Given a cluster point process model, this command returns a value beyond which the the probability density of the cluster offspring is neglible.
clusterradius(model, …)# S3 method for kppm
clusterradius(model, …, thresh = NULL, precision = FALSE)
# S3 method for character
clusterradius(model, …, thresh = NULL, precision = FALSE)
Cluster model. Either a fitted cluster or Cox model
    (object of class "kppm"), or a character string
    specifying the type of cluster model.
Parameter values for the model,
    when model is a character string.
Numerical threshold relative to the cluster kernel value at the origin (parent location) determining when the cluster kernel will be considered neglible. A sensible default is provided.
Logical. If precision=TRUE the precision of the calculated
    range is returned as an attribute to the range. See details.
A positive numeric.
Additionally, the precision related to this range value is returned as
  an attribute "prec", if precision=TRUE.
Given a cluster model this function by default returns the effective
  range of the model with the given parameters as used in spatstat. For
  the Matern cluster model (see e.g. rMatClust) this is
  simply the finite radius of the offsring density given by the paramter
  scale irrespective of other options given to this function. The
  remaining models in spatstat have infinite theoretical range, and an
  effective finite value is given as follows: For the Thomas model (see
  e.g. rThomas the default is 4*scale where scale
  is the scale or standard deviation parameter of the model. If
  thresh is given the value is instead found as described for the
  other models below.
For the Cauchy model (see e.g. rCauchy) and the Variance
  Gamma (Bessel) model (see e.g. rVarGamma) the value of
  thresh defaults to 0.001, and then this is used to compute the
  range numerically as follows. If \(k(x,y)=k_0(r)\)
  with \(r=\sqrt(x^2+y^2)\)
  denotes the isotropic cluster kernel then \(f(r) = 2 \pi r
  k_0(r)\) is the
  density function of the offspring distance from the parent. The range
  is determined as the value of \(r\) where \(f(r)\) falls below
  thresh times \(k_0(r)\).
If precision=TRUE the precision related to the chosen range is
  returned as an attribute. Here the precision is defined as the polar
  integral of the kernel from distance 0 to the calculated
  range. Ideally this should be close to the value 1 which would be
  obtained for the true theretical infinite range.
clusterkernel, kppm,
  rMatClust, rThomas, rCauchy,
  rVarGamma, rNeymanScott.
# NOT RUN {
  fit <- kppm(redwood ~ x, "MatClust")
  clusterradius(fit)
  clusterradius("Thomas", scale = .1)
  clusterradius("Thomas", scale = .1, thresh = 0.001)
  clusterradius("VarGamma", scale = .1, nu = 2, precision = TRUE)
# }
Run the code above in your browser using DataLab