Filling the gap in the IERS C01 polar motion series in 1858.9-1860.9
This paper addresses the two-year gap in the pole coordinate of the IERS C01 polar motion series (1858.9–1860.9) by comparing a parametric astronomical model with a data-driven Singular Spectrum Analysis (SSA) approach, ultimately recommending the SSA method as preferable due to its more complete modeling of polar motion.