Direct numerical simulation of a 30R long turbulent pipe flow at R+=685: large- and very large-scale motions

被引:93
|
作者
Wu, Xiaohua [2 ]
Baltzer, J. R. [1 ]
Adrian, R. J. [1 ]
机构
[1] Arizona State Univ, Sch Engn Matter Transport & Energy, Tempe, AZ 85287 USA
[2] Royal Mil Coll Canada, Dept Mech Engn, Kingston, ON K7K 7B4, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
pipe flow boundary layer; turbulent boundary layers; NEAR-WALL TURBULENCE; BOUNDARY-LAYER-FLOWS; CHANNEL FLOW; REYNOLDS-NUMBER; CONVECTION VELOCITIES; TAYLORS HYPOTHESIS; FLUCTUATIONS; FEATURES; SPECTRA; REGION;
D O I
10.1017/jfm.2012.81
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Fully developed incompressible turbulent pipe flow at Reynolds number Re-D = 24580 (based on bulk velocity) and Karman number R+ =684.8 is simulated in a periodic domain with a length of 30 pipe radii R. While single-point statistics match closely with experimental measurements, questions have been raised of whether streamwise energy spectra calculated from spatial data agree with the well-known bimodal spectrum shape in premultiplied spectra produced by experiments using Taylor's hypothesis. The simulation supports the importance of large- and very large- scale motions (VLSMs, with streamwise wavelengths exceeding 3R). Wavenumber spectral analysis shows evidence of a weak peak or flat region associated with VLSMs, independent of Taylor's hypothesis, and comparisons with experimental spectra are consistent with recent findings (del Alamo & Jimenez, J. Fluid Mech., vol. 640, 2009, pp. 5-26) that the long-wavelength streamwise velocity energy peak is overestimated when Taylor's hypothesis is used. Yet, the spectrum behaviour retains otherwise similar properties to those documented based on experiment. The spectra also reveal the importance of motions of long streamwise length to the uu energy and uv Reynolds stress and support the general conclusions regarding these quantities formed using experimental measurements. Space-time correlations demonstrate that low-level correlations involving very large scales persist over 40R/U-bulk in time and indicate that these motions convect at approximately the bulk velocity, including within the region approaching the wall. These very large streamwise motions are also observed to accelerate the flow near the wall based on force spectra, whereas smaller scales tend to decelerate the mean streamwise flow profile, in accordance with the behaviour observed in net force spectra of prior experiments. Net force spectra are resolved for the first time in the buffer layer and reveal an unexpectedly complex structure.
引用
收藏
页码:235 / 281
页数:47
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