Comparative Analysis of Martian Dust Devil Track Morphologies in Gusev and Russell Craters

Details Comparative Analysis of Martian Dust Devil Track Morphologies in Gusev and Russell Craters Comparative Analysis of Martian Dust Devil Track Morphologies in Gusev and Russell Craters

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1979v&link_type=abstract

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

Physics

Scientific paper

Seasonal variations of dust devil activity in Russell and Gusev craters
are influenced by topography, sediment supply, and altitude, as well as
latitudinal variations in the atmospheric dust cycle and local winds.

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