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dc.contributor.authorAbreu, P.-
dc.contributor.authorAglietta, M.-
dc.contributor.authorAhlers, M.-
dc.contributor.authorAhn, E. J.-
dc.contributor.authorPepe, Iuri Muniz-
dc.contributor.authorAlbuquerque, Ivone Freire da Mota e-
dc.contributor.authorAllekotte, I.-
dc.creatorAbreu, P.-
dc.creatorAglietta, M.-
dc.creatorAhlers, M.-
dc.creatorAhn, E. J.-
dc.creatorPepe, Iuri Muniz-
dc.creatorAlbuquerque, Ivone Freire da Mota e-
dc.creatorAllekotte, I.-
dc.date.accessioned2014-09-08T21:00:19Z-
dc.date.issued2013-
dc.identifier.issn0927-6505-
dc.identifier.urihttp://repositorio.ufba.br/ri/handle/ri/15845-
dc.descriptionTexto completo: acesso restrito. p. 92–101pt_BR
dc.description.abstractWe describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km2 of the Pierre Auger Observatory twice per hour with a spatial resolution of ∼2.4 km by ∼5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories.pt_BR
dc.language.isoenpt_BR
dc.rightsAcesso Abertopt_BR
dc.sourcehttp://dx.doi.org/10.1016/j.astropartphys.2013.09.004pt_BR
dc.subjectUltra-high energy cosmic rayspt_BR
dc.subjectPierre Auger Observatorypt_BR
dc.subjectExtensive air showerspt_BR
dc.subjectAtmospheric monitoringpt_BR
dc.subjectCloudspt_BR
dc.subjectSatellitespt_BR
dc.titleIdentifying clouds over the Pierre Auger Observatory using infrared satellite datapt_BR
dc.title.alternativeAstroparticle Physicspt_BR
dc.typeArtigo de Periódicopt_BR
dc.identifier.numberv. 50-52pt_BR
dc.embargo.liftdate10000-01-01-
Aparece en las colecciones: Artigo Publicado em Periódico (FIS)

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