Quasiperiodic structure of solar type IIId radio bursts with echo components.

Physics

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Solar Radio Bursts: Structure

Scientific paper

By solar observations with a UTR 2 antenna, the authors detected a new variety of type IIId radiation in which the narrow-band spectral elements have an explicit quasiperiodic structure and contain an additional component in the form of a triple echo. According to amplitude records at 25 MHz, the initial short radio burst looks like a weak precursor of a more powerful echo-like burst accompanied by a pair of final pulses which exceed slightly the background. Nine events of this kind were registered in August 19, 1992 during a type IIId noise storm related to the active region in the central heliolongitude sector. In each event, all the three time intervals between successive peaks of the complex amplitude-time profile were almost identical and were equal to 4.7, 5.1, and 5.7 s on the average. The discovery of a new complex variety of decameter type IIId radiation confirms the hypothesis of multiple quasiperiodic echoes after short radio bursts at the second harmonic of the local plasma frequency in the solar atmosphere.

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