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 4

Histogram of the occurrence number of events (blue bars), and the occurrence ratio (light-blue line) as a function of the solar zenith angle. The red-colored numbers indicate the number of passes in each 10° bin.

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