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Quasiperiodic oscillations in the atmospheres of the Sun, Earth, and planets

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Abstract

The published data on long-term observations on cycles of the activity of the Sun and stars of late spectral classes (F, G, K) were analyzed. Quasiperiodic oscillations (QPO) in solar activity with periods varying from 1.8 (7-year cycles) to 12.5 years (24-year cycles) were revealed for the first time. A high degree of correlation between QPO periods and long-term cycles of variations in the activity of the Sun and stars was revealed.

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Authors and Affiliations

  1. Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevskii per. 3, Moscow, 119017, Russia

    N. N. Shefov & A. I. Semenov

  2. Institute of Solar–Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, Lermontova ul. 126a, Irkutsk, 664033, Russia

    I. V. Medvedeva

Authors
  1. N. N. Shefov
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  2. A. I. Semenov
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  3. I. V. Medvedeva
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Corresponding author

Correspondence to A. I. Semenov.

Additional information

Original Russian Text © N.N. Shefov, A.I. Semenov, I.V. Medvedeva, 2016, published in Doklady Akademii Nauk, 2016, Vol. 468, No. 1, pp. 93–96.

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Shefov, N.N., Semenov, A.I. & Medvedeva, I.V. Quasiperiodic oscillations in the atmospheres of the Sun, Earth, and planets. Dokl. Earth Sc. 468, 490–492 (2016). https://doi.org/10.1134/S1028334X1605007X

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  • DOI: https://doi.org/10.1134/S1028334X1605007X

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