Turbulent pair dispersion in the presence of gravity

Turbulent pair dispersion of heavy particles is strongly altered when particles of two different Stokes numbers (bidisperse) are considered, and this is further compounded when a uniform gravitational acceleration is present. Lagrangian trajectories of fluid tracers, and bidisperse heavy particles w...

Full description

Bibliographic Details
Main Authors: Kelken Chang, Benedict J Malec, Raymond A Shaw
Format: Article
Language:English
Published: IOP Publishing 2015-01-01
Series:New Journal of Physics
Subjects:
Online Access:https://doi.org/10.1088/1367-2630/17/3/033010
_version_ 1797751188660158464
author Kelken Chang
Benedict J Malec
Raymond A Shaw
author_facet Kelken Chang
Benedict J Malec
Raymond A Shaw
author_sort Kelken Chang
collection DOAJ
description Turbulent pair dispersion of heavy particles is strongly altered when particles of two different Stokes numbers (bidisperse) are considered, and this is further compounded when a uniform gravitational acceleration is present. Lagrangian trajectories of fluid tracers, and bidisperse heavy particles with and without gravity were calculated from a direct numerical simulation of homogeneous, isotropic turbulence. Particle pair dispersion shows a short-time, ballistic (Batchelor) regime and a transition to super-ballistic dispersion that is suggestive of the emergence of Richardson scaling. A simple equation of motion for inertial, sedimenting particles captures the essential features of the pair dispersion at very short time and length scales. Kolmogorov scaling arguments are able to qualitatively describe the competition between gravity-induced and fluid-induced relative motion in modifying the amount of time the heavy particles spend in the ballistic regime. The transition from ballistic to super-ballistic dispersion for fluid tracers and monodisperse inertial particles exhibits a pronounced sub-ballistic behavior that can be attributed to the mixed velocity–acceleration structure function. The sub-ballistic behavior is strongly suppressed for bidisperse particles, both in the presence or absence of gravity, primarily because of a reduction in the correlation between velocity and acceleration increments.
first_indexed 2024-03-12T16:44:53Z
format Article
id doaj.art-c3619b56e9c34991a1fd29eee2271437
institution Directory Open Access Journal
issn 1367-2630
language English
last_indexed 2024-03-12T16:44:53Z
publishDate 2015-01-01
publisher IOP Publishing
record_format Article
series New Journal of Physics
spelling doaj.art-c3619b56e9c34991a1fd29eee22714372023-08-08T14:18:10ZengIOP PublishingNew Journal of Physics1367-26302015-01-0117303301010.1088/1367-2630/17/3/033010Turbulent pair dispersion in the presence of gravityKelken Chang0Benedict J Malec1Raymond A Shaw2Department of Physics, Michigan Technological UniversityDepartment of Physics, Michigan Technological UniversityDepartment of Physics, Michigan Technological UniversityTurbulent pair dispersion of heavy particles is strongly altered when particles of two different Stokes numbers (bidisperse) are considered, and this is further compounded when a uniform gravitational acceleration is present. Lagrangian trajectories of fluid tracers, and bidisperse heavy particles with and without gravity were calculated from a direct numerical simulation of homogeneous, isotropic turbulence. Particle pair dispersion shows a short-time, ballistic (Batchelor) regime and a transition to super-ballistic dispersion that is suggestive of the emergence of Richardson scaling. A simple equation of motion for inertial, sedimenting particles captures the essential features of the pair dispersion at very short time and length scales. Kolmogorov scaling arguments are able to qualitatively describe the competition between gravity-induced and fluid-induced relative motion in modifying the amount of time the heavy particles spend in the ballistic regime. The transition from ballistic to super-ballistic dispersion for fluid tracers and monodisperse inertial particles exhibits a pronounced sub-ballistic behavior that can be attributed to the mixed velocity–acceleration structure function. The sub-ballistic behavior is strongly suppressed for bidisperse particles, both in the presence or absence of gravity, primarily because of a reduction in the correlation between velocity and acceleration increments.https://doi.org/10.1088/1367-2630/17/3/033010turbulenceinertial particlesnumerical simulations
spellingShingle Kelken Chang
Benedict J Malec
Raymond A Shaw
Turbulent pair dispersion in the presence of gravity
New Journal of Physics
turbulence
inertial particles
numerical simulations
title Turbulent pair dispersion in the presence of gravity
title_full Turbulent pair dispersion in the presence of gravity
title_fullStr Turbulent pair dispersion in the presence of gravity
title_full_unstemmed Turbulent pair dispersion in the presence of gravity
title_short Turbulent pair dispersion in the presence of gravity
title_sort turbulent pair dispersion in the presence of gravity
topic turbulence
inertial particles
numerical simulations
url https://doi.org/10.1088/1367-2630/17/3/033010
work_keys_str_mv AT kelkenchang turbulentpairdispersioninthepresenceofgravity
AT benedictjmalec turbulentpairdispersioninthepresenceofgravity
AT raymondashaw turbulentpairdispersioninthepresenceofgravity