Relationship between the north–south asymmetry of sunspot formation and the amplitude of 11-year solar activity cycles
- 作者: Latyshev S.V.1, Olemskoy S.V.1
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隶属关系:
- Institute of Solar–Terrestrial Physics
- 期: 卷 42, 编号 7 (2016)
- 页面: 488-494
- 栏目: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/189762
- DOI: https://doi.org/10.1134/S1063773716060025
- ID: 189762
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详细
A relationship between the north–south asymmetry of sunspot formation and the amplitude of 11-year cycles has been established from the RGO/USAF/NOAA data on sunspots. It is shown that the higher the solar cycle amplitude, the smaller the absolute value of the north–south asymmetry. The revealed pattern has been investigated in a numerical dynamo model with irregular variations of the alpha-effect.
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作者简介
S. Latyshev
Institute of Solar–Terrestrial Physics
Email: osv@iszf.irk.ru
俄罗斯联邦, Irkutsk, 664033
S. Olemskoy
Institute of Solar–Terrestrial Physics
编辑信件的主要联系方式.
Email: osv@iszf.irk.ru
俄罗斯联邦, Irkutsk, 664033
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