Convective Instability in Ice I: Application to Callisto and Ganymede

Details Convective Instability in Ice I: Application to Callisto and Ganymede Convective Instability in Ice I: Application to Callisto and Ganymede

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1945b&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1945

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Scientific paper

The non-Newtonian behavior of ice adds complexity to the question of
whether we expect an ice I layer to convect or not; study of the
consequences of convection in an icy satellite must consider initial
conditions in addition to physical, thermal, and rheological parameters.

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