Conference papers
Original deep convection in the atmosphere of Mars driven by the radiative impact of dust and water-ice particles
Abstract : Two examples of aerosol-induced deep convection in the Martian atmosphere broaden the knowledge of both aerosols-atmosphere interactions and mechanisms underlying convection in planetary atmospheres, as well as the impact of convection in the regional and global scale (e.g. emission of gravity waves), with possible comparative planetology approaches where the convective dynamics of Martian water-ice clouds could be compared to Venusian sulfuric-acid clouds
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Cited literature [17 references]
https://hal-insu.archives-ouvertes.fr/insu-01621402
Contributor : Catherine Cardon <>
Submitted on : Monday, October 23, 2017 - 1:39:42 PM
Last modification on : Friday, January 10, 2020 - 3:42:30 PM
Document(s) archivé(s) le : Wednesday, January 24, 2018 - 2:17:46 PM
Contributor : Catherine Cardon <>
Submitted on : Monday, October 23, 2017 - 1:39:42 PM
Last modification on : Friday, January 10, 2020 - 3:42:30 PM
Document(s) archivé(s) le : Wednesday, January 24, 2018 - 2:17:46 PM
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EPSC2017-428-2.pdf
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