Radio observations of the Jupiter system, present and future, and synergies between space and Earth-based observations

Jupiter's radio emissions were first discovered in the 1950s. Since then, Earth-based radio telescopes have monitored Jupiter's emissions above 10 MHz, while several spacecraft have conducted flybys or have orbited the planet, like Juno. The synergy between space-based and ground-based observations has provided complementary data, including multi-point, in situ, and statistical measurements. In this presentation, we will review recent discoveries about auroral and Galilean moon-induced radio emissions made over the past few years using Juno and Earth-based radio telescopes. We will also look ahead to upcoming missions to Jupiter, such as JUICE, and discuss the crucial role of ground-based support observations.