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
概括
海洋号10号探测到金星上层大气中的,,碳和氧,使用客观格子光谱仪. 初步分析表明,金星的外层温度为400K.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 频谱学是一种光谱学.
背景情况:
- 了解行星大气层的组成对于理解行星演变至关重要.
- 之前对金星上层大气层的研究范围和波长覆盖范围有限.
研究的目的:
- 为了测量金星在紫外线范围内的空气发光.
- 为了确定金星上层大气层的组成.
- 为了研究金星的外层温度.
主要方法:
- 在Mariner 10号航天器上使用了客观格子光谱仪.
- 在200至1700安格斯特罗姆波长范围内收集了空气发光数据.
主要成果:
- 在金星上层大气层中检测到大量的,,碳和氧原子.
- 初步的气数据显示,外层温度为400K.
- 观测到强烈的空气发光辐射长度为1350安格斯特罗姆,空间广泛,存在于白天和夜晚两侧.
结论:
- 金星的上层大气层含有大量的关键元素.
- 金星的外层温度估计在400K左右.
- 强烈的空气发光辐射的性质需要进一步调查.
相关概念视频
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