June 2015 Gaussian random particles with flexible Hausdorff dimension
Linda V. Hansen, Thordis L. Thorarinsdottir, Evgeni Ovcharov, Tilmann Gneiting, Donald Richards
Author Affiliations +
Adv. in Appl. Probab. 47(2): 307-327 (June 2015). DOI: 10.1239/aap/1435236977

Abstract

Gaussian particles provide a flexible framework for modelling and simulating three-dimensional star-shaped random sets. In our framework, the radial function of the particle arises from a kernel smoothing, and is associated with an isotropic random field on the sphere. If the kernel is a von Mises-Fisher density, or uniform on a spherical cap, the correlation function of the associated random field admits a closed form expression. The Hausdorff dimension of the surface of the Gaussian particle reflects the decay of the correlation function at the origin, as quantified by the fractal index. Under power kernels we obtain particles with boundaries of any Hausdorff dimension between 2 and 3.

Citation

Download Citation

Linda V. Hansen. Thordis L. Thorarinsdottir. Evgeni Ovcharov. Tilmann Gneiting. Donald Richards. "Gaussian random particles with flexible Hausdorff dimension." Adv. in Appl. Probab. 47 (2) 307 - 327, June 2015. https://doi.org/10.1239/aap/1435236977

Information

Published: June 2015
First available in Project Euclid: 25 June 2015

zbMATH: 1352.60013
MathSciNet: MR3360379
Digital Object Identifier: 10.1239/aap/1435236977

Subjects:
Primary: 60D05
Secondary: 37F35 , 60G60

Keywords: Celestial body , correlation function , fractal dimension , Lévy basis , random field on a sphere , simulation of star-shaped random set

Rights: Copyright © 2015 Applied Probability Trust

JOURNAL ARTICLE
21 PAGES

This article is only available to subscribers.
It is not available for individual sale.
+ SAVE TO MY LIBRARY

Vol.47 • No. 2 • June 2015
Back to Top