Interpretation of the fine spectral structure during solar flare microwave radio emission

Astronomy and Astrophysics – Astronomy

Scientific paper

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Beam Injection, Microwave Emission, Solar Flares, Solar Flux Density, Solar Radio Bursts, Solar Spectra, Solar Wind, Coronal Loops, Electron Beams, Fine Structure, Ion Acoustic Waves, Magnetohydrodynamic Turbulence

Scientific paper

Characteristic features of the plasma model of radio emission from the extending fronts of the solar flare energy release are studied. Formation of the electron distribution near the thermal fronts is shown to have the character of stationary beam injection through a boundary into the cold plasma semispace. In quasi-linear approximation the plasma wave accumulation before the thermal fronts is typical of this case. The radio flux density from this region can reach essential value in the relative narrow frequency band. Possibilities of the flare loop structure analysis based on the narrow band emission parameters are shown.

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