Ozone Detector Based on Ultraviolet Observations on the Martian Surface
Ozone plays a key role in both atmospheric chemistry and UV absorption in planetary atmospheres. On Mars, upper-tropospheric ozone has been widely characterized by space-based instruments. However, surface ozone remains poorly characterized, hindered by the limited sensitivity of orbiters to the low...
| Autores: | , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/370800 |
| Acceso en línea: | http://hdl.handle.net/10261/370800 |
| Access Level: | acceso abierto |
| Palabra clave: | Mars atmosphere Ozone observations Atmospheric chemistry Remote sensing |
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Ozone Detector Based on Ultraviolet Observations on the Martian SurfaceViúdez-Moreiras, DanielSaiz-Lopez, A.Smith, Michael D.Apestigue, VíctorArruego, IgnacioGarcía, ElisaJiménez, Juan J.Rodríguez-Manfredi, José AntonioToledo, DanielWolff, MikeZorzano, María PazMars atmosphereOzone observationsAtmospheric chemistryRemote sensingOzone plays a key role in both atmospheric chemistry and UV absorption in planetary atmospheres. On Mars, upper-tropospheric ozone has been widely characterized by space-based instruments. However, surface ozone remains poorly characterized, hindered by the limited sensitivity of orbiters to the lowest scale height of the atmosphere and challenges in delivering payloads to the surface of Mars, which have prevented, to date, the measurement of ozone from the surface of Mars. Systematic measurements from the Martian surface could advance our knowledge of the atmospheric chemistry and habitability potential of this planet. NASA’s Mars 2020 mission includes the first ozone detector deployed on the Martian surface, which is based on discrete photometric observations in the ultraviolet band, a simple technology that could obtain the first insights into total ozone abundance in preparation for more sophisticated measurement techniques. This paper describes the Mars 2020 ozone detector and its retrieval algorithm, including its performance under different sources of uncertainty and the potential application of the retrieval algorithm on other missions, such as NASA’s Mars Science Laboratory. Pre-landing simulations using the UVISMART radiative transfer model suggest that the retrieval is robust and that it can deal with common issues affecting surface operations in Martian missions, although the expected low ozone abundance and instrument uncertainties could challenge its characterization in tropical latitudes of the planet. Other space missions will potentially include sensors of similar technology.This work was partially funded by Spanish Ministry of Science and Innovation, under projects SOLAUT_00046032 and PID2021-126719OB-C41. The APC was funded by PID2021-126719OB-C41. V.A., I.A., E.G., J.J.J and D.T are supported by projects ESP2014-54256-C4-3-R, ESP2016-80320-C2-1-R and RTI2018-099825-B-C31.Peer reviewedMultidisciplinary Digital Publishing InstituteMinisterio de Ciencia e Innovación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/370800reponame: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##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI//SOLAUT_00046032info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-126719OB-C41info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-126719OB-C41info:eu-repo/grantAgreement/MINECO//ESP2014-54256-C4-3-Rinfo:eu-repo/grantAgreement/MINECO//ESP2016-80320-C2-1-Rinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/RTI2018-099825-B-C31The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI https://doi.org/10.3390/rs16203914Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3708002026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| title |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| spellingShingle |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface Viúdez-Moreiras, Daniel Mars atmosphere Ozone observations Atmospheric chemistry Remote sensing |
| title_short |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| title_full |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| title_fullStr |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| title_full_unstemmed |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| title_sort |
Ozone Detector Based on Ultraviolet Observations on the Martian Surface |
| dc.creator.none.fl_str_mv |
Viúdez-Moreiras, Daniel Saiz-Lopez, A. Smith, Michael D. Apestigue, Víctor Arruego, Ignacio García, Elisa Jiménez, Juan J. Rodríguez-Manfredi, José Antonio Toledo, Daniel Wolff, Mike Zorzano, María Paz |
| author |
Viúdez-Moreiras, Daniel |
| author_facet |
Viúdez-Moreiras, Daniel Saiz-Lopez, A. Smith, Michael D. Apestigue, Víctor Arruego, Ignacio García, Elisa Jiménez, Juan J. Rodríguez-Manfredi, José Antonio Toledo, Daniel Wolff, Mike Zorzano, María Paz |
| author_role |
author |
| author2 |
Saiz-Lopez, A. Smith, Michael D. Apestigue, Víctor Arruego, Ignacio García, Elisa Jiménez, Juan J. Rodríguez-Manfredi, José Antonio Toledo, Daniel Wolff, Mike Zorzano, María Paz |
| author2_role |
author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Ministerio de Ciencia e Innovación (España) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Mars atmosphere Ozone observations Atmospheric chemistry Remote sensing |
| topic |
Mars atmosphere Ozone observations Atmospheric chemistry Remote sensing |
| description |
Ozone plays a key role in both atmospheric chemistry and UV absorption in planetary atmospheres. On Mars, upper-tropospheric ozone has been widely characterized by space-based instruments. However, surface ozone remains poorly characterized, hindered by the limited sensitivity of orbiters to the lowest scale height of the atmosphere and challenges in delivering payloads to the surface of Mars, which have prevented, to date, the measurement of ozone from the surface of Mars. Systematic measurements from the Martian surface could advance our knowledge of the atmospheric chemistry and habitability potential of this planet. NASA’s Mars 2020 mission includes the first ozone detector deployed on the Martian surface, which is based on discrete photometric observations in the ultraviolet band, a simple technology that could obtain the first insights into total ozone abundance in preparation for more sophisticated measurement techniques. This paper describes the Mars 2020 ozone detector and its retrieval algorithm, including its performance under different sources of uncertainty and the potential application of the retrieval algorithm on other missions, such as NASA’s Mars Science Laboratory. Pre-landing simulations using the UVISMART radiative transfer model suggest that the retrieval is robust and that it can deal with common issues affecting surface operations in Martian missions, although the expected low ozone abundance and instrument uncertainties could challenge its characterization in tropical latitudes of the planet. Other space missions will potentially include sensors of similar technology. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024 2024 2024 2024 |
| 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 |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/370800 |
| url |
http://hdl.handle.net/10261/370800 |
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Inglés |
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Inglés |
| dc.relation.none.fl_str_mv |
#PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# #PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/AEI//SOLAUT_00046032 info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-126719OB-C41 info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-126719OB-C41 info:eu-repo/grantAgreement/MINECO//ESP2014-54256-C4-3-R info:eu-repo/grantAgreement/MINECO//ESP2016-80320-C2-1-R info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/RTI2018-099825-B-C31 The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI https://doi.org/10.3390/rs16203914 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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Multidisciplinary Digital Publishing Institute |
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Multidisciplinary Digital Publishing Institute |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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