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Comparative statistics of selected subgrid-scale models in large-eddy simulations of decaying, supersonic magnetohydrodynamic turbulence

机译:衰减大型铸模大型模拟中所选亚级尺度模型的比较统计,超声磁力流体动力学湍流

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摘要

Large-eddy simulations (LES) are a powerful tool in understanding processes that are inaccessible by directsimulations due to their complexity, for example, in the highly turbulent regime. However, their accuracyand success depends on a proper subgrid-scale (SGS) model that accounts for the unresolved scales in thesimulation.We evaluate the applicability of two traditional SGS models, namely the eddy-viscosity (EV) and thescale-similarity (SS) models, and one recently proposed nonlinear (NL) SGS model in the realm of compressiblemagnetohydrodynamic (MHD) turbulence. Using 209 simulations of decaying, supersonic (initial sonic Machnumber M_s ≈ 3) MHD turbulence with a shock-capturing scheme and varying resolution, SGS model, and filter,we analyze the ensemble statistics of kinetic and magnetic energy spectra and structure functions. Furthermore,we compare the temporal evolution of lower- and higher-order statistical moments of the spatial distributions ofkinetic and magnetic energy, vorticity, current density, and dilatation magnitudes.We find no statistical influenceon the evolution of the flow by any model if grid-scale quantities are used to calculate SGS contributions. Inaddition, the SS models, which employ an explicit filter, have no impact in general. On the contrary, both the EVand NL models change the statistics if an explicit filter is used. For example, they slightly increase the dissipationon the smallest scales. We demonstrate that the nonlinear model improves higher-order statistics already witha small explicit filter, i.e., a three-point stencil. The results of, e.g., the structure functions or the skewness andkurtosis of the current density distribution are closer to the ones obtained from simulations at higher resolution.In addition, no additional regularization to stabilize the model is required.We conclude that the nonlinear modelwith a small explicit filter is suitable for application in more complex scenarios when higher-order statistics areimportant.
机译:大涡模拟(LES)是一种强大的工具,可以在理解进程无法访问的过程中例如,仿真由于它们的复杂性,例如,在高度动荡的状态下。但是,他们的准确性和成功取决于一个适当的子字符级(SGS)模型,其占尚未解决的尺度仿真。我们评估了两种传统SGS模型的适用性,即涡粘度(EV)和尺度相似性(SS)模型,以及最近提出的可压缩领域的非线性(NL)SGS模型磁力流体动力学(MHD)湍流。使用209模拟腐烂,超音速(初始声波马赫)数字M_S≈3)MHD湍流,具有冲击捕获方案和不同分辨率,SGS模型和过滤器,我们分析了动力学和磁能光谱和结构功能的集合统计。此外,我们比较了空间分布的低阶和高阶统计时刻的时间演变动力学和磁能,涡流,电流密度和扩张大小。我们没有发现统计影响在任何模型中,如果使用网格级数量来计算SGS贡献,则流动的进化。在另外,采用显式过滤器的SS模型一般没有影响。相反,ev如果使用显式过滤器,则NL模型更改统计信息。例如,它们略微增加了耗散在最小的鳞片上。我们证明非线性模型已经提高了高阶统计数据一个小的显式过滤器,即三点模版。结果,例如结构功能或偏斜电流密度分布的Kurtosis更接近从较高分辨率的模拟中获得的。此外,不需要额外的正则化来稳定模型。我们得出结论是非线性模型使用小型显式过滤器适用于在高阶统计数据中以更复杂的情况应用于应用程序重要的。

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  • 来源
    《PHYSICAL REVIEW E》 |2017年第4期|033206.1-033206.12|共12页
  • 作者单位

    Max-Planck-Institut fuer Sonnensystemforschung Justus-von-Liebig-Weg 3 D-37077 Goettingen Germany and Institut fuer Astrophysik Universitaet Goettingen Friedrich-Hund-Platz 1 D-37077 Goettingen Germany;

    Max-Planck-Institut fuer Dynamik und Selbstorganisation Am Fassberg 17 D-37077 Goettingen Germany;

    Hamburger Sternwarte Universitaet Hamburg Gojenbergsweg 112 D-21029 Hamburg Germany;

    Departamento de Astronomia Facultad Ciencias Fisicas y Matematicas Universidad de Concepcion Av. Esteban Iturra s Barrio Universitario Casilla 160-C Chile;

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