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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
Abstract
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