A model of solar flares based on arcade field reconnection and merging of magnetic islands-Reference-Cited by-同舟云学术

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A model of solar flares based on arcade field reconnection and merging of magnetic islands

Published:2002-05 Issue:5 Volume:9 Page:2330-2336
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Choe G. S.,Cheng C. Z.

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.1435565

Reference30 articles.

1. On the Origin of Solar Flares

2. Model of the High-Energy Phase of Solar Flares

3. Theoretical model of flares and prominences

4. Magnetic reconnection in the corona and the loop prominence phenomenon

5. Dynamical evolution of a solar coronal magnetic field arcade

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A comparison of the formation and evolution of magnetic flux ropes in solar coronal mass ejections and magnetotail plasmoids;Journal of Geophysical Research: Space Physics;2009-07-14

2. Force-free magnetic field extrapolation for MHD boundary conditions in simulations of the solar atmosphere;Astronomy & Astrophysics;2007-02-20

3. Evidence of Rapid Flux Emergence Associated with the M8.7 Flare on 2002 July 26;The Astrophysical Journal;2004-04-20

4. Flux Rope Acceleration and Enhanced Magnetic Reconnection Rate;The Astrophysical Journal;2003-10-20

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