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Isostasy Models and Correlations of Geoid and Topography Data for Characteristic Highlands on Venus

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dc.contributor.author Kucinskas, A. en_US
dc.contributor.author Turcotte, D. en_US
dc.date.accessioned 2004-10-04T22:26:19Z
dc.date.available 2004-10-04T22:26:19Z
dc.date.issued 1994-03-14 en_US
dc.identifier.citation 25th Lunar and Planetary Science Conference en_US
dc.identifier.citation Houston, Texas, USA en_US
dc.identifier.clearanceno 94-0136 en_US
dc.identifier.uri http://hdl.handle.net/2014/32399
dc.description.abstract We have used the newest solution for the Venus geopotential, incorporating tracking data from the circularized orbit of Magellan, along with global Venus topography data to study correlations of geoid and topography variations in several regions characteristic of the principal classes of highlands found on Venus. en_US
dc.format.extent 331295 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other geoid and topography data isostatic compensation models Venus en_US
dc.title Isostasy Models and Correlations of Geoid and Topography Data for Characteristic Highlands on Venus en_US


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