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

Abstract The upper layers of Jupiter's atmosphere, offering critical insights into the planet's deeper structure, are accessible through radio occultation experiments. Since July 2023, NASA's Juno extended mission has provided the first high‐resolution radio occultation measurements since the Voyager era, probing the thermal structure and composition down to approximately 0.5 bar. We use these measurements to study Jupiter's latitudinally dependent vertical thermal structure. We observe cooler stratospheric and warmer tropospheric temperatures at the equatorial region compared to mid‐ and high‐latitudes, and temporal variations in the North Equatorial Belt's thermal structure on a time scale of a few months. These observations align with archival mid‐infrared data from Cassini's CIRS and current ground‐based Texas Echelon Cross Echelle Spectrograph observations, as well as previous studies based on Voyager radio occultations and the Galileo probe, offering an enhanced view of Jupiter's lower stratosphere and upper troposphere thermal structure.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-11-14
DOI
https://doi.org/10.1029/2025gl116804
Citations
4
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
4.62
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Probing Jupiter's Atmosphere Through Juno Radio Occultations: Analysis of the Atmospheric Thermal Structure

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

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article en
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Abstract

Abstract The upper layers of Jupiter's atmosphere, offering critical insights into the planet's deeper structure, are accessible through radio occultation experiments. Since July 2023, NASA's Juno extended mission has provided the first high‐resolution radio occultation measurements since the Voyager era, probing the thermal structure and composition down to approximately 0.5 bar. We use these measurements to study Jupiter's latitudinally dependent vertical thermal structure. We observe cooler stratospheric and warmer tropospheric temperatures at the equatorial region compared to mid‐ and high‐latitudes, and temporal variations in the North Equatorial Belt's thermal structure on a time scale of a few months. These observations align with archival mid‐infrared data from Cassini's CIRS and current ground‐based Texas Echelon Cross Echelle Spectrograph observations, as well as previous studies based on Voyager radio occultations and the Galileo probe, offering an enhanced view of Jupiter's lower stratosphere and upper troposphere thermal structure.

Geophysical Research LettersVol. 52(22)
Southwest Research Institute (US), Planetary Science Institute (US), Georgia Institute of Technology (US), Jet Propulsion Laboratory (US), University of Arizona (US), University of Leicester (GB), Weizmann Institute of Science (IL), University of Bologna (IT)
Openalex Percentile: Top 5%
Astro and Planetary Science
4.62
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