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Fig. 16.


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Normalized flux (in logarithmic scale) of 100 keV O+ impacting Ganymede’s surface for two different configurations: (a) Ganymede is under Jupiter’s plasma sheet and (b) Ganymede is in the centre of Jupiter’s plasma sheet. The magnetic field configurations in each case are given by the Jia et al. (2009) model and they are consistent with the G8 (a) and G2 (b) Galileo flybys.

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