Solar radio signatures suggestive of proton beams

Details Solar radio signatures suggestive of proton beams Solar radio signatures suggestive of proton beams

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.320..508b&link_type=abstract

Nature (ISSN 0028-0836), vol. 320, April 10, 1986, p. 508, 509.

Physics

9

Plasma Frequencies, Proton Beams, Solar Corona, Solar Protons, Solar Radio Bursts, Flow Velocity, Plasma Radiation

Scientific paper

Electron beams propagating in the solar corona excite the ambient plasma to emit radio waves at the local plasma frequency and/or its harmonic. This general interpretation of type III radio bursts is well confirmed by in situ measurements. The rate at which peak flux drifts in frequency and time is a measure of the velocity of the exciter. The authors report a class of radio bursts with a significantly lower drift than normal. Possible exciters are slowly moving beams of protons.

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