotropic':

indicates that the model is isotropic

'space-isotropic':

indicates that the spatial part of a spatio-temporal model is isotropic

'zero-space-isotropic':

this property refers to space-time models; the model is called zerospaceisotropic if it is isotropic as soon as the time-component is zero

'vector-isotropic':

multivariate vector model (flow fields) have a different notion of isotropy

'symmetric':

the most basic property of any covariance function or variogram model

'cartesian system', 'earth system', 'spherical system', 'cylinder system':

different coordinate systems

'non-dimension-reducing':

the property f(x)=f(x)f(x) = f(-x)^\top does not hold

'parameter dependent':

indicates that the type of isotropy of the model depends on the parameters passed to the model; in particular parameters may be submodels if an operator model is considered

'<mismatch>':

this option is used only internally and should never appear

operator:

if TRUE, the model requires at least one submodel

monotone:
'mismatch in monotonicity':

used if a statement on the monotonocity does not make sense, e.g. for RRmodels

'submodel dependent monotonicity':

only for operators, e.g. RMS

'previous model dependent monotonicity':

internal; should not be used

'parameter dependent monotonicity':

some models change their properties according to the parameters

'not monotone':

none of the above categories; either the function is not monotone or properties are unknown

'monotone':

isotone or antitone

'Gneiting-Schaback class':

function belonging to Euclid's hat in Gneiting's 1999 paper

'normal mixture':

scale mixture of the Gaussian model

'completely monotone':

completely monotone function

'Bernstein':

Bernstein function

Note that

  • 'not monotone' includes 'monotone' and 'Bernstein'

  • 'monotone' includes 'Gneiting-Schaback class'

  • 'Gneiting-Schaback class' includes 'normal mixture'

  • 'normal mixture' includes 'completely monotone'

finiterange:

if TRUE, the covariance of the model has finite range

maxdim:

if a positive integer, maxdim gives the maximum dimension in which the model is a valid covariance model, can be Inf; maxdim=-1 means that the actual maxdim depends on the parameters; maxdim=-2 means that the actual maxdim depends on the submodel(s)

vdim:

if a positive integer, vdim gives the dimension of the random field, i.e. univariate, bi-variate, ...; vdim=-1 means that the actual vdim depends on the parameters; vdim=-2 means that the actual vdim depends on the submodel(s)

Author(s)

Alexander Malinowski, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (1999) Radial positive definite functions generated by Euclid's hat, J. Multivariate Anal., 69, 88-119.

See Also

RMmodel, RFgetModelNames

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
RFgetModelNames()

Overview over classes of RMmodels

Description

Various classes of models RMxxx are implemented in RandomFields, that have their own man pages. Here, an overview over these man pages are given.

Man pages

Beginners should start with RMmodels, then go for RMmodelsAdvanced if more information is needed.

RMmodels general introduction and a collection of simple models
RMmodelsAdvanced includes more advanced stationary and isotropic models, variogram models, non-stationary models and trend models
Bayesian hierarchical models
RMmodelsMultivariate multivariate covariance models and multivariate trend models
RMmodelsNonstationary non-stationary covariance models
RMmodelsSpaceTime space-time covariance models
Spherical models models based on the polar coordinate system, usually used in earth models
Tail correlation functions models related to max-stable random fields
trend modelling how to pass trend specifications
Mathematical functions simple mathematical functions that are typically used to build non-stationary covariance models and arbitrary trends
RMmodelsAuxiliary rather specialized models, most of them not having positive definiteness property, but used internally in certain simulation algorithms, for instance.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RC, RR, RF, R.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFgetModelNames(type="positive definite", domain="single variable",
                isotropy="isotropic", operator=!FALSE) ## RMmodel.Rd

Advanced features of the models

Description

Here, further models and advanced comments for RMmodel are given. See also RFgetModelNames.

Details

Further stationary and isotropic models

RMaskey Askey model (generalized test or triangle model)
RMbcw bridging model between RMcauchy and RMgenfbm
RMbessel Bessel family
RMcircular circular model
RMconstant spatially constant model
RMcubic cubic model (see Chiles and Delfiner)
RMdagum Dagum model
RMdampedcos exponentially damped cosine
RMqexp variant of the exponential model
RMfractdiff fractionally differenced process
RMfractgauss fractional Gaussian noise
RMgengneiting generalized Gneiting model
RMgneitingdiff Gneiting model for tapering
RMhyperbolic generalized hyperbolic model
RMlgd Gneiting's local-global distinguisher
RMlsfbm locally stationary fractal Brownian motion
RMpenta penta model (see Chiles and Delfiner)
RMpower Golubov's model
RMwave cardinal sine

Variogram models (stationary increments/intrinsically stationary)

RMbcw bridging model between RMcauchy and RMgenfbm
RMdewijsian generalized version of the DeWijsian model
RMgenfbm generalized fractal Brownian motion
RMflatpower similar to fractal Brownian motion but always smooth at the origin

General composed models (operators)

Here, composed models are given that can be of any kind (stationary/non-stationary), depending on the submodel.

RMbernoulli Correlation function of a binary field based on a Gaussian field
RMexponential exponential of a covariance model
RMintexp integrated exponential of a covariance model (INCLUDES ma2)
RMpower powered variograms
RMqam Porcu's quasi-arithmetic-mean model
RMS details on the optional transformation arguments (var, scale, Aniso, proj)

Stationary and isotropic composed models (operators)

RMcutoff Gneiting's modification towards finite range
RMintrinsic Stein's modification towards finite range
RMnatsc practical range
RMstein Stein's modification towards finite range
RMtbm Turning bands operator

Stationary space-time models
See RMmodelsSpaceTime.

Non-stationary models
See RMmodelsNonstationary.

Negative definite models that are not variograms

RMsum a non-stationary variogram model

Models related to max-stable random fields (tail correlation functions)
See RMmodelsTailCorrelation.

Other covariance models

RMcov covariance structure given by a variogram
RMfixcov User defined covariance structure
RMuser User defined model

Trend models

Aniso for space transformation (not really trend, but similar)
RMcovariate spatial covariates
RMprod to model variability of the variance
RMpolynome easy modelling of polynomial trends
RMtrend for explicit trend modelling
R.models for implicit trend modelling
R.c for multivariate trend modelling

Auxiliary models
See Auxiliary RMmodels.

Note

  • Note that, instead of the named arguments, a single argument k can be passed. This is possible if all the arguments are scalar. Then k must have a length equal to the number of arguments.

  • If an argument equals NULL the argument is not set (but must have a valid name).

  • Aniso can be given also by RMangle or any other RMmodel instead of a matrix

  • Note also that a completely different possibility exists to define a model, namely by a list. This format allows for easy flexible models and modifications (and some few more options, as well as some abbreviations to the model names, see PrintModelList()). Here, the argument var, scale, Aniso and proj must be passed by the model RMS. For instance,

    • model <- RMexp(scale=2, var=5)
      is equivalent to
      model <- list("RMS", scale=2, var=5, list("RMexp"))
      The latter definition can be also obtained by

      print(RMexp(scale=2, var=5))

    • model <- RMnsst(phi=RMgauss(var=7), psi=RMfbm(alpha=1.5), scale=2, var=5)
      is equivalent to
      model <- list("RMS", scale=2, var=5,
      list("RMnsst", phi=list("RMS", var=7, list("RMgauss")),
      psi=list("RMfbm", alpha=1.5)) ).

    All models have secondary names that stem from RandomFields versions 2 and earlier and that can also be used as strings in the list notation. See RFgetModelNames(internal=FALSE) for the full list.

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

  • Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’

    multivariate’, the corresponding vignette.

  • Yaglom, A.M. (1987) Correlation Theory of Stationary and Related Random Functions I, Basic Results. New York: Springer.

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3nd edition.

See Also

RFformula, RM, RMmodels, RMmodelsAuxiliary.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## a non-stationary field with a sharp boundary
## of the differentiabilities
x <- seq(-0.6, 0.6, len=50)
model <- RMwhittle(nu=0.8 + 1.5 * R.is(R.p(new="isotropic"), "<=", 0.5))
z <- RFsimulate(model=model, x, x, n=4)
plot(z)

Multivariate models

Description

Here, multivariate and vector-valued covariance models are presented.

Details

Bivariate covariance models

RMbicauchy a bivariate Cauchy model
RMbiwm full bivariate Whittle-Matern model (stationary and isotropic)
RMbigneiting bivariate Gneiting model (stationary and isotropic)
RMbistable a bivariate stable model

Physically motivated, vector valued covariance and variogram models

RMcurlfree curlfree (spatial) vector-valued field (stationary and anisotropic)
RMdivfree divergence free (spatial) vector-valued field (stationary and anisotropic)
RMkolmogorov Kolmogorov's model of turbulence
RMvector vector-valued field (combining RMcurlfree and RMdivfree)

Multivariate covariance models

RMdelay delay effect model (stationary)
RMderiv field and its gradient
RMmatrix linear model of coregionalization
RMparswm multivariate Whittle-Matern model (stationary and isotropic)

Operators

RMcov covariance structure given by a multivariate variogram
RMexponential functional returning eCe^C
RMmatrix linear model of coregionalization
RMmqam multivariate quasi-arithmetic mean (stationary)
RMschur element-wise product with a positive definite matrix
RMtbm turning bands operator

Trend models

RMtrend for explicit trend modelling
R.models for implicit trend modelling
R.c binding univariate trend models into a vector

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

  • Schlather, M., Malinowski, A., Menck, P.J., Oesting, M. and Strokorb, K. (2015) Analysis, simulation and prediction of multivariate random fields with package RandomFields. Journal of Statistical Software, 63 (8), 1-25, url = ‘http://www.jstatsoft.org/v63/i08/’

  • Wackernagel, H. (2003) Multivariate Geostatistics. Berlin: Springer, 3rd edition.

See Also

RFformula, RMmodels, RM, RMmodelsAdvanced

multivariate’, a vignette for multivariate geostatistics

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

n <- 100
x <- runif(n=n, min=1, max=50)
y <- runif(n=n, min=1, max=50)

rho <- matrix(nc=2, c(1, -0.8, -0.8, 1))
model <- RMparswmX(nudiag=c(0.5, 0.5), rho=rho)

## generation of artifical data
dta <- RFsimulate(model = model, x=x, y=y, grid=FALSE)

## introducing some NAs ...
dta@data$variable1[1:10] <- NA
if (interactive()) dta@data$variable2[90:100] <- NA

plot(dta)

## co-kriging
x <- y <- seq(0, 50, 1)

k <- RFinterpolate(model, x=x, y=y, data= dta)
plot(k, dta)

## conditional simulation
z <- RFsimulate(model, x=x, y=y, data= dta) ## takes a while
plot(z, dta)

Non-stationary features of the models

Description

Here, non-stationary covariance models are presented.

Details

Covariance models

RMnonstwm one of Stein's non-stationary Whittle-Matern models
RMprod scalar product
Aniso for space transformation, see the example in R.models.
scale, cf. RMS, can be any non-negative function for any scale mixture model, such as the whittle-matern-classes, the powered exponential family, and the RMgencauchy model.

Trend models See RMmodelsTrend.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFformula, RMmodels, RM, RMmodelsAdvanced

nonstationary’, a vignette for non-stationary geostatistics

Examples

# to do

Space-time Covariance Models

Description

Here, a collection of implemented space-time models is given.

Details

Stationary space-time models

Here, most of the models are composed models (operators). Note that in space-time modelling the argument proj may also take the values "space" for the projection on the space and "time" for the projection onto the time axis.

separable models are easily constructed using +, *, and proj, see also the example below
RMave space-time moving average model
RMcoxisham Cox-Isham model
RMcurlfree curlfree (spatial) field (stationary and anisotropic)
RMdivfree divergence free (spatial) vector-valued field (stationary and anisotropic)
RMgennsst generalization of Gneiting's non-separable space-time model
RMiaco non-separable space-time model
RMmastein Ma-Stein model
RMnsst Gneiting's non-separable space-time model
RMstein Stein's non-separable space-time model
RMstp Single temporal process
RMtbm Turning bands operator

Author(s)

Alexander Malinowski; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

See Also

RFformula, RM, RMmodels, RMmodelsAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## multiplicative separable model with exponential model in space
## and Gaussian in time
model <- RMexp(proj = "space") * RMgauss(proj = "time")
x <- T <- seq(0, 10, 0.1)
z <- RFsimulate(model, x=x, T=T)
plot(z)

## additive separable model with exponential model in space
## and Gaussian in time. The structure is getting rather simple,
## see the function stopifnot below
model <- RMexp(proj = "space") + RMgauss(proj = "time")
x <- T <- seq(0, 10, 0.1)
z <- RFsimulate(model, x=x, T=T)
stopifnot(sum(abs(apply(apply(z, 1, diff), 1, diff))) < 1e-14)
plot(z)

Mixture of shape functions

Description

RMmppplus is a multivariate covariance model which depends on up to 10 submodels C0,C1,...,C9C_0, C_1, ..., C_9.

Used together with RPsmith, it allows for mixed moving maxima with a finite number of shape functions.

Usage

RMmppplus(C0, C1, C2, C3, C4, C5, C6, C7, C8, C9, p)

Arguments

C0

an RMmodel

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional; each an RMmodel

p

vector of probabilities for the shape functions. The probabilities should add up to 1. The length of the vector equals the number of given submodels.

Value

RMmppplus returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMplus, RMmodel, RFsimulate, RFfit, RPsmith.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

multivariate quasi-arithmetic mean

Description

RMmqam is a multivariate stationary covariance model depending on a submodel ϕ\phi such that ψ():=ϕ(())\psi(\cdot) := \phi(\sqrt(\cdot)) is completely monotone, and depending on further stationary covariance models CiC_i. The covariance is given by

Cij(h)=ϕ((θi(ϕ1(Ci(h)))2+θj(ϕ1(Cj(h)))2))C_{ij}(h) = \phi(\sqrt(\theta_i (\phi^{-1}(C_i(h)))^2 + \theta_j (\phi^{-1}(C_j(h)))^2 ))

where ϕ\phi is a completely monotone function, CiC_i are suitable covariance functions and θi0\theta_i\ge0 such that iθi=1\sum_i \theta_i=1.

