210 research outputs found

    Sheared Rayleigh-Bénard Turbulence

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    On the Applicability of Low-Dimensional Models for Convective Flow Reversals at Extreme Prandtl Numbers

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    Constructing simpler models, either stochastic or deterministic, for exploring the phenomenon of flow reversals in fluid systems is in vogue across disciplines. Using direct numerical simulations and nonlinear time series analysis, we illustrate that the basic nature of flow reversals in convecting fluids can depend on the dimensionless parameters describing the system. Specifically, we find evidence of low-dimensional determinism in flow reversals occurring at zero Prandtl number, whereas we fail to find such signatures for reversals at infinite Prandtl number. Thus, even in a single system, as one varies the system parameters, one can encounter reversals that are fundamentally different in nature. Consequently, we conclude that a single general low-dimensional deterministic model cannot faithfully characterize flow reversals for every set of parameter values.Comment: 9 pages, 4 figure

    Phenomenology of buoyancy-driven turbulence: Recent results

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    In this paper, we review the recent developments in the field of buoyancy-driven turbulence. Scaling and numerical arguments show that the stably-stratified turbulence with moderate stratification has kinetic energy spectrum Eu(k)∼k−11/5E_u(k) \sim k^{-11/5} and the kinetic energy flux Πu(k)∼k−4/5\Pi_u(k) \sim k^{-4/5}, which is called Bolgiano-Obukhov scaling. The energy flux for the Rayleigh-B\'{e}nard convection (RBC) however is approximately constant in the inertial range that results in Kolmorogorv's spectrum (Eu(k)∼k−5/3E_u(k) \sim k^{-5/3}) for the kinetic energy. The phenomenology of RBC should apply to other flows where the buoyancy feeds the kinetic energy, e.g. bubbly turbulence and fully-developed Rayleigh Taylor instability. This paper also covers several models that predict the Reynolds and Nusselt numbers of RBC. Recent works show that the viscous dissipation rate of RBC scales as ∼Ra1.3\sim \mathrm{Ra}^{1.3}, where Ra\mathrm{Ra} is the Rayleigh number
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