| Title: | Species Distribution Modelling Tools: Tools for processing data associated with species distribution modelling exercises |
|---|---|
| Description: | This packages provides a set of tools for post processing the outcomes of species distribution modeling exercises. It includes novel methods for comparing models and tracking changes in distributions through time. It further includes methods for visualizing outcomes, selecting thresholds, calculating measures of accuracy and landscape fragmentation statistics, etc.. This package was made possible in part by financial support from the Australian Research Council & ARC Research Network for Earth System Science. |
| Authors: | Jeremy VanDerWal, Lorena Falconi, Stephanie Januchowski, Luke Shoo and Collin Storlie |
| Maintainer: | ORPHANED |
| License: | GPL (>= 3) |
| Version: | 1.1-221.2 |
| Built: | 2024-12-07 02:51:09 UTC |
| Source: | https://github.com/cran/SDMTools |
accuracy estimates six measures of accuracy for
presence-absence or presence-psuedoabsence data. These
include AUC, ommission rates, sensitivity, specificity,
proportion correctly identified and Kappa.
Note: this method will exclude any missing data.
accuracy(obs, pred, threshold = 0.5)accuracy(obs, pred, threshold = 0.5)
obs |
a vector of observed values which must be 0 for absences and 1 for occurrences |
pred |
a vector of the same length as |
threshold |
this can be: |
a data.frame with seven columns:
threshold |
the threshold values representing each row of data |
AUC |
the AUC given the defined threshold value |
ommission.rate |
the ommission rate as a proportion of true occurrences misidentified given the defined threshold value |
sensitivity |
the sensitivity given the defined threshold value |
specificity |
the specificity given the defined threshold value |
prop.correct |
the proportion of the presence and absence records correctly identified given the defined threshold value |
Kappa |
the Kappa statistic of the model given the defined threshold value |
Jeremy VanDerWal [email protected]
auc, Kappa,
omission, sensitivity,
specificity, prop.correct,
confusion.matrix
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate accuracy of the model with a single threshold value accuracy(obs,pred,threshold=0.5) #calculate accuracy given several defined thresholds accuracy(obs,pred,threshold=c(0.33,0.5,0.66)) #calculate accuracy given a number of equal interval thresholds accuracy(obs,pred,threshold=20)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate accuracy of the model with a single threshold value accuracy(obs,pred,threshold=0.5) #calculate accuracy given several defined thresholds accuracy(obs,pred,threshold=c(0.33,0.5,0.66)) #calculate accuracy given a number of equal interval thresholds accuracy(obs,pred,threshold=20)
asc.from.raster and asc.from.sp extracts data
from objects of class 'RasterLayer' (raster package) and
class 'SpatialGridDataFrame' (sp package) into an object of
class 'asc' (SDMTools & adehabitat packages). raster.from.asc and sp.from.asc does the
reverse.as.asc creates an object of class
'asc' (SDMTools & adehabitat packages) from a matrix of
data. Code & helpfile associated with as.asc were
modified from adehabitat package.
asc.from.raster(x) raster.from.asc(x, projs = NA) asc.from.sp(x) sp.from.asc(x, projs = CRS(as.character(NA))) as.asc(x, xll = 1, yll = 1, cellsize = 1, type = c("numeric", "factor"), lev = levels(factor(x)))asc.from.raster(x) raster.from.asc(x, projs = NA) asc.from.sp(x) sp.from.asc(x, projs = CRS(as.character(NA))) as.asc(x, xll = 1, yll = 1, cellsize = 1, type = c("numeric", "factor"), lev = levels(factor(x)))
x |
is an object of class 'asc', 'RasterLayer' or
'SpatialGridDataFrame'. For the function |
projs |
is a CRS projection string of the Proj4 package |
xll |
the x coordinate of the center of the lower left pixel of the map |
yll |
the y coordinate of the center of the lower left pixel of the map |
cellsize |
the size of a pixel on the studied map |
type |
a character string. Either |
lev |
if |
These functions provide capabilities of using scripts / functions from many packages including adehabitat (plus e.g, SDMTools), sp (plus e.g., maptools, rgdal) and raster.
Returns an object of class requested.
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) str(tasc) #convert to RasterLayer traster = raster.from.asc(tasc) str(traster) #convert to SpatialGridDataFrame tgrid = sp.from.asc(tasc) str(tgrid) #create a basic object of class asc tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc)#create a simple object of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) str(tasc) #convert to RasterLayer traster = raster.from.asc(tasc) str(traster) #convert to SpatialGridDataFrame tgrid = sp.from.asc(tasc) str(tgrid) #create a basic object of class asc tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc)
asc2dataframe converts a list of Esri ascii grid
formatted files to a data.frame consisting of only
locations with data.dataframe2asc converts a
data.frame or matrix with spatial data to Esri ascii grid
formatted files.
asc2dataframe(filenames, varnames = NULL, gz = FALSE) dataframe2asc(tdata, filenames = NULL, outdir = getwd(), gz = FALSE)asc2dataframe(filenames, varnames = NULL, gz = FALSE) dataframe2asc(tdata, filenames = NULL, outdir = getwd(), gz = FALSE)
filenames |
is a vector of file names |
varnames |
is a vector of names for the output columns, and must be the same length as files |
tdata |
is the data.frame which has y, x coordinates (OR lat,lon) and columns for the data to be output (MUST be in that order) |
outdir |
is the output directory, the default is the current working directory |
gz |
boolean defining if the ascii grid files are gzip compressed |
asc2dataframe: The ascii grid files can be read in gzip compress format. The dataframe returned contains the X and Y coordinate columns followed by columns of data.
dataframe2asc: If filenames is null, column names will be used. The data.frame has to contain the Y and X coordinates and the data as columns. The ascii grid files can be created as gzip compress format and would be saved in the outdir.
asc2dataframe |
Returns a dataframe with XY coordinates and the data of each ascii grid files, as columns. |
dataframe2asc |
Returns an asc grid file for each data column within the data.frame. |
Lorena Falconi [email protected]
#Create 2 ascii files y=seq(10,50,0.5) x=seq(140,180,0.5) cellsize=0.5 data1=sample(160,140) data2=sample(158,140) out1.asc=as.asc(matrix(data1,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) out2.asc=as.asc(matrix(data2,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) #write the ascii files to the work directory write.asc(out1.asc, 'out1.asc') write.asc(out2.asc, 'out2.asc') #list the ascii files ascfiles=c('out1.asc', 'out2.asc') #generate a dataframe from the ascii files tdata=asc2dataframe(ascfiles) tdata #remove the files unlink('out1.asc'); unlink('out2.asc') #convert the dataframe tdata to ascii grid files dataframe2asc(tdata) #remove the files unlink('var.1.asc'); unlink('var.2.asc')#Create 2 ascii files y=seq(10,50,0.5) x=seq(140,180,0.5) cellsize=0.5 data1=sample(160,140) data2=sample(158,140) out1.asc=as.asc(matrix(data1,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) out2.asc=as.asc(matrix(data2,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) #write the ascii files to the work directory write.asc(out1.asc, 'out1.asc') write.asc(out2.asc, 'out2.asc') #list the ascii files ascfiles=c('out1.asc', 'out2.asc') #generate a dataframe from the ascii files tdata=asc2dataframe(ascfiles) tdata #remove the files unlink('out1.asc'); unlink('out2.asc') #convert the dataframe tdata to ascii grid files dataframe2asc(tdata) #remove the files unlink('var.1.asc'); unlink('var.2.asc')
auc estimates the AUC of the ROC using a
Mann-Whitney U statistic.
Note: this method
will exclude any missing data.
auc(obs, pred)auc(obs, pred)
obs |
a vector of observed values which must be 0 for absences and 1 for occurrences |
pred |
a vector of the same length as |
Returns a single value represting the AUC value.