Usage

RMmqam(phi, C1, C2, C3, C4, C5, C6, C7, C8, C9, theta, var, scale, Aniso, proj)

Arguments

phi

a valid covariance RMmodel that is a normal scale mixture. See, for instance,
RFgetModelNames(monotone="normal mixture")

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional further stationary RMmodels

theta

is a vector of values in [0,1][0,1], summing up to 11.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Note that ψ():=ϕ(())\psi(\cdot) := \phi(\sqrt(\cdot)) is completely monotone if and only if ϕ\phi is a valid covariance function for all dimensions, e.g. RMstable, RMgauss, RMexponential.

Warning: RandomFields cannot check whether the combination of ϕ\phi and CiC_i is valid.

Value

RMmqam returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Porcu, E., Mateu, J. & Christakos, G. (2009) Quasi-arithmetic means of covariance functions with potential applications to space-time data. Journal of Multivariate Analysis, 100, 1830–1844.

See Also

RMqam, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions(modus_operandi="sloppy")
model <- RMmqam(phi=RMgauss(),RMgauss(),RMexp(),theta=c(0.4, 0.6), scale=0.5)
x <- seq(0, 10, 0.02)
plot(model)
z <- RFsimulate(model=model, x=x)
plot(z)

RFoptions(modus_operandi="normal")

Multiplication of Random Field Models

Description

RMmult is a multivariate covariance model which depends on up to 10 submodels C0,C1,...,C9C_0, C_1, ..., C_9. In general, realizations of the created RMmodel are pointwise products of independent realizations of the submodels.

In particular, if all submodels are given through a covariance function, the resulting model is defined through its covariance function, which is the product of the submodels' covariances.

Usage

RMmult(C0, C1, C2, C3, C4, C5, C6, C7, C8, C9, var, scale, Aniso, proj)

Arguments

C0

an RMmodel.

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional; each an RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above model remains unmodified.

Details

RMmodels can also be multiplied via the *-operator, e.g. C0 * C1.

The global arguments scale,Aniso,proj of RMmult are multiplied to the corresponding argument of the submodels (from the right side). E.g.,
RMmult(Aniso=A1, RMexp(Aniso=A2), RMspheric(Aniso=A3))
equals
RMexp(Aniso=A2 %*% A1) * RMspheric(Aniso=A3 %*% A1)

In case that all submodels are given through a covariance function, the global argument var of RMmult is multiplied to the product covariance of RMmult.

Value

RMmult returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMplus, RMmodel, RMprod, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

# separable, multiplicative model
model <- RMgauss(proj=1) * RMexp(proj=2, scale=5)
z <- RFsimulate(model=model, 0:10, 0:10, n=4)
plot(z)

The Multiquadric Family Covariance Model on the Sphere

Description

RMmultiquad is an isotropic covariance model. The corresponding covariance function, the multiquadric family, only depends on the angle θ[0,π]\theta \in [0,\pi] between two points on the sphere and is given by

ψ(θ)=(1δ)2τ/(1+delta22δcos(θ))τ\psi(\theta) = (1 - \delta)^{2*\tau} / (1 + delta^2 - 2*\delta*cos(\theta))^{\tau}

where δ(0,1)\delta \in (0,1) and τ>0\tau > 0.

Usage

RMmultiquad(delta, tau, var, scale, Aniso, proj)

Arguments

delta

a numerical value in (0,1)(0,1)

tau

a numerical value greater than 00

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Special cases (cf. Gneiting, T. (2013), p.1333) are known for fixed parameter τ=0.5\tau=0.5 which leads to the covariance function called 'inverse multiquadric'

ψ(θ)=(1δ)/(1+delta22δcos(θ))\psi(\theta) = (1 - \delta) / \sqrt( 1 + delta^2 - 2*\delta*cos(\theta) )

and for fixed parameter τ=1.5\tau=1.5 which gives the covariance function called 'Poisson spline'

ψ(θ)=(1δ)3/(1+delta22δcos(θ))1.5\psi(\theta) = (1 - \delta)^{3} / (1 + delta^2 - 2*\delta*cos(\theta))^{1.5}

For a more general form, see RMchoquet.

Value

RMmultiquad returns an object of class RMmodel.

Author(s)

Christoph Berreth, Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gneiting, T. (2013) Strictly and non-strictly positive definite functions on spheres Bernoulli, 19(4), 1327-1349.

See Also

RMmodel, RFsimulate, RFfit, RMchoquet, spherical models

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions(coord_system="sphere")
model <- RMmultiquad(delta=0.5, tau=1)
plot(model, dim=2)

## the following two pictures are the same
x <- seq(0, 0.12, 0.01)
z1 <- RFsimulate(model, x=x, y=x)
plot(z1)

x2 <- x * 180 / pi
z2 <- RFsimulate(model, x=x2, y=x2, coord_system="earth")
plot(z2)

stopifnot(all.equal(as.array(z1), as.array(z2)))

RFoptions(coord_system="auto")

Natural scale

Description

RMnatsc is a stationary isotropic covariance model that depends on a stationary isotropic covariance model ϕ\phi. The covariance is given by

C(h)=ϕ(h/s)C(h) = \phi(h / s)

where the argument s is chosen by RMnatsc such that the practical range or the mathematical range, if finite, is 1.

Usage

RMnatsc(phi, var, scale, Aniso, proj)

Arguments

phi

a stationary isotropic covariance RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

For internal use only.

Value

RMnatsc returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMnatsc(RMexp())
x <- seq(0, 10, 0.02)
plot(RMexp(), model=model)
RFcov(model, 1)

Non-stationary Whittle-Matern Covariance Model

Description

The non-stationary Whittle-Matern model CC is given by

C(x,y)=Γ(μ)Γ(ν(x))1/2Γ(ν(y))1/2Wμ(xy)C(x, y)=\Gamma(\mu) \Gamma(\nu(x))^{-1/2} \Gamma(\nu(y))^{-1/2} W_{\mu} (|x-y|)

where μ=[ν(x)+ν(y)]/2\mu = [\nu(x) + \nu(y)]/2, and ν\nu must be a positive function.

WμW_{\mu} is the covariance of the RMwhittle model or the RMmatern model.

Details

The non-stationary Whittle-Matern models are obtained by the respective stationary model, replacing the real-valued argument for nu by a non-negative function.

Note

It cannot be checked whether nu only takes positive values. So the responsibility is completely left to the user.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Stein, M. (2005) Nonstationary Spatial Covariance Functions. Tech. Rep., 2005

See Also

RMwhittle, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
x <- seq(-1.2, 1.2, len=50)
model <- RMwhittle(nu=RMgauss())
z <- RFsimulate(model=model, x, x, n=4)
plot(z)

Non-Separable Space-Time model

Description

RMnsst is a univariate stationary spaceisotropic covariance model whose corresponding covariance is given by

C(h,u)=(ψ(u)+1)δ/2ϕ(h/(ψ(u)+1))C(h,u)= (\psi(u)+1)^{-\delta/2} \phi(h /\sqrt(\psi(u) +1))

Usage

RMnsst(phi, psi, delta, var, scale, Aniso, proj)

Arguments

phi

is a normal mixture RMmodel, cf.
RFgetModelNames(monotone="normal mixture")

psi

is a variogram RMmodel.

delta

a numerical value; must be greater than or equal to the spatial dimension of the field.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model is used for space-time modelling where the spatial component is isotropic.

Value

RMnsst returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T. (1997) Normal scale mixtures and dual probability densitites, J. Stat. Comput. Simul. 59, 375-384.

  • Gneiting, T. (2002) Nonseparable, stationary covariance functions for space-time data, JASA 97, 590-600.

  • Gneiting, T. and Schlather, M. (2001) Space-time covariance models. In El-Shaarawi, A.H. and Piegorsch, W.W.: The Encyclopedia of Environmetrics. Chichester: Wiley.

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMgennsst, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMnsst(phi=RMgauss(), psi=RMfbm(alpha=1), delta=2)
x <- seq(0, 10, 0.25)
plot(model, dim=2)
plot(RFsimulate(model, x=x, y=x))

Nugget Effect Covariance Model

Description

RMnugget is a multivariate stationary isotropic covariance model called “nugget effect”. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given for i,ji,j in 1,...,1,...,vdim by

Cij(r)=δij10(r),C_{ij}(r) = \delta_{ij} 1_{0}(r),

where δij=1\delta_{ij}=1 if i=ji=j and δij=0\delta_{ij}=0 otherwise.

Usage

RMnugget(tol, vdim, var, Aniso, proj)

Arguments

tol

Only for advanced users. See RPnugget.

vdim

Must be set only for multivariate models (advanced).

var

optional argument; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Aniso, proj

(zonal modelling and repeated measurements(advanced)); see RPnugget for details.

Details

The nugget effect belongs to Gaussian white noise and is used for modeling measurement errors or to model spatial ‘nuggets’.

Value

RMnugget returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RFsimulate, RFfit, RPnugget (advanced users).

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- y <- 1:2
xy <- as.matrix(expand.grid(x, y)) ## we get 4 locations

## Standard use of the nugget effect
model <- RMnugget(var = 100)
RFcovmatrix(model, x=xy)
as.vector(RFsimulate(model, x=x, y=x, tol=1e-10))

Parsimonious Multivariate Whittle Matern Model

Description

RMparswm is a multivariate stationary isotropic covariance model whose corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given for i,j{1,2}i,j \in \{1,2\} by

Cij(r)=cijWνij(r).C_{ij}(r)= c_{ij} W_{\nu_{ij}}(r).

Here WνW_\nu is the covariance of the RMwhittle model.

RMparswmX ist defined as

ρijCij(r)\rho_{ij} C_{ij}(r)

where ρij\rho_{ij} is any covariance matrix.

Usage

RMparswm(nudiag, var, scale, Aniso, proj)
RMparswmX(nudiag, rho, var, scale, Aniso, proj)

Arguments

nudiag

a vector of arbitrary length of positive values; the vector (ν11,ν22,...)(\nu_{11},\nu_{22},...). The offdiagonal elements νij\nu_{ij} are calculated as 0.5(νii+νjj)0.5 (\nu_{ii} + \nu_{jj}).

rho

any positive definite m×mm \times m matrix; here, mm equals length(nudiag). For the calculation of cijc_{ij} see Details.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

In the equation above we have

cij=ρijGijc_{ij} = \rho_{ij} \sqrt{G_{ij}}

and

Gij=Γ(ν11+d/2)Γ(ν22+d/2)Γ(ν12)2Γ(ν11)Γ(ν22)Γ(ν12+d/2)2G_{ij} = \frac{\Gamma(\nu_{11} + d/2) \Gamma(\nu_{22} + d/2) \Gamma(\nu_{12})^2}{\Gamma(\nu_{11}) \Gamma(\nu_{22}) \Gamma(\nu_{12}+d/2)^2}

where Γ\Gamma is the Gamma function and dd is the dimension of the space.

Note that the definition of RMparswmX is RMschur(M=rho, RMparswm(nudiag, var, scale, Aniso, proj)).

Value

RMparswm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Gneiting, T., Kleiber, W., Schlather, M. (2010) Matern covariance functions for multivariate random fields JASA

See Also

RMbiwm, RMwhittle, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

rho <- matrix(nc=3, c(1, 0.5, 0.2, 0.5, 1, 0.6, 0.2, 0.6, 1))
model <- RMparswmX(nudiag=c(1.3, 0.7, 2), rho=rho)
plot(model)
x.seq <- y.seq <- seq(-10, 10, 0.1)
z <- RFsimulate(model = model, x=x.seq, y=y.seq)
plot(z)

Penta Covariance Model

Description

RMpenta is a stationary isotropic covariance model, which is only valid for dimensions d3d \le 3. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(1223r2+33r4772r5+332r7112r9+56r11)1[0,1](r).C(r) = (1 - \frac{22}{3}r^{2} + 33 r^{4} - \frac{77}{2} r^{5} + \frac{33}{2} r^{7} - \frac{11}{2} r^{9} + \frac{5}{6}r^{11}) 1_{[0,1]}(r) .

Usage

RMpenta(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimensions d3d \le 3.

It has a 4 times differentiable covariance function with compact support (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 84).

Value

RMpenta returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMpenta()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Addition of Random Field Models

Description

RMplus is an additive covariance model which depends on up to 10 submodels C0,C1,...,C9C_0, C_1, ..., C_9. In general, realizations of the created RMmodel are pointwise sums of independent realizations of the submodels.

In particular, if all submodels are given through a covariance function, the resulting model is defined through its covariance function, which is the sum of the submodels' covariances. Analogously, if all submodels are given through a variogram.

Usage

RMplus(C0, C1, C2, C3, C4, C5, C6, C7, C8, C9, var, scale, Aniso, proj)

Arguments

C0

an RMmodel.

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional; each an RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above model remains unmodified.

Details

RMmodels can also be summed up via the +-operator, e.g. C0 + C1.

The global arguments var,scale,Aniso,proj of RMplus are multiplied to the corresponding arguments of the submodels (from the right side).

Value

RMplus returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmult, RMmodel, RMsum, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMplus(RMgauss(), RMnugget(var=0.1))
model2<- RMgauss() + RMnugget(var=0.1)
plot(model, "model.+"=model2, type=c("p", "l"), pch=20, xlim=c(0,3)) # the same

RMpolygon

Description

RMpolygon refers to the indicator function of a typical Poisson polygon, used for instance in the (mixed) Storm process.

Usage

RMpolygon(lambda)

Arguments

lambda

intensity of the hyperplane process creating the random shape function.

The default value is 1.

