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dc.contributor.authorSánchez Lavega, Agustín María ORCID
dc.contributor.authorDel Río Gaztelurrutia, María Teresa
dc.contributor.authorHueso Alonso, Ricardo ORCID
dc.contributor.authorde la Torre Juárez, Manuel
dc.contributor.authorMartínez, Germán M.
dc.contributor.authorHarri, Ari Matti
dc.contributor.authorGenzer, Maria
dc.contributor.authorHieta, Maria
dc.contributor.authorPolkko, J.
dc.contributor.authorRodríguez Manfredi, José Antonio
dc.contributor.authorLemmon, Mark T.
dc.contributor.authorPlá García, Jorge
dc.contributor.authorToledo, Daniel
dc.contributor.authorVicente Retortillo, Álvaro
dc.contributor.authorViúdez Moreiras, Daniel
dc.contributor.authorMunguira Ruiz, Asier ORCID
dc.contributor.authorTamppari, Leslie
dc.contributor.authorNewman, Claire E.
dc.contributor.authorGómez Elvira, Javier
dc.contributor.authorGuzewich, Scott
dc.contributor.authorBertrand, Tanguy
dc.contributor.authorApestigue, Victor
dc.contributor.authorArruego, Ignacio
dc.contributor.authorWolff, Michael J.
dc.contributor.authorBanfield, Don
dc.contributor.authorJaakonaho, I.
dc.contributor.authorMakinen, T.
dc.date.accessioned2023-05-15T16:26:06Z
dc.date.available2023-05-15T16:26:06Z
dc.date.issued2023-01
dc.identifier.citationJGR Planets 128(1) : (2023) // Article ID e2022JE007480es_ES
dc.identifier.issn2169-9097
dc.identifier.urihttp://hdl.handle.net/10810/61119
dc.description.abstractThe pressure sensors on Mars rover Perseverance measure the pressure field in the Jezero crater on regular hourly basis starting in sol 15 after landing. The present study extends up to sol 460 encompassing the range of solar longitudes from Ls ∼ 13°–241° (Martian Year (MY) 36). The data show the changing daily pressure cycle, the sol-to-sol seasonal evolution of the mean pressure field driven by the CO2 sublimation and deposition cycle at the poles, the characterization of up to six components of the atmospheric tides and their relationship to dust content in the atmosphere. They also show the presence of wave disturbances with periods 2–5 sols, exploring their baroclinic nature, short period oscillations (mainly at night-time) in the range 8–24 min that we interpret as internal gravity waves, transient pressure drops with duration ∼1–150 s produced by vortices, and rapid turbulent fluctuations. We also analyze the effects on pressure measurements produced by a regional dust storm over Jezero at Ls ∼ 155°.es_ES
dc.description.sponsorshipThe UPV/EHU team (Spain) is supported by Grant PID2019-109467GB-I00 funded by 1042 MCIN/AEI/10.13039/501100011033/ and by Groups Gobierno Vasco IT1742-22. GM wants to acknowledge JPL funding from USRA Contract Number 1638782. A. Vicente-Retortillo is supported by the Spanish State Research Agency (AEI) Project No. MDM-2017-0737 Unidad de Excelencia “María de Maeztu”- Centro de Astrobiología (INTA-CSIC). Part of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). GM wants to acknowledge JPL funding from USRA Contract Number 1638782.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relationinfo:eu-repo/grantAgreement/MICINN/PID2019-109467GB-I00es_ES
dc.relationinfo:eu-repo/grantAgreement/MICIU/MDM-2017-0737es_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc/3.0/es/*
dc.subjectM2020 Perseverancees_ES
dc.subjectMars atmospherees_ES
dc.subjectpressure measurementses_ES
dc.titleMars 2020 Perseverance Rover Studies of the Martian Atmosphere Over Jezero From Pressure Measurementses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holder© 2022 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.es_ES
dc.rights.holderAtribución-NoComercial 3.0 España*
dc.relation.publisherversionhttps://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022JE007480es_ES
dc.identifier.doi10.1029/2022JE007480
dc.departamentoesFísica aplicada Ies_ES
dc.departamentoeuFisika aplikatua Ies_ES


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© 2022 The Authors.

This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.
Except where otherwise noted, this item's license is described as © 2022 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.