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The Quasi-Static Evolution of Magnetic Structures on the Sun and Their Topological Reconstruction

Published online by Cambridge University Press:  19 July 2016

Yu. G. Matyukhin  and
V.M. Tomozov
Yu. G. Matyukhin
Affiliation:
664033, Irkutsk 33, P.O. Box 4026, SibIZMIR, USSR
V.M. Tomozov
Affiliation:
664033, Irkutsk 33, P.O. Box 4026, SibIZMIR, USSR

Abstract

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We have considered the problem of quasi-static evolution of a magnetic configuration as it is affected by shear motions at field line footpoints. It is found that, with a certain character of the shear motions at the field line footpoints, topological reconstruction will, by necessity, occur in the magnetic configuration. A pattern of magnetic field lines during the course of configuration restructuring is constructed.

Type
VII. Magnetic Reconnection and Coronal Evolution
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 345 - 346
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Heyvaerts, J., Lasry, J.M., Schatzman, M., and Witomsky, G. (1980), Lecture Notes in Mathematics, 782, pp. 160–191.Google Scholar
Matyukhin, Yu.G. and Tomozov, V.M. (1989), In: AGU Chapman Conference on: Physics of Magnetic Flux Ropes, Extended Abstracts, Hamilton, Bermuda, March 27-31, pp. 146–157.Google Scholar