Saturn's He and CH4 Abundances from Cassini VIMS Occultations & CIRS Limb Spectra

Details Saturn's He and CH4 Abundances from Cassini VIMS Occultations & CIRS Limb Spectra Saturn's He and CH4 Abundances from Cassini VIMS Occultations & CIRS Limb Spectra

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1548b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1548

Computer Science

Scientific paper

Cassini VIMS stellar occultations by Saturn, in concert with Cassini CIRS Saturn limb spectra have been used to infer the Helium abundance on Saturn, as well as methane abundance and temperature profiles from about 5 mbar to about 0.01 mbar. In addition we will report some constraints on methane transmissivities inferred from the occultations. The techniques we employ are discussed in detail in a companion abstract by Gierasch et al. [1].

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