Passive scalar mixing and decay at finite correlation times in the Batchelor regime

被引:4
作者
Aiyer, Aditya K. [1 ,2 ,3 ]
Subramanian, Kandaswamy [4 ]
Bhat, Pallavi [4 ,5 ,6 ,7 ]
机构
[1] BITS Pilani, KK Birla Goa Campus, Zuarinagar 403726, Goa, India
[2] TIFR Ctr Interdisciplinary Sci Narsingi, Hyderabad 500075, Andhra Pradesh, India
[3] Johns Hopkins Univ, Dept Mech Engn, Baltimore, MD 21218 USA
[4] IUCAA, Post Bag 4, Pune 411007, Maharashtra, India
[5] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08543 USA
[6] Princeton Univ, Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA
[7] MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA
关键词
mixing; turbulent mixing; MAGNETIC-FIELD; HYDROMAGNETIC TURBULENCE; RANDOM FLOW; DYNAMO; SPECTRUM; SIMULATIONS; STATISTICS; FLUID;
D O I
10.1017/jfm.2017.364
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
An elegant model for passive scalar mixing and decay was given by Kraichnan (Phys. Fluids, vol. 11, 1968, pp. 945-953) assuming the velocity to be delta correlated in time. For realistic random flows this assumption becomes invalid. We generalize the Kraichnan model to include the effects of a finite correlation time, tau, using renewing flows. The generalized evolution equation for the three-dimensional (3-D) passive scalar spectrum ((M) over capk,t) or its correlation function M(r, t), gives the Kraichnan equation when tau -> 0, and extends it to the next order in tau. It involves third-and fourth-order derivatives of M or (M) over cap (in the high k limit). For small-tau (or small Kubo number), it can be recast using the Landau-Lifshitz approach to one with at most second derivatives of (M) over cap. We present both a scaling solution to this equation neglecting diffusion and a more exact solution including diffusive effects. To leading order in tau, we first show that the steady state 1-D passive scalar spectrum, preserves the Batchelor (J. Fluid Mech., vol. 5, 1959, pp. 113-133) form, E-theta(k) proportional to k(-1), in the viscous-convective limit, independent of tau. This result can also be obtained in a general manner using Lagrangian methods. Interestingly, in the absence of sources, when passive scalar fluctuations decay, we show that the spectrum in the Batchelor regime at late times is of the form E-theta(k) proportional to k(1/2) and also independent of tau. More generally, finite tau does not qualitatively change the shape of the spectrum during decay. The decay rate is however reduced for finite tau. We also present results from high resolution (1024(3)) direct numerical simulations of passive scalar mixing and decay. We find reasonable agreement with predictions of the Batchelor spectrum during steady state. The scalar spectrum during decay is however dependent on initial conditions. It agrees qualitatively with analytic predictions when power is dominantly in wavenumbers corresponding to the Batchelor regime, but is shallower when box-scale fluctuations dominate during decay.
引用
收藏
页码:785 / 817
页数:33
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