The sensitivity of rapidly rotating Rayleigh--Bénard convection to Ekman pumping
arXiv:1704.04696 · doi:10.1103/PhysRevFluids.2.094801
Abstract
The dependence of the heat transfer, as measured by the nondimensional Nusselt number , on Ekman pumping for rapidly rotating Rayleigh-Bénard convection in an infinite plane layer is examined for fluids with Prandtl number . A joint effort utilizing simulations from the Composite Non-hydrostatic Quasi-Geostrophic model (CNH-QGM) and direct numerical simulations (DNS) of the incompressible fluid equations has mapped a wide range of the Rayleigh number - Ekman number parameter space within the geostrophic regime of rotating convection. Corroboration of the - relation at from both methods along with higher covered by DNS and lower by the asymptotic model allows for this range of the heat transfer results. For stress-free boundaries, the relation has the dissipation-free scaling of for all . This is directly related to a geostrophic turbulent interior that throttles the heat transport supplied to the thermal boundary layers. For no-slip boundaries, the existence of ageostrophic viscous boundary layers and their associated Ekman pumping yields a more complex 2D surface in parameter space. For results suggest that the surface can be expressed as indicating the dissipation-free scaling law is enhanced by Ekman pumping by the multiplicative prefactor where . It follows for that the geostrophic turbulent interior remains the flux bottleneck in rapidly rotating Rayleigh-Bénard convection. For , where DNS and asymptotic simulations agree quantitatively, it is found that the effects of Ekman pumping are sufficiently strong to influence the heat transport with diminished exponent and .
arXiv comment9 pages, 14 figures
References in corpus (4)
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Cited by in corpus (6)
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- Effects of kinematic and magnetic boundary conditions on the dynamics of convection-driven plane layer dynamos
- Rigorous bounds on the heat transport of rotating convection with Ekman pumping