Interfacial Liquid Water On Mars: Can It Form Hill Gullies?

Details Interfacial Liquid Water On Mars: Can It Form Hill Gullies? Interfacial Liquid Water On Mars: Can It Form Hill Gullies?

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1702k&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1702

Physics

Scientific paper

We model both the diurnal and the seasonal cycle of the interfacial
liquid water in the context of a possible mechanism for formation of the
so called hill gullies.

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