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    Online Resource
    Online Resource
    Oxford University Press (OUP) ; 2008
    In:  Journal of the Royal Statistical Society Series C: Applied Statistics Vol. 57, No. 3 ( 2008-06-01), p. 343-355
    In: Journal of the Royal Statistical Society Series C: Applied Statistics, Oxford University Press (OUP), Vol. 57, No. 3 ( 2008-06-01), p. 343-355
    Abstract: To investigate the variability in energy output from a network of photovoltaic cells, solar radiation was recorded at 10 sites every 10 min in the Pentland Hills to the south of Edinburgh. We identify spatiotemporal auto-regressive moving average models as the most appropriate to address this problem. Although previously considered computationally prohibitive to work with, we show that by approximating using toroidal space and fitting by matching auto-correlations, calculations can be substantially reduced. We find that a first-order spatiotemporal auto-regressive (STAR(1)) process with a first-order neighbourhood structure and a Matern noise process provide an adequate fit to the data, and we demonstrate its use in simulating realizations of energy output.
    Type of Medium: Online Resource
    ISSN: 0035-9254 , 1467-9876
    RVK:
    Language: English
    Publisher: Oxford University Press (OUP)
    Publication Date: 2008
    detail.hit.zdb_id: 204797-4
    detail.hit.zdb_id: 1482300-7
    detail.hit.zdb_id: 1476894-X
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