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The Near-Saturn Magnetic Field Environment

Produktform: E-Buch Text Elektronisches Buch in proprietärem

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.weiterlesen

Dieser Artikel gehört zu den folgenden Serien

Elektronisches Format: PDF

Sprache(n): Englisch

ISBN: 978-3-319-49292-6 / 978-3319492926 / 9783319492926

Verlag: Springer International Publishing

Erscheinungsdatum: 16.11.2016

Seiten: 97

Autor(en): Ali Haidar Sulaiman

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