Plasma Physics for Astrophysics

Russell M. Kulsrud

468 pages, parution le 21/02/2005

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Résumé

In this book, a distinguished expert introduces plasma physics from the ground up, presenting it as a comprehensible field that can be grasped largely on the basis of physical intuition and qualitative reasoning, similar to other fields of physics. Plasmas are ionized gases that can be found in a hydrogen bomb explosion, the confinement chamber of an experimental fusion reactor, the solar corona, the aurora borealis, the interstellar medium, and the immediate vicinity of a gravitational black hole. Not surprisingly, plasma physics appears to consist of numerous topics arising independently from astrophysics, fusion physics, and other practical applications, and hence it remains a field poorly understood even by many astrophysicists. But, in fact, most of these topics can be approached from the same perspective, with a simple, physical intuition.

Selecting simple examples and presenting them in a simultaneously intuitive and rigorous manner, Russell Kulsrud guides readers through a careful derivation of the results and allows them to think through the physics for themselves. Thus, they are better prepared for complex cases and more general results. The first eleven chapters present topics by their importance to plasma physics while the last three chapters emphasize the field's astrophysical applications, applying the results accrued earlier. Throughout, many problems illustrate the field's applications. Based on a course the author taught for many years, Plasma Physics for Astrophysics is intended for graduate students as well as for working astrophysicists.

L'auteur - Russell M. Kulsrud

Russell M. Kulsrud is Professor Emeritus of Astrophysical Sciences at Princeton University. A former head of the theory division at Princeton Plasma Physics Laboratory, he has published nearly 150 research papers. His many honors include the James Clerk Maxwell Prize in Plasma Physics, awarded by the American Physical Society in 1993.

Sommaire

Preface
Introduction
Particle Motions
Magnetohydrodynamics
Conservation Relations
MHD Waves
Nonlinear Steepening and Shocks
The Energy Principle and Instabilities
Collisions and the Braginski Equations
Collisionless Plasmas
Collisionless Plasmas: Thermal Effects
Nonlinear Phenomena
Cosmic Rays
Astrophysical Dynamos
Magnetic Reconnection

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Caractéristiques techniques

	PAPIER
Éditeur(s)	Princeton University Press
Auteur(s)	Russell M. Kulsrud
Parution	21/02/2005
Nb. de pages	468
Format	15,5 x 23,5
Couverture	Broché
Poids	676g
Intérieur	Noir et Blanc
EAN13	9780691120737
ISBN13	978-0-691-12073-7