Abstract
Thus, we have considered one of the possible ways of flare magnetic structure formation due to fast reconnection process, which is accompanied by pre-flare energy release.
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References
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© 1992 Springer-Verlag
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Harutyunian, H.A., Hayrapetyan, V.S. (1992). On the dynamics of the emerging pre-flare magnetic configuration. In: Byrne, P.B., Mullan, D.J. (eds) Surface Inhomogeneities on Late-Type Stars. Lecture Notes in Physics, vol 397. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55310-X_171
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DOI: https://doi.org/10.1007/3-540-55310-X_171
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