Acceleration statistics of inertial particles from high resolution DNS turbulence

被引:3
|
作者
Toschi, Federico [1 ]
Bec, Jeremie [2 ]
Biferale, Luca [3 ]
Boffetta, Guido [4 ]
Celani, Antonio [5 ]
Cencini, Massimo [6 ]
Lanotte, Alessandra S. [7 ]
Musacchio, Stefano [8 ]
机构
[1] CNR, IAC, Viale Policlin 137, I-00161 Rome, Italy
[2] CNRS, Paris, France
[3] Univ Rome, Dept Phys, INFN, Rome, Italy
[4] Univ Turin, Dept Phys, Turin, Italy
[5] CNRS, Valbonne, France
[6] Univ Rome, Dept Phys, Rome, Italy
[7] CNR, Lecce, Italy
[8] Univ Turin, Ist Nazl Fis Nucl, Dept Phys, Turin, Italy
关键词
Lagrangian turbulence; heavy particles; Stokes particles; acceleration statistics;
D O I
10.1007/978-1-4020-6472-2_11
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results from recent direct numerical simulations of heavy particle transport in homogeneous, isotropic, fully developed turbulence, with grid resolution up to 512(3) and R-lambda approximate to 185. By following the trajectories of millions of particles with different Stokes numbers, St is an element of [0.16 : 3.5], we are able to characterize in full detail the statistics of particle acceleration. We focus on the probability density function of the normalised acceleration a/a(rms) and on the behaviour of their root-mean-squared acceleration a(rms) as a function of both St and R-lambda. We explain our findings in terms of two concurrent mechanisms: particle clustering, very effective for small St, and filtering induced by finite particle response time, taking over at larger St.
引用
收藏
页码:73 / +
页数:2
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