Fig. 1.

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Comparison between spatially integrated and normalized AIA UV and EUV intensities and the normalized GOES X-ray flux. The area between the dashed lines shows the time window over which the X2.2 and X9.3 flares have been enlarged for the lower two panels. The gray shaded area represents the time during which HARPS-N observed, and the blue shaded area represents when SST was observing.
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