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Estimate of plasma parameters in a coronal loop by means of a fiber burst

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Abstract

Analyzing a fiber burst occurring in the event on 19 August, 1981, plasma parameters of the burst source volume are estimated by means of Kuijpers' (1975) fiber burst model. The derived height dependence of the density in a coronal loop agrees with an isothermal barometric loop atmosphere.

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Authors and Affiliations

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

    H. Aurass, J. Kurths & G. Mann

  2. IZMIRAN, 142 092, Moscow Region, U.S.S.R.

    G. P. Chernov

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

    M. Karlický

Authors
  1. H. Aurass
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  2. J. Kurths
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  3. G. Mann
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  4. G. P. Chernov
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  5. M. Karlický
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Aurass, H., Kurths, J., Mann, G. et al. Estimate of plasma parameters in a coronal loop by means of a fiber burst. Sol Phys 108, 131–137 (1987). https://doi.org/10.1007/BF00152082

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  • DOI: https://doi.org/10.1007/BF00152082

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