TY - JOUR
T1 - Max-stable processes for modeling extremes observed in space and time
AU - Davis, Richard A.
AU - Klüppelberg, Claudia
AU - Steinkohl, Christina
N1 - Funding Information:
All authors gratefully acknowledge the support by the TUM Institute for Advanced Study (TUM-IAS). The third author would also like to thank the International Graduate School of Science and Engineering (IGSSE) of the Technische Universität München for their support. The research of Richard A. Davis was also supported in part by the National Science Foundation grant DMS-1107031 .
PY - 2013/9
Y1 - 2013/9
N2 - Max-stable processes have proved to be useful for the statistical modeling of spatial extremes. For statistical inference it is often assumed that there is no temporal dependence; i.e., that the observations at spatial locations are independent in time. In a first approach we construct max-stable space-time processes as limits of rescaled pointwise maxima of independent Gaussian processes, where the space-time covariance functions satisfy weak regularity conditions. This leads to so-called Brown-Resnick processes. In a second approach, we extend Smith's storm profile model to a space-time setting. We provide explicit expressions for the bivariate distribution functions, which are equal under appropriate choice of the parameters. We also show how the space-time covariance function of the underlying Gaussian process can be interpreted in terms of the tail dependence function in the limiting max-stable space-time process.
AB - Max-stable processes have proved to be useful for the statistical modeling of spatial extremes. For statistical inference it is often assumed that there is no temporal dependence; i.e., that the observations at spatial locations are independent in time. In a first approach we construct max-stable space-time processes as limits of rescaled pointwise maxima of independent Gaussian processes, where the space-time covariance functions satisfy weak regularity conditions. This leads to so-called Brown-Resnick processes. In a second approach, we extend Smith's storm profile model to a space-time setting. We provide explicit expressions for the bivariate distribution functions, which are equal under appropriate choice of the parameters. We also show how the space-time covariance function of the underlying Gaussian process can be interpreted in terms of the tail dependence function in the limiting max-stable space-time process.
KW - Brown-Resnick process
KW - Gneiting's class
KW - Max-stable process
KW - Random field in space and time
KW - Smith's storm profile model
KW - Spatio-temporal correlation function
UR - http://www.scopus.com/inward/record.url?scp=84880045343&partnerID=8YFLogxK
U2 - 10.1016/j.jkss.2013.01.002
DO - 10.1016/j.jkss.2013.01.002
M3 - Article
AN - SCOPUS:84880045343
SN - 1226-3192
VL - 42
SP - 399
EP - 414
JO - Journal of the Korean Statistical Society
JF - Journal of the Korean Statistical Society
IS - 3
ER -