解密太阳磁活动:关于太阳 "天气 "与 "气候 "耦合的一些(不受欢迎的)想法

Scott W. McIntosh, Robert J. Leamon
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引用次数: 0

摘要

太阳在一系列时间和空间尺度上表现出偶发性的磁活动激增,其中最突出的是太阳黑子产生的 11 年左右的变化。除了太阳黑子生成的大约 170 个(最小到最大)十年变化之外,还有一个较少被探索的准年变化,其幅度为 25-50 个太阳黑子/年。此外,太阳黑子数量还有一个较慢的周期,约为 80 年,变化幅度在 10-50 之间,通常被称为 "格莱斯伯格周期"。我们将利用一系列当代和历史观测数据来说明恒星周期性行为的这些要素,并提出一个假设,该假设可能为观测到的恒星 "气候"、"十年 "和 "季节 "磁场变化之间提供一致的物理联系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Deciphering Solar Magnetic Activity: Some (Unpopular) Thoughts On the Coupling of the Sun's "Weather" and "Climate"
The Sun exhibits episodic surges of magnetic activity across a range of temporal and spatial scales, the most prominent of which is the 11-ish year modulation of sunspot production. Beside the ~170 (min to max) decadal variation in sunspot production there is a less-explored quasi-annual variation in the range of 25-50 sunspots/year in magnitude. In addition, there is there is a slower, ~80 year period, 10-50 variation in the sunspot number, that is commonly referred to as the 'Gleissberg Cycle.' Using a suite of contemporary and historical observations we will illustrate these elements of our star's episodic behavior and present a hypothesis that may provide a consistent physical link between the observed 'climatic', 'decadal' and 'seasonal' magnetic variation of our star.
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