The magnetic memory of Titan's ionized atmosphere
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...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00368075_v321_n5895_p1475_Bertucci |
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todo:paper_00368075_v321_n5895_p1475_Bertucci2023-10-03T14:47:52Z The magnetic memory of Titan's ionized atmosphere Bertucci, C. 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. magnetic field magnetopause magnetosphere planetary atmosphere Saturn solar wind Titan article atmosphere geometry magnetic field magnetism priority journal 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00368075_v321_n5895_p1475_Bertucci |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
magnetic field magnetopause magnetosphere planetary atmosphere Saturn solar wind Titan article atmosphere geometry magnetic field magnetism priority journal |
| spellingShingle |
magnetic field magnetopause magnetosphere planetary atmosphere Saturn solar wind Titan article atmosphere geometry magnetic field magnetism priority journal Bertucci, C. 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. The magnetic memory of Titan's ionized atmosphere |
| topic_facet |
magnetic field magnetopause magnetosphere planetary atmosphere Saturn solar wind Titan article atmosphere geometry magnetic field magnetism priority journal |
| 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. |
| format |
JOUR |
| author |
Bertucci, C. 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_facet |
Bertucci, C. 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_sort |
Bertucci, C. |
| title |
The magnetic memory of Titan's ionized atmosphere |
| 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 |
magnetic memory of titan's ionized atmosphere |
| url |
http://hdl.handle.net/20.500.12110/paper_00368075_v321_n5895_p1475_Bertucci |
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