太阳风的外流和色球磁网
1Southwest Research Institute, 1050 Walnut Street, Boulder, CO 80302, USA. Max-Planck-Institut fur Aeronomie, D-37191 Katlenburg-Lindau, Germany. Institut d'Astrophysique Spatiale, Unite Mixte CNRS- Universite Paris XI, 91405 Orsay, France. Ins.
概括
太阳风起源于冠状孔中的特定区域,与色球磁网相连. 这些发现提高了对太阳风的理解.
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:
- 冠状孔是太阳冠状的开放磁场线的区域.
- 了解太阳风的起源对于太空天气预报至关重要.
- 之前的观测缺乏在冠状基础上的详细速度映射.
研究的目的:
- 为了研究外流速度与冠冕底部的磁性结构之间的关系.
- 为了确定太阳风的特定来源区域.
- 为了提高对冠状动态的理解.
主要方法:
- 使用太阳和日球观测站 (SOHO) 航天器.
- 创建了Ne7+的速度图,使用其在770安格斯特罗姆的共振线.
- 与染色球磁性网络结构相关的外流速度.
主要成果:
- 冠状孔的外流速度与染色球磁网有明显的关系.
- 太阳风似乎起源于沿磁网络细胞边界和交叉点的局部区域.
- 观察到大量的外流速度标志,与这个网络结构有关.
结论:
- 太阳风植根于冠状基础上的色球磁网中.
- 沿磁网边界的局部区域是太阳风的关键来源区域.
- 这些发现为太阳风起源的动态提供了新的见解.
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