where ∥⋅∥ is the Euclidean distance, and δx=0 is 1 when x=0 and 0 otherwise. Here h∈R2 and u∈R. By default beta = 0 and it reduces to the separable model.
References
Gneiting, T. (2002). Nonseparable, Stationary Covariance Functions for Space–Time Data, Journal of the American Statistical Association, 97:458, 590-600.