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The Dynamic Evolutionary Processes of the Magnetic Fields in the Solar Active Region Boulder 5395

Published online by Cambridge University Press:  12 April 2016

Xin Ping Liu ,
Hong Qi Zhang ,
Jing Lin  and
Gui Lin Liu
Xin Ping Liu
Affiliation:
Institute of Mechanics, Chinese Academy of Sciences, Beijing 100080, China
Hong Qi Zhang
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Jing Lin
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Gui Lin Liu
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China

Abstract

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In this paper, based on observational information we proposed an opening bipolar magnetic field model and studied numerically the dynamic evolutionary processes of the magnetic fields by solving a complete set of MHD equations. The aim is to discuss one of the mechanisms of energy build up of solar flares produced in the active region Boulder 5395.

Type
Session 7. Magnetic Shear and Electric Currents
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 457 - 460
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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