Probing Jupiter's Atmosphere Through Juno Radio Occultations: Methodology and Initial Observations

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Initial observations reveal Jupiter's atmospheric dynamics through a novel methodology, suggesting new insights into its composition.

Observations reveal characteristics of Jupiter's atmosphere, enhancing current understanding.
Key findings include the derivation of pressure and temperature profiles from radio frequencies.
Methodology includes ray-tracing inversion algorithms based on two-way radio links in X- and Ka-bands.
Findings suggest contributions to atmospheric dynamics that build on prior Voyager and CIRS insights.

Caruso et al. (2025) studied this question.

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