The Second Waldmeier Rule and the Form of the 11-Year Cycle
- 作者: Ivanov V.G.1
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隶属关系:
- Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences
- 期: 卷 59, 编号 8 (2019)
- 页面: 1070-1074
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157962
- DOI: https://doi.org/10.1134/S0016793219080085
- ID: 157962
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详细
It is known that the form of the 11-year solar-activity cycle can be approximately described by its amplitude A and the arrangement of three characteristic moments: the moment of the minimum (Tmin), maximum (Tmax), and the subsequent minimum (Tmin2). According to the classical Waldmeier rule, there is an anticorrelation between the maximum activity value (amplitude) of cycle A and the duration of its ascending branch Tmax – Tmin, while the correlation between A and the length of the downward branch of the cycle Tmin2 – Tmax is much lower. Following Waldmeier, the moment TV can be entered near the end of the downward branch of the cycle, in which the activity falls within a certain (low) specified level V. The relationship between the length of the corresponding phase of cycle TV – Tmax and the amplitude of this cycle is quite strong. We demonstrate that this connection, which can be called the “second Waldmeier rule,” agrees well with the fact that the downward branch of the cycle has a universal appearance. Thus, one parameter, its value is at the maximum, is enough for an approximate qualitative description of the form of a single 11-year cycle that takes into account the two Waldmeier rules.
作者简介
V. Ivanov
Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences
编辑信件的主要联系方式.
Email: vg.ivanov@gaoran.ru
俄罗斯联邦, St. Petersburg
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