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Enabling repeat-pass interferomtetry from low Venus orbit

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dc.contributor.author Wallace, Mark S.
dc.contributor.author Sweetser, Theodore H.
dc.contributor.author Haw, Robert J.
dc.contributor.author Lau, Eunice
dc.contributor.author Hensley, Scott
dc.date.accessioned 2021-01-21T21:45:49Z
dc.date.available 2021-01-21T21:45:49Z
dc.date.issued 2019-01-13
dc.identifier.citation 29th AAS/AIAA Space Flight Mechanics Meeting, Ka'anapali, Hawaii, January 13-17, 2019 en_US
dc.identifier.clearanceno 19-0936
dc.identifier.uri http://hdl.handle.net/2014/50750
dc.description.abstract Repeat-pass interferometry is a powerful technique for determining changes in topography by flying a radar over the terrain two or more times. These overflights must be very close to each other in space. To design and maintain a low Venus orbit that enables this requires the consideration of drag, non-spherical gravity effects, and solar tides. Once the orbit is designed, the spacecraft must be navigated. To do so requires the use of radar-based terrain-relative navigation in addition to the traditional radiometric datatypes. The mission design and navigation to enable repeat-pass interferometry at Venus are described. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2019 en_US
dc.title Enabling repeat-pass interferomtetry from low Venus orbit en_US
dc.type Preprint en_US


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