The harmonic structure of a type II burst on 12 May, 1983

Details The harmonic structure of a type II burst on 12 May, 1983 The harmonic structure of a type II burst on 12 May, 1983

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..379b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 129, Oct. 1990, p. 379-386.

Physics

7

Electron Cyclotron Heating, Harmonics, Solar Magnetic Field, Type 2 Bursts, Magnetic Flux, Solar Flares, Solar Protons, Sunspots

Scientific paper

During the May 12, 1983 type II radio burst, the fundamental and the second, third, and possibly fourth harmonics were observed. The emission on the first three harmonics starts almost simultaneously but ceases at different moments of time. The emission intensity of the third harmonic is much smaller than that of the fundamental and second harmonics. It is suggested that the emission is observed on the first harmonics of the electron-cyclotron frequency and originates in regions satisfying the conditions for double plasma resonance. The magnetic field estimated in these regions exceeds the generally accepted value by one order of magnitude.

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