Jeremy VanDerWal [email protected]
Kappa, omission,
sensitivity, specificity,
prop.correct, confusion.matrix,
accuracy
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA) pred = runif(length(obs),0,1) #calculate AUC from the random data auc(obs,pred) #calculate an example 'perfect' AUC obs = obs[order(obs)] pred = pred[order(pred)] auc(obs,pred)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA) pred = runif(length(obs),0,1) #calculate AUC from the random data auc(obs,pred) #calculate an example 'perfect' AUC obs = obs[order(obs)] pred = pred[order(pred)] auc(obs,pred)
circular.averaging calculates the average direction
(0 - 360) given a vector of directions.vector.averaging calculates the average distance and
direction given a vector of directions and a vector of
distances.
circular.averaging(direction, deg = TRUE) vector.averaging(direction, distance, deg = TRUE)circular.averaging(direction, deg = TRUE) vector.averaging(direction, distance, deg = TRUE)
direction |
a vector of directions given in degrees
(0 - 360) if |
distance |
a vector of distances associated with each direction |
deg |
a boolean object defining if |
functions return NA if the average distance or direction is not valid... e.g., when averaging directions of 0 & 180 degrees, the result could theoretically be 90 or 270 but is practically neither.
circular.averaging returns the average direction
while vector.averaging returns a list with 2
elements distance & direction
Jeremy VanDerWal [email protected] & Lorena Falconi [email protected]
#EXAMPLE circular.averaging circular.averaging(c(0,90,180,270)) #result is NA circular.averaging(c(70,82,96,110,119,259)) #EXAMPLE vector.averaging vector.averaging(c(10,20,70,78,108), distance=10) vector.averaging(c(159,220,258,273,310),distance=runif(5))#EXAMPLE circular.averaging circular.averaging(c(0,90,180,270)) #result is NA circular.averaging(c(70,82,96,110,119,259)) #EXAMPLE vector.averaging vector.averaging(c(10,20,70,78,108), distance=10) vector.averaging(c(159,220,258,273,310),distance=runif(5))
ClassStat calculates the class statistics for patch
types identified in a matrix of data or in a raster of
class 'asc' (SDMTools & adehabitat packages), 'RasterLayer'
(raster package) or 'SpatialGridDataFrame' (sp package).
ClassStat(mat, cellsize = 1, bkgd = NA, latlon = FALSE)ClassStat(mat, cellsize = 1, bkgd = NA, latlon = FALSE)
mat |
a matrix of data with patches identified as classes (unique integer values) as e.g., a binary lanscape of a species distribution or a vegetation map. Matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
cellsize |
cell size (in meters) is a single value representing the width/height of cell edges (assuming square cells) |
bkgd |
the background value for which statistics will not be calculated |
latlon |
boolean value representing if the data is geographic. If latlon == TRUE, matrix must be of class 'asc', 'RasterLayer' or 'SpatialGridDataFrame' |
The class statistics are based on statistics calculated by fragstats http://www.umass.edu/landeco/research/fragstats/fragstats.html.
a data.frame listing
class |
a particular patch type
from the original input matrix ( |
n.patches |
the number of patches of a particular patch type or in a class. |
total.area |
the sum of the areas (m2) of all patches of the corresponding patch type. |
prop.landscape |
the proportion of the total lanscape represented by this class |
patch.density |
the numbers of patches of the corresponding patch type divided by total landscape area (m2). |
total.edge |
the total edge length of a particular patch type. |
edge.density |
edge length on a per unit area basis that facilitates comparison among landscapes of varying size. |
landscape.shape.index |
a standardized measure of total edge or edge density that adjusts for the size of the landscape. |
largest.patch.index |
largest patch index quantifies the percentage of total landscape area comprised by the largest patch. |
mean.patch.area |
average area of patches. |
sd.patch.area |
standard deviation of patch areas. |
min.patch.area |
the minimum patch area of the total patch areas. |
max.patch.area |
the maximum patch area of the total patch areas. |
perimeter.area.frac.dim |
perimeter-area fractal dimension equals 2 divided by the slope of regression line obtained by regressing the logarithm of patch area (m2) against the logarithm of patch perimeter (m). |
mean.perim.area.ratio |
the mean of the ratio patch perimeter. The perimeter-area ratio is equal to the ratio of the patch perimeter (m) to area (m2). |
sd.perim.area.ratio |
standard deviation of the ratio patch perimeter. |
min.perim.area.ratio |
minimum perimeter area ratio |
max.perim.area.ratio |
maximum perimeter area ratio. |
mean.shape.index |
mean of shape index |
sd.shape.index |
standard deviation of shape index. |
min.shape.index |
the minimum shape index. |
max.shape.index |
the maximum shape index. |
mean.frac.dim.index |
mean of fractal dimension index. |
sd.frac.dim.index |
standard deviation of fractal dimension index. |
min.frac.dim.index |
the minimum fractal dimension index. |
max.frac.dim.index |
the maximum fractal dimension index. |
total.core.area |
the sum of the core areas of the patches (m2). |
prop.landscape.core |
proportional landscape core |
mean.patch.core.area |
mean patch core area. |
sd.patch.core.area |
standard deviation of patch core area. |
min.patch.core.area |
the minimum patch core area. |
max.patch.core.area |
the maximum patch core area. |
prop.like.adjacencies |
calculated from the adjacency matrix, which shows the frequency with which different pairs of patch types (including like adjacencies between the same patch type) appear side-by-side on the map (measures the degree of aggregation of patch types). |
aggregation.index |
computed simply as an area-weighted mean class aggregation index, where each class is weighted by its proportional area in the landscape. |
lanscape.division.index |
based on the cumulative patch area distribution and is interpreted as the probability that two randomly chosen pixels in the landscape are not situated in the same patch |
splitting.index |
based on the cumulative patch area distribution and is interpreted as the effective mesh number, or number of patches with a constant patch size when the landscape is subdivided into S patches, where S is the value of the splitting index. |
effective.mesh.size |
equals 1 divided by the total landscape area (m2) multiplied by the sum of patch area (m2) squared, summed across all patches in the landscape. |
patch.cohesion.index |
measures the physical connectedness of the corresponding patch type. |
Jeremy VanDerWal [email protected]
McGarigal, K., S. A. Cushman, M. C. Neel, and E. Ene. 2002. FRAGSTATS: Spatial Pattern Analysis Program for Categorical Maps. Computer software program produced by the authors at the University of Massachusetts, Amherst. Available at the following web site: www.umass.edu/landeco/research/fragstats/fragstats.html
#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1))) #calculate the patch statistics ps.data = PatchStat(ccl.mat) ps.data #calculate the class statistics cl.data = ClassStat(tmat) cl.data #identify background data is 0 cl.data = ClassStat(tmat,bkgd=0) cl.data#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1))) #calculate the patch statistics ps.data = PatchStat(ccl.mat) ps.data #calculate the class statistics cl.data = ClassStat(tmat) cl.data #identify background data is 0 cl.data = ClassStat(tmat,bkgd=0) cl.data
COGravity calculates the Centre of Gravity (or also
known as Centre of Mass) for point or raster spatial
data.
Note: NA data is automatically ommitted
from analysis.
COGravity(x, y = NULL, z = NULL, wt = NULL)COGravity(x, y = NULL, z = NULL, wt = NULL)
x |
a vector of e.g., longitudes or eastings, or a raster of class 'asc', 'RasterLayer' or 'SpatialGridDataFrame'. |
y |
a vector of e.g., latitudes or northings. |
z |
a vector of e.g., elevations. |
wt |
a vector or raster of class 'asc', 'RasterLayer' or 'SpatialGridDataFrame' representing weights for data. |
For raster-based data, if wt is missing, the values
of the ascii are assumed to be the weights; otherwise, the
values are assumed to be the z values.
Returns a named vector of data representing the Centre of Gravity in x, y & z dimensions (depending on data supplied).
Jeremy VanDerWal [email protected]
#create some points x = seq(154,110,length=25) y = seq(-10,-54,length=25) z = seq(100,200,length=25) wt = runif(25) #random weights #calculate the Centre of Gravity for these points COGravity(x,y,z,wt) #create a simple objects of class 'asc' x = as.asc(matrix(1:50,nr=50,nc=50)) wt = as.asc(matrix(runif(50),nr=50,nc=50)) #calculate COG with weighting defined in x COGravity(x) #calculate COG with weighting defined in wt (values in x are assumed elevation (z)) COGravity(x,wt=wt)#create some points x = seq(154,110,length=25) y = seq(-10,-54,length=25) z = seq(100,200,length=25) wt = runif(25) #random weights #calculate the Centre of Gravity for these points COGravity(x,y,z,wt) #create a simple objects of class 'asc' x = as.asc(matrix(1:50,nr=50,nc=50)) wt = as.asc(matrix(runif(50),nr=50,nc=50)) #calculate COG with weighting defined in x COGravity(x) #calculate COG with weighting defined in wt (values in x are assumed elevation (z)) COGravity(x,wt=wt)
compare.matrix compares the values within two
matrices (e.g., ESRI ArcInfo ASCII raster files) and
produces a biplot that shows the frequency of each data
combination shared between the matrices. The plot is
overlayed with contour lines that demarcate parts of the
the plot that share the same frequency of data
combinations.
