Fig. 5
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Distributions of intensity (in dB above the Galactic background, and normalized to the average Earth-Jupiter distance of 5.2 AU) of the Ga-DAM emission (a) and the Eu-DAM emission (b) compared to those of the Io-DAM emission and the non-Io-Ga-Eu emission. In (a), the histogram in light blue is the intensity distribution of the Ga-DAM emission multiplied by 7.8 (Zarka et al. 2018) for comparison.
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