自从毛恩德最小期以来,太阳大规模磁场的演变
S K Solanki1, M Schüssler, M Fligge
1Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany. solanki@linmpi.mpg.de
Nature
|December 2, 2000
概括
太阳的磁场表现出11年的周期和长期变化. 一个新的模型解释了最近行星间磁场强度的翻倍,将其与太阳黑子周期变化联系起来.
科学领域:
- 太阳物理 太阳物理
- 太空物理学 太空物理学
- 天体物理学 天体物理学
背景情况:
- 太阳的磁场表现出周期性行为,特别是11年的太阳黑子周期.
- 世俗变化和历史事件,如马恩德最小值,表明长期的磁场变化.
- 行星间磁场强度在过去一个世纪中意外地翻了一番.
研究的目的:
- 为了调查最近太阳行星间磁场强度翻一番的原因.
- 开发一个模型来解释太阳大规模磁场的长期演变.
- 探索太阳黑子周期长度与世俗磁场变化之间的关系.
主要方法:
- 太阳大规模磁场演变的计算模型的开发.
- 模拟了几个世纪以来的长期磁场变化.
- 分析模型的输出,以确定太阳周期参数与行星间场强度之间的相关性.
主要成果:
- 拟议的模型成功地复制了在过去100年中观测到的行星间磁场强度的翻倍.
- 该模型表明,太阳黑子周期的持续时间与磁场的世俗变化之间存在直接联系.
- 这项研究为最近行星间磁场强度的增加提供了潜在的解释.
结论:
- 太阳磁场的长期演变与太阳黑子周期密切相关.
- 太阳磁场的长期变化可以解释观测到的行星间磁场强度的增加.
- 这项研究为了解太阳磁场动态及其对日球的影响提供了一个新的框架.
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