Developments in Deriving Best-Fit Thermal Inertia of the Surface of Mars Using THEMIS Images

Details Developments in Deriving Best-Fit Thermal Inertia of the Surface of Mars Using THEMIS Images Developments in Deriving Best-Fit Thermal Inertia of the Surface of Mars Using THEMIS Images

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1773s&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

We improve the resolution and accuracy of derived thermal inertia of the
martian surface by 1) Implementing a validity test for THEMIS images
based on a thermal model and 2) Using HRSC topography to produce high
resolution slope and azimuth data.

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