Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data

Autores
Simon, S.; Motschmann, U.; Kleindienst, G.; Glassmeier, K. H.; Bertucci, Cesar; Dougherty, M. K.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
During the T34 flyby on 19 July 2007, the Cassini spacecraft passed through the magnetic pile-up region at Titan's ramside. The magnetic environment of Titan during this flyby is studied using a three-dimensional hybrid simulation model. This approach treats the electrons of the plasma as a massless, charge-neutralizing fluid, whereas the effects of finite ion gyroradii are taken into account by modeling the ions as individual particles. The simulation results are compared to data collected by the Cassini Magnetometer Instrument. The key features of the measured magnetic field signature have shown to be fully reproducible in the framework of the simulation model. Several signatures in the observed magnetic field can be ascribed to the passage of the Cassini spacecraft through the magnetic barrier upstream of Titan.
Fil: Simon, S.. Technische Universitat Braunschweig; Alemania
Fil: Motschmann, U.. Technische Universitat Braunschweig; Alemania
Fil: Kleindienst, G.. Technische Universitat Braunschweig; Alemania
Fil: Glassmeier, K. H.. Technische Universitat Braunschweig; Alemania
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: Dougherty, M. K.. Imperial College London; 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:11336/20680
Acceder
id CONICETDig_464823e30aaf12bd90b736f7d34be52c
oai_identifier_str oai:ri.conicet.gov.ar:11336/20680
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG dataSimon, S.Motschmann, U.Kleindienst, G.Glassmeier, K. H.Bertucci, CesarDougherty, M. K.Titan's magnetic fieldhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1During the T34 flyby on 19 July 2007, the Cassini spacecraft passed through the magnetic pile-up region at Titan's ramside. The magnetic environment of Titan during this flyby is studied using a three-dimensional hybrid simulation model. This approach treats the electrons of the plasma as a massless, charge-neutralizing fluid, whereas the effects of finite ion gyroradii are taken into account by modeling the ions as individual particles. The simulation results are compared to data collected by the Cassini Magnetometer Instrument. The key features of the measured magnetic field signature have shown to be fully reproducible in the framework of the simulation model. Several signatures in the observed magnetic field can be ascribed to the passage of the Cassini spacecraft through the magnetic barrier upstream of Titan.Fil: Simon, S.. Technische Universitat Braunschweig; AlemaniaFil: Motschmann, U.. Technische Universitat Braunschweig; AlemaniaFil: Kleindienst, G.. Technische Universitat Braunschweig; AlemaniaFil: Glassmeier, K. H.. Technische Universitat Braunschweig; AlemaniaFil: 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: Dougherty, M. K.. Imperial College London; 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/11336/20680Simon, S.; Motschmann, U.; Kleindienst, G.; Glassmeier, K. H.; Bertucci, Cesar; et al.; Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data; American Geophysical Union; Geophysical Research Letters; 35; 4; 12-2008; 1-40094-8276CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1029/2007GL033056info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2007GL033056/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 Técnicas2025-09-29T10:34:51Zoai:ri.conicet.gov.ar:11336/20680instacron: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 10:34:51.917CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
title Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
spellingShingle Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
Simon, S.
Titan's magnetic field
title_short Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
title_full Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
title_fullStr Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
title_full_unstemmed Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
title_sort Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
dc.creator.none.fl_str_mv Simon, S.
Motschmann, U.
Kleindienst, G.
Glassmeier, K. H.
Bertucci, Cesar
Dougherty, M. K.
author Simon, S.
author_facet Simon, S.
Motschmann, U.
Kleindienst, G.
Glassmeier, K. H.
Bertucci, Cesar
Dougherty, M. K.
author_role author
author2 Motschmann, U.
Kleindienst, G.
Glassmeier, K. H.
Bertucci, Cesar
Dougherty, M. K.
author2_role author
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 During the T34 flyby on 19 July 2007, the Cassini spacecraft passed through the magnetic pile-up region at Titan's ramside. The magnetic environment of Titan during this flyby is studied using a three-dimensional hybrid simulation model. This approach treats the electrons of the plasma as a massless, charge-neutralizing fluid, whereas the effects of finite ion gyroradii are taken into account by modeling the ions as individual particles. The simulation results are compared to data collected by the Cassini Magnetometer Instrument. The key features of the measured magnetic field signature have shown to be fully reproducible in the framework of the simulation model. Several signatures in the observed magnetic field can be ascribed to the passage of the Cassini spacecraft through the magnetic barrier upstream of Titan.
Fil: Simon, S.. Technische Universitat Braunschweig; Alemania
Fil: Motschmann, U.. Technische Universitat Braunschweig; Alemania
Fil: Kleindienst, G.. Technische Universitat Braunschweig; Alemania
Fil: Glassmeier, K. H.. Technische Universitat Braunschweig; Alemania
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: Dougherty, M. K.. Imperial College London; Reino Unido
description During the T34 flyby on 19 July 2007, the Cassini spacecraft passed through the magnetic pile-up region at Titan's ramside. The magnetic environment of Titan during this flyby is studied using a three-dimensional hybrid simulation model. This approach treats the electrons of the plasma as a massless, charge-neutralizing fluid, whereas the effects of finite ion gyroradii are taken into account by modeling the ions as individual particles. The simulation results are compared to data collected by the Cassini Magnetometer Instrument. The key features of the measured magnetic field signature have shown to be fully reproducible in the framework of the simulation model. Several signatures in the observed magnetic field can be ascribed to the passage of the Cassini spacecraft through the magnetic barrier upstream of Titan.
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/11336/20680
Simon, S.; Motschmann, U.; Kleindienst, G.; Glassmeier, K. H.; Bertucci, Cesar; et al.; Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data; American Geophysical Union; Geophysical Research Letters; 35; 4; 12-2008; 1-4
0094-8276
CONICET Digital
CONICET
url http://hdl.handle.net/11336/20680
identifier_str_mv Simon, S.; Motschmann, U.; Kleindienst, G.; Glassmeier, K. H.; Bertucci, Cesar; et al.; Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data; American Geophysical Union; Geophysical Research Letters; 35; 4; 12-2008; 1-4
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/10.1029/2007GL033056
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2007GL033056/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
_version_ 1844614366205313024
score 13.070432

Publicaciones similares