fields (version 2.3)

matern.cov: Matern covariance function

Description

Given two sets of locations computes the Matern cross covariance matrix for covariances among all pairings. In the case of matern.earth.cov the locations are assumed to be lon/lat coordinates and the covariance function is a spherical modification.

Usage

matern.cov(x1, x2, theta = 1.0, smoothness = 0.5, scale=1)
matern.earth.cov(x1, x2, theta = 1, 
smoothness = 0.5, scale = 1, miles = TRUE, R = NULL)

Value

The cross covariance matrix between locations x1 and x2. If x1 is equal to x2 then this is the covariance matrix for this set of locations. In general if nrow(x1)=m and nrow( x2)=n then the returned matrix, Sigma will be mXn. Under some cases when the range is very small calculation of the Bessel functions fails and if so an NA will be returned.

Details

Derivatives of sample paths: In d dimensions a Gaussian process with Matern covariance and smoothness parameter nu will have nu + d/2 derivatives that exist in a mean square sense. The marginal variance is given by the parameter scale. When this parameter is set to one this yields a correlation function.

There several different ways to parameterize the Matern family and the reader is referred to Stein's book page 49 for discussion. In terms of the more geostatistical terminology, we note that out theta is also the "range" and the scale is also the "sill" if there is no nugget variance included in the covariance. We caution that the range for this function gives a qualitatively different scaling as one varies the smoothness.

Functional Form: If x1 and x2 are matrices where nrow(x1)=m and nrow( x2)=n and each row are the coordinates of a location, then this function should 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 H( D.ij) where D.ij is the Euclidean distance between x1[i,] and x2[j,] but having first been scaled by theta. H is proportional to a modified Bessel function of third kind using denoted by K.nu . In our parameterization we take smoothness = nu and H is normalized so that H(0)=1. (See the function matern for a succinct definition as R code.) The reader is referred to Stein's book, page 31 for more details. Note that we do not use Stein's normalization, however, as it seems more useful to normalize the covariance so that .

Definition of the distance matrix: D.ij = sqrt( sum.k (( x1[i,k] - x2[j,k]) /theta[k])**2 ).

Note that if theta is a scalar then this defines an isotropic covariance function.

Implementation: The function rdist is a useful FIELDS function that finds the cross distance matrix ( D defined above) for two sets of locations. Thus in compact S code we have

u <- t(solve(theta)v <- t(solve(theta)H(-rdist(u, v))

where solve(theta) is the (matrix) inverse for theta.

The adaptation to the sphere is to transform the angular separation among locations by 2R sin( angle/2). This is a measure of distance is then used in the matern functional form for the covariance. For small regions this will approximate the usual Matern but is a valid covariance at all distances. (See last example below.)

See Also

Krig, matern, rdist, rdist.earth, gauss.cov, exp.image.cov, matern.imag.cov

Examples

#
# Presenting the Matern family:
# the function matern is called by matern.cov
d<- seq( 0,5,,200)
sm<- seq( .5, 8,,5)
temp<- matrix( NA, 200, 5)
for ( k in 1:5){
temp[,k] <- matern(d, smoothness=sm[k])
}
matplot( d, temp, type="l", lty=1)
# note differing correlation scales depending on smoothness 


# Matern covariance matrix ( marginal variance =1) for the ozone
# locations 
out<- matern.cov( ozone$x, theta=100, smoothness=1.0)
# out is a 20X20 matrix

out2<- matern.cov( ozone$x[6:20,],ozone$x[1:2,], theta=100, 
smoothness=1.0)

# out2 is 15X2 cross covariance matrix 

# Kriging fit using a Matern covariance and where the nugget  and 
# sill variances are found by GCV 
fit<- Krig( ozone$x, ozone$y, matern.cov, theta=100, smoothness=1.0)


######## examples with  matern.earth.cov

# create a 1 degree patch of lon/lats  at the equator:
x<- seq( -1,1,,25)
y<- x
make.surface.grid( list( x=x, y=y))-> xg

# find covariance with the  (lon,lat) =(0,0)  
# theta = 30 , a degree at the equator is about 69.17333 miles. 

matern.earth.cov( xg,rbind( c(0,0)), theta = 30 )-> look

# covariance surface
image.plot( x,y,matrix(look, 25,25)) 

# compare to matern.cov( xg,rbind( c(0,0)), theta = 30/69.17333)

# now change the grid to be close to the north pole
# create a 1 degree patch of lon/lats  at  (0, 80N) :

x<-  seq( -1,1,,25)
y<- x + 80
make.surface.grid( list( x=x, y=y))-> xg

# evaluate the same covariance function at this point

matern.earth.cov( xg,rbind( c(0,80)), theta = 30 )-> look

# plot covariance surface 
#     stretching is an artifact of this Mercator projection 

image.plot( x,y,matrix(look, 25,25)) 

# a Kriging example with the ozone data

data(ozone2)

Krig( ozone2$lon.lat, ozone2$y[16,], cov.function= matern.earth.cov, 
    theta=300, na.rm=TRUE)-> look

surface( look, type="C")
US( add=TRUE, lwd=2)