Lagrangian vs Eulerian view on the mean drift and streaming flows in orbital sloshing
Alessandro Bongarzone, Fran\c{c}ois Gallaire

TL;DR
This paper investigates the differences between Lagrangian and Eulerian flows in orbital sloshing, using a combined analytical and experimental approach to clarify the contributions of viscous effects and wave dynamics.
Contribution
It introduces a truncated asymptotic approximation to distinguish Lagrangian and Eulerian flows in viscous orbital sloshing, validated by experiments and numerical analysis.
Findings
Viscous effects significantly influence the mean flow structure.
The analytical model agrees well with experiments off-resonance.
Viscous corrections to Stokes drift are crucial for accurate flow description.
Abstract
Orbital sloshing is a technique to gently mix a container's liquid content and it is commonly used in fermentation and cell cultivation processes. Besides the rich wave dynamics observed at the interface, Bouvard et al. (2017) [1] unveiled the structure of the Lagrangian mean flow hiding in the fluid bulk. The latter flow shows a global toroidal (azimuthal) rotation co-directed with the wave and nontrivial poloidal vortices near the contact line. Rotating sloshing waves are known to induce a net motion of fluid particles and hence a wave-averaged difference between the Eulerian flow - viscous streaming - and the Lagrangian flow, that is commonly referred to as Stokes drift. Nevertheless, discerning these two components in an experiment is challenging as they scale similarly with the forcing amplitude and frequency. Their relative contributions remain therefore unquantified, particularly…
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Taxonomy
TopicsAstro and Planetary Science · Geophysics and Gravity Measurements · Spacecraft and Cryogenic Technologies
