Driven reconnection in a quadrupole cusp field
Creators
- 1. Institute for Fusion Studies, University of Texas at Austin, Austin, Texas 78712 (United States)
Description
Driven magnetic reconnection in a quadrupole cusp field is examined numerically in various collisionality regimes. Quasi-steady-state reconnection rates far in excess of often-quoted limits are observed. As expected, the rate is determined by external boundary conditions and appears to be limited only by computational concerns; thus, in this configuration the slow reconnection is differentiated from the fast one only by changes in the reconnection-layer geometry. Collisional reconnection exhibits the typical extended current layer of the Sweet-Parker model, whereas the collisionless reconnection mediated by kinetic-Alven or whistler waves has the Petschek-type 'X-layer' configuration. The current density at the X point is reduced in the collisionless cases, in qualitative agreement with the results from the Versatile Toroidal Facility experiment
Additional details
Identifiers
- DOI
- 10.1063/1.2032647;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 12
- Journal Issue
- 8
- Journal Page Range
- p. 080706-080706.4
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37070472
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALFVEN WAVES; BOUNDARY CONDITIONS; CHARGED-PARTICLE TRANSPORT; CURRENT DENSITY; CUSPED GEOMETRIES; ELECTRIC CURRENTS; ELECTRON COLLISIONS; GEOMETRY; LAYERS; MAGNETIC RECONNECTION; MAGNETOHYDRODYNAMICS; PLASMA; PLASMA CONFINEMENT; QUADRUPOLES; STEADY-STATE CONDITIONS; WHISTLERS
- Descriptors DEC
- COLLISIONS; CONFINEMENT; CURRENTS; ELECTROMAGNETIC RADIATION; FLUID MECHANICS; HYDRODYNAMICS; HYDROMAGNETIC WAVES; MAGNETIC FIELD CONFIGURATIONS; MATHEMATICS; MECHANICS; MULTIPOLES; NOISE; OPEN CONFIGURATIONS; RADIATION TRANSPORT; RADIATIONS; RADIO NOISE; RADIOWAVE RADIATION
Optional Information
- Notes
- (c) 2005 American Institute of Physics