dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade de São Paulo (USP)
dc.contributorUniversidade Federal de Goiás (UFG)
dc.date.accessioned2014-05-20T15:24:13Z
dc.date.accessioned2022-10-05T16:27:09Z
dc.date.available2014-05-20T15:24:13Z
dc.date.available2022-10-05T16:27:09Z
dc.date.created2014-05-20T15:24:13Z
dc.date.issued2003-09-01
dc.identifierTheoretical and Applied Climatology. Vienna: Springer-verlag Wien, v. 75, n. 3-4, p. 213-224, 2003.
dc.identifier0177-798X
dc.identifierhttp://hdl.handle.net/11449/34867
dc.identifier10.1007/s00704-003-0733-9
dc.identifierWOS:000185964800007
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3906921
dc.description.abstractFive minute-averaged values of sky clearness, direct and diffuse indices, were used to model the frequency distributions of these variables in terms of optical air mass. From more than four years of solar radiation observations it was found that variations in the frequency distributions of the three indices of optical air mass for Botucatu, Brazil, are similar to those in other places, as published in the literature. The proposed models were obtained by linear combination of normalized Beta probability functions, using the observed distributions derived from three years of data. The versatility of these functions allows modelling of all three irradiance indexes to similar levels of accuracy. A comparison with the observed distributions obtained from one year of observations indicate that the models are able to reproduce the observed frequency distributions of all three indices at the 95% confidence level.
dc.languageeng
dc.publisherSpringer
dc.relationTheoretical and Applied Climatology
dc.relation2.321
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titleModelling frequency distributions of 5 minute-averaged solar radiation indexes using Beta probability functions
dc.typeArtigo


Este ítem pertenece a la siguiente institución