Numerical simulation of an asymptotically reduced system for rotationally constrained convection

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Dedalus: A flexible framework for numerical simulations with spectral methods (2019, background): “[93].”
Simulations of Dynamo Action in Fully Convective Stars (2007, background): “…recent numerical modeling and asymptotic analysis of unstratified turbulence has shown that a preference for one sign of vorticity, and hence a high net helicity, is established at moderate rotation rates with Ro ≈ 0.1 → 1, but eliminated as rotation becomes even more rapid (Sprague et al. 2006).”
Rotating convective turbulence in Earth and planetary cores (2015, methodology): “The asymptotically-reduced equations are modeled in rectilinear domains using a semi-implicit, spectral code, which employs a Fourier decomposition on horizontal planes and a Chebyshev decomposition in the vertical direction (Sprague et al., 2006; Grooms et al., 2010).”