Energy flux fluctuations in a finite volume of turbulent flow
被引:7
作者:
Bandi, MM
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机构:
Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USAUniv Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
Bandi, MM
[1
]
Goldburg, WI
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h-index: 0
机构:Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
Goldburg, WI
Cressman, JR
论文数: 0引用数: 0
h-index: 0
机构:Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
Cressman, JR
Pumir, A
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h-index: 0
机构:Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
Pumir, A
机构:
[1] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[2] George Mason Univ, Krasnow Inst, Fairfax, VA 22030 USA
[3] CNRS, Inst Non Lineaire Nice, F-06270 Valbonne, France
[4] Univ Nice, F-06270 Valbonne, France
来源:
PHYSICAL REVIEW E
|
2006年
/
73卷
/
02期
关键词:
D O I:
10.1103/PhysRevE.73.026308
中图分类号:
O35 [流体力学];
O53 [等离子体物理学];
学科分类号:
070204 [等离子体物理];
080103 [流体力学];
080704 [流体机械及工程];
摘要:
The flux of turbulent kinetic energy from large to small spatial scales is measured in a small domain B of varying size R. The probability distribution function of the flux is obtained using a time-local version of Kolmogorov four-fifths law. The measurements, made at a moderate Reynolds number, show frequent events where the flux is backscattered from small to large scales, their frequency increasing as R is decreased. The observations are corroborated by a numerical simulation based on the motion of many particles and on an explicit form of the eddy damping.