Aeolian Sediment Sources and Transport in Ganges Chasma, Mars: Morphology and Atmospheric Modeling

Details Aeolian Sediment Sources and Transport in Ganges Chasma, Mars: Morphology and Atmospheric Modeling Aeolian Sediment Sources and Transport in Ganges Chasma, Mars: Morphology and Atmospheric Modeling

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2441f&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2441

Physics

Scientific paper

We present first results from aeolian bedform mapping and atmospheric
modeling in Ganges Chasma that suggest (1) sand sources are widespread
throughout the chasma and (2) saltation threshold friction velocities
may be lower than expected.

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