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Three-Dimensional Shear-Flow Instability Saturation via Stable Modes

Fluid Dynamics 2023-10-19 v2 Computational Physics Plasma Physics Space Physics

Abstract

Turbulence in three dimensions (33D) supports vortex stretching that has long been known to accomplish energy transfer to small scales. Moreover, net energy transfer from large-scale, forced, unstable flow-gradients to smaller scales is achieved by gradient-flattening instability. Despite such enforcement of energy transfer to small scales, it is shown here not only that the shear-flow-instability-supplied 33D-fluctuation energy is largely inverse-transferred from the fluctuation to the mean-flow gradient, but that such inverse transfer is more efficient for turbulent fluctuations in 33D than in two dimensions (22D). The transfer is due to linearly stable eigenmodes that are excited nonlinearly. The stable modes, thus, reduce both the nonlinear energy cascade to small scales and the viscous dissipation rate. The vortex-tube stretching is also suppressed. Up-gradient momentum transport by the stable modes counters the instability-driven down-gradient transport, which also is more effective in 33D than in 22D (70%vs.50%\mathrm{\approx} 70\% \mathrm{\,\, vs.\,\,}\mathrm{\approx} 50\%). From unstable modes, these stable modes nonlinearly receive energy via zero-frequency fluctuations that vary only in the direction orthogonal to the plane of 22D shear flow. The more widely occurring 33D turbulence is thus inherently different from the commonly studied 22D turbulence, despite both saturating via stable modes.

Keywords

Cite

@article{arxiv.2310.09339,
  title  = {Three-Dimensional Shear-Flow Instability Saturation via Stable Modes},
  author = {B. Tripathi and P. W. Terry and A. E. Fraser and E. G. Zweibel and M. J. Pueschel},
  journal= {arXiv preprint arXiv:2310.09339},
  year   = {2023}
}

Comments

To appear in Physics of Fluids

R2 v1 2026-06-28T12:50:16.179Z