Half-Spectral Space-Time Covariance Models
Michael T. Horrell, Michael L. Stein

TL;DR
This paper introduces two novel classes of space-time Gaussian process models using half-spectral covariance functions, providing theoretical insights and demonstrating improved data fitting over existing models.
Contribution
The paper develops two new space-time Gaussian process models based on half-spectral covariance functions and analyzes their theoretical properties.
Findings
Models fit wind power data better than existing space-time models.
Derived conditions for mean-square differentiability of processes.
Established regularity conditions for spectral densities.
Abstract
We develop two new classes of space-time Gaussian process models by specifying covariance functions using what we call a half-spectral representation. The half-spectral representation of a covariance function, , is a special case of standard spectral representations. In addition to the introduction of two new model classes, we also develop desirable theoretical properties of certain half-spectral forms. In particular, for a half-spectral model, , we determine spatial and temporal mean-square differentiability properties of a Gaussian process governed by , and we determine whether or not the spectral density of meets a regularity condition motivated by a screening effect analysis. We fit models we develop in this paper to a wind power dataset, and we show our models fit these data better than other separable and non-separable space-time models.
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