Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights

International audience Martian CO2 ice clouds are intriguing features, representing a rare occurrence of atmosphericcondensation of a major component. These clouds play a crucial role due to their radiative properties,interactions with surface, and coupling with microphysical cycles of aerosols. Obs...

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Published in:Geophysical Research Letters
Main Authors: Caillé, Vincent, Spiga, Aymeric, Määttänen, Anni, Falletti, Lola, Mathé, Christophe
Other Authors: Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-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), PLANETO - LATMOS, Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), ANR-18-CE31-0013,MECCOM,Modéliser des nuages exotiques de CO2 sur Mars(2018)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2024
Subjects:
Online Access:https://insu.hal.science/insu-04620042
https://insu.hal.science/insu-04620042/document
https://insu.hal.science/insu-04620042/file/GRL-%202024%20-%20Caille%CC%81%20-%20Resolving%20.pdf
https://doi.org/10.1029/2023gl106923
id ftecoleponts:oai:HAL:insu-04620042v1
record_format openpolar
institution Open Polar
collection École des Ponts ParisTech: HAL
op_collection_id ftecoleponts
language English
topic atmosphere
CO2 clouds
LES Modelization
Mars
platenology
[SDU]Sciences of the Universe [physics]
spellingShingle atmosphere
CO2 clouds
LES Modelization
Mars
platenology
[SDU]Sciences of the Universe [physics]
Caillé, Vincent
Spiga, Aymeric
Määttänen, Anni
Falletti, Lola
Mathé, Christophe
Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
topic_facet atmosphere
CO2 clouds
LES Modelization
Mars
platenology
[SDU]Sciences of the Universe [physics]
description International audience Martian CO2 ice clouds are intriguing features, representing a rare occurrence of atmosphericcondensation of a major component. These clouds play a crucial role due to their radiative properties,interactions with surface, and coupling with microphysical cycles of aerosols. Observations have been limited,prompting modeling studies to understand their formation and dynamics. Here, we present the first high‐resolution 3D simulations of CO2 ice clouds using a Large‐Eddy Simulation (LES) model incorporating CO2microphysics. We investigate cloud formation in idealized temperature perturbations in the polar night. Areference simulation with a 2K perturbation demonstrates that the formed CO2 ice cloud possesses aconvective potential, leading to its ascent in the troposphere. We determine the timescales and orders ofmagnitude of various phenomena involved in the lifecycle of a CO2 ice cloud. Sensitivity tests show thatconvection can be inhibited or intensified by the thermodynamic and microphysical conditions of the simulatedenvironment.
author2 Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Météorologie Dynamique (UMR 8539) (LMD)
Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)
Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-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)
PLANETO - LATMOS
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
ANR-18-CE31-0013,MECCOM,Modéliser des nuages exotiques de CO2 sur Mars(2018)
format Article in Journal/Newspaper
author Caillé, Vincent
Spiga, Aymeric
Määttänen, Anni
Falletti, Lola
Mathé, Christophe
author_facet Caillé, Vincent
Spiga, Aymeric
Määttänen, Anni
Falletti, Lola
Mathé, Christophe
author_sort Caillé, Vincent
title Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
title_short Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
title_full Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
title_fullStr Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
title_full_unstemmed Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights
title_sort resolving convection of co 2 ice clouds in the martian polar nights
publisher HAL CCSD
publishDate 2024
url https://insu.hal.science/insu-04620042
https://insu.hal.science/insu-04620042/document
https://insu.hal.science/insu-04620042/file/GRL-%202024%20-%20Caille%CC%81%20-%20Resolving%20.pdf
https://doi.org/10.1029/2023gl106923
genre polar night
genre_facet polar night
op_source ISSN: 0094-8276
EISSN: 1944-8007
Geophysical Research Letters
https://insu.hal.science/insu-04620042
Geophysical Research Letters, 2024, 51 (12), pp.e2023GL106923. ⟨10.1029/2023gl106923⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1029/2023gl106923
insu-04620042
https://insu.hal.science/insu-04620042
https://insu.hal.science/insu-04620042/document
https://insu.hal.science/insu-04620042/file/GRL-%202024%20-%20Caille%CC%81%20-%20Resolving%20.pdf
doi:10.1029/2023gl106923
op_rights http://creativecommons.org/licenses/by-nc-nd/
info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1029/2023gl106923
container_title Geophysical Research Letters
container_volume 51
container_issue 12
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spelling ftecoleponts:oai:HAL:insu-04620042v1 2024-09-15T18:31:18+00:00 Resolving Convection of CO 2 Ice Clouds in the Martian Polar Nights Caillé, Vincent Spiga, Aymeric Määttänen, Anni Falletti, Lola Mathé, Christophe Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de Météorologie Dynamique (UMR 8539) (LMD) Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X) Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-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) PLANETO - LATMOS Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) ANR-18-CE31-0013,MECCOM,Modéliser des nuages exotiques de CO2 sur Mars(2018) 2024-06-20 https://insu.hal.science/insu-04620042 https://insu.hal.science/insu-04620042/document https://insu.hal.science/insu-04620042/file/GRL-%202024%20-%20Caille%CC%81%20-%20Resolving%20.pdf https://doi.org/10.1029/2023gl106923 en eng HAL CCSD American Geophysical Union info:eu-repo/semantics/altIdentifier/doi/10.1029/2023gl106923 insu-04620042 https://insu.hal.science/insu-04620042 https://insu.hal.science/insu-04620042/document https://insu.hal.science/insu-04620042/file/GRL-%202024%20-%20Caille%CC%81%20-%20Resolving%20.pdf doi:10.1029/2023gl106923 http://creativecommons.org/licenses/by-nc-nd/ info:eu-repo/semantics/OpenAccess ISSN: 0094-8276 EISSN: 1944-8007 Geophysical Research Letters https://insu.hal.science/insu-04620042 Geophysical Research Letters, 2024, 51 (12), pp.e2023GL106923. ⟨10.1029/2023gl106923⟩ atmosphere CO2 clouds LES Modelization Mars platenology [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2024 ftecoleponts https://doi.org/10.1029/2023gl106923 2024-08-13T23:47:27Z International audience Martian CO2 ice clouds are intriguing features, representing a rare occurrence of atmosphericcondensation of a major component. These clouds play a crucial role due to their radiative properties,interactions with surface, and coupling with microphysical cycles of aerosols. Observations have been limited,prompting modeling studies to understand their formation and dynamics. Here, we present the first high‐resolution 3D simulations of CO2 ice clouds using a Large‐Eddy Simulation (LES) model incorporating CO2microphysics. We investigate cloud formation in idealized temperature perturbations in the polar night. Areference simulation with a 2K perturbation demonstrates that the formed CO2 ice cloud possesses aconvective potential, leading to its ascent in the troposphere. We determine the timescales and orders ofmagnitude of various phenomena involved in the lifecycle of a CO2 ice cloud. Sensitivity tests show thatconvection can be inhibited or intensified by the thermodynamic and microphysical conditions of the simulatedenvironment. Article in Journal/Newspaper polar night École des Ponts ParisTech: HAL Geophysical Research Letters 51 12