Self-Induced Large-Scale Motions in a Three-Dimensional Diffuser

被引:2
作者
Miro, Arnau [1 ]
Eiximeno, Benet [1 ,2 ]
Rodriguez, Ivette [2 ]
Lehmkuhl, Oriol [1 ]
机构
[1] Barcelona Supercomp Ctr, Placa Eusebi Guell 1-3, Barcelona 08034, Spain
[2] Univ Politecn Cataluna, TUAREG Turbulence & Aerodynam Res Grp, C Colom 11, Barcelona 08222, Spain
基金
欧盟地平线“2020”;
关键词
DNS; POD; DMD; Separation; Confined flow; High-fidelity dataset; MAGNETIC-RESONANCE VELOCIMETRY; COHERENT STRUCTURES; SIMULATION; FLOW; JET;
D O I
10.1007/s10494-023-00483-6
中图分类号
O414.1 [热力学];
学科分类号
摘要
A direct numerical simulation of a three-dimensional diffuser at Reynolds number Re = 10,000 (based on inlet bulk velocity) has been performed using a low-dissipation finite element code. The geometry chosen for this work is the Stanford diffuser, introduced by Cherry et al. (Int. J. Heat Fluid Flow 29:803-811, 2008). Results have been exhaustively compared with the published data with a quite good agreement. Additionally, further turbulent statistics have been provided such as the Reynolds stresses or the turbulent kinetic energy. A proper orthogonal decomposition and a dynamic mode decomposition analyses of the main flow variables have been performed to identify the main characteristics of the large-scale motions. A combined, self-induced movement of the large-scales has been found to originate in the top-right expansion corner with two clear features. A low-frequency diagonal cross-stream travelling wave first reported by Malm et al. (J. Fluid Mech. 699:320-351, 2012), has been clearly identified in the spatial modes of the streamwise velocity components and the pressure, associated with the narrow band frequency of St. [0.083, 0.01]. This movement is caused by the geometrical expansion of the diffuser in the cross-stream direction. A second low-frequency trait has been identified associated with the persisting secondary flows and acting as a back and forth global acceleratingdecelerating motion located on the straight area of the diffuser, with associated frequencies of St < 0.005. The smallest frequency observed in this work has been St = 0.0013. This low-frequency observed in the Stanford diffuser points out the need for longer simulations in order to obtain further turbulent statistics.
引用
收藏
页码:303 / 320
页数:18
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