Topography and Roughness Signatures of Erosion of Crusted Soils on Mars

Details Topography and Roughness Signatures of Erosion of Crusted Soils on Mars Topography and Roughness Signatures of Erosion of Crusted Soils on Mars

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1999c&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1999

Physics

Scientific paper

MOLA slope and roughness data shed light on the erosion of regional
duricrust and suggest it follows preexisting topography. This implies
that cementation of the duricrust was likely due to atmosphere-surface
interactions or in situ alteration.

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