从几何角度看MHD和布拉金斯基发电机

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2019-11-15 DOI:10.1080/03091929.2020.1839896
Andrew D. Gilbert, J. Vanneste
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引用次数: 4

摘要

摘要:本文从微分几何的角度考虑了理想流体在一般三维流形上的流动和磁场的动力学,并考虑了磁流体力学及其一些应用。这种抽象层次的好处是,它澄清了流体动力学的基本方面,比如某些量是如何传输的,它们在映射的作用下是如何变换的(例如拉格朗日标签和欧拉位置之间的流图),守恒定律是如何产生的,以及保留经典力学数学结构的某些近似的起源。首先,利用李氏导数和作用原理,在一般情况下导出了理想MHD的控制方程。详细介绍了这些方程在将流体包裹的位置映射到背景位置的拉回下的变换方式。然后利用伪动量和伪场的概念,与流体力学中广义拉格朗日平均理论的发展并行,将其用于参数化alfvsamn波。最后,对非理想MHD进行了研究,并简述了布拉金斯基发电机在一般情况下的发展情况。得到了α-张量的表达式,包括以连接系数表示的新的几何公式,并与文献中其他地方的公式相关。
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A geometric look at MHD and the Braginsky dynamo
ABSTRACT This paper considers magnetohydrodynamics (MHD) and some of its applications from the perspective of differential geometry, considering the dynamics of an ideal fluid flow and magnetic field on a general three-dimensional manifold, equipped with a metric and an induced volume form. The benefit of this level of abstraction is that it clarifies basic aspects of fluid dynamics such as how certain quantities are transported, how they transform under the action of mappings (e.g. the flow map between Lagrangian labels and Eulerian positions), how conservation laws arise, and the origin of certain approximations that preserve the mathematical structure of classical mechanics. First, the governing equations for ideal MHD are derived in a general setting by means of an action principle and making use of Lie derivatives. The way in which these equations transform under a pull back by the map taking the position of a fluid parcel to a background location is detailed. This is then used to parameterise Alfvén waves using concepts of pseudomomentum and pseudofield, in parallel with the development of Generalised Lagrangian Mean theory in hydrodynamics. Finally non-ideal MHD is considered with a sketch of the development of the Braginsky -dynamo in a general setting. Expressions for the α-tensor are obtained, including a novel geometric formulation in terms of connection coefficients, and related to formulae found elsewhere in the literature.
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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.
期刊最新文献
Zonostrophic instabilities in magnetohydrodynamic Kolmogorov flow Scales of vertical motions due to an isolated vortex in ageostrophic balanced flows Can the observable solar activity spectrum be reproduced by a simple dynamo model? Solitary wave scattering by segmented arc-shaped breakwater Self-adjointness of sound-proof models for magnetic buoyancy
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