Fig. 2
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Ground tracks of the Cassini flybys over the SPT of Enceladus. E5, E17, and E18 (shown in red) are flybys for which compositional spectra were obtained. From flybys E7 and E21 (shown in black), we used profiles of particle count rates to constrain our model. Cross symbols mark times measured from the respective closest approach of the spacecraft to Enceladus.
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