CFD simulation of turbulent flow in a rod bundle with spacer grids (MATIS-H) using STAR-CCM

被引:42
|
作者
Cinosi, N. [1 ]
Walker, S. P. [1 ]
Bluck, M. J. [1 ]
Issa, R. [1 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, Dept Mech Engn, London, England
基金
英国工程与自然科学研究理事会;
关键词
D O I
10.1016/j.nucengdes.2014.06.019
中图分类号
TL [原子能技术]; O571 [原子核物理学];
学科分类号
0827 ; 082701 ;
摘要
This paper presents the CFD simulation of the turbulent flow generated by a model PWR spacer grid within a rod bundle. The investigation was part of the MATIS-H benchmark exercise, organized by the OECD-NEA, with measurements performed at the KAERI facilities in Daejeon, Korea. The study employed the CD-Adapco code Star-CCM+. An initial sensitivity study was conducted to attempt to assess the importance to the overall flow of components such as the outlet plenum and the end support grid; these were shown to be able to be safely neglected, but the tapered end portion of the rods was found to be significant, and this was incorporated in the model analyzed. A RANS model using any of K-epsilon. K-omega and Reynolds-stress turbulence models was found to be adequate for the prediction of mean velocity profiles, but they all three underestimate the time-averaged turbulent velocity components. Vorticity seems to be better predicted, although the measured values of vorticity are only presented via colored contour plots, making quantitative comparison rather difficult. Circulation, calculated via an integral for each channel, seems to be well predicted by all three models. (C) 2014 Elsevier B.V. All rights reserved.
引用
收藏
页码:37 / 49
页数:13
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