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...
Συγγραφή απο Οργανισμό/Αρχή: | |
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Άλλοι συγγραφείς: | , , , |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Dordrecht :
Springer Netherlands,
2005.
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Σειρά: | Space Sciences Series of ISSI,
20 |
Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- 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.