The Near-Saturn Magnetic Field Environment
This thesis focuses on the very high Mach number shock wave that is located sunward of Saturn's strong magnetic field in the continuous high-speed flow of charged particles from the Sun (the solar wind). The author exploits the fact that the Cassini spacecraft is the only orbiter in a unique pa...
Κύριος συγγραφέας: | |
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Συγγραφή απο Οργανισμό/Αρχή: | |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Cham :
Springer International Publishing : Imprint: Springer,
2017.
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Σειρά: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- Introduction to Space Plasmas
- The Sun-Saturn Connection
- Spacecraft and Instrumentation
- Magnetic Field Characterisation of Saturn’s Bow Shock
- Quasi-perpendicular High Mach Number Collisionless Shocks
- The Magnetic Structure of Saturn’s Magnetosheath
- Summary and Perspective
- Bibliography.