https://github.com/cran/RandomFields
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Tip revision: 9298a5792ec3101f8d2a98edeb37d86b7263e34e authored by Martin Schlather on 24 July 2015, 00:00:00 UTC
version 3.1.0
Tip revision: 9298a57
RMgencauchy.Rd
\name{RMgencauchy}
\alias{RMgencauchy}
\title{Generalized Cauchy Family Covariance Model}
\description{
 \command{\link{RMgencauchy}} is a stationary isotropic covariance model
 belonging to the generalized Cauchy family.
 The corresponding covariance function only depends on the distance \eqn{r \ge 0}{r \ge 0} between
 two points and is given by
 \deqn{C(r) = (1 + r^\alpha)^(-\beta/\alpha)}{C(r) = (1 + r^\alpha)^(-\beta/\alpha)}
 where \eqn{\alpha \in (0,2]}{0 < \alpha \le 2} and \eqn{\beta > 0}{\beta > 0}.
 See also \command{\link{RMcauchy}}.
}
\usage{
RMgencauchy(alpha, beta, var, scale, Aniso, proj)
}
\arguments{
 \item{alpha}{a numerical value; should be in the interval (0,2]
 to provide a valid covariance function for a random field of any dimension.}
 \item{beta}{a numerical value; should be positive to provide a valid
 covariance function for a random field of any dimension.}
 \item{var,scale,Aniso,proj}{optional arguments; same meaning for any
 \command{\link{RMmodel}}. If not passed, the above
 covariance function remains unmodified.}
}
\details{
 This model has a smoothness parameter \eqn{\alpha}{\alpha} and a
 paramater \eqn{\beta}{\beta} which determines the asymptotic power law.
 More precisely, this model admits simulating random fields where fractal dimension
 \emph{D} of the Gaussian sample and Hurst coefficient \emph{H}
 can be chosen independently (compare also with \command{\link{RMlgd}}.): Here, we have
 \deqn{ D = d + 1 - \alpha/2, \alpha \in (0,2]}{ D = d + 1 - \alpha/2, 0
 < \alpha \le 2}
 and
 \deqn{ H = 1 - \beta/2, \beta > 0.}{ H = 1 - \beta/2, \beta > 0.}
 
 I. e. the smaller \eqn{\beta}{\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 \command{\link{RMcauchy}}) is included
 in this family for the choice \eqn{\alpha = 2}{\alpha = 2} and
 \eqn{\beta = 2 \gamma}{\beta = 2 \gamma}. 
}
\value{
 \command{\link{RMgencauchy}} returns an object of class \code{\link[=RMmodel-class]{RMmodel}}
}
\references{
  Covariance function
  \itemize{
    % \item Gneiting, T. (2002) Compactly supported correlation
    % functions. \emph{J. Multivariate Anal.} \bold{83} 493--508.
    
    \item Gneiting, T. and Schlather, M. (2004)
    Stochastic models which separate fractal dimension and Hurst effect.
    \emph{SIAM review} \bold{46}, 269--282.
  }

  Tail correlation function (for \eqn{\alpha \in (0,1]}{0 < \alpha \le 1})
  \itemize{
    \item 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. 
    \emph{Extremes}, \bold{} Submitted.
  }
}


\author{Martin Schlather, \email{schlather@math.uni-mannheim.de}
}
\seealso{
 \command{\link{RMcauchy}},
 \command{\link{RMcauchytbm}},
 \command{\link{RMmodel}},
 \command{\link{RFsimulate}},
 \command{\link{RFfit}}.
}


\keyword{spatial}
\keyword{models}




\examples{
RFoptions(seed=0) ## *ANY* simulation will have the random seed 0; set
##                   RFoptions(seed=NA) to make them all random again
\dontshow{StartExample()}
model <- RMgencauchy(alpha=1.5, beta=1.5, scale=0.3)
x <- seq(0, 10, 0.02)
plot(model)
plot(RFsimulate(model, x=x))


\dontshow{FinalizeExample()}
}
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