Fig. 3: JADE-E and Waves in situ observations. | Nature Communications

Fig. 3: JADE-E and Waves in situ observations.

From: In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft

Fig. 3

a Electron energy-time spectrogram. b Pitch angle (PA)-time spectrogram for electrons with energies  between 1.1 and 30.2 keV. The size of the loss cone is indicated by the dashed gray lines. c Partial electron downward energy flux (EF Down, in black) and characteristic energy (EC Down, in blue). Electrons with energy between 1.1 and 30.2 keV have been considered. d Frequency-time spectrogram of the ratio of the electric (E) to magnetic (cB) spectral densities. Color bands above (a) indicate on which auroral structure on Jupiter’s northern pole Juno’s magnetic footprint maps. Juno’s M-Shell, altitude (Alt), magnetic latitude (MLat), and longitude separation to Callisto as a function of time are indicated below the panel (d).

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