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The near-Saturn magnetic field envir...

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The near-Saturn magnetic field environment

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	The near-Saturn magnetic field environment/ by Ali Haidar Sulaiman.
作者:	Sulaiman, Ali Haidar.
出版者:	Cham :Springer International Publishing : : 2017.,
面頁冊數:	xxv, 97 p. :ill., digital ; : 24 cm.;
Contained By:	Springer eBooks
標題:	Interplanetary magnetic fields. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-49292-6
ISBN:	9783319492926

The near-Saturn magnetic field environment
Sulaiman, Ali Haidar.

The near-Saturn magnetic field environment[electronic resource] /by Ali Haidar Sulaiman. - Cham :Springer International Publishing :2017. - xxv, 97 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction to Space Plasmas -- The Sun-Saturn Connection -- Spacecraft and Instrumentation -- Magnetic Field Characterisation of Saturn's Bow Shock -- Quasi-perpendicular High Mach Number Collisionless Shocks -- The Magnetic Structure of Saturn's Magnetosheath -- Summary and Perspective -- Bibliography.

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: 9783319492926

Standard No.: 10.1007/978-3-319-49292-6doiSubjects--Topical Terms:

1249078
Interplanetary magnetic fields.

LC Class. No.: QC809.M25

Dewey Class. No.: 523.0188

The near-Saturn magnetic field environment
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520 $a 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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