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Fast-moving radio sources in the solar atmosphere

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Abstract

This paper presents observations of the unusual phenomenon of fast-moving microwave sources using the Siberian solar radio telescope (SSRT). We observed two sources characterized by two features in common: the fast proper regular motion (with averaged velocity 180–200 km/s) and the long lifetime. By analyzing the instrumental and artificial interference, we conclude that the observed sources are of solar origin.

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References

  1. G. B. Gelfreikh, D. V. Korol'kov, G. Ya. Smol'kov, and G. A. Treskov, in:Observations and Research over the MGSS Period: Siberia and the Far East [in Russian], Nauka, Moscow (1967), No. 4, p. 168.

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Authors and Affiliations

  1. Institute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, Irkutsk

    D. V. Prosovetsky, B. I. Lubyshev, G. Ya. Smol'kov, T. A. Treskov, B. B. Krissinel & V. G. Miller

Authors
  1. D. V. Prosovetsky
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  2. B. I. Lubyshev
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  3. G. Ya. Smol'kov
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  4. T. A. Treskov
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  5. B. B. Krissinel
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  6. V. G. Miller
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Additional information

Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 39, Nos. 11–12, pp. 1466–1472, November–December, 1996.

This work was supported in part by the “Astronomiya” Foundation and the Russian Foundation for Fundamental Research.

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Prosovetsky, D.V., Lubyshev, B.I., Smol'kov, G.Y. et al. Fast-moving radio sources in the solar atmosphere. Radiophys Quantum Electron 39, 978–983 (1996). https://doi.org/10.1007/BF02250976

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  • DOI: https://doi.org/10.1007/BF02250976

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