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| Titel |
Magnetic indices and geoeffectiveness of the solar wind from the radiation belts point of view |
| VerfasserIn |
Sandrine Rochel Grimald, Daniel Boscher, Sebastien Bourdarie, Angélica Sicard-Piet, Vincent Maget, Didier Lazaro |
| Konferenz |
EGU General Assembly 2013
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| Medientyp |
Artikel
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| Sprache |
Englisch
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 15 (2013) |
| Datensatznummer |
250076574
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| Zusammenfassung |
| The SALAMMBÔ code is a physical model of the radiation belts. It is well known that the radiation belts changes are indirectly linked to the solar wind parameter evolution. It is well known that CME and CIR disturb the magnetosphere in a different way and that they are more or less geoeffective. Then the impact in the radiation belts will also be different. Unfortunately, it is quite difficult to establish a direct link between the inner magnetosphere populations state and the solar wind parameters. As a consequence, the SALAMMBÔ code use the magnetic index Kp as a proxy. In this paper, we will discuss the use of Kp and other magnetic indices and of the geoeffectiveness of the solar wind structures from the radiation belts point of view. |
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