A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations

We describe a huge planetary-scale disturbance in the highest-speed Jovian jet at latitude 23.5°N that was first observed in October 2016 during the Juno perijove-2 approach. An extraordinary outburst of four plumes was involved in the disturbance development. They were located in the range of plane...

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Autores: Sanchez-Lavega, Agustin, Rogers, John H, Orton, Glenn, García Melendo, Enrique José|||0000-0002-3354-1140, Legarreta, Jon, Colas, Françoise, Dauvergne, J, Hueso, Ricardo, Rojas, Jose Félix, Perez-Hoyos, Santiago, Mendikoa, Iñigo, Iñurrigarro, P, Gómez-Forrellad, Josep M., Momary, T, Hansen, C. J., Eichstaedt, G., Miles, P, Wesley, A
Tipo de recurso: artículo
Fecha de publicación:2017
País:España
Institución:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/111256
Acceso en línea:https://hdl.handle.net/2117/111256
https://dx.doi.org/10.1002/2017GL073421
Access Level:acceso abierto
Palabra clave:Planets
Jupiter (Planet)
JUPITER’S NTB JET DISTURBANCE
Planetes
Júpiter (Planeta)
Àrees temàtiques de la UPC::Física
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repository_id_str
spelling A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observationsSanchez-Lavega, AgustinRogers, John HOrton, GlennGarcía Melendo, Enrique José|||0000-0002-3354-1140Legarreta, JonColas, FrançoiseDauvergne, JHueso, RicardoRojas, Jose FélixPerez-Hoyos, SantiagoMendikoa, IñigoIñurrigarro, PGómez-Forrellad, Josep M.Momary, THansen, C. J.Eichstaedt, G.Miles, PWesley, APlanetsJupiter (Planet)JUPITER’S NTB JET DISTURBANCEPlanetesJúpiter (Planeta)Àrees temàtiques de la UPC::FísicaWe describe a huge planetary-scale disturbance in the highest-speed Jovian jet at latitude 23.5°N that was first observed in October 2016 during the Juno perijove-2 approach. An extraordinary outburst of four plumes was involved in the disturbance development. They were located in the range of planetographic latitudes from 22.2° to 23.0°N and moved faster than the jet peak with eastward velocities in the range 155 to 175 m s 1. In the wake of the plumes, a turbulent pattern of bright and dark spots (wave number 20–25) formed and progressed during October and November on both sides of the jet, moving with speeds in the range 100–125 m s 1 and leading to a new reddish and homogeneous belt when activity ceased in late November. Nonlinear numerical models reproduce the disturbance cloud patterns as a result of the interaction between local sources (the plumes) and the zonal eastward jet.Peer Reviewed20172017-05-2520172017-11-27journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/2117/111256https://dx.doi.org/10.1002/2017GL073421reponame:UPCommons. Portal del coneixement obert de la UPCinstname:Universitat Politècnica de Catalunya (UPC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution-NonCommercial-NoDerivs 3.0 Spainhttp://creativecommons.org/licenses/by-nc-nd/3.0/es/info:eu-repo/semantics/openAccessoai:upcommons.upc.edu:2117/1112562026-05-27T15:37:01Z
dc.title.none.fl_str_mv A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
title A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
spellingShingle A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
Sanchez-Lavega, Agustin
Planets
Jupiter (Planet)
JUPITER’S NTB JET DISTURBANCE
Planetes
Júpiter (Planeta)
Àrees temàtiques de la UPC::Física
title_short A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
title_full A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
title_fullStr A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
title_full_unstemmed A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
title_sort A planetary-scale disturbance in the most intense Jovian atmospheric jet from JunoCam and ground-based observations
dc.creator.none.fl_str_mv Sanchez-Lavega, Agustin
Rogers, John H
Orton, Glenn
García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon
Colas, Françoise
Dauvergne, J
Hueso, Ricardo
Rojas, Jose Félix
Perez-Hoyos, Santiago
Mendikoa, Iñigo
Iñurrigarro, P
Gómez-Forrellad, Josep M.
Momary, T
Hansen, C. J.
Eichstaedt, G.
Miles, P
Wesley, A
author Sanchez-Lavega, Agustin
author_facet Sanchez-Lavega, Agustin
Rogers, John H
Orton, Glenn
García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon
Colas, Françoise
Dauvergne, J
Hueso, Ricardo
Rojas, Jose Félix
Perez-Hoyos, Santiago
Mendikoa, Iñigo
Iñurrigarro, P
Gómez-Forrellad, Josep M.
Momary, T
Hansen, C. J.
Eichstaedt, G.
Miles, P
Wesley, A
author_role author
author2 Rogers, John H
Orton, Glenn
García Melendo, Enrique José|||0000-0002-3354-1140
Legarreta, Jon
Colas, Françoise
Dauvergne, J
Hueso, Ricardo
Rojas, Jose Félix
Perez-Hoyos, Santiago
Mendikoa, Iñigo
Iñurrigarro, P
Gómez-Forrellad, Josep M.
Momary, T
Hansen, C. J.
Eichstaedt, G.
Miles, P
Wesley, A
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Planets
Jupiter (Planet)
JUPITER’S NTB JET DISTURBANCE
Planetes
Júpiter (Planeta)
Àrees temàtiques de la UPC::Física
topic Planets
Jupiter (Planet)
JUPITER’S NTB JET DISTURBANCE
Planetes
Júpiter (Planeta)
Àrees temàtiques de la UPC::Física
description We describe a huge planetary-scale disturbance in the highest-speed Jovian jet at latitude 23.5°N that was first observed in October 2016 during the Juno perijove-2 approach. An extraordinary outburst of four plumes was involved in the disturbance development. They were located in the range of planetographic latitudes from 22.2° to 23.0°N and moved faster than the jet peak with eastward velocities in the range 155 to 175 m s 1. In the wake of the plumes, a turbulent pattern of bright and dark spots (wave number 20–25) formed and progressed during October and November on both sides of the jet, moving with speeds in the range 100–125 m s 1 and leading to a new reddish and homogeneous belt when activity ceased in late November. Nonlinear numerical models reproduce the disturbance cloud patterns as a result of the interaction between local sources (the plumes) and the zonal eastward jet.
publishDate 2017
dc.date.none.fl_str_mv 2017
2017-05-25
2017
2017-11-27
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/2117/111256
https://dx.doi.org/10.1002/2017GL073421
url https://hdl.handle.net/2117/111256
https://dx.doi.org/10.1002/2017GL073421
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:UPCommons. Portal del coneixement obert de la UPC
instname:Universitat Politècnica de Catalunya (UPC)
instname_str Universitat Politècnica de Catalunya (UPC)
reponame_str UPCommons. Portal del coneixement obert de la UPC
collection UPCommons. Portal del coneixement obert de la UPC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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