Exogenetic processes and the roughness of the Venus surface according to radar observations

Details Exogenetic processes and the roughness of the Venus surface according to radar observations Exogenetic processes and the roughness of the Venus surface according to radar observations

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..268k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Mar.-Apr. 1985, p. 268-275. In Russian.

Mathematics

Logic

Radar Measurement, Surface Roughness, Venus Radar Echoes, Venus Surface, Height, Landing Sites, Pioneer Venus Spacecraft, Space Based Radar

Scientific paper

Earth-based and Pioneer-Venus radar observations of the Venus surface were used to analyze the two-scale (centimeter and meter-decameter) roughness distribution at different hypsometric levels. The distribution of roughness classes with change in height is compared with the character of the hypsometric curve, which made it possible to identify the height zonality of roughness. These zones are characterized from the viewpoint of exogenetic processes on the basis of a comparison of geological situations at the landing sites of the Venera 9, 10, 13, and 14 with the degree of roughness in these areas.

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