概括
地球的旋转速度因大气角运动量交换而波动. 这些变化,通过无线电干扰测量和卫星激光测距来跟踪,显著影响一天的长度,特别是在厄尔尼诺事件期间.
科学领域:
- 地质物理学 地质物理学
- 天文学 天文学
- 大气科学 大气科学
背景情况:
- 地球的旋转表现出复杂的变化,包括在宇宙时间1 (UT1) 中的亚毫秒波动.
- 追踪这些变化对于理解地球系统动态和保持精确的计时至关重要.
研究的目的:
- 为了调查地球旋转和一天的长度短期变化的原因.
- 量化大气过程对地球自转速率的影响.
主要方法:
- 使用天文无线电干扰测量对地球旋转的分毫秒精度测量.
- 激光射程到LAGEOS卫星进行精确的地质测量.
- 观察到的地球旋转变化的比较与全球大气角运动量数据.
主要成果:
- 观察到的UT1波动在几周内达到了5毫秒.
- 发现日长变化与全球大气角度动量的变化之间存在很强的相关性.
- 大气和固体地球 (地幔) 之间的角动量交换被确定为周到多年时间尺度上旋转速率变化的主要驱动因素.
结论:
- 大气角运动量交换是影响地球自转速率在各种时间尺度上的变化的主要因素.
- 显著的地球旋转变化,包括一天长度的显著峰值,与1982-1983年强烈的厄尔尼诺现象有关.
- 这些发现突出了地球大气层和固体在调节其旋转中的相互联系.
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