相关实验视频
Updated: Jul 12, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
概括
从地面对金星的近红外观测揭示了独特的云的特征和运动. 不同的旋转周期表明,这些特征是在金星大气中不同高度形成的.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 金星科学 金星科学
背景情况:
- 金星的夜侧大气表现出动态云的特征.
- 了解这些特征对于大气动力学研究至关重要.
研究的目的:
- 分析金星夜侧近红外标记的形态和运动.
- 用地面观测来调查大气动力学和云的高度.
主要方法:
- 1990年1月至2月利用来自全球地面天文台网络的近红外图像.
- 分析了利略与金星相遇之前,期间和之后的云形态,范围和旋转周期.
主要成果:
- 一个持久的低度黑云 (旋转周期为5.5天) 被观察到.
- 在低度的较小标记显示了不同的旋转周期 (7.4天),表明高度不同.
- 中度有明亮的波段,而高度是黑暗的,没有特征,表明高不透明度.
- 水蒸气分布在较低大气层中没有显著的水平梯度.
结论:
- 金星云层特征的独特旋转周期表明不同的形成高度.
- 高度的黑暗表明,在更高的海拔上,云的不透明度更大.
- 下层大气层在水蒸气含量上看起来相对均.
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