The Near-Saturn Magnetic Field Environment / Springer Theses (PDF)
(Sprache: Englisch)
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...
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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.
Autoren-Porträt von Ali Haidar Sulaiman
Dr. Sulaiman graduated from Imperial College London with a Masters in Aeronautical Engineering with first class honors. He holds a Ph.D. in Space Physics at Imperial College London under Professor Michele Dougherty FRS. He is currently a postdoctoral scholar at the University of Iowa.Bibliographische Angaben
- Autor: Ali Haidar Sulaiman
- 2016, 1st ed. 2017, 97 Seiten, Englisch
- Verlag: Springer-Verlag GmbH
- ISBN-10: 3319492926
- ISBN-13: 9783319492926
- Erscheinungsdatum: 16.11.2016
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