相关实验视频
Updated: Jul 11, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
金星的紫外线光谱:来自先驱金星轨道器的初步结果
概括
紫外线光谱仪在金星云层上方检测到二氧化硫 (SO2),揭示了大气和云层结构的不均性. 夜间的空气发光排放表明能量沉到热层.
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:
- 金星拥有充满活力的大气,复杂的云层结构.
- 了解大气组成和动态对于行星研究至关重要.
研究的目的:
- 用紫外线光谱学研究金星上层大气的组成.
- 通过分散的太阳光测量来分析云结构和大气动力学.
- 为了描述金星的外层温度和能量平衡.
主要方法:
- 紫外线光谱检测,以确定大气吸收特征.
- 对2663安格斯特罗姆的散射阳光进行分析,以探测云层结构.
- 在二氧化硫 (SO(2) 吸收波长的成像.
- 测量空气发光排放以确定外层温度.
主要成果:
- 在金星云顶上方发现了归因于二氧化硫 (SO(2) 的吸收特征.
- 观察到云结构中水平和垂直不均性的证据.
- 在SO(2) 波长的阿尔贝多特征与Mariner 10看到的相似.
- 外层温度估计大约为275K.
- 检测到一个夜间的空气发光辐射,这意味着能量沉.
结论:
- 在金星云层以上的大气中存在二氧化硫.
- 金星的云结构表现出显著的不均性.
- 能量沉在金星的黑暗热层中,正如夜间空气发光所证明的那样.
相关概念视频
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