On the relaxation of braided magnetic fields

TY - GEN

T1 - On the relaxation of braided magnetic fields

AU - Pontin, D. I.

AU - Wilmot-Smith, A. L.

AU - Hornig, G.

PY - 2013

Y1 - 2013

N2 - We discuss the properties of braided magnetic fields, in particular with regard to their relaxation towards equilibrium both in the absence and presence of finite plasma resistivity. We consider a model magnetic field in which a subset of field lines are braided in the mathematical sense (in the form of a pigtail braid), and stretch between two perfectly conducting plates. An ideal relaxation yields an approximate force-free equilibrium without thin current sheets. However, in the presence of a finite resistivity the field spontaneously develops thin (but finite) current layers. Subsequently, the system undergoes a fast relaxation on an Alfvénic timescale via a myriad of thin current layers. The current layer structure becomes increasingly complex, and is increasingly long-lived, for higher magnetic Reynolds numbers. The effect of the resistive relaxation is to unbraid the magnetic field, that is to significantly simplify the mapping of field lines between the end plates. This process involves magnetic flux being reconnected multiple times. The final state of the resistive relaxation approximates a non-linear force-free field, implying the presence of additional constraints beyond the magnetic helicity on the relaxation process. The 'topological dissipation' hypothesis, which proposes to explain the heating of the solar corona via braiding of the coronal field by photospheric motions, is one of the most controversial ideas of solar physics. We therefore consider in some detail the relevance of our results to this debate.

AB - We discuss the properties of braided magnetic fields, in particular with regard to their relaxation towards equilibrium both in the absence and presence of finite plasma resistivity. We consider a model magnetic field in which a subset of field lines are braided in the mathematical sense (in the form of a pigtail braid), and stretch between two perfectly conducting plates. An ideal relaxation yields an approximate force-free equilibrium without thin current sheets. However, in the presence of a finite resistivity the field spontaneously develops thin (but finite) current layers. Subsequently, the system undergoes a fast relaxation on an Alfvénic timescale via a myriad of thin current layers. The current layer structure becomes increasingly complex, and is increasingly long-lived, for higher magnetic Reynolds numbers. The effect of the resistive relaxation is to unbraid the magnetic field, that is to significantly simplify the mapping of field lines between the end plates. This process involves magnetic flux being reconnected multiple times. The final state of the resistive relaxation approximates a non-linear force-free field, implying the presence of additional constraints beyond the magnetic helicity on the relaxation process. The 'topological dissipation' hypothesis, which proposes to explain the heating of the solar corona via braiding of the coronal field by photospheric motions, is one of the most controversial ideas of solar physics. We therefore consider in some detail the relevance of our results to this debate.

UR - https://www.scopus.com/pages/publications/84887446317

U2 - 10.1016/j.piutam.2013.09.010

DO - 10.1016/j.piutam.2013.09.010

M3 - Conference contribution

AN - SCOPUS:84887446317

T3 - Procedia IUTAM

SP - 110

EP - 120

BT - IUTAM Symposium on Understanding Common Aspects of Extreme Events in Fluids

A2 - Bustamante, M. D.

A2 - Newell, A. C.

A2 - Kerr, R. M.

A2 - Tsubota, M.

PB - Elsevier

T2 - IUTAM Symposium 2012: "Understanding Common Aspects of Extreme Events in Fluids"

Y2 - 2 July 2012 through 6 July 2012

ER -