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Flares of radio type II and coronal emission in the course of cycle No 20

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Abstract

The butterfly diagram was constructed for the coronal emission of Fe XIV line (530.3 nm) in the course of cycle 1965–1976 complemented with the positions of the source flares with coronal shock waves.

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Authors and Affiliations

  1. Astronomical Institute, Czechoslovak Academy of Sciences, 251 65, Ondřejov, Czechoslovakia

    L. Křiyský

  2. Astronomical Institute, Slovak Academy of Sciences, 059 60, Tatranská Lomnica, Czechoslovakia

    M. Rybanský & V. Rušín

Authors
  1. L. Křiyský
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  2. M. Rybanský
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  3. V. Rušín
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Křiyský, L., Rybanský, M. & Rušín, V. Flares of radio type II and coronal emission in the course of cycle No 20. Sol Phys 133, 399–402 (1991). https://doi.org/10.1007/BF00149898

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