The Near-Saturn Magnetic Field Environment
Softcover reprint of the original 1st ed. 2017
Book Details
Format
Paperback / Softback
Book Series
Springer Theses
ISBN-10
3319841246
ISBN-13
9783319841243
Edition
Softcover reprint of the original 1st ed. 2017
Publisher
Springer International Publishing AG
Imprint
Springer International Publishing AG
Country of Manufacture
GB
Country of Publication
GB
Publication Date
Jun 29th, 2018
Print length
97 Pages
Product Classification:
Solar system: the Sun & planetsSolar system: the Sun and planetsApplied physicsAstrophysics
Ksh 16,200.00
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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).
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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