1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170
|
\name{ExtremeValueCopulae}
\alias{ExtremeValueCopulae}
\alias{revCopula}
\alias{pevCopula}
\alias{devCopula}
\alias{revSlider}
\alias{pevSlider}
\alias{devSlider}
\title{Bivariate Extreme Value Copulae}
\description{
A collection and description of functions to investigate
bivariate extreme value copulae.
\cr
Extreme Value Copulae Functions:
\tabular{ll}{
\code{revCopula} \tab Generates extreme value copula random variates, \cr
\code{pevCopula} \tab computes extreme value copula probability, \cr
\code{devCopula} \tab computes extreme value copula density, \cr
\code{revSlider} \tab displays interactive plots of extreme value random variates, \cr
\code{pevSlider} \tab displays interactive plots of extreme value probability, \cr
\code{devSlider} \tab displays interactive plots of extreme value density. }
}
\usage{
revCopula(n, param = NULL, type = evList())
pevCopula(u = 0.5, v = u, param = NULL, type = evList(),
output = c("vector", "list"), alternative = FALSE )
devCopula(u = 0.5, v = u, param = NULL, type = evList(),
output = c("vector", "list"), alternative = FALSE )
revSlider(B = 10)
pevSlider(type = c("persp", "contour"), B = 10)
devSlider(type = c("persp", "contour"), B = 10)
}
\arguments{
\item{alternative}{
[evRho][evTau][*evCopula] - \cr
Should the probability be computed alternatively in a
direct way from the probability formula or by default
via the dependency function?
}
\item{B}{
[*Slider] - \cr
the maximum slider menu value when the boundary value is
infinite. By default this is set to 10.
}
%\item{error}{
% [evRho] - \cr
% the error bound to be achieved by the \code{integrate2d}
% integration formula. A numeric value, by default \code{error=1.0e-5}.
% }
\item{n}{
[revCopula][evCopulaSim] - \cr
the number of random deviates to be generated, an integer value.
}
\item{output}{
[*evCopula] - \cr
output - a character string specifying how the output should
be formatted. By default a vector of the same length as
\code{u} and \code{v}. If specified as \code{"list"}
then \code{u} and \code{v} are
expected to span a two-dimensional grid as outputted by the
function \code{grid2d} and the function returns a list with
elements \code{$x}, \code{y}, and \code{z} which can be directly
used for example by 2D plotting functions.
}
\item{param}{
[*ev*][A*] - \cr
distribution and copulae parameters.
A numeric value or vector of named parameters as required by
the copula specified by the variable \code{type}.
If set to \code{NULL}, then the default parameters will be taken.
}
\item{type}{
[*ev*][Afunc] - \cr
the type of the extreme value copula. A character
string selected from: "gumbel", "galambos", "husler.reiss",
"tawn", or "bb5".
\cr
[evSlider] - \cr
a character string specifying the plot type. Either a
perspective plot which is the default or a contour plot
with an underlying image plot will be created.
}
\item{u, v}{
[*evCopula][*archmCopula] - \cr
two numeric values or vectors of the same length at which
the copula will be computed. If \code{u} is a list then the
the \code{$x} and \code{$y} elements will be used as \code{u}
and \code{v}. If \code{u} is a two column matrix then the
first column will be used as \code{u} and the the second
as \code{v}.
}
}
\value{
The function \code{pcopula} returns a numeric matrix of probabilities
computed at grid positions \code{x}|\code{y}.
\cr
The function \code{parchmCopula} returns a numeric matrix with values
computed for the Archemedean copula.
\cr
The function \code{darchmCopula} returns a numeric matrix with values
computed for thedensity of the Archemedean copula.
\cr
The functions \code{Phi*} return a numeric vector with the values
computed from the Archemedean generator, its derivatives, or its
inverse.
\cr
The functions \code{cK} and \code{cKInv} return a numeric vector with the
values of the density and inverse for Archimedian copulae.
}
\author{
Diethelm Wuertz for the Rmetrics \R-port.
}
\examples{
## fCOPULA -
getClass("fCOPULA")
getSlots("fCOPULA")
## revCopula -
# Not yet implemented
# revCopula(n = 10, type = "galambos")
## pevCopula -
pevCopula(u = grid2d(), type = "galambos", output = "list")
## devCopula -
devCopula(u = grid2d(), type = "galambos", output = "list")
## AfuncSlider -
# Generator, try:
\dontrun{AfuncSlider()}
}
\keyword{models}
|