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PHYSICS OF THE SOLAR CORONA. AN INTRODUCTION View all abstracts by submitter

Markus J. Aschwanden   Submitted: 2004-09-15 16:45

Chapters: 1. Introduction 2. Thermal Radiation 3. Hydrostatics 4. Hydrodynamics 5. Magnetic Fields 6. Magneto-Hydrodynamics (MHD) 7. MHD Oscillations 8. Propagating MHD Waves 9. Coronal Heating 10. Magnetic Reconnection 11. Particle Acceleration 12. Particle Kinematics 13. Hard X-Rays 14. Gamma Rays 15. Radio Emission 16. Flare Plasma Emission 17. Coronal Mass Ejections (CMEs) - Cover text: Over the past ten years, results from a new generation of solar space missions have become available. Based on those missions and observations made at many wavelengths, from hard X-rays, soft X-rays, extreme UV and radio wavelengths, this book is a comprehensive introduction to solar physics. It describes the solar corona, and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities, plasma heating, magnetic reconnection and particle acceleration processes. The latest results on coronal heating and radiation - fundamental processes in all stars - are presented. Spectacular phenomena, such as solar flares and coronal mass ejections, are described in detail.

Authors: Markus J. Aschwanden
Projects: None,RHESSI,Soho-EIT,Soho-MDI,Soho-CDS,Soho-LASCO,Yohkoh-BCS,Yohkoh-HXT,Yohkoh-SXT,Yohkoh-WBS,TRACE

Publication Status: ISBN: 3-540-22321-5, Praxis Publishing (Chichester, UK) and Springer (Berlin), September 2004
Last Modified: 2004-09-15 16:45
Go to main E-Print page  Electron acceleration in reconnecting current sheets  Determination Of Electron Flux Spectra In A Solar Flare With An Augmented Regularization Method: Application To RHESSI Data  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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