Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD

Observations of water ice clouds and aerosols on Mars can provide important insights into the complexity of the water cycle. Recent observations have indicated an important link between dust activity and the water cycle, as intense dust activity can significantly raise the hygropause, and subsequent...

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Autores: Liuzzi, Giuliano, Villanueva, Geronimo L., Crismani, Matteo M. J., Smith, Michael D., Mumma, Michael J., Daerden, Frank, Aoki, Shohei, Vandaele, Ann Carine, Clancy, R. Todd, Erwin, Justin T., Thomas, Ian R., Ristic, Bojan, López-Moreno, José Juan, Bellucci, Giancarlo, Patel, Manish R.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/211779
Acceso en línea:http://hdl.handle.net/10261/211779
Access Level:acceso abierto
Palabra clave:Mars atmosphere
Water ice mesospheric clouds
NOMAD ExoMars
Global dust storm
Retrieval
Cloud formation on Mars
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network_name_str España
repository_id_str
dc.title.none.fl_str_mv Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
title Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
spellingShingle Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
Liuzzi, Giuliano
Mars atmosphere
Water ice mesospheric clouds
NOMAD ExoMars
Global dust storm
Retrieval
Cloud formation on Mars
title_short Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
title_full Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
title_fullStr Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
title_full_unstemmed Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
title_sort Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMAD
dc.creator.none.fl_str_mv Liuzzi, Giuliano
Villanueva, Geronimo L.
Crismani, Matteo M. J.
Smith, Michael D.
Mumma, Michael J.
Daerden, Frank
Aoki, Shohei
Vandaele, Ann Carine
Clancy, R. Todd
Erwin, Justin T.
Thomas, Ian R.
Ristic, Bojan
López-Moreno, José Juan
Bellucci, Giancarlo
Patel, Manish R.
author Liuzzi, Giuliano
author_facet Liuzzi, Giuliano
Villanueva, Geronimo L.
Crismani, Matteo M. J.
Smith, Michael D.
Mumma, Michael J.
Daerden, Frank
Aoki, Shohei
Vandaele, Ann Carine
Clancy, R. Todd
Erwin, Justin T.
Thomas, Ian R.
Ristic, Bojan
López-Moreno, José Juan
Bellucci, Giancarlo
Patel, Manish R.
author_role author
author2 Villanueva, Geronimo L.
Crismani, Matteo M. J.
Smith, Michael D.
Mumma, Michael J.
Daerden, Frank
Aoki, Shohei
Vandaele, Ann Carine
Clancy, R. Todd
Erwin, Justin T.
Thomas, Ian R.
Ristic, Bojan
López-Moreno, José Juan
Bellucci, Giancarlo
Patel, Manish R.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Belgian Science Policy Office
European Space Agency
Ministerio de Ciencia e Innovación (España)
European Commission
UK Space Agency
Agenzia Spaziale Italiana
Ministerio de Ciencia, Innovación y Universidades (España)
NASA
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Mars atmosphere
Water ice mesospheric clouds
NOMAD ExoMars
Global dust storm
Retrieval
Cloud formation on Mars
topic Mars atmosphere
Water ice mesospheric clouds
NOMAD ExoMars
Global dust storm
Retrieval
Cloud formation on Mars
description Observations of water ice clouds and aerosols on Mars can provide important insights into the complexity of the water cycle. Recent observations have indicated an important link between dust activity and the water cycle, as intense dust activity can significantly raise the hygropause, and subsequently increase the escape of water after dissociation in the upper atmosphere. Here present observations from Nadir and Occultation for MArs Discovery/Trace Gas Orbiter that investigate the variation of water ice clouds in the perihelion season of Mars year 34 (April 2018-2019), their diurnal and seasonal behavior, and the vertical structure and microphysical properties of water ice and dust. These observations reveal the recurrent presence of a layer of mesospheric water ice clouds subsequent to the 2018 global dust storm. We show that this layer rose from 45 to 80 km in altitude on a time scale of days from heating in the lower atmosphere due to the storm. In addition, we demonstrate that there is a strong dawn-dusk asymmetry in water ice abundance, related to nighttime nucleation and subsequent daytime sublimation. Water ice particle sizes are retrieved consistently and exhibit sharp vertical gradients (from 0.1 to 4.0 mu m), as well as mesospheric differences between the global dust storm (<0.5 mu m) and the 2019 regional dust storm (1.0 mu m), which suggests differing water ice nucleation efficiencies. These results form the basis to advance our understanding of mesospheric water ice clouds on Mars, and further constrain the interactions between water ice and dust in the middle atmosphere. © 2020 American Geophysical Union
publishDate 2020
dc.date.none.fl_str_mv 2020
2020
2020
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/211779
url http://hdl.handle.net/10261/211779
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
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#PLACEHOLDER_PARENT_METADATA_VALUE#
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info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-101836-B-100
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/ESP2017-87143-R
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/SEV-2017-0709
http://dx.doi.org/10.1029/2019JE006250

