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  4. Radar Subsurface Sounding Over the Putative Frozen Sea in Cerberus Palus, Mars
 
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Radar Subsurface Sounding Over the Putative Frozen Sea in Cerberus Palus, Mars

Author(s)
Flamini, Enrico  
Orosei, R.
Cartacci, M.
Cicchetti, A.
Subjects

5422 Ices

5464 Remote sensing

5470 Surface material...

6225 Mars

6949 Radar astronomy

Date Issued
2007-12-01
Abstract
The area of Mars known as Cerberus Palus, suspected of harboring a frozen body of water, has been observed by the two subsurface sounding radar MARSIS and SHARAD. SHARAD data reveal subsurface interfaces at depths ranging from 50 m to 150 m which could be interpreted as either the bottom of an ice sheet lying over bedrock, or an interface between two lava flows. Echoes have been analyzed to estimate the dielectric properties of the surface layer, and results favor the interpretation that no ice is present in the area.
URI
https://hdl.handle.net/20.500.13025/2170
URL
http://adsabs.harvard.edu/abs/2007AGUFM.P14B..05O
http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=5550143
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