A Sweet-Parker-type scaling analysis for asymmetric antiparallel reconnection (in which the reconnecting magnetic field strengths and plasma densities are different on opposite sides of the dissipation region) is performed. Scaling laws for the reconnection rate, outflow speed, the density of the outflow, and the structure of the dissipation region are derived from first principles. These results are independent of the dissipation mechanism. It is shown that a generic feature of asymmetric reconnection is that the X-line and stagnation point are not colocated, leading to a bulk flow of plasma across the X-line. The scaling laws are verified using two-dimensional resistive magnetohydrodynamics numerical simulations for the special case of asymmetric magnetic fields with symmetric density. Observational signatures and applications to reconnection in the magnetosphere are discussed.
Skip Nav Destination
Article navigation
October 2007
Research Article|
October 31 2007
Scaling of asymmetric magnetic reconnection: General theory and collisional simulations
P. A. Cassak;
P. A. Cassak
Department of Physics and Astronomy,
University of Delaware
, Newark, Delaware 19716, USA
Search for other works by this author on:
M. A. Shay
M. A. Shay
Department of Physics and Astronomy,
University of Delaware
, Newark, Delaware 19716, USA
Search for other works by this author on:
Phys. Plasmas 14, 102114 (2007)
Article history
Received:
July 10 2007
Accepted:
September 19 2007
Connected Content
A commentary has been published:
Response to “Comment on ‘Scaling of asymmetric magnetic reconnection: General theory and collisional simulations’ ” [Phys. Plasmas 16, 034701 (2009)]
A related article has been published:
Comment on “Scaling of asymmetric magnetic reconnection: General theory and collisional simulations” [Phys. Plasmas 14, 102114 (2007)]
Citation
P. A. Cassak, M. A. Shay; Scaling of asymmetric magnetic reconnection: General theory and collisional simulations. Phys. Plasmas 1 October 2007; 14 (10): 102114. https://doi.org/10.1063/1.2795630
Download citation file:
Pay-Per-View Access
$40.00
Sign In
You could not be signed in. Please check your credentials and make sure you have an active account and try again.
Citing articles via
A prospectus on laser-driven inertial fusion as an energy source
Debra A. Callahan
Weakly nonlinear incompressible Rayleigh–Taylor–Kelvin–Helmholtz instability in plane geometry
Zhen-Qi Zou, Jun-Feng Wu, et al.
Related Content
Structure of the dissipation region in fluid simulations of asymmetric magnetic reconnection
Phys. Plasmas (March 2009)
Asymmetric magnetic reconnection driven by ultraintense femtosecond lasers
Phys. Plasmas (December 2019)
Asymmetric magnetic reconnection with out-of-plane shear flows in a two dimensional hybrid model
Phys. Plasmas (May 2015)
The Hall fields and fast magnetic reconnection
Phys. Plasmas (April 2008)
Forced Hall magnetic reconnection: Parametric variation of the “Newton Challenge”
Phys. Plasmas (June 2006)