在太阳冠冕中存在小规模扭曲阿尔弗温波的证据
R J Morton1, Y Gao2,3, E Tajfirouze1,4
1School of Engineering, Physics and Mathematics, Northumbria University, Newcastle, UK.
概括
太阳的外层大气层,即冠状,是连续的扭曲阿尔弗文波的宿主. 这些波扭曲了磁场线,并可能有助于为安静的太阳和太阳风提供动力.
科学领域:
- 太阳物理 太阳物理
- 等离子体天体物理学
背景情况:
- 太阳王冠是太阳的外层大气层,其特点是热血流入行星间空间作为太阳风.
- 推动太阳风的能量和动量转移机制仍在争论中.
- 扭曲的阿尔夫恩波是一种受欢迎的机制,特别是在不均的等离子体流量管中.
研究的目的:
- 为了研究静止的太阳冠冕中小规模扭曲阿尔夫恩波的存在和特征.
- 确定这些波在冠状体内的能量和动量转移中的潜在作用.
主要方法:
- 利用来自丹尼尔·K·伊诺耶太阳望远镜的Cryo-NIRSP仪器的高空间和光谱分辨率的冠状观测.
- 分析数据以识别和测量静止冠状的波幅和特性.
主要成果:
- 这项研究提供了证据,证明在静止的太阳冠冕中不断存在扭曲的阿尔夫恩波.
- 这些波表现出磁场线的扭动运动.
- 测量的波幅虽然很小,但由于视线整合,可能被低估.
结论:
- 这些发现证实,静止的冠状体支持扭曲的阿尔弗文波.
- 这些波是安静的太阳和太阳风的能源预算的一个重要因素.
- 结果突出了阿尔弗文波在冠状动力学和太阳风加速中的重要性.
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