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Radio observations of the solar neutron flare of 3 June, 1982

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Abstract

In this paper the solar neutron and white-light flare is studied on the basis of radioastronomical observations. It is shown that the 3 June, 1982 flare had an impulsive character. A strong shock wave (M A ≥ 2.9) was observed unusually soon after the impulsive phase of the flare. The radio spectrum of this event shows that the primary acceleration process probably occurred in the region with an electron density of n e = 4.4 × 1015 m−3. The pulsations of the type IV radio burst, observed 15 min after the mass ejection process, manifest the reconnection process in the post-flare stage.

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Authors and Affiliations

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

    M. Karlický

  2. Zentralinstitut für Astrophysik der Akademie der Wissenschaften der DDR, Observatorium für solare Radioastronomie, 1501, Tremsdorf, D.D.R.

    H. Aurass & G. Mann

Authors
  1. M. Karlický
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  2. H. Aurass
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  3. G. Mann
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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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Karlický, M., Aurass, H. & Mann, G. Radio observations of the solar neutron flare of 3 June, 1982. Sol Phys 104, 165–168 (1986). https://doi.org/10.1007/BF00159957

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  • DOI: https://doi.org/10.1007/BF00159957

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