A Self-Consistent Numerical Magnetohydrodynamic (MHD) Model of Helmet Streamer and Flux-Rope Interactions: Initiation and Propagation of Coronal Mass Ejections (CMEs)-Reference-Cited by-同舟云学术

A Self-Consistent Numerical Magnetohydrodynamic (MHD) Model of Helmet Streamer and Flux-Rope Interactions: Initiation and Propagation of Coronal Mass Ejections (CMEs)

Published:2013-03-18 Issue: Volume: Page:83-89
ISSN:2328-8779
Container-title:Coronal Mass Ejections
language:
Short-container-title:

Author:

Wu S. T.,Guo W. P.

Publisher

American Geophysical Union

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/GM099p0083/fullpdf

Reference33 articles.

1. Some properties of force-free magnetic fields in infinite regions of space;Aly;Astrophys. J.,1984

2. How much energy can be stored in a three-dimensional force-free magnetic field?;Aly;Astrophys. J.,1991

3. Magnetic arcade evolution and instability;Biskamp;Solar Phys.,1989

4. Magnetohydrodynamic models of coronal transients in the meridional plane. II. Simulation of the coronal transient of 1973 August 21;Dryer;Solar Phys.,1979

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