Radial variation of lunar crater rim topography

Details Radial variation of lunar crater rim topography Radial variation of lunar crater rim topography

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977icar...31..123s&link_type=abstract

Icarus, vol. 31, May 1977, p. 123-135.

Mathematics

Logic

8

Geomorphology, Lunar Craters, Lunar Surface, Structural Properties (Geology), Topography, Data Acquisition, Data Reduction, Elevation, Plateaus

Scientific paper

The paper presents results of determinations of variations of rim topography as a function of range from the crater rim for a group of morphologically fresh craters. It is found that the rate at which exterior crater topography converges with the surrounding surface is highly variable among different radial directions at individual craters as well as between different craters, and that at several craters, oblique impact appears to have contributed to azimuthal elevation/range variations.

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