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 |