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Titlebook: Energy Conversion and Particle Acceleration in the Solar Corona; Karl-Ludwig Klein Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromo

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https://doi.org/10.1007/978-94-007-0585-2ion events, as evidenced by the 2000 July 14 (“Bastille Day”) flare; (5) radio imaging of CMEs and filament eruptions; (6) the relationship of coronal and interplanetary shock waves to flares, CMEs, and other coronal waves; and (7) the origin of solar energetic particles.
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Introductioneractions between plasmas and magnetic fields. The manner in which magnetically stored energy is converted to other forms, and prominently to energetic particle populations, is clearly of central importance for coronal physics.
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On the Origin of Solar Energetic Particle Events events, low energy protons (<6 MeV) are released roughly an hour later than the electrons and are most likely accelerated at the shock fronts of coronal mass ejections. The remaining third of proton events show a puzzling velocity dispersion that could be explained by a non-simultaneous release of protons at different energy.
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