Dynamic planar magnetic reconnection solutions for incompressible plasmas

Citation
Ijd. Craig et Pg. Watson, Dynamic planar magnetic reconnection solutions for incompressible plasmas, ASTROPHYS J, 516(2), 1999, pp. 924-933
Citations number
22
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
516
Issue
2
Year of publication
1999
Part
1
Pages
924 - 933
Database
ISI
SICI code
0004-637X(19990510)516:2<924:DPMRSF>2.0.ZU;2-V
Abstract
The planar magnetic reconnection problem for viscous, resistive plasmas is addressed. We show that solutions can be developed by superposing transient nonlinear disturbances onto quiescent "background" fields. The disturbance fields are unrestricted in form, but the spatial part of the background fi eld must satisfy del(2)K = -lambda K. This decomposition allows previous an alytic reconnection solutions, based on one-dimensional disturbance fields of "plane wave" form, to be recovered as special cases. However, we point o ut that planar disturbance fields must be fully two-dimensional to avoid th e pressure problem associated with analytic merging models, that is, to avo id unbounded current sheet pressures in the limit of small plasma resistivi ties. The details of the reconnection problem are then illustrated using ce llular background field simulations in doubly periodic geometries. The flux pile-up rate is shown to saturate when the pressure of the current sheet e xceeds the hydromagnetic pressure of the background field. Although the pre saturation regime is well described by one-dimensional current sheet theory , the nonlinear postsaturation regime remains poorly understood. Preliminar y evidence suggests that, although after saturation the early evolution of the field can be described by slow Sweet-Parker scalings, the first implosi on no longer provides the bulk of the energy release.