A model of diffuse radar scattering from Martian surface rocks
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference19 articles.
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2. Martian dust mantling and surface composition: Interpretation of thermophysical properties;Christensen;J. Geophys. Res.,1982
3. The spatial distribution of rocks on Mars;Christensen;Icarus,1986
4. Regional dust deposits on Mars: Physical properties, age, and history;Christensen;J. Geophys. Res.,1986
5. Martian topography and surface properties as seen by radar: The 1971 opposition;Downs;Icarus,1973
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1. The effects of the martian regolith on GCM water cycle simulations;Icarus;2005-09
2. Asteroid 4179 Toutatis: 1996 Radar Observations;Icarus;1999-01
3. Estimation of Mars radar backscatter from measured surface rock populations;Journal of Geophysical Research: Planets;1998-09-01
4. Interpretation of planetary radar observations: the relationship between actual and inferred slope distributions;Journal of Geophysical Research: Planets;1993-01-25
5. Mars radar scattering: Arecibo/Goldstone results at 12.6- and 3.5-cm wavelengths;Icarus;1992-08
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