Thermal inertias in the upper millimeters of the Martian surface derived using Phobos' shadow

Author:

Betts Bruce H.,Murray Bruce C.,Svítek Tomáš

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference19 articles.

1. Edited Termoskan and raw data files and descriptions;Betts;PDS (Planetary Data System) Phobos '88 CD-ROM,1992

2. Thermal and visible studies of Mars using the Termoskan data set;Betts,1993

3. Preliminary quantitative assessment and analysis of Phobos 88 Termoskan observations of Mars (abstract);Betts;Lunar Planet. Sci.,1990

4. Martian dust mantling and surface composition: Interpretation of thermophysical properties;Christensen;J. Geophys. Res.,1982

5. The Distribution of rocks on Mars (abstract);Christensen;Lunar Planet. Sci.,1983

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