Abstract
It is shown analytically that self-generated magnetic fields are modulationally unstable with respect to the uniform state of a plasma; such an instability would localize the magnetic field. This localized magnetic flux may well produce small-scale intermittent magnetic fields in coronal active regions or solar flares.
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References
Benz, A. O.: 1986, Solar Phys. 104, 99.
Crannel, C. J., Dulk, G. A., Kosugi, T., and Magun, A.: 1988, Solar Phys. 118, 155.
Gary, D. E., Hurford, G. J., and Flees, D. J.: 1991, Astrophys. J. 369, 255.
Li, X. Q. and Ma, Y. H.: 1993, Astron. Astrophys. 270, 534.
Li, X. Q. and Ma, Y. H.: 1994, Phys. Plasmas 1(9), 3008.
McKean, M. E., Winglee, R. M., and Dulk, G. A.: 1989, Solar Phys. 122, 53.
McKean, M. E., Winglee, R. M., and Dulk, G. A.: 1990, in R. M. Winglee and A. L. Kiplinger (eds.), Max'91 Workshop, No. 3: Max' 91/SMM Solar Flares: Observations and Theory, University of Colorado, Boulder, Colorado, p. 29.
Parker, E. M.: 1978, Astrophys. J. 221, 368.
Priest, E. R.: 1982, Solar Magnetohydrodynamics, Kluwer Academic Publishers, Dordrecht, Holland.
Priest, E. R., Hood, A. W., and Anzer, U.: 1991, Solar Phys. 132, 199.
Slottje, C.: 1978, Nature 275, 520.
Spruit, H. C.: 1979, Solar Phys. 61, 363.
Tandberg-Hanssen, E. and Emslie, A. G.: 1988, The Physics of Solar Flares, Cambridge University Press, New York.
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Li, X.Q., Zhang, Z.D. Modulational instability of self-generated magnetic fields. Sol Phys 169, 69–77 (1996). https://doi.org/10.1007/BF00153834
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DOI: https://doi.org/10.1007/BF00153834