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Open flux estimates in Saturn's magnetosphere during the January 2004 Cassini HST campaign, and implications for reconnection rates

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Figure

Figure 1.Upstream interplanetary conditions for the interval 1–31 January 2004 as measured by theCassini spacecraft
Figure 2.Selection of UV images of Saturn’s southern aurora taken during January 2004, with the visitnumber, date, and start time of each image shown at the top of each plot
Figure 3.The intensity profile (kR) for co-latitudes 0�–30� along meridians at 0, 06, 12, and 18 MLTfor visit V-13 (see Figure 2)
Figure 4.The open flux content of the southern polar cap estimated from the HST images is plottedThe top and middle panels show the solar wind dynamic pressure and interplanetary magnetic fieldstrength, respectively, measured by the Cassini spacecraft for
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