We have conducted experiments on an asymmetrically forced quasi-two-dimensional turbulent flow in a rapidly rotating annulus. Assuming conservation of potential enstrophy and energy, we maximize a nonextensive entropy function to obtain the azimuthally averaged vorticity as a function of radial posi
Nonextensivity in turbulence in rotating two-dimensional and three-dimensional flows
โ Scribed by Charles N Baroud; Harry L Swinney
- Publisher
- Elsevier Science
- Year
- 2003
- Tongue
- English
- Weight
- 332 KB
- Volume
- 184
- Category
- Article
- ISSN
- 0167-2789
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โฆ Synopsis
Our experiments on turbulent flow in a rotating annulus yield probability distribution functions (PDFs) for velocity increments ฮดv( ), where is the separation between points. We fit these PDFs to a form derived for turbulent flows by Beck, who used the Tsallis nonextensive statistical mechanics formalism. For slow rotation rates, we find that the fit parameter q is 1.25 for small . At large , q decreases to unity, the value corresponding to the usual Boltzmann-Gibbs statistics. These results agree with those previously measured in experiments on Couette-Taylor turbulence. However, with rapid rotation of the annulus, the turbulent flow becomes strongly two-dimensional (2D) rather than three-dimensional (3D), and we find q = 1.32 ยฑ 0.04, independent of . This suggests that the coherent structures (vortices), which are a source of intermittency, are important at all length scales in the 2D case.
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