Vortex stretching and enstrophy production in high Reynolds number turbulence

TL;DR

This study investigates vortex stretching and enstrophy production in high Reynolds number turbulence using large-scale direct numerical simulations, revealing how vorticity and strain interact and contribute to extreme events.

Contribution

It provides detailed statistical analysis of vorticity-strain correlations at unprecedented resolutions, highlighting the role of strain eigenvalues and viscous effects in enstrophy dynamics.

Findings

Vorticity aligns more strongly with the intermediate strain eigenvector at high enstrophy.

Strain magnitude grows as a power law with enstrophy, steeper at higher Reynolds numbers.

Intense enstrophy is mainly depleted through viscous diffusion.

Abstract

An essential ingredient of turbulent flows is the vortex stretching mechanism, which emanates from the non-linear interaction of vorticity and strain-rate tensor and leads to formation of extreme events. We analyze the statistical correlations between vorticity and strain rate by using a massive database generated from very well resolved direct numerical simulations of forced isotropic turbulence in periodic domains. The grid resolution is up to $12288^3$, and the Taylor-scale Reynolds number is in the range $140-1300$. In order to understand the formation and structure of extreme vorticity fluctuations, we obtain statistics conditioned on enstrophy (vorticity-squared). The magnitude of strain, as well as its eigenvalues, is approximately constant when conditioned on weak enstrophy; whereas they grow approximately as power laws for strong enstrophy, which become steeper with increasing $R_\lambda$. We find that the well-known preferential alignment between vorticity and the intermediate eigenvector of strain tensor is even stronger for large enstrophy, whereas vorticity shows a tendency to be weakly orthogonal to the most extensive eigenvector (for large enstrophy). Yet the dominant contribution to the production of large enstrophy events arises from the most extensive eigendirection, the more so as $R_\lambda$ increases. Nevertheless, the stretching in intense vorticity regions is significantly depleted, consistent with the kinematic properties of weakly-curved tubes in which they are organized. Further analysis reveals that intense enstrophy is primarily depleted via viscous diffusion, though viscous dissipation is also significant. Implications for modeling are nominally addressed as appropriate.