https://github.com/cran/spatstat
Tip revision: 852fedfb753a3c090dfb9096fa726b5fc7cb7b28 authored by Adrian Baddeley on 31 March 2005, 07:03:17 UTC
version 1.6-2
version 1.6-2
Tip revision: 852fedf
predict.ppm.Rd
\name{predict.ppm}
\alias{predict.ppm}
\title{Prediction from a Fitted Point Process Model}
\description{
Given a fitted point process model obtained by \code{\link{ppm}},
evaluate the spatial trend and the conditional intensity of the model
at new locations.
}
\usage{
predict.ppm(object, window, ngrid=NULL, locations=NULL,
covariates=NULL, type="trend", \dots)
}
\arguments{
\item{object}{
A fitted point process model, typically obtained from
the model-fitting algorithm \code{\link{ppm}}. An object of
class \code{"ppm"} (see \code{\link{ppm.object}}).
}
\item{window}{
window delimiting the locations where predictions
should be computed. Defaults to the window of the
original data used to fit the model \code{object}.
}
\item{ngrid}{dimensions (either (\code{ngrid[1]} by \code{ngrid[2]}
or \code{ngrid} by \code{ngrid}) of a rectangular grid of locations
inside \code{window} where predictions should be computed.
(Incompatible with \code{locations})
}
\item{locations}{
data giving the \eqn{x,y} coordinates (and marks, if required)
at which predictions should be computed. Either a data frame
or a binary image mask.
(Incompatible with \code{ngrid})
}
\item{covariates}{
Values of external covariates required by the model.
Either a data frame or a list of images.
See Details.
}
\item{type}{
character string.
Indicates which property of the fitted model should be predicted.
Options are \code{"trend"} for the spatial trend, and
\code{"cif"} or \code{"lambda"} for the conditional intensity.
}
\item{\dots}{
Ignored.
}
}
\value{
\emph{If \code{locations} is given and is a data frame:}
a vector of predicted values for the spatial locations
(and marks, if required) given in \code{locations}.
\emph{If \code{ngrid} is given, or if \code{locations} is given
and is a binary image mask:}
If \code{object} is an unmarked point process,
the result is an image object (of class \code{"im"}, see
\code{\link{im.object}}) containing the predictions.
If \code{object} is a multitype point process,
the result is a list of images, containing the predictions
for each type at the same grid of locations.
The ``predicted values'' are either values of the spatial trend
(if \code{type="trend"}) or values of the conditional intensity
(if \code{type="cif"} or \code{type="lambda"}).
}
\details{
This function computes the spatial trend
and the conditional intensity of a fitted spatial point process model.
See Baddeley and Turner (2000) for explanation and examples.
Given a point pattern dataset, we may fit
a point process model to the data using the
model-fitting algorithm \code{\link{ppm}}. This
returns an object of class \code{"ppm"} representing
the fitted point process model (see \code{\link{ppm.object}}).
The parameter estimates in this fitted model can be read off
simply by printing the \code{ppm} object.
The spatial trend and conditional intensity of the
fitted model are evaluated using this function \code{predict.ppm}.
The default action is to create a rectangular grid of points
in the observation window of the data point pattern, and evaluate
the spatial trend and conditional intensity at these locations.
Note that by ``spatial trend'' we mean the
(exponentiated) first order potential
and not the intensity of the process. [For example if we fit the
stationary Strauss process with parameters
\eqn{\beta}{beta} and \eqn{\gamma}{gamma},
then the spatial trend is constant and equal to \eqn{\beta}{beta}. ]
The conditional intensity \eqn{\lambda(u, X)}{lambda(u,X)} of the
fitted model is evaluated at each required spatial location \eqn{u},
with respect to the data point pattern \eqn{X}.
If the argument \code{ngrid} is present, then
predictions are performed at an \code{ngrid} by \code{ngrid}
pixel grid of locations in the window \code{window}.
The result of prediction will be a pixel image or images.
If \code{locations} is present, then predictions
will be performed at the spatial locations given by
this dataset. The result of prediction will be either a
vector of values or a pixel image or a list of images, depending
on the format of \code{locations}.
