The Near-Saturn Magnetic Field Environment

Ali Haidar Sulaiman

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Springer International Publishing img Link Publisher

Naturwissenschaften, Medizin, Informatik, Technik / Astronomie

Beschreibung

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.

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Schlagwörter

Cassini Spacecraft, Collisionless Shock Waves, Specular Reflection, Saturn Magnetosphere, Alfven Mach Number, Saturn Magnetosheath