Detection of turbulent thermal diffusion of particles in numerical simulations
arXiv:1101.4188 · doi:10.1063/1.4733450
Abstract
The phenomenon of turbulent thermal diffusion in temperature-stratified turbulence causing a non-diffusive turbulent flux of inertial and non-inertial particles in the direction of the turbulent heat flux is found using direct numerical simulations (DNS). In simulations with and without gravity, this phenomenon is found to cause a peak in the particle number density around the minimum of the mean fluid temperature for Stokes numbers less than 1, where the Stokes number is the ratio of particle Stokes time to turbulent Kolmogorov time at the viscous scale. Turbulent thermal diffusion causes the formation of large-scale inhomogeneities in the spatial distribution of inertial particles. The strength of this effect is maximum for Stokes numbers around unity, and decreases again for larger values. The dynamics of inertial particles is studied using Lagrangian modelling in forced temperature-stratified turbulence, whereas non-inertial particles and the fluid are described using DNS in an Eulerian framework.
9 pages, 6 figures, REVTEX4-1, extended paper
References in corpus (6)
- Heavy particle concentration in turbulence at dissipative and inertial scales
- Turbulent pair dispersion of inertial particles
- Hydrodynamic and hydromagnetic energy spectra from large eddy simulations
- Turbulent Diffusion and Turbulent Thermal Diffusion of Aerosols in Stratified Atmospheric Flows
- Tangling clustering of inertial particles in stably stratified turbulence
- Turbulent thermal diffusion in a multi-fan turbulence generator with the imposed mean temperature gradient
Cited by in corpus (18)
- Tangling clustering instability for small particles in temperature stratified turbulence
- Turbophoresis in forced inhomogeneous turbulence
- Compressibility in turbulent MHD and passive scalar transport: mean-field theory
- Turbulent thermal diffusion in strongly stratified turbulence: theory and experiments
- Turbulent Thermal Diffusion: A Way to Concentrate Dust in Protoplanetary Discs
- Spectral characterisation of inertial particle clustering in turbulence
- Turbulent magnetic helicity fluxes in solar convective zone
- Energy and flux budget closure theory for passive scalar in stably stratified turbulence
- Experimental study of turbulent thermal diffusion of particles in an inhomogeneous forced convective turbulence
- Experimental study of turbulent transport of nanoparticles in convective turbulence
- Turbulent diffusion of chemically reacting gaseous admixtures
- Experimental study of turbulent thermal diffusion of particles in inhomogeneous and anisotropic turbulence
- Large-scale clustering of inertial particles in a rotating, stratified and inhomogeneous turbulence
- Helicity effect on turbulent passive and active scalar diffusivities
- Compressibility effects in a turbulent transport of temperature field
- Generation of a large-scale vorticity in a fast rotating density stratified turbulence or turbulent convection
- Experimental investigation of turbulence and turbulent thermal diffusion in strongly inhomogeneous and anisotropic forced convection
- Turbulent transport of radiation in the solar convective zone