arXiv · 1404.2148
Energy spectrum of Buoyancy-driven Flows
Abstract
Using high-resolution direct numerical simulation and arguments based on the kinetic energy flux $Π_u$, we demonstrate that for stably stratified flows, the kinetic energy spectrum $E_u(k) \sim k^{-11/5}$, the entropy spectrum $E_θ(k) \sim k^{-7/5}$, and $Π_u(k) \sim k^{-4/5}$ (Bolgiano-Obukhov scaling). This scaling is due to the depletion of kinetic energy because of buoyancy. For weaker buoyancy in stratified flows, $E_u(k)$ follows Kolmgorov's spectrum with a constant energy flux. We also argue that for Rayleigh Bénard convection, the Bolgiano-Obukhov scaling will not hold for the bulk flow due to the positive energy supply by buoyancy and non-decreasing $Π_u(k)$.
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Abhishek Kumar, Anando G. Chatterjee, Mahendra K. Verma. 2014-04-08. Energy spectrum of Buoyancy-driven Flows. https://arxiv.org/abs/1404.2148
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