Sudden decrease of microwave solar radio emission

Physics

Scientific paper

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Microwave Emission, Radiant Flux Density, Solar Activity Effects, Solar Radio Emission, Microwave Interferometers, Polarimeters, Solar X-Rays, Very High Frequencies

Scientific paper

Total flux observations on the microwave solar radio emission sometimes show depressions after bursts or without bursts. These, classified as 'post burst decrease' or 'absorption', are gradual phenomena and the duration is usually more than an hour. In contrast to these phenomena, the authors found two sudden decreases of the total flux just before the bursts of July 21, 1978 and September 7-8, 1978. The durations were shorter than 10 minutes. The observational results are given which were obtained by four microwave polarimeters and two interferometers at Toyokawa. A preliminary interpretation is also given for the event of September 7-8, 1978 using the data of optical, soft X-ray and meter-wave observations.

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