Treats the origin of magnetic fields in planets, stars and galaxies, and the manner of their evolution over time.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Keith Moffatt FRS is Emeritus Professor of Mathematical Physics at the University of Cambridge. He has served as Head of the Department of Applied Mathematics and Theoretical Physics, and as Director of the Isaac Newton Institute for Mathematical Sciences in Cambridge. A former editor of the Journal of Fluid Mechanics, he has published papers in fluid dynamics and magnetohydrodynamics, and was a pioneer in the development of topological fluid dynamics. He is a Fellow of the Royal Society, a member of Academia Europæa, and a Foreign Member of the Academies of France, Italy, the Netherlands and USA. He has been awarded numerous prizes, most recently the 2018 Fluid Dynamics Prize of the American Physical Society.
Inhaltsangabe
Preface Part I. Basic Theory and Observations: 1. Introduction 2. Magnetokinematic preliminaries 3. Advection, distortion and diffusion 4. The magnetic field of the Earth and planets 5. Astrophysical magnetic fields Part II. Foundations of Dynamo Theory: 6. Laminar dynamo theory 7. Mean-field electrodynamics 8. Nearly axisymmetric dynamos 9. Solution of the mean-field equations 10. The fast dynamo Part III. Dynamic Aspects of Dynamo Action: 11. Low-dimensional models of the geodynamo 12. Dynamic equilibration 13. The geodynamo: instabilities and bifurcations 14. Astrophysical dynamic models 15. Helical turbulence 16. Magnetic relaxation under topological constraints 17. Magnetic relaxation in a low-ß plasma Appendix. Orthogonal curvilinear coordinates References Author index Subject index.
Preface Part I. Basic Theory and Observations: 1. Introduction 2. Magnetokinematic preliminaries 3. Advection, distortion and diffusion 4. The magnetic field of the Earth and planets 5. Astrophysical magnetic fields Part II. Foundations of Dynamo Theory: 6. Laminar dynamo theory 7. Mean-field electrodynamics 8. Nearly axisymmetric dynamos 9. Solution of the mean-field equations 10. The fast dynamo Part III. Dynamic Aspects of Dynamo Action: 11. Low-dimensional models of the geodynamo 12. Dynamic equilibration 13. The geodynamo: instabilities and bifurcations 14. Astrophysical dynamic models 15. Helical turbulence 16. Magnetic relaxation under topological constraints 17. Magnetic relaxation in a low-ß plasma Appendix. Orthogonal curvilinear coordinates References Author index Subject index.
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