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This review focuses on the so called three-part CMEs which essentiallyrepresent the standard picture of a CME eruption. It is shown how themulti-wavelength observations obtained in the last decade, especially thosewith high cadence, have validated the early models and contributed to theirevolution. These observations cover a broad spectral range including the EUV,white-light, and radio domains.

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