- 118 pages
- English
- PDF
- Available on iOS & Android
eBook - PDF
The Near-Saturn Magnetic Field Environment
About this book
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.
Information
Topic
Physical SciencesSubtopic
Astronomy & AstrophysicsTable of contents
- Supervisor’s Foreword
- Preface
- Acknowledgements
- Contents
- Nomenclature
- List of Figures
- List of Tables
- 1 Introduction to Space Plasmas
- 2 The Sun-Saturn Connection
- 3 Spacecraft and Instrumentation
- 4 Magnetic Field Characterisation of Saturn’s Bow Shock
- 5 Quasi-Perpendicular High Mach Number Collisionless Shocks
- 6 The Magnetic Structure of Saturn’s Magnetosheath
- 7 Summary and Perspective
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Yes, you can access The Near-Saturn Magnetic Field Environment by Ali Haidar Sulaiman in PDF and/or ePUB format, as well as other popular books in Physical Sciences & Astronomy & Astrophysics. We have over 1.5 million books available in our catalogue for you to explore.