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AGU: Geophysical Research Letters

 

Keywords

  • reconnection
  • magnetopause

Index Terms

  • Magnetospheric Physics: Magnetic reconnection
  • Magnetospheric Physics: Magnetopause and boundary layers
  • Magnetospheric Physics: Magnetosheath
  • Magnetospheric Physics: Solar wind/magnetosphere interactions
  • Solar Physics, Astrophysics, and Astronomy: Magnetic reconnection

Abstract

Scaling of asymmetric Hall magnetic reconnection

P. A. Cassak

Department of Physics and Astronomy, University of Delaware, Newark, Delaware, USA

M. A. Shay

Department of Physics and Astronomy, University of Delaware, Newark, Delaware, USA

The scaling of the reconnection rate and ion and electron outflow speeds with upstream magnetic field strengths and plasma mass densities during asymmetric collisionless (Hall) reconnection without a guide field is studied using two-dimensional two-fluid simulations. The results agree with a recent theory by Cassak and Shay (2007). It is found that the normalized reconnection rate is on the order of 0.1 and is independent of the asymmetry in field or density. Signatures of asymmetric Hall reconnection and applications to the magnetopause are briefly discussed.

Received 7 July 2008; accepted 20 August 2008; published 2 October 2008.

Citation: Cassak, P. A., and M. A. Shay (2008), Scaling of asymmetric Hall magnetic reconnection, Geophys. Res. Lett., 35, L19102, doi:10.1029/2008GL035268.

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