Topological constraints on magnetic field relaxation
Abstract
Magnetic field relaxation is determined by both the field's geometry and its topology. For relaxation processes, however, it turns out that its topology is a much more stringent constraint. As quantifier for the topology we use magnetic helicity and test whether it is a stronger condition than the linking of field lines. Further, we search for evidence of other topological invariants, which give rise to further restrictions in the field's relaxation. We find that magnetic helicity is the sole determinant in most cases. Nevertheless, we see evidence for restrictions not captured through magnetic helicity.
- Publication:
-
Solar and Astrophysical Dynamos and Magnetic Activity
- Pub Date:
- July 2013
- DOI:
- arXiv:
- arXiv:1212.0879
- Bibcode:
- 2013IAUS..294..353C
- Keywords:
-
- Magnetic field relaxation;
- magnetic helicity;
- field topology;
- Astrophysics - Solar and Stellar Astrophysics;
- Mathematics - General Topology;
- Physics - Plasma Physics
- E-Print:
- 5 pages, 5 figures, proceedings of IAU Symp. 294, Solar and Astrophysical Dynamos and Magnetic Activity