JPL Technical Report Server

Geological interpretations of the topography of selected regions of Venus from Arecibo to Goldstone radar interferometry

Show simple item record

dc.contributor.author Jurgens, R. F. en_US
dc.contributor.author Margot, J. L. en_US
dc.contributor.author Simons, M. en_US
dc.contributor.author Pritchard, M. E. en_US
dc.contributor.author Slade, M. A. en_US
dc.date.accessioned 2004-11-09T22:47:58Z
dc.date.available 2004-11-09T22:47:58Z
dc.date.issued 2002-03-04 en_US
dc.identifier.citation 33rd Lunar and Planetary Science Conference en_US
dc.identifier.citation Houston, TX, USA en_US
dc.identifier.clearanceno 02-0507 en_US
dc.identifier.uri http://hdl.handle.net/2014/37095
dc.description.abstract We report on the geological interpretation of the mapping analysis of several successful radar experiments, which are part of a program to generate a high resolution digital elevation model (DEM) of the equatorial region of Venus between Phoebe Regio and far western Ovda Regio. These experiments used radar interferometry with Arecibo transmitting and Goldstone receiving. en_US
dc.format.extent 2947846 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Venus radar interferometry en_US
dc.title Geological interpretations of the topography of selected regions of Venus from Arecibo to Goldstone radar interferometry en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account