在太阳突出处等离子体的部分电离
Petr Heinzel1,2, Stanislav Gunár1, Sonja Jejčič1,3
1Astronomical Institute of the Czech Academy of Sciences, Ondřejov 25165, The Czech Republic.
概括
太阳突出等离子是部分电离,主要是由周围辐射的光电离,而不仅仅是温度和密度. 了解这一点需要复杂的辐射转移建模,以准确研究太阳大气层.
科学领域:
- 血物理学的等离子体物理学
- 太阳大气物理 太阳大气物理
- 原子和分子物理学 原子和分子物理学
背景情况:
- 太阳突出部分是部分电离的等离子体结构.
- 电离度通常取决于等离子体温度,密度和特定的离子.
- 以前的模型经常简化了电离机制.
研究的目的:
- 为了确定冷的太阳突出核心中主要的电离机制.
- 通过散射辐射来研究光电离的作用.
- 在非平衡条件下分析和等关键物种的电离.
主要方法:
- 解决非LTE (非局部热力学平衡) 辐射转移问题.
- 通过来自周围太阳大气层的辐射对光电离的建模.
- 分析,和其他物种的电离.
主要成果:
- 辐射扩散的光电离是冷突出核中部分电离的主要驱动因素.
- 电离度对发生辐射场非常敏感.
- 非平衡的电离效应是显著的,并影响血成分.
结论:
- 精确建模太阳突出电离需要详细的辐射转移解决方案.
- 光电离是部分电离太阳等离子体中至关重要的,经常占主导地位的过程.
- 了解这些过程对于推进太阳大气研究至关重要.
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