Abstract
Parker laid the foundation for the subject of magnetic reconnection in his fundamental early papers. We first of all summarise his contributions and give a new generalisation of the Sweet-Parker relations for a current sheet in which the outflow pressure is an extra parameter. Then we review the models for fast reconnection that have since been proposed, beginning with the Petschek mechanism and continuing to the more general Almost-Uniform and Nonuniform families. A comparison with numerical experiments is also made and the conditions under which fast reconnection exists are elucidated.
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References
Biskamp, D (1986) Magnetic reconnection via current sheets Phys. Fluids 29 1520–1531
Cowling T.G. (1953) Solar electrodynamics, in The Sun (ed. G. Kuiper) Chapter 8 University of Chicago Press
Craig I.J.D. and Henton S.M. (1995) “Exact solutions for steady-state incompressible magnetic reconnection” , preprint
Dungey, J. VV. (1953) Conditions for the occurrence of electrical discharges in astrophysical systems, Phil. Mag. 44 725–738
Forbes, T G and Priest, E R. (1987) A comparison of analytical and numerical models for steadily driven reconnection Rev. Geophys 25, 1583–1607.
Giovanelli, R.G. (1947) Magnetic and electric phenomena in the Sun’s atmosphere associated with sunspots, Mon. Not. Roy. Astron. Soc. 107, 338–355.
Jardine, M and Priest, E R (1988) Weakly nonlinear theory of fast steady-state magnetic reconnection J Plasma Phys. 40, 143–161.
**, S P and Ip, W H (1991) Two-dimensional compressible MHD simulation of a driven reconnection process Phys. Fluids B3, 1927–1936.
Lee, L C and Fu, Z F (1986) Multiple x-line reconnection J Geophys Res. 91, 6807–6815
Parker, E.N.(1957) Sweet’s mechanism for merging magnetic fields in conducting fluids, J. Geophys. Res. 62, 509–520
Parker, E N (1963) The solar flare phenomenon and theory of reconnection and annihilation of magnetic fields Ap. J. Supp 8, 177–211.
Parker, E.N. (1973) Comments on the reconnection rate of magnetic fields, J. Plasma Phys. 9, 49–63.
Petschek, H E (1964) Magnetic field annihilation AAS-NASA Symp. on Phys. of Solar Flares, NASA SP-50, 425–439.
Prest, E R (1986) Magnetic reconnection on the Sun Mit. Astron. Ges. 65. 41–51.
Priest, E R and Forbes, T G (1986) New models for fast steady-state magnetic reconnection J Geophys Res. 91 5579–5588.
Priest, E R and Forbes T G (1992) Does fast reconnection exist? J Geophys Res., 97 16757–16772
Priest, E R and Lee, L C (1990) Nonlinear magnetic reconnection models with separatrix jets J Plasma Phys 44 337–360
Scholer, M (1989) Undriven magnetic reconnection in an isolated current sheet J Geophys Res. 94 8805–8812
Sonneru, B.U.O. and Priest, E.R. (1975) Resistive MHD stagnation point flows at a current sheet J. Plasma Phys 14, 417–431
Sweet P A (1058) The neutral point theory of solar flares IAU symp 6 123–134
Yan, M, Lee, L C and Priest, E R (1992) Fast magnetic reconnection with small shock angles J Geophys Res. 97 , 8277–8293
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© 1996 Kluwer Academic Publishers
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Priest, E.R. (1996). Reconnection of Magnetic Lines of Force. In: Tsinganos, K.C. (eds) Solar and Astrophysical Magnetohydrodynamic Flows. NATO ASI Series, vol 481. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0265-7_8
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DOI: https://doi.org/10.1007/978-94-009-0265-7_8
Publisher Name: Springer, Dordrecht
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