Author(s)

Felix Ballani, https://tu-freiberg.de/fakult1/sto/ballani

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Poisson polygons / Poisson hyperplane tessellation

  • Lantuejoul, C. (2002) Geostatistical Simulation: Models and Algorithms. Springer.

Poisson storm process

  • Lantuejoul, C., Bacro, J.N., Bel L. (2011) Storm processes and stochastic geometry. Extremes, 14(4), 413-428.

Mixed Poisson storm process

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMball, RMspheric, RFsimulate, RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Creating polynomial models

Description

Polynomials, mainly used in trend models, can be created easily with this function.

Usage

RMpolynome(degree, dim, value=NA, coordnames = c("x", "y", "z", "T"),
           proj=1:4)

Arguments

degree

degree of the polynome

dim

number of variables in the polynome

value

values of the coefficients. See Details.

coordnames

the names of the variables

proj

the projection to certain dimensions

Details

If the length of value is smaller than the number of monomials, the remaining terms are filled with NAs. If the length is larger, the vector is cut.

Value

RMpolynome returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMtrend, RFfit.

Examples

## For examples see the help page of 'RFformula' ##

RMpolynome(1, 1)
RMpolynome(1, 2)
RMpolynome(2, 1)
RMpolynome(2, 2)
RMpolynome(3, 3)

Power operator for Variograms and Covariance functions

Description

RMpower yields a variogram or covariance model from a given variogram or covariance model. The variogram γ\gamma of the model is given by

γ=ϕα\gamma = \phi^\alpha

if ϕ\phi is a variogram model. The covariance CC of the model is given by

C(h)=ϕ(0)(ϕ(0)ϕ(h))αC(h) = \phi(0)-(\phi(0)-\phi(h))^\alpha

if ϕ\phi is a covariance model.

Usage

RMpower(phi, alpha, var, scale, Aniso, proj)

Arguments

phi

a valid RMmodel; either a variogram model or a covariance model

alpha

a numerical value in the interval [0,1]

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

If γ\gamma is a variogram, then γα\gamma^\alpha is a valid variogram for α\alpha in the interval [0,1].

Value

RMpower returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Schlather, M. (2012) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J. M., Schlather, M. Advances and Challenges in Space-time Modelling of Natural Events, Springer, New York.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMpower(RMgauss(), alpha=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Plain scalar product

Description

RMprod is a non-stationary covariance model given by

C(x,y)=ϕ(x),ϕ(y)C(x,y) = \langle \phi(x), \phi(y)\rangle

Usage

RMprod(phi, var, scale, Aniso, proj)

Arguments

phi

any function of class RMmodel

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

In general, this model defines a positive definite kernel and hence a covariance model for all functions ϕ\phi with values in an arbitrary Hilbert space. However, as already mentioned above, ϕ\phi should stem from a covariance or variogram model, here.

Value

RMprod returns an object of class RMmodel.

Note

Do not mix up this model with RMmult.

See also RMS for a simple, alternative method to set an arbitrary, i.e. location dependent, univariate variance.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Wendland, H. Scattered Data Approximation (2005) Cambridge: Cambridge University Press.

See Also

RMid, RMid, RMsum, RMmodel, RMmult.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again


RFcov(RMprod(RMid()), as.matrix(1:10), as.matrix(1:10), grid=FALSE)


## C(x,y) =  exp(-||x|| + ||y||)
RFcov(RMprod(RMexp()), as.matrix(1:10), as.matrix(1:10), grid=FALSE)

## C(x,y) =  exp(-||x / 10|| + ||y / 10 ||)
model <- RMprod(RMexp(scale=10))
x <- seq(0,10,len=100)
z <- RFsimulate(model=model, x=x, y=x)
plot(z)

Quasi-arithmetic mean

Description

RMqam is a univariate stationary covariance model depending on a submodel ϕ\phi such that ψ():=ϕ(())\psi(\cdot) := \phi(\sqrt(\cdot)) is completely monotone, and depending on further stationary covariance models CiC_i. The covariance is given by

C(h)=ϕ((iθi(ϕ1(Ci(h)))2))C(h) = \phi(\sqrt(\sum_i \theta_i (\phi^{-1}(C_i(h)))^2))

Usage

RMqam(phi, C1, C2, C3, C4, C5, C6, C7, C8, C9, theta, var, scale, Aniso, proj)

Arguments

phi

a valid covariance RMmodel that is a normal scale mixture. See, for instance,
RFgetModelNames(monotone="normal mixture").

C1, C2, C3, C4, C5, C6, C7, C8, C9

optional further univariate stationary RMmodels

theta

a vector with positive entries

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Note that ψ():=ϕ(())\psi(\cdot) := \phi(\sqrt(\cdot)) is completely monotone if and only if ϕ\phi is a valid covariance function for all dimensions, e.g. RMstable, RMgauss, RMexponential.

Warning: RandomFields cannot check whether the combination of ϕ\phi and CiC_i is valid.

Value

RMqam returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Porcu, E., Mateu, J. & Christakos, G. (2007) Quasi-arithmetic means of covariance functions with potential applications to space-time data. Submitted to Journal of Multivariate Analysis.

See Also

RMmqam, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMqam(phi=RMgauss(), RMexp(), RMgauss(),
               theta=c(0.3, 0.7), scale=0.5)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Variant of the exponential model

Description

The covariance function is

C(x)=(2exαe2x)/(2α)C(x)= ( 2 e^{-x} - \alpha e^{-2x} ) / ( 2 - \alpha )

Usage

RMqexp(alpha, var, scale, Aniso, proj)

Arguments

alpha

value in [0,1][0,1]

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMqexp returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • ?

See Also

RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMqexp(alpha=0.95, scale=0.2)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Rational function

Description

Defines a simple rational function.

f(h)=(a1+a2z(h))/(1+z(h))f(h) = (a_1 + a_2 z(h)) / (1 + z(h))

where

z(h)=hAAhz(h) = h^\top A A^\top h

Usage

RMrational(A, a)

Arguments

A

a d×dd \times d matrix

a

a vector of one or two components; the second component has default value zero.

Value

RMrational returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, S10.

Examples

# see S10

Rotation matrices

Description

RMrotat and RMrotation are auxiliary space-time functions that create some rotation

f(h,t)=s(cos(ϕt)h1+sin(ϕt)h2)/hf(h, t) = s (\cos(\phi t) h_1 + \sin(\phi t) h_2) / \|h\|

and

f(h,t)=(cos(ϕt)h1+sin(ϕt)h2,sin(ϕt)h1+cos(ϕt)h2,t),f(h, t) = (\cos(\phi t) h_1 + \sin(\phi t) h_2, - \sin(\phi t) h_1 + \cos(\phi t) h_2, t),

respectively.

Usage

RMrotat(speed, phi) 
RMrotation(phi)

Arguments

speed

real value ss

phi

angle

Details

RMrotat and RMrotation are space-time models for two-dimensional space.

Value

RMrotat and RMrotation return an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, S10.

Examples

# see S10

Scaling operator

Description

RMS is an operator that modifies the variance and the coordinates or distances of a submodel ϕ\phi by

C(h)=vϕ(Ah/s).C(h) = v * \phi(A*h/s).

Most users will never call RMS directly, see Details. However, the following describes the arguments var, scale, Aniso, proj that are common to nearly all models. See RMSadvanced for advanced use of these arguments.

Usage

RMS(phi, var, scale, Aniso, proj, anisoT)

Arguments

phi

submodel

var

is the optional variance parameter vv.

scale

scaling parameter ss which is positive.

Aniso

matrix or RMmodel. The optional anisotropy matrix AA, multiplied from the right by a distance vector xx, i.e. AxAx.

proj

is the optional projection vector which defines a diagonal matrix of zeros and ones and proj gives the positions of the ones (integer values between 1 and the dimension of xx). It also allows for the values 'space' and 'time' in case of space-time modelling.

anisoT

the transpose of the anisotropy matrix BB, multiplied from the left by a distance vector xx, i.e. xBx^\top B.

Details

The call in the usage section is equivalent to phi(..., var, scale, anisoT, Aniso, proj), where phi has to be replaced by a valid RMmodel.

Most users will never call RMS directly.

Value

RMS returns an object of class RMmodel.

Note

At most one of the arguments Aniso, anisoT and proj may be given at the same time.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMSadvanced, RMmodel,

RMprod for an alternative way to define an arbitrary, location dependent variance. There, the standard deviation is given so that RMprod might be used even in the multivariate case.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model1 <- RMS(RMexp(), scale=2)
model2 <- RMexp(scale=2)
x <- seq(0, 10, 0.02)
print(all(RFcov(model1, x) == RFcov(model2, x))) # TRUE

Scaling operator – comments for advanced applications

Description

Here advances uses are given for the arguments var, scale, Aniso, proj that are available to most of the models

Usage

RMS(phi, var, scale, Aniso, proj, anisoT)

Arguments

phi

submodel

var

Instead of a constant it can be also an arbitrary non-negative function, see R. and RMuser for defining arbitrary functions.

scale

instead of a positive constant it can be an arbitrary, positive deterministic function. In case of the latter, the scale should be given by one of the functions RMbubble or RMscale. In case none of them are given, RMscale is assumed with scale penality s(x)s(y)2\|s(x) - s(y)\|^2 for the square of the norm.

The scale can be also a random variable in case of Bayesian modelling.

Aniso

matrix or RMmodel. Instead of a matrix, Aniso can be an arbitrary, vector-valued function .

proj

is the optional projection vector which defines a diagonal matrix of zeros and ones and proj gives the positions of the ones (integer values between 1 and the dimension of xx). It also allows for the values 'space' and 'time' in case of space-time modelling.

anisoT

the transpose of the anisotropy matrix BB, multiplied from the left by a distance vector xx, i.e. xBx^\top B.

Details

See the reference for Gneitings nsst model used for modelling scales. See also the example below.

Value

RMSadvanced returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Bonat, W.H. , Ribeiro, P. Jr. and Schlather, M. (2019) Modelling non-stationarity in scale. In preparation.

See Also

RMS, RMblend for a different approach on modelling different scales

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,1, if (interactive()) 0.01 else 0.5)
d <- sqrt(rowSums(as.matrix(expand.grid(x-0.5, x-0.5))^2))
d <- matrix(d < 0.25, nc=length(x))
image(d)

scale <- RMcovariate(data=as.double(d) * 2 + 0.5, raw=TRUE)

S <- RMexp(scale = scale)
plot(zS <- RFsimulate(S, x, x))
CS <- RFcovmatrix(S, x, x)

Scale model for arbitrary areas of scales

Description

Let sxs_x the scaling at location xx and pp a bijective penalizing function for (different) scales. Then covariance function is given by

C(x,y)=ϕ(xy+p(sx)p(sy))C(x,y) = \phi(\|x-y\| + |p(s_x) - p(s_y)|)

Usage

RMscale(phi, scaling, penalty, var, scale, Aniso, proj)

Arguments

phi

isotropic submodel

scaling

model that gives the non-stationary scaling sxs_x

penalty

bijective function pp applied to the scaling

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMscale returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Bonat, W.H. , Ribeiro, P. Jr. and Schlather, M. (2019) Modelling non-stationarity in scale. In preparation.

See Also

RMSadvanced, RMblend, RMbubble

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0,1, 0.01)
scale <- RMcovariate(x=c(0,1), y=c(1,0),#2 areas separated by the 1st bisector
                     grid=FALSE, data=c(1, 3))

model <- RMscale(RMexp(), scaling = scale, penalty=RMid() / 2)
plot(z <- RFsimulate(model, x, x))

Covariance Model for binary field based on Gaussian field

Description

RMschlather gives the tail correlation function of the extremal Gaussian process, i.e.

C(h)=1(1ϕ(h)/ϕ(0))/2C(h) = 1 - \sqrt{ (1-\phi(h)/\phi(0)) / 2 }

where ϕ\phi is the covariance of a stationary Gaussian field.

Usage

RMschlather(phi, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This model yields the tail correlation function of the field that is returned by RPschlather.

Value

RMschlather returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RPschlather, RMmodel, RFsimulate.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## This example considers an extremal Gaussian random field
## with Gneiting's correlation function.

## first consider the covariance model and its corresponding tail
## correlation function
model <- RMgneiting()
plot(model, model.tail.corr.fct=RMschlather(model),  xlim=c(0, 5))


## the extremal Gaussian field with the above underlying
## correlation function that has the above tail correlation function
x <- seq(0, 10, 0.1)
z <- RFsimulate(RPschlather(model), x)
plot(z)

## Note that in RFsimulate R-P-schlather was called, not R-M-schlather.
## The following lines give a Gaussian random field with correlation
## function equal to the above tail correlation function.
z <- RFsimulate(RMschlather(model), x)
plot(z)

Schur product

Description

The covariance function is

C(x)=Mϕ(x)C(x)= M * \phi(x)

where ‘*’ denotes the Schur product, i.e. elementwise multiplication.

Usage

RMschur(phi, M,  diag, rhored, var, scale, Aniso, proj)

Arguments

phi

covariance function of class RMmodel

M

constant n×nn \times n covariance matrix of the same size as multivariate model phi

diag, rhored

alternative way of passing M: diag is a vector of variances, rhored is a vector containing the correlations of the lower triangle of the M.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMschur returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • ?

See Also

RMmodel, RMmatrix.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMschur(M=matrix(c(2, 1, 1, 1), ncol=2), RMparswm(nudiag=c(0.5, 2)))
plot(model)
x <- seq(0, 10, 0.02)
plot(RFsimulate(model, x=x))

Random sign

Description

RMsign defines a random sign. It can be used as part of the model definition of a Poisson field.

Usage

RMsign(phi, p)

Arguments

phi

shape function of class RMmodel

p

probability of keeping the sign

Details

RMsign changes the sign of the shape function phi with probability 1-p and keeps it otherwise.

Value

RMsign returns an object of class RMmodel.

