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Figure 8


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Differential number flux of precipitating protons at 1.6 keV (background colour) and at 8.9 keV (isocontour lines) as a function of time in the simulation and geomagnetic latitude (MLAT) at selected magnetic local times (MLT) on the nightside. Panels a–c show the northern hemisphere, whereas panels d–f show the southern hemisphere.

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