A method for finding three-dimensional magnetic skeletons

被引:40
|
作者
Haynes, A. L. [1 ]
Parnell, C. E. [1 ]
机构
[1] Univ St Andrews, Dept Math & Stat, St Andrews KY16 9SS, Fife, Scotland
关键词
plasma magnetohydrodynamics; QUASI-SEPARATRIX LAYERS; CURRENT SHEET FORMATION; HYPERBOLIC FLUX TUBES; KINEMATIC RECONNECTION; 3D RECONNECTION; CORONAL FIELD; NULL POINTS; EMERGENCE; TOPOLOGY; COMPLEX;
D O I
10.1063/1.3467499
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Magnetic fields are an essential component of a plasma. In many astrophysical, solar, magnetospheric, and laboratory situations the magnetic field in the plasma can be very dynamic and form highly complex structures. One approach to unraveling these structures is to determine the magnetic skeleton of the field, a set of topological features that divide the magnetic field into topologically distinct domains. In general, the features of the magnetic skeleton are difficult to locate, in particular those given by numerical experiments. In this paper, we propose a new set of tools to find the skeleton of general magnetic fields including null points, spines, separatrix surfaces, and separators. This set of tools is found to be considerably better at finding the skeleton than the currently favored methods used in magnetohydrodynamics. (C) 2010 American Institute of Physics. [doi:10.1063/1.3467499]
引用
收藏
页数:9
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