在8个月内观察太阳全球冠状磁场的演变
Zihao Yang1,2, Hui Tian1,3, Steven Tomczyk2,4
1School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China.
概括
这项研究展示了太阳冠状状体的114个新磁图, 这些观测为太阳磁场动态和能量储存提供了前所未有的洞察力.
科学领域:
- 太阳物理
- 磁动力学
- 血物理
背景情况:
- 太阳的冠状在磁场中储存能量, 驱动太阳喷发和等离子体加热.
- 之前的全球冠状磁场测量仅限于罕见的快照.
研究的目的:
- 提供全球冠状磁场的持续,长期观测.
- 确定磁场与高度的分布,并监测其随时间和度的演变.
主要方法:
- 使用升级的冠状多通道极光计 (UCOMP) 捕获114个磁图.
- 在太阳四肢上方观察全球冠状体大约8个月.
- 分析不同高度和度的磁场强度和分布.
主要成果:
- 测量的冠状磁场强度在1.05和1.60太阳半径之间,范围为<1到~20高斯.
- 通过多次太阳旋转观察磁场在不同度上的演变.
- 在冠状磁场测量中检测到活跃的长度.
结论:
- 这项研究为了解冠状磁场动态提供了全面的数据集.
- 冠状模型通常与观测一致,在高度地区发现差异.
- 这些发现增强了我们对太阳冠状体能量储存和释放机制的理解.
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