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Compressible models of fast steady-state magnetic reconnection

  • M. Jardine (a1) and E. R. Priest (a2)

Abstract

We investigate the effects of compressibility on magnetic reconnection, using as a basis the incompressible models of Priest & Forbes and Jardine & Priest. Our results show that compressibility modifies the reconnection process, without changing its essential character. In the region of inflowing plasma, compressibility tends to increase the convergence or divergence of the flow. Also, for regimes with a compression in the inflow the maximum rate of reconnection is increased, while for regimes with an expansion in the inflow the magnetic Mach number at the entrance to the diffusion region is increased. In the region of outflowing plasma the main effects of compressibility are to produce faster and narrower outflow jets, with a lower magnetic field strength.

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Asseo, E. & Sol, H. 1986 Phys. Rep. 148, 308.
Biskamp, D. 1982 Phys. Lett. 87A, 357.
Biskamp, D. 1984 a Phys. Lett. 105A, 124.
Biskamp, D. 1984 b Magnetic Reconnection in Space and Laboratory Plasmas (ed. Hones, M.), p. 369. A.G.U., Washington, D.C.
Biskamp, D. 1986 Phys. Fluids, 29, 1520.
Bonnet, R. M. & Dupree, A. K. (eds) 1981 Solar Phenomena in Stars and Stellar Systems. Reidel.
Forbes, T. G. & Priest, E. R. 1982 Planet. Space Sci. 30, 1183.
Forbes, T. G. & Priest, E. R. 1987 Rev. Geophys. 25, 1583.
Fu, Z. F. & Lee, L. C. 1985 Geophys. Res. Lett. 12, 291.
Gradshteyn, I. S. & Ryzhik, I. M. 1980 Tables of Integrais, Series, and Products, 4th edn.Academic.
Hones, M. (ed.) 1984 Magnetic Reconnection in Space and Laboratory Plasmas. A.G.U., Washington, D.C.
Jardine, M. & Priest, E. R. 1988 a J. Plasma Phys. 40, 143.
Jardine, M. & Priest, E. R. 1988 b Geophys. Astrophys. Fluid Dyn. 42, 163.
Jardine, M. & Priest, E. R. 1988 c J. Plasma Phys. 40, 505.
Jeffrey, A. & Taniuti, T. 1964 Non-Linear Wave Propagation. Academic.
Lee, L.-C. & Fu, Z. F. 1986 a J. Geophys. Res. 91, 6807.
Lee, L.-C. & Fu, Z. F. 1986 b J. Geophys. Res. 91, 4551.
Mestel, L. 1985 Physica Scripta, T11, 53.
Petschek, H. E. 1964 Magnetic field annihilation. AAS-NASA Symposium on the Physics of Solar Flares; NASA Spec. Publ. SP-50, pp 425439.
Priest, E. R. 1984 Solar Magnetohydrodynamics. Reidel.
Priest, E. R. 1985 Rep. Prog. Phys. 48, 955.
Priest, E. R. & Forbes, T. G. 1986 J. Geophys. Res. 91, 5579.
Pudovkin, M. I. & Semenov, V. S. 1977 Ann. Geophys. 33, 429.
Semenov, V. S., Kubyshkin, I. V. & Heyn, M. F. 1983 J. Plasma Phys. 30, 303.
Shivamoggi, B. K. 1985 Phys. Rep. 127, 99.
Sonnerup, B. U. O. 1970 J. Plasma Phys. 4, 161.
Sonnerup, B. U. O. 1979 Solar System Plasma Physics (ed. Lanzerotti, L. T., Kennel, C. F. & Parker, E. N.), p. 45. North-Holland.
Sonnerup, B. U. O. & Priest, E. R. 1975 J. Plasma Phys. 14, 283.
Soward, A. & Priest, E. R. 1977 Phil. Trans. R. Soc. Lond. A 284, 369.
Soward, A. & Priest, E. R. 1982 J. Plasma Phys. 28, 335.
Ugai, M. 1984 Phys. Fluids, 27, 1463.
Vasyliunas, V. M. 1975 Rev. Geophys. Space Phys. 13, 303.
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Compressible models of fast steady-state magnetic reconnection

  • M. Jardine (a1) and E. R. Priest (a2)

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