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  • Textbook
  • © 2005

Physics of the Solar Corona

An Introduction with Problems and Solutions

  • Problems and Solutions for Students now included in this paperback edition
  • Draws on the most recent observations of solar phenomena obtained by the current generation of space missions, and includes the very latest imaging material most consistent with current observations
  • Incorporates all the new results and discoveries made and presents them in a systematic form, suitable for students and researchers
  • Includes high quality data and previously unseen images obtained as a result of the author’s access to the data archives of all current solar space missions

Part of the book series: Springer Praxis Books (PRAXIS)

Part of the book sub series: Astronomy and Planetary Sciences (ASTRONOMY)

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Table of contents (17 chapters)

  1. Front Matter

    Pages i-xxii
  2. Introduction

    Pages 1-36
  3. Thermal Radiation

    Pages 37-66
  4. Hydrostatics

    Pages 67-116
  5. Hydrodynamics

    Pages 117-174
  6. Magnetic Fields

    Pages 175-239
  7. MHD Oscillations

    Pages 283-330
  8. Propagating MHD Waves

    Pages 331-354
  9. Coronal Heating

    Pages 355-406
  10. Magnetic Reconnection

    Pages 407-464
  11. Particle Acceleration

    Pages 465-515
  12. Particle Kinematics

    Pages 517-550
  13. Hard X-Rays

    Pages 551-606
  14. Gamma-Rays

    Pages 607-636
  15. Radio Emission

    Pages 637-670
  16. Flare Plasma Dynamics

    Pages 671-702
  17. Back Matter

    Pages 739-909

About this book

Solar science has evolved rapidly over the past ten years as the results of a new generation of solar space missions have become available. This book provides a thorough introduction to the subject of solar physics, based on those spacecraft observations. The author introduces the solar corona, which has a temperature of several million degrees, and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation, which are fundamental processes in all stars, are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth. The author draws together observations made at many wavelengths from hard X-rays, soft X-rays, extreme UV and radio wavelengths.

This paperback study edition of Markus Aschwanden’s highly acclaimed Physics of the Solar Corona will include 50 pages of problems and solutions which will much enhance the value of the book to students.

Authors and Affiliations

  • Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Palo Alto, USA

    Markus J Aschwanden

Bibliographic Information

Buy it now

Buying options

eBook USD 99.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 129.99
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