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Abstract
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]
Original language | English |
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Article number | 012102 |
Number of pages | 5 |
Journal | Physics of Plasmas |
Volume | 20 |
Issue number | 1 |
DOIs | |
Publication status | Published - Jan 2013 |
Keywords
- SOLAR CORONA
- DYNAMICS
- RECONNECTION
- RELAXATION
- LINES
- MAPS
- FORM
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Dive into the research topics of 'Unique topological characterization of braided magnetic fields'. Together they form a unique fingerprint.Projects
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Parallel Computing Resources UK MHD: Parallel computing resources
Hood, A. W. (PI)
Science & Technology Facilities Council
1/12/09 → 30/11/12
Project: Standard