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...
| Autores: | , , , , , , , , , , , , , , |
|---|---|
| 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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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 |
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article |
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publishedVersion |
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http://hdl.handle.net/10261/211779 |
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http://hdl.handle.net/10261/211779 |
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Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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American Geophysical Union |
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American Geophysical Union |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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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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