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Analysis of 25 Years of Polar Motion Derived from the DORIS Space Geodetic Technique Using FFT and SSA Methods

机译:利用FFT和SSA方法分析DORIS空间大地测量技术得出的25年极地运动

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摘要

Polar motion (PM) has a close relation to the Earth’s structure and composition, seasonal changes of the atmosphere and oceans, storage of waters, etc. As one of the four major space geodetic techniques, doppler orbitography and radiopositioning integrated by satellite (DORIS) is a mature technique that can monitor PM through precise ground station positioning. There are few articles that have analyzed the PM series derived by the DORIS solution in detail. The aim of this research was to assess the PM time-series based on the DORIS solution, to better capture the time-series. In this paper, Fourier fast transform (FFT) and singular spectrum analysis (SSA) were applied to analyze the 25 years of PM time-series solved by DORIS observation from January 1993 to January 2018, then accurately separate the trend terms and periodic signals, and finally precisely reconstruct the main components. To evaluate the PM time-series derived from DORIS, they were compared with those obtained from EOP 14 C04 (IAU2000). The results showed that the RMSs of the differences in PM between them were 1.594 mas and 1.465 mas in the X and Y directions, respectively. Spectrum analysis using FFT showed that the period of annual wobble was 0.998 years and that of the Chandler wobble was 1.181 years. During the SSA process, after singular value decomposition (SVD), the time-series was reconstructed using the eigenvalues and corresponding eigenvectors, and the results indicated that the trend term, annual wobble, and Chandler wobble components were accurately decomposed and reconstructed, and the component reconstruction results had a precision of 3.858 and 2.387 mas in the X and Y directions, respectively. In addition, the tests also gave reasonable explanations of the phenomena of peaks of differences between the PM parameters derived from DORIS and EOP 14 C04, trend terms, the Chandler wobble, and other signals detected by the SSA and FFT. This research will help the assessment and explanation of PM time-series and will offer a good method for the prediction of pole shifts.
机译:极地运动(PM)与地球的结构和组成,大气和海洋的季节性变化,水的储藏等密切相关。作为四大空间大地测量技术之一,多普勒轨道成像和卫星综合定位(DORIS)是一项可以通过精确的地面站定位来监视PM的成熟技术。很少有文章详细分析了DORIS解决方案衍生的PM系列。这项研究的目的是评估基于DORIS解决方案的PM时间序列,以更好地捕获时间序列。本文使用傅里叶快速变换(FFT)和奇异频谱分析(SSA)分析了DORIS观测从1993年1月至2018年1月求解的25年PM时间序列,然后准确地分离了趋势项和周期信号,最后精确地重建主要组成部分。为了评估源自DORIS的PM时间序列,将其与从EOP 14 C04(IAU2000)获得的PM时间序列进行了比较。结果表明,它们之间的PM差异的RMS在X和Y方向分别为1.594 mas和1.465 mas。使用FFT进行频谱分析表明,年度摆动周期为0.998年,而钱德勒摆动周期为1.181年。在SSA过程中,经过奇异值分解(SVD)后,使用特征值和相应的特征向量重构时间序列,结果表明趋势项,年摆动和Chandler摆动分量得到了准确的分解和重构,并且分量重建结果在X和Y方向上的精度分别为3.858和2.387 mas。此外,测试还合理解释了DORIS和EOP 14 C04导出的PM参数之间的差异峰值,趋势项,Chandler摆动以及SSA和FFT检测到的其他信号。这项研究将有助于对PM时间序列的评估和解释,并将为极移预测提供良好的方法。

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