Observations of an unusual pair of homologous flares on March 17, 1970

Physics

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Solar Flares, Solar Physics, Solar Radio Emission, Solar X-Rays, H Alpha Line, Homology, Solar Electrons, Solar Radio Bursts, Solar Spectra, Sunspots

Scientific paper

Correlated optical, radio and X-ray observations are presented for a pair of 'consequently' homologous flares which occurred on March 17, 1970. A rich complexity of behavior in a bright sub-flare with maximum at 14:44 UT is repeated in a flare of importance 1B with maximum at 22:49 UT. The unusual and interesting aspect of these flares is that the second flare developed at approximately half the rate of the first. A difference in the trigger mechanism of the two flares is suggested as a possible explanation.

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