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arxiv: 1304.8064 · v1 · pith:3SPKTBGTnew · submitted 2013-04-30 · ⚛️ physics.plasm-ph · astro-ph.SR· math-ph· math.MP

A complete topological invariant for braided magnetic fields

classification ⚛️ physics.plasm-ph astro-ph.SRmath-phmath.MP
keywords magneticfieldfunctiontopologicalfluxcross-sectionfieldsinvariant
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A topological flux function is introduced 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, whose integral over the cross-section yields the relative magnetic helicity. Recognising that the topological flux function is an action in the Hamiltonian formulation of the field line equations, a simple formula for its differential is obtained. We use this to prove that the topological flux function uniquely characterises the field line mapping and hence the magnetic topology. A simple example is presented.

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