Stably stratified turbulence in the presence of large-scale forcing

TL;DR

This study uses high-resolution simulations to explore how stratification influences turbulence, revealing similarities in energy distribution and spectral behaviors across different stratification intensities, with implications for geophysical flows.

Contribution

The paper provides new insights into the spectral and energetic properties of stratified turbulence at high Reynolds numbers, highlighting the roles of buoyancy and Ozmidov scales.

Findings

Similar kinetic and potential enstrophy evolution in different stratification regimes

Potential to total energy ratio remains around 0.1 in both flows

Spectral slopes vary with angle and stratification strength, showing flat and power-law behaviors

Abstract

We perform two high resolution direct numerical simulations of stratified turbulence for Reynolds number equal to Re~25000 and Froude number respectively of Fr~0.1 and Fr~0.03. The flows are forced at large scale and discretized on an isotropic grid of 2048^3 points. Stratification makes the flow anisotropic and introduces two extra characteristic scales with respect to homogeneous isotropic turbulence: the buoyancy scale, L_B, and the Ozmidov scale, l_{oz}. The former is related to the number of layers that the flow develops in the direction of gravity, the latter is regarded as the scale at which isotropy is recovered. The values of L_B and l_{oz} depend on the Froude number and their absolute and relative size affect the repartition of energy among Fourier modes. By contrasting the behavior of the two simulated flows we identify some surprising similarities: after an initial transient the two flows evolve towards comparable values of the kinetic and potential enstrophy, and energy dissipation rate. Further similarities emerge at large scales: the same ratio between potential and total energy (~0.1) is spontaneously selected by the flows, and slow modes grow monotonically in both regimes causing a slow increase of the total energy in time. The axisymmetric total energy spectrum shows a wide variety of spectral slopes as a function of the angle between the imposed stratification and the wave vector. One-dimensional energy spectra computed in the direction parallel to gravity are flat from the forcing up to buoyancy scale. At intermediate scales a ~ k^{-3} parallel spectrum develops for the Fr ~ 0.03 run, whereas for weaker stratification, the saturation spectrum does not have enough scales to develop and instead one observes a power law compatible with Kolmogorov scaling. Finally, the spectrum of helicity is flat until L_B, as observed in the nocturnal planetary boundary layer.