Abstract

Dynamical Modeling and Excitation Reconstruction as Fundamental of Earth Rotation Prediction Though pure mathematical approximations such as regression models and neural networks show good results in Earth rotation forecasting, dynamical modeling remains the only base for the physically meaningful prediction. That assumes the knowledge of cause-effect relationships and physical model of the rotating Earth. Excitation reconstruction from the observed Earth orientation parameters (EOP) is a crucial stage, needed for comparison with known causes, such as tidal forcing, atmospheric (AAM), oceanic (OAM) angular momentum changes, and uncovering unknown ones. We demonstrate different approaches, which can be used to avoid ill-conditionality and amplification of noises during the inversion. We present amplitude and phase studies of the model and reconstructed excitations of Chandler wobble. We found out, that modulation of Chandler excitation is synchronous with 18-yr tidal effects in the Earth's rotation rate changes. The results of the study can be used for excitation and EOP forecast. The key issues of the EOP prediction are discussed.

Highlights

  • The results of the Earth orientation parameters (EOP) PCC have shown, that various mathematical methods of EOP prediction compete with each other at approximately equal level, but the best results are given by the methods based on the physical modeling of the Earth's rotation

  • The following key issues related to the EOP prediction by means of physical modeling can be raised

  • The problem of the Earth's rotation dynamical modeling and excitation functions reconstruction was raised by Jereys (1940) among the rst

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Summary

INTRODUCTION

The results of the EOP PCC have shown, that various mathematical methods of EOP prediction compete with each other at approximately equal level, but the best results are given by the methods based on the physical modeling of the Earth's rotation. They use dynamical model and involve a number of additional data about the processes that cause variations in the rotation velocity and orientation of the poles of the planet. Physical models are based on the identied cause-eect relationships, they have mathematical representation, possibly with fewer parameters They should explain observations and have a predictive power.

SINGUALAR SPECTRUM ANALYSIS OF POLAR MOTION
DYNAMICAL MODELLING AND EXCITATION RECONSTRUCTION
CHANDLER EXCITATION STUDY
CONCLUSIONS
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