Abstract

AbstractThis study aims to improve the polar motion theory by developing refined frequency‐dependent transfer functions with the most current models for ocean tides, the Earth's rheology, and core‐mantle coupling. First, we present a power law for mantle anelasticity constrained by the Chandler period TCW and quality factor QCW and an empirical quasi‐fluid rheology model with a linear dependence on frequency, which is suitable for a period as long as ~18.6 years. Then we adopt the diurnal ocean tides from the International Earth Rotation and Reference Systems Service Conventions (2010), the long‐period ocean model of Dickman and Gross (2010), and the equilibrium ocean pole tide model of Desai (2002) to calculate the oceanic corrections to the Love numbers. Further, we present discussions on the geophysical and observational aspects of the Chandler period TCW and quality factor QCW, and provide preferred values and intervals for TCW and QCW, which allow us to place some constraints on the mantle anelasticity and core‐mantle coupling ratio ηCW. Although ηCW is affected by uncertainties in TCW and QCW, we find its real part should be around 2%–3% while its imaginary part might be only a few thousandths. Finally, the frequency‐dependent polar motion transfer functions T L and T NL are determined based on the models of frequency‐dependent Love numbers and core‐mantle coupling discussed above. Our transfer functions are related to the values of TCW and QCW, however, our analyses demonstrate that our transfer functions are rather stable and not sensitive to perturbations in TCW and QCW.

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