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Weakening of Jupiter's main auroral emission during January 2014

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Figure

Figure 1. Gallery of selected images of Jupiter’s northern UV aurora imaged by HST/STIS in January 2014
Figure 2. Auroral power and solar wind dynamic pressure during 1–16 January 2014. (a) Total emitted FUV auroralpower observed by HST/STIS (crosses), their mean (dotted line), and standard deviation about the mean (shading)
Figure 3. Auroral electron parameters estimated from the observations and using the linear Knight relation during10 kR [the source electrons in the equatorial middle magnetosphere assuming constant source electron temperature.1–16 January 2014

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