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MHD Simulation of Dark Filament Eruption in the Quadrupole Source Model
Published online by Cambridge University Press: 12 April 2016
Abstract
A magnetohydrodynamic simulation in a 2.5D approximation is performed for the quadrupole source model for arcade flares treated years ago by Uchida (1980), and recently supported by the observations from Yohkoh. It is shown that this model can explain several key characteristic features of arcade flares found by Yohkoh, and can avoid some of the paradoxes existing in the “classical model”.
- Type
- Birth and Death of Filaments
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 384 - 387
- Copyright
- Copyright © Astronomical Society of the Pacific 1998
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