Note

Random univariate or multivariate objects usually start with RR, not with RM. This is an exception here, as it operates on shape functions.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RR.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RPpoisson(RMsign(RMtent(), p=0.8))
x <- seq(0, 10, 0.02)
plot(RFsimulate(model, x=x))

The Sinepower Covariance Model on the Sphere

Description

RMsinepower is an isotropic covariance model. The corresponding covariance function, the sine power function of Soubeyrand, Enjalbert and Sache, only depends on the angle θ[0,π]\theta \in [0,\pi] between two points on the sphere and is given by

ψ(θ)=1(sinθ2)α\psi(\theta) = 1 - ( sin\frac{\theta}{2} )^{\alpha}

where α(0,2]\alpha\in (0,2].

Usage

RMsinepower(alpha, var, scale, Aniso, proj)

Arguments

alpha

a numerical value in (0,2](0,2]

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

For the sine power function of Soubeyrand, Enjalbert and Sache, see Gneiting, T. (2013), equation (17). For a more general form see RMchoquet.

Value

RMsinepower returns an object of class RMmodel.

Author(s)

Christoph Berreth; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gneiting, T. (2013) Strictly and non-strictly positive definite functions on spheres Bernoulli, 19(4), 1327-1349.

See Also

RMmodel, RFsimulate, RFfit, spherical models, RMchoquet

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFoptions(coord_system="sphere")
model <- RMsinepower(alpha=1.7)
plot(model, dim=2)

## the following two pictures are the same
x <- seq(0, 0.4, 0.01)
z1 <- RFsimulate(model, x=x, y=x)
plot(z1)

x2 <- x * 180 / pi
z2 <- RFsimulate(model, x=x2, y=x2, coord_system="earth")
plot(z2)

stopifnot(all.equal(as.array(z1), as.array(z2)))

RFoptions(coord_system="auto")

The Spherical Covariance Model

Description

RMspheric is a stationary isotropic covariance model which is only valid up to dimension 3. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=(132r+12r3)1[0,1](r)C(r) = \left(1 - \frac{3}{2} r + \frac{1}{2} r^3\right) 1_{[0,1]}(r)

Usage

RMspheric(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

This covariance model is valid only for dimensions less than or equal to 3.

The covariance function has a finite range.

Value

RMspheric returns an object of class RMmodel.

Note

Although this model is valid on a sphere, do not mix up this model with valid models on a sphere; see spherical models for a list of the latter.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

See Also

RMmodel, RFsimulate, RFfit, spherical models.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMspheric()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Stable Family / Powered Exponential Model

Description

RMstable is a stationary isotropic covariance model belonging to the so called stable family. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=erαC(r) = e^{-r^\alpha}

where α(0,2]\alpha \in (0,2].

Usage

RMstable(alpha, var, scale, Aniso, proj)
RMpoweredexp(alpha, var, scale, Aniso, proj)

Arguments

alpha

a numerical value; should be in the interval (0,2] to provide a valid covariance function for a random field of any dimension.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The parameter α\alpha determines the fractal dimension DD of the Gaussian sample paths:

D=d+1α2D = d + 1 - \frac{\alpha}{2}

where dd is the dimension of the random field. For α<2\alpha < 2 the Gaussian sample paths are not differentiable (cf. Gelfand et al., 2010, p. 25).

Each covariance function of the stable family is a normal scale mixture.

The stable family includes the exponential model (see RMexp) for α=1\alpha = 1 and the Gaussian model (see RMgauss) for α=2\alpha = 2.

The model is called stable, because in the 1-dimensional case the covariance is the characteristic function of a stable random variable (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 90).

Value

RMstable returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Covariance function

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Diggle, P. J., Tawn, J. A. and Moyeed, R. A. (1998) Model-based geostatistics (with discussion). Applied Statistics 47, 299–350.

  • Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

Tail correlation function (for α(0,1]\alpha \in (0,1])

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

RMbistable, RMexp, RMgauss, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMstable(alpha=1.9, scale=0.4)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Stein's non-separable space-time model

Description

RMstein is a univariate stationary covariance model whose corresponding covariance function only depends on the difference hh between two points and is given by

C(h,t)=Wν(y)(<h,z>t)/((ν1)(2ν+d))Wν1(y)C(h, t) = W_{\nu}(y) - ( < h, z > t)/((\nu - 1)(2\nu + d)) * W_{\nu-1}(y)

Here, WνW_\nu is the covariance of the RMwhittle model with smoothness parameter ν\nu; y=(h,t)y=\|(h,t)\| is the norm of the vector (h,t)(h,t), dd is the dimension of the space on which the random field is considered.

Usage

RMstein(nu, z, var, scale, Aniso, proj)

Arguments

nu

numerical value; greater than 1; smoothness parameter of the RMwhittle model

z

a vector; the norm of zz must be less or equal to 1.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

See Stein (2005).

Value

RMstein returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Stein, M.L. (2005) Space-time covariance functions. J. Amer. Statist. Assoc. 100, 310-321. Equation (8).

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMstein(nu=1.5, z=0.9)
x <- seq(0, 10, 0.05)
plot(RFsimulate(model, x=x, y=x))

Single temporal process

Description

RMstp is a univariate covariance model which depends on a normal mixture submodel ϕ\phi. The covariance is given by

C(x,y)=Sx1/4Sy1/4A1/2ϕ(Q(x,y)1/2)C(x,y) = |S_x|^{1/4} |S_y|^{1/4} |A|^{-1/2} \phi(Q(x,y)^{1/2})

where

Q(x,y)=c2m2+ht(Sx+2(m+c)M)A1(Sy+2(mc)M)h,Q(x,y) = c^2 - m^2 + h^t (S_x + 2(m + c)M) A^{-1} (S_y + 2 (m-c)M)h,

c=zth+ξ2(x)ξ2(y),c = -z^t h + \xi_2(x) - \xi_2(y),

A=Sx+Sy+4MhhtMA = S_x + S_y + 4 M h h^t M

m=htMhm = h^t M h

h=xyh = x - y

Usage

RMstp(xi, phi, S, z, M, var, scale, Aniso, proj)

Arguments

xi

arbitrary univariate function on RdR^d

phi

an RMmodel that is a normal mixture model, cf.
RFgetModelNames(monotone="normal mixture")

S

functions that returns strictly positive definite d×dd\times d

z

arbitrary vector, zRdz \in R^d

M

an arbitrary, symmetric d×dd \times d matrix

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

See Schlather (2008) formula (13). The model allows for mimicking cyclonic behaviour.

Value

RMstp returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Paciorek C.J., and Schervish, M.J. (2006) Spatial modelling using a new class of nonstationary covariance functions, Environmetrics 17, 483-506.

  • Schlather, M. (2010) Some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

See Also

RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMstp(xi = RMrotat(phi= -2 * pi, speed=1),
               phi = RMwhittle(nu = 1),
               M=matrix(nc=3, rep(0, 9)),
               S=RMetaxxa(E=rep(1, 3), alpha = -2 * pi,
                          A=t(matrix(nc=3, c(2, 0, 0, 1, 1 , 0, 0, 0, 0))))
              )
x <- seq(0, 10, 0.7)
plot(RFsimulate(model, x=x, y=x, z=x))

Plain scalar product

Description

RMsum is given by

C(x,y)=ϕ(x)+ϕ(y)C(x,y) = \phi(x) + \phi(y)

It is a negative definite function although not a variogram.

Usage

RMsum(phi, var, scale, Aniso, proj)

Arguments

phi

any function of class RMmodel

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Value

RMsum returns an object of class RMmodel.

Note

Do not mix up this model with RMplus.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RMplus, RMprod.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Turning Bands Method

Description

RMtbm is a univariate or multivaraiate stationary isotropic covariance model in dimension reduceddim which depends on a univariate or multivariate stationary isotropic covariance ϕ\phi in a bigger dimension fulldim. For formulas for the covariance function see details.

Usage

RMtbm(phi, fulldim, reduceddim, layers, var, scale, Aniso, proj)

Arguments

phi, fulldim, reduceddim, layers

See RPtbm.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The turning bands method stems from the 1:1 correspondence between the isotropic covariance functions of different dimensions. See Gneiting (1999) and Strokorb and Schlather (2014).

The standard case is reduceddim=1 and fulldim=3. If only one of the arguments is given, then the difference of the two arguments equals 2.

For d == n + 2, where n=reduceddim and d==fulldim the original dimension, we have

C(r)=ϕ(r)+rϕ(r)/nC(r) = \phi(r) + r \phi'(r) / n

which for n=1 reduces to the standard TBM operator

C(r)=ddrrϕ(r)C(r) =\frac {d}{d r} r \phi(r)

For d == 2 && n == 1 we have

C(r)=ddr0ruϕ(u)r2u2duC(r) = \frac{d}{dr}\int_0^r \frac{u\phi(u)}{\sqrt{r^2 - u^2}} d u

‘Turning layers’ is a generalization of the turning bands method, see Schlather (2011).

Value

RMtbm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Turning bands

  • Gneiting, T. (1999) On the derivatives of radial positive definite function. J. Math. Anal. Appl, 236, 86-99

  • Matheron, G. (1973). The intrinsic random functions and their applications. Adv . Appl. Probab., 5, 439-468.

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

Turning layers

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

See Also

RPtbm, RFsimulate.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0, 10, 0.02)
model <- RMspheric()
plot(model, model.on.the.line=RMtbm(RMspheric()), xlim=c(-1.5, 1.5))

z <- RFsimulate(RPtbm(model), x, x)
plot(z)

Transformation of coordinate systems

Description

The functions transform a coordinate system into another coordinate system. Currently, essentially only from the earth system to cartesian.

RMtrafo is the internal basic function that also allows to reduce vectors to their norm.

Usage

RMtrafo(phi, new)
RFearth2cartesian(coord, units=NULL, system="cartesian", grid=FALSE)
RFearth2dist(coord, units=NULL, system="cartesian", grid=FALSE, ...)

Arguments

new

integer or character. One of the values RC_ISOTROPIC, RC_SPACEISOTROPIC, RC_CARTESIAN_COORD, RC_GNOMONIC_PROJ, RC_ORTHOGRAPHIC_PROJ

or the corresponding RC_ISONAMES.

Note that RMtrafo only allows for integer values.

Default: RC_CARTESIAN_COORD.

phi

optional submodel

coord

matrix or vector of earth coordinates

units

"km" or "miles"; if not given and RFoptions()$general$units != "", the latter is used. Otherwise "km".

system

integer or character. The coordinate system, e.g. "cartesian", "gnomonic" or "orthographic".

grid

logical. Whether the given coordinates are considered to be on a grid given by c(start, step, length).

Default: FALSE.

...

the optional arguments of dist

Details

The functions transform between different coordinate systems.

Value

The function RMtrafo returns a matrix, in general. For fixed column, the results, applied to each row of the matrix, are returned.

The function RFearth2cartesian returns a matrix in one-to-one correspondence with coord assuming that the earth is an ellipsoid.

The function RFearth2dist calculates distances, cf. dist, assuming that the earth is an ellipsoid.

Note

Important options are units and coordinate_system, see RFoptions.

Note also that the zenit must be given explicitly for projection onto a plane. See the examples below.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

For calculating the earth coordinates as ellipsoid:

See Also

constants, RMangle, RMid, RMidmodel.

Examples

data(weather)
(coord <- weather[1:5, 3:4])

(z <- RFfctn(RMtrafo(new=RC_CARTESIAN_COORD), coord))
(z1 <- RFearth2cartesian(coord)) ## equals z
z1 - z ## 0, i.e., z1 and t(z) are the same
dist(z)


(d <- RFearth2dist(coord)) 
d - dist(z) ## 0, i.e., d and dist(z) are the same


## projection onto planes
RFoptions(zenit=c(-122,   47))
RFearth2cartesian(coord, system="gnomonic")
RFearth2cartesian(coord, system="orthographic")

Trend Model

Description

RMtrend is a pure trend model with covariance 0.

Usage

RMtrend(mean)

Arguments

mean

numeric or RMmodel. If it is numerical, it should be a vector of length pp, where pp is the number of variables taken into account by the corresponding multivariate random field (Z1(),,Zp())(Z_1(\cdot),\ldots,Z_p(\cdot)); the ii-th component of mean is interpreted as constant mean of Zi()Z_i(\cdot).

Details

Note that this function refers to trend surfaces in the geostatistical framework. Fixed effects in the mixed models framework are also being implemented, see RFformula.

Value

RMtrend returns an object of class RMmodel.

Note

Using uncapsulated subtraction to build up a covariance function is ambiguous, see the examples below. Best to define the trend separately, or to use R.minus.

Author(s)

Marco Oesting, [email protected], https://www.isa.uni-stuttgart.de/institut/team/Oesting/; Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Chiles, J. P., Delfiner, P. (1999) Geostatistics: Modelling Spatial Uncertainty. New York: John Wiley & Sons.

See Also

RMmodel, RFformula, RFsimulate, RMplus

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## first simulate some data with a sine and a mean as trend
repet <- 100
 
x <- seq(0, pi, len=10)
trend <- 2 * sin(R.p(new="isotropic")) + 3
model1 <- RMexp(var=2, scale=1) + trend
dta <- RFsimulate(model1, x=x, n=repet)



## now, let us estimate variance, scale, and two parameters of the trend
model2 <- RMexp(var=NA, scale=NA) + NA * sin(R.p(new="isotropic")) + NA

print(RFfit(model2, data=dta))

## model2 can be made explicit by enclosing the trend parts by
## 'RMtrend'
model3 <- RMexp(var=NA, scale=NA) + NA *
          RMtrend(sin(R.p(new="isotropic"))) + RMtrend(NA)
print(RFfit(model2, data=dta))


## IMPORTANT:  subtraction is not a way to combine definite models
##             with trends
trend <- -1
(model0 <- RMexp(var=0.4) + trend) ## exponential covariance with mean -1
(model1 <- RMexp(var=0.4) + -1)    ## same as model0
(model2 <- RMexp(var=0.4) + RMtrend(-1)) ## same as model0
(model3 <- RMexp(var=0.4) - 1) ## this is a purely deterministic model
                               ## with exponential trend
plot(RFsimulate(model=model0, x=x, y=x)) ## exponential covariance
                               ##           and mean -1
plot(RFsimulate(model=model1, x=x, y=x)) ## dito
plot(RFsimulate(model=model2, x=x, y=x)) ## dito
plot(RFsimulate(model=model3, x=x, y=x)) ## purely deterministic model!

