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首页> 外文期刊>Journal of Fluid Mechanics >Clustering of rapidly settling, low-inertia particle pairs in isotropic turbulence. Part 1. Drift and diffusion flux closures
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Clustering of rapidly settling, low-inertia particle pairs in isotropic turbulence. Part 1. Drift and diffusion flux closures

机译:各向同性湍流快速沉降,低惯性粒子对的聚类。 第1部分漂移和扩散通量闭合

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In this two-part study, we present the development and analysis of a stochastic theory for characterizing the relative positions of monodisperse, low-inertia particle pairs that are settling rapidly in homogeneous isotropic turbulence. In the limits of small Stokes number and Froude number such that Fr ? St_η ? 1, closures are developed for the drift and diffusion fluxes in the probability density function (p.d.f.) equation for the pair relative positions. The theory focuses on the relative motion of particle pairs in the dissipation regime of turbulence, i.e. for pair separations smaller than the Kolmogorov length scale. In this regime, the theory approximates the fluid velocity field in a reference frame following the primary particle as locally linear. In this part 1 paper, we present the derivation of closure approximations for the drift and diffusion fluxes in the p.d.f. equation for pair relative positions r. The drift flux contains the time integral of the third and fourth moments of the ‘seen’ fluid velocity gradients along the trajectories of primary particles. These moments may be analytically resolved by making approximations regarding the ‘seen’ velocity gradient. Accordingly, two closure forms are derived specifically for the drift flux. The first invokes the assumption that the fluid velocity gradient along particle trajectories has a Gaussian distribution. In the second drift closure, we account for the correlation time scales of dissipation rate and enstrophy by decomposing the velocity gradient into the strain-rate and rotation-rate tensors scaled by the turbulent dissipation rate and enstrophy, respectively. An analytical solution to the p.d.f. ?P?(r,θ) is then derived, where θ is the spherical polar angle. It is seen that the p.d.f. has a power-law dependence on separation r of the form ?P?(r,θ) with ~ St_η~2 and β< 0, analogous to that for the radial distribution function of non-settling pairs. An explicit expression is derived for in
机译:在这两部分的研究中,我们展示了表征单分散,低惯性粒子对的相对位置的随机理论的开发和分析,其在均匀各向同性湍流中迅速稳定。在小型斯托克斯号码和弗劳德号码的限制中,使得fr? st_η?如图1所示,对于该对相对位置的概率密度函数(P.D.F.)方程中的漂移和扩散通量,开发了封闭件。该理论侧重于磁湍流耗散制度中粒子对的相对运动,即对小于Kolmogorov长度尺度的对分离。在该制度中,该理论在局部线性的主要粒子之后的参考框架中接近流体速度场。在该第1部分纸张中,我们介绍了P.D.F中漂移和扩散通量的闭合近似的推导。配对相对位置的等式R。漂移通量包含沿着初级粒子轨迹的“看到”流体速度梯度的第三和第四矩的时间积分。通过对“看到”速度梯度的近似来说,可以分析这些瞬间。因此,两个闭合形式衍生用于漂移通量。首先调用假设沿粒子轨迹的流体速度梯度具有高斯分布。在第二漂移闭合中,我们考虑分别将速度梯度分解成湍流耗散速率和敌对的应变速率和旋转速率张量分解散流速率和敌对的相关时间尺度。 p.d.f的分析解决方案。然后导出p?(r,θ),其中θ是球形极性角度。看来p.d.f.具有〜ST_η〜2和β<0的形式的分离r对形式的分离r的动力律依赖性,类似于非沉降对的径向分布函数的形式的α(r,θ)。导出了一个显式表达式

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