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Physical and statistical modeling of Saturn's troposphere

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dc.contributor.author Yanamandra-Fisher, P. A. en_US
dc.contributor.author Braverman, A. en_US
dc.contributor.author Orton, G. S. en_US
dc.date.accessioned 2004-09-17T07:26:39Z
dc.date.available 2004-09-17T07:26:39Z
dc.date.issued 2002-08-22 en_US
dc.identifier.citation SPIE Proceedings Astronomical Telescopes and Instrumentation en_US
dc.identifier.citation Waikoloa, HI, USA en_US
dc.identifier.clearanceno 02-1939 en_US
dc.identifier.uri http://hdl.handle.net/2014/9789
dc.description.abstract We analyze the 5.2-pm spectra of Saturn by utilizing two independent methods: (a) physical models based on the relevant atmospheric parameters and (b) statistical analysis, based on principal components analysis (PCA), to determine the influence of the variation of phosphine and the opacity of clouds deep within Saturn's atmosphere to understand the dynamics in its atmosphere. en_US
dc.format.extent 3234755 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Saturn planetary atmospheres spectroscopy Phosphine statistical methods PCA en_US
dc.title Physical and statistical modeling of Saturn's troposphere en_US


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