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arXiv 1006.5585nlin.CD
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均匀各向同性磁流体动力学turbulence的磁普朗特数依赖性的系统学

Systematics of the magnetic-Prandtl-number dependence of homogeneous, isotropic magnetohydrodynamic turbulence

Ganapati Sahoo, Prasad Perlekar, Rahul Pandit

摘要:

我们提出了我们详细的伪谱直接数值模拟(DNS)的研究结果,与$1024^3$配置点,不可压缩,磁流体动力学(MHD)湍流在三维空间,没有平均磁场。我们的研究集中在衰减和统计稳定的MHD湍流的各种统计特性的依赖磁普朗特数${\rm Pr_M}$在一个大的范围内,即$0.01 \leq {\rm Pr_M} \leq 10$。我们获得了各种各样的统计测量数据,如涡度和电流密度模量的概率分布函数(PDF),能量耗散率,速度和磁场增量,能量和其他光谱,速度和磁场结构函数,我们使用它们来解释涡度和电流密度,如涡度和电流模量等量的等值面,以及诸如流体和磁耗散率的联合PDF。我们的系统研究揭示了迄今为止尚未注意到的有趣结果。特别是,我们发现了一个交叉,从磁场中较大的不稳定性比在速度场,在大${\rm Pr_M}$,在磁场中较小的不稳定性比在速度场,在低${\rm Pr_M}$。此外,我们的结果的衰减MHD湍流和它的强迫,统计稳定的模拟比较表明,我们有很强的普遍性的意义上说,对于一个固定的值${\rm Pr_M}$,多标度指数比同意,至少在我们的误差棒,衰减和统计稳定的均匀,各向同性MHD湍流。

英文摘要:

We present the results of our detailed pseudospectral direct numerical simulation (DNS) studies, with up to $1024^3$ collocation points, of incompressible, magnetohydrodynamic (MHD) turbulence in three dimensions, without a mean magnetic field. Our study concentrates on the dependence of various statistical properties of both decaying and statistically steady MHD turbulence on the magnetic Prandtl number ${\rm Pr_M}$ over a large range, namely, $0.01 \leq {\rm Pr_M} \leq 10$. We obtain data for a wide variety of statistical measures such as probability distribution functions (PDFs) of moduli of the vorticity and current density, the energy dissipation rates, and velocity and magnetic-field increments, energy and other spectra, velocity and magnetic-field structure functions, which we use to characterise intermittency, isosurfaces of quantities such as the moduli of the vorticity and current, and joint PDFs such as those of fluid and magnetic dissipation rates. Our systematic study uncovers interesting results that have not been noted hitherto. In particular, we find a crossover from larger intermittency in the magnetic field than in the velocity field, at large ${\rm Pr_M}$, to smaller intermittency in the magnetic field than in the velocity field, at low ${\rm Pr_M}$. Furthermore, a comparison of our results for decaying MHD turbulence and its forced, statistically steady analogue suggests that we have strong universality in the sense that, for a fixed value of ${\rm Pr_M}$, multiscaling exponent ratios agree, at least within our errorbars, for both decaying and statistically steady homogeneous, isotropic MHD turbulence.

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