Unraveling the influence of deep geodynamic processes on the Earth's surface stress field is critical for understanding the driving forces of tectonic deformation. To date, it is well-established that there are two main sources of stress in the lithosphere: (a) internal buoyancy forces arising from lateral density and thickness variations within the crust and lithospheric mantle (Lachenbruch & Morgan, 1990;Lachenbruch et al., 1985), and (b) vertical and horizontal basal tractions arising from buoyancy-driven mantle convection below the lithosphere (Hager et al., 1985;Steinberger et al., 2001). Stresses are continuous across plate boundaries and are not generated there. While substantial work has been done to define the kinematics of these two sources, their relative contribution on both the long-term stability of continents and their state of stress is largely unknown. Here, we investigate how mantle-based stresses affect the dynamics of the lithosphere through the analysis of crustal anisotropy.In general, the difficulty of elucidating the origin of lithospheric stresses stems from our imperfect knowledge of the physical properties of the crust and the lack of constrains on the degree of coupling between the tectonic plates and the convective flow of the mantle. Over the last few decades, numerous studies have aimed at constraining the mechanical structure of the crust. These efforts typically involve the modeling of the Earth's topographic response to tectonic loading (e.g., Kaufman & Royden, 1994;Wdowinski & Axen, 1992) or the use of seismic data (e.g., Schutt et al., 2018) to derive estimates of crustal viscosity and temperature. Findings show, for instance, that there can exist large compositional lateral variations across a single craton (e.g., Tesauro et al., 2014), and that certain regions around the world have the conditions for the lower crust to act as a weak viscous layer capable of accommodating the lateral pressure gradients within the lithosphere (e.g., Bird, 1991;Block & Royden, 1990). Methods