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Updated: Jul 9, 2025

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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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研究太阳日冕旋转与磁场结构的关系
N B Xiang1,2, X H Zhao3, L H Deng4
1Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China. nanbin@ynao.ac.cn.
Scientific reports
|November 30, 2023
概括
太阳光谱辐射和磁元素影响冠状旋转. 不同的磁结构在太阳最大和最小活动期间主导旋转.
科学领域:
- 太阳物理 太阳物理
- 太空物理学 太空物理学
- 等离子体物理学的物理学
背景情况:
- 冠状旋转是太阳动力学的一个关键方面.
- 以前的研究表明,关于冠状元旋转速率的结果不一致.
- 了解磁场对冠状旋转的影响至关重要.
研究的目的:
- 为了研究冠状元旋转的时间变化.
- 分析冠状旋转和太阳磁场结构之间的关系.
- 为了解释之前的冠状旋转研究中的差异.
主要方法:
- 在特定波长间隔中利用每日太阳光谱辐射 (SSI).
- 分析了四种类型的太阳小规模磁性元素.
- 采用连续波形变换和皮尔森相关性分析.
主要成果:
- 确定了磁结构对整个太阳周期的冠状旋转变化的独特贡献.
- 在太阳最大值期间,[公式:参见文本]元素主要驱动旋转.
- 在太阳最小值期间,旋转受到[公式:参见文本]和[公式:参见文本]元素的联合作用的影响,随着活动减弱,[公式:参见文本]效应会增强.
结论:
- 不同的磁性结构在日冕旋转中起着不同的作用,这取决于太阳活动水平.
- 解释了之前的冠状旋转研究中不一致的发现.
- 提供了了解为什么冠状在旋转的速度比光球更快.
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