Nonlinear evolution of double tearing mode with guiding magnetic field
- Institute for Fusion Theory and Simulation, Zhejiang University, Hangzhou 310027 (China)
Nonlinear dynamic evolution of the double tearing mode (DTM) with a guiding magnetic field (B{sub y0}) is investigated by magnetohydrodynamical numerical simulation. The dynamic process of DTM depends weakly on the guiding field in the weak guiding field regime (B{sub y0{<=}}1), but is suppressed by a strong guiding field (B{sub y0}>2). During the explosive nonlinear phase, the maximum reconnection rate ({gamma}{sub max}) increases weakly with the increase of the resistivity as {gamma}{sub max{approx}{eta}}{sup 0.06} for B{sub y0{<=}}1, but for B{sub y0}>2, {gamma}{sub max} is nearly independent of the resistivity. The maximum reconnection rate in the explosive growth phase increases with increase of the initial current sheet separation. A secondary tearing instability is observed at moderate current sheet separation. A strong guiding field suppresses the formation of a secondary island. Based on the simulation results, it is found that the secondary tearing instability occurs only when the length-to-thickness aspect ratio of the reconnection region exceeds about 20.
- OSTI ID:
- 21537799
- Journal Information:
- Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 5 Vol. 18; ISSN PHPAEN; ISSN 1070-664X
- Country of Publication:
- United States
- Language:
- English
Similar Records
Reconnection dynamics with secondary tearing instability in compressible Hall plasmas
Small-scale reconnection due to lower-hybrid drift instability in current sheets with sheared fields
Nonlinear evolution of double tearing mode in Hall magnetohydrodynamics
Journal Article
·
Mon Jun 15 00:00:00 EDT 2015
· Physics of Plasmas
·
OSTI ID:22410429
Small-scale reconnection due to lower-hybrid drift instability in current sheets with sheared fields
Journal Article
·
Fri Dec 31 23:00:00 EST 2004
· Physics of Plasmas
·
OSTI ID:20657963
Nonlinear evolution of double tearing mode in Hall magnetohydrodynamics
Journal Article
·
Mon Dec 14 23:00:00 EST 2009
· Physics of Plasmas
·
OSTI ID:21371312