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Analyzing a database of 26 years of observations of Jupiter from theNan\c{c}ay Decameter Array, we study the occurrence of Io-independent emissionsas a function of the orbital phase of the other Galilean satellites andAmalthea. We identify unambiguously the emissions induced by Ganymede andcharacterize their intervals of occurrence in CML and Ganymede phase andlongitude. We also find hints of emissions induced by Europa and, surprisingly,by Amalthea. The signature of Callisto-induced emissions is more tenuous.

Radio emission from satellite-Jupiter interactions (especially Ganymede)