The use of solar radiation models to derive atmospheric turbidity: An inter-comparison study

Sbarbaro, Daniel; Trigo Gonzalez, M.; Fuentealba Vidal, E.; Moran, Luis

Abstract

© 2019. The Authors. Published by International Solar Energy Society Selection and/or peer review under responsibility of Scientific CommitteeThis study inter-compares the most important retrieval methods that derive atmospheric turbidity from measured Direct Normal Irradiance. A number of parametric solar radiation models are used backward to estimate the atmospheric turbidity indices. To reduce error propagation, each turbidity index are derived using a specific set of models. Then, an inter-comparison between all the selected models are carried out to establish degree of agreement between the models. High-resolution solar radiation data, at one-minute intervals, taken from Plataforma Solar del Desierto de Atacama, is used in this investigation. Results shows that seven models (among 11 models) generally agree well, with a maximum difference of 0.004 in the estimation of the Angstrom coefficient. Besides, Kasten's pyrheliometric method performs as good as sophisticated solar radiation models such as METSTAT, MWLT1, MWLT2, REST and Yang.

Más información

Título según WOS: The use of solar radiation models to derive atmospheric turbidity: An inter-comparison study
Fecha de publicación: 2019
Página de inicio: 1871
Página final: 1882
DOI:

10.18086/SWC.2019.42.02

Notas: ISI