Dust Storms and Water Ice Clouds: Feature Detection for Use Onboard THEMIS

Details Dust Storms and Water Ice Clouds: Feature Detection for Use Onboard THEMIS Dust Storms and Water Ice Clouds: Feature Detection for Use Onboard THEMIS

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2287w&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2287

Physics

Scientific paper

We present results from three regression models that can detect
atmospheric features such as dust storms and water ice clouds on Mars.
These models show promise for future use onboard THEMIS.

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