Abstract
Fifteen examples of quasi-periodic 2.8 GHz burst emission observed at the La Posta Astrogeophysical Observatory during the period 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.
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Cliver, E.W., Hurst, M.D., Wefer, F.L. et al. Quasi-periodic burst structure at 2.8 GHz and its relationship to burst morphological parameters. Sol Phys 48, 307–320 (1976). https://doi.org/10.1007/BF00151998
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DOI: https://doi.org/10.1007/BF00151998