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Nonlinear stage of instability due to local Joule-overheating in the solar active regions

✍ Scribed by V. S. Sokolov; A. G. Kosovichev


Publisher
Springer
Year
1978
Tongue
English
Weight
393 KB
Volume
57
Category
Article
ISSN
0038-0938

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✦ Synopsis


The numerical solution by a computer of the system of magnetohydrodynamics equations in the one-dimensional approximation serves as the basis for studying the non-linear stage of the instability due to local Joule-overheating of zones with large values of magnetic field gradients in the active regions of the Sun. We have demonstrated the formation of a system of current layers responsible for efficient transformation of magnetic energy into Joule heat and kinetic energy of the macroscopic motion. The specific features of quasi-stationary skinning of magnetic field with gravitation have been noted.