Quasiperiodic oscillations in the atmospheres of the Sun, Earth, and planets
- 作者: Shefov N.N.1, Semenov A.I.1, Medvedeva I.V.2
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隶属关系:
- Institute of Atmospheric Physics
- Institute of Solar–Terrestrial Physics, Siberian Branch
- 期: 卷 468, 编号 1 (2016)
- 页面: 490-492
- 栏目: Geophysics
- URL: https://ogarev-online.ru/1028-334X/article/view/188380
- DOI: https://doi.org/10.1134/S1028334X1605007X
- ID: 188380
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详细
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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