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extRemes (version 2.0-9)

abba: Implementation of Stephenson-Shaby-Reich-Sullivan

Description

Implements MCMC methodology for fitting spatial extreme value models using Stephenson et al. (2014). Experimental.

Usage

abba(y, sites, iters, Qb = NULL, knots = sites, X = cbind(1, sites), 
  beta = NULL, alpha = 0.5, logbw = 0, tau = c(1, 1, 1), 
  logs = matrix(0, nrow = nf, ncol = nt), 
  u = matrix(0.5, nrow = nf, ncol = nt), 
  MHbeta = matrix(rep(c(0.15, 0.03, 0.015), each = n), ncol = 3), 
  MHalpha = 0.01, MHlogbw = 0, 
  MHs = matrix(0.5, nrow = nf, ncol = nt), 
  MHu = matrix(2.5, nrow = nf, ncol = nt), 
  pribeta = c(10, 10, 10), prialpha = c(1, 1), prilogbw = c(0, 1), 
  pritau = c(0.1, 0.1, 0.1), trace = 0) 
abba_latent(y, sites, iters, Qb = NULL, X = cbind(1, sites), 
  beta = NULL, tau = c(1, 1, 1), 
  MHbeta = matrix(rep(c(0.15, 0.03, 0.015), each = n), ncol = 3), 
  pribeta = c(10, 10, 10), pritau = c(0.1, 0.1, 0.1), trace = 0)

Arguments

y

A numeric matrix. The data for the ith site should be in the ith row. Missing values are allowed, however each site must have at least one non-missing value. If starting values for beta are not specified, then each site must have at least two non-missing values.

sites

A numeric matrix with 2 columns giving site locations. It is best to normalized the columns.

iters

The number of iterations in the MCMC chain.

Qb

A symmetric non-negative definite neighbourhood matrix. If not specified, the off-diagonal elements are taken to be proportional to the negative inverse of the squared Euclidean distance, with the diagonal elements specified so that the rows and columns sum to zero. It is probably better to specify your own neighbourhood structure. Note that this implementation does not explicitly take advantage of any sparsity, so having a large numbers of zeros will not necessarily speed things up.

knots

A numeric matrix with 2 columns giving knot locations. By default the knots are taken to be the site locations.

X

The design matrix or matrices of the GEV parameters. Should be a list of length three containing design matrices for the location, log scale and shape respectively. Can also be a matrix, which is then used by all three parameters. By default, an intercept and the 2 columns in sites are used. Note that the intercept will not be affected by the data if the rows and columns of Qb sum to zero.

beta

A matrix with 3 columns with GEV parameter starting values for every site. If not specified, marginal method of moment estimators, assuming a zero shape, are used.

alpha

Starting value for alpha.

logbw

Starting value for the log bandwidth.

tau

Starting values for tau, for the three GEV parameters. This is the inverse of the delta values in the publication, so a lack of variation corresponds to large values. Since the posterior for the tau values has a closed form, this argument is relatively unimportant as it usually affects only the first couple of iterations.

logs

A matrix with rows equal to the number of knots and columns equal to the number of columns in y. Gives the starting values for the log of the positve stable variables.

u

A matrix with rows equal to the number of knots and columns equal to the number of columns in y. Gives the starting values for the U variables.

MHbeta

A matrix with 3 columns with GEV parameter jump standard deviations for every site.

MHalpha

Jump standard deviation value for alpha. It can be set to zero to fix alpha at the starting value.

MHlogbw

Jump standard deviation value for the log bandwidth. It can be set to zero to fix the bandwidth at the starting value.

MHs

A matrix with rows equal to the number of knots and columns equal to the number of columns in y. Gives the jump standard deviations for the log of the positve stable variables. It can be challenging to specify this to make the acceptance rates reasonable.

MHu

A matrix with rows equal to the number of knots and columns equal to the number of columns in y. Gives the jump standard deviations for the U variables.

pribeta

A vector of length three giving prior parameters for the three beta vectors. For simplicity each beta has a MVN(0, pI) prior, where p is a single parameter and I is the identity matrix of dimension corresponding to X.

prialpha

Shape1 and shape2 parameters of the prior beta distribution for alpha. See rbeta.

prilogbw

Mean and standard deviation parameters for the prior normal distribution for log bandwidth. See rnorm.

pritau

A vector of length three giving prior parameters for each of the three taus. For simplicity each tau has a beta(p,p) prior, where p is a single parameter, equal to both shape1 and shape2.See rbeta.

trace

Prints the log posterior density after every trace iterations. Use zero to supress printing.

Value

A list object with the following components

beta.samples

A three dimensional array containing the simulated GEV parameter values for each site. The first dimension is the number of iterations, the second is the number of sites, and the third corresponds to the three GEV parameters of location, log scale and shape.

param.samples

A matrix containing the linear predictor and tau parameters, and for abba also alpha and log bandwidth. The last column contains log posterior values.

psrv.samples

Only exists for function abba. A three dimensional array containing the simulated postive stable variables. The first dimension is the number of iterations, the second is the number of knots, and the third is the number of columns in y.

urv.samples

Only exists for function abba. A three dimensional array containing the simulated U variables. The first dimension is the number of iterations, the second is the number of knots, and the third is the number of columns in y.

Details

The function abba implements the method of Stephenson et al. (2014), which is a variation of Reich and Shaby (2012). The function abba_latent implements a standard latent variable approach which is a special case of abba, obtained when the parameter alpha is equal to one.

The function abba can be challenging to implement. In particular, it can be difficult to specify MHs to achieve suitable acceptance rates for all positive stable random variables. Also, alpha and the bandwidth may mix slowly. It is recommended that (i) the variables in sites, knots and X are standardized, and that (ii) the function abba_latent be used first in order to pass on good starting values to abba, and that (iii) you consider fixing either alpha or the bandwidth if there is slow mixing.

References

Stephenson, A. G., Shaby, B.A., Reich, B.J. and Sullivan, A.L. (2015). Estimating spatially varying severity thresholds of the forest fire danger rating system using max-stable extreme event modelling. Journal of Applied Meteorology and Climatology. In Press.

Reich, B.J. and Shaby, B.A. (2012). A hierarchical max-stable spatial model for extreme precipitation. Ann. Appl. Stat. 6(4), 1430-1451

See Also

rbeta, rnorm

Examples

Run this code
# NOT RUN {
  dat <- matrix(-log(rexp(9 * 20)), nrow = 9, ncol = 20)
  sites <- cbind(rep(c(-1,0,1),3), rep(c(-1,0,1),each = 3))
  abba_latent(dat, sites, iters = 50, trace = 10)
# }

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