Abstract
As one can see from above considerations, in no other situation except for that during solar flares the acceleration of charged particles can be explored in such details, because (a) events can be studied in their temporal history and (b)the Sun is near enough to investigate the phenomenon in a very wide energy range from X-rays to gamma rays — two main kinds of flare neutral radiation, where the accelerated particles leave their “fingerprints” more clearly.
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© 2001 Springer Science+Business Media Dordrecht
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Miroshnichenko, L.I. (2001). Interactions of Accelerated Particles with the Solar Atmosphere. In: Solar Cosmic Rays. Astrophysics and Space Science Library, vol 260. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9646-6_6
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DOI: https://doi.org/10.1007/978-94-015-9646-6_6
Publisher Name: Springer, Dordrecht
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