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
先金星探测器在金星云中发现了显著的温度和压力变化,表明强烈的区域风和大气不稳定. 这些发现凸显了金星上复杂的大气动态.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 维纳斯探索 维纳斯探索
背景情况:
- 金星拥有密集的大气层,复杂的云层.
- 之前的任务提供了关于金星大气结构和动态的有限数据.
研究的目的:
- 为了分析来自Pioneer金星探测器的温度和压力概况.
- 为了研究金星大气中的大气动力学和云特性.
主要方法:
- 使用四个先金星探测器下降测量温度和压力.
- 分析海拔概况以确定变化和大气现象.
主要成果:
- 在金星云层 (45-61公里高度) 中观察到显著的温度和压力差异.
- 高度探测器记录了25 K的较低温度和高达49 mbar的较低压力.
- 区域风力计算在40-60公里之间,有非轴对称风组成部分的证据.
- 金星云比预期的温度高10到20克,中层云层是对流不稳定的.
- 在云层上方的失效率急剧下降,在100公里处观察到叠加的波.
结论:
- 观察到的压力差异支持强带风的周期性平衡.
- 云的升温和不稳定性归因于吸收的热辐射.
- 云层以上的大气结构显示出明显的平流层特征.
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