The argument \code{locations} may be either a data frame or list
specifying arbitrary locations,
or a binary image mask (an object of class \code{"owin"}
with type \code{"mask"}) specifying (a subset of) a rectangular
grid of locations.
If \code{locations} is a data frame or list, then it must contain
vectors \code{locations$x} and \code{locations$y} specifying the
\eqn{x,y} coordinates of the prediction locations. Additionally, if
the model is a marked point process, then \code{locations} must also contain
a factor \code{locations$marks} specifying the marks of the
prediction locations. These vectors must have equal length.
The result of prediction will be a vector of predicted values,
of the same length.
If \code{locations} is a binary image mask, then prediction will be
performed at each pixel in this binary image where the pixel value
is \code{TRUE} (in other words, at each pixel that is inside the
window). If the fitted model is an unmarked point process, then the
result of prediction will be an image. If the fitted model is a
marked point process, then prediction will
be performed for each possible value of the mark at each such
location, and the result of prediction will be a
list of images, one for each mark value.
If neither \code{ngrid} nor \code{locations} is given, then
\code{ngrid} is assumed. It defaults to 50.
The argument \code{covariates} gives the values of any spatial covariates
at the prediction locations.
If the trend formula in the fitted model
involves spatial covariates (other than
the Cartesian coordinates \code{x}, \code{y})
then \code{covariates} is required.
The format and use of \code{covariates} are analogous to those of the
argument of the same name in \code{\link{ppm}}.
It is either a data frame or a list of images.
If \code{covariates} is a list of images, then
the names of the entries should correspond to
the names of covariates in the model formula \code{trend}.
Each entry in the list must be an image object (of class \code{"im"},
see \code{\link{im.object}}).
The software will look up
the pixel values of each image at the quadrature points.
If \code{covariates} is a data frame, then the
\code{i}th row of \code{covariates}
is assumed to contain covariate data for the \code{i}th location.
When \code{locations} is a data frame,
this just means that each row of \code{covariates} contains the
covariate data for the location specified in the corresponding row of
\code{locations}. When \code{locations} is a binary image
mask, the row \code{covariates[i,]} must correspond to the location
\code{x[i],y[i]} where \code{x = as.vector(raster.x(locations))}
and \code{y = as.vector(raster.y(locations))}.
Note that if you only want to use prediction in order to
generate a plot of the predicted values,
it may be easier to use \code{\link{plot.ppm}} which calls
this function and plots the results.
}
\references{
Baddeley, A. and Turner, R.
Practical maximum pseudolikelihood for spatial point patterns.
\emph{Australian and New Zealand Journal of Statistics}
\bold{42} (2000) 283--322.
Berman, M. and Turner, T.R.
Approximating point process likelihoods with GLIM.
\emph{Applied Statistics} \bold{41} (1992) 31--38.
}
\seealso{
\code{\link{ppm}},
\code{\link{ppm.object}},
\code{\link{plot.ppm}},
\code{\link{print.ppm}},
\code{\link{fitted.ppm}}
}
\section{Warnings}{
The current implementation invokes \code{\link{predict.glm}}
so that \bold{prediction is wrong} if the trend formula in
\code{object} involves terms in \code{ns()},
\code{bs()} or \code{poly()}.
This is a weakness of \code{\link{predict.glm}} itself!
Error messages may be very opaque,
as they tend to come from deep in the workings of
\code{\link{predict.glm}}.
If you are passing the \code{covariates} argument
and the function crashes,
it is advisable to start by checking that all the conditions
listed above are satisfied.
}
\examples{
data(cells)
m <- ppm(cells, ~ polynom(x,y,2), Strauss(0.05), rbord=0.05)
trend <- predict(m, type="trend")
\dontrun{
image(trend)
points(cells)
}
cif <- predict(m, type="cif")
\dontrun{
persp(cif)
}
}
\author{Adrian Baddeley
\email{adrian@maths.uwa.edu.au}
\url{http://www.maths.uwa.edu.au/~adrian/}
and Rolf Turner
\email{rolf@math.unb.ca}
\url{http://www.math.unb.ca/~rolf}
}
\keyword{spatial}