Fig. 4
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Comparison of the magnetospheric electron flux j(E) from Strobel et al. (1990) (dotted blue line), derived from Voyager 2 observations, and the modified flux j*(E) (dash-dotted red line), computed following the recommendations of Sittler & Hartle (1996). The flux j* (E) is computed from the flux j(E) multiplied by a precipitation probability p(E).
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