概括
旅行者2号的图像揭示了海王星上持久的云层特征,旋转周期在15.8至18.4小时之间. 云顶风速在金星到海王星之间是相似的,尽管太阳能输入的巨大差异.
科学领域:
- 行星科学 行星科学
- 大气动力学 大气动力学
- 海王星研究 海王星研究
背景情况:
- 海王星的大气表现出动态云的特征.
- 以前的研究表明大气旋转周期有所变化.
研究的目的:
- 分析海王星云层特征的旋转周期和风速.
- 为了比较整个太阳系内部和外部的大气动力学.
主要方法:
- 来自旅行者2号的窄角摄像头图像的分析.
- 计算云特征旋转周期的计算.
- 计算相对于行星内部旋转周期的风速.
主要成果:
- 在海王星上确定了大规模的,持久的云层特征.
- 这些特征的确定的旋转周期从15.8到18.4小时不等.
- 计算的云顶风速从东向20米/秒到西向325米/秒.
结论:
- 海王星的大气表现出复杂的动态,有不同的旋转周期.
- 海王星上的云顶风速与金星的风速相当,尽管太阳能输入量有1000倍的差异.
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