Beat structure in pulsating type IV solar radio bursts and a possible mechanism

Details Beat structure in pulsating type IV solar radio bursts and a possible mechanism Beat structure in pulsating type IV solar radio bursts and a possible mechanism

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111..137l&link_type=abstract

(Observatoire de Paris, CNRS, CNES, et al., CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, 2nd, Aubigny-s

Physics

8

Periodic Variations, Solar Oscillations, Type 4 Bursts, Magnetic Field Configurations, Solitary Waves, Whistlers

Scientific paper

Pulsating type IV solar radio bursts with beat structure are presented and analyzed in this paper. Based upon the theory of whistler soliton emission, the beat structure is interpreted by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model.

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