Fig. 1.
RHESSI and EIT images of the M1.8 GOES class solar flare on 20 September 2002. Left panel: RHESSI image restored using the PIXON method in 6–12 keV (isophote) and 25–35 keV (red scale) energy bands. The signal was accumulated between 09:26:42 UT and 09:26:50 UT (Falewicz et al. 2015). Middle: SOHO/EIT 195 Å image taken at 09:47:59 UT (green scale) overplotted with the RHESSI 6 keV–12 keV and 25–35 keV images registered at 09:26:42 UT (dark and light blue contours). The isophotes shown correspond to 30% of the peak intensity. Right panel: SOHO/EIT image shown without RHESSI contours.
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