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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/41851
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dc.contributor.authorEscobedo, João Francisco-
dc.contributor.authorGomes, Eduardo N.-
dc.contributor.authorOliveira, Amauri P.-
dc.contributor.authorSoares, Jacyra-
dc.date.accessioned2014-05-20T15:33:08Z-
dc.date.accessioned2016-10-25T18:09:36Z-
dc.date.available2014-05-20T15:33:08Z-
dc.date.available2016-10-25T18:09:36Z-
dc.date.issued2009-03-01-
dc.identifierhttp://dx.doi.org/10.1016/j.apenergy.2008.04.013-
dc.identifier.citationApplied Energy. Oxford: Elsevier B.V., v. 86, n. 3, p. 299-309, 2009.-
dc.identifier.issn0306-2619-
dc.identifier.urihttp://hdl.handle.net/11449/41851-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/41851-
dc.description.abstractIn this analysis, using available hourly and daily radiometric data performed at Botucatu, Brazil, several empirical models relating ultraviolet (UV), photosynthetically active (PAR) and near infrared (NIR) solar global components with solar global radiation (G) are established. These models are developed and discussed through clearness index K(T) (ratio of the global-to-extraterrestrial solar radiation). Results obtained reveal that the proposed empirical models predict hourly and daily values accurately. Finally. the overall analysis carried Out demonstrates that the sky conditions are more important in developing correlation models between the UV component and the global solar radiation. The linear regression models derived to estimate PAR and NIR components may be obtained without sky condition considerations within a maximum variation of 8%. In the case of UV, not taking into consideration the sky condition may cause a discrepancy of up to 18% for hourly values and 15% for daily values. (C) 2008 Elsevier Ltd. All rights reserved.en
dc.format.extent299-309-
dc.language.isoeng-
dc.publisherElsevier B.V.-
dc.sourceWeb of Science-
dc.subjectGlobal UVen
dc.subjectPARen
dc.subjectNIR solar componentsen
dc.subjectGlobal solar radiationen
dc.subjectClearness indexen
dc.subjectPercent UVen
dc.subjectPARen
dc.subjectNIR ratiosen
dc.subjectBotucatuen
dc.subjectBrazilen
dc.titleModeling hourly and daily fractions of UV, PAR and NIR to global solar radiation under various sky conditions at Botucatu, Brazilen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv São Paulo, Inst Astron Geophys & Atmospher Sci, Dept Atmospher Sci, São Paulo, Brazil-
dc.description.affiliationState Univ São Paulo, Sch Agron Sci, Dept Nat Resources, São Paulo, Brazil-
dc.description.affiliationUnespState Univ São Paulo, Sch Agron Sci, Dept Nat Resources, São Paulo, Brazil-
dc.identifier.doi10.1016/j.apenergy.2008.04.013-
dc.identifier.wosWOS:000262219600004-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofApplied Energy-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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