NOTE: it is assumed the
matrices are of the same extent, cell size and scaled to be
the same units.
compare.matrix(x, y, nbins, ...)compare.matrix(x, y, nbins, ...)
x |
a matrix of data; the matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
y |
a matrix of data of the same extent, cell size and class as 'x' |
nbins |
number of equally spaced bins used to partition range of values in 'x' & 'y' |
... |
other graphical parameters defined by image(), contour(), or plot() |
Nothing is returned but images are created.
Luke Shoo [email protected]
#create some simple objects of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 10000, min = -1, max = 1) tasc2 = tasc + rnorm(n = 10000, mean = 1, sd = 1) #create some images #basic plot showing the density of data combinations shared #by the two matrices compare.matrix(tasc1,tasc2,20) #same as previous but with data partioned amoung more bins compare.matrix(tasc1,tasc2,50) #same as previous but altering the number of contour levels #and adding more graphical functions compare.matrix(tasc1,tasc2,50,nlevels=5, xlab='asc1',ylab='asc2', main='Comparison between asc and asc2', bg="grey")#create some simple objects of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 10000, min = -1, max = 1) tasc2 = tasc + rnorm(n = 10000, mean = 1, sd = 1) #create some images #basic plot showing the density of data combinations shared #by the two matrices compare.matrix(tasc1,tasc2,20) #same as previous but with data partioned amoung more bins compare.matrix(tasc1,tasc2,50) #same as previous but altering the number of contour levels #and adding more graphical functions compare.matrix(tasc1,tasc2,50,nlevels=5, xlab='asc1',ylab='asc2', main='Comparison between asc and asc2', bg="grey")
confusion.matrix calculates a confusion matrix.
Note: this method will exclude any missing data
confusion.matrix(obs, pred, threshold = 0.5)confusion.matrix(obs, pred, threshold = 0.5)
obs |
a vector of observed values which must be 0 for absences and 1 for occurrences |
pred |
a vector of the same length as |
threshold |
a single threshold value between 0 & 1 |
Returns a confusion matrix (table) of class 'confusion.matrix' representing counts of true & false presences and absences.
Jeremy VanDerWal [email protected]
auc, Kappa,
omission, sensitivity,
specificity, prop.correct,
accuracy
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix confusion.matrix(obs,pred,threshold=0.5)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix confusion.matrix(obs,pred,threshold=0.5)
ConnCompLabel is a 1 pass implementation of
connected components labelling. Here it is applied to
identify disjunt patches within a distribution.
The
raster matrix can be a raster of class 'asc' (adehabitat
package), 'RasterLayer' (raster package) or
'SpatialGridDataFrame' (sp package).
ConnCompLabel(mat)ConnCompLabel(mat)
mat |
is a binary matrix of data with 0 representing background and 1 representing environment of interest. NA values are acceptable. The matrix can be a raster of class 'asc' (this & adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
A matrix of the same dim and class of mat in which
unique components (individual patches) are numbered 1:n
with 0 remaining background value.
Jeremy VanDerWal [email protected]
Chang, F., C.-J. Chen, and C.-J. Lu. 2004. A linear-time component-labeling algorithm using contour tracing technique. Comput. Vis. Image Underst. 93:206-220.
#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1)))#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1)))
destination estimates the destination latitude and
longitude given a starting latitude and longitude, a
bearing and distance.
For general information on
Vincenty's formula, see e.g.,
http://en.wikipedia.org/wiki/Vincenty's_formulae. It
states:
Vincenty's formulae are two related
iterative methods used in geodesy to calculate the distance
between two points on the surface of an spheroid, developed
by Thaddeus Vincenty in 1975. They are based on the
assumption that the figure of the Earth is an oblate
spheroid, and hence are more accurate than methods such as
great-circle distance which assume a spherical Earth.
Note: this method assumes a locations are lat &
lon given in WGS 84.
destination(lat, lon, bearing, distance)destination(lat, lon, bearing, distance)
lat |
a single value or vector of values representing latitude in decimal degrees from -90 to 90 degrees. |
lon |
a single value or vector of values representing longitude in decimal degrees from -180 to 180 degrees. |
bearing |
a single value or vector of values representing the bearings (directions) of interest ranging from 0 to 360 degrees. |
distance |
a single value or vector of values representing the distances in metres to the destination. |
Typical useages are:
a single start
location, bearing and distance to give a single output
location
–output would be a single destination location
a single start location with one or more bearings or
distances to give multiple output locations
–output
would be a destination locations for each combination of
bearings and distances
multiple start locations with
a single bearing or distance
–output would be a
destination locations representing the bearing and distance
from each of the start locations
multiple start
locations with multiple bearings or distances
–output
would be a destination locations representing the
combinations of bearings and distances from each of the
start locations
– NOTE that the bearing and distance
vectors must be of the same length of the input lat and
long.
See examples for all possible usages.
Returns a data.frame with:
lon1 |
the original longitude |
lat1 |
the original latitude |
bearing |
the bearing used |
distance |
the distance used |
lon2 |
the destination longitude |
lat2 |
the destination latitude |
Jeremy VanDerWal [email protected]
The source code here was modified from
http://www.movable-type.co.uk/scripts/latlong-vincenty-direct.html.
Destinations were validated against Geoscience
Australia calculations
(http://www.ga.gov.au/geodesy/datums/vincenty_direct.jsp).
Vincenty, T. 1975. Direct and Inverse Solutions of Geodesics on the Ellipsoid with application of Nested Equations. Survey Review, vol XXII no 176. http://www.ngs.noaa.gov/PUBS_LIB/inverse.pdf
###single lat lons lats = -85; lons = 165 #single bearing & single distance destination(lats,lons,bearing=180,distance=500000) #multiple bearings destination(lats,lons,bearing=seq(0,360,length.out=9),distance=500000) #multiple bearings destination(lats,lons,bearing=45,distance=seq(0,5000000,length.out=11)) #multiple bearings, multiple distances destination(lats,lons,bearing=seq(0,360,length.out=9), distance=seq(0,5000000,length.out=11)) ###multiple lat lons lats = seq(-90,90,length.out=9); lons = seq(-180,180,length.out=9) #multiple lat lons but single bearings / distances destination(lats,lons,bearing=45,distance=500000) #different bearings for each lat lon destination(lats,lons,bearing=seq(0,360,length.out=9),distance=500000) #different distances for each lat lon destination(lats,lons,bearing=45,distance=seq(0,5000000,length.out=9)) #different bearings & distances for each lat lon destination(lats,lons,bearing=seq(0,360,length.out=9), distance=seq(0,5000000,length.out=9))###single lat lons lats = -85; lons = 165 #single bearing & single distance destination(lats,lons,bearing=180,distance=500000) #multiple bearings destination(lats,lons,bearing=seq(0,360,length.out=9),distance=500000) #multiple bearings destination(lats,lons,bearing=45,distance=seq(0,5000000,length.out=11)) #multiple bearings, multiple distances destination(lats,lons,bearing=seq(0,360,length.out=9), distance=seq(0,5000000,length.out=11)) ###multiple lat lons lats = seq(-90,90,length.out=9); lons = seq(-180,180,length.out=9) #multiple lat lons but single bearings / distances destination(lats,lons,bearing=45,distance=500000) #different bearings for each lat lon destination(lats,lons,bearing=seq(0,360,length.out=9),distance=500000) #different distances for each lat lon destination(lats,lons,bearing=45,distance=seq(0,5000000,length.out=9)) #different bearings & distances for each lat lon destination(lats,lons,bearing=seq(0,360,length.out=9), distance=seq(0,5000000,length.out=9))
distance estimates the distance given a starting &
ending latitude and longitude.
For general
information on Vincenty's formula, see e.g.,
http://en.wikipedia.org/wiki/Vincenty's_formulae. It
states:
Vincenty's formulae are two related
iterative methods used in geodesy to calculate the distance
between two points on the surface of an spheroid, developed
by Thaddeus Vincenty in 1975. They are based on the
assumption that the figure of the Earth is an oblate
spheroid, and hence are more accurate than methods such as
great-circle distance which assume a spherical Earth.
