A simple, analytical model of collisionless magnetic reconnection in a pair plasma
Phys. Plasmas 16, 102106 (2009); doi:10.1063/1.3246005
Published 15 October 2009
You are not logged in to this journal. Log in
A set of conservation equations is utilized to derive balance equations in the reconnection diffusion region of a symmetric pair plasma. The reconnection electric field is assumed to have the function to maintain the current density in the diffusion region and to impart thermal energy to the plasma by means of quasiviscous dissipation. Using these assumptions it is possible to derive a simple set of equations for diffusion region parameters in dependence on inflow conditions and on plasma compressibility. These equations are solved by means of a simple, iterative procedure. The solutions show expected features such as dominance of enthalpy flux in the reconnection outflow, as well as combination of adiabatic and quasiviscous heating. Furthermore, the model predicts a maximum reconnection electric field of E*=0.4, normalized to the parameters at the inflow edge of the diffusion region.
©2009 American Institute of Physics
| History: | Received 13 May 2009; accepted 18 September 2009; published 15 October 2009 |
| Permalink: |
http://link.aip.org/link/?PHPAEN/16/102106/1 |
KEYWORDS and PACS
RELATED DATABASES
PUBLICATION DATA
1070-664X (print)
1089-7674 (online)
REFERENCES (18)
For access to fully linked references, you need to log in.
For access to fully linked references, you need to Log in.
- H. E. Petschek, in AAS/NASA Symposium on the Physics of Solar Flares, edited by W. N. Ness (NASA, Washington, DC, 1964), p. 425.
- V. M. Vasyliunas,
Rev. Geophys. Space Phys. 13, 303, doi:10.1029/RG013i001p00303 (1975) . - P. A. Cassak and M. A. Shay, Phys. Plasmas 14, 102114 (2007).
- P. A. Cassak and M. A. Shay, Phys. Plasmas 16, 055704 (2009).
- J. Borovsky and M. Hesse, Phys. Plasmas 14, 102309 (2007).
- J. Birn, J. E. Borovsky, and M. Hesse, Phys. Plasmas 15, 032101 (2008).
- L. Chacón, A. N. Simakov, V. S. Lukin, and A. Zocco, Phys. Rev. Lett. 101, 025003 (2008).
- A. N. Simakov and L. Chacón, Phys. Plasmas 16, 055701 (2009).
- N. Bessho and A. Bhattacharjee, Phys. Rev. Lett. 95, 245001 (2005).
- N. Bessho and A. Bhattacharjee, Phys. Plasmas 14, 056503 (2007).
- W. Daughton and H. Karimabadi, Phys. Plasmas 14, 072303 (2007).
- M. Swisdak, Y. -H. Liu, and J. F. Drake,
Astrophys. J. 680, 999 (2008) . - D. Tsiklauri, Phys. Plasmas 15, 112903 (2008).
- M. Kuznetsova, M. Hesse, and D. Winske,
J. Geophys. Res. 103, 199, doi:10.1029/97JA02699 (1998) . - J. Birn, J. F. Drake, M. A. Shay, B. N. Rogers, R. E. Denton, M. Hesse, M. Kuznetsova, Z. W. Ma, A. Bhattacharjee, A. Otto, and P. L. Pritchett,
J. Geophys. Res. 106, 3715, doi:10.1029/1999JA900449 (2001) . - A. Klimas, M. Hesse, and S. Zenitani, Phys. Plasmas 15, 082102 (2008).
- E. N. Parker,
J. Geophys. Res. 62, 509, doi:10.1029/JZ062i004p00509 (1957) . - M. A. Shay, J. F. Drake, M. Swisdak, and B. N. Rogers, Phys. Plasmas 11, 2199 (2004).







