Titan's influence on Saturnian substorm occurrence

Autores
Russell, C. T.; Jackman, C. M.; Wei, H. Y.; Bertucci, Cesar; Dougherty, M. K.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Substorms play an important role in the energization and transport of plasmas in planetary magnetospheres, including the shedding of the mass added by moons in the case of Jupiter and Saturn. Mass shedding occurs through rapid reconnection in the near tail resulting in dipolarization on the magnetospheric side of the reconnection point and plasmoid formation down tail. Observations of these sudden reconnection events in Saturn’s near-tail region provide additional insight into this process. Saturnian substorms, at least on occasion, have a plasmoid formation phase leading to a traveling compression region. Changes in the field strength across reconnection events suggest that open flux has been removed from the tail. The timing of tail reconnection events appears to be controlled by both the orbital phase of Titan, and the variable stretching of the near-tail field as Saturn rotates.
Fil: Russell, C. T.. University of California; Estados Unidos
Fil: Jackman, C. M.. Imperial College London; Reino Unido
Fil: Wei, H. Y.. University of California; Estados Unidos
Fil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Imperial College Of Science And Technology; Reino Unido
Fil: Dougherty, M. K.. Imperial College Of Science And Technology; Reino Unido
Materia
Titan's magnetic field
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/20684
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Titan's influence on Saturnian substorm occurrenceRussell, C. T.Jackman, C. M.Wei, H. Y.Bertucci, CesarDougherty, M. K.Titan's magnetic fieldhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Substorms play an important role in the energization and transport of plasmas in planetary magnetospheres, including the shedding of the mass added by moons in the case of Jupiter and Saturn. Mass shedding occurs through rapid reconnection in the near tail resulting in dipolarization on the magnetospheric side of the reconnection point and plasmoid formation down tail. Observations of these sudden reconnection events in Saturn’s near-tail region provide additional insight into this process. Saturnian substorms, at least on occasion, have a plasmoid formation phase leading to a traveling compression region. Changes in the field strength across reconnection events suggest that open flux has been removed from the tail. The timing of tail reconnection events appears to be controlled by both the orbital phase of Titan, and the variable stretching of the near-tail field as Saturn rotates.Fil: Russell, C. T.. University of California; Estados UnidosFil: Jackman, C. M.. Imperial College London; Reino UnidoFil: Wei, H. Y.. University of California; Estados UnidosFil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Imperial College Of Science And Technology; Reino UnidoFil: Dougherty, M. K.. Imperial College Of Science And Technology; Reino UnidoAmerican Geophysical Union2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/20684Russell, C. T.; Jackman, C. M.; Wei, H. Y.; Bertucci, Cesar; Dougherty, M. K.; Titan's influence on Saturnian substorm occurrence; American Geophysical Union; Geophysical Research Letters; 35; 12; 12-2008; 1-5; L121050094-8276CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1029/2008GL034080info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2008GL034080/abstractinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:14:25Zoai:ri.conicet.gov.ar:11336/20684instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:14:25.878CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Titan's influence on Saturnian substorm occurrence
title Titan's influence on Saturnian substorm occurrence
spellingShingle Titan's influence on Saturnian substorm occurrence
Russell, C. T.
Titan's magnetic field
title_short Titan's influence on Saturnian substorm occurrence
title_full Titan's influence on Saturnian substorm occurrence
title_fullStr Titan's influence on Saturnian substorm occurrence
title_full_unstemmed Titan's influence on Saturnian substorm occurrence
title_sort Titan's influence on Saturnian substorm occurrence
dc.creator.none.fl_str_mv Russell, C. T.
Jackman, C. M.
Wei, H. Y.
Bertucci, Cesar
Dougherty, M. K.
author Russell, C. T.
author_facet Russell, C. T.
Jackman, C. M.
Wei, H. Y.
Bertucci, Cesar
Dougherty, M. K.
author_role author
author2 Jackman, C. M.
Wei, H. Y.
Bertucci, Cesar
Dougherty, M. K.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Titan's magnetic field
topic Titan's magnetic field
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Substorms play an important role in the energization and transport of plasmas in planetary magnetospheres, including the shedding of the mass added by moons in the case of Jupiter and Saturn. Mass shedding occurs through rapid reconnection in the near tail resulting in dipolarization on the magnetospheric side of the reconnection point and plasmoid formation down tail. Observations of these sudden reconnection events in Saturn’s near-tail region provide additional insight into this process. Saturnian substorms, at least on occasion, have a plasmoid formation phase leading to a traveling compression region. Changes in the field strength across reconnection events suggest that open flux has been removed from the tail. The timing of tail reconnection events appears to be controlled by both the orbital phase of Titan, and the variable stretching of the near-tail field as Saturn rotates.
Fil: Russell, C. T.. University of California; Estados Unidos
Fil: Jackman, C. M.. Imperial College London; Reino Unido
Fil: Wei, H. Y.. University of California; Estados Unidos
Fil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Imperial College Of Science And Technology; Reino Unido
Fil: Dougherty, M. K.. Imperial College Of Science And Technology; Reino Unido
description Substorms play an important role in the energization and transport of plasmas in planetary magnetospheres, including the shedding of the mass added by moons in the case of Jupiter and Saturn. Mass shedding occurs through rapid reconnection in the near tail resulting in dipolarization on the magnetospheric side of the reconnection point and plasmoid formation down tail. Observations of these sudden reconnection events in Saturn’s near-tail region provide additional insight into this process. Saturnian substorms, at least on occasion, have a plasmoid formation phase leading to a traveling compression region. Changes in the field strength across reconnection events suggest that open flux has been removed from the tail. The timing of tail reconnection events appears to be controlled by both the orbital phase of Titan, and the variable stretching of the near-tail field as Saturn rotates.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/20684
Russell, C. T.; Jackman, C. M.; Wei, H. Y.; Bertucci, Cesar; Dougherty, M. K.; Titan's influence on Saturnian substorm occurrence; American Geophysical Union; Geophysical Research Letters; 35; 12; 12-2008; 1-5; L12105
0094-8276
CONICET Digital
CONICET
url http://hdl.handle.net/11336/20684
identifier_str_mv Russell, C. T.; Jackman, C. M.; Wei, H. Y.; Bertucci, Cesar; Dougherty, M. K.; Titan's influence on Saturnian substorm occurrence; American Geophysical Union; Geophysical Research Letters; 35; 12; 12-2008; 1-5; L12105
0094-8276
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1029/2008GL034080
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2008GL034080/abstract
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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