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Energy Conversion and Particle Acceleration in the Solar Corona [electronic resource] / edited by Karl-Ludwig Klein.

Contributor(s): Material type: TextTextSeries: Lecture Notes in Physics ; 612Publisher: Berlin, Heidelberg : Springer Berlin Heidelberg, 2003Description: X, 319 p. online resourceContent type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9783540362425
Subject(s): Additional physical formats: Printed edition:: No title; Printed edition:: No title; Printed edition:: No titleDDC classification:
  • 520 23
  • 500.5 23
LOC classification:
  • QB495-500.269
Online resources:
Contents:
Energy Release and Magnetic Reconnection -- Magnetic Reconnection on the Sun and in the Earth’s Magnetosphere -- Magnetic 3-D Configurations of Energy Release in Solar Flares -- Theoretical Models of Magnetic Configurations Relevant to Energy Release -- The Energy Release Process in Solar Flares; Constraints from TRACE Observations -- Radio Diagnostics of Flare Energy Release -- Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliograph -- How Well Do We Understand Magnetic Reconnection? -- Energetic Particles at and from the Sun -- What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations? -- Transport of Energy from the Corona to the Chromosphere During Flares -- On the Origin of Solar Energetic Particle Events -- Acceleration and Propagation of Solar Energetic Particles -- Particle Acceleration by Magnetic Reconnection -- Particle Acceleration Processes in Cosmic Plasmas -- Aspects of Current Research -- Recent Progress in Understanding Energy Conversion and Particle Acceleration in the Solar Corona -- Solar Observations at Submillimeter Wavelengths.
In: Springer eBooksSummary: The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews the current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students.
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Energy Release and Magnetic Reconnection -- Magnetic Reconnection on the Sun and in the Earth’s Magnetosphere -- Magnetic 3-D Configurations of Energy Release in Solar Flares -- Theoretical Models of Magnetic Configurations Relevant to Energy Release -- The Energy Release Process in Solar Flares; Constraints from TRACE Observations -- Radio Diagnostics of Flare Energy Release -- Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliograph -- How Well Do We Understand Magnetic Reconnection? -- Energetic Particles at and from the Sun -- What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations? -- Transport of Energy from the Corona to the Chromosphere During Flares -- On the Origin of Solar Energetic Particle Events -- Acceleration and Propagation of Solar Energetic Particles -- Particle Acceleration by Magnetic Reconnection -- Particle Acceleration Processes in Cosmic Plasmas -- Aspects of Current Research -- Recent Progress in Understanding Energy Conversion and Particle Acceleration in the Solar Corona -- Solar Observations at Submillimeter Wavelengths.

The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews the current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students.

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