Formation of a falling particle curtain

P. Vorobieff, P. Wayne, S. Lingampally, G. Vigil, Josh Ludwigsen, D. Freelong, C. Truman, G. Jacobs
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引用次数: 2

Abstract

Falling particle curtains are important in many engineering applications, including receivers for concentrating solar power facilities. During the formation of such a curtain, we observe a multiphase analog of Rayleigh–Taylor instability (RTI). It was originally described in 2011 for a situation when air sparsely seeded with glycol droplets was placed above a volume of unseeded air, producing an unstably stratified average density distribution that was characterized by an effective Atwood number 0.03. In that case, the evolution of the instability was indistinguishable from single-phase RTI with the same Atwood number, as the presence of the droplets largely acted as an additional contribution to the mean density of the gaseous medium. Here, we present experiments where the volume (and mass) fraction of the seeding particles in gas is considerably higher, and the gravity-driven flow is dominated by the particle movement. In this case, the evolution of the observed instability appears significantly different.
粒子落幕的形成
下落粒子幕在许多工程应用中都很重要,包括聚光太阳能发电设施的接收器。在形成这种帷幕的过程中,我们观察到瑞利-泰勒不稳定性(RTI)的多相模拟。它最初是在2011年描述的一种情况,即将含有乙二醇滴的空气稀疏地放置在未播种的空气上方,产生不稳定的分层平均密度分布,其有效阿特伍德数为0.03。在这种情况下,不稳定性的演变与具有相同阿特伍德数的单相RTI难以区分,因为液滴的存在在很大程度上对气体介质的平均密度起了额外的作用。在这里,我们提出的实验中,播种颗粒在气体中的体积(和质量)分数相当高,并且重力驱动的流动主要由颗粒运动控制。在这种情况下,观察到的不稳定性的演变显得明显不同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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