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Early signatures of large-scale field line opening
2005
Astronomy and Astrophysics
A fast "halo"-type coronal mass ejection (CME) associated with a two-ribbon flare, GOES class M 1.3, was observed on February 8, 2000. Soft X-ray and EUV images revealed several loop ejections and one wave-like moving front that started from a remote location, away from the flare core region. A radio type-II burst was observed near the trajectory of the moving soft X-ray front, although association with the CME itself cannot be ruled out. Large-scale dimmings were observed in EUV and soft
doi:10.1051/0004-6361:20041378
fatcat:fjihsr6dafgqjcntb4mewemtnu