activity
20242026
collaborators

8 papers

physics.flu-dyn2026

Turbophoresis of inertial particles in inhomogeneous turbulence generated by oscillating grids

E. Elmakies, O. Shildkrot, N. Kleeorin +2

Turbophoresis in inhomogeneous turbulent flows leads to the formation of large-scale nonuniform particle number density distributions of inertial particles. This effect is associat…

physics.flu-dyn2026

Experimental study of turbulent thermal diffusion of inertial particles in a convective turbulence forced by oscillating grids

E. Elmakies, O. Shildkrot, N. Kleeorin +2

We investigate the phenomenon of turbulent thermal diffusion of inertial solid particles in laboratory experiments with convective turbulence forced by one or two oscillating grids…

astro-ph.GA2026

Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds

Igor Rogachevskii, Nathan Kleeorin

A joint effect of the density-stratified turbulence (or inhomogeneous turbulence) and a large-scale shear for arbitrary Mach numbers results in the effect and mean-field dynam…

physics.flu-dyn2025

Experimental investigation of turbulence and turbulent thermal diffusion in strongly inhomogeneous and anisotropic forced convection

E. Zarbib, E. Elmakies, O. Shildkrot +3

We investigate properties of turbulence and turbulent transport of non-inertial particles described in terms of turbulent thermal diffusion in strongly inhomogeneous and anisotropi…

physics.flu-dyn2025

Large-scale clustering of inertial particles in a rotating, stratified and inhomogeneous turbulence

Nathan Kleeorin, Igor Rogachevskii

We develop a theory of various kinds of large-scale clustering of inertial particles in a rotating density stratified or inhomogeneous turbulent fluid flows. The large-scale partic…

physics.flu-dyn2025

Theory of the kinetic helicity effect on turbulent diffusion of magnetic and scalar fields

Igor Rogachevskii, Nathan Kleeorin, Axel Brandenburg

Kinetic helicity is a fundamental characteristics of astrophysical turbulent flows. It is not only responsible for the generation of large-scale magnetic fields in the Sun, stars,…