Comments on the duration-peak-flux-density diagram for 2800 MHz solar bursts

Details Comments on the duration-peak-flux-density diagram for 2800 MHz solar bursts Comments on the duration-peak-flux-density diagram for 2800 MHz solar bursts

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jrasc..75...15c&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 75, Feb. 1981, p. 15-28.

Physics

Solar Flares, Solar Flux Density, Solar Protons, Solar Radio Bursts, Annual Variations, Frequency Response, H Alpha Line, Pulse Duration, Solar Physics

Scientific paper

The existence of an essentially two-pronged distribution in the duration-peak-flux-density scatter plot for simple 2800 MHz solar bursts (Covington and Harvey, 1958) was verified for a more recent data set. An investigation was made of events that fall between the impulsive and gradual rise and fall branches of the duration-peak-flux-density diagram. Such events are rare, with only 51 observed at Ottawa during the 11 year period studied. A relatively high percentage of these bursts were associated with proton flares. (This fact may aid in the prediction of some otherwise difficult-to-forecast proton events.) Smaller subgroups in the sample include bursts from behind-the-limb flares and events associated with 'spotless' flares (Dodson and Hedeman, 1970).

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