Geology and surface characteristics of Bell Regio, Venus

Details Geology and surface characteristics of Bell Regio, Venus Geology and surface characteristics of Bell Regio, Venus

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..247c&link_type=abstract

In Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F p 247-248 (SEE N94-12015 01-91)

Mathematics

Logic

Backscattering, Planetary Geology, Topography, Venus Surface, Volcanology, Morphology, Scattering Cross Sections, Venus (Planet), Volcanoes

Scientific paper

Bell Regio is a broad topographic rise located at approximately 30 deg N, 45 deg E which extends approximately 1500 km in the N-S direction and is characterized by extensive volcanism. The geology and surface characteristics of Bell Regio are examined in order to understand the geologic evolution of the region and the surface characteristics of the major volcanic units. Relationships between Magellan SAR backscatter values and altimeter-derived ring slope data are analyzed, and terrestrial SAR data are used to suggest possible surface morphologies.

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