The Great Solar Radio Burst of may 23, 1967
John P. Castelli, J. Aarons, Glen A. Michael
Abstract
John P. Castelli, J. Aarons, Glen A. Michael
Abstract
On May 23, 1967, a solar radio burst was observed that was one of the largest ever recorded; it was associated with an Importance 2B flare. Using high-accuracy flux-density measurements at five fre- quencies ranging from 606 to 8800 MHz, its flux-density spectrum was compared with spectra of other flares observed in white light. It was found that along with most of the other white-light flares it dis- played the U-type flux-density spectrum, i.e, high flux density in the meter and centimeter range and lower flux density in the decimeter range. The flare produced a PCA
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On May 23, 1967, a solar radio burst was observed that was one of the largest ever recorded; it was associated with an Importance 2B flare. Using high-accuracy flux-density measurements at five fre- quencies ranging from 606 to 8800 MHz, its flux-density spectrum was compared with spectra of other flares observed in white light. It was found that along with most of the other white-light flares it dis- played the U-type flux-density spectrum, i.e, high flux density in the meter and centimeter range and lower flux density in the decimeter range. The flare produced a PCA
Key concepts: Physics, Flux (metallurgy), Solar flare, Astrophysics, Solar radio, Flare, Astronomy, White light