The Magnetic Memory of Titan's Ionized Atmosphere
- Autores
- Bertucci, Cesar; Achilleos, N.; Dougherty, M. K.; Modolo, R.; Coates, A. J.; Szego, K.; Masters, A.; Ma, Y.; Neubauer, F. M.; Garnier, P.; Wahlund, J. E.; Young, D. T.
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- After 3 years and 31 close flybys of Titan by the Cassini Orbiter, Titan was finally observed in the shocked solar wind, outside of Saturn’s magnetosphere. These observations revealed that Titan’s flow-induced magnetosphere was populated by “fossil” fields originating from Saturn, to which the satellite was exposed before its excursion through the magnetopause. In addition, strong magnetic shear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been involved in the replacement of the fossil fields by the interplanetary magnetic field.
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: Achilleos, N.. University College London; Estados Unidos
Fil: Dougherty, M. K.. Imperial College London; Reino Unido
Fil: Modolo, R.. University of Iowa; Estados Unidos
Fil: Coates, A. J.. University College London; Estados Unidos
Fil: Szego, K.. Research Institute for Particle and Nuclear Physics; Hungría
Fil: Masters, A.. Imperial College London; Reino Unido
Fil: Ma, Y.. University of California; Estados Unidos
Fil: Neubauer, F. M.. Köln University; Alemania
Fil: Garnier, P.. Swedish Institute of Space Physics; Suecia
Fil: Wahlund, J. E.. Swedish Institute of Space Physics; Suecia
Fil: Young, D. T.. Southwest Research Institute; Estados Unidos - Materia
- Titan'S Magnetic Field
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/20688
Ver los metadatos del registro completo
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The Magnetic Memory of Titan's Ionized AtmosphereBertucci, CesarAchilleos, N.Dougherty, M. K.Modolo, R.Coates, A. J.Szego, K.Masters, A.Ma, Y.Neubauer, F. M.Garnier, P.Wahlund, J. E.Young, D. T.Titan'S Magnetic Fieldhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1After 3 years and 31 close flybys of Titan by the Cassini Orbiter, Titan was finally observed in the shocked solar wind, outside of Saturn’s magnetosphere. These observations revealed that Titan’s flow-induced magnetosphere was populated by “fossil” fields originating from Saturn, to which the satellite was exposed before its excursion through the magnetopause. In addition, strong magnetic shear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been involved in the replacement of the fossil fields by the interplanetary magnetic field.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; ArgentinaFil: Achilleos, N.. University College London; Estados UnidosFil: Dougherty, M. K.. Imperial College London; Reino UnidoFil: Modolo, R.. University of Iowa; Estados UnidosFil: Coates, A. J.. University College London; Estados UnidosFil: Szego, K.. Research Institute for Particle and Nuclear Physics; HungríaFil: Masters, A.. Imperial College London; Reino UnidoFil: Ma, Y.. University of California; Estados UnidosFil: Neubauer, F. M.. Köln University; AlemaniaFil: Garnier, P.. Swedish Institute of Space Physics; SueciaFil: Wahlund, J. E.. Swedish Institute of Space Physics; SueciaFil: Young, D. T.. Southwest Research Institute; Estados UnidosAmerican Association for the Advancement of Science2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/20688Bertucci, Cesar; Achilleos, N.; Dougherty, M. K.; Modolo, R.; Coates, A. J.; et al.; The Magnetic Memory of Titan's Ionized Atmosphere; American Association for the Advancement of Science; Science; 321; 5895; 12-2008; 1475-14780036-8075CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1126/science.1159780info:eu-repo/semantics/altIdentifier/url/http://science.sciencemag.org/content/321/5895/1475info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:26:02Zoai:ri.conicet.gov.ar:11336/20688instacron: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 10:26:02.598CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The Magnetic Memory of Titan's Ionized Atmosphere |
| title |
The Magnetic Memory of Titan's Ionized Atmosphere |