Note: this method assumes a locations are lat &
lon given in WGS 84.
Direction, if requested, is the
the initial bearing (sometimes referred to as forward
azimuth) for which one would follow as a straight line
along a great-circle arc from start to finish.
Note: this will fail if there are NA's in the data.
distance(lat1, lon1 = NULL, lat2 = NULL, lon2 = NULL, bearing = FALSE)distance(lat1, lon1 = NULL, lat2 = NULL, lon2 = NULL, bearing = FALSE)
lat1 |
a single value or vector of values representing latitude in decimal degrees from -90 to 90 degrees. Alternatively, a data.frame or matrix can be used here with each column representing lat1, lon1, lat2, lon2 (in that order). |
lon1 |
a single value or vector of values representing longitude in decimal degrees from -180 to 180 degrees. If NULL, lat1 is assumed to be a matrix or data.frame. |
lat2 |
a single value or vector of values representing latitude in decimal degrees from -90 to 90 degrees. If NULL, lat1 is assumed to be a matrix or data.frame. |
lon2 |
a single value or vector of values representing longitude in decimal degrees from -180 to 180 degrees. If NULL, lat1 is assumed to be a matrix or data.frame. |
bearing |
boolean value as to calculate the direction as well as the distance. |
Returns a data.frame with:
lon1 |
the original longitude |
lat1 |
the original latitude |
lon2 |
the destination longitude |
lat2 |
the destination latitude |
distance |
the distance used |
bearing |
if requested, the bearing between the two points |
Jeremy VanDerWal [email protected]
The source code for the distance algorithm here was
modified from
http://www.movable-type.co.uk/scripts/latlong-vincenty.html.
Distances were validated against Geoscience Australia
calculations
(http://www.ga.gov.au/geodesy/datums/vincenty_inverse.jsp).
Bearings were from multiple sources including
http://williams.best.vwh.net/avform.htm#Crs.
Vincenty, T. 1975. Direct and Inverse Solutions of Geodesics on the Ellipsoid with application of Nested Equations. Survey Review, vol XXII no 176. http://www.ngs.noaa.gov/PUBS_LIB/inverse.pdf
#get the distance of 1 degree longitude at each 5 degrees latitude from -90 to 90 distance(lat1=seq(-90,90,5),lon1=rep(0,37),lat2=seq(-90,90,5),lon2=rep(1,37),bearing=TRUE)#get the distance of 1 degree longitude at each 5 degrees latitude from -90 to 90 distance(lat1=seq(-90,90,5),lon1=rep(0,37),lat2=seq(-90,90,5),lon2=rep(1,37),bearing=TRUE)
extract.data extracts data from raster object of
class 'asc' (this and the adehabitat package),
'RasterLayer' (raster package) or 'SpatialGridDataFrame'
(sp package) at specified locations. This represents a
faster version of 'join.asc' of the adehabitat package that
assumes all locations are within the map extents.
Note: there is no interpolation done here. The
values reported are simply the values of the raster cell
the point falls into.
## S3 method for class 'data' extract(pts, x)## S3 method for class 'data' extract(pts, x)
pts |
a two-column data frame or matrix with the x and y coordinates of the locations of interest. |
x |
a raster matrix of class 'asc' (this and the adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
Implements a faster version of 'join.asc' from the
adehabitat package.
NOTE: this assumes all
locations are within the extent of the raster map. Values
outside the extent will be given a value of NA.
Returns a vector equal in length to the number of locations in pnts.
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #define some point locations points = data.frame(x=runif(25,1,50),y=runif(25,1,50)) #extract the data points$values = extract.data(points,tasc) #show the data print(points)#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #define some point locations points = data.frame(x=runif(25,1,50),y=runif(25,1,50)) #extract the data points$values = extract.data(points,tasc) #show the data print(points)
getXYcoords computes the geographical coordinates of
the rows and columns of pixels of a raster map of class
asc. Code & helpfile were modified from adehabitat
package.
getXYcoords(w)getXYcoords(w)
w |
an object of class |
Returns a list with two components:
x |
the x coordinates of the columns of pixels of the map |
y |
the y coordinates of the rows of pixels of the map |
Jeremy VanDerWal [email protected]
tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) getXYcoords(tasc)tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) getXYcoords(tasc)
Creates a grid of cell areas or perimeters for spatial grids in geographic (lat-lon) projections.
grid.area(mat) grid.perimeter(mat)grid.area(mat) grid.perimeter(mat)
mat |
a matrix representing a raster of class 'asc' (this & adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
grid.area |
Returns an ascii grid file which contains the values of the area in each cell. |
grid.perimter |
Returns an ascii grid file which contains the values of the perimeter in each cell. |
Jeremy VanDerWal [email protected] & Lorena Falconi [email protected]
#Create an ascii file y=seq(10,50,0.5) x=seq(140,180,0.5) cellsize=0.5 data1=sample(160,140) out1.asc=as.asc(matrix(data1,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) grid.area(out1.asc)[,] grid.perimeter(out1.asc)[,]#Create an ascii file y=seq(10,50,0.5) x=seq(140,180,0.5) cellsize=0.5 data1=sample(160,140) out1.asc=as.asc(matrix(data1,nc=y, nr=x), xll=min(x), yll=min(y), cellsize=cellsize) grid.area(out1.asc)[,] grid.perimeter(out1.asc)[,]
Since spatial grids in geographic projections do not have
equal area or perimeters, grid.info extracts
perimeter & area related information for latitudinal bands
with differing longitudinal widths.
Outputs lengths
are in m using Vincenty's equation (distance)and
areas in m2. Surface areas are calculated summing surface
areas of spherical polygons as estimated using l'Huiller's
formula.
grid.info(lats, cellsize, r = 6378137)grid.info(lats, cellsize, r = 6378137)
lats |
is a vector of latitudes representing the midpoint of grid cells |
cellsize |
is a single value (assuming square cells) or a two value vector (rectangular cells) representing the height (latitude) and width (longitude) of the cells |
r |
is a single value representing the radius of the globe in m. Default is for the WGS84 elipsoid |
a data.frame listing:
lat |
the latitude representing the midpoint of the cell |
top |
length of the top of the cell (m) |
bottom |
length of the bottom of the cell (m) |
side |
length of the side of the cell (m) |
diagnal |
length of the diagnals of the cell (m) |
area |
area of the cell (m2) |
Jeremy VanDerWal [email protected]
information on l'Huiller's formula http://williams.best.vwh.net/avform.htm for moreinfo) code for estimating area of polygon on sphere was modified from http://forum.worldwindcentral.com/showthread.php?t=20724
#show output for latitudes from -87.5 to 87.5 at 5 degree intervals grid.info(lats=seq(-87.5,87.5,5), 5)#show output for latitudes from -87.5 to 87.5 at 5 degree intervals grid.info(lats=seq(-87.5,87.5,5), 5)
Istat computes the I similarity statistic of Warren
et al. 2008. It is a method for defining niche overlap from
predictions of species' distributions.
NOTE:
it is assumed the input data are of the same extent and
cellsize, and all values are positive.
Istat(x, y, old = FALSE)Istat(x, y, old = FALSE)
x |
a vector or matrix of data; the matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
y |
a vector or matrix of data with the same dimensions and class of 'x' |
old |
a boolean identifying if "old" equation is to be used (see description). This was kept for legacy issues. |
The I similarity statistic sums the pair-wise differences between two predictions to create a single value representing the similarity of the two distributions. The I similarity statistic ranges from a value of 0, where two distributions have no overlap, to 1 where two distributions are identical (Warren et al., 2008).
NOTE: updated to correct equation but not to worry about old... see explanation at http://enmtools.blogspot.com.au/2010_09_01_archive.html.
A single value that is the I similarity statistic
Jeremy VanDerWal [email protected]
Warren, D. L., R. E. Glor, M. Turelli, and D. Funk. 2008. Environmental Niche Equivalency versus Conservatism: Quantitative Approaches to Niche Evolution. Evolution 62:2868-2883.
