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We present results from direct numerical simulations of rotating Rayleigh--B\'enard convection (RRBC), the quintessential paradigm for investigating buoyancy-driven rotating turbulence, at rather extreme values of the governing parameters and bounded by experimentally realizable no-slip boundary conditions. We provide a statistical characterization of the RRBC flow regimes that can be used as a framework for identification of these flow states in future experiments and simulations at even more extreme parameter values, and for extrapolation to geophysical and astrophysical flow systems.
Guzmán et al. (Thu,) studied this question.
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