TY  - BOOK
AU  - Sulaiman,Ali Haidar
ED  - SpringerLink (Online service)
TI  - The Near-Saturn Magnetic Field Environment
T2  - Springer Theses, Recognizing Outstanding Ph.D. Research,
SN  - 9783319492926
AV  - QB495-500.269 
U1  - 520 23
PY  - 2017///
CY  - Cham
PB  - Springer International Publishing, Imprint: Springer
KW  - Space sciences
KW  - Solar system
KW  - Planetary science
KW  - Astrophysics
KW  - Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)
KW  - Solar and Heliospheric Physics
KW  - Planetary Sciences
KW  - Astrophysics and Astroparticles
N1  - 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; Available to subscribing member institutions only. Доступно лише організаціям членам підписки
N2  - 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
UR  - https://doi.org/10.1007/978-3-319-49292-6
ER  -