Magnetic Reconnection
MHD Theory and Applications
Seiten
2000
Cambridge University Press (Verlag)
978-0-521-48179-3 (ISBN)
Cambridge University Press (Verlag)
978-0-521-48179-3 (ISBN)
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This authoritative volume gives a comprehensive overview of magnetic reconnection. Providing a lucid introduction to the theory, and a wide-ranging review of its applications, it is ideal for graduate students and researchers in solar physics, astrophysics, plasma physics and space science.
Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak disruptions. In an authoritative volume, two world leaders on the subject give a comprehensive overview of this fundamental process. The book provides both a full account of the basic theory and a wide-ranging review of the physical phenomena created by reconnection - from laboratory machines, the Earth's magnetosphere, and the Sun's atmosphere to flare stars and astrophysical accretion disks. It also provides a succinct account of various mechanisms of particle acceleration and of how reconnection can be important in such mechanisms. The clear and pedagogical style makes this book an essential introduction for graduate students and an authoritative reference for researchers in solar physics, astrophysics, plasma physics and space science.
Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak disruptions. In an authoritative volume, two world leaders on the subject give a comprehensive overview of this fundamental process. The book provides both a full account of the basic theory and a wide-ranging review of the physical phenomena created by reconnection - from laboratory machines, the Earth's magnetosphere, and the Sun's atmosphere to flare stars and astrophysical accretion disks. It also provides a succinct account of various mechanisms of particle acceleration and of how reconnection can be important in such mechanisms. The clear and pedagogical style makes this book an essential introduction for graduate students and an authoritative reference for researchers in solar physics, astrophysics, plasma physics and space science.
Preface; 1. Introduction; 2. Current-sheet formation; 3. Magnetic annihilation; 4. Steady reconnection: the classical solutions; 5. Steady reconnection: new generation of fast regimes; 6. Unsteady reconnection: the tearing mode; 7. Unsteady reconnection: other approaches; 8. Reconnection in three dimensions; 9. Laboratory applications; 10. Magnetospheric applications; 11. Solar applications; 12. Astrophysical applications; 13. Particle acceleration; References; Appendices; Index.
| Erscheint lt. Verlag | 18.5.2000 |
|---|---|
| Zusatzinfo | 6 Tables, unspecified; 1 Halftones, unspecified; 192 Line drawings, unspecified |
| Verlagsort | Cambridge |
| Sprache | englisch |
| Maße | 179 x 256 mm |
| Gewicht | 1340 g |
| Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
| Naturwissenschaften ► Physik / Astronomie ► Plasmaphysik | |
| ISBN-10 | 0-521-48179-1 / 0521481791 |
| ISBN-13 | 978-0-521-48179-3 / 9780521481793 |
| Zustand | Neuware |
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