Advances in solar system magnetohydrodynamics
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Advances in solar system magnetohydrodynamics
Cambridge University Press, 1991
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Includes index
Description and Table of Contents
Description
Most of the solar system is in the plasma state and its subtle non-linear interaction with the magnetic field is described for many purposes by the equations of magnetohydrodynamics (MHD). Over the past few years this important and complex field has become one of the most actively pursued areas of research, with increasingly diverse applications in geophysics, space physics and astrophysics. This book examines the basic MHD topics, such as equilibria, waves, instabilities and reconnection and examines each in the context of different areas that utilize MHD. Many of the world's leading experts have contributed to this volume, which has been edited by two of the key enthusiasts. It is hoped that it can help the reader to appreciate and understand the common threads between the different branches of magnetohydrodynamics. This book will be a timely exposition of recent advances made in the field.
Table of Contents
- 1. Introduction to solar system MHD E. R. Priest
- 2. Dynamo models and Taylor's constraint C. A. Jones
- 3. Problems of planetary dynamo theory F. H. Buse
- 4. Convection near the earth's core-mantle boundary D. R. Fearn
- 5. Magnetic buoyancy D. W. Hughes
- 6. MHD waves in the Sun B. Roberts
- 7. MHD waves and wave heating in nonuniform plasmas M. Goossens
- 8. Weak solutions of magnetostactis T. Amari
- 9. Magnetic reconnection in solar flares M. Jardine
- 10. Three-dimensional magnetic reconnection M. Hesse
- 11. Magnetic heating of the solar corona M. A. Berger
- 12. Hydromagnetic equilibrium K. Tsinganos
- 13. Solar prominences P. Demoulin
- 14. MHD of solar flares A. W. Hood
- 15. MHD turbulence in the solar wind A. Mangeney
- 16. The earth's magnetosphere M. Saunders
- 17. MHD forces in astrophysical disks and jets J. Heyvaerts.
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