Characteristics of radio emission of solar white-light flares; moving type IV bursts and short-term pulsations with associated post-flare loops.

Astronomy and Astrophysics – Astronomy

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Solar Flares: Solar Radio Bursts

Scientific paper

The white-light flares (WLFs) associated with radio moving type IV bursts and post-flare loops and their accompanied radio short-term pulsations are relatively rare. So far their relations have not been sufficiently investigated in literature. In this paper a complicated solar activity on June 6, 1991 is analyzed. It includes a WLF in the impulsive phase of the flare (from Beijing Observatory), a moving type IV burst (from Yunnan Observatory) and multiple radio pulsations with periods of about 1 - 4s with a time resolution of 1 ms at two frequencies. The characteristics of radio emission associated with the WLF are studied.

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