Whistler-mode Waves in a Hot Plasma

Sergei Sazhin

doi:10.1017/CBO9780511525094

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Whistler-mode Waves in a Hot Plasma

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Cited by 46
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Crossref Citations

This Book has been cited by the following publications. This list is generated based on data provided by Crossref.

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Sergei Sazhin, University of Sheffield

Publisher:: Cambridge University Press
Online publication date:: October 2009
Print publication year:: 1993
Online ISBN:: 9780511525094
DOI:: https://doi.org/10.1017/CBO9780511525094

Subjects:: Atmospheric Science and Meteorology, Physics and Astronomy, Astrophysics
Series:: Cambridge Atmospheric and Space Science Series

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The book provides an extensive theoretical treatment of whistler-mode propagation, instabilities and damping in a collisionless plasma. This book fills a gap between oversimplified analytical studies of these waves, based on the cold plasma approximation, and studies based on numerical methods. Although the book is primarily addressed to space plasma physicists and radio physicists, it will also prove useful to laboratory plasma physicists. Mathematical methods described in the book can be applied in a straightforward way to the analysis of other types of plasma waves. Problems included in this book, along with their solutions, allow it to be used as a textbook for postgraduate students.

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Whistler-mode Waves in a Hot Plasma

This Book has been cited by the following publications. This list is generated based on data provided by Crossref.

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Contents

Frontmatter
pp i-vi

Contents
pp vii-viii

Acknowledgements
pp ix-x

Introduction
pp 1-4

1 - Basic equations
pp 5-35

2 - Propagation in a cold plasma
pp 36-60

3 - Parallel propagation (weakly relativistic approximation)
pp 61-75

4 - Parallel propagation (non-relativistic approximation)
pp 76-93

5 - Quasi-longitudinal approximation
pp 94-120

6 - Quasi-electrostatic approximation
pp 121-143

7 - Growth and damping of the waves
pp 144-184

8 - Non-linear effects
pp 185-209

9 - Applications to the Earth's magnetosphere
pp 210-235

References
pp 236-249

Solutions to the problems
pp 250-257

Index
pp 258-259

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