相关实验视频
Updated: Jul 9, 2026

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
染色体 Alfvenic 波的强度足以为太阳风提供动力
B De Pontieu1, S W McIntosh, M Carlsson
1Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Organization ADBS, Building 252, Palo Alto, CA 94304, USA. bdp@lmsal.com
概括
在太阳的染色层中检测到强烈的阿尔夫文波,为太阳风加速和冠状热提供了潜在的解释. 这些观测弥合了理解太阳大气动态的关键差距.
科学领域:
- 太阳物理 太阳物理
- 等离子体物理学的物理学
- 天体物理学 天体物理学
背景情况:
- 理论上说,阿尔夫文波可以加热太阳的冠状和加速太阳风.
- 在太阳大气层中缺乏足够强大的阿尔夫恩波的直接观测.
研究的目的:
- 研究太阳大气中的阿尔弗文波的存在和特征.
- 为了确定观察到的阿尔夫文波是否具有足够的能量来进行冠状热和太阳风加速.
主要方法:
- 利用来自Hinode卫星上的太阳光学望远镜的高时间和空间分辨率图像.
- 分析了染色体内的波形特性,即太阳表面和冠状之间的一层.
主要成果:
- 检测到Alfvén波具有显著的幅度 (10-25公里/秒) 和周期 (100-500秒) 透染色体.
- 估计了这些波带来的能量流.
结论:
- 观测到的阿尔夫文波具有足够的能量,有可能加速太阳风.
- 这些波也可能有助于加热安静的太阳冠状.
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