相关实验视频
Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
利略紫外线光谱仪实验:初始的金星和行星间巡航结果
概括
利略号航天器检测到金星大气中的,电离氧和原子排放. 星际原子主导莱曼-α排放,太阳流量因太阳周期和旋转而变化.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 频谱学是一种光谱学.
背景情况:
- 金星拥有复杂的大气层,各种元素和电离成分.
- 太阳风和星际介质相互作用显著影响行星外层.
研究的目的:
- 用极端紫外线光谱学分析金星的大气排放.
- 调查太阳系里莱曼-阿尔法辐射的来源和变化.
主要方法:
- 使用利略极端紫外光谱仪捕获光谱.
- 在55.0至125.0纳米波长范围内观察到的排放,分辨率为3.5nm.
- 在太阳最大值期间建模了利略观测结果.
主要成果:
- 检测到来自 (58.4 nm),电离原子氧 (83.4 nm) 和原子 (121.6 nm) 的排放.
- 观察到原子 (莱曼-β) 和原子氧 (102.5 nm) 的混合特征.
- 确定星际原子是莱曼-α发射的主要来源,并注意到太阳流变化.
结论:
- 利略的观测提供了有关金星上层大气层的详细光谱数据.
- 星际原子在太阳系的莱曼-α排放中起着至关重要的作用.
- 太阳活动显著影响莱曼-α流量,显示与太阳周期和旋转的变化.
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