The nature of the mesoscale field-aligned currents in the auroral oval for positive IMF BZ: More frequent occurrence in the dawnside sector than in the duskside sector | Journal of Space Weather and Space Climate

Open Access

Figure 3

Distribution of the latitudinal size of the upward FAC and downward FAC observed by SW-C in the dawnside sector and the duskside sector. The horizontal axis represents 10-km bins from 10–20 km to 120–130 km.

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