In this paper, three-dimensional. time-dependent calculations are carried out using the finite volume CFD code CFX4 and the VLES approach with standard k-epsilon model to simulate the turbulent swirl flow in an axisymmetric sudden expansion with an expansion ratio of 5.0 for a Reynolds number of 10(5). This flow is unstable over the entire swirl number range considered between 0 and 0.48, and a large-scale coherent structure is found to precess about the centerline. Compared with the unswirled case, inclusion of a slight inlet swirl (swirl number below 0.23) can reduce the precession speed, cause the precession to be against the mean swirl and suppress the flapping motion. Several modes of precession are predicted as the swirl intensity increases. in which the precession, as well as the spiral structure, reverses direction. Accompanying the transition between different modes, abrupt changes in precession frequency are also experienced. Grid sensitivity and comparison with smaller expansion ratio data are also discussed. (C) 2002 Elsevier Science Inc. All rights reserved.
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Politecn Milan, Dept Energy, Via Lambruschini 4, I-20156 Milan, ItalyPolitecn Milan, Dept Energy, Via Lambruschini 4, I-20156 Milan, Italy
Dehkordi, P. Babakhani
Azdarpour, A.
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Islamic Azad Univ, Dept Petr Engn, Marvdasht Branch, Marvdasht, IranPolitecn Milan, Dept Energy, Via Lambruschini 4, I-20156 Milan, Italy
Azdarpour, A.
Mohammadian, E.
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Ton Duc Thang Univ, Dept Management Sci & Technol Dev, Ho Chi Minh City, Vietnam
Ton Duc Thang Univ, Fac Sci Appl, Ho Chi Minh City, VietnamPolitecn Milan, Dept Energy, Via Lambruschini 4, I-20156 Milan, Italy