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Figure 1
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(a) Solar flare, (b)–(f) coronal dimming, and (g) and (h) coronal mass ejections (CMEs). Data used are from GOES 16 X-ray flux, SDO/AIA 193 and 94, STEREO-A/ COR2, and SOHO/LASCO. Dashed circles mark possibly overlapped CMEs.
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