The proton detector telescopes(especially the 30 - 80 keV and the 80 - 250 keV energy channels), will measure very elevated fluxes over a region extending from the outer Van Allen radiation belt to the auroral zone (geographic latitudes from 45° to 75° ) during global magnetic storms.

2500-6900 keV Protons (0° detector)

2500-6900 keV Protons (0 detector)
The red box in the plot shows the location of the beginning of the satellite track for this plot. The red triangle indicates the location of the end of the track. Data gaps or missing orbits appear as gaps in the satellite track around the earth.

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