| Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
|---|---|---|
| Page(s) | 299 - 311 | |
| Section | CMEs and Space Weather | |
| DOI | https://doi.org/10.1051/eas/1255042 | |
| Published online | 27 June 2012 | |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 299-311
CME development in the corona and interplanetary medium : A multi-wavelength approach
1
Observatoire de Paris, LESIA, Place Jules Janssen, 92195
Meudon Cedex,
France
2
University of Potsdam, Institute of Physics and
Astronomy, 14476
Potsdam,
Germany
3
University College London, Mullard Space Science
Laboratory, Holmbury St.
Mary, UK
This review focuses on the so called three-part CMEs which essentially represent the standard picture of a CME eruption. It is shown how the multi-wavelength observations obtained in the last decade, especially those with high cadence, have validated the early models and contributed to their evolution. These observations cover a broad spectral range including the EUV, white-light, and radio domains.
© EAS, EDP Sciences 2012