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首页> 外文期刊>International Journal of Multiphase Flow >High-fidelity modeling and numerical simulation of cratering induced by the interaction of a supersonic jet with a granular bed of solid particles
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High-fidelity modeling and numerical simulation of cratering induced by the interaction of a supersonic jet with a granular bed of solid particles

机译:超声波射流与颗粒状固体颗粒相互作用诱导的高保真建模与数值模拟

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AbstractThe dynamics of cratering caused by a supersonic jet on a granular bed of solid particles is investigated using a high fidelity, two-phase model and numerical simulations. To model the gas phase, the Large Eddy Simulation (LES) approach is used and a kinetic theory based model is employed for the solid phase. Three-dimensional time-dependent simulations are conducted for the purpose of elucidating the morphological features of the crater and their evolution with time. Parametric variations of the initial conditions are performed to understand the effect of the initial solid volume fraction in the bed, of the coefficient of restitution, of the jet Mach number, of the particle diameter, and of the particle material density. Simulation snapshots of the craters are in qualitative agreement with images from the Mars Science Laboratory (MSL) mission and from Earth-based experiments. Analysis of the results shows that solid particle compaction at the crater base and side walls increases with increasing volume fraction of the undisturbed particle bed and reaches solid volume fractions close to 0.65. The coefficient of restitution is shown to have no effect on the large scale dynamics of the crater but affects the small scale features, particularly the shape of elongated bursts of solid particle clouds as well as radially aligned structures on the outer crater walls. A smaller jet Mach number results in a smaller crater characterized by ridge-like structures and walls at an angle of approximately 45° with respect to the undisturbed bed whereas larger Mach number jets create craters with walls approximately perpendicular to the undisturbed bed. A smaller particle size and a lighte
机译:<![cdata [ 抽象 使用高保真,两相模型和数值模拟研究了由超音速射流上的超音速喷射器引起的陨石坑的动态。为了模拟气相,使用大涡模拟(LES)方法,采用基于动力学理论的模型来用于固相。为了阐明火山口的形态特征及其随着时间的推移,进行三维时间依赖模拟。进行初始条件的参数变化以了解床中初始固体体积分数的效果,粒径和颗粒材料密度的恢复系数的恢复系数的恢复系数。探测陨石坑的仿真快照与来自火星科学实验室(MSL)使命和基于地球实验的图像进行定性协议。结果分析表明,在不受干扰的颗粒床的增加的体积分数上增加了火山口底座和侧壁处的固体颗粒压缩,并且达到近0.65的固体体积级分。显示恢复系数对火山口的大规模动力学没有影响,而是影响小规模特征,特别是固体颗粒云的细长突发的形状以及外部火山口壁上的径向对齐结构。较小的喷射马赫数导致较小的喷雾器,其特征在于脊状结构和相对于未受干扰的床的角度,壁以大约45°的角度,而较大的马赫数夹具产生壁的陨石布,壁大约垂直于未受干扰的床。较小的粒径和灯光

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