Photochemical activity of HCN-C 4 H 2 ices in Titan's lower atmosphere
International audience Revealed by the Cassini and Voyager Missions, a plethora of volatile species are formed in Titan's upper atmosphere from the initial N 2 /CH 4 (~98/2%) composition. As they precipitate, most of the volatiles condense in the colder lower atmosphere where they can form icy...
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Bibliographic Details
Main Authors: |
Dubois, David,
Gudipati, Murthy,
Carrasco, Nathalie |
Other Authors: |
PLANETO - LATMOS,
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS),
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS),
Jet Propulsion Laboratory (JPL),
California Institute of Technology (CALTECH)-NASA |
Format: | Conference Object
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Language: | English |
Published: |
HAL CCSD
2018
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Subjects: |
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Online Access: | https://hal.archives-ouvertes.fr/hal-01796628
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