Outer magnetospheric boundaries : cluster results
When the stream of plasma emitted from the Sun (the solar wind) encounters Earth's magnetic field, it slows down and flows around it, leaving behind a cavity, the magnetosphere. The magnetopause is the surface that separates the solar wind on the outside from the Earth's magnetic field on...
Zapisane w:
| Kolejni autorzy: | , , , |
|---|---|
| Format: | Livre numérique |
| Język: | Anglais |
| Wydane: |
Dordrecht :
Springer Netherlands
[20..].
Cham : Springer Nature |
| Wydanie: | 1st ed. 2005. |
| Seria: | Space Sciences Series of ISSI
20 |
| Dostęp online: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Komentarz: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Outer Magnetospheric Boundaries: Cluster Results, Texte imprimé, 9781402034886 |
Spis treści:
- Solar Wind, Foreshock, Magnetosheath The Near-Earth Solar Wind The Foreshock The Magnetosheath The Bow Shock Cluster at the Bow Shock: Introduction Quasi-perpendicular Shock Structure and Processes Quasi-parallel Shock Structure and Processes Cluster at the Bow Shock: Status and Outlook Magnetopause and CUSP Magnetopause and Boundary Layer Cluster at the Magnetospheric Cusps Magnetopause Processes