Abstract
Dissipation of magnetic energy during field-line reconnection could lead to runaway acceleration of charged particles to high energies. The particle energy gain is directly proportional to the product of the strength of the pre-merging magnetic field and the plasma resistivity. Particle acceleration to relativistic energies is possible provided that plasma turbulence or some form of instability leads to a drastic reduction of the classical (Coulomb) conductivity.
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References
Alfvén, H. 1972, in Cosmic Plasma Physics, ed. K. Schindler (New York: Plenum Press), p. 1.
Baum, P. J., and Bratenahl, A. 1976, Sol. Phys., 47, 331.
Baum, P. J., and Bratenahl, A. 1980, Advances in Electronics and Electron Physics, ed. L. Marton and C. Marton (Academic Press), p. 1.
Cassé, M. 1983, in Composition and Origin of Cosmic Rays, ed. M. M. Shapiro, (Dordrecht: Reidel), p. 193.
Coroniti, F. V., and Eviatar, A. 1977, Astrophys. J. Suppl., 33, 189.
Cowling, T. G. 1945, Proc. Roy. Soc. London A., 183, 453.
Dungey, J. W. 1953, Phil. Mag., 44, 725.
Huba, J. D. 1985, in IAU Symposium No. 107, Unstable Current Systems and Plasma Instabilities in Astrophysics, eds. M.R. Kundu and G.D. Holman (Dordrecht: Reidel), p. 315.
Kerr, R. A. 1984, Science, 226, 1298.
Kuperus, M. 1976, Sol. Phys., 47, 79.
Lynden-Bell, D. 1969, Nature, 223, 690.
Meyer, P., Parker, P. N., and Simpson, J. A. 1956, Phys. Rev., Second Series, 104, 768.
Mullan, D. J. 1981, I. A. J., 15, 9.
Parker, E. N. 1973, Astrophys. J., 180, 247.
Parker, E. N. 1976, in The Physics of Non-Thermal Radio Sources, ed. G. Setti (Dordrecht: Reidel), p. 169.
Pudritz, R. E., and Fahlman, G. G. 1982, Mon. Not. R. Astr. Soc., 198, 689.
Sagdeev, R. Z., and Galeev, A. A. 1969, in Non-Linear Plasma Theory, ed. T. N. O’Neil and D. L. Book (New York: W. A. Benjamin).
Sato, T., Hayashi, T., Walker, R. J., and Ashour-Abdalla, M. 1983, Geophys. Res. (Letters), 10, 221.
Smith, R. A. 1985, in IAU Symposium No. 107, Unstable Current Systems and Plasma Instabilities in Astrophysics, eds. M.R. Kundu and G.D. Holman (Dordrecht: Reidel), p. 113.
Spitzer, L. 1962, Physics of Fully Ionized Gases.
Van Hoven, G. 1985, in IAU Symposium No. 107, Unstable Current Systems and Plasma Instabilities in Astrophysics, eds. M.R. Kundu and G.D. Holman (Dordrecht: Reidel), p. 263.
Vasyliunas, V. M. 1985, in IAU Symposium No. 107, Unstable Current Systems and Plasma Instabilities in Astrophysics, eds. M.R. Kundu and G.D. Holman (Dordrecht: Reidel), p. 529.
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© 1986 D. Reidel Publishing Company
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Sorrell, W.H. (1986). Particle Acceleration by Magnetic Reconnection. In: Shapiro, M.M. (eds) Cosmic Radiation in Contemporary Astrophysics. NATO ASI Series, vol 162. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5488-5_5
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DOI: https://doi.org/10.1007/978-94-009-5488-5_5
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