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风沙输运的颗粒尺度建模与溅蚀参数化

Grain-scale modeling and splash parametrization for aeolian sand transport.

作者信息

Lämmel Marc, Dzikowski Kamil, Kroy Klaus, Oger Luc, Valance Alexandre

机构信息

Institut für Theoretische Physik, Universität Leipzig, Postfach 100920, 04009 Leipzig, Germany.

Institut de Physique de Rennes, CNRS UMR 6251, Université de Rennes I, 35042 Rennes, France.

出版信息

Phys Rev E. 2017 Feb;95(2-1):022902. doi: 10.1103/PhysRevE.95.022902. Epub 2017 Feb 3.

Abstract

The collision of a spherical grain with a granular bed is commonly parametrized by the splash function, which provides the velocity of the rebounding grain and the velocity distribution and number of ejected grains. Starting from elementary geometric considerations and physical principles, like momentum conservation and energy dissipation in inelastic pair collisions, we derive a rebound parametrization for the collision of a spherical grain with a granular bed. Combined with a recently proposed energy-splitting model [Ho et al., Phys. Rev. E 85, 052301 (2012)PLEEE81539-375510.1103/PhysRevE.85.052301] that predicts how the impact energy is distributed among the bed grains, this yields a coarse-grained but complete characterization of the splash as a function of the impact velocity and the impactor-bed grain-size ratio. The predicted mean values of the rebound angle, total and vertical restitution, ejection speed, and number of ejected grains are in excellent agreement with experimental literature data and with our own discrete-element computer simulations. We extract a set of analytical asymptotic relations for shallow impact geometries, which can readily be used in coarse-grained analytical modeling or computer simulations of geophysical particle-laden flows.

摘要

球形颗粒与颗粒床的碰撞通常由飞溅函数来参数化,该函数给出了反弹颗粒的速度以及喷射颗粒的速度分布和数量。从基本的几何考虑和物理原理出发,如非弹性对撞中的动量守恒和能量耗散,我们推导出了球形颗粒与颗粒床碰撞的反弹参数化。结合最近提出的能量分裂模型[Ho等人,《物理评论E》85,052301(2012年)],该模型预测了冲击能量如何在床层颗粒之间分配,这给出了飞溅作为冲击速度和冲击器-床层颗粒尺寸比的函数的粗粒度但完整的表征。预测的反弹角、总恢复系数和垂直恢复系数、喷射速度以及喷射颗粒数量的平均值与实验文献数据以及我们自己的离散元计算机模拟结果非常吻合。我们提取了一组浅冲击几何形状的解析渐近关系,可直接用于地球物理含颗粒流的粗粒度解析建模或计算机模拟。

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