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arXiv 1010.3248physics.flu-dyn
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Shock Wave冲浪的实验研究

Experimental Investigation of Shock Wave Surfing

N. J. Parziale, S. J. Laurence, R Deiterding, H. G. Hornung, J. E. Shepherd

摘要:

在GALCIT马赫数为4.0的路德维希管中对激波冲浪进行了实验研究。冲击波冲浪发生在次级自由体跟随初级自由体形成的弓形冲击之后;冲击波冲浪的一个例子发生在陨石破碎期间。目前研究中的自由体是尼龙球。在Ludwieg管中的每次运行期间,使用高速相机来捕获一系列纹影图像;使用边缘跟踪软件来测量每个球体的位置。速度和加速度是通过处理位置数据得到的。两个球体的半径比和初始取向在测试矩阵中是变化的。球体半径比和初始重心夹角的变化对系统的动力学行为有显著影响。每个流体动力学视频中的气流是从左到右的。马赫数为4.0,每次运行的总压力约为200 kPa。每次运行开始时,球体被拴在一起,没有流动。水流来了,绳子很快就断了。然后,球体是自由体,其主导力是球体表面周围的压力分布,在次级球体的情况下,该压力分布受到冲击波相互作用的强烈操纵。重力不是一个相当大的体力,因为在这些实验中的测试时间很短。可以看到次级球体受到初级体的弓形激波的影响,形成了非常漂亮的轨迹。使用AMROC代码从模拟中获得计算图像。对两个自由飞行的物体进行了全三维模拟,假定为无粘流,从而根据所受的瞬时气动力计算出每个球体的轨迹。

英文摘要:

Shock wave surfing is investigated experimentally in GALCIT's Mach 4.0 Ludwieg Tube. Shock wave surfing occurs when a secondary free-body follows the bow shock formed by a primary free-body; an example of shock wave surfing occurs during meteorite breakup. The free-bodies in the current investigation are nylon spheres. During each run in the Ludwieg tube a high speed camera is used to capture a series of schlieren images; edge tracking software is used to measure the position of each sphere. Velocity and acceleration are had from processing the position data. The radius ratio and initial orientation of the two spheres are varied in the test matrix. The variation of sphere radius ratio and initial angle between the centers of gravity are shown to have a significant effect on the dynamics of the system. The air flow in each fluid dynamics video is from left to right. The Mach number is 4.0 with total pressure in each run of roughly 200kPa. Each run begins with the spheres tethered and no flow. Flow arrives and the tethers are quickly broken. The spheres are then free-bodies with the dominant force being the pressure distribution around the surface of the sphere, which, in the case of the secondary sphere, is strongly manipulated by the shock wave interaction. Gravity is not a considerable body force because of the short test times in these experiments. The secondary spheres are visibly seen to be affected by the bow shock wave of the primary bodies in the form of quite beautiful trajectories. Computational images were obtained from a simulation using the AMROC code. A fully three-dimensional simulation of two free-flying bodies was performed, assuming inviscid flow, whereby the trajectory of each sphere was calculated according to the instantaneous aerodynamic forces experienced.

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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