Transport-driven formation of an ozone layer on Venus and Mars as evidenced by SPICAM and SPICAV
Cross-hemispheric circulation of the atmosphere is a major feature of the Martian troposphere and Venusian thermosphere. On Mars, it is driven by the latitudinal gradient of insolation at the surface, which generates a global summer-to-winter Hadley cell reversing orientation during equinoxes and ma...
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Bibliographic Details
Main Authors: |
Montmessin, Franck,
Bertaux, Jean-Loup,
Lefèvre, Franck,
Gondet, Brigitte,
Marcq, Emmanuel,
Reberac, Aurélie,
Sarago, Vincent |
Other Authors: |
PLANETO - LATMOS,
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS),
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS),
Institut d'astrophysique spatiale (IAS),
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES),
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) |
Format: | Conference Object
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Language: | English |
Published: |
HAL CCSD
2010
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Subjects: |
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Online Access: | https://hal.science/hal-00667054
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