Covariance functions {fields} | R Documentation |
Given two sets of locations computes the cross covariance matrix for some covariance families. In addition these functions can take advantage of spareness, implement more efficient multiplcation of the cross covariance by a vector or matrix and also return a marginal variance to be consistent with calls by the Krig function.
Note: These functions have been been renamed from the previous fields functions
using 'Exp' in place of 'exp' to avoid conflict with the generic exponential
function (exp(...)
)in R.
Exp.cov(x1, x2, theta = rep(1, ncol(x1)), p = 1, C = NA, marginal=FALSE) Exp.simple.cov(x1, x2, theta =1, C=NA,marginal=FALSE) Rad.cov(x1, x2, p = 1, with.log = TRUE, with.constant = TRUE, C=NA,marginal=FALSE) cubic.cov(x1, x2, theta = 1, C=NA, marginal=FALSE) Rad.simple.cov(x1, x2, p=1, with.log = TRUE, with.constant = TRUE, C = NA, marginal=FALSE) stationary.cov(x1, x2, Covariance="Exponential", Distance="rdist", Dist.args=NULL, theta=1.0,C=NA, marginal=FALSE,...) stationary.taper.cov(x1, x2, Covariance="Exponential", Taper="Wendland", Dist.args=NULL, Taper.args=NULL, theta=1.0, C=NA, marginal=FALSE, spam.format=TRUE,...) wendland.cov(x1, x2, theta = rep(1, ncol(x1)), k = 2, C = NA, marginal =FALSE,Dist.args = NULL, spam.format = TRUE, derivative = 0)
x1 |
Matrix of first set of locations where each row gives the coordinates of a particular point. |
x2 |
Matrix of second set of locations where each row gives the coordinates of a particular point. If this is missing x1 is used. |
theta |
Range (or scale) parameter. This can be a scalar, vector or matrix.
If a scalar or vector these are expanded to be the diagonal elements of
a linear transformation of the coordinates. In R code the transformation
applied before distances are found is: x1 %*% t(solve(theta)) or
if theta is a scalar: x1/theta .
Default is theta=1. See Details below.
|
C |
A vector with the same length as the number of rows of x2. If specified the covariance matrix will be multiplied by this vector. |
marginal |
If TRUE returns just the diagonal elements of the
covariance matrix using the x1 locations. In this case this is
just 1.0. The marginal argument will trivial for this function is a
required argument and capability for all covariance functions used with
Krig.
|
p |
Exponent in the exponential form. p=1 gives an exponential and p=2 gives a
Gaussian. Default is the exponential form.
For the radial basis function this is the exponent for the distance between locations. |
with.constant |
If TRUE includes complicated constant for radial basis functions.
See the function radbad.constant for more details. The
default is TRUE include the constant. Without the usual constant
the lambda used here will differ by a constant from estimators ( e.g.
cubic smoothing splines) that use the constant. Also a negative value
for the constant may be necessary to make the radial basis positive
definite as opposed to negative definite. |
with.log |
If TRUE include a log term for even dimensions. This is needed to be a thin plate spline of integer order. |
Covariance |
Character string that is the name of the covariance
shape function for the distance between
locations. Choices in fields are Exponential , Matern |
Distance |
Character string that is the name of the distance
function to use. Choices in fields are rdist , rdist.earth |
Taper |
Character string that is the name of the taper function to use. Choices in fields are listed in help(taper). |
Dist.args |
A list of optional arguments to pass to the Distance function. |
Taper.args |
A list of optional arguments to pass to the Taper
function. theta should always be the name for the range (or scale)
paremeter. |
spam.format |
If TRUE returns matrix in sparse matrix format implemented in the spam package. If FALSE just returns a full matrix. |
k |
The order of the Wendland covariance function. See help on Wendland. |
derivative |
If nonzero evaluates the partials of the covariance function at locations x1. This must be used with "C" option and is mainly called from within a predict function. |
... |
Any other arguments that will be passed to the
covariance function. e.g. smoothness for the Matern. |
For purposes of illustration, the function Exp.cov.simple
is
provided as a simple example and implements the R code discussed below.
It can also serve as a template for creating new covariance functions for the
Krig
and mKrig
functions. Also see the higher level function
stationary.cov
to mix and match different covariance shapes and
distance functions.
Functional Form: If x1 and x2 are matrices where nrow(x1)=m and nrow(x2)=n then this function will return a mXn matrix where the (i,j) element is the covariance between the locations x1[i,] and x2[j,]. The covariance is found as exp( -(D.ij **p)) where D.ij is the Euclidean distance between x1[i,] and x2[j,] but having first been scaled by theta.
Specifically if theta
is a matrix to represent a linear
transformation of the coordinates, then let
u= x1%*% t(solve( theta)) and v= x2%*% t(solve(theta)).
Form the mXn distance matrix with elements:
D[i,j] = sqrt( sum( ( u[i,] - v[j,])**2 ) ).
and the cross covariance matrix is found by exp(-D)
.
The tapered form (ignoring scaling parameters) is a matrix with i,j entry
exp(-D[i,j])*T(D[i,j]). With T being a positive definite tapering function that is also
assumed to be zero beyond 1.
