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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/20686
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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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1846083502566539264 |
score |
13.22299 |