Io's UV-V Eclipse Emission: Implications for Pele-type Plumes

Details Io's UV-V Eclipse Emission: Implications for Pele-type Plumes Io's UV-V Eclipse Emission: Implications for Pele-type Plumes

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2353m&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2353

Physics

1

Scientific paper

Simulations of Io's NUV-V emission in eclipse show that S2-rich giant
plumes' S2 concentrations and activity levels effect the absolute
brightness and the east/west intensity ratio across Io allowing for
plume activity to be determined from observed spectra.

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