Physics
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111..347g&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 111, no. 2, 1987, p. 347-363.
Physics
13
Electron Energy, Particle Acceleration, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Type 3 Bursts, Decametric Waves, Electromagnetic Spectra, Electron Acceleration, Kinetic Energy
Scientific paper
The results of a study of the evolution of the February 3, 1986 flare at meter-decameter wavelengths are presented, using the two-dimensional imaging observations made with the Clark Lake multifrequency radioheliograph. The flare was complex and produced various types of meter-decameter bursts. The preflare activity was observed in the form of type III bursts some tens of minutes prior to the impulsive onset. From the positional analysis of the preflare and impulsive phase type III bursts and other measured characteristics, the characteristics of energy release and possible magnetic field configurations in the vicinity of the energy release region are discussed. From positional and temporal studies of the flare continuum and type II burst in relation to the microwave and hard X-ray emissions, the possible magnetic field structures in which the accelerated particles are confined or along which they propagate are discussed; a schematic model of the flaring region is developed, based upon this study.
Gopalswamy Nat
Kundu Mukul R.
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