Characterization of the wake of a submarine propeller via Large-Eddy simulation

被引:91
作者
Posa, Antonio [1 ]
Broglia, Riccardo [1 ]
Felli, Mario [1 ]
Falchi, Massimo [1 ]
Balaras, Elias [2 ]
机构
[1] Natl Res Council Italy, Inst Marine Engn, CNR INM Ex CNR INSEAN, Via Vallerano 139, I-00128 Rome, Italy
[2] George Washington Univ, Dept Mech & Aerosp Engn, 800 22nd St NW, Washington, DC 20052 USA
基金
欧盟地平线“2020”;
关键词
Submarine propellers; Naval hydrodynamics; Coherent structures; Large eddy simulation; Immersed boundary method; MARINE PROPELLER; EVOLUTION; PRESSURE; FLOW; MECHANISMS; DYNAMICS; MODEL; PIV;
D O I
10.1016/j.compfluid.2019.03.011
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
Results of large-eddy simulations of a submarine propeller in open-water (isolated) configuration are presented for three load conditions. An immersed boundary approach is adopted to handle the rotating geometry of the propeller within a stationary cylindrical grid composed of about 840 million nodes. Direct comparisons with Particle Image Velocimetry experiments conducted in parallel demonstrate that the simulations reproduce the wake very accurately. In particular the wake dynamics are mainly dominated by tip and hub vortices. Strong structures are also shed in the near wake from the suction side of the propeller blades, correlating with local maxima of turbulent kinetic energy. However, they are not a long standing feature of the propeller wake. In contrast, helical structures originating form the root of the propeller blades are more persistent and their footprint is still visible few propeller diameters downstream. We verified that load conditions affect substantially both hub vortex and tip vortices. In a similar way, for increasing loads turbulent kinetic energy experiences a faster growth at the wake axis, populated by the hub vortex, compared to the outer radii, dominated by the tip vortices. Also, the evolution of turbulent kinetic energy at the outer edge of the wake is not monotonic, in contrast with that in the wake core, due to mutual interaction and associated shear between tip vortices and the wake of the following blades. (C) 2019 Elsevier Ltd. All rights reserved.
引用
收藏
页码:138 / 152
页数:15
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