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(abstract) Radiophysical Properties of Venusian Impact CratersAn analysis of 222 large (greater than 20-km-diameter) impact craters on Venus using both cycle 1 and cycle 2 Magellan data is being conducted to determine the radiophysical properties (i.e., backscatter cross section, emissivity, reflectivity, rms slope) of the craters and to search for correlations with target region properties and subsequent geological history.
Document ID
20060038747
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/35004
Authors
Weitz, C. M.
Saunders, R. S.
Plaut, J. J.
Elachi, C.
Moore, H. J.
Date Acquired
August 23, 2013
Publication Date
May 24, 1993
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Other
Keywords
morphology
Venus Magellan terrain radar imaging radiophysical properties impact craters

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