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An Energy Storage Mechanism for A Solar Flare by Shearing the Magnetic Field

Published online by Cambridge University Press:  30 March 2016

Xinping Liu
Xinping Liu*
Affiliation:
Institute of Mechanics, Academy of Sciences, Beijing, China

Abstract

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The complete set of MHD equations is solved by numerical calculation. The aim is to study the energy storage mechanism of a solar flare by shearing the magnetic field. Results show that the magnetic energy is stored in local regions and is large enough to explain a big solar flare.

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 767 - 768
Copyright
Copyright © Reidel 1986

References

Gold, T. and Hoyle, F., Monthly Notice RAS., 120, 89, 1960.Google Scholar
Xinping, Liu and Chao, Ao, Chinese Journal of Space Science, 1. 60, 1981.Google Scholar
Tanaka, K. and Nakagawa, Y., Solar physics, 33. 187, 1973.Google Scholar
Xinping, Liu, ‘A New Method for Stipulating Boundary Conditions in Initial Boundary Problem of Magnetohydrodynamics, Submitted to J. Comp. Phys. in China, 1985.Google Scholar