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

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

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...46..437f&link_type=abstract

Solar Physics, vol. 46, Feb. 1976, p. 437-446.

Physics

17

Electron Flux Density, High Energy Electrons, Radiant Flux Density, Solar Electrons, Type 3 Bursts, Data Correlation, Radiation Measurement, Radio Observation, Solar Physics, Thresholds

Scientific paper

We compare the flux of fast solar electrons and the intensity of the type III radio emission generated by these particles at 1 AU. We find that there are two regimes in the generation of type III radiation: one where the radio intensity is linearly proportional to the electron flux, and the second regime, which occurs above a threshold electron flux, where the radio intensity is proportional to the approximately 2.4 power of the electron flux. This threshold appears to reflect a transition to a different emission mechanism.

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