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A vortex-tube model of eddies in the inertial range

 

作者: Stephen Childress,  

 

期刊: Geophysical & Astrophysical Fluid Dynamics  (Taylor Available online 1984)
卷期: Volume 29, issue 1-4  

页码: 29-64

 

ISSN:0309-1929

 

年代: 1984

 

DOI:10.1080/03091928408248182

 

出版商: Taylor & Francis Group

 

数据来源: Taylor

 

摘要:

A vortex-tube geometry of the cascade of energy to small-scale eddies, in the inertial range of fully-developed turbulence, is proposed. The model is a special case of the beta model of Frisch, Sulem and Nelkin (1978). We require that the cascade conserve the principal invariants of inviscid, incompressible flow, namely volume, topological knottedness, circulation, and, at discrete times marking the termination of steps in the cascade, energy. The process terminates in a finite time, as in any beta model, leaving behind a self-similar network of “inactive” tubes. We associate a self-similar scaling dimensionDwith the structure, equal to the Hausdorff dimension of the set of “active” tubes at the termination of the cascade. Because circulation Λ plays a key role in the analysis of the cascade, we refer to these vortex-tube geometries as “gamma models”. The viewpoint throughout is entirely deterministic.

 

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