Truncating the Support of a Shape Function

Description

RMtruncsupport may be used to truncate the support of a shape function when Poisson fields or M3 processes are created.

Usage

RMtruncsupport(phi, radius)

Arguments

phi

function of class RMmodel

radius

truncation at radius

Value

RMtruncsupport returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2002) Models for stationary max-stable random fields. Extremes 5, 33-44.

See Also

RMmodel, RMmatrix, RPpoisson.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again 

model <- RMgauss()
model1 <- RMtruncsupport(model, radius=1)
plot(model)
lines(model1, col="red")

## For a real application of 'RMtruncsupport' see example 2 of 'RPpoisson'.

User-Defined Function

Description

RMuser allows for a user-defined covariance function, variogram model, or arbitrary function.

RMuser is very slow – users should avoid this model whenever possible.

Usage

RMuser(type, domain, isotropy, vdim, beta,
       coordnames = c("x", "y", "z", "T"), fctn, fst, snd, envir,  
       var, scale, Aniso, proj)

Arguments

type

See RMmodelgenerator for the range of values of the arguments.

Default: "shape function".

domain

See RMmodelgenerator for the range of values of the arguments.

Default: XONLY.

isotropy

See RMmodelgenerator for the range of values of the arguments.

Default:

  • 'isotropic' if type equals 'tail correlation function', 'positive definite' or 'negative definite';

  • 'cartesian system' if type indicates a process or simulation method or a shape function.

vdim

multivariability.

Default: vdim is identified from beta if given; otherwise the default value is 1.

beta

a fixed matrix that is multiplied to the return value of the given function; the dimension must match. Defining a vector valued function and beta as a vector, an arbitrary linear model can be defined. Estimation of beta is, however, not established yet.

coordnames

Just the names of the variables. More variable names might be given here than used in the function. See Details for the interpretation of variables.

fctn, fst, snd

a user-defined function and its first, second and third derivative, given as quote(myfunction(x)) or as quote(myfunction(x, y)), see Details and Examples below.

envir

the environment where the given function shall be evaluated

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

Primarily, a function is expected that depends on a vector whose components, x,y,z,Tx, y, z, T, are given separately as scalar quantities.

Alternatively, the function might depend only on the first argument given by coordnames.

A kernel should depend on the first two arguments given by coordnames.

Value

RMuser returns an object of class RMmodel.

Note

  • The use of RMuser is completely on the risk of the user. There is no way to check whether the expressions of the user are correct in any sense.

  • Note that x, y, z and T are reserved argument names that define solely the coordinates. Hence, none of these names might be used for other arguments within these functions.

  • In user-defined functions, the models of RandomFields are not recognized, so they cannot be included in the function definitions.

  • RMuser may not be used in connection with obsolete commands of RandomFields.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMcovariate, RMfixcov, RFfit, RMmodelgenerator, RMmodel, RFsimulate, RC_ISO_NAMES, RC_DOMAIN_NAMES.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## Alternatively to 'model <- RMexp()' one may define the following
## (which is, however, much slower and cannot use all features of
## RandomFields)

## user-defined exponential covariance model
model <- RMuser(type="positive definite", domain="single variable",
                iso="isotropic", fctn=exp(-x))
x <- y <- seq(1, 10, len=100)
plot(model)
z <- RFsimulate(model, x=x, y=y)
plot(z)

## the kernel, which is the scalar product (see RMprod)
model <- RMnugget(var=1e-5) +
         RMuser(type="positive definite", domain="kernel",
                iso="symmetric", fctn=sum(x * y))
x <- y <- seq(1, 10, len=35)
z <- RFsimulate(model, x=x, y=y, n=6, svdtol=1e-9) 
plot(z)

Vector Covariance Model

Description

RMvector is a multivariate covariance model which depends on a univariate covariance model that is stationary in the first DspaceDspace coordinates hh and where the covariance function phi(h,t) is twice differentiable in the first component hh.

The corresponding matrix-valued covariance function C of the model only depends on the difference hh between two points in the first component. It is given by

C(h,t)=(0.5(a+1)Δ+aT)C0(h,t)C(h,t)=( -0.5 * (a + 1) \Delta + a \nabla \nabla^T ) C_0(h, t)

where the operator is applied to the first component hh only.

Usage

RMvector(phi, a, Dspace, var, scale, Aniso, proj)

Arguments

phi

an RMmodel; has two components hh (2- or 3-dimensional and stationary) and tt (arbitrary dimension).

a

a numerical value; should be in the interval [1,1][-1,1].

Dspace

an integer; either 2 or 3; the first DspaceDspace coordinates give the first component hh.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

C0C_0 is either a spatio-temporal model (then tt is the time component) or it is an isotropic model. Then, the first DspaceDspace coordinates are considered as hh coordinates and the remaining ones as tt coordinates. By default, DspaceDspace equals the dimension of the field (and there is no tt component). If a=1a=-1 then the field is curl free; if a=1a=1 then the field is divergence free.

Value

RMvector returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Scheuerer, M. and Schlather, M. (2012) Covariance Models for Divergence-Free and Curl-Free Random Vector Fields. Stochastic Models 28:3.

See Also

RMcurlfree, RMdivfree, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMvector(RMgauss(), scale=0.3)
x <- seq(0, 10, 0.4)
plot(RFsimulate(model, x=x, y=x, z=0), select.variables=list(1:2))

Wave Covariance Model / Cardinal Sine

Description

RMwave is a stationary isotropic covariance model, which is valid only for dimensions d3d \le 3. The corresponding covariance function only depends on the distance r0r \ge 0 between two points and is given by

C(r)=sin(r)/r1r>0+1r=0.C(r) = sin(r)/r 1_{r>0} + 1_{r=0} .

It is a special case of RMbessel.

Usage

RMwave(var, scale, Aniso, proj)
RMcardinalsine(var, scale, Aniso, proj)

Arguments

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The model is only valid for dimensions d3d \le 3. It is a special case of RMbessel for ν=0.5\nu = 0.5.

This covariance models a hole effect (cf. Chiles, J.-P. and Delfiner, P. (1999), p. 92).

Value

RMwave returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

See Also

RMbessel, RMmodel, RFsimulate, RFfit.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMwave(scale=0.1)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))

Whittle-Matern Covariance Model

Description

RMmatern is a stationary isotropic covariance model belonging to the Matern family. The corresponding covariance function only depends on the distance r0r \ge 0 between two points.

The Whittle model is given by

C(r)=Wν(r)=21νΓ(ν)1rνKν(r)C(r)=W_{\nu}(r)=2^{1- \nu} \Gamma(\nu)^{-1}r^{\nu}K_{\nu}(r)

where ν>0\nu > 0 and KνK_\nu is the modified Bessel function of second kind.

The Matern model is given by

C(r)=21νΓ(ν)(2νr)νKν(2νr)C(r) = \frac{2^{1-\nu}}{\Gamma(\nu)} (\sqrt{2\nu}r)^\nu K_\nu(\sqrt{2\nu}r)

The Handcock-Wallis parametrisation is given by

C(r)=21νΓ(ν)(2νr)νKν(2νr)C(r) = \frac{2^{1-\nu}}{\Gamma(\nu)} (2\sqrt{\nu}r)^\nu K_\nu(2 \sqrt{\nu}r)

Usage

RMwhittle(nu, notinvnu, var, scale, Aniso, proj)

RMmatern(nu, notinvnu, var, scale, Aniso, proj)

RMhandcock(nu, notinvnu, var, scale, Aniso, proj)

Arguments

nu

a numerical value called “smoothness parameter”; should be greater than 0.

notinvnu

logical. If FALSE then in the definition of the models ν\nu is replaced by 1/ν1/\nu. This parametrization seems to be more natural. Default is, however, TRUE according with the definitions in literature.

var, scale, Aniso, proj

optional arguments; same meaning for any RMmodel. If not passed, the above covariance function remains unmodified.

Details

The three models are alternative parametrizations of the same covariance function. The Matern model or the Handcock-Wallis parametrisation should be preferred as they seperate the effects of the scaling parameter and the shape parameter.

The Whittle-Matern model is the model of choice if the smoothness of a random field is to be parametrized: the sample paths of a Gaussian random field with this covariance structure are mm times differentiable if and only if ν>m\nu > m (see Gelfand et al., 2010, p. 24).

Furthermore, the fractal dimension (see also RFfractaldim) D of the Gaussian sample paths is determined by ν\nu: We have

D=d+1ν,ν(0,1)D = d + 1 - \nu, \nu \in (0,1)

and D=dD = d for ν>1\nu > 1 where dd is the dimension of the random field (see Stein, 1999, p. 32).

If ν=0.5\nu=0.5 the Matern model equals RMexp.

For ν\nu tending to \infty a rescaled Gaussian model RMgauss C(r)=r2C(r) = -r^2 appears as limit of the above Handcock-Wallis parametrisation.

For generalizations see section ‘See Also’.

Value

The functions return an object of class RMmodel.

Note

The Whittle-Matern model is a normal scale mixture.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Covariance function

  • Chiles, J.-P. and Delfiner, P. (1999) Geostatistics. Modeling Spatial Uncertainty. New York: Wiley.

  • Gelfand, A. E., Diggle, P., Fuentes, M. and Guttorp, P. (eds.) (2010) Handbook of Spatial Statistics. Boca Raton: Chapman & Hall/CRL.

  • Guttorp, P. and Gneiting, T. (2006) Studies in the history of probability and statistics. XLIX. On the Matern correlation family. Biometrika 93, 989–995.

  • Handcock, M. S. and Wallis, J. R. (1994) An approach to statistical spatio-temporal modeling of meteorological fields. JASA 89, 368–378.

  • Stein, M. L. (1999) Interpolation of Spatial Data – Some Theory for Kriging. New York: Springer.

Tail correlation function (for ν(0,1/2]\nu \in (0,1/2])

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

See Also

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

x <- seq(0, 1, len=100)
model <- RMwhittle(nu=1, Aniso=matrix(nc=2, c(1.5, 3, -3, 4)))
plot(model, dim=2, xlim=c(-1,1))
z <- RFsimulate(model=model, x, x)
plot(z)

Simulation of Binary Random Fields

Description

Indicator or binary field which has the value 1, if an underfield field exceeds a given threshold, 0 otherwise.

Usage

RPbernoulli(phi, stationary_only, threshold)

Arguments

phi

the RMmodel. Either a model for a process or a covariance model must be specified. In the latter case, a Gaussian process RPgauss is tacitely assumed.

stationary_only

optional arguments; same meaning as for RPgauss. It is ignored if the submodel is a process definition.

threshold

real valued. RPbernoulli returns 11 if value of the random field given by phi is equal to or larger than the value of threshold, and 00 otherwise. In the multivariate case, a vector might be given. If the threshold is not finite, then the original field is returned.

threshold default value is 0.

Details

RPbernoulli can be applied to any field. If only a covariance model is given, a Gaussian field is simulated as underlying field.

Value

The function returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

Auxiliary RMmodels, RP, RMbernoulli.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
x <- seq(0, 10, 0.1)
model <- RPbernoulli(RMexp(), threshold=0)
z <- RFsimulate(model, x, x, n=4)
plot(z)

model <- RPbernoulli(RPbrownresnick(RMexp(), xi=1), threshold=1)
z <- RFsimulate(model, x, x, n=4)
plot(z)

Simulation of Chi2 Random Fields

Description

RPchi2 defines a chi2 field.

Usage

RPchi2(phi, boxcox, f)

Arguments

phi

the RMmodel. If a model for the distribution is not specified, RPgauss is used as default and a covariance model is expected.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

f

integer. Degree of freedom.

Value

The function returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

Auxiliary RMmodels, RP, RPgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RPchi2(RMexp(), f=2)
x <- seq(0, 10, 0.1)
z <- RFsimulate(model=model, x, x, n=4)
plot(z)

Simulation of Gaussian Random Fields

Description

This function is used to specify a Gaussian random field that is to be simulated or estimated. Returns an object of class RMmodel.

Usage

RPgauss(phi, boxcox, stationary_only)

Arguments

phi

the RMmodel.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

stationary_only

Logical or NA. Used for the automatic choice of methods.

  • TRUE: The simulation of non-stationary random fields is refused. In particular, the intrinsic embedding method is excluded and the simulation of Brownian motion is rejected.

  • FALSE: Intrinsic embedding is always allowed; actually, it's the first one considered in the automatic selection algorithm.

  • NA: The simulation of the Brownian motion is allowed, but intrinsic embedding is not used for translation invariant (“stationary”) covariance models.

Default: NA.

Value

The function returns an object of class RMmodel.

Note

In most cases, RPgauss need not be given explicitly as Gaussian random fields are assumed as default.

RPgauss may not find the fastest method neither the most precise one. It just finds any method among the available methods. (However, it guesses what is a good choice.) See RFgetMethodNames for further information. Note that some of the methods do not work for all covariance or variogram models, see RFgetModelNames(intern=FALSE).

By default, all Gaussian random fields have zero mean. Simulating with trend can be done by including RMtrend in the model.

RPgauss allows to simulate different classes of random fields, controlled by the wrapping model:

If the submodel is a pure covariance or variogram model, i.e. of class RMmodel, a corresponding centered Gaussian field is simulated. Not only stationary fields but also non-stationary and anisotropic models can be used, e.g. zonal anisotropy, geometrical anisotropy, separable models, non-separable space-time models, multiplicative or nested models; see RMmodel for a list of all available models.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RP, Gaussian, RMmodel, RFoptions, RPbrownresnick, RPchi2, RPopitz, RPt, RPschlather.

