Near-Surface Wind Speeds Inferred from Movement of Sand Grains Observed by Spirit in Gusev Crater, Mars

Details Near-Surface Wind Speeds Inferred from Movement of Sand Grains Observed by Spirit in Gusev Crater, Mars Near-Surface Wind Speeds Inferred from Movement of Sand Grains Observed by Spirit in Gusev Crater, Mars

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2218w&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

1

Scientific paper

Wind is the dominant agent of surface modification on Mars in the
current environment, as evidenced by active dust storms and abundant
wind-related surface features observed from orbit and the ground.

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