Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations
International audience The Martian polar night distribution of 1.27 μm (0-0) band emission from O 2 singlet delta [O 2 ( 1 Δ g )] is determined from an extensive set of Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectral Mapping (CRISM) limb scans observed over a wide range of...
Published in: | Journal of Geophysical Research: Planets |
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Main Authors: | , , , , , , , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2012
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Online Access: | https://hal.science/hal-00716395 https://hal.science/hal-00716395/document https://hal.science/hal-00716395/file/2011JE004018.pdf https://doi.org/10.1029/2011JE004018 |
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ftsorbonneuniv:oai:HAL:hal-00716395v1 |
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record_format |
openpolar |
institution |
Open Polar |
collection |
HAL Sorbonne Université |
op_collection_id |
ftsorbonneuniv |
language |
English |
topic |
Singlet delta Mars Photochemistry Atmosphere Polar O 2 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] |
spellingShingle |
Singlet delta Mars Photochemistry Atmosphere Polar O 2 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] Clancy, R. Todd Sandor, Brad J. Wolff, Michael J. Smith, Michael D. Lefèvre, Franck Madeleine, Jean-Baptiste Forget, François Murchie, Scott L. Seelos, Frank Seelos, Kim D. Nair, Hari A. Toigo, Anthony D. Humm, David Kass, David M. Kleinböhl, Armin Heavens, Nicholas Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
topic_facet |
Singlet delta Mars Photochemistry Atmosphere Polar O 2 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] |
description |
International audience The Martian polar night distribution of 1.27 μm (0-0) band emission from O 2 singlet delta [O 2 ( 1 Δ g )] is determined from an extensive set of Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectral Mapping (CRISM) limb scans observed over a wide range of Mars seasons, high latitudes, local times, and longitudes between 2009 and 2011. This polar nightglow reflects meridional transport and winter polar descent of atomic oxygen produced from CO 2 photodissociation. A distinct peak in 1.27 μm nightglow appears prominently over 70-90NS latitudes at 40-60 km altitudes, as retrieved for over 100 vertical profiles of O 2 ( 1 Δ g ) 1.27 μm volume emission rates (VER). We also present the first detection of much (x80±20) weaker 1.58 μm (0-1) band emission from Mars O 2 ( 1 Δ g ). Co-located polar night CRISM O 2 ( 1 Δ g ) and Mars Climate Sounder (MCS, McCleese et al, 2007) temperature profiles are compared to the same profiles as simulated by the Laboratoire de Meteorologie Dynamique (LMD) general circulation/photochemical model (e.g., Lefevre et al, 2004). Both standard and interactive aerosol LMD simulations (Madeleine et al, 2011) underproduce CRISM O 2 ( 1 Δ g ) total emission rates by 40%, due to inadequate transport of atomic oxygen to the winter polar emission regions. Incorporation of interactive cloud radiative forcing on the global circulation leads to distinct but insufficient improvements in modeled polar O 2 ( 1 Δ g ) and temperatures. The observed and modeled anti-correlations between temperatures and 1.27 μm band VER reflect the temperature dependence of the rate coefficient for O 2 ( 1 Δ g ) formation, as provided in Roble (1995). |
author2 |
Space Science Institute Boulder (SSI) NASA Goddard Space Flight Center (GSFC) 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 Pierre-Simon-Laplace (IPSL) École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-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 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) Université Pierre et Marie Curie - Paris 6 (UPMC) Johns Hopkins University Applied Physics Laboratory Laurel, MD (APL) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) |
format |
Article in Journal/Newspaper |
author |
Clancy, R. Todd Sandor, Brad J. Wolff, Michael J. Smith, Michael D. Lefèvre, Franck Madeleine, Jean-Baptiste Forget, François Murchie, Scott L. Seelos, Frank Seelos, Kim D. Nair, Hari A. Toigo, Anthony D. Humm, David Kass, David M. Kleinböhl, Armin Heavens, Nicholas |
author_facet |
Clancy, R. Todd Sandor, Brad J. Wolff, Michael J. Smith, Michael D. Lefèvre, Franck Madeleine, Jean-Baptiste Forget, François Murchie, Scott L. Seelos, Frank Seelos, Kim D. Nair, Hari A. Toigo, Anthony D. Humm, David Kass, David M. Kleinböhl, Armin Heavens, Nicholas |
author_sort |
Clancy, R. Todd |
title |
Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
title_short |
Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
title_full |
Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
title_fullStr |
Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
title_full_unstemmed |
Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations |
title_sort |
extensive mro crism observations of 1.27 μm o 2 airglow in mars polar night and their comparison to mro mcs temperature profiles and lmd gcm simulations |
publisher |
HAL CCSD |
publishDate |
2012 |
url |
https://hal.science/hal-00716395 https://hal.science/hal-00716395/document https://hal.science/hal-00716395/file/2011JE004018.pdf https://doi.org/10.1029/2011JE004018 |
genre |
polar night |
genre_facet |
polar night |
op_source |
ISSN: 2169-9097 EISSN: 2169-9100 Journal of Geophysical Research. Planets https://hal.science/hal-00716395 Journal of Geophysical Research. Planets, 2012, 117, pp.E00J10. ⟨10.1029/2011JE004018⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1029/2011JE004018 hal-00716395 https://hal.science/hal-00716395 https://hal.science/hal-00716395/document https://hal.science/hal-00716395/file/2011JE004018.pdf BIBCODE: 2012JGRE.11700J10C doi:10.1029/2011JE004018 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1029/2011JE004018 |
container_title |
Journal of Geophysical Research: Planets |
container_volume |
117 |
container_issue |
E11 |
container_start_page |
n/a |
op_container_end_page |
n/a |
_version_ |
1801381392275210240 |
spelling |
ftsorbonneuniv:oai:HAL:hal-00716395v1 2024-06-09T07:49:09+00:00 Extensive MRO CRISM observations of 1.27 μm O 2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations Clancy, R. Todd Sandor, Brad J. Wolff, Michael J. Smith, Michael D. Lefèvre, Franck Madeleine, Jean-Baptiste Forget, François Murchie, Scott L. Seelos, Frank Seelos, Kim D. Nair, Hari A. Toigo, Anthony D. Humm, David Kass, David M. Kleinböhl, Armin Heavens, Nicholas Space Science Institute Boulder (SSI) NASA Goddard Space Flight Center (GSFC) 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 Pierre-Simon-Laplace (IPSL) École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales Toulouse (CNES)-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 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) Université Pierre et Marie Curie - Paris 6 (UPMC) Johns Hopkins University Applied Physics Laboratory Laurel, MD (APL) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) 2012 https://hal.science/hal-00716395 https://hal.science/hal-00716395/document https://hal.science/hal-00716395/file/2011JE004018.pdf https://doi.org/10.1029/2011JE004018 en eng HAL CCSD Wiley-Blackwell info:eu-repo/semantics/altIdentifier/doi/10.1029/2011JE004018 hal-00716395 https://hal.science/hal-00716395 https://hal.science/hal-00716395/document https://hal.science/hal-00716395/file/2011JE004018.pdf BIBCODE: 2012JGRE.11700J10C doi:10.1029/2011JE004018 info:eu-repo/semantics/OpenAccess ISSN: 2169-9097 EISSN: 2169-9100 Journal of Geophysical Research. Planets https://hal.science/hal-00716395 Journal of Geophysical Research. Planets, 2012, 117, pp.E00J10. ⟨10.1029/2011JE004018⟩ Singlet delta Mars Photochemistry Atmosphere Polar O 2 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] info:eu-repo/semantics/article Journal articles 2012 ftsorbonneuniv https://doi.org/10.1029/2011JE004018 2024-05-16T23:56:30Z International audience The Martian polar night distribution of 1.27 μm (0-0) band emission from O 2 singlet delta [O 2 ( 1 Δ g )] is determined from an extensive set of Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectral Mapping (CRISM) limb scans observed over a wide range of Mars seasons, high latitudes, local times, and longitudes between 2009 and 2011. This polar nightglow reflects meridional transport and winter polar descent of atomic oxygen produced from CO 2 photodissociation. A distinct peak in 1.27 μm nightglow appears prominently over 70-90NS latitudes at 40-60 km altitudes, as retrieved for over 100 vertical profiles of O 2 ( 1 Δ g ) 1.27 μm volume emission rates (VER). We also present the first detection of much (x80±20) weaker 1.58 μm (0-1) band emission from Mars O 2 ( 1 Δ g ). Co-located polar night CRISM O 2 ( 1 Δ g ) and Mars Climate Sounder (MCS, McCleese et al, 2007) temperature profiles are compared to the same profiles as simulated by the Laboratoire de Meteorologie Dynamique (LMD) general circulation/photochemical model (e.g., Lefevre et al, 2004). Both standard and interactive aerosol LMD simulations (Madeleine et al, 2011) underproduce CRISM O 2 ( 1 Δ g ) total emission rates by 40%, due to inadequate transport of atomic oxygen to the winter polar emission regions. Incorporation of interactive cloud radiative forcing on the global circulation leads to distinct but insufficient improvements in modeled polar O 2 ( 1 Δ g ) and temperatures. The observed and modeled anti-correlations between temperatures and 1.27 μm band VER reflect the temperature dependence of the rate coefficient for O 2 ( 1 Δ g ) formation, as provided in Roble (1995). Article in Journal/Newspaper polar night HAL Sorbonne Université Journal of Geophysical Research: Planets 117 E11 n/a n/a |