Figure 7
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Differential number flux of precipitating protons at 1.6 keV (background colour) and 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 dayside. Panels a–c show the northern hemisphere, whereas panels d–f show the southern hemisphere. Note that the colour scales corresponding to the two energy bins differ from each other.
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