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
旅行者号对顿的观测显示了它的高邦德白度 (0.82±0.05),表明表面很亮. 这项研究使用Hapke的光度模型和大气雾数据来模拟Triton的光散射.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 摄影测量是一种摄影仪.
背景情况:
- 海王星最大的卫星顿 (Triton) 拥有稀薄的气氛.
- 旅行者号的观测提供了关键的数据,以了解顿的表面特性.
研究的目的:
- 为了估计顿的几何色度,相积和邦德色度.
- 为了模拟Triton大气层和表面的光散射.
- 研究大气组成和表面特性之间的关系.
主要方法:
- 哈普克的光度模型被应用于旅行者的整个磁盘观测.
- 一个平面平行的薄型大气雾模型被纳入.
- 分析了紫色,蓝色和绿色波长波段的数据.
主要成果:
- 在高相角的数据上升是由大气雾散射解释的.
- 雾的光学深度随着波长的增加而减少.
- 最适合的哈克参数产生了0.82 ± 0.05.05的邦德白度.
结论:
- 特里顿的高邦德白度表明它的表面非常明亮.
- 如果大气处于蒸汽平衡状态,波德的白度意味着表面发射率为0.59±0.16.
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