#create some simple objects of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 2500, min = -1, max = 1) tasc2 = tasc + rnorm(n = 2500, mean = 1, sd = 1) #ensure all data is positive tasc1 = abs(tasc1) tasc2 = abs(tasc2) #calculate the I similarity statistic I = Istat(tasc1,tasc2) print(I) #high niche overlap #using a more variable map tasc2 = tasc + rnorm(n = 2500, mean = 25, sd = 15);tasc2 = abs(tasc2) I = Istat(tasc1,tasc2) print(I) #lower niche overlap#create some simple objects of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 2500, min = -1, max = 1) tasc2 = tasc + rnorm(n = 2500, mean = 1, sd = 1) #ensure all data is positive tasc1 = abs(tasc1) tasc2 = abs(tasc2) #calculate the I similarity statistic I = Istat(tasc1,tasc2) print(I) #high niche overlap #using a more variable map tasc2 = tasc + rnorm(n = 2500, mean = 25, sd = 15);tasc2 = abs(tasc2) I = Istat(tasc1,tasc2) print(I) #lower niche overlap
Kappa estimates the Kappa statistic for model
accuracy.
Kappa(mat)Kappa(mat)
mat |
a confusion matrix of class 'confusion.matrix'
from |
Returns a single value represting the Kappa statistic.
Jeremy VanDerWal [email protected]
auc, omission,
sensitivity, specificity,
prop.correct, confusion.matrix,
accuracy
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix mat = confusion.matrix(obs,pred,threshold=0.5) #calculate the Kappa statistic Kappa(mat)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix mat = confusion.matrix(obs,pred,threshold=0.5) #calculate the Kappa statistic Kappa(mat)
This is a moving window that for each cell returns the minimum 'cost' based on surrounding data cells and some dispersal distance cost.
lcmw(mat, mw, mnc)lcmw(mat, mw, mnc)
mat |
a matrix of values that can be based on a raster dataset. Lower values should represent lower cost. The matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
mw |
a distance-cost matrix to be applied to each cell of 'mat'. This matrix can be dispersal costs. Lower values should represent lower cost. |
mnc |
an integer value representing the radius for 'mw' in number of cells. |
This method moves over the matrix of values, summing the
moving window cost mw and the matrix mat,
returning the minimum cost value. This was created to
estimate the least cost path through time for all cells in
a matrix (see example).
A matrix of values of the same dimensions and class as
input mat
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(1:100,nr=10,nc=10)); print(tasc) #show the input matrix print(tasc[1:10,1:10]) #vary the moving windows ###no cost window of 2 cell radius tcost = matrix(0,nr=5,nc=5); print(tcost) out = lcmw(tasc, tcost, 2); print(out[1:10,1:10]) ###no cost with a circular radius of 2 tcost = matrix(NA,nr=5,nc=5) #populate the distances for (y in 1:5){ for (x in 1:5){ tcost[y,x] = sqrt((3-y)^2 + (3-x)^2) } } #remove distance values > max.num.cells tcost[which(tcost>2)]=NA #no cost matrix tcost1 = tcost; tcost1[is.finite(tcost1)]=1; print(tcost1) out = lcmw(tasc, tcost1, 2); print(out[1:10,1:10]) #linear cost tcost = tcost/2; print(tcost) out = lcmw(tasc, tcost, 2); print(out[1:10,1:10])#create a simple object of class 'asc' tasc = as.asc(matrix(1:100,nr=10,nc=10)); print(tasc) #show the input matrix print(tasc[1:10,1:10]) #vary the moving windows ###no cost window of 2 cell radius tcost = matrix(0,nr=5,nc=5); print(tcost) out = lcmw(tasc, tcost, 2); print(out[1:10,1:10]) ###no cost with a circular radius of 2 tcost = matrix(NA,nr=5,nc=5) #populate the distances for (y in 1:5){ for (x in 1:5){ tcost[y,x] = sqrt((3-y)^2 + (3-x)^2) } } #remove distance values > max.num.cells tcost[which(tcost>2)]=NA #no cost matrix tcost1 = tcost; tcost1[is.finite(tcost1)]=1; print(tcost1) out = lcmw(tasc, tcost1, 2); print(out[1:10,1:10]) #linear cost tcost = tcost/2; print(tcost) out = lcmw(tasc, tcost, 2); print(out[1:10,1:10])
legend.gradient creates and displays a gradient
legend on a plot or image file. The place and size of the
legend is defined by coordinates, previously identified.
legend.gradient(pnts, cols = heat.colors(100), limits = c(0, 1), title = "Legend", ...)legend.gradient(pnts, cols = heat.colors(100), limits = c(0, 1), title = "Legend", ...)
pnts |
x and y coordinates of the gradient location in the plot |
cols |
a set of 2 or more colors used in the image, to create the gradient |
limits |
to label the min and max values of the gradient in the legend |
title |
to specify the title of the legend |
... |
other graphical parameters defined by image() or plot() |
nothing is returned, a gradient legend is added to a plot or a image.
Lorena Falconi [email protected]
#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,0, 0,1,0,0,0,1,0,NA,NA,NA, 0,0,1,1,1,0,0,NA,NA,NA, 1,1,1,0,0,0,0,NA,NA,NA),nr=10,byrow=TRUE) } #do the connected component labeling tasc = ConnCompLabel(tmat) # Create a color ramp colormap=c("grey","yellow","yellowgreen","olivedrab1","lightblue4") #create an image image(tasc,col=colormap, axes=FALSE, xlab="", ylab="", ann=FALSE) #points for the gradient legend pnts = cbind(x =c(0.8,0.9,0.9,0.8), y =c(1.0,1.0,0.8,0.8)) #create the gradient legend legend.gradient(pnts,colormap,c("Low","High"))#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,0, 0,1,0,0,0,1,0,NA,NA,NA, 0,0,1,1,1,0,0,NA,NA,NA, 1,1,1,0,0,0,0,NA,NA,NA),nr=10,byrow=TRUE) } #do the connected component labeling tasc = ConnCompLabel(tmat) # Create a color ramp colormap=c("grey","yellow","yellowgreen","olivedrab1","lightblue4") #create an image image(tasc,col=colormap, axes=FALSE, xlab="", ylab="", ann=FALSE) #points for the gradient legend pnts = cbind(x =c(0.8,0.9,0.9,0.8), y =c(1.0,1.0,0.8,0.8)) #create the gradient legend legend.gradient(pnts,colormap,c("Low","High"))
Estimates different measures of accurracy given a confusion matrix.
omission(mat) sensitivity(mat) specificity(mat) prop.correct(mat)omission(mat) sensitivity(mat) specificity(mat) prop.correct(mat)
mat |
a confusion matrix of class 'confusion.matrix'
from |
returns single values representing the:
ommission |
the ommission rate as a proportion of true occurrences misidentified given the defined threshold value |
sensitivity |
the sensitivity given the defined threshold value |
specificity |
the specificity given the defined threshold value |
prop.correct |
the proportion of the presence and absence records correctly identified given the defined threshold value |
Jeremy VanDerWal [email protected]
auc, Kappa,
confusion.matrix, accuracy
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix mat = confusion.matrix(obs,pred,threshold=0.5) #calculate the accuracy measures omission(mat) sensitivity(mat) specificity(mat) prop.correct(mat)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the confusion matrix mat = confusion.matrix(obs,pred,threshold=0.5) #calculate the accuracy measures omission(mat) sensitivity(mat) specificity(mat) prop.correct(mat)
optim.thresh estimates optimal threshold values
given eight methods.
Note: this method will
exclude any missing data.
optim.thresh(obs, pred, threshold = 101)optim.thresh(obs, pred, threshold = 101)
obs |
a vector of observed values which must be 0 for absences and 1 for occurrences |
pred |
a vector of the same length as |
threshold |
a single integer value representing the number of equal interval threshold values between 0 & 1 |
Returns a list of the optimal thresholds for the different
methods. If the list item is a single value, that is the
optimal threshold but if two values are reported for the
method, this represents the range in thresholds that are
equal for that threshold selection method.
