A high resolution study of the Martian water cycle with a global climate model
International audience The martian water cycle's main source is the northern polar cap. Running high resolution models, up to 360° per 180°, help better resolve this ice cap, and better mimic the gradual retreat of the seasonal cap. Atmospheric circulation is also better resolved. Water vapor a...
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ftepunivpsaclay:oai:HAL:insu-01217131v1 2024-06-09T07:46:41+00:00 A high resolution study of the Martian water cycle with a global climate model Pottier, Alizée Montmessin, Franck Forget, François Navarro, Thomas Millour, Ehouarn Madeleine, Jean-Baptiste Spiga, Aymeric 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) Laboratoire de Météorologie Dynamique (UMR 8539) (LMD) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL) Nantes, France 2015-09-27 https://insu.hal.science/insu-01217131 https://insu.hal.science/insu-01217131/document https://insu.hal.science/insu-01217131/file/EPSC2015-215.pdf en eng HAL CCSD Copernicus Meetings insu-01217131 https://insu.hal.science/insu-01217131 https://insu.hal.science/insu-01217131/document https://insu.hal.science/insu-01217131/file/EPSC2015-215.pdf info:eu-repo/semantics/OpenAccess European Planetary Science Congress 2015, 27 September – 02 October 2015, La Cité des Congrès, Nantes, France European Planetary Science Congress 2015 https://insu.hal.science/insu-01217131 European Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-215 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] info:eu-repo/semantics/conferenceObject Conference papers 2015 ftepunivpsaclay 2024-05-16T12:40:51Z International audience The martian water cycle's main source is the northern polar cap. Running high resolution models, up to 360° per 180°, help better resolve this ice cap, and better mimic the gradual retreat of the seasonal cap. Atmospheric circulation is also better resolved. Water vapor advection and the subsequent formation of clouds quite differ when we compare these brand new high resolution simulations and the usual lower resolution ones at 64 per 48 grid points. Conference Object Ice cap École Polytechnique, Université Paris-Saclay: HAL |
institution |
Open Polar |
collection |
École Polytechnique, Université Paris-Saclay: HAL |
op_collection_id |
ftepunivpsaclay |
language |
English |
topic |
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] |
spellingShingle |
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] Pottier, Alizée Montmessin, Franck Forget, François Navarro, Thomas Millour, Ehouarn Madeleine, Jean-Baptiste Spiga, Aymeric A high resolution study of the Martian water cycle with a global climate model |
topic_facet |
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] |
description |
International audience The martian water cycle's main source is the northern polar cap. Running high resolution models, up to 360° per 180°, help better resolve this ice cap, and better mimic the gradual retreat of the seasonal cap. Atmospheric circulation is also better resolved. Water vapor advection and the subsequent formation of clouds quite differ when we compare these brand new high resolution simulations and the usual lower resolution ones at 64 per 48 grid points. |
author2 |
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) Laboratoire de Météorologie Dynamique (UMR 8539) (LMD) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL) |
format |
Conference Object |
author |
Pottier, Alizée Montmessin, Franck Forget, François Navarro, Thomas Millour, Ehouarn Madeleine, Jean-Baptiste Spiga, Aymeric |
author_facet |
Pottier, Alizée Montmessin, Franck Forget, François Navarro, Thomas Millour, Ehouarn Madeleine, Jean-Baptiste Spiga, Aymeric |
author_sort |
Pottier, Alizée |
title |
A high resolution study of the Martian water cycle with a global climate model |
title_short |
A high resolution study of the Martian water cycle with a global climate model |
title_full |
A high resolution study of the Martian water cycle with a global climate model |
title_fullStr |
A high resolution study of the Martian water cycle with a global climate model |
title_full_unstemmed |
A high resolution study of the Martian water cycle with a global climate model |
title_sort |
high resolution study of the martian water cycle with a global climate model |
publisher |
HAL CCSD |
publishDate |
2015 |
url |
https://insu.hal.science/insu-01217131 https://insu.hal.science/insu-01217131/document https://insu.hal.science/insu-01217131/file/EPSC2015-215.pdf |
op_coverage |
Nantes, France |
genre |
Ice cap |
genre_facet |
Ice cap |
op_source |
European Planetary Science Congress 2015, 27 September – 02 October 2015, La Cité des Congrès, Nantes, France European Planetary Science Congress 2015 https://insu.hal.science/insu-01217131 European Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-215 |
op_relation |
insu-01217131 https://insu.hal.science/insu-01217131 https://insu.hal.science/insu-01217131/document https://insu.hal.science/insu-01217131/file/EPSC2015-215.pdf |
op_rights |
info:eu-repo/semantics/OpenAccess |
_version_ |
1801376649044819968 |