Flow visualization of supersonic laminar flow over a backward-facing step via NPLS
Flow visualization of supersonic laminar flow over a backward-facing step via NPLS
复制标题
通过 NPLS 对向后台阶上的超音速层流进行流动可视化
DOI:
10.1007/s00193-012-0378-7
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发表时间:
2013-07
期刊:
影响因子:
2.2
通讯作者:
Zhu, Y. Z.
中科院分区:
文献类型:
--
作者:
Yi, S. H.;Tian, L. F.;He, L.;Zhu, Y. Z.
An experimental study on a supersonic laminar flow over a backward-facing step of 5 mm height was undertaken in a low-noise indraft wind tunnel. To investigate the fine structures ofMa= 3.0 and 3.8 laminar flow over a backward-facing step, nanotracer planar laser scattering was adopted for flow visualization. Flow structures, including supersonic laminar boundary layer, separation, reattachment, redeveloping turbulent boundary layer, expansion wave fan and reattachment shock, were revealed in the transient flow fields. In theMa= 3.0 BFS (backward-facing step) flow, by measuring four typical regions, it could be found that the emergence of weak shock waves was related to the K–H (Kelvin–Helmholtz) vortex which appeared in the free shear layer and that the convergence of these waves into a reattachment shock was distinct. Based on large numbers of measurements, the structure of time-averaging flow field could be gained. Reattachment occurred at the location downstream from the step, about 7–7.5 h distance. After reattachment, the recovery boundary layer developed into turbulence quickly and its thickness increased at an angle of 4.6°. At the location ofX= 14h, the redeveloping boundary layer was about ten times thicker than its original thickness, but it still had not changed into fully developed turbulence. However, in theMa= 3.8 flow, the emergence of weak shock waves could be seen seldom, due to the decrease of expansion. The reattachment point was thought to be nearX= 15haccording to the averaging result. The reattachment shock was not legible, which meant the expansion and compression effects were not intensive.
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DOI:
10.1007/s11433-009-0180-4
发表时间:
2009-08
期刊:
Science in China Series G: Physics, Mechanics and Astronomy
影响因子:
--
作者:
L. Tian;S. Yi;Yu-xin Zhao;Lin He;Zhongyu Cheng
通讯作者:
L. Tian;S. Yi;Yu-xin Zhao;Lin He;Zhongyu Cheng
影响因子:
2.4
作者:
G. Shen;G. Ma
通讯作者:
G. Shen;G. Ma
DOI:
10.2514/6.1998-939
发表时间:
1998-01
期刊:
--
影响因子:
--
作者:
A. Matsuo;M. Mizomoto
通讯作者:
A. Matsuo;M. Mizomoto
DOI:
10.1007/s11431-009-0281-3
发表时间:
2009-12
期刊:
Science in China Series E: Technological Sciences
影响因子:
--
作者:
Yu-xin Zhao;S. Yi;L. Tian;Zhongyu Cheng
通讯作者:
Yu-xin Zhao;S. Yi;L. Tian;Zhongyu Cheng
DOI:
10.1007/s11433-009-0301-0
发表时间:
2009-12
期刊:
Science in China - Series G: Physics Mechanics and Astronomy
影响因子:
--
作者:
He Lin;Zhao YuXin;Tian LiFeng;Cheng ZhongYu
通讯作者:
Cheng ZhongYu