CME development in the corona and interplanetary medium: A multi-wavelength approach
arXiv:1407.2271 · doi:10.1051/eas/1255042
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.
arXiv commentInvited review at the 4th French-Chinese Meeting on Solar Physics, Nice, 2011
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