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Abstract
A model is investigated describing the resistive dissipation of a finite, two-dimensional current sheet subject to suddenly enhanced resistivity. The resistivity rapidly diffuses the current to a distance where it couples to fast magnetosonic modes. The current then propagates away as a sheath moving at the local Alfven speed. A current density peak remains at the X-point producing a steady electric field independent of the resistivity. This transfers flux across the separatrix at a rate consistent with the external wave propagation. The majority of the magnetic energy stored by the initial current sheet is converted into kinetic energy, far from the reconnection site, during the fast mode propagation. (c) 2007 American Institute of Physics.
Original language | English |
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Number of pages | 11 |
Journal | Physics of Plasmas |
Volume | 14 |
DOIs | |
Publication status | Published - Dec 2007 |
Keywords
- FAST MAGNETIC RECONNECTION
- CORONAL LOOP OSCILLATIONS
- NULL POINT
- NEIGHBORHOOD
- RESISTIVITY
- EVOLUTION
- REGION
- FIELDS
- MODEL
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Dive into the research topics of 'Fast magnetosonic waves launched by transient, current sheet reconnection'. Together they form a unique fingerprint.Projects
- 1 Finished
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Solar&Magnetospheric Plasma Theory PP/E1: Solar and Magnetospheric Plasma Theory
Neukirch, T. (PI), Hood, A. W. (CoI), Parnell, C. E. (CoI), Priest, E. (CoI), Roberts, B. (CoI) & Wright, A. N. (CoI)
1/04/07 → 31/03/12
Project: Standard