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Abstract
The manner in which the rate of magnetic reconnection scales with the Lundquist number in realistic three-dimensional (3D) geometries is still an unsolved problem. It has been demonstrated that in 2D rapid non-linear tearing allows the reconnection rate to become almost independent of the Lundquist number (the “plasmoid instability”). Here, we present the first study of an analogous instability in a fully 3D geometry, defined by a magnetic null point. The 3D null current layer is found to be susceptible to an analogous instability but is marginally more stable than an equivalent 2D Sweet-Parker-like layer. Tearing of the sheet creates a thin boundary layer around the separatrix surface, contained within a flux envelope with a hyperbolic structure that mimics a spine-fan topology. Efficient mixing of flux between the two topological domains occurs as the flux rope structures created during the tearing process evolve within this envelope. This leads to a substantial increase in the rate of reconnection between the two domains.
Copyright (2014) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.
Copyright (2014) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.
Original language | English |
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Article number | 082114 |
Number of pages | 10 |
Journal | Physics of Plasmas |
Volume | 21 |
Issue number | 8 |
DOIs | |
Publication status | Published - Aug 2014 |
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Dive into the research topics of 'Non-linear tearing of 3D null point current sheets'. Together they form a unique fingerprint.Projects
- 1 Finished
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Complex Magnetic Fields: An Enigma of Solar Plasmas (joint with Durham University)
Hornig, G. (Investigator), Pontin, D. (Investigator) & Wilmot-Smith, A. (Investigator)
Science and Technology Facilities Council
1/04/13 → 30/06/16
Project: Research