EGU25-20656, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-20656
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Radio observations of the Jupiter system, present and future, and synergies between space and Earth-based observations
Corentin Louis
Corentin Louis
  • Observatoire de Paris CNRS, LIRA, Meudon, France (corentin.louis@obspm.fr)

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.

How to cite: Louis, C.: Radio observations of the Jupiter system, present and future, and synergies between space and Earth-based observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20656, https://doi.org/10.5194/egusphere-egu25-20656, 2025.