Sand Dunes Across the Dichotomy Boundary of Mars

Details Sand Dunes Across the Dichotomy Boundary of Mars Sand Dunes Across the Dichotomy Boundary of Mars

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1328s&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

MOC images were searched for aeolian ripples or dunes in a region from
60°S to 60°N latitude and 0° to 10°W longitude. The
majority of dunes were observed to be close to the dichotomy boundary
between the northern and southern hemispheres.

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