Fig. 5
Base-difference images of STEREO/SECCHI/EUVI-B 195 Å for: a) 20:00–19:50 UT (initial expansion of the CME, ~3 min before the onset of the type II emission); b) 20:05–19:50 UT (fast expansion of the CME during the intensification of the type II emission); and c) 20:10–19:50 UT (disruption of the CME flux rope at the end of the type II emission).
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