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Survey of Thermal Plasma Composition in Saturn's Magnetosphere Using Time of Flight Data From Cassini/CAPS

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Figure

Figure 2. Schematic of the data processing, and as example for the binning step, the case in which the bins are in XY in KSMAG coordinates.
Figure 3. Ratio [(m/q=2)]/[H + ] before the data reduction (left) and after the data reduction (right)
Figure 4. Ratio [(m/q=2)]/[H + ]. We reported data binned in 2 R S × 2 R S bins in the equatorial plane (X-Y in KSMAG coordinate system)
Figure 5. Ratio of counts [(m/q=2)]/[H+] in the Y-Z plane, X between -26 R S and -14 R S in the tail
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