Large-scale dynamics of Saturn's magnetopause: Observations by Cassini

Autores
Achilleos, N.; Arridge, C. S.; Bertucci, Cesar; Jackman, C. M.; Dougherty, M. K.; Khurana, K. K.; Russell, C. T.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been investigated. Established statistical techniques for Jupiter have been applied to the kronian system, employing Cassini magnetometer data and a new empirical shape model of the magnetopause based on these data. The resulting distribution of standoff distance RMP for Saturn, covering a time interval of 400 days, is welldescribed by a ‘‘dual’’ or ‘‘bimodal’’ model—the sum of two normal distributions with different means at 22 and 27 planetary radii. We have made a comparison between the dual model’s prediction for the probability distribution of solar wind dynamic pressure at Saturn with a sequence of observations from the Cassini Plasma Spectrometer (CAPS) instrument. Although the solar wind dynamic pressure observations are limited to a smaller time interval than the magnetometer data, we find that their overall range is in broad agreement with the that of the modeled pressures. However, the bimodal structure exhibited by the model is not apparent in the solar wind data for the corresponding range of dynamic pressures ( 0.008 – 0.06 nPa), which suggests that other mechanisms at Saturn also influence the size distribution of the magnetopause. Considering internal processes at Saturn and their influence on magnetopause size, we conclude that the effect of internal mass loading and loss from the magnetospheric disk is plausibly able to explain the observed bimodal distribution in magnetopause standoff distance.
Fil: Achilleos, N.. University College London; Estados Unidos
Fil: Arridge, C. S.. Imperial College London; Reino Unido
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
Fil: Jackman, C. M.. Imperial College London; Reino Unido
Fil: Dougherty, M. K.. Imperial College London; Reino Unido
Fil: Khurana, K. K.. University of California; Estados Unidos
Fil: Russell, C. T.. University of California; Estados Unidos
Materia
Magnetosphere
Saturn
Magnetopause
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:11336/20686

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spelling Large-scale dynamics of Saturn's magnetopause: Observations by CassiniAchilleos, N.Arridge, C. S.Bertucci, CesarJackman, C. M.Dougherty, M. K.Khurana, K. K.Russell, C. T.MagnetosphereSaturnMagnetopausehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been investigated. Established statistical techniques for Jupiter have been applied to the kronian system, employing Cassini magnetometer data and a new empirical shape model of the magnetopause based on these data. The resulting distribution of standoff distance RMP for Saturn, covering a time interval of 400 days, is welldescribed by a ‘‘dual’’ or ‘‘bimodal’’ model—the sum of two normal distributions with different means at 22 and 27 planetary radii. We have made a comparison between the dual model’s prediction for the probability distribution of solar wind dynamic pressure at Saturn with a sequence of observations from the Cassini Plasma Spectrometer (CAPS) instrument. Although the solar wind dynamic pressure observations are limited to a smaller time interval than the magnetometer data, we find that their overall range is in broad agreement with the that of the modeled pressures. However, the bimodal structure exhibited by the model is not apparent in the solar wind data for the corresponding range of dynamic pressures ( 0.008 – 0.06 nPa), which suggests that other mechanisms at Saturn also influence the size distribution of the magnetopause. Considering internal processes at Saturn and their influence on magnetopause size, we conclude that the effect of internal mass loading and loss from the magnetospheric disk is plausibly able to explain the observed bimodal distribution in magnetopause standoff distance.Fil: Achilleos, N.. University College London; Estados UnidosFil: Arridge, C. S.. Imperial College London; Reino UnidoFil: 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; ArgentinaFil: Jackman, C. M.. Imperial College London; Reino UnidoFil: Dougherty, M. K.. Imperial College London; Reino UnidoFil: Khurana, K. K.. University of California; Estados UnidosFil: Russell, C. T.. University of California; Estados UnidosAmerican Geophysical Union2008-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/20686Achilleos, N.; Arridge, C. S.; Bertucci, Cesar; Jackman, C. M.; Dougherty, M. K.; et al.; Large-scale dynamics of Saturn's magnetopause: Observations by Cassini; American Geophysical Union; Journal of Geophysical Research; 113; A11; 11-2008; 1-140148-0227CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2008JA013265info:eu-repo/semantics/altIdentifier/doi/10.1029/2008JA013265info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:38:22Zoai:ri.conicet.gov.ar:11336/20686instacron: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:34982025-10-15 15:38:22.851CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
title Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
spellingShingle Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
Achilleos, N.
