Evidences for Sand Motion in the Equatorial Region of Mars

Details Evidences for Sand Motion in the Equatorial Region of Mars Evidences for Sand Motion in the Equatorial Region of Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2452c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2452

Physics

Scientific paper

In this work we investigate HiRISE images that allow multi-temporal
analysis of an erg in Herschel basin. We observed dune activity
suggesting that the dark dunes in the studied area are movable under the
present-day wind conditions.

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