constant and surface roughness estimation over the lunar surface using multi- frequency data.
(c) Investigation of geo- morphological features especially in the polar regions and preparation
of geomorphological maps and high- resolution crater oor maps. (d) Quantitative estimation
of regolith thickness and distribution over selected regions using data from dual- frequency
radiometer mode. [19]
17.4 CRATER FORMATION
Impact craters usually occur to all celestial bodies in the solar system that have solid surfaces in
nature. Earth has a thick atmosphere, however, so meteoroids that enter the atmosphere ...
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