Convective Heat Transfer in Europa's Ocean and the Formation of Chaos Terrain

Details Convective Heat Transfer in Europa's Ocean and the Formation of Chaos Terrain Convective Heat Transfer in Europa's Ocean and the Formation of Chaos Terrain

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2903s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2903

Physics

Scientific paper

This work implies that thermal gradients along the bottom of the ice
shell due to underlying ocean circulation are important to consider for
the formation of chaos terrain and evolution of Europa’s ice
shell.

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