Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-10-21
Phys. Rev. E 81, 036401 (2010)
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
7 pages, 10 figures
Scientific paper
10.1103/PhysRevE.81.036401
The resistive decay of chains of three interlocked magnetic flux rings is considered. Depending on the relative orientation of the magnetic field in the three rings, the late-time decay can be either fast or slow. Thus, the qualitative degree of tangledness is less important than the actual value of the linking number or, equivalently, the net magnetic helicity. Our results do not suggest that invariants of higher order than that of the magnetic helicity need to be considered to characterize the decay of the field.
Brandenburg Axel
Candelaresi Simon
Sordo Fabio Del
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