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Titan's global map combining VIMS and ISS mosaics

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dc.contributor.author Seignovert, Benoit
dc.contributor.author Le Mouelic, Stephan
dc.contributor.author Brown, Robert H.
dc.contributor.author Joseph, Emily C.S.
dc.contributor.author Karkoschka, Erick
dc.contributor.author Pasek, Virginia
dc.contributor.author Sotin, Christophe
dc.contributor.author Turtle, Elizabeth P.
dc.date.accessioned 2021-03-03T20:19:00Z
dc.date.available 2021-03-03T20:19:00Z
dc.date.issued 2019-09-15
dc.identifier.citation EPSC - European Planetary Science Congress 2019,Geneva, Switzerland, September 15-20, 2019 en_US
dc.identifier.clearanceno 19-2585
dc.identifier.uri http://hdl.handle.net/2014/51203
dc.description.abstract Titan, Saturn’s largest moon, is the only ocean world, besides Earth, with a dense atmosphere. This outstanding feature is also a challenge since it was believed before the launch of the Cassini mission that optical cameras (visible and infrared) could not see the surface and that only radar instruments could map Titan’s surface. However, the Visual and Infrared Mapping Spectrometer (VIMS) and the Imaging Science Subsystem (ISS) onboard the Cassini spacecraft demonstrated that Titan’s surface can be observed in several infrared atmospheric windows. 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 Titan's global map combining VIMS and ISS mosaics en_US
dc.type Preprint en_US


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