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Optical counterpart of the radio event accompanying the 3B flare of 13 May 1981

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Abstract

Excepting intermittent type III activity, all the radio events over the frequency range 8–8000 MHz accompanying the initial stage of the 3B flare of 13 May, 1981 had their onset in a 2-min interval immediately preceding the peak of an impulsive Hα brightening (kernel) well away from the main flare. This kernel is identified as one footpoint of a loop of magnetic flux whose other end terminated in a transient brightening in an adjacent active region.

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Authors and Affiliations

  1. CSIRO Division of Applied Physics, 2070, Sydney, Australia

    R. E. Loughhead & Wang Jia-Long

  2. CSIRO Division of Radiophysics, 2121, Sydney, Australia

    R. A. Duncan

Authors
  1. R. E. Loughhead
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  2. Wang Jia-Long
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  3. R. A. Duncan
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On leave from the Bei**g Astronomical Observatory, Academia Sinica, Bei**g, China.

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Loughhead, R.E., Jia-Long, W. & Duncan, R.A. Optical counterpart of the radio event accompanying the 3B flare of 13 May 1981. Sol Phys 83, 257–266 (1983). https://doi.org/10.1007/BF00148279

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  • DOI: https://doi.org/10.1007/BF00148279

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