Studies at the McMath-Hulbert Observatory of Radio Frequency Radiation at the Time of Solar Flares

Details Studies at the McMath-Hulbert Observatory of Radio Frequency Radiation at the Time of Solar Flares Studies at the McMath-Hulbert Observatory of Radio Frequency Radiation at the Time of Solar Flares

Jan 1958

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1958pire...46..149d&link_type=abstract

Proceedings of the IRE, vol. 46, issue 1, pp. 149-159

Computer Science

4

Scientific paper

The complex flare phenomenon is described in terms of its photographic aspect on Hα spectroheliograms, associated prominence activity, terrestrial effects, and the general pattern of radio frequency emission. Flare-associated events at 2800 and 200 mc are reviewed, and the association between flares and the onset of 200-mc noise storms is discussed. Records of 2800 and 200-mc radiation at the time of 277 flares are compared. Flare-events at frequencies less than 200 mc are considered, and a study of 496 flares at 80 mc is summarized.

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