概括
高分辨率望远镜和光谱仪的观测揭示了太阳宏观球的动态. 这项研究发现,过渡区的排放源自70公里以下宽的微型,次分辨率结构.
科学领域:
- 太阳物理 太阳物理
- 天文学 天文学
- 太空科学 太空科学
背景情况:
- 太阳染色层和过渡区是理解太阳活动至关重要的动态区域.
- 之前的观测缺乏空间和时间分辨率来分辨这些层内的细结构.
研究的目的:
- 为了研究太阳肢体上的宏观体的时间发育.
- 为了确定C IV过渡区的排放结构的特征尺度.
主要方法:
- 使用了高分辨率望远镜和光谱仪 (HRTS) 仪器.
- 在Spacelab-2航天飞机任务期间进行了扩展观测.
- 分析紫外线光谱图以捕获高空间和时间分辨率数据.
主要成果:
- 观察了太阳四肢上的宏观的时间演变.
- 在C IV过渡区内确定了离散的排放元素.
- 确定这些元素是由小于70公里的亚分辨率结构组成的.
结论:
- 宏观分子在太阳肢体表现出动态行为.
- C IV过渡区的排放不均,而是来自非常细的,未解决的结构.
- 这些发现为太阳大气层的微物理提供了新的见解.
相关概念视频
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