JPL Technical Report Server

(abstract) Radiophysical Properties of Venusian Impact Craters

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account