Drop impact onto a liquid layer of finite thickness: Dynamics of the cavity evolution

E Berberović, NP van Hinsberg, S Jakirlić… - Physical Review E …, 2009 - APS
Physical Review E—Statistical, Nonlinear, and Soft Matter Physics, 2009APS
In the present work experimental, numerical, and theoretical investigations of a normal drop
impact onto a liquid film of finite thickness are presented. The dynamics of drop impact on
liquid surfaces, the shape of the cavity, the formation and propagation of a capillary wave in
the crater, and the residual film thickness on the rigid wall are determined and analyzed. The
shape of the crater within the film and the uprising liquid sheet formed upon the impact are
observed using a high-speed video system. The effects of various influencing parameters …
In the present work experimental, numerical, and theoretical investigations of a normal drop impact onto a liquid film of finite thickness are presented. The dynamics of drop impact on liquid surfaces, the shape of the cavity, the formation and propagation of a capillary wave in the crater, and the residual film thickness on the rigid wall are determined and analyzed. The shape of the crater within the film and the uprising liquid sheet formed upon the impact are observed using a high-speed video system. The effects of various influencing parameters such as drop impact velocity, liquid film thickness and physical properties of the liquids, including viscosity and surface tension, on the time evolution of the crater formation are investigated. Complementary to experiments the direct numerical simulations of the phenomena are performed using an advanced free-surface capturing model based on a two-fluid formulation of the classical volume-of-fluid (VOF) model in the framework of the finite volume numerical method. In this model an additional convective term is introduced into the transport equation for phase fraction, contributing decisively to a sharper interface resolution. Furthermore, an analytical model for the penetration depth of the crater is developed accounting for the liquid inertia, viscosity, gravity, and surface tension. The model agrees well with the experiments at the early times of penetration far from the wall if the impact velocity is high. Finally, a scaling analysis of the residual film thickness on the wall is conducted demonstrating a good agreement with the numerical predictions.
American Physical Society
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