TY - JOUR
T1 - Thin shear layers in high reynolds number turbulence - DNS results
AU - Ishihara, Takashi
AU - Kaneda, Yukio
AU - Hunt, Julian C.R.
N1 - Funding Information:
Acknowledgements This paper greatly benefited from discussions at the Isaac Newton Institute Workshop in 2008 and at the Kavli Institute for Theoretical Physics in 2011. Professor G. I. Barenblatt, H. K. Moffatt, and Z. Warhaft helped us understand this model better and its historical context. Professor Sreenivasan clarified our thinking about cascades. JCRH is grateful for being invited to give an early version of the theoretical ideas in this paper [36] at Hong Kong University of Science and Technology in Dec 2009, as well as to support from Arizona State University, Notre Dame University, HongKong University, T.U.Delft. JCRH has been supported by Qinetiq and Atlas Elektronik for turbulence structure studies. Travel funds for visiting Nagoya were provided by Trinity College Cambridge. Support for JCRH by NERC Centre for Polar observation and Modelling at UCL is gratefully acknowledged. We acknowledge useful comments by the referees. The computations were carried out on the Earth Simulator at Japan Agency for Marine-Earth Science and Technology and on the Fx1 system at the Information Technology Center of Nagoya University. This work was partly supported by Grant-in-Aids for Scientific Research (C)23540447 and (C)23560194, from the Japan Society for the Promotion of Science, and also by JST, CREST.
PY - 2013/12
Y1 - 2013/12
N2 - Using direct numerical simulation of turbulence in a periodic box driven by homogeneous forcing, with a maximum of 40963 grid points and Taylor micro-scale Reynolds numbers Rλ up to 1131, it is shown that there is a transition in the forms of the significant, high vorticity, intermittent structures, from isolated vortices when Rλ is less than 102 to complex thin-shear layers when Rλ exceeds about 103. Both the distance between the layers and their widths are comparable with the integral length scale. The thickness of each of the layers is of the order of the Taylor micro-scale λ. Across the layers the velocity 'jumps' are of the order of the rms velocity uo of the whole flow. Within the significant layers, elongated vortical eddies are generated, with microscale thickness ℓν ∼ 10η << λ, with associated peak values of vorticity as large as 35ωrms and with velocity jumps as large as 3.4uo, where η is the Kolmogorov micro scale and ωrms the rms vorticity. The dominant vortical eddies in the layers, which are approximately parallel to the vorticity averaged over the layers, are separated by distances of order ℓν. The close packing leads to high average energy dissipation inside the layer, as large as ten times the mean rate of energy dissipation over the whole flow. The interfaces of the layers act partly as a barrier to the fluctuations outside the layer. However, there is a net energy flux into the small scale eddies within the thin layers from the larger scale motions outside the layer.
AB - Using direct numerical simulation of turbulence in a periodic box driven by homogeneous forcing, with a maximum of 40963 grid points and Taylor micro-scale Reynolds numbers Rλ up to 1131, it is shown that there is a transition in the forms of the significant, high vorticity, intermittent structures, from isolated vortices when Rλ is less than 102 to complex thin-shear layers when Rλ exceeds about 103. Both the distance between the layers and their widths are comparable with the integral length scale. The thickness of each of the layers is of the order of the Taylor micro-scale λ. Across the layers the velocity 'jumps' are of the order of the rms velocity uo of the whole flow. Within the significant layers, elongated vortical eddies are generated, with microscale thickness ℓν ∼ 10η << λ, with associated peak values of vorticity as large as 35ωrms and with velocity jumps as large as 3.4uo, where η is the Kolmogorov micro scale and ωrms the rms vorticity. The dominant vortical eddies in the layers, which are approximately parallel to the vorticity averaged over the layers, are separated by distances of order ℓν. The close packing leads to high average energy dissipation inside the layer, as large as ten times the mean rate of energy dissipation over the whole flow. The interfaces of the layers act partly as a barrier to the fluctuations outside the layer. However, there is a net energy flux into the small scale eddies within the thin layers from the larger scale motions outside the layer.
KW - High Reynolds number turbulence
KW - Intermittency
KW - Thin shear layers
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U2 - 10.1007/s10494-013-9499-z
DO - 10.1007/s10494-013-9499-z
M3 - Article
AN - SCOPUS:84892369286
SN - 1386-6184
VL - 91
SP - 895
EP - 929
JO - Flow, Turbulence and Combustion
JF - Flow, Turbulence and Combustion
IS - 4
ER -