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CME Trigger and Initiation

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
J. Lin  and
N. Wu
J. Lin
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, Yunnan 650011, China
N. Wu
Affiliation:
School of Tourism and Geography, Yunnan Normal University, Kunming, Yunnan 650031, China
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Abstract

This presentation displays several well-known CME models and the related theories, figuring out both advantages and disadvantages of each model through looking at aspects that fit and do not fit observations. It is also aim to enhance the mutual understanding between observers and modelers, helping modelers to improve their models by putting more realistic constrains on the models and helping observers to get detailed physics behind the observations. Therefore, the models and observations are connected to one another such that what the modelers may expect and what the observers can tell.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 55: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges , 2012 , pp. 273 - 285
Copyright
© EAS, EDP Sciences 2012

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