Quantitative comparisons of type 3 radio burst intensity and fast electron flux at 1 AU

Details Quantitative comparisons of type 3 radio burst intensity and fast electron flux at 1 AU Quantitative comparisons of type 3 radio burst intensity and fast electron flux at 1 AU

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7611985f&link_type=abstract

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Comparison, Flux (Rate), High Energy Electrons, Solar Electrons, Type 3 Bursts, Electron Flux Density, Radio Emission, Thresholds

Scientific paper

The flux of fast solar electrons and the intensity of the type 111 radio emission generated by these particles were compared at one AU. Two regimes were found in the generation of type 111 radiation: one where the radio intensity is linearly proportional to the electron flux, and another, which occurs above a threshold electron flux, where the radio intensity is approximately proportional to the 2.4 power of the electron flux. This threshold appears to reflect a transition to a different emission mechanism.

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