冠状暗变以及它们告诉我们关于太阳和恒星冠状质量喷射的信息
Astrid M Veronig1,2, Karin Dissauer3, Bernhard Kliem4
1Institute of Physics, University of Graz, Universitätsplatz 5, 8010 Graz, Austria.
概括
冠状暗变,观察到太阳辐射突然减少,是冠状质量喷射 (CME) 的关键指标. 本综述综合了当前的知识,提出了新的分类,并探讨了它们在了解太阳和恒星喷发中的用途.
科学领域:
- 太阳物理 太阳物理
- 恒星天体物理学 恒星天体物理学
- 等离子体物理学的物理学
背景情况:
- 冠状暗变是EUV和SXR波长中观察到的太阳辐射的突然,局部下降.
- 首次在20世纪90年代末观察到,它们与冠状质量喷射 (CME) 的升起和膨胀相有关.
- 它们被解释为喷发的流动绳的足迹和冠状质量损失的指标.
研究的目的:
- 审查当前对冠状暗射的理解和观察结果.
- 探索光,CME模拟和触发机制之间的关系.
- 引入新的物理驱动的调光分类,并讨论它们对恒星CME的应用.
主要方法:
- 来自SOHO/EIT和Yohkoh/SXT仪器的观测数据的审查.
- 对CME模拟的分析及其与调暗观测的相关性.
- 基于磁流系统的冠状暗变的新型分类方案的开发.
主要成果:
- 冠状暗射提供了关于CME触发,磁连接和冠状重构的见解.
- 基于磁流系统的新分类提供了对调暗物理学的更深入的理解.
- 研究扩展了对光的分析到类似太阳的和晚期类型的恒星,以诊断恒星CME.
结论:
- 冠状暗变对于理解CME和太阳爆发的动态至关重要.
- 拟议的分类增强了对太阳和恒星现象的诊断能力.
- 对恒星变暗的进一步研究可以阐明系外行星CME的特性.
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