Numerical Simulations of Convection in Europa's Ice Shell: Implications for Surface Features

Details Numerical Simulations of Convection in Europa's Ice Shell: Implications for Surface Features Numerical Simulations of Convection in Europa's Ice Shell: Implications for Surface Features

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1806s&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1806

Physics

1

Scientific paper

Numerical simulations of convection in Europa's ice shell show that
100-200 m-amplitude topography results from the convection under
reasonable conditions. This may help explain some, though not all, of
the numerous pits, uplifts, and spots seen on Europa's surface.

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