Comparison of Cassini-CIRS Thermal Observations of Saturn's B Ring to a New Multi-Scale Heat Transfer Model

Details Comparison of Cassini-CIRS Thermal Observations of Saturn's B Ring to a New Multi-Scale Heat Transfer Model Comparison of Cassini-CIRS Thermal Observations of Saturn's B Ring to a New Multi-Scale Heat Transfer Model

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1979r&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1979

Physics

Scientific paper

The thermal evolution of Saturn’s B ring has been monitored using
the Cassini-CIRS spectrometer. Confrontation to a new multiscale heat
transfer model allows retrieval of the physical properties of the
particles and the structure of the ring.

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