Our aim is to investigate the resistive relaxation of a magnetic loop that contains braided magnetic flux but no net current or helicity. The loop final state is found to be a non-linear force-free field, consisting of two flux tubes of oppositely-signed twist embedded in an approximately uniform background field.
CITATION STYLE
Pontin, D. I., Wilmot-Smith, A. L., Hornig, G., & Galsgaard, K. (2011). Dynamics of braided coronal loops. Astronomy & Astrophysics, 525, A57. https://doi.org/10.1051/0004-6361/201014544
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