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Fig. 20.

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Distribution of the flare locations with respect to the longitudinal distance of the solar flare from the footpoint of the Parker spiral leading to L1 point (ΔΦ). The dashed lines indicate a “cone of observations” within [−50°, 50°]. The five groups, i.e. G1–G5, are color coded on the plot. The events attributed to each group follow the same color code.

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