Turbulent stirring in the ocean disperses tracers and suspended material over time. The eddies, jets, and fronts that characterize this turbulent motion occur at a range of spatial and temporal scales. Since ocean models have a finite resolution, structures with spatial s cales of the order of the grid resolution or smaller are not resolved explicitly. Current state-of-the-art global ocean models use nominal 1/48° grid resolutions (Fox-Kemper et al., 2019;Su et al., 2018), resolving the mesoscale and part of the submesoscale spectrum. Still, computational constraints limit the simulation length of models at such resolutions to only a few years. Many of the latest generation of Earth system models that are used for CMIP6 use ocean grid resolutions of 1° and 1/4° (Hewitt et al., 2020). The models at 1° do not resolve any mesoscale eddies. While the 1/4° models are eddy-permitting in parts of the ocean, much higher resolutions are required to resolve the first baroclinic Rossby radius at higher latitudes, such