A Search for Activity on Mimas, Tethys, and Dione with the Cassini Visual and Infrared Mapping Spectrometer

Details A Search for Activity on Mimas, Tethys, and Dione with the Cassini Visual and Infrared Mapping Spectrometer A Search for Activity on Mimas, Tethys, and Dione with the Cassini Visual and Infrared Mapping Spectrometer

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1389b&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1389

Computer Science

Scientific paper

Observations of the forward-scattered component of the solar phase
curves of Mimas, Tethys, and Dione places a limit on plume activity of
less than 1% that of Enceladus.

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