| Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
|---|---|---|
| Page(s) | 273 - 285 | |
| Section | CMEs and Space Weather | |
| DOI | https://doi.org/10.1051/eas/1255039 | |
| Published online | 27 June 2012 | |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 273-285
CME Trigger and Initiation
1
Yunnan Astronomical Observatory, Chinese Academy of
Sciences, Kunming,
Yunnan
650011,
China
2
School of Tourism and Geography, Yunnan Normal
University, Kunming, Yunnan
650031,
China
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.
© EAS, EDP Sciences 2012