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Fig. 6

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Single flare light curves for the X17 flare of October 28, 2003. The grey curve in the third panel is the flux coming from a region of  ~ 900 arcsec2 that includes the flare site and was observed by the VIRGO/LOI instrument (Appourchaux et al. 1997) in the same passband as SPM/Green. SEM and GOES 0.01–0.5 nm are not shown beacause they are polluted by saturation and particle effects.

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