Do not mix up with RMgauss or RRgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMexp()
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x, seed=0))
plot(RFsimulate(RPgauss(model), x=x, seed=0), col=2) ## the same

Simulation of Poisson Random Fields

Description

Shot noise model, which is also called moving average model, trigger process, dilution random field, and by several other names.

Usage

RPpoisson(phi, intensity)

Arguments

phi

the model, RMmodel, gives the shape function to be used

intensity

the intensity of the underlying stationary Poisson point process

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RP, RPcoins.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

# example 1: Posson field based on disks with radius 1
x <- seq(0,25, 0.02)
model <- RMball()
z <- RFsimulate(RPpoisson(model), x, intensity = 2)
plot(z)
par(mfcol=c(2,1))
plot(z@data[,1:min(length(z@data), 1000)], type="l")
hist(z@data[,1], breaks=0.5 + (-1 : max(z@data)))


# example 2: Poisson field based on the normal density function
# note that
# (i) the normal density as unbounded support that has to be truncated
# (ii) the intensity is high so that the CLT holds
x <- seq(0, 10, 0.01)
model <- RMtruncsupport(radius=5, RMgauss())
z <- RFsimulate(RPpoisson(model), x, intensity = 100)
plot(z)

Models for classes of random fields (RP commands)

Description

Here, all classes of random fields are described that can be simulated.

Implemented processes

Gaussian Random Fields see Gaussian
Max-stable Random Fields see Maxstable
Other Random Fields Binary field
chi2 field
composed Poisson (shot noise, random coin)
t field

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RC, RR, RM, RF, R.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
x <- seq(0, 10, 0.1)
model <- RMexp()

## a Gaussian field with exponential covariance function
z <- RFsimulate(model, x)
plot(z)

## a binary field obtained as a thresholded Gaussian field
b <- RFsimulate(RPbernoulli(model), x)
plot(b)

sum( abs((z@data$variabl1 >=0 ) - b@data$variable1)) == 0 ## TRUE,
## i.e. RPbernoulli is indeed a thresholded Gaussian process

Simulation of T Random Fields

Description

RPt defines a t field.

Usage

RPt(phi, boxcox, nu)

Arguments

phi

the RMmodel. If a model for the distribution is not specified, RPgauss is used as default and a covariance model is expected.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

nu

non-negative number. Degree of freedom.

Value

The function returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Related to the extremal t process

  • T. Opitz (2012) A spectral construction of the extremal t process. arxiv 1207.2296.

See Also

Auxiliary RMmodels, RP, RPgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RPt(RMexp(), nu=2)
x <- seq(0, 10, 0.1)
z <- RFsimulate(model, x, x, n=4)
plot(z)

Degenerate Distributions

Description

RRdeterm refers to the distribution of a deterministic variable.

Usage

RRdeterm(mean)

Arguments

mean

the deterministic value

Value

RRdeterm returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RRdistr, RRgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
x <- seq(-2, 2, 0.001)
p <- RFpdistr(RRdeterm(mean=1), q=x)
plot(x, p, type="l")

Definition of Distribution Families

Description

RRdistr defines a distribution family given by fct. It is used to introduce random parameters based on distributions defined on R.

Usage

RRdistr(name, nrow, ncol, 
        envir, ...)

Arguments

name

an arbitrary family of distributions. E.g. norm() for the family dnorm, pnorm, qnorm, rnorm. See examples below.

nrow, ncol

The matrix size (or vector if ncol=1) the family returns. Except for very advanced modelling we always have nrow=ncol=1, which is the default.

envir

an environment; defaults to new.env().

...

Second possibility to pass the distribution family is to pass a character string as name and to give the argument within .... See examples below.

Details

RRdistr returns an object of class RMmodel.

Note

RRdistr is the generic model introduced automatically when distribution families in R are used in the model definition. See the examples below.

Note

See Bayesian Modelling for a less technical introduction to hierarchical modelling.

The use of RRdistr is completely on the risk of the user. There is no way to check whether the expressions of the user are mathematically correct.

Further, RRdistr may not be used in connection with obsolete commands of RandomFields.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RR, RFsimulate, RFdistr.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## here a model with random scale parameter
model <- RMgauss(scale=exp(rate=1))
x <- seq(0,10,0.02)
n <- 10
 
for (i in 1:n) {  
  readline(paste("Simulation no.", i, ": press return", sep=""))
  plot(RFsimulate(model, x=x, seed=i))
}

## another possibility to define exactly the same model above is
## model <- RMgauss(scale=exp())

## note that however, the following two definitions lead
## to covariance models with fixed scale parameter:
## model <- RMgauss(scale=exp(1))   # fixed to 2.7181
## model <- RMgauss(scale=exp(x=1)) # fixed to 2.7181


## here, just two other examples:
## fst
model <- RMmatern(nu=unif(min=0.1, max=2)) # random
for (i in 1:n) {
  readline(paste("Simulation no.", i, ": press return", sep=""))
  plot(RFsimulate(model, x=x, seed=i))
}

## snd, part 1
## note that the fist 'exp' refers to the exponential function,
## the second to the exponential distribution.
(model1 <- RMgauss(var=exp(3), scale=exp(rate=1)))
x <- 1:100/10
plot(z1 <- RFsimulate(model=model, x=x))

## snd, part 2
## exactly the same result as in the previous example
(model2 <- RMgauss(var=exp(3), scale=RRdistr("exp", rate=1)))
plot(z2 <- RFsimulate(model=model, x=x))
all.equal(model1, model2)

Vector Of Independent Gaussian Random Variables

Description

RRgauss defines the d-dimensional vector of independent Gaussian random variables.

Usage

RRgauss(mu, sd, log)

Arguments

mu, sd, log

see Normal. Here, the components can be vectors, leading to multivariate distibution with independent components.

Details

It has the same effect as RRdistr(norm(mu=mu, sd=sd, log=log)).

Value

RRgauss returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RRdistr, RRunif.

Do not mix up RRgauss with RMgauss or RPgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
r <- RFrdistr(RRgauss(mu=c(1,5)), n=1000, dim=2)
plot(r[1,], r[2, ])

Location and Scale Modification of A Distribution

Description

RRloc modifies location and scale of a distribution.

Usage

RRloc(phi, mu, scale, pow)

Arguments

phi

distribution RMmodel

mu

location shift

scale

scale modification

pow

argument for internal use only

Details

It has the same effect as RRdistr(norm(mu=mu, sd=sd, log=log))

Value

RRloc returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RRdistr, RRgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## empirical density of the distribution 'RRspheric'
model <- RRspheric(balldim=2)
hist(RFrdistr(model, n=1000), 50)

## empirical density of the distribution 'RRspheric', shifted by 3
model <- RRloc(mu=3, RRspheric(balldim=2))
hist(RFrdistr(model, n=1000), 50)

Random Sample From The Modulus Of A Function

Description

RRmcmc draws a random sample from the modulus of any given function (provided the integral is finite).

Usage

RRmcmc(phi, mcmc_n, sigma, normed, maxdensity, rand.loc, gibbs)

Arguments

phi

an arbitrary integrable function

mcmc_n

positive integer. Every mcmc_nth element of the MCMC chain is returned.

sigma

positive real number. The MCMC update is done by adding a normal variable with standard deviation sigma.

normed

logical. Only used if the value of the density is calculated. If FALSE the unnormed value given by phi is returned.

Default: FALSE.

maxdensity

positive real number. The given density is truncated at maxdensity.

Default: 1000.

rand.loc

logical. Internal. Do not change the value.

Default: FALSE.

gibbs

logical. If TRUE only one component is updated at a time.

Default: FALSE.

Value

RRmcmc returns an object of class RMmodel.

Note

The use of RRmcmc is completely on the risk of the user. There is no way to check whether the integral of the modulus is finite.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RR, RRdistr, RMuser.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
## here a model with random scale parameter

## not exponential, but the Laplace distribution as symmetry is assumed
z <- RFrdistr(RRmcmc(RMexp(), sigma=1), n=10000, cores=1)
hist(z, 100, freq=FALSE)
curve(0.5 * exp(-abs(x)), add=TRUE, col="blue") ## Laplace distribution

Random scaling used with balls

Description

Approximates an isotropic decreasing density function by a density function that is isotropic with respect to the l1l_1 norm.

Usage

RRrectangular(phi, safety, minsteplen, maxsteps, parts, maxit,
             innermin, outermax, mcmc_n, normed, approx, onesided)

Arguments

phi

a shape function; it is the user's responsibility that it is non-negative. See Details.

safety, minsteplen, maxsteps, parts, maxit, innermin, outermax, mcmc_n

Technical arguments to run an algorithm to simulate from this distribution. See RFoptions for the default values.

normed

logical. If FALSE then the norming constant cc in the Details is set to 11. This affects the values of the density function, the probability distribution and the quantile function, but not the simulation of random variables.

approx

logical. Default is TRUE. If TRUE the isotropic distribution with respect to the l1l_1 norm is returned. If FALSE then the exact isotropic distribution with respect to the l2l_2 norm is simulated. Neither the density function, nor the probability distribution, nor the quantile function will be available if approx=TRUE.

onesided

logical. Only used for univariate distributions. If TRUE then the density is assumed to be non-negative only on the positive real axis. Otherwise the density is assumed to be symmetric.

Details

This model defines an isotropic density function $f$ with respect to the l1l_1 norm, i.e. f(x)=cϕ(xl1)f(x) = c \phi(\|x\|_{l_1}) with some function ϕ\phi. Here, cc is a norming constant so that the integral of ff equals one.

In case that ϕ\phi is monotonically decreasing then rejection sampling is used, else MCMC.

The function ϕ\phi might have a polynomial pole at the origin and asymptotical decreasing of the form xβexp(xδ)x^\beta exp(-x^\delta).

Value

RRrectangular returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RRdistr, RRgauss.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
# simulation of Gaussian variables (in a not very straightforward way):
distr <- RRrectangular(RMgauss(), approx=FALSE)
z <- RFrdistr(distr, n=1000000)
hist(z, 200, freq=!TRUE)
x <- seq(-10, 10, 0.1)
lines(x, dnorm(x, sd=sqrt(0.5)))


#creation of random variables whose density is proportional
# to the spherical model:
distr <- RRrectangular(RMspheric(), approx=FALSE)
z <- RFrdistr(distr, n=1000000)
hist(z, 200, freq=!TRUE)

x <- seq(-10, 10, 0.01)
lines(x, 4/3 * RFcov(RMspheric(), x))

Random scaling used with balls

Description

This model delivers the distribution of the radius of a ball obtained by the intersection of a balldim-dimensional ball with diameter R by a spacedimspacedim-dimensional hyperplane that has uniform distance from the center.

Usage

RRspheric(spacedim, balldim, R)

Arguments

spacedim

dimension of the hyperplane; defaults to 1.

balldim

the dimension of the ball

R

radius. Default: 1.

Value

RRspheric returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RMball.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

hist(RFrdistr(RRspheric(balldim=2), n=1000), 50)

Uniform Distribution in Higher Dimensions

Description

The model refers to the d-dimensional uniform distribution on a rectangular window.

Usage

RRunif(min, max, normed)

Arguments

min, max

lower and upper corner of a rectangular window

normed

logical with default value TRUE.

Advanced. If FALSE then the indicator function for the window is not normed to get a probability distribution. Nonetheless, random drawing from the distribution still works.

Details

In the one-dimensional case it has the same effect as RRdistr(unif(min=min, max=max, log=log)).

Value

RRunif returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RMmodel, RRdistr, RRgauss, RRspheric.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
## uniform distribution on [0,2] x [-2, -1]
RFrdistr(RRunif(c(0, -2), c(2, -1)), n=5, dim=2)
RFpdistr(RRunif(c(0, -2), c(2, -1)), q=c(1, -1.5), dim=2)
RFddistr(RRunif(c(0, -2), c(2, -1)), x=c(1, -1.5), dim=2)

Models for stationary max-stable random fields

Description

Here, the code of the paper on ‘Models for stationary max-stable random fields’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2002) Models for stationary max-stable random fields. Extremes 5, 33-44.

Examples

RFoptions(seed=0, xi=1)
## seed = 0 : *ANY* simulation will have the random seed 0; set
##            RFoptions(seed=NA) to make them all random again
## xi = 0.5: Frechet margins with alpha=2

## Due to change in the handling the seeds here are different from the
## seeds in the paper.

x <- seq(0, 10, length=128)

# Fig. 1-4
## Not run: \dontshow{plot(RFsimulate(RPsmith(RMgauss(s=1.5)), x, x))   # < 1 sec
plot(RFsimulate(RPsmith(RMball(s=RRspheric(2, 3,
R=3.3))), x, x)) # 30  sec
plot(RFsimulate(RPschlather(RMexp()), x, x))      #   1 sec
plot(RFsimulate(RPschlather(RMgauss()), x, x))    #  17 sec
}
## End(Not run)

On some covariance models based on normal scale mixtures

Description

Here, the code of the paper on ‘On some covariance models based on normal scale mixtures’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (2010) On some covariance models based on normal scale mixtures. Bernoulli, 16, 780-797.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

### Example 10 in Schlather (2010).
## The field below has more than 80 million points. So the simulation
## takes a while
y <- x <- seq(0, 10, len=256) ## currently does not work
T <- c(0, 0.02, 1275)
col <- c(topo.colors(300)[1:100], cm.colors(300)[c((1:50) * 2,
         101:150)])
y <- x <- seq(0, 10, len=5)
T <- c(0, 0.02, 4)
model <- RMcoxisham(mu=c(1, 1), D=matrix(nr=2, c(1, 0.5, 0.5, 1)),
                    RMwhittle(nu=1))
z <- RFsimulate(model, x, y, T=T, sp_lines=1500, every=10)
plot(z, MARGIN.slices=3, col=col)
plot(z, MARGIN.movie=3) # add 'file="ci.avi"' to get it stored

Systematic co-occurrence of tail correlation functions among max-stable processes

Description

Here, the code of the paper on ‘On some covariance models based on normal scale mixtures’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Strokorb, K., Ballani, F. and Schlather, M. (2014) Systematic co-occurrence of tail correlation functions among max-stable processes. Work in progress.

