Eruptive Event with Unusually Fast-Drifting Type II Radio Burst . ... The frequency drift velocity of the latter was about 5 times larger than that of the first type II burst. It is argued that such unusual fast drift of the radio emission was caused by a peculiarity of the accompanied coronal mass ejection (CME): the brightest southeastern sector of the CME front had an inclined, flat shape and propagated on a large angle relative to the radial direction. ... Coronal Mass Ejection To main page ...