“…Continuously advancing observations and modeling studies have led to remarkable progress in understanding the Cascadia megathrust and the processes of great subduction earthquakes (Walton et al., 2021; K. Wang & Tréhu, 2016). These observational and modeling advances include long‐term seismological and geodetic monitoring (e.g., Bartlow, 2020; Dragert et al., 2001; McCaffrey et al., 2013; McCrory et al., 2012; Rogers & Dragert, 2003; Stone et al., 2018; Toomey et al., 2014), lithospheric scale geophysical imaging (e.g., Audet & Schaeffer, 2018; Carbotte et al., 2022; Davis & Hyndman, 1989; Han et al., 2017; Nedimović et al., 2003; Yuan et al., 1994), paleo‐seismology and ‐tsunami studies of historical ruptures (e.g., Atwater et al., 1995; Goldfinger et al., 2012; Priest et al., 2010; P. L. Wang et al., 2013), laboratory studies of fault‐rock frictional properties (e.g., Ikari et al., 2009; Stanislowski et al., 2022), and modeling of the seismogenic extent constrained by thermal and/or deformation observations (e.g., Hyndman & Wang, 1993; Melgar et al., 2022; Schmalzle et al., 2014; K. Wang et al., 2003). Nonetheless, existing models of the Cascadia megathrust locking distribution are all constrained solely by land‐based GNSS measurements (Li et al., 2018; Pollitz & Evans, 2017; Schmalzle et al., 2014; K. Wang et al., 2003).…”