Fig. 2.
Light curves of the X9.3 flare. Panel a: light curves by the KONUS instruments (upper plot) and by GOES (bottom plot). Panel b: light curve in Ly-α line observed by the LYRA instrument (Hochedez et al. 2006; Dominique et al. 2013) showing flaring events 1 (after 11:55 UT) and 2 (after 12:04 UT, see the text for details). Panel c: light curves of HXR emission during or after the flaring event 2 observed after 12:08 UT by RHESSI, green line −25–50 keV; cyan line: 50–100 keV (scaled).
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