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Occurrence of solar decimetric spike bursts over a period of 4 years during the 21st cycle

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Abstract

A total number of 460 DCIM events, single or groups, were observed during the period of October 1980 to December 1984 with the Weissenau spectrograph as dynamic film spectra. Several parameters describing these data were evaluated statistically and the main features were discussed in context with associated burst types.

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References

  • Markeev, A. K., Styazhkin, V. A., and Chertok, I. M.: 1972, Soviet Astron. 15, 995.

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  • Urbarz, H. W.: 1980–1984, Institute Bulletin, Weissenau.

  • Wiehl, H. J., Benz, A. O., and Aschwanden, M. J.: 1985, Solar Phys. 95, 210.

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Authors and Affiliations

  1. Astronomical Institute of Tuebingen University, Weissenau Station, F.R.G.

    H. W. Urbarz

Authors
  1. H. W. Urbarz
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Additional information

Proceedings of the Workshop on Radio Continua during Solar Flares, held at Duino (Trieste), Italy, 27–31 May, 1985.

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Urbarz, H.W. Occurrence of solar decimetric spike bursts over a period of 4 years during the 21st cycle. Sol Phys 104, 125–129 (1986). https://doi.org/10.1007/BF00159953

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  • DOI: https://doi.org/10.1007/BF00159953

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