ON THE BEHAVIOR OF VELOCITY-GRADIENT TENSOR INVARIANTS IN DIRECT NUMERICAL SIMULATIONS OF TURBULENCE

被引:86
|
作者
CANTWELL, BJ
机构
[1] Department of Aeronautics and Astronautics, Stanford University, Stanford
来源
PHYSICS OF FLUIDS A-FLUID DYNAMICS | 1993年 / 5卷 / 08期
关键词
D O I
10.1063/1.858828
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Studies of direct numerical simulations of incompressible, homogeneous, and inhomogeneous turbulence indicate that, in regions of high kinetic energy dissipation rate, the geometry of the local velocity gradient field has a universal character. The velocity gradient tensor satisfies the nonlinear evolution equation (dA(ij)/dt)+A(ik)A(kj)-1/3(A(mn)A(nm)delta(ij) = H(ij) where A(ij) = partial derivative u(i)/partial derivative x(j) and the tensor H(ij) contains terms involving the action of cross derivatives of the pressure field and viscous diffusion of A(ij). The restricted Euler equation corresponding to H(ij) = 0 can be solved in closed form [Cantwell, Phys. Fluids A 4, 782 (1992)] and the solution has the property that, for any initial condition, A(ij) (t) evolves to an asymptotic state of the form A(ij)(t) is-approximately-equal-to K(ij)[R(t)]1/3 where R(t) is a function which becomes singular in a finite time and K(ij) is a constant matrix. A number of the universal features of fine-scale motions observed in direct numerical simulations are reproduced by K(ij). In the simulation studies the first invariant of A(ij) is zero by incompressibility. The second and third invariants, Q and R, are determined at every grid point in the flow and the entire data set is cross-plotted to search for significant features in the space of tensor invariants. Such features can then be associated with corresponding local flow structures in physical space. When a variety of incompressible simulations are studied, scatter plots of Q vs R reveal that a fairly significant fraction of the data lies in the lower right quadrant. This is consistent with behavior predicted by the restricted Euler solution. However, the bulk of the data lies more or less uniformly distributed in a slightly elliptical region about the origin. In a direct numerical simulation of a plane, time-developing, mixing layer a small fraction of the data collects along a very pronounced, nearly straight, ridgeline extending into the upper left quadrant. This data can be traced to regions with local vorticity much larger than the local strain lying within streamwise rib vortices which connect adjacent spanwise rollers in the mixing layer simulation. Neither the predominant tendency for Q and R to lie near the origin nor the possibility for Q and R to lie far from the origin in the upper left quadrant are predicted by the restricted Euler solution. The purpose of this paper is to show that, by relaxing the assumption H(ij) = 0 while retaining a model of dA(ij)/dt motivated by the asymptotic form of the restricted Euler solution, one can begin to account for these features of the (Q,R) scatter plots. The results suggest that the velocity gradient tensor in three-dimensional flow tends to evolve toward an attractor in the space of tensor invariants. A significant feature of the model is that, although H(ij) not-equal 0, singular behavior of A(ij)(t) can still occur along specific paths in the (Q,R) plane corresponding to zero values of the discriminant of H(ij).
引用
收藏
页码:2008 / 2013
页数:6
相关论文
共 50 条
  • [31] Invariants of the velocity gradient tensor in a spatially developing compressible round jet
    Thaker, Parth
    Mathew, Joseph
    Ghosh, Somnath
    JOURNAL OF FLUID MECHANICS, 2023, 971
  • [32] Triple decomposition of velocity gradient tensor in homogeneous isotropic turbulence
    Nagata, Ryosuke
    Watanabe, Tomoaki
    Nagata, Koji
    da Silva, Carlos B.
    COMPUTERS & FLUIDS, 2020, 198
  • [33] NUMERICAL EVALUATION OF EXTINCTION ANGLE AND BIREFRINGENCE IN VARIOUS DIRECTIONS AS A FUNCTION OF VELOCITY-GRADIENT
    CRESSELY, R
    HOCQUART, R
    WYDRO, T
    DECRUPPE, JP
    RHEOLOGICA ACTA, 1985, 24 (04) : 419 - 426
  • [34] Waves and turbulence in magnetohydrodynamic direct numerical simulations
    Dmitruk, Pablo
    Matthaeus, W. H.
    PHYSICS OF PLASMAS, 2009, 16 (06)
  • [35] Bubble generated turbulence and direct numerical simulations
    Joshi J.B.
    Nandakumar K.
    Evans G.M.
    Pareek V.K.
    Gumulya M.M.
    Sathe M.J.
    Khanwale M.A.
    Joshi, Jyeshtharaj B., 1600, Elsevier Ltd (157): : 26 - 75
  • [36] AN EXAMINATION OF FORCING IN DIRECT NUMERICAL SIMULATIONS OF TURBULENCE
    ESWARAN, V
    POPE, SB
    COMPUTERS & FLUIDS, 1988, 16 (03) : 257 - 278
  • [37] Direct Numerical Simulations of Capillary Wave Turbulence
    Deike, Luc
    Fuster, Daniel
    Berhanu, Michael
    Falcon, Eric
    PHYSICAL REVIEW LETTERS, 2014, 112 (23)
  • [38] Direct numerical simulations of turbulence with confinement and rotation
    Godeferd, FS
    Lollini, L
    JOURNAL OF FLUID MECHANICS, 1999, 393 : 257 - 307
  • [39] Study of turbulent boundary layer structure using the invariants of the velocity gradient tensor
    Dept of Mechanical Engineering, Stanford University, Stanford CA 94305, United States
    Exper Therm Fluid Sci, 4 (308-317):
  • [40] Dynamics and geometry of developing planar jets based on the invariants of the velocity gradient tensor
    吴楠楠
    SAKAI Yasuhiko
    NAGATA Kouji
    ITO Yasumasa
    Journal of Hydrodynamics, 2015, 27 (06) : 894 - 906