Note that if theta is a scalar then this defines an isotropic covariance
function and the functional form is essentially exp(-D/theta)
.
Implementation:
The function r.dist
is a useful FIELDS function that finds
the cross Euclidean distance matrix (D defined above) for two sets of
locations. Thus in compact R code we have
exp(-rdist(u, v)**p)
Note that this function must also support two other kinds of calls:
If marginal is TRUE then just the diagonal elements are returned
(in R code diag( exp(-rdist(u,u)**p) )
).
If C is passed then the returned value is
exp(-rdist(u, v)**p) %*% C
Radial basis functions Rad.cov
: The functional form is
Constant* rdist(u, v)**p for odd dimensions
and Constant* rdist(u,v)**p * log( rdist(u,v)
For an m th order thin plate spline in d dimensions p= 2*m-d and must
be positive. The constant, depending on m and d, is coded in the fields
function radbas.constant
. This form is only a generalized
covariance function – it is only positive definite when restricted to
linear subspace. See Rad.simple.cov
for a coding of the radial
basis functions in R code.
Stationary covariance stationary.cov
:
Here the computation is to apply the function
Covariance to the distances found by the Distance function.
For example
Exp.cov(x1,x2, theta=MyTheta)
and
stationary.cov( x1,x2, theta=MyTheta, Distance= "rdist",
Covariance="Exponential")
are the same. This also the same as
stationary.cov( x1,x2, theta=MyTheta, Distance= "rdist",
Covariance="Matern",smoothness=.5)
.
Stationary tapered covariance stationary.taper.cov
: The resulting
cross covariance is the direct or Shure product of the tapering function
and the covariance. In R code given location matrices, x1
and
x2
and using Euclidean distance.
Covariance(rdist( x1, x2))*Taper( rdist( x1, x2))
By convention, the Taper
function is assumed to be identically
zero outside the interval [0,1]. Some efficiency is introduced within
the function to search for pairs of locations that are nonzero with
respect to the Taper. This search may find more nonzero pairs than
dimensioned by max.points
. Given this error just pass a larger
for max.points
explicitly. For spam.format TRUE the
multiplication with the C
argument is done with the spam sparse
multiplication routines through the "overloading" of the %*%
operator. Currently this function only supports the Euclidean distance
function.
About the FORTRAN: The actual function Exp.cov
and
Rad.cov
calls FORTRAN to
make the evaluation more efficient this is especially important when the
C argument is supplied. So unfortunately the actual production code in
Exp.cov is not as crisp as the R code sketched above. See
Rad.simple.cov
for a R coding of the radial basis functions.
If the argument C is NULL the cross covariance matrix is returned.
In general if nrow(x1)=m and nrow(x2)=n then the returned
matrix will be mXn.
Moreover,
if x1 is equal to x2 then this is the covariance matrix for this set of
locations.
If C is a vector of length n,
then returned value is the multiplication of the cross covariance matrix
with this vector.
Krig, rdist, rdist.earth, gauss.cov, Exp.image.cov, Exponential, Matern, Wendland.cov, mKrig
# exponential covariance matrix ( marginal variance =1) for the ozone #locations out<- Exp.cov( ozone$x, theta=100) # out is a 20X20 matrix out2<- Exp.cov( ozone$x[6:20,],ozone$x[1:2,], theta=100) # out2 is 15X2 matrix # Kriging fit where the nugget variance is found by GCV # Matern covariance shape with range of 100. # fit<- Krig( ozone$x, ozone$y, Covariance="Matern", theta=100,smoothness=2) data( ozone2) x<- ozone2$lon.lat y<- ozone2$y[16,] # example of calling the taper version directly # Note that default covariance is exponential and default taper is # Wendland (k=2). ## Not run: stationary.taper.cov( x,x, theta=1.5, Taper.args= list(k=2, theta=2.0), mean.neighbor= 200 )-> temp # temp is a tapered covariance matrix in sparse format. is.spam( temp) # evaluates to TRUE temp<- spam2full(temp) # should be identical to temp2<- Exp.cov( x,x, theta=1.5) * wendland.cov(x,x, theta= 2.0*1.5,spam.format=FALSE) test.for.zero( temp, temp2) ## End(Not run) # Here is an example of how the cross covariance multiply works # and lots of options on the arguments Ctest<- rnorm(10) temp<- stationary.cov( x,x[1:10,], C= Ctest, Covariance= "Wendland", k=2, dimension=2, theta=1.5 ) # do multiply explicitly temp2<- stationary.cov( x,x[1:10,], Covariance= "Wendland", k=2, dimension=2, theta=1.5 )%*% Ctest test.for.zero( temp, temp2) # use the tapered stationary version # cov.args is part of the argument list passed to stationary.taper.cov # within Krig. # This example needs the spam package. # ## Not run: Krig(x,y, cov.function = "stationary.taper.cov", theta=1.5, cov.args= list( Taper.args= list(k=2, theta=2.0) ) ) -> out2 ## End(Not run) # BTW this is very similar to ## Not run: Krig(x,y, theta= 1.5)-> out ## End(Not run)