Multi-parameter Polar Motion Prediction Based on Effective Angular Momentum Function

Q4 Physics and Astronomy Chinese Astronomy and Astrophysics Pub Date : 2022-10-01 DOI:10.1016/j.chinastron.2022.11.009
ZHAO Xin , WU Yuan-wei , YANG Xin-yu , YANG Xu-hai , ZHANG Shou-gang
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Abstract

The change of polar motion is closely related to a variety of excitations. These excitations include atmospheric surface pressure and atmospheric wind, seabed pressure and ocean currents, land water distribution, and sea level changes caused by climate warming, and can be estimated by the effective angular momentum function. In the polar motion prediction, the effective angular momentum function is included through the Liouville equation, and combined the least square and autoregressive method for data fitting and extrapolation. At the same time, more options are set for the adjustable parameters of the autoregressive model. In different phases of polar motion prediction, the predictions of each components are matched with optimized parameters, which effectively improves the prediction accuracy of polar motion. In 441 polar motion prediction experiments from 1 to 90 days, the short and medium term predictions were improved more obviously. In the 1–6 day and 7–30 day of the polar motion X (PMX) prediction results, there were 56.9% and 53.5% respectively better than the IERS (International Earth Rotation Service) prediction; in the 1–6 day and 7–30 day of the polar motion Y (PMY) prediction results, 66.5% and 59.7% are better than the IERS prediction, respectively. In General, the performance of PMY prediction is better than that of PMX. Taking IERS EOP (Earth Orientation Parameters) C04 as a reference, the MAE (Mean Absolute Error) of the polar motion X prediction on the 1st-day and 5th-day is improved by 2.6% and 33.0%, respectively compared with the IERS prediction. Compared with the IERS prediction, the MAE of Y prediction on the 1st-day and 5th-day is improved by 20.8% and 49.0%, respectively.

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基于有效角动量函数的多参数极运动预测
极性运动的变化与各种激励密切相关。这些激励包括大气表面压力和大气风、海底压力和洋流、陆地水分布以及气候变暖引起的海平面变化,可以通过有效角动量函数来估计。在极运动预测中,通过Liouville方程引入有效角动量函数,并结合最小二乘法和自回归法进行数据拟合和外推。同时,为自回归模型的可调参数设置了更多的选项。在极运动预测的不同阶段,将各分量的预测结果与优化后的参数进行匹配,有效地提高了极运动预测的精度。在1 ~ 90 d的441次极移预报试验中,中短期预报的改善较为明显。极移X (PMX) 1 ~ 6天和7 ~ 30天的预报结果分别比IERS (International Earth Rotation Service)预报好56.9%和53.5%;极移Y (PMY)在1 ~ 6天和7 ~ 30天的预报结果中,分别优于IERS预报的66.5%和59.7%。总体而言,PMY的预测性能优于PMX。以IERS EOP (Earth Orientation Parameters) C04为参考,极移X第1天和第5天预报的MAE (Mean Absolute Error)分别比IERS预报提高了2.6%和33.0%。与IERS预测相比,Y预测第1天和第5天的MAE分别提高了20.8%和49.0%。
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来源期刊
Chinese Astronomy and Astrophysics
Chinese Astronomy and Astrophysics Physics and Astronomy-Astronomy and Astrophysics
CiteScore
0.70
自引率
0.00%
发文量
20
期刊介绍: The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.
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