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  • © 1993

Plasma Astrophysics

Kinetic Processes in Solar and Stellar Coronae

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Part of the book series: Astrophysics and Space Science Library (ASSL, volume 184)

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Table of contents (11 chapters)

  1. Front Matter

    Pages i-xvii
  2. Introduction

    • Arnold Benz
    Pages 1-21
  3. Basic Concepts

    • Arnold Benz
    Pages 22-50
  4. Magnetohydrodynamics

    • Arnold Benz
    Pages 51-68
  5. Waves in a Cold, Collisionless Plasma

    • Arnold Benz
    Pages 69-88
  6. Kinetic Plasma and Particle Beams

    • Arnold Benz
    Pages 89-114
  7. Astrophysical Electron Beams

    • Arnold Benz
    Pages 115-153
  8. Electrons Trapped in Magnetic Fields

    • Arnold Benz
    Pages 177-211
  9. Electric Currents

    • Arnold Benz
    Pages 212-233
  10. Collisionless Shock Waves

    • Arnold Benz
    Pages 234-257
  11. Propagation of Radiation

    • Arnold Benz
    Pages 258-281
  12. Back Matter

    Pages 282-299

About this book

This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a back­ ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. Sort­ ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena - such as one period of a high-frequency wave - or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such pro­ cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star.

Authors and Affiliations

  • Institute of Astronomy, ETH Zurich, Switzerland

    Arnold Benz

Bibliographic Information

  • Book Title: Plasma Astrophysics

  • Book Subtitle: Kinetic Processes in Solar and Stellar Coronae

  • Authors: Arnold Benz

  • Series Title: Astrophysics and Space Science Library

  • DOI: https://doi.org/10.1007/978-94-011-2064-7

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: Springer Science+Business Media Dordrecht 1993

  • Hardcover ISBN: 978-0-7923-2429-4Published: 30 September 1993

  • Softcover ISBN: 978-94-010-4915-3Published: 29 October 2012

  • eBook ISBN: 978-94-011-2064-7Published: 06 December 2012

  • Series ISSN: 0067-0057

  • Series E-ISSN: 2214-7985

  • Edition Number: 1

  • Number of Pages: XVII, 299

  • Topics: Astrophysics and Astroparticles, Nuclear Physics, Heavy Ions, Hadrons

Buy it now

Buying options

eBook USD 84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access