Effect of turbulent fluctuations on the drag and lift forces on a towed sphere and its boundary layer

TL;DR

This study uses high-resolution simulations to analyze how turbulent fluctuations influence the drag and lift forces on a towed sphere, revealing significant force increases in turbulent conditions and proposing a novel computational approach.

Contribution

The paper introduces a new numerical scheme combining Fourier pseudo-spectral and immersed-boundary methods for simulating particle-fluid interactions in turbulent flows.

Findings

Drag force increases with turbulent intensity and Reynolds number.

Mean velocity deficit follows an inverse relation with distance from the sphere.

Turbulent fluctuations significantly modify the flow around the particle, increasing drag beyond laminar predictions.

Abstract

The impact of turbulent fluctuations on the forces exerted by a fluid on a towed spherical particle is investigated by means of high-resolution direct numerical simulations. The measurements are carried out using a novel scheme to integrate the two-way coupling between the particle and the incompressible surrounding fluid flow maintained in a high-Reynolds-number turbulent regime. The main idea consists in combining a Fourier pseudo-spectral method for the fluid with an immersed-boundary technique to impose the no-slip boundary condition on the surface of the particle. Benchmarking of the code shows a good agreement with experimental and numerical measurements from other groups. A study of the turbulent wake downstream the sphere is also reported. The mean velocity deficit is shown to behave as the inverse of the distance from the particle, as predicted from classical similarity analysis. This law is reinterpreted in terms of the principle of "permanence of large eddies" that relates infrared asymptotic self-similarity to the law of decay of energy in homogeneous turbulence. The developed method is then used to attack the problem of an upstream flow that is in a developed turbulent regime. It is shown that the average drag force increases as a function of the turbulent intensity and the particle Reynolds number. This increase is significantly larger than predicted by standard drag correlations based on laminar upstream flows. It is found that the relevant parameter is the ratio of the viscous boundary layer thickness to the dissipation scale of the ambient turbulent flow. The drag enhancement can be motivated by the modification of the mean velocity and pressure profile around the sphere by small scale turbulent fluctuations.