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Fig. 5.


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Electron production rate q(h) profiles calculated with CORIMIA for ACR main constituents: protons (p) (Simpson 1992); Helium (He), Nitrogen (N), Oxygen (O) and Neon (Ne) (Cummings et al. 1984). GCR ionization q(h) profile is at minimal solar activity for cusp region (Fig. 1).

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