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Manifestation of the 160-min solar oscillations in velocity and brightness (optical and radio observations)

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Abstract

All evidence of the solar origin of 160-min period oscillations is collected, and the present state of observations of this oscillation in optical and radio-ranges is considered. The main results are summarized: (a) the 160-min oscillation was observed in 1981 as well as before, (b) an attempt to find a nonradial component with l = 2 has failed, (c) the intensity and circular polarization of radioemission show with statistical significance the presence of this 160-min periodicity.

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Authors and Affiliations

  1. Crimean Astrophysical Observatory, 334413, Crimea, U.S.S.R.

    V. A. Kotov, A. B. Severny, T. T. Tsap, I. G. Moiseev, V. A. Efanov & N. S. Nesterov

Authors
  1. V. A. Kotov
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  2. A. B. Severny
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  3. T. T. Tsap
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  4. I. G. Moiseev
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  5. V. A. Efanov
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  6. N. S. Nesterov
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Additional information

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

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Kotov, V.A., Severny, A.B., Tsap, T.T. et al. Manifestation of the 160-min solar oscillations in velocity and brightness (optical and radio observations). Sol Phys 82, 9–19 (1983). https://doi.org/10.1007/BF00145541

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  • DOI: https://doi.org/10.1007/BF00145541

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