“…Confirmation of the physical origin of these peaks comes from the fact that, when the contents of the white boxes of Figures 4a,b is plotted versus the longitude of Ganymede Λ Ga , they gather in a single broad region in Λ Ga (Figure 4e) that coincides with the higher half of the distributions of Io emissions versus Λ Io (Figure 2c). The peaks in Figures 4c and 4d match the maxima found in Galileo data by Menietti et al [1998] and Hospodarsky et al [2001], but they have a much better signal-to-noise ratio and characterize in greater details the occurrence of the emission, as further illustrated by Figures 4a,b. Also, emission events attributed to the Ganymede-Jupiter interaction are individually identified, allowing us to study their dynamic spectrum, polarization, hemisphere and limb of origin, and compare them to magnetic field models [e.g.…”