The
returned list includes the single or range in thresholds
selected using the following methods:
min.occurence.prediction |
is the minimum prediction for the occurrence (presence) records |
mean.occurence.prediction |
is the mean prediction for the occurrence (presence) records |
'10.percent.omission' |
is the threshold value or range in values that excludes approx. 10 percent of the occurrence records |
'sensitivity=specificity' |
is the threshold value or range in values where sensitivity is equal to sensitivity |
'max.sensitivity+specificity' |
is the threshold value or range in values that maximizes sensitivity plus specificity |
maxKappa |
is the threshold value or range in values with the maximum Kappa statistic |
max.prop.correct |
is the threshold value or range in values with the maximum proportion of presence and absence records correctly identified |
min.ROC.plot.distance |
is the threshold value or range in values where the ROC curve is closest to point (0,1) (or perfect fit) |
Jeremy VanDerWal [email protected]
accuracy, auc,
Kappa, omission,
sensitivity, specificity,
prop.correct, confusion.matrix
#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the optimal thresholds optim.thresh(obs,pred)#create some data obs = c(sample(c(0,1),20,replace=TRUE),NA); obs = obs[order(obs)] pred = runif(length(obs),0,1); pred = pred[order(pred)] #calculate the optimal thresholds optim.thresh(obs,pred)
PatchStat calculates the patch statistics for
individual patches identified in a matrix of data. The
matrix can be a raster of class 'asc' (adehabitat package),
'RasterLayer' (raster package) or 'SpatialGridDataFrame'
(sp package).
PatchStat(mat, cellsize = 1, latlon = FALSE)PatchStat(mat, cellsize = 1, latlon = FALSE)
mat |
a matrix of data with individual patches
identified as with |
cellsize |
cell size (in meters) is a single value representing the width/height of cell edges (assuming square cells) |
latlon |
boolean value representing if the data is geographic. If latlon == TRUE, matrix must be of class 'asc', 'RasterLayer' or 'SpatialGridDataFrame' |
The patch statistics are based on statistics calculated by fragstats http://www.umass.edu/landeco/research/fragstats/fragstats.html.
a data.frame listing
patchID |
the unique ID for each patch. |
n.cell |
the number of cells for each patch, specified in square meters. |
n.core.cell |
the number of cells in the core area, without the edge area. |
n.edges.perimeter |
the number of outer perimeter cell edges of the patch. |
n.edges.internal |
the number of internal cell edges of the patch. |
area |
the area of each patch comprising a landscape mosaic. |
core.area |
represents the interior area of the patch, greater than the specified depth-of-edge distance from the perimeter. |
perimeter |
the perimeter of the patch, including any internal holes in the patch, specified in meters. |
perim.area.ratio |
the ratio of the patch perimeter (m) to area (m2). |
shape.index |
the shape complexity, sum of each patches perimeter divided by the square root of patch area. |
frac.dim.index |
fractal dimension index reflects shape complexity across a range of spatial scales; approaches 2 times the logarithm of patch perimeter (m) divided by the logarithm of patch area (m2). |
core.area.index |
quantifies core area as a percentage of patch area. |
Jeremy VanDerWal [email protected]
McGarigal, K., S. A. Cushman, M. C. Neel, and E. Ene. 2002. FRAGSTATS: Spatial Pattern Analysis Program for Categorical Maps. Computer software program produced by the authors at the University of Massachusetts, Amherst. Available at the following web site: www.umass.edu/landeco/research/fragstats/fragstats.html
#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1))) #calculate the patch statistics ps.data = PatchStat(ccl.mat) ps.data#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat image(t(ccl.mat[10:1,]),col=c('grey',rainbow(length(unique(ccl.mat))-1))) #calculate the patch statistics ps.data = PatchStat(ccl.mat) ps.data
pnt.in.poly works out if 2D points lie within the
boundaries of a defined polygon.
Note:
Points that lie on the boundaries of the polygon or
vertices are assumed to be within the polygon.
pnt.in.poly(pnts, poly.pnts)pnt.in.poly(pnts, poly.pnts)
pnts |
a 2-column matrix or dataframe defining locations of the points of interest |
poly.pnts |
a 2-column matrix or dataframe defining the locations of vertices of the polygon of interest |
The algorithm implements a sum of the angles made between
the test point and each pair of points making up the
polygon. The point is interior if the sum is 2pi,
otherwise, the point is exterior if the sum is 0. This
works for simple and complex polygons (with holes) given
that the hole is defined with a path made up of edges into
and out of the hole.
This sum of angles is not able
to consistently assign points that fall on vertices or on
the boundary of the polygon. The algorithm defined here
assumes that points falling on a boundary or polygon vertex
are part of the polygon.
A 3-column dataframe where the first 2 columns are the original locations of the points. The third column (names pip) is a vector of binary values where 0 represents points not with the polygon and 1 within the polygon.
Jeremy VanDerWal [email protected]
#define the points and polygon pnts = expand.grid(x=seq(1,6,0.1),y=seq(1,6,0.1)) polypnts = cbind(x=c(2,3,3.5,3.5,3,4,5,4,5,5,4,3,3,3,2,2,1,1,1,1,2), y=c(1,2,2.5,2,2,1,2,3,4,5,4,5,4,3,3,4,5,4,3,2,2)) #plot the polygon and all points to be checked plot(rbind(polypnts, pnts)) polygon(polypnts,col='#99999990') #create check which points fall within the polygon out = pnt.in.poly(pnts,polypnts) head(out) #identify points not in the polygon with an X points(out[which(out$pip==0),1:2],pch='X')#define the points and polygon pnts = expand.grid(x=seq(1,6,0.1),y=seq(1,6,0.1)) polypnts = cbind(x=c(2,3,3.5,3.5,3,4,5,4,5,5,4,3,3,3,2,2,1,1,1,1,2), y=c(1,2,2.5,2,2,1,2,3,4,5,4,5,4,3,3,4,5,4,3,2,2)) #plot the polygon and all points to be checked plot(rbind(polypnts, pnts)) polygon(polypnts,col='#99999990') #create check which points fall within the polygon out = pnt.in.poly(pnts,polypnts) head(out) #identify points not in the polygon with an X points(out[which(out$pip==0),1:2],pch='X')
put.data replaces data in raster object of class
'asc' (this and adehabitat package) at specified
locations.
Note: there is no interpolation
done here. The values given replace the values of the
raster cell the point falls into.
put.data(pts, x)put.data(pts, x)
pts |
a three-column data frame or matrix with the x and y coordinates of the locations of interest and the third column being the z values to put in the ascii grid file. |
x |
a raster matrix of class 'asc' (this and the adehabitat package) |
Implements a faster version of 'join.asc' from the
adehabitat package.
NOTE: this assumes all
locations are within the extent of the raster map. Values
outside the extent will be given a value of NA.
Returns a raster matrix of class 'asc' equal in size to input 'x'.
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) ## Not run: image(tasc) #define some point locations points = data.frame(x=runif(25,1,50),y=runif(25,1,50),z=50) #put the new data tasc = put.data(points,tasc) #show the data ## Not run: image(tasc)#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) ## Not run: image(tasc) #define some point locations points = data.frame(x=runif(25,1,50),y=runif(25,1,50),z=50) #put the new data tasc = put.data(points,tasc) #show the data ## Not run: image(tasc)
quick.map creates and displays an image, identifying
the threshold as the background color, and create the
gradient legend in the map.
quick.map(sdm.asc, threshold, bkgd.col = "grey", cols = heat.colors(100), zlim = NULL, pnts = NULL, ...)quick.map(sdm.asc, threshold, bkgd.col = "grey", cols = heat.colors(100), zlim = NULL, pnts = NULL, ...)
sdm.asc |
an object of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
threshold |
to indicate the threshold limit of
|
bkgd.col |
to specify the background color |
cols |
a set of 2 or more colors to be used in the image and the gradient legend |
zlim |
to specify the upper an lower limits, which are going to be the labels of the gradient legend |
pnts |
location information for adding the
|
... |
other graphical parameters defined by image() or plot() |
An image is created of the map requested. A gradient legend
(legend.gradient) will be added if
pnts (the position of the legend) is specified.
Nothing is returned, an image is created.
