On the generation of high-energy particles in solar flares

Physics

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Scientific paper

This paper discusses the relationship between some characteristics of microwave type IV radio bursts and solar cosmic ray protons of MeV energy. It is shown that the peak flux intensity of those bursts is almost linearly correlated with the MeV proton peak flux observed by satellites near the Earth and that protons and electrons would be accelerated simultaneously by a similar mechanism during the explosive phase of solar flares. sBrief discussion is given on the propagation of olar cosmic rays in the ssolar envelope after ejection from the flare regions. NASA Associate with University of Maryland.

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