Article ID Journal Published Year Pages File Type
1773648 Icarus 2012 17 Pages PDF
Abstract
► The regolith thickness of four regions over the lunar nearside is inverted. ► A relation among dielectric constant of regolith and its composition is derived. ► A tradeoff relation between lunar surface roughness and buried rocks is derived. ► Regolith thickness of the maria is generally smaller than that of highlands.
Keywords
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
Preview
Regolith thickness over the lunar nearside: Results from Earth-based 70-cm Arecibo radar observations
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