North-South Roughness Anisotropy on Venus: Magellan Altimeter Data Revisited

Details North-South Roughness Anisotropy on Venus: Magellan Altimeter Data Revisited North-South Roughness Anisotropy on Venus: Magellan Altimeter Data Revisited

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1236b&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1236

Computer Science

Scientific paper

Shift of the strongest radar altimeter echo from nadir is used to map
north-south small-scale slope asymmetry. We compare the asymmetry
features with geology. The asymmetry map is useful for studies of
surficial deposits and their evolution.

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