Unique topological characterization of braided magnetic fields

被引:26
作者
Yeates, A. R. [1 ]
Hornig, G. [2 ]
机构
[1] Univ Durham, Dept Math Sci, Durham DH1 3LE, England
[2] Univ Dundee, Div Math, Dundee DD1 4HN, Scotland
关键词
SOLAR CORONA; RECONNECTION SCENARIOS; DYNAMICS; RELAXATION; LINES; FORM;
D O I
10.1063/1.4773903
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
We introduce a topological flux function to quantify the topology of magnetic braids: non-zero, line-tied magnetic fields whose field lines all connect between two boundaries. This scalar function is an ideal invariant defined on a cross-section of the magnetic field, and measures the average poloidal magnetic flux around any given field line, or the average pairwise crossing number between a given field line and all others. Moreover, its integral over the cross-section yields the relative magnetic helicity. Using the fact that the flux function is also an action in the Hamiltonian formulation of the field line equations, we prove that it uniquely characterizes the field line mapping and hence the magnetic topology. (C) 2013 American Institute of Physics. [http://dx.doi.org/10.1063/1.4773903]
引用
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页数:5
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