GeoSimapprox {GeoModels}R Documentation

Fast simulation of Gaussian and non Gaussian Random Fields.

Description

Simulation of Gaussian and some non Gaussian spatial, spatio-temporal and spatial bivariate random fields using approximate methods of simulation (circulant embeeding and turning bands) (see Examples).

Usage

GeoSimapprox(coordx, coordy=NULL, coordt=NULL, 
coordx_dyn=NULL,corrmodel, distance="Eucl",GPU=NULL, 
grid=FALSE,local=c(1,1),max.ext=1,
method="TB",M=30, L=2000,model='Gaussian',
n=1,param,anisopars=NULL, radius=6371,X=NULL,spobj=NULL,nrep=1)

Arguments

coordx

A numeric (d \times 2)-matrix (where d is the number of spatial sites) giving 2-dimensions of spatial coordinates or a numeric d-dimensional vector giving 1-dimension of spatial coordinates. Coordinates on a sphere for a fixed radius radius are passed in lon/lat format expressed in decimal degrees.

coordy

A numeric vector giving 1-dimension of spatial coordinates; coordy is interpreted only if coordx is a numeric vector or grid=TRUE otherwise it will be ignored. Optional argument, the default is NULL then coordx is expected to be numeric a (d \times 2)-matrix.

coordt

A numeric vector giving 1-dimension of temporal coordinates. Optional argument, the default is NULL then a spatial RF is expected.

coordx_dyn

A list of m numeric (d_t \times 2)-matrices containing dynamical (in time) spatial coordinates. Optional argument, the default is NULL

corrmodel

String; the name of a correlation model, for the description see the Section Details.

distance

String; the name of the spatial distance. The default is Eucl, the euclidean distance. See the Section Details of GeoFit.

GPU

Numeric; if NULL (the default) no GPU computation is performed.

grid

Logical; if FALSE (the default) the data are interpreted as spatial or spatial-temporal realisations on a set of non-equispaced spatial sites (irregular grid).

local

Numeric; number of local work-items of the GPU

max.ext

Numeric; The maximum extension of the simulation window (for the spatial CE method).

method

String; the type of approximation method. Default is TB that is the turning band method. The other possible choice is Vecchia that is the Vechia method for the Matern model and CE (circular embeeding) for the space time case .

M

Numeric; the number of neighboords in the Vecchia method.

L

Numeric; the number of lines in the turning band method.

model

String; the type of RF and therefore the densities associated to the likelihood objects. Gaussian is the default, see the Section Details.

n

Numeric; the number of trials for binomial RFs. The number of successes in the negative Binomial RFs. Default is 1.

param

A list of parameter values required in the simulation procedure of RFs, see Examples.

anisopars

A list of two elements "angle" and "ratio" i.e. the anisotropy angle and the anisotropy ratio, respectively.

radius

Numeric; a value indicating the radius of the sphere when using the great circle distance. Default value is the radius of the earth in Km (i.e. 6371)

X

Numeric; Matrix of space-time covariates.

spobj

An object of class sp or spacetime

nrep

Numeric; Numbers of indipendent replicates.

Value

Returns an object of class GeoSim. An object of class GeoSim is a list containing at most the following components:

bivariate

Logical:TRUE if the Gaussian RF is bivariate, otherwise FALSE;

coordx

A d-dimensional vector of spatial coordinates;

coordy

A d-dimensional vector of spatial coordinates;

coordt

A t-dimensional vector of temporal coordinates;

coordx_dyn

A list of dynamical (in time) spatial coordinates;

corrmodel

The correlation model; see GeoCovmatrix.

data

The vector or matrix or array of data, see GeoFit;

distance

The type of spatial distance;

method

The method of simulation

model

The type of RF, see GeoFit.

n

The number of trial for Binomial RFs;the number of successes in a negative Binomial RFs;

numcoord

The number of spatial coordinates;

numtime

The number the temporal realisations of the RF;

param

The vector of parameters' estimates;

radius

The radius of the sphere if coordinates are passed in lon/lat format;

spacetime

TRUE if spatio-temporal and FALSE if spatial RF;

nrep

The number of indipendent replicates;

Author(s)

Moreno Bevilacqua, moreno.bevilacqua89@gmail.com,https://sites.google.com/view/moreno-bevilacqua/home, Víctor Morales Oñate, victor.morales@uv.cl, https://sites.google.com/site/moralesonatevictor/, Christian", Caamaño-Carrillo, chcaaman@ubiobio.cl,https://www.researchgate.net/profile/Christian-Caamano

