Probing Jupiter's Atmosphere Through Juno Radio Occultations: Analysis of the Atmospheric Thermal Structure

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Observational analysis reveals thermal structure differences in jupiter's atmosphere, indicating significant latitudinal effects.

Jupiter's atmosphere shows distinct thermal structures influenced by latitude, with variations noted between equatorial and polar regions.
Analysis of radio occultation data from the Juno mission provides new insights into the thermal dynamics of jupiter's atmosphere.
This research utilizes recent high-resolution measurements to compare thermal structures against archival data from cassini and previous missions.
Findings suggest that variations in thermal structure may influence atmospheric dynamics, highlighting the need for further exploration.

Smirnova et al. (2025) studied this question.

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