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Origins 1. Discover how moon and ring material in the Jovian space environment contribute to radiation belts 2. Reveal the additional particle sources of the Jovian radiation belts Acceleration 3. Discover how Jupiter accelerates charged particles to such exceptionally high energies Loss 4. Reveal the loss processes of energetic charged particles in Jupiter's magnetosphere and resulting X-ray emissions 2036 2036 2037 10 months 3 months 3 months Synchrotron Region 1 5 R J Callisto Io X-ray remote sensing In -S it u Bu rs t < 15 RJ Burst-select short periods of high interest Public outreach camera observations Mission Timeline
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Clark et al. (2023) studied this question.