Fig. 1
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Occurrence probability of the emission not induced by Io nor by Ganymede as a function of the orbital phases of Io and Ganymede, and the Jovian longitude (CML) of the Earth-Jupiter line. The emission was detected by the NDA from 1990 to 2020. The probability was calculated in 5° × 5° bins (CML × phase) for each component of the Jovian emission (A, B, C, and D).
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