太阳的产生和随后的大气加热
Tanmoy Samanta1, Hui Tian2, Vasyl Yurchyshyn3
1School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China.
概括
由磁场相互作用所驱动的小太阳喷气被称为尖. 这些事件与太阳的上层大气层加热有关.
科学领域:
- 太阳物理
- 等离子天体物理学
- 磁动力学
背景情况:
- 在太阳染色体中观察到的精细等离子喷射是动态的.
- 脊柱的起源和大气加热作用尚不清楚.
- 对于了解太阳大气动态至关重要.
研究的目的:
- 为了研究太阳的起源.
- 在太阳大气中的作用.
- 探索磁场动力学与螺纹形成之间的关系.
主要方法:
- 用大熊太阳天文台的古德太阳望远镜进行观测.
- 分析磁流的出现和螺纹活动.
- 使用太阳动力学天文台的数据与太阳冠热相关联.
主要成果:
- 在相反极性的磁流出现后不久,
- 在较低的太阳大气层中观察到磁场相互作用,
- 太阳冠状体的升温事件是在状物出现后被检测到的.
结论:
- 部分电离的太阳大气中的磁场动态会产生螺纹.
- 的产生与太阳冠状的升温有关.
- 这项研究提供了太阳大气加热的机制.
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