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"Bar Code" Events in the Juno-UVS Data: A Signature ~10 MeV Electron Microbursts at Jupiter

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Figure 1. Example of a bar code event. The first strip represents the signal collected in the 126- to 160-nm range, typical of H 2 far-ultraviolet auroral emissions
Figure 2. (a and b) Two examples of 5-s-long bar code time series. In each panel, the top plot shows a time series of the detected noise, together with the gyroradius of a 10-MeV electron with pitch angles of 1 ∘ , 10 ∘ , and 90 ∘ , respectively
Figure 3. (a) The top plot shows an example of the penetrating particle count rate in the radiation belts during the PJ12 perijove (1 April 2018)
Figure 4. Polar projection of the far-ultraviolet aurora for the northern (top part) and southern hemispheres (bottom part)

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