Examples


Methods relying on square roots of the covariance matrix

Description

Sequential method relying on square roots of the covariance matrix

Usage

RPsequential(phi, boxcox, back_steps, initial)

Arguments

phi

object of class RMmodel; specifies the covariance model to be simulated.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

back_steps

Number of previous instances on which the algorithm should condition. If less than one then the number of previous instances equals max / (number of spatial points).

Default: 10.

initial

First, N=(number of spatial points) * back_steps number of points are simulated. Then, sequentially, all spatial points for the next time instance are simulated at once, based on the previous back_steps instances. The distribution of the first N points is the correct distribution, but differs, in general, from the distribution of the sequentially simulated variables. We prefer here to have the same distribution all over (although only approximatively the correct one), hence do some initial sequential steps first. If initial is non-negative, then initial first steps are performed. If initial is negative, then back_steps - initial initial steps are performed. The latter ensures that none of the very first N variables are returned.

Default: -10.

Details

RPsequential is programmed for spatio-temporal models where the field is modelled sequentially in the time direction conditioned on the previous kk instances. For k=5k=5 the method has its limits for about 1000 spatial points. It is an approximative method. The larger kk the better. It also works for certain grids where the last dimension should contain the highest number of grid points.

Value

RPsequential returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

See Also

Gaussian, RP, RPdirect.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMgauss(var=10, s=10) + RMnugget(var=0.01)
plot(model, xlim=c(-25, 25))

z <- RFsimulate(model=RPsequential(model), 0:10, 0:10, n=4)
plot(z)

(Mixed) Moving Maxima

Description

RPsmith defines a moving maximum process or a mixed moving maximum process with finite number of shape functions.

Usage

RPsmith(shape, tcf, xi, mu, s)

Arguments

shape

an RMmodel giving the spectral function

tcf

an RMmodel specifying the extremal correlation function; either shape or tcf must be given. If tcf is given a shape function is tried to be constructed via the RMm2r construction of deterministic, monotone functions.

xi, mu, s

the extreme value index, the location parameter and the scale parameter, respectively, of the generalized extreme value distribution. See Details.

Details

The argument xi is always a number, i.e. ξ\xi is constant in space. In contrast, μ\mu and ss might be constant numerical values or (in future!) be given by an RMmodel, in particular by an RMtrend model.
For xi=0xi=0, the default values of mumu and ss are 00 and 11, respectively. For xi0xi\not=0, the default values of mumu and ss are 11 and ξ|\xi|, respectively, so that it defaults to the standard Frechet case if ξ>0\xi > 0.

It simulates max-stable processes ZZ that are referred to as “Smith model”.

Z(x)=maxi=1XiYi(xWi),Z(x) = \max_{i=1}^\infty X_i Y_i(x-W_i),

where (Wi,Xi)(W_i, X_i) are the points of a Poisson point process on Rd×(0,)\R^d \times (0, \infty) with intensity dwc/x2dxdw * c/x^2 dx and YiYY_i \sim Y are iid measurable random functions with E[max(0,Y(x))dx]<E[\int \max(0, Y(x)) dx] < \infty. The constant cc is chosen such that ZZ has standard Frechet margins.

Note

IMPORTANT: For consistency reasons with the geostatistical definitions in this package the scale argument differs froms the original definition of the Smith model! See the example below.

RPsmith depends on RRrectangular and its arguments.

Advanced options are maxpoints and max_gauss, see RFoptions.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Haan, L. (1984) A spectral representation for max-stable processes. Ann. Probab., 12, 1194-1204.

  • Smith, R.L. (1990) Max-stable processes and spatial extremes Unpublished Manuscript.

See Also

Advanced RMmodels, Auxiliary RMmodels, RMmodel, RPbernoulli, RPgauss, maxstable, maxstableAdvanced.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMball()
x <- seq(0, 1000, 0.2)
z <- RFsimulate(RPsmith(model, xi=0), x)
plot(z)
hist(z@data$variable1, 50, freq=FALSE)
curve(exp(-x) * exp(-exp(-x)), from=-3, to=8, add=TRUE)

## 2-dim
x <- seq(0, 10, 0.1) 
z <- RFsimulate(RPsmith(model, xi=0), x, x)
plot(z)

## original Smith model
x <- seq(0, 10, 0.05)
model <- RMgauss(scale = sqrt(2)) # !! cf. definition of RMgauss
z <- RFsimulate(RPsmith(model, xi=0), x, x)
plot(z)




## for some more sophisticated models see 'maxstableAdvanced'

Soil data of North Bavaria, Germany

Description

Soil physical and chemical data collected on a field in the Weissenstaedter Becken, Germany

Usage

data(soil)

Format

This data frame contains the following columns:

x.coord

x coordinates given in cm

y.coord

y coordinates given in cm

nr

number of the samples, which were taken in this order

moisture

moisture content [Kg/Kg * 100%]

NO3.N

nitrate nitrogen [mg/Kg]

Total.N

total nitrogen [mg/Kg]

NH4.N

ammonium nitrogen [mg/Kg]

DOC

dissolved organic carbon [mg/Kg]

N20N

nitrous oxide [mg/Kg dried substance]

Details

For technical reasons some of the data were obtained as differences of two measurements (which are not available anymore). Therefore, some of the data have negative values.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Source

The data were collected by Wolfgang Falk, Soil Physics Group, University of Bayreuth, Germany.

References

Falk, W. (2000) Kleinskalige raeumliche Variabilitaet von Lachgas und bodenchemischen Parameters [Small Scale Spatial Variability of Nitrous Oxide and Pedo-Chemical Parameters], Master thesis, University of Bayreuth, Germany.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

################################################################
## ##
## a geostatistical analysis that demonstrates ##
## features of the package 'RandomFields' ##
## ##
################################################################


data(soil)
str(soil)
soil <- RFspatialPointsDataFrame(
 coords = soil[ , c("x.coord", "y.coord")],
 data = soil[ , c("moisture", "NO3.N", "Total.N", "NH4.N", "DOC", "N20N")],
 RFparams=list(vdim=6, n=1)
)
dta <- soil["moisture"]


## plot the data first
colour <- rainbow(100)
plot(dta, col=colour)


## fit by eye
gui.model <- RFgui(dta) 
 

## fit by ML
model <- ~1 + RMwhittle(scale=NA, var=NA, nu=NA) + RMnugget(var=NA)
(fit <- RFfit(model, data=dta))
plot(fit, method=c("ml", "plain", "sqrt.nr", "sd.inv"),
     model = gui.model, col=1:8)

## Kriging ...
x <- seq(min(dta@coords[, 1]), max(dta@coords[, 1]), l=121)
k <- RFinterpolate(fit, x=x, y=x, data=dta)
plot(x=k, col=colour)
plot(x=k, y=dta, col=colour)

## what is the probability that at no point of the
## grid given by x and y the moisture is greater than 24 percent?
cs <- RFsimulate(model=fit@ml, x=x, y=x, data=dta, n=50)
plot(cs, col=colour)
plot(cs, y=dta, col=colour)
Print(mean(apply(as.array(cs) <= 24, 3, all))) ## about 40 percent ...

Transformation of an 'sp' object to an 'RFsp' object

Description

The function transforms an 'sp' object to an 'RFsp' object.

This explicit transformation is only necessary if several variables and repeated measurements are given.

Usage

sp2RF(sp, param=list(n=1, vdim=1))

Arguments

sp

an ‘sp’ object

param

n: number of repetitions; vdim: the number of variables (multivariability)

Value

sp2RF returns an object of class RFsp.

Note

The two options varnames and coordnames, cf. section ‘coords’ in RFoptions, might be useful.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFsp

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

p <- 100
n <- 5
x <- runif(p, 0, 1)
y <- runif(p, 0, 1)
z <- RFsimulate(RMexp(), x=x, y=y, n=n)
z1 <- z2 <- as.data.frame(z)
coordinates(z2) <- ~coords.x1 + coords.x2

(emp.var <- RFvariogram(data=z))
(emp.var1 <- RFvariogram(data=z1))
(emp.var2 <- RFvariogram(data=sp2RF(z2, param=list(n=n, vdim=1))))

stopifnot(all.equal(emp.var, emp.var1))
stopifnot(all.equal(emp.var, emp.var2))

Methods that are specific to certain covariance models

Description

This model determines that the (Gaussian) random field should be modelled by a particular method that is specific to the given covariance model.

Usage

RPspecific(phi, boxcox)

Arguments

phi

object of class RMmodel; specifies the covariance model to be simulated.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

Details

RPspecific is used for specific algorithms or specific features for simulating certain covariance functions.

  • RMplus is able to simulate separately the fields given by its summands. This is necessary, e.g., when a trend model RMtrend is involved.

  • RMmult for Gaussian random fields only. RMmult simulates the random fields of all the components and multiplies them. This is repeated several times and averaged.

  • RMS Then, for instance, sqrt(var) is multiplied onto the (Gaussian) random field after the field has been simulated. Hence, when var is random, then for each realization of the Gaussian field (for n>1 in RFsimulate) a new realization of var is used.

    Further, new coordinates are created where the old coordinates have been divided by the scale and/or multiplied with the Aniso matrix or a projection has been performed.

    RPspecific(RMS()) is called internally when the user wants to simulate Anisotropic fields with isotropic methods, e.g. RPtbm.

  • RMmppplus

  • RMtrend

Note that RPspecific applies only to the first model or operator in the argument phi.

Value

RPspecific returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

See Also

Gaussian, RP.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## example for implicit use
model <- RMgauss(var=10, s=10) + RMnugget(var=0.1)
plot(model)
plot(RFsimulate(model=model, 0:10, 0:10, n=4))
## The following function shows the internal structure of the model.
## In particular, it can be seen that RPspecific is applied to RMplus.
RFgetModelInfo(level=0, which="internal")

## example for explicit use: every simulation has a different variance
model <- RPspecific(RMS(var=unif(min=0, max=100), RMgauss()))
x <- seq(0,50,0.02)
plot(RFsimulate(model, x=x, n=4), ylim=c(-15,15))

Spectral turning bands method

Description

The spectral turning bands method is a simulation method for stationary Gaussian random fields (Mantoglou and Wilson, 1982). It makes use of Bochners's theorem and the corresponding spectral measure Ξ\Xi for a given covariance function C(h)C(h). For xRdx \in {\bf R}^d, the field

Y(x)=2cos(<V,x>+2πU)Y(x)= \sqrt{2} cos(<V,x> + 2 \pi U)

with V ΞV ~ \Xi and U Ufo((0,1))U ~ Ufo((0,1)) is a random field with covariance function C(h)C(h). A scaled superposition of many independent realizations of YY gives a Gaussian field according to the central limit theorem. For details see Lantuejoul (2002). The standard method allows for the simulation of 2-dimensional random fields defined on arbitrary points or arbitrary grids.

Usage

RPspectral(phi, boxcox, sp_lines, sp_grid, prop_factor, sigma)

Arguments

phi

object of class RMmodel; specifies the covariance model to be simulated.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

sp_lines

Number of lines used (in total for all additive components of the covariance function).

Default: 2500.

sp_grid

Logical. The angle of the lines is random if grid=FALSE, and kπ/k\pi/sp_lines for kk in 1:sp_lines, otherwise. This argument is only considered if the spectral measure, not the density is used.

Default: TRUE.

prop_factor

positive real value. Sometimes, the spectral density must be sampled by MCMC. Let pp be the average rejection rate. Then the chain is sampled every nnth point where n=log(p)n = |log(p)| *prop_factor.

Default: 50.

sigma

real. Considered if the Metropolis algorithm is used. It gives the standard deviation of the multivariate normal distribution of the proposing distribution. If sigma is not positive then RandomFields tries to find a good choice for sigma itself.

Default: 0.

Value

RPspectral returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Lantuejoul, C. (2002) Geostatistical Simulation: Models and Algorithms. Springer.

  • Mantoglou, A. and J. L. Wilson (1982), The Turning Bands Method for simulation of random fields using line generation by a spectral method. Water Resour. Res., 18(5), 1379-1394.

See Also

Gaussian, RP, RPtbm.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RPspectral(RMmatern(nu=1))
y <- x <- seq(0,10, len=400)
z <- RFsimulate(model, x, y, n=2)
plot(z)

Covariance models valid on a sphere

Description

This page summarizes the covariance models that can be used for spherical coordinates (and earth coordinates).

Details

The following models are available:

Completely monotone functions allowing for arbitrary scale

RMbcw Model bridging stationary and intrinsically stationary processes for α1\alpha \le 1 and β<0\beta < 0
RMcubic cubic model
RMdagum Dagum model with β<γ\beta < \gamma and γ1\gamma \le 1
RMexp exponential model
RMgencauchy generalized Cauchy family with α1\alpha \le 1 (and arbitrary β>0\beta> 0)
RMmatern Whittle-Matern model with ν1/2\nu \le 1/2
RMstable symmetric stable family or powered exponential model with α1\alpha \le 1
RMwhittle Whittle-Matern model, alternative parametrization with ν1/2\nu \le 1/2

Other isotropic models with arbitrary scale

RMconstant spatially constant model
RMnugget nugget effect model

Compactly supported covariance functions allowing for scales up to π\pi (or 180180 degrees)

RMaskey Askey's model
RMcircular circular model
RMgengneiting Wendland-Gneiting model; differentiable models with compact support
RMgneiting differentiable model with compact support
RMspheric spherical model

Anisotropic models

None up to now.

