Elevation-Corrected thermal inertia and derived particle size on Mars and implications for the Tharsis Montes
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v021/i009/94GL00368/94GL00368.pdf
Reference15 articles.
1. Regional dust deposits on Mars: Physical properties, age, and history;Christensen;J. of Geophys. Res.,1986
2. The spatial distribution of rocks on Mars;Christensen;Icarus,1986
3. Atmospheric effects on the remote determination of thermal inertia on Mars;Haberle;Icarus,1991
4. On the thermal properties of Martian fines;Jakosky;Icarus,1986
5. Global duricrust on Mars: Analysis of remote-sensing data;Jakosky;J. Geophys. Res.,1986
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1. Aeolian bedforms, yardangs, and indurated surfaces in the Tharsis Montes as seen by the HiRISE Camera: Evidence for dust aggregates;Icarus;2010-01
2. MGS-TES thermal inertia study of the Arsia Mons Caldera;Journal of Geophysical Research;2008-06-25
3. Windy Mars: A dynamic planet as seen by the HiRISE camera;Geophysical Research Letters;2007-12-15
4. The geology of the Viking Lander 2 site revisited;Icarus;2007-11
5. High-resolution thermal inertia derived from the Thermal Emission Imaging System (THEMIS): Thermal model and applications;Journal of Geophysical Research: Planets;2006-12
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