Fig. 5.
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Distribution of the solar flare heliolongitudes (in 10° bins) for all 20 429 > C1.0 flares in our sample from 1984–2013 (A) and for the 314 SEP events (B). The error bars denote the statistical error. Solar flare latitude (in degrees) as a function of the flare longitude (in degrees) for all 20 429 > C1.0 flares in our database from 1984–2013 (red open circles) (C) and for the 314 SEP events (black filled circles) (D).
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