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- W1642774675 abstract "In the search for buried water ice on Mars, radar sounding instruments have unique abilities. Their capacity to resolve glacial structures down to kilometers depth has already provided a huge amount of information related to Martian glaciers [e.g. 1, 2]. Sounding radars are also relevant tools to determine the composition of the surface, since the radar-waves reflectivity is sensitive to the dielectric properties of the sounding materials. It also has the originality to be representative of the first decameter of the surface (depending on the bandwidth), whereas other observations method do not exceed few millimeters. A reflectivity map from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) has been recently presented [3]. Here we present a method to extract the surface reflectivity from the SHAllow RADar (SHARAD/ASI) data, and the related results. The SHARAD along-track resolution gives the advantage to study areas at regional scales. SHARAD is a subsurface sounding instrument" @default.
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- W1642774675 date "2009-09-01" @default.
- W1642774675 modified "2023-10-18" @default.
- W1642774675 title "Mapping the radar reflectivity of the Martian surface with the SHAllow RADar (SHARAD)" @default.
- W1642774675 hasPublicationYear "2009" @default.
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