Fig. 11.
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Comparison of solar flare energy distributions derived by different studies. Shown are EUV nanoflares observed with either SOHO/EIT by Benz & Krucker (2002) or TRACE by Parnell & Jupp (2000) and Aschwanden et al. (2000). Microflares were observed with Yohkoh/SXT by Shimizu (1995) and with RHESSI by Hannah et al. (2008). The combined AIA nanoflare observations from this study is also included and indicated by the black dashed line. The figure was adapted from Hannah et al. (2011).
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