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Polar motion prediction using the combination of SSA and Copula-based analysis

Authors :
Sadegh Modiri
Santiago Belda
Robert Heinkelmann
Mostafa Hoseini
Harald Schuh
José M. Ferrándiz
Universidad de Alicante. Departamento de Matemática Aplicada
Geodesia Espacial y Dinámica Espacial
Source :
RUA. Repositorio Institucional de la Universidad de Alicante, Universidad de Alicante (UA), Earth, Planets and Space, Earth Planets and Space, Earth, Planets and Space, Vol 70, Iss 1, Pp 1-18 (2018), Earth, Planets, and Space

Abstract

The real-time estimation of polar motion (PM) is needed for the navigation of Earth satellite and interplanetary spacecraft. However, it is impossible to have real-time information due to the complexity of the measurement model and data processing. Various prediction methods have been developed. However, the accuracy of PM prediction is still not satisfactory even for a few days in the future. Therefore, new techniques or a combination of the existing methods need to be investigated for improving the accuracy of the predicted PM. There is a well-introduced method called Copula, and we want to combine it with singular spectrum analysis (SSA) method for PM prediction. In this study, first, we model the predominant trend of PM time series using SSA. Then, the difference between PM time series and its SSA estimation is modeled using Copula-based analysis. Multiple sets of PM predictions which range between 1 and 365 days have been performed based on an IERS 08 C04 time series to assess the capability of our hybrid model. Our results illustrate that the proposed method can efficiently predict PM. The improvement in PM prediction accuracy up to 365 days in the future is found to be around 40% on average and up to 65 and 46% in terms of success rate for the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\hbox{PM}}_{x}$$\end{document}PMx and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\hbox{PM}}_{y}$$\end{document}PMy, respectively.

Details

Language :
English
ISSN :
18805981
Volume :
70
Issue :
1
Database :
OpenAIRE
Journal :
Earth, Planets and Space
Accession number :
edsair.doi.dedup.....930d7f36ada0ee88ada1351e17a88136
Full Text :
https://doi.org/10.1186/s40623-018-0888-3