Magnetosphere
Saturn
Magnetopause
title_short Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
title_full Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
title_fullStr Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
title_full_unstemmed Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
title_sort Large-scale dynamics of Saturn's magnetopause: Observations by Cassini
dc.creator.none.fl_str_mv Achilleos, N.
Arridge, C. S.
Bertucci, Cesar
Jackman, C. M.
Dougherty, M. K.
Khurana, K. K.
Russell, C. T.
author Achilleos, N.
author_facet Achilleos, N.
Arridge, C. S.
Bertucci, Cesar
Jackman, C. M.
Dougherty, M. K.
Khurana, K. K.
Russell, C. T.
author_role author
author2 Arridge, C. S.
Bertucci, Cesar
Jackman, C. M.
Dougherty, M. K.
Khurana, K. K.
Russell, C. T.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Magnetosphere
Saturn
Magnetopause
topic Magnetosphere
Saturn
Magnetopause
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been investigated. Established statistical techniques for Jupiter have been applied to the kronian system, employing Cassini magnetometer data and a new empirical shape model of the magnetopause based on these data. The resulting distribution of standoff distance RMP for Saturn, covering a time interval of 400 days, is welldescribed by a ‘‘dual’’ or ‘‘bimodal’’ model—the sum of two normal distributions with different means at 22 and 27 planetary radii. We have made a comparison between the dual model’s prediction for the probability distribution of solar wind dynamic pressure at Saturn with a sequence of observations from the Cassini Plasma Spectrometer (CAPS) instrument. Although the solar wind dynamic pressure observations are limited to a smaller time interval than the magnetometer data, we find that their overall range is in broad agreement with the that of the modeled pressures. However, the bimodal structure exhibited by the model is not apparent in the solar wind data for the corresponding range of dynamic pressures ( 0.008 – 0.06 nPa), which suggests that other mechanisms at Saturn also influence the size distribution of the magnetopause. Considering internal processes at Saturn and their influence on magnetopause size, we conclude that the effect of internal mass loading and loss from the magnetospheric disk is plausibly able to explain the observed bimodal distribution in magnetopause standoff distance.
Fil: Achilleos, N.. University College London; Estados Unidos
Fil: Arridge, C. S.. Imperial College London; Reino Unido
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
Fil: Jackman, C. M.. Imperial College London; Reino Unido
Fil: Dougherty, M. K.. Imperial College London; Reino Unido
Fil: Khurana, K. K.. University of California; Estados Unidos
Fil: Russell, C. T.. University of California; Estados Unidos
description The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been investigated. Established statistical techniques for Jupiter have been applied to the kronian system, employing Cassini magnetometer data and a new empirical shape model of the magnetopause based on these data. The resulting distribution of standoff distance RMP for Saturn, covering a time interval of 400 days, is welldescribed by a ‘‘dual’’ or ‘‘bimodal’’ model—the sum of two normal distributions with different means at 22 and 27 planetary radii. We have made a comparison between the dual model’s prediction for the probability distribution of solar wind dynamic pressure at Saturn with a sequence of observations from the Cassini Plasma Spectrometer (CAPS) instrument. Although the solar wind dynamic pressure observations are limited to a smaller time interval than the magnetometer data, we find that their overall range is in broad agreement with the that of the modeled pressures. However, the bimodal structure exhibited by the model is not apparent in the solar wind data for the corresponding range of dynamic pressures ( 0.008 – 0.06 nPa), which suggests that other mechanisms at Saturn also influence the size distribution of the magnetopause. Considering internal processes at Saturn and their influence on magnetopause size, we conclude that the effect of internal mass loading and loss from the magnetospheric disk is plausibly able to explain the observed bimodal distribution in magnetopause standoff distance.
publishDate 2008
dc.date.none.fl_str_mv 2008-11
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/11336/20686
Achilleos, N.; Arridge, C. S.; Bertucci, Cesar; Jackman, C. M.; Dougherty, M. K.; et al.; Large-scale dynamics of Saturn's magnetopause: Observations by Cassini; American Geophysical Union; Journal of Geophysical Research; 113; A11; 11-2008; 1-14
0148-0227
CONICET Digital
CONICET
url http://hdl.handle.net/11336/20686
identifier_str_mv Achilleos, N.; Arridge, C. S.; Bertucci, Cesar; Jackman, C. M.; Dougherty, M. K.; et al.; Large-scale dynamics of Saturn's magnetopause: Observations by Cassini; American Geophysical Union; Journal of Geophysical Research; 113; A11; 11-2008; 1-14
0148-0227
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2008JA013265
info:eu-repo/semantics/altIdentifier/doi/10.1029/2008JA013265
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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