Fig. 5
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N2 and N escape rates induced by magnetospheric N+ (upper panels) and H+ (lower panels) precipitation as functions of incident energy, ranging from 60-140 eV for N+ and 1-100 keV for H+. Results are shown for three scattering angle distributions corresponding to strong forward (αE = −1.5), isotropic (αE = 0.01), and backward (αE = 1.5) scattering conditions.
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