Persistent cyclonic structures in self-similar turbulent flows
P.D. Mininni, A. Pouquet

TL;DR
This paper investigates how rotation and helicity influence turbulence, revealing persistent cyclonic vortices and self-similar small-scale behavior, which enhances understanding of geophysical and astrophysical flows.
Contribution
It uncovers the coexistence of long-lived cyclonic vortices with turbulence and identifies self-similarity at small scales in rotating helical turbulence.
Findings
Long-lived laminar cyclonic vortices observed
Small scales exhibit complete self-similarity
No deviations from Gaussianity at small scales
Abstract
Invariance properties of a physical system govern its behavior: energy conservation in turbulence drives a wide distribution of energy among modes, as observed in geophysics, astrophysics and engineering. In hydrodynamic turbulence, the role of helicity (which measures departures from mirror symmetry) remains unclear since it does not alter this distribution. However, the interplay of rotation and helicity leads to significant differences. Using numerical simulations we show the occurence of long-lived laminar cyclonic vortices together with turbulent vortices, reminiscent of recent tornado observations. Furthermore, the small scales are completely self-similar with no deviations from Gaussianity. This result points to the discovery of a small parameter in rotating helical turbulence.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Fluid Dynamics and Turbulent Flows · Geomagnetism and Paleomagnetism Studies
