TL;DR
This paper introduces a new shell model based on helical modes to investigate how helicity influences triad interactions and energy cascades in 3D turbulence, providing insights into the dominance of dual cascades.
Contribution
The paper develops a novel shell model derived from the Navier-Stokes equations in the helical basis to analyze triad interactions and cascades in 3D turbulence.
Findings
A subset of helical triadic interactions can lead to inverse energy cascades.
Helical mode decomposition clarifies the role of helicity in energy transfer.
The model explains the dominance of dual cascades in 3D turbulence.
Abstract
Fully developed homogeneous isotropic turbulence in 2D is fundamentally different from 3D. In 2D, the simultaneous conservation of both energy and enstrophy in the inertial ranges of scales leads to a forward cascade of enstrophy and a reverse cascade of energy. In 3D, helicity, the integral of the scalar product of velocity and vorticity, is also an inviscid flow invariant along with kinetic energy. Unlike enstrophy, however, helicity does not block the cascade of energy to small scales. Energy and helicity are not only globally conserved but also conserved within each non-linear triadic interaction between three plane waves in the spectral form of the Navier--Stokes equation (NSE). By decomposing each plane wave into two helical modes of opposite helicities each triadic interaction is split into a set of eight triadic interactions between helical modes (Waleffe 1992). Biferale et al.…
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