The directions of the triadic energy transfers assumed in a previous paper [Phys. Fluids A 4, 350 (1992)] agree with the spectral closures, in a similarity range, if the exponent of the power‐law energy spectrum is less than unity. The helical interactions showing a strong local energy transfer when the triad is nonlocal, sum up to a reverse cascade unless the spectrum falls off faster than a −7/3 power of the wave number. The energy cascades from each type of helical interaction are calculated for a −5/3 inertial range using the eddy damped quasinormal Markovian (EDQNM) model. One type of interaction is responsible for 86% of the cascade. The contributions of the two classes of helical interactions to the subgrid‐scale eddy viscosity are presented, together with the contributions from the forward and reverse cascading interactions. An application of the assumption on the triadic energy transfers to turbulence under rapid rotation gives a simple argument for the tendency toward nonlinear two‐dimensionalization of the flow.
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March 1993
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Physics of Fluids A: Fluid Dynamics
Research Article|
March 01 1993
Inertial transfers in the helical decomposition Available to Purchase
Fabian Waleffe
Fabian Waleffe
Center for Turbulence Research, Stanford University/NASA Ames Research Center, MS 202A‐1, Moffett Field, California 94035‐1000
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Fabian Waleffe
Center for Turbulence Research, Stanford University/NASA Ames Research Center, MS 202A‐1, Moffett Field, California 94035‐1000
Phys. Fluids 5, 677–685 (1993)
Article history
Received:
June 01 1992
Accepted:
October 16 1992
Citation
Fabian Waleffe; Inertial transfers in the helical decomposition. Phys. Fluids 1 March 1993; 5 (3): 677–685. https://doi.org/10.1063/1.858651
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