Microwave activities associated with McMath regions 14943 and 14979

Mathematics

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Microwave Emission, Solar Activity Effects, Solar Radio Bursts, Microwave Spectra, Polarimetry, Radiant Flux Density, Solar Magnetic Field, Spectroheliographs, Superhigh Frequencies

Scientific paper

The paper presents polarimetric and east-west scan data on microwave burst activity associated with the solar McMath regions 14943 and 14979 for the period September and October 1977. It was found that the latitude of the active region is low and its polarity is reversed from what would be expected for cycle 21, while its activity is high and caused several large bursts. The activity was divided into two phases and the frequency spectra of the burst which occurred during these two phases were divided into two groups. This division may be caused by changes in the intensity and/or morphology of the magnetic field.

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