Preliminary Evidence for a Debris Flow Gully Slope-Area Relationship on Mars and Implications for a Source Liquid

Details Preliminary Evidence for a Debris Flow Gully Slope-Area Relationship on Mars and Implications for a Source Liquid Preliminary Evidence for a Debris Flow Gully Slope-Area Relationship on Mars and Implications for a Source Liquid

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2225l&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Computer Science

Scientific paper

We compare morphometric characteristics of terrestrial gullies
associated with debris flows with a subset of martian gullies to test
the hypothesis that these martian gullies are formed by saturation and
failure of the regolith.

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