Large-scale vortices in rapidly rotating Rayleigh–Bénard convection
By C. Guervilly, D. Hughes, Chris A. Jones. Journal of Fluid Mechanics, 2014
139 citations recorded by the source corpus.
Abstract Using numerical simulations of rapidly rotating Boussinesq convection in a Cartesian box, we study the formation of long-lived, large-scale, depth-invariant coherent structures. These structures, which consist of concentrated cyclones, grow to the horizontal scale of the box, with velocities significantly larger than the convective motions. We vary the rotation rate, the thermal driving and the aspect ratio in order to determine the domain of existence of these large-scale vortices (LSV). We find that two conditions are required for their formation. First, the Rayleigh number, a measure of the thermal driving, must be several times its value at the linear onset of convection; this corresponds to Reynolds numbers, based on the convective velocity and the box depth, $\def \xmlpi #1{}\def \mathsfbi #1{\boldsymbol {\mathsf {#1}}}\let \le =\leqslant \let \leq =\leqslant \let \ge =\geqslant \let \geq =\geqslant \def \Pr {\mathit {Pr}}\def \Fr {\mathit {Fr}}\def \Rey {\mathit {Re}}{\gtrsim }100$ . Second, the rotational constraint on the convective structures must be strong. This requires that the local Rossby number, based on the convective velocity and the horizontal convective scale, ${\lesssim }0.15$ . Simulations in which certain wavenumbers are artificially suppressed in spectral space suggest that the LSV are produced by the interactions of small-scale, depth-dependent convective motions. The presence of LSV significantly reduces the efficiency of the convective heat transport.
Subfields: Computational Mechanics, Computer Networks and Communications
View Paper: https://www.semanticscholar.org/paper/77d443107f0e4c5cc840f1f48a32f9108e066ccc
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In Computational Mechanics
Citations in the corpus
- Rotating convective turbulence in Earth and planetary cores (2015, background): “Indeed, turbulent exchanges can still occur between small-scale inertial flows and large scale axialized modes (e.g., Julien et al., 2012b; Favier et al., 2014; Guervilly et al., 2014; Stellmach et al., 2014).”