The Near-saturn Magnetic Field Environment - ENG
| ISBN: | 9783319492926 |
|---|---|
| Formato: | Page Fidelity |
| Idioma: | Inglés |
| Editorial: | Springer Nature |
| Tema: | Ciencia |
| Subtema: | Física astrofísica |
| Año de publicación: | 2016-11-16 |
This thesis focuses on the very high Mach number shock wave that is located sunward of Saturns 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 parameter regime, far different from the more familiar near-Earth space, to provide in-situ insights into the unreachable exotic regime of supernova remnants. This thesis bridges the gap between shock physics in the Solar System and the physics of ultra-high Mach number shocks around the remnants of supernova explosions, since to date research into the latter has been restricted to theory, remote observations, and simulations.










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