Lorena Falconi [email protected]
#create a matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,0, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,1,1,1, 1,1,1,0,0,0,0,1,1,1),nr=10,byrow=TRUE) } #do the connected component labeling tasc = ConnCompLabel(tmat) #put in the gradient scale pnts = cbind(x =c(1.1,1.2,1.2,1.1), y =c(0.9,0.9,0.7,0.7)) # Set the map and gradient leyend colors tasc.col=colorRampPalette(c("yellow","orange", "red"))(5) #Create an image with the gradient legend quick.map(tasc,0.09,bkgd.col = 'darkgrey', cols=tasc.col, axes=FALSE, xlim=c(0.0,1.35)) ######################### # Create an image with two colors: below the threshold and # above the threshold # The next version of SDM Tools will let you create the legend.gradient # at a specific side of your image, and the user would not need to set # the coordinates. # To create the legend.gradient at the bottom left of your image without # setting up the coordinates at the image you can do this: xlim = c(-0.5,1) ylim = c(0,1) wid = diff(xlim)*0.05 ht = diff(ylim)*0.1 xvals = c(xlim[1]+wid,xlim[1]+2*wid,xlim[1]+2*wid,xlim[1]+wid) yvals = c(ylim[1]+ht,ylim[1]+ht,ylim[1]+2*ht,ylim[1]+2*ht) #Create the points for the legend.gradient pnts=(cbind(xvals,yvals)) # Set the images colors: above the threshold is black and # below the threshold is darkgrey. quick.map(tasc,0.09,bkgd.col = 'darkgrey', cols="black", axes=FALSE, xlim=c(-0.8, 1))#create a matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,0, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,1,1,1, 1,1,1,0,0,0,0,1,1,1),nr=10,byrow=TRUE) } #do the connected component labeling tasc = ConnCompLabel(tmat) #put in the gradient scale pnts = cbind(x =c(1.1,1.2,1.2,1.1), y =c(0.9,0.9,0.7,0.7)) # Set the map and gradient leyend colors tasc.col=colorRampPalette(c("yellow","orange", "red"))(5) #Create an image with the gradient legend quick.map(tasc,0.09,bkgd.col = 'darkgrey', cols=tasc.col, axes=FALSE, xlim=c(0.0,1.35)) ######################### # Create an image with two colors: below the threshold and # above the threshold # The next version of SDM Tools will let you create the legend.gradient # at a specific side of your image, and the user would not need to set # the coordinates. # To create the legend.gradient at the bottom left of your image without # setting up the coordinates at the image you can do this: xlim = c(-0.5,1) ylim = c(0,1) wid = diff(xlim)*0.05 ht = diff(ylim)*0.1 xvals = c(xlim[1]+wid,xlim[1]+2*wid,xlim[1]+2*wid,xlim[1]+wid) yvals = c(ylim[1]+ht,ylim[1]+ht,ylim[1]+2*ht,ylim[1]+2*ht) #Create the points for the legend.gradient pnts=(cbind(xvals,yvals)) # Set the images colors: above the threshold is black and # below the threshold is darkgrey. quick.map(tasc,0.09,bkgd.col = 'darkgrey', cols="black", axes=FALSE, xlim=c(-0.8, 1))
read.asc and read.asc.gz reads ESRI ArcInfo
ASCII raster file either uncompressed or compressed using
gzip. write.asc and write.asc.gz
writes an asc object to a ESRI ArcInfo ASCII raster file.
The output can be either compressed or uncompressed.
These functions are faster methods based on the
adehabitat import.asc and export.asc.write.asc2 and write.asc2.gz are even faster
implementations but have less error checking. image.asc and print.asc are generic methods
associated with plotting & summarizing data of class 'asc';
they were modified from adehabitat package.
read.asc(file, gz = FALSE) read.asc.gz(file) write.asc(x, file, gz = FALSE) write.asc.gz(x, file) write.asc2(x, file, sigdig = 0, gz = FALSE) write.asc2.gz(x, file, sigdig = 0) ## S3 method for class 'asc' image(x, col = gray((240:1)/256), clfac = NULL, ...) ## S3 method for class 'asc' print(x, ...)read.asc(file, gz = FALSE) read.asc.gz(file) write.asc(x, file, gz = FALSE) write.asc.gz(x, file) write.asc2(x, file, sigdig = 0, gz = FALSE) write.asc2.gz(x, file, sigdig = 0) ## S3 method for class 'asc' image(x, col = gray((240:1)/256), clfac = NULL, ...) ## S3 method for class 'asc' print(x, ...)
file |
a character string representing the filename of the input/output file. The file extension should always be '.asc'. |
gz |
defines if the object is or should be compressed using gzip |
x |
an object of class 'asc' as defined in the adehabitat package |
sigdig |
is the number of significant digits to write when creating the ascii grid file |
col |
for maps of type |
clfac |
for maps of type |
... |
additional arguments to be passed to the
generic function |
Implements a faster version of import.asc or export.asc
from the adehabitat package. In addition, files can be read
in and written to in gzip compressed format.
Generic
methods of print and image were modified from adehabitat.
Further details of them are found there.
Returns a raster matrix of the class 'asc' defined in the adehabitat package with the following attributes:
xll |
the x coordinate of the center of the lower left pixel of the map |
yll |
the y coordinate of the center of the lower left pixel of the map |
cellsize |
the size of a pixel on the studied map |
type |
either 'numeric' or 'factor' |
levels |
if type = 'factor', the levels of the factor. |
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) #write out the raster grid file write.asc(tasc,'t.raster.asc') write.asc.gz(tasc,'t.raster.asc') #actually save file name as t.raster.asc.gz #read in the raster grid files tasc2 = read.asc('t.raster.asc') tasc3 = read.asc.gz('t.raster.asc.gz') #remove the temporary raster unlink(c('t.raster.asc','t.raster.asc.gz'))#create a simple object of class 'asc' tasc = as.asc(matrix(rep(x=1:10, times=1000),nr=100)); print(tasc) #write out the raster grid file write.asc(tasc,'t.raster.asc') write.asc.gz(tasc,'t.raster.asc') #actually save file name as t.raster.asc.gz #read in the raster grid files tasc2 = read.asc('t.raster.asc') tasc3 = read.asc.gz('t.raster.asc.gz') #remove the temporary raster unlink(c('t.raster.asc','t.raster.asc.gz'))
Scalebar adds a distance scalebar onto a projected
map. It is not appropriate for geographic projections.
Scalebar(x, y, distance, unit = "km", scale = 1, t.cex = 0.8)Scalebar(x, y, distance, unit = "km", scale = 1, t.cex = 0.8)
x |
the x-axis position for the lower left corner of the bar |
y |
the x-axis position for the lower left corner of the bar |
distance |
the distance for which the scale bar should represent |
unit |
the units to report as the scaling |
scale |
the scaling factor to rescale the distance to a different unit. e.g., if your map is in m and want the scalebar to be in km, use a scale of 0.01 |
t.cex |
the scaling of the font size to be used for the scalebar |
nothing is returned, simply a scalebar is added to a plot.
Jeremy VanDerWal [email protected]
#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #plot the image image(tasc,axes=FALSE,ann=FALSE) #add a distance scalebar Scalebar(x=5,y=5,distance=20) #show values in km Scalebar(x=5,y=10,distance=20,unit='m',scale=1000) #show values in meters#create a simple object of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #plot the image image(tasc,axes=FALSE,ann=FALSE) #add a distance scalebar Scalebar(x=5,y=5,distance=20) #show values in km Scalebar(x=5,y=10,distance=20,unit='m',scale=1000) #show values in meters
SigDiff computes the significance of the pairwise
differences relative to the mean and variance of all
differences between the two input datasets. This is useful
for identifying regions of significant difference between
two datasets (e.g., different DEMs (Januchowski et al.
2010) or different species distribution model predictions
(Bateman et al 2010)). ImageDiff is a
wrapper to the image.asc command in adehabitat package that
uses the result from SigDiff to create an image
mapping the regions of significant differences (positive
and negative).
NOTE: it is assumed the input
data are of the same extent and cellsize.
SigDiff(x, y, pattern = TRUE) ImageDiff(tasc, sig.levels = c(0.025, 0.975), tcol = terrain.colors(3), ...)SigDiff(x, y, pattern = TRUE) ImageDiff(tasc, sig.levels = c(0.025, 0.975), tcol = terrain.colors(3), ...)
x |
a vector or matrix of data; the matrix can be of can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
y |
a vector or matrix of data with the same dimensions and class of 'x' |
pattern |
logical value defining if differences are respective to relative patterning (TRUE) or absolute values (FALSE) |
tasc |
a matrix of probability values (0 to 1)
likely created by |
sig.levels |
the significance levels to define significantly above and below. Default settings represent significance at the 0.05 level |
tcol |
a set of 3 colors for use in the image to represent significantly lower or greater, and not significant |
... |
other graphical parameters defined by image() or plot() |
SigDiff returns a vector or matrix of the same
dimensions and class of the input representing the
significance of the pairwise difference relative to the
mean and variance of all differences between the two
inputs. ImageDiff returns nothing but
creates an image of the areas of significant differences
Stephanie Januchowski [email protected]
Januchowski, S., Pressey, B., Vanderwal, J. & Edwards, A.
