On the question of solar flare site in the active region.

Physics

Scientific paper

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Solar Flares: Solar Radio Bursts

Scientific paper

The site of the solar flares in the active region has been estimated in a statistical way. The correlation coefficient between the integrated flare intensity in Hα and the peak flux of the associated radio burst has been found out for various observed frequencies of radio emission. The aforesaid coefficient is found to peak around 2 - 4 GHz at which the flare-burst association is found to be maximum, giving rise to the fact that most of the Hα flare onset takes place in the region of 2 - 4 GHz radio emission.

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