Physics
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006georl..3311202s&link_type=abstract
Geophysical Research Letters, Volume 33, Issue 11, CiteID L11202
Physics
11
Atmospheric Composition And Structure: Planetary Atmospheres (5210, 5405, 5704), Atmospheric Processes: Land/Atmosphere Interactions (1218, 1631, 1843), Atmospheric Processes: Planetary Meteorology (5445, 5739), Planetary Sciences: Solar System Objects: Mars
Scientific paper
Fourteen active dust devils were observed by the High Resolution Stereo Camera (HRSC) on Mars Express, which enable the first analysis of the forward speed of dust devils on Mars determined from orbit. Results show speeds on the order of 20 m/s, which compares favorably with values of the wind profiles estimated from the Martian Climate Database for higher altitudes. Smaller dust devils of 1 km height and very small diameters were found moving only at 1.5 to 6.0 m/s in agreement with surface wind speeds.
Gerhard Neukum
Greeley Ronald
Hauber Ernst
Pätzold Martin
Stanzel Christina
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