相关实验视频
Updated: Jul 11, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
概括
原子跟踪月球大气层,在100公里以下被检测到. 观测显示,延伸到几个月球半径,主要是由太阳光子和风释放的,而不是微型石.
科学领域:
- 月球科学 月球科学
- 大气科学 大气科学
- 原子物理 原子物理
背景情况:
- 原子是月球外层的有效追踪剂,因为它在波长D(1) 和D(2) 的有效散射阳光.
- 在1988年以前的地球观测中,在100公里以下的海拔上检测到的密度低于50原子/厘米3.
研究的目的:
- 调查月球大气中的原子的分布和来源.
- 了解负责从月球表面释放的过程.
主要方法:
- 利用望远镜观测和冠状图技术来掩盖月球盘.
- 分析了月球周围原子的空间分布和密度.
主要成果:
- 证实了原子的存在,从月球延伸到几个月球半径.
- 在分布中证明了太阳顶点角度的依赖性.
- 发现100公里以下的密度小于50原子/厘米3.
结论:
- 高海拔月球的主要来源可能是太阳光子相互作用 (加热/喷射) 和太阳风的影响.
- 在更高的海拔地区,微型石轰炸并不是月球的主要来源.
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