反应性球形颗粒在线性分层流体中下落的动力学

L. Huguet, Victor Barge-Zwick, M. L. Bars
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引用次数: 0

摘要

在众多地球物理应用的推动下,我们在大雷诺数和弗劳德数的条件下,在分层环境中进行了反应性(即熔化)实心球在重力作用下自由落体的实验室实验。我们将我们的结果与相同体系下的非反应性球体进行比较。首先,我们确认,对于较大的Re值,先前观察到的低Re和中等Re的分层阻力增强(Magnaudet和Mercier, 2020)。我们还显示了由于融化而产生的更显著的阻力增强,比分层引起的阻力增强大得多。我们认为,这两种增强的机制是相似的,因为浮力效应和相关斜压扭矩所形成的涡度场的特定结构,正如Zhang等人(2019)为分层所解读的那样。利用粒子图像测速技术,我们描述了由球体尾迹产生的内波场的长期演化(时间为$t \gg 1/N$,频率为$N$)。反应球和惰性球的测量波场是相似的:实际上,每个球的下落可以被认为是时间和水平方向上的准脉冲能量源,因为下落时间(p。球面半径)远小于$N$ (p。比槽宽)。内部重力波是由尾流湍流在广谱上产生的,最小阻尼分量在Br\“unt-V\”ais\“al\”a频率和最大允许的水平波长。在探测范围内,每个球体的初始势能约有1%转化为内部波的动能,与弗劳德数没有明显的关系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dynamics of a reactive spherical particle falling in a linearly stratified fluid
Motivated by numerous geophysical applications, we have carried out laboratory experiments of a reactive (i.e. melting) solid sphere freely falling by gravity in a stratified environment, in the regime of large Reynolds ($Re$) and Froude numbers. We compare our results to non-reactive spheres in the same regime. First, we confirm for larger values of $Re$, the stratification drag enhancement previously observed for low and moderate Re (Magnaudet and Mercier, 2020). We also show an even more significant drag enhancement due to melting, much larger than the stratification-induced one. We argue that the mechanism for both enhancements is similar, due to the specific structure of the vorticity field sets by buoyancy effects and associated baroclinic torques, as deciphered for stratification by Zhang et al. (2019). Using particle image velocimetry, we then characterize the long-term evolution (at time $t \gg 1/N$ with $N$ the Br\"unt-V\"ais\"al\"a frequency) of the internal wave field generated by the wake of the spheres. Measured wave field is similar for both reactive and inert spheres: indeed, each sphere fall might be considered as a quasi impulsive source of energy in time and the horizontal direction, as the falling time (resp. the sphere radius) is much smaller than $N$ (resp. than the tank width). Internal gravity waves are generated by wake turbulence over a broad spectrum, with the least damped component being at the Br\"unt-V\"ais\"al\"a frequency and the largest admissible horizontal wavelength. About 1% of the initial potential energy of each sphere is converted in to kinetic energy in the internal waves, with no significant dependence on the Froude number over the explored range.
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