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Fig. 7.


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(A) Observations of the CME associated with the filament eruption on August 14, 2010. These observations were made by STEREO-B/COR2, SOHO/LASCO, and STEREO-A/COR2, respectively (from left to right). (B) CACTus detections of the coronal mass ejections based on observations from the same instruments. The white lines indicate the estimated angular width of the CME. Images taken from

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