An experimental study on the settling velocity of inertial particles in different homogeneous isotropic turbulent flows

TL;DR

This experimental study investigates how turbulence intensity, flow conditions, and large-scale forcing affect the settling velocity of inertial particles in isotropic turbulent flows, revealing dependencies on Reynolds number, Rouse number, and volume fraction.

Contribution

It provides new experimental data on inertial particle settling velocities across a wide range of turbulence conditions and examines the effects of flow forcing and secondary flows.

Findings

Settling velocity enhancement decreases with increasing Reynolds number.

Higher volume fractions significantly affect settling velocity modifications.

Large-scale forcing alters particle settling behavior under similar turbulence intensities.

Abstract

We propose an experimental study on the gravitational settling velocity of dense, sub-Kolmogorov inertial particles under different background turbulent flows. We report Phase Doppler Particle Analyzer measurements in a low-speed wind tunnel uniformly seeded with micrometer scale water droplets. Turbulence is generated with three different grids (two consisting on different active-grid protocols while the third is a regular static grid), allowing us to cover a very wide range of turbulence conditions in terms of Taylor-scale based Reynolds numbers ($Re_\lambda \in [30-520]$), Rouse numbers ($Ro \in [0-5]$) and volume fractions ($\phi_v \in[0.5\times10^{-5} - 2.0\times10^{-5}]$). We find, in agreement with previous works, that enhancement of the settling velocity occurs at low Rouse number, while hindering of the settling occurs at higher Rouse number for decreasing turbulence energy levels. The wide range of flow parameters explored allowed us to observe that enhancement decreases significantly with the Taylor Reynolds number and is significantly affected by the volume fraction $\phi_v$. We also studied the effect of large-scale forcing on settling velocity modification. The possibility of changing the inflow conditions by using different grids allowed us to test cases with fixed $Re_\lambda$ and turbulent intensity but different integral length scale. Finally, we assess the existence of secondary flows in the wind tunnel and their role on particle settling. This is achieved by characterising the settling velocity at two different positions, the centreline and close to the wall, with the same streamwise coordinate.