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 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.
- ISBN:
- 9783319492919
- 9783319492919
-
Category:
- Solar system: the Sun & planets
- Format:
- Hardback
- Publication Date:
-
24-03-2017
- Publisher:
- Springer International Publishing AG
- Country of origin:
- Switzerland
- Pages:
- 97
- Dimensions (mm):
- 235x155x8mm
- Weight:
- 0.45kg
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