Overview

An outgrowth of a workshop held by the Community of European Solar Radio Astronomers (CESRA), this volume collects reviews on current research and perspectives on the variable solar corona: high-energy particles, large-scale disturbances such as mass ejections and waves, and radio diagnostics of the coronal plasma. Multiwavelength observations of the Sun with radio instruments and recent space missions are drawn on extensively, as well as input from neighbouring fields e.g. solar wind, Earth's bow shock. Recent developments are discussed alongside key developments in this rapidly evolving field.

Full Product Details

Author:   Karl L. Klein ,  Alexander L. MacKinnon
Publisher:   Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Imprint:   Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Edition:   2007 ed.
Volume:   725
Dimensions:   Width: 15.60cm , Height: 1.70cm , Length: 23.50cm
Weight:   1.310kg
ISBN:  

9783540715696

ISBN 10:   354071569
Pages:   284
Publication Date:   29 August 2007
Audience:   College/higher education ,  Professional and scholarly ,  Undergraduate ,  Postgraduate, Research & Scholarly
Format:   Hardback
Publisher's Status:   Active
Availability:   In Print  
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Table of Contents

Introduction: The High-energy Corona – Waves, Eruptions, Particles.- Introduction: The High-energy Corona – Waves, Eruptions, Particles.- Particle Acceleration During Flares.- Magnetic Complexity, Fragmentation, Particle Acceleration and Radio Emission from the Sun.- Review of Selected RHESSI Solar Results.- RHESSI Results – Time for a Rethink?.- Small Scale Energy Release and the Acceleration and Transport of Energetic Particles.- Large-scale Disturbances.- Large-scale Waves and Shocks in the Solar Corona.- Energetic Particles Related with Coronal and Interplanetary Shocks.- Particle Acceleration at the Earth’s Bow Shock.- On the Existence of Non-maxwellian Velocity Distribution Functions in the Corona and their Consequences for the Solar Wind Acceleration.- Recent Research: Large-scale Disturbances, their Origin and Consequences.- Plasma of the Solar Corona.- Quasi-periodic Pulsations as a Diagnostic Tool for Coronal Plasma Parameters.- Pulsating Solar Radio Emission.

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