| spellingShingle |
The Magnetic Memory of Titan's Ionized Atmosphere Bertucci, Cesar Titan'S Magnetic Field |
| title_short |
The Magnetic Memory of Titan's Ionized Atmosphere |
| title_full |
The Magnetic Memory of Titan's Ionized Atmosphere |
| title_fullStr |
The Magnetic Memory of Titan's Ionized Atmosphere |
| title_full_unstemmed |
The Magnetic Memory of Titan's Ionized Atmosphere |
| title_sort |
The Magnetic Memory of Titan's Ionized Atmosphere |
| dc.creator.none.fl_str_mv |
Bertucci, Cesar Achilleos, N. Dougherty, M. K. Modolo, R. Coates, A. J. Szego, K. Masters, A. Ma, Y. Neubauer, F. M. Garnier, P. Wahlund, J. E. Young, D. T. |
| author |
Bertucci, Cesar |
| author_facet |
Bertucci, Cesar Achilleos, N. Dougherty, M. K. Modolo, R. Coates, A. J. Szego, K. Masters, A. Ma, Y. Neubauer, F. M. Garnier, P. Wahlund, J. E. Young, D. T. |
| author_role |
author |
| author2 |
Achilleos, N. Dougherty, M. K. Modolo, R. Coates, A. J. Szego, K. Masters, A. Ma, Y. Neubauer, F. M. Garnier, P. Wahlund, J. E. Young, D. T. |
| author2_role |
author author author author author author 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 |
After 3 years and 31 close flybys of Titan by the Cassini Orbiter, Titan was finally observed in the shocked solar wind, outside of Saturn’s magnetosphere. These observations revealed that Titan’s flow-induced magnetosphere was populated by “fossil” fields originating from Saturn, to which the satellite was exposed before its excursion through the magnetopause. In addition, strong magnetic shear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been involved in the replacement of the fossil fields by the interplanetary magnetic field. 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: Achilleos, N.. University College London; Estados Unidos Fil: Dougherty, M. K.. Imperial College London; Reino Unido Fil: Modolo, R.. University of Iowa; Estados Unidos Fil: Coates, A. J.. University College London; Estados Unidos Fil: Szego, K.. Research Institute for Particle and Nuclear Physics; Hungría Fil: Masters, A.. Imperial College London; Reino Unido Fil: Ma, Y.. University of California; Estados Unidos Fil: Neubauer, F. M.. Köln University; Alemania Fil: Garnier, P.. Swedish Institute of Space Physics; Suecia Fil: Wahlund, J. E.. Swedish Institute of Space Physics; Suecia Fil: Young, D. T.. Southwest Research Institute; Estados Unidos |
| description |
After 3 years and 31 close flybys of Titan by the Cassini Orbiter, Titan was finally observed in the shocked solar wind, outside of Saturn’s magnetosphere. These observations revealed that Titan’s flow-induced magnetosphere was populated by “fossil” fields originating from Saturn, to which the satellite was exposed before its excursion through the magnetopause. In addition, strong magnetic shear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been involved in the replacement of the fossil fields by the interplanetary magnetic field. |
| publishDate |
2008 |
| dc.date.none.fl_str_mv |
2008-12 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/20688 Bertucci, Cesar; Achilleos, N.; Dougherty, M. K.; Modolo, R.; Coates, A. J.; et al.; The Magnetic Memory of Titan's Ionized Atmosphere; American Association for the Advancement of Science; Science; 321; 5895; 12-2008; 1475-1478 0036-8075 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/20688 |
| identifier_str_mv |
Bertucci, Cesar; Achilleos, N.; Dougherty, M. K.; Modolo, R.; Coates, A. J.; et al.; The Magnetic Memory of Titan's Ionized Atmosphere; American Association for the Advancement of Science; Science; 321; 5895; 12-2008; 1475-1478 0036-8075 CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1126/science.1159780 info:eu-repo/semantics/altIdentifier/url/http://science.sciencemag.org/content/321/5895/1475 |
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American Association for the Advancement of Science |
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American Association for the Advancement of Science |
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