中国物理B ›› 2007, Vol. 16 ›› Issue (10): 2848-2854.doi: 10.1088/1009-1963/16/10/004
陈式刚1, 王光瑞1, 赵英奎2
Zhao Ying-Kui(赵英奎)a)b)†, Chen Shi-Gang(陈式刚)b), and Wang Guang-Rui(王光瑞)b)
摘要: In this paper, we have introduced a shell-model of Kraichnan's passive scalar problem. Different from the original problem, the prescribed random velocity field is non-Gaussian and $\delta$ correlated in time, and its introduction is inspired by She and L\'{e}v\^{e}que (Phys. Rev. Lett. {\bf 72}, 336 (1994)). For comparison, we also give the passive scalar advected by the Gaussian random velocity field. The anomalous scaling exponents $H(p)$ of passive scalar advected by these two kinds of random velocities above are determined for structure function with values of $p$ up to 15 by Monte Carlo simulations of the random shell model, with Gear methods used to solve the stochastic differential equations. We find that the $H(p)$ advected by the non-Gaussian random velocity is not more anomalous than that advected by the Gaussian random velocity. Whether the advecting velocity is non-Gaussian or Gaussian, similar scaling exponents of passive scalar are obtained with the same molecular diffusivity.
中图分类号: (Fluctuation phenomena, random processes, noise, and Brownian motion)