Title of article
Why are there stationary EIT wave fronts Original Research Article
Author/Authors
P.F. Chen، نويسنده , , C. Fang، نويسنده , , Dean K. Shibata، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2006
Pages
5
From page
456
To page
460
Abstract
EIT waves are often observed to be propagating EUV enhancements followed by an expanding dimming region after the launch of CMEs. It was widely assumed that they are the coronal counterparts of the chromospheric Moreton waves, though the former are three or more times slower. The existence of a stationary “EIT wave” front in some events, however, posed a big challenge to the wave explanation. Simulations are performed to reproduce the stationary “EIT wave” front, which is exactly located near the footpoint of the magnetic separatrix, consistent with observations. The formation of the stationary front is explained in the framework of our model where “EIT waves” are supposed to be generated by successive opening of the field lines covering the erupting flux rope in CMEs.
Keywords
Coronal mass ejections , waves , Numerical simulations
Journal title
Advances in Space Research
Serial Year
2006
Journal title
Advances in Space Research
Record number
1130995
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