Modeling the Sublimation-driven Atmosphere of Io with DSMC

Details Modeling the Sublimation-driven Atmosphere of Io with DSMC Modeling the Sublimation-driven Atmosphere of Io with DSMC

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1548w&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1548

Physics

Scientific paper

Io’s sublimation-driven atmosphere is modeled using the Direct
Simulation Monte Carlo (DSMC) method. The effects of plasma heating,
planetary rotation, inhomogeneous surface frost, molecular residence
time, and surface temperature distribution are investigated.

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