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


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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.

作者简介

N. Shefov

Institute of Atmospheric Physics

Email: anasemenov@yandex.ru
俄罗斯联邦, Pyzhevskii per. 3, Moscow, 119017

A. Semenov

Institute of Atmospheric Physics

编辑信件的主要联系方式.
Email: anasemenov@yandex.ru
俄罗斯联邦, Pyzhevskii per. 3, Moscow, 119017

I. Medvedeva

Institute of Solar–Terrestrial Physics, Siberian Branch

Email: anasemenov@yandex.ru
俄罗斯联邦, Lermontova ul. 126a, Irkutsk, 664033

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