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.
Proceedings of the 66th IAU Colloqium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.
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© 1983 D. Reidel Publishing Co, Dordrecht, Holland, and Boston, U.S.A.
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Kotov, V.A., Severny, A.B., Tsap, T.T., Moiseev, I.G., Efanov, V.A., Nesterov, N.S. (1983). Manifestation of the 160-min Solar Oscillations in Velocity and Brightness (Optical and Radio Observations). In: Gough, D.O. (eds) Problems of Solar and Stellar Oscillations. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7088-5_2
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DOI: https://doi.org/10.1007/978-94-009-7088-5_2
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