太阳冠状环的无衰减曲振荡的极化
Sihui Zhong1, Valery M Nakariakov2,3, Dmitrii Y Kolotkov1,4
1Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry, CV4 7AL, UK.
Nature communications
|September 12, 2023
概括
在太阳冠冕中,无衰变的扭曲振荡显示了水平线性极化. 这一发现支持准稳定流作为冠状热的能源.
科学领域:
- 太阳物理 太阳物理
- 等离子体天体物理学
- 冠状元的动态 冠状元动态
背景情况:
- 太阳冠状体等离子环中的无衰减曲振荡是太阳和恒星冠状体加热问题的潜在解决方案.
- 振荡偏振提供了关于激发机制和能量供应的关键信息,但很难明确确定.
研究的目的:
- 为了确定无衰变的扭曲振荡的偏振.
- 研究振荡偏振对冠状热机制的影响.
主要方法:
- 使用两个非平行视线,同时观察4分钟无衰变的扭曲振荡.
- 利用太阳轨道器上的高分辨率成像仪 (HRI) 和太阳动力学天文台 (SDO) 上的大气成像组件 (AIA) 的数据.
- 观察数据与各种极化类型的前建模的比较.
主要成果:
- 从两条相距很远的视线成功同时检测出无衰变的扭曲振荡.
- 揭示了振荡的水平或弱斜线性偏振.
- 观察到的两极分化与特定的前建模场景是一致的.
结论:
- 没有衰变的扭曲振荡的确定偏振有利于通过近乎稳定的流动实现可持续性.
- 几乎稳定的流量可能是导致冠状热的能源来源.
- 这项研究为了解太阳冠状热提供了关键证据.
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