“…Mass motion and redistribution in geophysical fluids excite Earth's wobbles and length‐of‐day changes with varying efficacy on different time scales. While atmospheric contributions to these rotational fluctuations are relatively well determined through reanalysis data sets (Bizouard & Seoane, 2010; Gross et al., 2003, 2004; Neef & Matthes, 2012; Schindelegger et al., 2013), uncertainties increase as one invokes—apart from the somewhat elusive core processes (Kuang et al., 2019; Mound, 2005; Pais & Hulot, 2000)—oceanic (Harker et al., 2021; Marcus et al., 1998; Ponte et al., 1998; Quinn et al., 2019; Zhou et al., 2005), hydrological (Adhikari & Ivins, 2016; Meyrath & van Dam, 2016; Nastula et al., 2019), and cryospheric (J. L. Chen, Wilson, et al., 2013; Göttl et al., 2021) effects in the planet's angular momentum budget. Here we are primarily concerned with modeling the non‐tidal oceanic component in polar motion and length‐of‐day excitations, on time scales from a few days out to several years.…”