Advances in Nonlinear Dynamos
Seiten
2019
CRC Press (Verlag)
978-0-367-45450-0 (ISBN)
CRC Press (Verlag)
978-0-367-45450-0 (ISBN)
Nonlinear dynamo theory is central to understanding the magnetic structures of planets, stars, and galaxies. In chapters contributed by leading scientists, this text explores some of the recent advances in the field.
Nonlinear dynamo theory is central to understanding the magnetic structures of planets, stars and galaxies. In chapters contributed by some of the leading scientists in the field, this text explores some of the recent advances in the field. Both kinetic and dynamic approaches to the subject are considered, including fast dynamos, topological methods in dynamo theory, physics of the solar cycle and the fundamentals of mean field dynamo. Advances in Nonlinear Dynamos is ideal for graduate students and researchers in theoretical astrophysics and applied mathematics, particularly those interested in cosmic magnetism and related topics, such as turbulence, convection, and more general nonlinear physics.
Nonlinear dynamo theory is central to understanding the magnetic structures of planets, stars and galaxies. In chapters contributed by some of the leading scientists in the field, this text explores some of the recent advances in the field. Both kinetic and dynamic approaches to the subject are considered, including fast dynamos, topological methods in dynamo theory, physics of the solar cycle and the fundamentals of mean field dynamo. Advances in Nonlinear Dynamos is ideal for graduate students and researchers in theoretical astrophysics and applied mathematics, particularly those interested in cosmic magnetism and related topics, such as turbulence, convection, and more general nonlinear physics.
Manuel Nunez Antonio Ferriz-Mas
The Field, the Mean and the Meaning. Fast Dynamos. On the Theory of Convection in the Earth's Core. Dynamo Action of Magnetostropic Waves. Magnetic Flux Tubes and the Dynamo Problem. Physics of the Solar Cycle. Highly Supercritical Convection in Strong Magnetic Fields. Thin Aspect Ratio Alpha-Omega-Dynamos in Galactic Disks and Stellar Shells. Computational Aspects of Astrophysical MHD and Turbulence. Topological Quantities in Magnetohydrodynamics.
| Erscheinungsdatum | 03.12.2019 |
|---|---|
| Verlagsort | London |
| Sprache | englisch |
| Maße | 174 x 246 mm |
| Gewicht | 453 g |
| Themenwelt | Mathematik / Informatik ► Mathematik ► Angewandte Mathematik |
| Naturwissenschaften ► Biologie | |
| Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik | |
| ISBN-10 | 0-367-45450-5 / 0367454505 |
| ISBN-13 | 978-0-367-45450-0 / 9780367454500 |
| Zustand | Neuware |
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