It is known that the disintegration of vertical liquid curtains (sheets) is affected crucially by the amplification of free edge holes forming inside the curtain. This paper aims to investigate the influence of the hole expansion dynamics, driven by the so-called rim retraction, on the breakup of a liquid curtain, in both supercritical (Weber number 1$]]>) and subcritical (We) conditions. The analysis is based on three-dimensional direct numerical simulations. For a selected supercritical configuration, the steady flow topology is first analysed. The investigation reveals the classic triangular shape regime of the steady curtain, due to the surface-tension-induced borders retraction towards its centre plane. The unsteady dynamics is then investigated as the curtain response to a hole perturbation introduced artificially in the steady flow configuration. The hole evolution determines a rim retraction phenomenon inside the curtain, which is influenced by both capillary and gravity forces. In supercritical conditions, the hole does not influence the curtain flow dynamics in the long-time limit. By reducing the Weber number slightly under the critical threshold , the initial amplification rate of the hole area increases, due to the stronger retraction effect of surface tension acting on the hole rims. The free hole expansion in fully subcritical conditions (We) is investigated finally by simulating an edge-free curtain flow. As decreases progressively, the hole expands while it is convected downstream by gravity acceleration. In the range 0.4< We, the subcritical curtain returns to the intact unperturbed configuration after the hole expulsion at the downstream outflow. For We, the surface tension force becomes strong enough to reverse the gravitational motion of the hole top point, which retracts upstream towards the sheet inlet section while expanding along the lateral directions. This last phenomenon causes finally the breakup of the curtain, which results in a columnar regime strictly resembling similar experimental findings of the literature.
Hole-driven dynamics of a three-dimensional gravitational liquid curtain / Acquaviva, MARIA ROSARIA; DELLA PIA, Alessandro; Chiatto, Matteo; DE LUCA, Luigi. - In: JOURNAL OF FLUID MECHANICS. - ISSN 1469-7645. - 968:(2023). [10.1017/jfm.2023.543]
Hole-driven dynamics of a three-dimensional gravitational liquid curtain
Maria Rosaria Acquaviva
Primo
;Alessandro Della PiaSecondo
;Matteo ChiattoPenultimo
;Luigi de LucaUltimo
2023
Abstract
It is known that the disintegration of vertical liquid curtains (sheets) is affected crucially by the amplification of free edge holes forming inside the curtain. This paper aims to investigate the influence of the hole expansion dynamics, driven by the so-called rim retraction, on the breakup of a liquid curtain, in both supercritical (Weber number 1$]]>) and subcritical (We) conditions. The analysis is based on three-dimensional direct numerical simulations. For a selected supercritical configuration, the steady flow topology is first analysed. The investigation reveals the classic triangular shape regime of the steady curtain, due to the surface-tension-induced borders retraction towards its centre plane. The unsteady dynamics is then investigated as the curtain response to a hole perturbation introduced artificially in the steady flow configuration. The hole evolution determines a rim retraction phenomenon inside the curtain, which is influenced by both capillary and gravity forces. In supercritical conditions, the hole does not influence the curtain flow dynamics in the long-time limit. By reducing the Weber number slightly under the critical threshold , the initial amplification rate of the hole area increases, due to the stronger retraction effect of surface tension acting on the hole rims. The free hole expansion in fully subcritical conditions (We) is investigated finally by simulating an edge-free curtain flow. As decreases progressively, the hole expands while it is convected downstream by gravity acceleration. In the range 0.4< We, the subcritical curtain returns to the intact unperturbed configuration after the hole expulsion at the downstream outflow. For We, the surface tension force becomes strong enough to reverse the gravitational motion of the hole top point, which retracts upstream towards the sheet inlet section while expanding along the lateral directions. This last phenomenon causes finally the breakup of the curtain, which results in a columnar regime strictly resembling similar experimental findings of the literature.File | Dimensione | Formato | |
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