Abstract
The coronal explosions, discovered by De Jager and Boelee (1984), and interpreted by them as manifestations of plasma streaming out of the flare kernels, can also be interpreted as signatures of current loop coalescence in the flaring region.
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References
Brown, J. C.: 1973, Solar Phys. 31, 143.
De Jager, C.: 1986, Space Sci. Rev. 44, 43.
De Jager, C.: 1987, Solar Phys. 110, 337.
De Jager, C. and Boelee, A: 1984, Solar Phys. 92, 227.
De Jager, C. and Svestka, Z: 1985, Solar Phys. 100, 435.
Fisher, G.H., Canfield, R.C. and McClymont, A.N.: 1984, Astrophys. J. 281, L79.
Fisher, G.H., Canfield, R.C. and McClymont, A.N.: 1985, Astrophys. J. 289, 434.
Lemmens, A. and De Jager, C.: 1986, Solar Phys. 106, 365.
Loran, J.M. and Brown, J.C.: 1985, Astrophys. Space Sci. 117, 173.
Sakai, J.: 1989a, Solar Phys. 120, 117.
Sakai, J.: 1989b, Astrophys. J. Suppl. in press.
Sakai, J. and De Jager, C.: 1989, Solar Phys. in press
Sakai, J. and Oshawa, Y.: 1987, Space Sci. Rev. 46, 113.
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Sakai, JI., de Jager, C. Coronal explosions as a signature of current loop coalescence in solar flares. Sol Phys 123, 393–396 (1989). https://doi.org/10.1007/BF00149116
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DOI: https://doi.org/10.1007/BF00149116