Transition from laminar to turbulent dynamo: the effect of varying Prandtl number

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-08-20 DOI:10.1080/03091929.2020.1804900
J. Šimkanin, J. Kyselica
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Abstract

We carry out numerical dynamo simulations in a spherical shell to assess the influence of varying Prandtl number on the morphology of the induced magnetic field in both cases when the convection is laminar and turbulent. We work in a regime of large magnetic Prandtl number ( ) due to computational constraints of the full three-dimensional numerical model. We consider dynamos driven by thermal convection in the regimes of small and unit Prandtl numbers. Unlike the laminar convection, in the turbulent regime the morphology of the induced magnetic fields depends only weakly on the Prandtl number. For both values of considered the magnetic field is non-dipolar and small-scale. Together with the previous results of other authors, who found that the morphology of the magnetic field does not change substantially with when is small, the results of our study suggest that the induced magnetic field does not vary substantially with regardless of the strength of the magnetic diffusion.
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层流发电机向湍流发电机的转变:普朗特数变化的影响
我们在一个球壳中进行了数值发电机模拟,以评估在对流为层流和湍流两种情况下,不同普朗特数对感应磁场形态的影响。由于全三维数值模型的计算限制,我们在大磁普朗特数()的情况下工作。我们考虑在小普朗特数和单位普朗特数情况下由热对流驱动的发电机。与层流对流不同,在紊流状态下,感应磁场的形态仅对普朗特数有微弱的依赖。对于考虑的两个值,磁场是非偶极的和小尺度的。结合其他作者之前的研究结果,发现磁场的形态不随时间的小而发生很大的变化,我们的研究结果表明,无论磁扩散的强度如何,感应磁场都不会发生很大的变化。
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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