X-point collapse and saturation in the nonlinear tearing mode reconnection
| dc.creator | Loureiro, N. F. | |
| dc.creator | Cowley, S. C. | |
| dc.creator | Dorland, W. D. | |
| dc.creator | Haines, M. G. | |
| dc.creator | Schekochihin, A. A. | |
| dc.date | 2005-07-28 | |
| dc.date.accessioned | 2026-07-07T10:47:01Z | |
| dc.date.available | 2026-07-07T10:47:01Z | |
| dc.description | We study the nonlinear evolution of the resistive tearing mode in slab geometry in two dimensions. We show that, in the strongly driven regime (large Delta'), a collapse of the X-point occurs once the island width exceeds a certain critical value ~1/Delta'. A current sheet is formed and the reconnection is exponential in time with a growth rate ~eta^1/2, where eta is the resistivity. If the aspect ratio of the current sheet is sufficiently large, the sheet can itself become tearing-mode unstable, giving rise to secondary islands, which then coalesce with the original island. The saturated state depends on the value of Delta'. For small Delta', the saturation amplitude is ~Delta' and quantitatively agrees with the theoretical prediction. If Delta' is large enough for the X-point collapse to have occured, the saturation amplitude increases noticeably and becomes independent of Delta'. | |
| dc.description | revtex4, 4 pages, 18 figures | |
| dc.identifier | https://arxiv.org/abs/physics/0507206 | |
| dc.identifier | http://arxiv.org/abs/physics/0507206 | |
| dc.identifier | Phys.Rev.Lett.95:235003,2005 | |
| dc.identifier | doi:10.1103/PhysRevLett.95.235003 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183432 | |
| dc.subject | Plasma Physics | |
| dc.subject | Astrophysics | |
| dc.subject | Space Physics | |
| dc.title | X-point collapse and saturation in the nonlinear tearing mode reconnection | |
| dc.type | text |