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Fig. 4

image

Distribution of the SEP associated flare longitude in the cases with inferred radio association. The red dash-dotted and blue dashed lines correspond to different well-connected magnetic flux tubes, according to Parker’s model of the interplanetary magnetic field, with their longitudes calculated from Eq. (2) using different solar wind velocities (υsw). The red lines correspond to 50°60° western longitude (υsw ~ 415–500 km s-1). The right blue dashed line corresponds to longitude φ0 = 80° (~312 km s-1) and the left blue dashed line corresponds to φ0 = 30° (~832 km s-1). We also label the 50°60° longitudes as “Well-Connected Region”.

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