The structure of the dissipation region during asymmetric magnetic reconnection is studied assuming antiparallel magnetic fields in two dimensions. A physics-based prediction for the scaling of the thickness of the dissipation region in (collisionless) Hall reconnection is presented and confirmed with two-fluid simulations. However, the substructure of the dissipation region in these and additional single-fluid (magnetohydrodynamics) simulations disagrees with a recent model [Cassak and Shay, Phys. Plasmas 14, 102114 (2007)]. We attribute the disagreement to the lack of plasma mixing along newly reconnected field lines in fluid models, rendering the use of a fluid description of questionable validity for determining the dissipation region substructure. Applications to the dayside magnetopause are discussed.
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May 2009
Research Article|
March 24 2009
Structure of the dissipation region in fluid simulations of asymmetric magnetic reconnectiona)
P. A. Cassak;
P. A. Cassak
c)
1Department of Physics,
West Virginia University
, Morgantown, West Virginia 26506, USA
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M. A. Shay
M. A. Shay
2Department of Physics and Astronomy,
University of Delaware
, Newark, Delaware 19716, USA
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Phys. Plasmas 16, 055704 (2009)
Article history
Received:
December 07 2008
Accepted:
February 02 2009
Citation
P. A. Cassak, M. A. Shay; Structure of the dissipation region in fluid simulations of asymmetric magnetic reconnection. Phys. Plasmas 1 May 2009; 16 (5): 055704. https://doi.org/10.1063/1.3086867
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