High time resolution observational characteristics of solar radio radiation at four frequencies: evidence for the energy release of microflares.

Details High time resolution observational characteristics of solar radio radiation at four frequencies: evidence for the energy release of microflares. High time resolution observational characteristics of solar radio radiation at four frequencies: evidence for the energy release of microflares.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acasn..37..187x&link_type=abstract

Acta Astron. Sin., Vol. 37, No. 2, p. 187 - 200

Statistics

Solar Flares: Radio Radiation, Solar Microwave Bursts: Structure

Scientific paper

As the evidence for the energy release of microflares, the high time resolution observational characteristics of solar radio emission obtained from "synchronous observation system of solar radio radiation with high time resolution at four frequencies" (1.42, 2.13, 2.84 and 4.26 GHz) are presented. It includes the weak radio ms spikes, spike-like, fast pulsations and two kinds of new fast fine structures - microwave type III bursts and microwave patch-like structures. The statistics of durations of fast fine structures (1989.12 - 1993.4) is shown. The various types of phenomena are presented with examples based on the statistics.

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