Creates a standard covariance model (cmodStd)
object for geostatistical data.
cmod_std(
model,
psill,
r,
evar = 0,
fvar = 0,
par3 = 0.5,
longlat = FALSE,
angle = 0,
ratio = 1,
radians = FALSE,
invert = TRUE
)A covariance model (e.g.,
"exponential"). See Details for the complete
list of choices.
The partial sill of the model. Must be a positive number.
The range parameter r. Must be a
positive number.
The variance of the errors. Must be non-negative number. The default is 0.
The finescale variance (microscale error). Must be a non-negative number. The default is 0.
The value of the third parameter for 3 parameter models. Must be a positive number. The default is 0.5.
A logical value indicating whether great
circle distance should be used. The default is
FALSE.
The major axis of geometric anisotropy (the
direction of strongest spatial dependence). Must be
between [0, 180) if radians = FALSE, otherwise
it must be between [0, \(\pi\)).
The ratio of the minor axis range over the major axis range. The value must be between (0, 1].
A logical value indicating whether the
angles returned should be in degrees or radians. The
default is FALSE, indicating that the returned
angles are in degrees.
A logical value indicating whether the axes
of the coordinates should be inverted (i.e., the x- and
y-axis are switched). The default is TRUE to
mimic results from other geostatistical R packages like
gstat, geoR, and other software like
GSLIB and GeoEAS. Set to FALSE to
use the typical x- and y-axes.
Returns a cmodStd object.
The general, isotropic form of the specified covariance function is
psill * \(\rho\)(d; r) +
(evar + fvar) * (d == 0), where
\(\rho\) is the correlation function of the parametric
models and d is the distance between the
relevant coordinates.
For the exponential model, \(\rho\)(d;
r) is exp(-d/r).
For the gaussian model, \(\rho\)(d;
r) is exp(-d^2/r^2).
For the matern model, \(\rho\)(d;
r) is
2^(1-par3)/gamma(par3)*sd^par3*besselK(sd,
nu = par3), where sd = d/r.
For the amatern (alternative Matern) model,
\(\rho\)(d; r) is
2^(1-par3)/gamma(par3)*sd^par3*besselK(sd, nu =
par3), where sd = 2 * sqrt(par3) * d/r.
For the spherical model, \(\rho\)(d;
r) is 1 - 1.5*sd + 0.5*(sd)^3 if d <
r, and 0 otherwise, with sd = d/r.
For the wendland1 model, \(\rho\)(d;
r) is (1 - sd)^4 * (4*sd + 1) if d <
r, and 0 otherwise, with sd = d/r.
For the wendland2 model, \(\rho\)(d;
r) is (1 - sd)^6 * (35*sd^2 + 18*sd + 3))/3
if d < r, and 0 otherwise, with sd = d/r.
For the wu1 model, \(\rho\)(d; r)
is (1 - sd)^3 * (1 + 3*sd + sd^2) if d < r,
and 0 otherwise, with sd = d/r.
For the wu2 model, \(\rho\)(d; r)
is (1 - sd)^4*(4 + 16*sd + 12*sd^2 + 3*sd^3))/4 if
d < r, and 0 otherwise, with sd = d/r.
For the wu3 model, \(\rho\)(d; r)
is (1 - sd)^6 * (1 + 6*sd + 41/3*sd^2 + 12*sd^3 +
5*sd^4 + 5/6*sd^5) if d < r, and 0 otherwise,
with sd = d/r.
Waller, L. A., & Gotway, C. A. (2004). Applied Spatial Statistics for Public Health Data. John Wiley & Sons.
# NOT RUN {
cmod_std(model = "exponential", psill = 1, r = 1)
# }
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