References

T. Gneiting, H. Sevcikova, D. B. Percival, M. Schlather and Y. Jiang (2006) Fast and Exact Simulation of Large Gaussian Lattice Systems in R2: Exploring the Limits Journal of Computational and Graphical Statistics 15 (3)

D. Arroyo, X. Emery (2020) An R Implementation of a Continuous Spectral Algorithm for Simulating Vector Gaussian Random Fields in Euclidean Spaces ACM Transactions on Mathematical Software 47(1)

J. Guiness (2018) Permutation and Grouping Methods for Sharpening Gaussian Process Approximations Technometrics 60(4) 415-429.

Examples

library(GeoModels)


################################################################
###
### Example 1. Simulation of a large spatial Gaussian RF 
###            with  Matern  covariance model
###            using circulant embeeding method
###            It works only for regular grid
###            for any typpe of correlation model
###############################################################
set.seed(68)
x = seq(0,1,0.005)
y = seq(0,1,0.005)
param=list(smooth=1.5,mean=0,sill=1,scale=0.2/3,nugget=0)
# Simulation of a spatial Gaussian RF with Matern correlation function
data1 <- GeoSimapprox(coordx=x,coordy=y, grid=TRUE,corrmodel="Matern", model="Gaussian",
                      method="CE",param=param)$data
fields::image.plot( matrix(data1, length(x), length(y), byrow = TRUE) )

################################################################
###
### Example 2. Simulation of a large spatial Gaussian RF 
###            with  Matern  covariance model
###            using Turning band method
###            It works for (ir)regular grid
###            for the Matern model
###############################################################
set.seed(68)
x = runif(10000)
y = runif(10000)
coords=cbind(x,y)
param=list(smooth=0.5,mean=0,sill=1,scale=0.1,nugget=0)
# Simulation of a spatial Gaussian RF with Matern correlation function
data1 <- GeoSimapprox(coords, corrmodel="Matern", model="Gaussian",
                      method="TB",param=param)$data
quilt.plot(coords,data1)


################################################################
###
### Example 3. Simulation of a large spatial Gaussian RF 
###            with  matern  covariance model
###            using Vecchia's method
###            It works  for (ir)regular grid
###            for the Matern model
###############################################################
set.seed(68)
x = runif(6000)
y = runif(6000)
coords=cbind(x,y)
param=list(smooth=0.5,mean=0,sill=1,scale=0.1,nugget=0)
# Simulation of a spatial Gaussian RF with Matern correlation function
data1 <- GeoSimapprox(coords, corrmodel="Matern", model="Gaussian",
                      method="Vecchia",param=param)$data
quilt.plot(coords,data1)



################################################################
###
### Example 4. Simulation of a large spacetime Gaussian RF 
###            with separable matern  covariance model
###            using  Circular embeeding method
###            It works  for (large) regular time grid
###            and separable spacetime models
###############################################################
set.seed(68)
coordt <- (0:100)
coords <- cbind( runif(100, 0 ,1), runif(100, 0 ,1))
param <- list(mean  = 0, sill = 1, nugget = 0.25,
              scale_s = 0.05, scale_t = 2, 
              smooth_s = 0.5, smooth_t = 0.5)
# Simulation of a spatial Gaussian RF with Matern correlation function
param<-list(nugget=0,mean=0,scale_s=0.2/3,scale_t=2/3,sill=1,smooth_s=0.5,smooth_t=0.5)

data <- GeoSimapprox(coordx=coords, coordt=coordt, corrmodel="Matern_Matern",
                     model="Gaussian",method="CE",param=param)$data
dim(data)

################################################################
###
### Example 5. Simulation of a large spacetime Gaussian RF 
###            with separable GenWend covariance model
###            using  Circular embeeding method in time
###############################################################
set.seed(68)
# Simulation of a spatial Gaussian RF with Matern correlation function
param<-list(nugget=0,mean=0,scale_s=0.2,scale_t=3,sill=1,
             smooth_s=0,smooth_t=0, power2_s=4,power2_t=4)

data <- GeoSimapprox(coordx=coords, coordt=coordt, corrmodel="GenWend_GenWend",
                     model="Gaussian",method="CE",param=param)$data
dim(data)







[Package GeoModels version 2.0.1 Index]