TY - JOUR
T1 - Thin shear layer structures in high Reynolds number turbulence
T2 - Tomographic experiments and a local distortion model
AU - Hunt, Julian C.R.
AU - Ishihara, Takashi
AU - Worth, Nicholas A.
AU - Kaneda, Yukio
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 [104] 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. 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 - 2014/3
Y1 - 2014/3
N2 - Three-dimensional tomographic time dependent PIV measurements of high Reynolds number (Re) laboratory turbulence are presented which show the existence of long-lived, highly sheared thin layer eddy structures with thickness of the order of the Taylor microscale and internal fluctuations. Highly sheared layer structures are also observed in direct numerical simulations of homogeneous turbulence at higher values of Re (Ishihara et al., Annu Rev Fluid Mech 41:165-180, 2009). But in the latter simulation, where the fluctuations aremore intense, the layer thickness is greater. A rapid distortion model describes the structure and spectra for the velocity fluctuations outside and within 'significant' layers; their spectra are similar to the Kolmogorov (C R Acad Sci URSS 30:299-303, 1941) and Obukhov (Dokl Akad Nauk SSSR 32:22-24, 1941) statistical model (KO) for the whole flow. As larger-scale eddy motions are blocked by the shear layers, they distort smaller-scale eddies leading to local zones of down-scale and up-scale transfer of energy. Thence the energy spectrum for high wave number k is EX (k) ∼Bk?2p. The exponent p depends on the forms of the large eddies. The non-linear interactions between the distorted inhomogeneous eddies produce a steady local structure, which implies that 2p = 5/3 and a flux of energy into the thin-layers balancing the intense dissipation, which is much greater than the mean (σ). Thence B ∼ (σ) ?2/3 as in KO. Within the thin layers the inward flux energises extended vortices whose thickness and spacing are comparable with the viscous microscale. Although peak values of vorticity and velocity of these vortices greatly exceed those based on the KO scaling, the form of the viscous range spectrum is consistent with their model.
AB - Three-dimensional tomographic time dependent PIV measurements of high Reynolds number (Re) laboratory turbulence are presented which show the existence of long-lived, highly sheared thin layer eddy structures with thickness of the order of the Taylor microscale and internal fluctuations. Highly sheared layer structures are also observed in direct numerical simulations of homogeneous turbulence at higher values of Re (Ishihara et al., Annu Rev Fluid Mech 41:165-180, 2009). But in the latter simulation, where the fluctuations aremore intense, the layer thickness is greater. A rapid distortion model describes the structure and spectra for the velocity fluctuations outside and within 'significant' layers; their spectra are similar to the Kolmogorov (C R Acad Sci URSS 30:299-303, 1941) and Obukhov (Dokl Akad Nauk SSSR 32:22-24, 1941) statistical model (KO) for the whole flow. As larger-scale eddy motions are blocked by the shear layers, they distort smaller-scale eddies leading to local zones of down-scale and up-scale transfer of energy. Thence the energy spectrum for high wave number k is EX (k) ∼Bk?2p. The exponent p depends on the forms of the large eddies. The non-linear interactions between the distorted inhomogeneous eddies produce a steady local structure, which implies that 2p = 5/3 and a flux of energy into the thin-layers balancing the intense dissipation, which is much greater than the mean (σ). Thence B ∼ (σ) ?2/3 as in KO. Within the thin layers the inward flux energises extended vortices whose thickness and spacing are comparable with the viscous microscale. Although peak values of vorticity and velocity of these vortices greatly exceed those based on the KO scaling, the form of the viscous range spectrum is consistent with their model.
KW - High Reynolds number turbulence
KW - Intermittency
KW - Local distortion model
KW - Thin shear layers
KW - Tomographic experiments
UR - http://www.scopus.com/inward/record.url?scp=84899481680&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84899481680&partnerID=8YFLogxK
U2 - 10.1007/s10494-013-9518-0
DO - 10.1007/s10494-013-9518-0
M3 - Article
AN - SCOPUS:84899481680
SN - 1386-6184
VL - 92
SP - 607
EP - 649
JO - Flow, Turbulence and Combustion
JF - Flow, Turbulence and Combustion
IS - 3
ER -