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Abstract: Analysis of Jupiter’s atmospheric thermal structure using two years of Juno radio occultations (AGU25)

Analysis of Jupiter’s atmospheric thermal structure using two years of Juno radio occultations

Yohai Kaspi1, Maria Smirnova1, Eli Galanti1, Andrea Caruso2, Leigh N. Fletcher3, Luis Gomez Casajus4, William B Hubbard5, Glenn Orton6, Marzia Parisi7, Marco Zannoni4, Paul G Steffes8, Steven Levin9, Paolo Tortora4 and Scott J Bolton10, (1)Weizmann Institute of Science, Earth and Planetary Sciences, Rehovot, Israel, (2)Centro Interdipartimentale di Ricerca Industriale - Aerospaziale, Università di Bologna, Italy, (3)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (4)University of Bologna, Department of Industrial Engineering, Forlì, Italy, (5)University of Arizona, Tucson, AZ, United States, (6)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (8)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (9)Jet Propulsion Laboratory, Pasadena, United States, (10)Southwest Research Institute, San Antonio, United States
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