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Titlebook: Solar Flares; Zdeněk Švestka Book 1976 D. Reidel Publishing Company, Dordrecht, Holland 1976 Corona.Photosphere.Planet.Solar flare.Sunspot

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978-90-277-0663-8D. Reidel Publishing Company, Dordrecht, Holland 1976
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Particle Emission From Solar Flares, their transit over the visible hemisphere of the Sun. The particle flux sets in on about the second day after the appearance of the region on the eastern solar limb (cf. Figure 100) and continues until the region moves to about 40° behind the western limb (Fan .., 1968). Figure 90 shows an example
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The High-Temperature Flare,regions. The reason for this is that thermal and non-thermal effects are coupled in the high temperature flare regions in the solar corona; non-thermal effects arise from pre-heated plasma and eventually become thermalized.
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