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      Layer formation in horizontally forced stratified turbulence: connecting exact coherent structures to linear instabilities

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      Journal of Fluid Mechanics
      Cambridge University Press (CUP)

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          Abstract

          We consider turbulence in a stratified ‘Kolmogorov’ flow, driven by horizontal shear in the form of sinusoidal body forcing in the presence of an imposed background linear stable stratification in the third direction. This flow configuration allows the controlled investigation of the formation of coherent structures, which here organise the flow into horizontal layers by inclining the background shear as the strength of the stratification is increased. By numerically converging exact steady states from direct numerical simulations of chaotic flow, we show, for the first time, a robust connection between linear theory predicting instabilities from infinitesimal perturbations to the robust finite-amplitude nonlinear layered state observed in the turbulence. We investigate how the observed vertical length scales are related to the primary linear instabilities and compare to previously considered examples of shear instability leading to layer formation in other horizontally sheared flows.

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          Most cited references52

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          The energy cascade in a strongly stratified fluid

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            Periodic motion embedded in plane Couette turbulence: regeneration cycle and burst

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              Scaling analysis and simulation of strongly stratified turbulent flows

              Direct numerical simulations of stably and strongly stratified turbulent flows with Reynolds number Re ≫ 1 and horizontal Froude number F h ≪ 1 are presented. The results are interpreted on the basis of a scaling analysis of the governing equations. The analysis suggests that there are two different strongly stratified regimes according to the parameter $\mathcal{R} \,{=}\, \hbox{\it Re} F^2_h\(. When \)\mathcal{R} \,{\gg}\, 1\(, viscous forces are unimportant and l v scales as l v ∼ U / N ( U is a characteristic horizontal velocity and N is the Brunt–Väisälä frequency) so that the dynamics of the flow is inherently three-dimensional but strongly anisotropic. When \)\mathcal{R} \,{\ll}\, 1\(, vertical viscous shearing is important so that \)l_v \,{\sim}\, l_h/\hbox{\it Re}^{1/2}\( ( l h is a characteristic horizontal length scale). The parameter \)\cal R\( is further shown to be related to the buoyancy Reynolds number and proportional to ( l O /η) 4/3 , where l O is the Ozmidov length scale and η the Kolmogorov length scale. This implies that there are simultaneously two distinct ranges in strongly stratified turbulence when \)\mathcal{R} \,{\gg}\, 1\(: the scales larger than l O are strongly influenced by the stratification while those between l O and η are weakly affected by stratification. The direct numerical simulations with forced large-scale horizontal two-dimensional motions and uniform stratification cover a wide Re and F h range and support the main parameter controlling strongly stratified turbulence being \)\cal R\(. The numerical results are in good agreement with the scaling laws for the vertical length scale. Thin horizontal layers are observed independently of the value of \)\cal R\( but they tend to be smooth for \)\cal R\( 1 small-scale three-dimensional turbulent disturbances are increasingly superimposed. The dissipation of kinetic energy is mostly due to vertical shearing for \)\cal R\( 1, the horizontal spectra of kinetic and potential energy exhibit an approximate k −5/3 h -power-law range and a clear forward energy cascade is observed.
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                Author and article information

                Journal
                applab
                Journal of Fluid Mechanics
                J. Fluid Mech.
                Cambridge University Press (CUP)
                0022-1120
                1469-7645
                December 10 2017
                October 26 2017
                December 2017
                : 832
                : 409-437
                Article
                10.1017/jfm.2017.661
                4e2abed3-8406-41fd-abbf-a33f46c1cfaf
                © 2017
                History

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