(2010) Characterizing errors in topographic models and
estimating the financial costs of accuracy. International
Journal of Geographical Information Science, In Press.
Bateman, B.L., VanDerWal, J., Williams, S.E. & Johnson,
C.N. (2010) Inclusion of biotic interactions in species
distribution models improves predictions under climate
change: the northern bettong Bettongia tropica, its food
resources and a competitor. Journal of Biogeography, In
Review.
#create some simple objects of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 2500, min = -1, max = 1) tasc2 = tasc + rnorm(n = 2500, mean = 1, sd = 1) #create graphical representation par(mfrow=c(2,2),mar=c(1,1,4,1)) image(tasc1,main='first grid',axes=FALSE) image(tasc2,main='second grid',axes=FALSE) #get significant difference by spatial patterning out = SigDiff(tasc1,tasc2) ImageDiff(out,main="Pattern Differences",axes=FALSE) #get significant difference out = SigDiff(tasc1,tasc2,pattern=FALSE) ImageDiff(out,main="Absolute Differences",axes=FALSE) legend('topleft',legend=c('-ve','ns','+ve'),title='significance', fill=terrain.colors(3),bg='white')#create some simple objects of class 'asc' tasc = as.asc(matrix(1:50,nr=50,nc=50)); print(tasc) #modify the asc objects so that they are slightly different tasc1 = tasc + runif(n = 2500, min = -1, max = 1) tasc2 = tasc + rnorm(n = 2500, mean = 1, sd = 1) #create graphical representation par(mfrow=c(2,2),mar=c(1,1,4,1)) image(tasc1,main='first grid',axes=FALSE) image(tasc2,main='second grid',axes=FALSE) #get significant difference by spatial patterning out = SigDiff(tasc1,tasc2) ImageDiff(out,main="Pattern Differences",axes=FALSE) #get significant difference out = SigDiff(tasc1,tasc2,pattern=FALSE) ImageDiff(out,main="Absolute Differences",axes=FALSE) legend('topleft',legend=c('-ve','ns','+ve'),title='significance', fill=terrain.colors(3),bg='white')
slope and aspect calculates the slope and
aspect of raster surfaces of class 'asc' (SDMTools &
adehabitat packages), 'RasterLayer' (raster package) or
'SpatialGridDataFrame' (sp package).
Methods are
based on Burrough and McDonell (1998).
slope(mat, latlon = FALSE) aspect(mat, latlon = FALSE)slope(mat, latlon = FALSE) aspect(mat, latlon = FALSE)
mat |
a matrix of data representing z heights. Matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
latlon |
boolean value representing if the data is geographic. |
Slope returns values representing the 'rise over run' with
"run" units representing cellsize if latlon=FALSE or
km if latlon=TRUE. This can be changed to percentage
(multiply by 100) or to degrees by ATAN ( output ) *
57.29578.
Aspect returns the direction (0 to 360)
with North being 0. Values of -1 are flat areas with no
slope or aspect.
As this method requires information
from the surrounding cells, missing data (NAs or edges) are
populated with the value from the 'cell-of-interest').
an object of the same class as mat.
Jeremy VanDerWal [email protected]
Burrough, P. A. and McDonell, R.A., 1998. Principles of Geographical Information Systems (Oxford University Press, New York), p. 190.
#define a simple asc with some slope and direction tasc = as.asc(matrix(1:50,nr=10,nc=5),yll=75); tasc[,] slope(tasc)[,] #show the output of slope aspect(tasc)[,] #show the output of the aspect #define a FLAT simple asc tasc = as.asc(matrix(10,nr=10,nc=5),yll=75); tasc[,] slope(tasc)[,] #show the output of slope aspect(tasc)[,] #show the output of the aspect#define a simple asc with some slope and direction tasc = as.asc(matrix(1:50,nr=10,nc=5),yll=75); tasc[,] slope(tasc)[,] #show the output of slope aspect(tasc)[,] #show the output of the aspect #define a FLAT simple asc tasc = as.asc(matrix(10,nr=10,nc=5),yll=75); tasc[,] slope(tasc)[,] #show the output of slope aspect(tasc)[,] #show the output of the aspect
wt.mean calculates the mean given a weighting of the
values. wt.var is the unbiased variance of
the weighted mean calculation using equations of GNU
Scentific Library
(http://www.gnu.org/software/gsl/manual/html_node/Weighted-Samples.htmland.wt.sd is the standard deviation of the weighted mean
calculated as the sqrt of wt.var.
Note: NA data is automatically ommitted from
analysis.
wt.mean(x, wt) wt.var(x, wt) wt.sd(x, wt)wt.mean(x, wt) wt.var(x, wt) wt.sd(x, wt)
x |
is a vector of numerical data. |
wt |
is a vector of equal length to |
returns a single value from analysis requested.
Jeremy VanDerWal [email protected]
#define simple data x = 1:25 # set of numbers wt = runif(25) #some arbitrary weights #display means & variances (unweighted and then weighted) mean(x); wt.mean(x,wt) var(x); wt.var(x,wt) sd(x); wt.sd(x,wt)#define simple data x = 1:25 # set of numbers wt = runif(25) #some arbitrary weights #display means & variances (unweighted and then weighted) mean(x); wt.mean(x,wt) var(x); wt.var(x,wt) sd(x); wt.sd(x,wt)
ZonalStat calculates the statistics of data for
specified zones of two matrices of data. The matrix can be
a raster of class 'asc' (adehabitat package), 'RasterLayer'
(raster package) or 'SpatialGridDataFrame' (sp package).
ZonalStat(mat, zones, FUN = "all")ZonalStat(mat, zones, FUN = "all")
mat |
a matrix of data to be summarized; The matrix can be a raster of class 'asc' (adehabitat package), 'RasterLayer' (raster package) or 'SpatialGridDataFrame' (sp package) |
zones |
a matrix of data with individual patches
identified as with |
FUN |
a single or vector of functions to be applied to each 'zone'; the default of 'all' will calculate min, 1st quarter, median, 3rd quarter, max, mean, standard deviation and n |
The code summarizes the data for defined zones. Nearly any
function can be used for summarizing the data.
The
FUN defined with 'all' as one of or the only function will
append the functions of min, 1st quarter, median, 3rd
quarter, max, mean, standard deviation and n to what is
being calculated.
a data.frame listing
zone |
the unique ID for each zone. |
functions... |
a column for each of the functions identified |
The data.frame will have an atribute defining the number of NA values that were excluded from the analysis.
Jeremy VanDerWal [email protected]
#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat #this is the zone matrix to be used #create a random data matrix data.mat = matrix(runif(100),nr=10,nc=10) data.mat #calculate the zonal statistics zs.data = ZonalStat(data.mat,ccl.mat,FUN='all') zs.data #just calculate the sum zs.data = ZonalStat(data.mat,ccl.mat,FUN='sum') zs.data #calculate sum & n & 'all' and show when a function is not defined zs.data = ZonalStat(data.mat,ccl.mat, FUN=c('sum','length','not.a.function','all')) zs.data attr(zs.data,'excluded NAs') #show how many NAs were omitted from analysis#define a simple binary matrix tmat = { matrix(c( 0,0,0,1,0,0,1,1,0,1, 0,0,1,0,1,0,0,0,0,0, 0,1,NA,1,0,1,0,0,0,1, 1,0,1,1,1,0,1,0,0,1, 0,1,0,1,0,1,0,0,0,1, 0,0,1,0,1,0,0,1,1,0, 1,0,0,1,0,0,1,0,0,1, 0,1,0,0,0,1,0,0,0,1, 0,0,1,1,1,0,0,0,0,1, 1,1,1,0,0,0,0,0,0,1),nr=10,byrow=TRUE) } #do the connected component labelling ccl.mat = ConnCompLabel(tmat) ccl.mat #this is the zone matrix to be used #create a random data matrix data.mat = matrix(runif(100),nr=10,nc=10) data.mat #calculate the zonal statistics zs.data = ZonalStat(data.mat,ccl.mat,FUN='all') zs.data #just calculate the sum zs.data = ZonalStat(data.mat,ccl.mat,FUN='sum') zs.data #calculate sum & n & 'all' and show when a function is not defined zs.data = ZonalStat(data.mat,ccl.mat, FUN=c('sum','length','not.a.function','all')) zs.data attr(zs.data,'excluded NAs') #show how many NAs were omitted from analysis