Instability and disintegration of vortex rings during head-on collisions and wall interactions

TL;DR

This study systematically investigates how vortex ring collisions and wall impacts lead to various phenomena like secondary rings, vortex sheets, or turbulence, depending on instabilities influenced by parameters like Reynolds number and slenderness ratio.

Contribution

It provides a detailed numerical analysis of the dominant azimuthal instabilities in vortex ring collisions and wall interactions across a range of parameters, elucidating the mechanisms behind different outcomes.

Findings

Higher Reynolds numbers promote vortex disintegration into turbulence.

Wall interactions can produce secondary rings or vortex structures depending on boundary conditions.

Slenderness ratio influences the stability and resulting phenomena of vortex collisions.

Abstract

The head-on collision of two vortex rings can produce diverse phenomena: a tiara of secondary rings, vortex sheets which flatten and interact iteratively, or the violent disintegration of the rings into a turbulent cloud. The outcome of the interaction is determined by the nature of the instability affecting two impinging vortex rings. Here, we carry out a systematic study to determine the dominant instability as a function of the parameters of the problem. To this end, we numerically simulate the head on collision of vortex rings with circulation Reynolds numbers between $1000$ and $3500$ and varying slenderness ratios $\Lambda=a/R$ ranging from $\Lambda=0.1$ to $0.35$, with $a$ the core radius and $R$ the ring radius. By studying the temporal evolution of the energy and viscous dissipation, we elucidate the role azimuthal instabilities play in determining what the outcomes of the collision are. We then compare these collisions to the head-on impact of a vortex ring on a free-slip and a no-slip wall. The free-slip wall imposes a mirror symmetry, which impedes certain instabilities and at sufficiently large Reynolds numbers leads to the formation of a half-tiara of vortices. Impact against a no-slip wall results in the process where a secondary vortex ring is formed after the ejection of the resulting boundary layer. When the Reynolds number is above a certain threshold, which increases with $\Lambda$, the vortices disintegrate through azimuthal instabilities, resulting in a turbulent cloud.