# Turbulent bifurcations in intermittent shear flows: from puffs to   oblique stripes

**Authors:** Takahiro Ishida, Yohann Duguet, Takahiro Tsukahara

arXiv: 1705.02945 · 2017-08-01

## TL;DR

This paper investigates the formation and transition of localized turbulent structures in annular pipe flows, revealing a gradual shift from puffs to oblique stripes as azimuthal confinement decreases, with implications for subcritical shear flows.

## Contribution

It provides a detailed analysis of the transition from puffs to oblique stripes in shear flows, highlighting the role of azimuthal confinement and large-scale flow properties.

## Key findings

- Transition from puffs to stripes is gradual.
- Oblique stripes emerge as azimuthal confinement relaxes.
- The transition mechanism is applicable to various subcritical shear flows.

## Abstract

Localised turbulent structures such as puffs or oblique stripes are building blocks of the intermittency regimes in subcritical wall-bounded shear flows. These turbulent structures are investigated in incompressible pressure-driven annular pipe flow using direct numerical simulations in long domains. For low enough radius ratio $\eta$, these coherent structures have a dynamics comparable to that of puffs in cylindrical pipe flow. For $\eta$ larger than 0.5, they take the shape of helical stripes inclined with respect to the axial direction. The transition from puffs to stripes is analysed statistically by focusing on the axisymmetry properties of the associated large-scale flows. It is shown that the transition is gradual : as the azimuthal confinement relaxes, allowing for an azimuthal large-scale component, oblique stripes emerge as predicted in the planar limit. The generality of this transition mechanism is discussed in the context of subcritical shear flows.

## Full text

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## Figures

60 figures with captions in the complete paper: https://tomesphere.com/paper/1705.02945/full.md

## References

32 references — full list in the complete paper: https://tomesphere.com/paper/1705.02945/full.md

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Source: https://tomesphere.com/paper/1705.02945