Solar Radio Phenomena and their Physical Interpretation

Physics

Scientific paper

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Solar Activity, Solar Radio Bursts, Solar Flares, Energy Transfer, Type 4 Bursts, Type 2 Bursts, Solar Prominences, Sun, Storms, Solar Cosmic Rays, Plasma Heating, Particle Energy, Oscillations, Excitation

Scientific paper

Centimeter bursts and type 4 bursts are interpreted as synchrotron sradiation. Type 3 and type 2 bursts are probably due to excitation of soscillations of the coronal plasma by high energy particles. The sparticles that create type R are probably trapped in a magneto-dynamic swave. Radio storms are similarly due to particles ejected during an seruption and remaining-trapped for several days in the magnetic sconfigurations near the sun.

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