Scale interactions and scaling laws in rotating flows at moderate Rossby numbers and large Reynolds numbers
P.D. Mininni, A. Alexakis, and A. Pouquet

TL;DR
This study uses direct numerical simulations to explore how rotation influences turbulence at moderate Rossby numbers and high Reynolds numbers, revealing non-local energy transfers and preserved intermittency similar to homogeneous turbulence.
Contribution
It provides new insights into the spectral behavior, energy transfer mechanisms, and intermittency in rotating turbulent flows at moderate Rossby numbers with large Reynolds numbers.
Findings
Inverse energy cascade is non-local, transferring energy directly from small to large scales.
Energy transfer at small scales is mediated by interactions with the largest eddies.
Intermittency in the direct cascade remains consistent with homogeneous turbulence.
Abstract
The effect of rotation is considered to become important when the Rossby number is sufficiently small, as is the case in many geophysical and astrophysical flows. Here we present direct numerical simulations to study the effect of rotation in flows with moderate Rossby numbers (down to Ro~0.1) but at Reynolds numbers large enough to observe the beginning of a turbulent scaling at scales smaller than the energy injection scale. We use coherent forcing at intermediate scales, leaving enough room in the spectral space for an inverse cascade of energy to also develop. We analyze the spectral behavior of the simulations, the shell-to-shell energy transfer, scaling laws, and intermittency, as well as the geometry of the structures in the flow. At late times, the direct transfer of energy at small scales is mediated by interactions with the largest scale in the system, the energy containing…
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