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arXiv 1708.04049physics.flu-dyn
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来自非球形空化气泡的Shock waves

Shock waves from non-spherical cavitation bubbles

Outi Supponen, Danail Obreschkow, Philippe Kobel, Marc Tinguely, Nicolas Dorsaz, Mohamed Farhat

摘要:

我们提出了详细的观察,在单一的空化气泡崩溃时发出的冲击波,同时使用时间分辨阴影和水听器压力测量。气泡的几何形状系统地从球形变化到非常非球形,通过减小它们到自由或刚性表面的距离或通过调制抛物线飞行上的重力引起的压力梯度。非球形的崩溃产生多个冲击,显然与不同的过程,如射流的影响和不同的气泡段的个人崩溃。对于在自由表面附近塌陷的气泡,作为各向异性参数$ζ$的函数,分别测量每个冲击的能量和时间,该参数代表开尔文脉冲的无量纲等效值。对于给定的气泡变形源(自由表面、刚性表面或重力),归一化激波能量仅取决于$ζ$,而与气泡半径$R_{0}$和驱动压力$Δp$无关。基于这一发现,我们开发了一个预测框架的峰值压力和能量的冲击波从非球形气泡崩溃。结合实验数据的统计分析和理论推导,我们发现冲击波峰值压力可以用射流冲击诱导的锤击压力来估算,表示为$p_{h} = 0.45\left(ρc^{2}Δp\right)^{1/2} ζ^{-1}$ at $ζ> 10^{-3}$。同样的方法被发现来解释作为$ζ^{-2/3}$的函数的冲击能量淬火。

英文摘要:

We present detailed observations of the shock waves emitted at the collapse of single cavitation bubbles using simultaneous time-resolved shadowgraphy and hydrophone pressure measurements. The geometry of the bubbles is systematically varied from spherical to very non-spherical by decreasing their distance to a free or rigid surface or by modulating the gravity-induced pressure gradient aboard parabolic flights. The non-spherical collapse produces multiple shocks that are clearly associated with different processes, such as the jet impact and the individual collapses of the distinct bubble segments. For bubbles collapsing near a free surface, the energy and timing of each shock are measured separately as a function of the anisotropy parameter $ζ$, which represents the dimensionless equivalent of the Kelvin impulse. For a given source of bubble deformation (free surface, rigid surface or gravity), the normalized shock energy depends only on $ζ$, irrespective of the bubble radius $R_{0}$ and driving pressure $Δp$. Based on this finding, we develop a predictive framework for the peak pressure and energy of shock waves from non-spherical bubble collapses. Combining statistical analysis of the experimental data with theoretical derivations, we find that the shock peak pressures can be estimated as jet impact-induced hammer pressures, expressed as $p_{h} = 0.45\left(ρc^{2}Δp\right)^{1/2} ζ^{-1}$ at $ζ> 10^{-3}$. The same approach is found to explain the shock energy quenching as a function of $ζ^{-2/3}$.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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