Basic Operators

RMmult, * product of covariance models
RMplus, + sum of covariance models or variograms

See RMmodels for cartesian models.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

coordinate systems, RMmodels, RMtrafo.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

RFgetModelNames(isotropy=c("spherical isotropic"))

## an example of a simple model valid on a sphere
model <- RMexp(var=1.6, scale=0.5) + RMnugget(var=0) #exponential + nugget
plot(model)


## a simple simulation
l <- seq(0, 85, 1.2)
coord <- cbind(lon=l, lat=l)


z <- RFsimulate(RMwhittle(s=30, nu=0.45), coord, grid=TRUE) # takes 1 min
plot(z)


z <- RFsimulate(RMwhittle(s=500, nu=0.5), coord, grid=TRUE,
                new_coord_sys="orthographic", zenit=c(25, 25)) 
plot(z)


z <- RFsimulate(RMwhittle(s=500, nu=0.5), coord, grid=TRUE,
                new_coord_sys="gnomonic", zenit=c(25, 25)) 
plot(z)


## space-time modelling on the sphere
sigma <- 5 * sqrt((R.lat()-30)^2 + (R.lon()-20)^2)
model <- RMprod(sigma) * RMtrafo(RMexp(s=500, proj="space"), "cartesian") *
  RMspheric(proj="time") 
z <- RFsimulate(model, 0:10, 10:20, T=seq(0, 1, 0.1),
                coord_system="earth", new_coordunits="km")
plot(z, MARGIN.slices=3)

Methods relying on square roots of the covariance matrix

Description

Methods relying on square roots of the covariance matrix

Usage

RPdirect(phi, boxcox)

Arguments

phi

object of class RMmodel; specifies the covariance model to be simulated.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

Details

RPdirect is based on the well-known method for simulating any multivariate Gaussian distribution, using the square root of the covariance matrix. The method is pretty slow and limited to about 12000 points, i.e. a 20x20x20 grid in three dimensions. This implementation can use the Cholesky decomposition and the singular value decomposition. It allows for arbitrary points and arbitrary grids.

Value

RPdirect returns an object of class RMmodel.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Schlather, M. (1999) An introduction to positive definite functions and to unconditional simulation of random fields. Technical report ST 99-10, Dept. of Maths and Statistics, Lancaster University.

See Also

Gaussian, RP, RPsequential.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
model <- RMgauss(var=10, s=10) + RMnugget(var=0.01)
plot(model, xlim=c(-25, 25))

z <- RFsimulate(model=RPdirect(model), 0:10, 0:10, n=4)
plot(z)

Covariance Models for Random Vector Fields

Description

Here, the code of the paper on ‘Covariance Models for Random Vector Fields’ is given.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Scheuerer, M. and Schlather, M. (2012) Covariance Models for Random Vector Fields. Stochastic Models, 82, 433-451.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

Tail correlation function of the Brown-Resnick process

Description

The models define various shape functions for max-stable processes for a given tail correlation function.

Usage

RMm2r(phi)
RMm3b(phi)
RMmps(phi)

Arguments

phi

a model for a tail correlation function belonging to the Gneiting class HdH_d

Details

RMm2r used with RPsmith defines a monotone shape function that corresponds to a tail correlation function belonging to Gneiting's class HdH_d. Currently, the function is implemented for dimensions 1 and 3. Called as such it returns the corresponding monotone function.

RMm3b used with RPsmith defines balls with random radius that corresponds to a tail correlation function belonging to Gneiting's class HdH_d. Currently, the function is implemented for dimensions 1 and 3. (Note that in Strokorb et al. (2014) the density function for twice the radius is considered.) Called as such it returns the corresponding density function for the radius of the balls.

RMmps used with RPsmith defines random hyperplane polygons that correspond to a tail correlaton function belonging to Gneiting's class HdH_d. It currently only allows for RMbrownresnick(RMfbm(alpha=1)) and dimension 2. Called as such it returns the tcf defined by the submodel – this definition may change in future.

Value

object of class RMmodel

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Strokorb, K. (2013) Properties of the Extremal Coefficient Functions. Univ. Goettingen. PhD thesis.

  • Strokorb, K., Ballani, F. and Schlather, M. (2014) In Preparation.

See Also

RFsimulate, RMmodel.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

model <- RMbrownresnick(RMfbm(alpha=1.5, s=0.2))
plot(RMm2r(model))

x <- seq(0, 10, 0.005)
z <- RFsimulate(RPsmith(RMm2r(model), xi=0), x)
plot(z, type="p", pch=20)

Covariance models valid for max-stable random fields

Description

This page summarizes the models that can be used for tail correlation functions.

Details

The following models are available:

Completely monotone functions allowing for arbitrary scale

RMbcw Model bridging stationary and intrinsically stationary processes for alpha <= 1 and beta < 0
RMdagum Dagum model with β<γ\beta < \gamma and γ1\gamma \le 1
RMexp exponential model
RMgencauchy generalized Cauchy family with α1\alpha \le 1 (and arbitrary β>0\beta> 0)
RMmatern Whittle-Matern model with ν1/2\nu \le 1/2
RMstable symmetric stable family or powered exponential model with α1\alpha \le 1
RMwhittle Whittle-Matern model, alternative parametrization with ν1/2\nu \le 1/2

Other isotropic models with arbitrary scale

RMnugget nugget effect model

Compactly supported covariance functions

RMaskey Askey's model
RMcircular circular model
RMconstant identically constant
RMcubic cubic model
RMgengneiting Wendland-Gneiting model; differentiable models with compact support
RMgneiting differentiable model with compact support
RMspheric spherical model

Anisotropic models

None up to now.

Basic Operators

RMmult, * product of covariance models
RMplus, + sum of covariance models or variograms

Operators related to process constructions

RMbernoulli correlation of binary fields
RMbrownresnick tcf of a Brown-Resnick process
RMschlather tcf of an extremal Gaussian process / Schlather process
RMm2r M2 process with monotone shape function
RMm3b M3 process with balls of random radius
RMmps M3 process with hyperplane polygons

See RMmodels for cartesian models.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

  • Strokorb, K., Ballani, F., and Schlather, M. (2015) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, 18, 241-271

See Also

coordinate systems, RM, RMmodels, RMtrafo.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
RFgetModelNames(type="tail")

## an example of a simple model
model <- RMexp(var=1.6, scale=0.5) + RMnugget(var=0) #exponential + nugget
plot(model)

Turning Bands method

Description

The Turning Bands method is a simulation method for stationary, isotropic (univariate or multivariate) random fields in any dimension and defined on arbitrary points or arbitrary grids. It performs a multidimensional simulation by superposing lower-dimensional fields. In fact, the Turning Bands method is called with the Turning Bands model, see RMtbm.
For details see RMtbm.

Usage

RPtbm(phi, boxcox, fulldim, reduceddim, layers, lines,
      linessimufactor, linesimustep, center, points)

Arguments

phi

object of class RMmodel; specifies the covariance function to be simulated; a univariate stationary isotropic covariance model (see RFgetModelNames(type="positive definite", domain="single variable", isotropy="isotropic", vdim=1)) which is valid in dimension fulldim.

boxcox

the one or two parameters of the box cox transformation. If not given, the globally defined parameters are used. See RFboxcox for details.

fulldim

a positive integer. The dimension of the space of the random field to be simulated.

reduceddim

a positive integer; less than fulldim. The dimension of the auxiliary hyperplane (most frequently a line, i.e. reduceddim=1) used in the simulation.

layers

a boolean value; for space-time model. If TRUE then the turning layers are used whenever a time component is given. If NA the turning layers are used only when the traditional TBM is not applicable. If FALSE then turning layers may never be used.

Default: TRUE.

lines

Number of lines used. Default: 60.

linessimufactor

linessimufactor or linesimustep must be non-negative; if linesimustep is positive then linessimufactor is ignored. If both arguments are naught then points is used (and must be positive). The grid on the line is linessimufactor-times finer than the smallest distance. See also linesimustep.

Default: 2.0.

linesimustep

If linesimustep is positive the grid on the line has lag linesimustep. See also linessimufactor.

Default: 0.0.

center

Scalar or vector. If not NA, the center is used as the center of the turning bands for fulldim. Otherwise the center is determined automatically such that the line length is minimal. See also points and the examples below.

Default: NA.

points

integer. If greater than 0, points gives the number of points simulated on the TBM line, hence must be greater than the minimal number of points given by the size of the simulated field and the two parameters linessimufactor and linesimustep. If points is not positive the number of points is determined automatically. The use of center and points is highlighted in an example below.

Default: 0.

Details

  • 2-dimensional case
    It is generally difficult to use the turning bands method (RPtbm) directly in the 2-dimensional space. Instead, 2-dimensional random fields are frequently obtained by simulating a 3-dimensional random field (using RPtbm) and taking a 2-dimensional cross-section. See also the arguments fulldim and reduceddim.

  • 4-dimensional case
    The turning layers can be used for the simulations with a (formal) time component. It works for all isotropic models, some special models such as RMnsst, and multiplicative models that separate the time component.

Value

RPtbm returns an object of class RMmodel.

Note

Both the precision and the simulation time depend heavily on linesimustep and linessimufactor. For covariance models with larger values of the scale parameter, linessimufactor=2 is too small.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

References

Turning bands

  • Lantuejoul, C. (2002) Geostatistical Simulation: Models and Algorithms. Springer.

  • Matheron, G. (1973). The intrinsic random functions and their applications. Adv. Appl. Probab., 5, 439-468.

  • Strokorb, K., Ballani, F., and Schlather, M. (2014) Tail correlation functions of max-stable processes: Construction principles, recovery and diversity of some mixing max-stable processes with identical TCF. Extremes, Submitted.

Turning layers

  • Schlather, M. (2011) Construction of covariance functions and unconditional simulation of random fields. In Porcu, E., Montero, J.M. and Schlather, M., Space-Time Processes and Challenges Related to Environmental Problems. New York: Springer.

See Also

Gaussian, RP, RPspectral.

Examples

RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again

## isotropic example that forces the use of the turning bands method
model <- RPtbm(RMstable(s=1, alpha=1.8))
x <- seq(-3, 3, 0.1)
z <- RFsimulate(model=model, x=x, y=x)
plot(z)

## anisotropic example that forces the use of the turning bands method
model <- RPtbm(RMexp(Aniso=matrix(nc=2, rep(1,4))))
z <- RFsimulate(model=model, x=x, y=x)
plot(z)

## isotropic example that uses the turning layers method
model <- RMgneiting(orig=FALSE, scale=0.4)
x <- seq(0, 10, 0.1)
z <- RFsimulate(model, x=x, y=x, z=x, T=c(1,1,5))
plot(z, MARGIN.slices=4, MARGIN.movie=3)

Trend Modelling

Description

The coding of trends, in particular multivariate trends, will be described here.

Details

See RFcalc, RMtrend and also the examples below for some insight on the possibilities of trend modelling.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

See Also

RFcalc, RM, RMmodels, RMtrend, RMmodelsMultivariate.

Examples

data(ca20) ## data set originally from geoR
head(ca20.df)
RFoptions(coordnames=c("east", "north"), varnames="data") 

## covariance model with variance, scale and nugget to be estimated;
## just to abbreviate later on
M <- RMexp(var=NA, scale=NA) + RMnugget(var=NA)
 

## short definition of a trend using the fact that ca20.df is a
## data.frame
ca20.RFmod02 <- ~ 1 + altitude + M
(ca20.fit02.RF <- RFfit(ca20.RFmod02, data=ca20.df, M=M))

## long definition which also allows for more general constructions
ca20.RFmod02 <- NA + NA*RMcovariate(ca20.df$altitude) + M 
(ca20.fit02.RF <- RFfit(ca20.RFmod02, data=ca20.df))

## Not run: 
## Note that the following also works.
## Here, the covariance model must be the first summand
ca20.RFmod02 <- M + NA + ca20.df$altitude 
print(ca20.fit02.RF <- RFfit(ca20.RFmod02, data=ca20.df))

### The following does NOT work, as R assumes (NA + ca20.df$altitude) + M
### In particular, the model definition gives a warning, and the
### RFfit call gives an error: 
(ca20.RFmod02 <- NA + ca20.df$altitude + M) 
try(ca20.fit02.RF <- RFfit(ca20.RFmod02, data=ca20.df)) ### error ...

## factors:
ca20.RFmod03 <- ~ 1 + area + M ### 
(ca20.fit03.RF <- RFfit(ca20.RFmod03, data=ca20.df, M=M))

## End(Not run)

Pressure and temperature forecast errors over the Pacific Northwest

Description

Meteorological dataset, which consists of differences between forecasts and observations (forecasts minus observations) of temperature and pressure at 157 locations in the North American Pacific Northwest.

Usage

data(weather)

Format

The data frame weather contains the following columns:

pressure

in units of Pascal

temperature

in units of degree Celcius

lon

longitudinal coordinates of the locations

lat

latitude coordinates of the locations

Furthermore, some results obtained from the data analysis in jss14 are delivered that are pars.model, pars, whole.model, whole.

Finally, the variable information contains packing information (the date and the version of RandomFields).

Details

The forecasts are from the GFS member of the University of Washington regional numerical weather prediction ensemble (UWME; Grimit and Mass 2002; Eckel and Mass 2005); they were valid on December 18, 2003 at 4 pm local time, at a forecast horizon of 48 hours.

Author(s)

Martin Schlather, [email protected], https://www.wim.uni-mannheim.de/schlather/

Source

The data were obtained from Cliff Mass and Jeff Baars from the University of Washington Department of Atmospheric Sciences.

References

  • Eckel, A. F. and Mass, C. F. (2005) Aspects of effective mesoscale, short-range ensemble forecasting Wea. Forecasting 20, 328-350.

  • Gneiting, T., Kleiber, W. and Schlather, M. (2010) Matern cross-covariance functions for multivariate random fields J. Amer. Statist. Assoc. 105, 1167-1177.

  • Grimit, E. P. and Mass, C. F. (2002) Initial results of a mesoscale short-range forecasting system over the Pacific Northwest Wea. Forecasting 17, 192-205.

See Also

A reanalysis has been performed in Section 5 of the jss14 paper.

Examples

## See 'jss14'.