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dc.contributor.authorSanchez-Lavega, Agustin
dc.contributor.authorGarcía Melendo, Enrique José
dc.contributor.authorPerez-Hoyos, Santiago
dc.contributor.authorHueso, Ricardo
dc.contributor.authorWong, Michael
dc.contributor.authorSimon, Amy A.
dc.contributor.authorSanz-Requena, Jose Francisco
dc.contributor.authorAntuñano, Arrate
dc.contributor.authorBarrado-Izaguirre, Naiara
dc.contributor.authorGarate-López, Itziar
dc.contributor.authorRojas, Jose Félix
dc.contributor.authordel Rio-Gaztelurrutia, Teresa
dc.contributor.authorGómez-Forrellad, Josep M.
dc.contributor.authorde Pater, Imke
dc.contributor.authorLi, Liming
dc.contributor.authorBarry, Trevor
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2017-11-29T14:37:33Z
dc.date.available2017-11-29T14:37:33Z
dc.date.issued2016-11-08
dc.identifier.citationSanchez-Lavega, A., Garcia-Melendo, E., Perez-Hoyos, S., Hueso, R., Wong, M., Simon, A., Sanz-Requena, J., Antuñano, A., Barrado-Izaguirre, N., Garate-López, I., Rojas, J., del Rio-Gaztelurrutia, T., Gómez-Forrellad, J., de Pater, I., Li, L., Barry, T. An enduring rapidly moving storm as a guide to Saturn's Equatorial jet's complex structure. "Nature communications", 8 Novembre 2016, p. 1-10.
dc.identifier.issn2041-1723
dc.identifier.urihttp://hdl.handle.net/2117/111337
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0
dc.description.abstractSaturn has an intense and broad eastward equatorial jet with a complex three-dimensional structure mixed with time variability. The equatorial region experiences strong seasonal insolation variations enhanced by ring shadowing, and three of the six known giant planetary-scale storms have developed in it. These factors make Saturn’s equator a natural laboratory to test models of jets in giant planets. Here we report on a bright equatorial atmospheric feature imaged in 2015 that moved steadily at a high speed of 450 ms-1 not measured since 1980–1981 with other equatorial clouds moving within an ample range of velocities. Radiative transfer models show that these motions occur at three altitude levels within the upper haze and clouds. We find that the peak of the jet (latitudes 10ºN to 10º S) suffers intense vertical shears reaching þ2.5 ms-1 km-1, two orders of magnitude higher than meridional shears, and temporal variability above 1 bar altitude level.
dc.format.extent10 p.
dc.language.isoeng
dc.rightsAttribution 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshAtmospheric physics
dc.subject.lcshSaturn (Planet)
dc.subject.otherAtmospheric dynamics
dc.subject.otherGiant planets
dc.titleAn enduring rapidly moving storm as a guide to Saturn's Equatorial jet's complex structure
dc.typeArticle
dc.subject.lemacFísica atmosfèrica
dc.subject.lemacMeteorologia dinàmica
dc.subject.lemacSaturn (Planeta)
dc.identifier.doi10.1038/ncomms13262
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://www.nature.com/articles/ncomms13262
dc.rights.accessOpen Access
local.identifier.drac21621828
dc.description.versionPostprint (published version)
local.citation.authorSanchez-Lavega, A.; Garcia-Melendo, E.; Perez-Hoyos, S.; Hueso, R.; Wong, M.; Simon, A.; Sanz-Requena, J.; Antuñano, A.; Barrado-Izaguirre, N.; Garate-López, I.; Rojas, J.; del Rio-Gaztelurrutia, T.; Gómez-Forrellad, J.; de Pater, I.; Li, L.; Barry, T.
local.citation.publicationNameNature communications
local.citation.startingPage1
local.citation.endingPage10


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Attribution 3.0 Spain
Except where otherwise noted, content on this work is licensed under a Creative Commons license : Attribution 3.0 Spain