title: Energy spectrum of buoyancy-driven turbulence.
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)∼k(-11/5), the potential energy spectrum E(θ)(k)∼k(-7/5), and Π(u)(k)∼k(-4/5) are consistent with the Bolgiano-Obukhov scaling. This scaling arises due to the conversion of kinetic energy to the potential energy by buoyancy. For weaker buoyancy, this conversion is weak, hence E(u)(k) follows Kolmogorov's spectrum with a constant energy flux. For Rayleigh-Bénard convection, we show that the energy supply rate by buoyancy is positive, which leads to an increasing Π(u)(k) with k, thus ruling out Bolgiano-Obukhov scaling for the convective turbulence. Our numerical results show that convective turbulence for unit Prandt number exhibits a constant Π(u)(k) and E(u)(k)∼k(-5/3) for a narrow band of wave numbers.
authors.affiliation: Department of Physics, Indian Institute of Technology Kanpur, Kanpur, India 208016.
authors.forename: Abhishek
authors.initials: A
authors.lastname: Kumar
authors.affiliation: Department of Physics, Indian Institute of Technology Kanpur, Kanpur, India 208016.
authors.forename: Anando G
authors.initials: AG
authors.lastname: Chatterjee
authors.affiliation: Department of Physics, Indian Institute of Technology Kanpur, Kanpur, India 208016.
authors.forename: Mahendra K
authors.initials: MK
authors.lastname: Verma
mesh_terms: D003198:Computer Simulation; D019277:Entropy; D007700:Kinetics; D008962:Models, Theoretical; D009038:Motion; D013696:Temperature