Fig. 5.
Evolution of the centroids of the moving radio sources through time. The centroids of the three moving sources are shown from top to bottom overlaid on SDO/AIA (left), PROBA2/SWAP (middle), and STEREO/EUVI-A and COR1-A (right) running-difference images of the Sun. The colour scale for the centroids represents minutes from the start time of each moving radio burst. The bursts are located at the northern CME flank in both the Earth (SDO and PROBA2) and STEREO-A perspectives.
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