Relationship between the north–south asymmetry of sunspot formation and the amplitude of 11-year solar activity cycles


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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.

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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