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Covariance functions for multivariate Gaussian fields evolving temporally over planet earth

机译:行星地球上随时间演化的多元高斯场的协方差函数

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The construction of valid and flexible cross-covariance functions is a fundamental task for modeling multivariate space-time data arising from, e.g., climatological and oceanographical phenomena. Indeed, a suitable specification of the covariance structure allows to capture both the space-time dependencies between the observations and the development of accurate predictions. For data observed over large portions of planet earth it is necessary to take into account the curvature of the planet. Hence the need for random field models defined over spheres across time. In particular, the associated covariance function should depend on the geodesic distance, which is the most natural metric over the spherical surface. In this work, we propose a flexible parametric family of matrix-valued covariance functions, with both marginal and cross structure being of the Gneiting type. We also introduce a different multivariate Gneiting model based on the adaptation of the latent dimension approach to the spherical context. Finally, we assess the performance of our models through the study of a bivariate space-time data set of surface air temperatures and precipitable water content.
机译:有效和灵活的互协方差函数的构建是建模例如气候和海洋学现象产生的多元时空数据的基本任务。确实,协方差结构的合适规范允许捕获观测值之间的时空依赖性以及精确预测的发展。对于在地球大部分区域观察到的数据,必须考虑到行星的曲率。因此,需要跨时间跨球定义的随机场模型。特别是,相关的协方差函数应取决于测地线距离,该距离是球面上最自然的度量。在这项工作中,我们提出了矩阵值协方差函数的一个灵活的参数族,其边际结构和交叉结构均为Gneiting类型。我们还基于潜在维度方法对球形上下文的适应性引入了不同的多元Gneiting模型。最后,我们通过研究地表气温和可降水量的双变量时空数据集来评估模型的性能。

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