Interpretation of hard X-ray, γ-ray and microwave burst spectra on 27 April 1981.

Computer Science

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Solar Flares: Hard X Rays, Solar Flares: Gamma-Ray Spectra, Solar Flares: Microwave Spectra

Scientific paper

The authors analyse the variations of microwave, X-ray and γ-ray burst spectra with time on 27 April 1981. They compare spectral indices and time profiles of seven major pulses. The observational features may be explained in terms of the stochastic electron acceleration in the turbulent plasma and by an oscillating solution of the electron kinetic equation in a pulsed injection.

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