(abstract) Radiophysical Properties of Venusian Impact Craters

Weitz, C.M.; Saunders, R.S.; Plaut, J.J.; Elachi, C.; Moore, H.J.

dc.contributor.author	Weitz, C.M.	en_US
dc.contributor.author	Saunders, R.S.	en_US
dc.contributor.author	Plaut, J.J.	en_US
dc.contributor.author	Elachi, C.	en_US
dc.contributor.author	Moore, H.J.	en_US
dc.date.accessioned	2004-10-06T01:42:20Z
dc.date.available	2004-10-06T01:42:20Z
dc.date.issued	1993-05-24	en_US
dc.identifier.citation	Baltimore, MD	en_US
dc.identifier.clearanceno	93-0476	en_US
dc.identifier.uri	http://hdl.handle.net/2014/35004
dc.description.abstract	An 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.	en_US
dc.format.extent	24101 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	Venus Magellan terrain radar imaging radiophysical properties impact craters morphology	en_US
dc.title	(abstract) Radiophysical Properties of Venusian Impact Craters	en_US