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CME development in the corona and interplanetary medium : A multi-wavelength approach

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
M. Pick  and
B. Kliem
M. Pick
Affiliation:
Observatoire de Paris, LESIA, Place Jules Janssen, 92195 Meudon Cedex, France
B. Kliem
Affiliation:
University of Potsdam, Institute of Physics and Astronomy, 14476 Potsdam, Germany University College London, Mullard Space Science Laboratory, Holmbury St. Mary, UK
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Abstract

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.

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. 299 - 311
Copyright
© EAS, EDP Sciences 2012

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