相关实验视频
Updated: Jul 9, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
半阴色染色体中的小规模喷气状特征
Y Katsukawa1, T E Berger, K Ichimoto
1National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan. yukio.katsukawa@nao.ac.jp
概括
科学家们在太阳黑子中发现了微小的,快速移动的射流,称为半阴微射流. 这些喷气,可能来自磁重新连接,可能会在太阳黑子上方加热太阳冠状.
科学领域:
- 太阳物理 太阳物理
- 天文学 天文学
- 等离子体物理学的物理学
背景情况:
- 太阳黑子在其半阴影中表现出复杂的磁场.
- 染色体喷流是太阳大气层中观察到的动态现象.
研究的目的:
- 为了识别和描述太阳黑斑染色体中的微型喷射状特征.
- 调查这些微喷气的起源和潜在影响.
主要方法:
- 使用Hinode卫星上的太阳光学望远镜观测太阳黑子.
- 通过Ca II H线过器捕获的图像序列的分析.
主要成果:
- 发现半暗微喷气,其宽度为400公里,持续时间不到1分钟.
- 这些特征很难用现有的观测能力来检测.
结论:
- 半阴微喷气可能起源于太阳黑子复杂磁场内的磁再连接.
- 这些微型喷气有可能导致太阳黑子以上的冠状热.
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