在接近太阳的太阳风中磁性回转器的属性
Samuel T Badman1, Naïs Fargette2,3, Lorenzo Matteini3
1Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA 02138 USA.
概括
帕克太阳探测器观察到的磁反转是太阳风常见的偏移. 这些阿尔夫尼克波动和相关的喷流对于理解内部日球和太阳风至关重要.
科学领域:
- 空间物理 空间物理
- 太阳物理 太阳物理
- 等离子体物理学的物理学
背景情况:
- 磁反转是太阳风的偏移,其中行星间磁场急剧折叠.
- 这些事件与阿尔夫尼克波动相关,并形成向外喷射,特别是在辐射背景场.
- 帕克太阳探测器透露,在0.3AU以内的日球内部,回转是无处不在的.
研究的目的:
- 审查磁性回调的现场测量,主要来自帕克太阳探测器.
- 讨论这些结构的识别和测量.
- 呈现观测性质并确定需要进一步研究的领域.
主要方法:
- 从帕克太阳探测器进行现场测量的审查.
- 分析磁场和速度数据以识别回调.
- 单个回调的特征及其集体排列成补丁.
主要成果:
- 磁反转几乎无处不在内部的日球.
- 交换机背表现出特有的速度喷射,并且与阿尔夫尼克波动有很好的相关性.
- 观测性质显示出共识和需要进一步调查的领域.
结论:
- 磁反转在太阳风动力学中起着重要作用.
- 需要进一步的研究才能充分了解它们的流行程度和影响.
- 确定了对未来研究的开放问题和建议.
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