The Origin of Jupiter's Great Red Spot
dc.contributor.author | Sánchez Lavega, Agustín María | |
dc.contributor.author | García Melendo, Enrique José | |
dc.contributor.author | Legarreta Etxagibel, Jon Josu | |
dc.contributor.author | Miró, Arnau | |
dc.contributor.author | Soria, Manel | |
dc.contributor.author | Ahrens Velásquez, Kevin | |
dc.date.accessioned | 2024-08-05T11:51:07Z | |
dc.date.available | 2024-08-05T11:51:07Z | |
dc.date.issued | 2024-06 | |
dc.identifier.citation | Geophysical Research Letters 51(12) : (2024) // Article ID e2024GL108993 | es_ES |
dc.identifier.issn | 0094-8276 | |
dc.identifier.issn | 1944-8007 | |
dc.identifier.uri | http://hdl.handle.net/10810/69147 | |
dc.description.abstract | Jupiter's Great Red Spot (GRS) is the largest and longest-lived known vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude, known as the “Permanent Spot” (PS) that was observed until 1713. We show from historical observations of its size evolution and motions that PS is unlikely to correspond to the current GRS, that was first observed in 1831. Numerical simulations rule out that the GRS formed by the merging of vortices or by a superstorm, but most likely formed from a flow disturbance between the two opposed Jovian zonal jets north and south of it. If so, the early GRS should have had a low tangential velocity so that its rotation velocity has increased over time as it has shrunk. | es_ES |
dc.description.sponsorship | ASL and JL were supported by Grupos Gobierno Vasco IT1742-22 and by Grant PID2019-109467GB-I00 funded by MCIN/AEI/10.13039/501100011033/. EGM, AM, MS and KAV thankfully acknowledge the computer resources provided by Red Española de Supercomputación (RES) under the projects AECT-2020-1-0005 and RES-AECT-2021-2-0009. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | American Geophysical Union | es_ES |
dc.relation | info:eu-repo/grantAgreement/MICINN/PID2019-109467GB-I00 | es_ES |
dc.rights | info:eu-repo/semantics/openAccess | es_ES |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.title | The Origin of Jupiter's Great Red Spot | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.rights.holder | © 2024. The Author(s). This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made | es_ES |
dc.rights.holder | Atribución-NoComercial-SinDerivadas 3.0 España | * |
dc.relation.publisherversion | https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024GL108993 | es_ES |
dc.identifier.doi | 10.1029/2024GL108993 | |
dc.departamentoes | Física aplicada I | es_ES |
dc.departamentoes | Ingeniería de sistemas y automática | es_ES |
dc.departamentoeu | Fisika aplikatua I | es_ES |
dc.departamentoeu | Sistemen ingeniaritza eta automatika | es_ES |
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