Modeling Thermal Transprt and Emission of Particle Ensembles

Details Modeling Thermal Transprt and Emission of Particle Ensembles Modeling Thermal Transprt and Emission of Particle Ensembles

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1666p&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1666

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Since 2004, Cassini's Composite Infra-Red Spectrometer (CIRS) has taken over a million spectra of Saturn's main rings. Almost all spectra are well fit with a Planck function and scalar multiplier, producing a database of effective temperature and emissivity that vary with location, illumination and viewing geometry. Use of this data to extract information about the rings has been complicated by the many parameters influencing the emission, and by computational difficulties. Here we present a new method for addressing two of the basic computational hurdles in producing verifiable models of Saturn's ring emission.

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