Radio observations of the solar neutron flare of 3 June, 1982

Astronomy and Astrophysics – Astronomy

Scientific paper

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Neutron Flux Density, Radio Astronomy, Solar Corpuscular Radiation, Solar Flares, Solar Neutrons, Stellar Spectrophotometry, Electron Acceleration, Electron Density (Concentration), Shock Wave Propagation, Spectrum Analysis, Stellar Mass Ejection, Type 4 Bursts

Scientific paper

In this paper the solar neutron and white-light flare is studied on the basis of radioastronomical observations. It is shown that the 3 June, 1982 flare had an impulsive character. A strong shock wave (MA ≥ 2.9) was observed unusually soon after the impulsive phase of the flare. The radio spectrum of this event shows that the primary acceleration process probably occurred in the region with an electron density of ne = 4.4×1015m-3. The pulsations of the type IV radio burst, observed 15 min after the mass ejection process, manifest the reconnection process in the post-flare stage.

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