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dc.contributor.authorHueso Alonso, Ricardo ORCID
dc.contributor.authorSánchez Lavega, Agustín María ORCID
dc.contributor.authorFouchet, Thierry
dc.contributor.authorde Pater, Imke
dc.contributor.authorAntuñano Martín, Arrate ORCID
dc.contributor.authorFletcher, Leigh N.
dc.contributor.authorWong, Michael H.
dc.contributor.authorRodríguez-Ovalle, Pablo
dc.contributor.authorSromovsky, Lawrence, A.
dc.contributor.authorFry, Patrick M.
dc.contributor.authorOrton, Glenn S. ORCID
dc.contributor.authorGuerlet, Sandrine
dc.contributor.authorIrwin, Patrick G.J.
dc.contributor.authorLellouch, Emmanuel
dc.contributor.authorHarkett, Jake
dc.contributor.authorde Kleer, Katherine
dc.contributor.authorMelin, Henrik
dc.contributor.authorHue, Vincent
dc.contributor.authorSimon, Amy A.
dc.contributor.authorLuszcz-Cook, Statia
dc.contributor.authorSayanagi, Kunio M.
dc.date.accessioned2023-11-14T18:29:41Z
dc.date.available2023-11-14T18:29:41Z
dc.date.issued2023-10-19
dc.identifier.citationNature Astronomy : (2023) // https://doi.org/10.1038/s41550-023-02099-2es_ES
dc.identifier.issn2397-3366
dc.identifier.urihttp://hdl.handle.net/10810/63020
dc.description.abstractThe atmosphere of Jupiter has east–west zonal jets that alternate as a function of latitude as tracked by cloud motions at tropospheric levels. Above and below the cold tropopause at ~100 mbar, the equatorial atmosphere is covered by hazes at levels where thermal infrared observations used to characterize the dynamics of the stratosphere lose part of their sensitivity. James Webb Space Telescope observations of Jupiter in July 2022 show these hazes in higher detail than ever before and reveal the presence of an intense (140 m s−1) equatorial jet at 100–200 mbar (70 m s−1 faster than the zonal winds at the cloud level) that is confined to ±3° of the equator and is located below stratospheric thermal oscillations that extend at least from 0.1 to 40 mbar and repeat in multiyear cycles. This suggests that the new jet is a deep part of Jupiter’s Equatorial Stratospheric Oscillation and may therefore vary in strength over time.es_ES
dc.description.sponsorshipJWST-ERS-01373, NASA/ESA Hubble Space Telescope programmes no. 16913, 15502 and 16790, PID2019-109467GB-I00 funded by MCIN/AEI/10.13039/501100011033/, Grupos Gobierno Vasco IT1742-22. I.d.; European Research Council Consolidator Grant (under the European Union’s Horizon 2020 research and innovation programme, grant agreement no. 723890), STFC PhD Studentship, NASA grants 80NSSC21K1418 and 80NSSC19K0894.es_ES
dc.language.isoenges_ES
dc.publisherSpringer Naturees_ES
dc.relationinfo:eu-repo/grantAgreement/EC/H2020/723890es_ES
dc.relationinfo:eu-repo/grantAgreement/MCIN/PID2019-109467GB-I00es_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectJupiteres_ES
dc.subjectequatorial dynamicses_ES
dc.subjectJWSTes_ES
dc.titleAn intense narrow equatorial jet in Jupiter’s lower stratosphere observed by JWSTes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holder(cc) 2023 This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.es_ES
dc.relation.publisherversionhttps://www.nature.com/articles/s41550-023-02099-2es_ES
dc.identifier.doi10.1038/s41550-023-02099-2
dc.contributor.funderEuropean Commission
dc.departamentoesFísica aplicada Ies_ES
dc.departamentoeuFisika aplikatua Ies_ES


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(cc) 2023 This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
Except where otherwise noted, this item's license is described as (cc) 2023 This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.