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地球在亚季节时间尺度上的角动量收支。

The Earth's Angular Momentum Budget on Subseasonal Time Scales.

出版信息

Science. 1992 Jan 17;255(5042):321-4. doi: 10.1126/science.255.5042.321.

Abstract

Irregular length of day (LOD) fluctuations on time scales of less than a few years are largely produced by atmospheric torques on the underlying planet. Significant coherence is found between the respective time series of LOD and atmospheric angular momentum (AAM) determinations at periods down to 8 days, with lack of coherence at shorter periods caused by the declining signal-to-measurement noise ratios of both data types. Refinements to the currently accepted model of tidal Earth rotation variations are required, incorporating in particular the nonequilibrium effect of the oceans. The remaining discrepancies between LOD and AAM in the 100- to 10-day period range may be due to either a common error in the AAM data sets from different meteorological centers, or another component of the angular momentum budget.

摘要

不规则的日长(LOD)波动在小于几年的时间尺度上主要是由大气扭矩对下伏行星产生的。在 8 天以下的周期内,LOD 和大气角动量(AAM)的时间序列之间存在显著的相关性,而在较短的周期内,由于两种数据类型的信噪比下降,相关性缺失。需要对目前接受的潮汐地球自转变化模型进行改进,特别是要纳入海洋的非平衡效应。在 100 到 10 天的周期范围内,LOD 和 AAM 之间的剩余差异可能是由于来自不同气象中心的 AAM 数据集的共同误差,或者是角动量预算的另一个组成部分。

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