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Saturn's auroral morphology and activity during quiet magnetospheric conditions

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Figure

Figure 1. Segment of Cassini’s orbit in the X-Y plane (Saturn’s equatorial plane) for part of revolution 17
Figure 5 shows the time evolution of the radiated power in the H 2 bands associated with the average of the seven images of each HST orbit, also listed in Table 1
Figure 7 shows a sequence of frames illustrating the time evolution of the 20 – 50 keV H atom flux between 2100 and

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