<p dir="ltr">Supporting data for the paper "The cross-over from viscous to inertial lengthscales in rapidly-rotating convection" submitted to Geophysical Research Letters.</p><p dir="ltr">In this work we study rotating convection in planar and spherical geometries. We focus on the transition from viscously-dominated to inertia-dominated regimes, and in particular how this affects the typical lengthscale of the flow.</p><p dir="ltr">The deposit includes the key post-processed data input parameters and time-averaged output values for the simulations in:</p><ul><li>plane layer geometry.</li><li>quasi-geostrophic spherical geometry.</li></ul><p dir="ltr">Instruments, hardware and software used:</p><ol><li>Data in plane layer geometry were produced by the open-source Dedalus code (Burns et al 2020 DOI:<a href="https://doi.org/10.1103/PhysRevResearch.2.023068" rel="noreferrer" target="_blank">10.1103/PhysRevResearch.2.023068</a>)</li><li>Data in QG spherical geometry were produced by an in-house code (Guervilly et al. 2019 DOI:<a href="https://doi.org/10.1038/s41586-019-1301-5" rel="noreferrer" target="_blank">10.1038/s41586-019-1301-5</a>)</li></ol><p dir="ltr"><br></p>
Funding
A new model of the geodynamo: large-scale vortices in the Earth's core