A theoretical model and radioburst-proton flux spectral correlations for U-shaped solar flare radio bursts

Details A theoretical model and radioburst-proton flux spectral correlations for U-shaped solar flare radio bursts A theoretical model and radioburst-proton flux spectral correlations for U-shaped solar flare radio bursts

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975bc...repts....k&link_type=abstract

Final Report, Aug. 1971 - Jul. 1975 Boston Coll., Chestnut Hill, MA. Dept. of Physics.

Physics

Solar Flares, Solar Radio Emission, Astronomical Models, Extraterrestrial Radio Waves, Flux Density, Mathematical Models, Protons, Solar Radiation

Scientific paper

A theoretical model for the explanation of the origin of U-shaped solar burst spectra was developed. The model is based on the concept of one single group of radiating electrons, whose low frequency radiation is enhanced by the ambient magnetoplasma. Model spectra were computer generated. The conversion of the radiated waves, their propagation through and escape from the solar corona were considered and demonstrated.

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