Fig. 9
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Mean Juno-footprint UV auroral brightness vs. mean JEDI downward electron energy flux observed during low-altitude (<3 RJ) bridge crossings between PJ1 and PJ30. Uncertainties (grey) are estimated using the 50th and 100th-percentile values observed during crossings. The gradient and R2 value of the least-squares linear relation (solid blue line) is given in the legend.
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