On two formulations of polar motion and identification of its sources
F. Lopes, V. Courtillot, JL. Le Mou\"el, and D Gibert

TL;DR
This paper compares two formulations of celestial mechanics equations for polar motion, revealing a strong link between Earth's rotation variations and external astronomical forces, with implications for understanding Earth's rotational dynamics.
Contribution
It demonstrates the equivalence of classical and modern formulations of Earth's polar motion equations and highlights the astronomical origins of observed variations.
Findings
Strong correlation between Earth's polar motion and planetary torques.
Identification of nine physical components in length of day variations.
Evidence of a link between Earth's rotation and extraterrestrial periodicities.
Abstract
Differences in interpretation may arise from differences in formulation of the equations of celestial mechanics. This paper focuses on the Liouville system of differential equations. In a "modern" presentation of the equations, variations in polar motion (PM) and variations in length of day (lod) are decoupled. Their source terms result from redistribution of masses and torques. Elasticity of the Earth, large earthquakes, or external forcing by the fluid envelopes have been successively invoked in the "modern" approach. In the "classical" presentation, PM is governed by the inclination of Earth's rotation pole and the derivative of its declination (close to the derivative of lod). These are coupled by the Liouville system and all "source" terms are astronomical. The "classical" approach also implies that there should be a link between the rotations and the torques exerted by the planets…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Solar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies