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
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spelling Strong Variability of Martian Water Ice Clouds During Dust Storms Revealed From ExoMars Trace Gas Orbiter/NOMADLiuzzi, GiulianoVillanueva, Geronimo L.Crismani, Matteo M. J.Smith, Michael D.Mumma, Michael J.Daerden, FrankAoki, ShoheiVandaele, Ann CarineClancy, R. ToddErwin, Justin T.Thomas, Ian R.Ristic, BojanLópez-Moreno, José JuanBellucci, GiancarloPatel, Manish R.Mars atmosphereWater ice mesospheric cloudsNOMAD ExoMarsGlobal dust stormRetrievalCloud formation on MarsObservations of water ice clouds and aerosols on Mars can provide important insights into the complexity of the water cycle. Recent observations have indicated an important link between dust activity and the water cycle, as intense dust activity can significantly raise the hygropause, and subsequently increase the escape of water after dissociation in the upper atmosphere. Here present observations from Nadir and Occultation for MArs Discovery/Trace Gas Orbiter that investigate the variation of water ice clouds in the perihelion season of Mars year 34 (April 2018-2019), their diurnal and seasonal behavior, and the vertical structure and microphysical properties of water ice and dust. These observations reveal the recurrent presence of a layer of mesospheric water ice clouds subsequent to the 2018 global dust storm. We show that this layer rose from 45 to 80 km in altitude on a time scale of days from heating in the lower atmosphere due to the storm. In addition, we demonstrate that there is a strong dawn-dusk asymmetry in water ice abundance, related to nighttime nucleation and subsequent daytime sublimation. Water ice particle sizes are retrieved consistently and exhibit sharp vertical gradients (from 0.1 to 4.0 mu m), as well as mesospheric differences between the global dust storm (<0.5 mu m) and the 2019 regional dust storm (1.0 mu m), which suggests differing water ice nucleation efficiencies. These results form the basis to advance our understanding of mesospheric water ice clouds on Mars, and further constrain the interactions between water ice and dust in the middle atmosphere. © 2020 American Geophysical UnionExoMars is a space mission of the European Space Agency (ESA) and Roscosmos. The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB-BIRA), assisted by Co-PI teams from Spain (IAA-CSIC), Italy (INAF-IAPS), and the United Kingdom (Open University). This project acknowledges funding by the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401, 4000121493), by the Spanish MICINN through its Plan Nacional and by European funds under grants PGC2018-101836-B-I00 and ESP2017-87143-R (MINECO/FEDER), and by UK Space Agency through grants ST/R005761/1, ST/P001262/1, ST/R001405/1, and ST/S00145X/1 and Italian Space Agency through grant 2018-2-HH.0. The IAA/CSIC team acknowledges financial support from the State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award for the Instituto de Astrofisica de Andalucia (SEV-2017-0709). This work was supported by NASA's Mars Program Office under WBS 604796, "Participation in the TGO/NOMAD Investigation of Trace Gases on Mars" and by NASA's SEEC initiative under grant NNX17AH81A, "Remote sensing of Planetary Atmospheres in the Solar System and Beyond." M.C. is supported by the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Universities Space Research Association (USRA) under contract with NASA. The retrieval package used in this study is the Planetary Spectrum Generator, free and available online at https://psg.gsfc.nasa.gov/helpatm.php#retrieval, at the PSG GitHub site: https://github.com/nasapsg/retrievalOE, and on Zenodo (Liuzzi, 2020a). The database with the retrieved values is available of the PSG Exomars server at https://psg.gsfc.nasa.gov/apps/exomars.php and on Zenodo (Liuzzi, 2020b). The data used in this analysis are available at https://nomad.aeronomie.be/index.php/data.Peer reviewedAmerican Geophysical UnionBelgian Science Policy OfficeEuropean Space AgencyMinisterio de Ciencia e Innovación (España)European CommissionUK Space AgencyAgenzia Spaziale ItalianaMinisterio de Ciencia, Innovación y Universidades (España)NASAConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202020202020info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/211779reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-101836-B-100info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/ESP2017-87143-Rinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/SEV-2017-0709http://dx.doi.org/10.1029/2019JE006250Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2117792026-05-22T06:33:51Z
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