Quasi-periodic burst structure at 2.8 GHz and its relationship to burst morphological parameters

Details Quasi-periodic burst structure at 2.8 GHz and its relationship to burst morphological parameters Quasi-periodic burst structure at 2.8 GHz and its relationship to burst morphological parameters

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...48..307c&link_type=abstract

Solar Physics, vol. 48, June 1976, p. 307-320.

Astronomy and Astrophysics

Astronomy

8

Microwave Emission, Radio Astronomy, Solar Radio Bursts, Annual Variations, Energy Spectra

Scientific paper

Fifteen examples of quasi-periodic 2.8-GHz burst emission observed during the period from December 1966 through May 1973 were identified. The periods of these events and those of 22 additional events previously reported in the literature were plotted against burst morphological parameters. The relationship between period and event energy was found to be considerably weaker than initially reported by Cribbens and Matthews (1969).

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