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Abstract: 3D Hydrodynamical Modeling of Jupiter’s Disequilibrium Carbon Monoxide – Latitudinal trends and Meridional Transport (AGU25)

3D Hydrodynamical Modeling of Jupiter’s Disequilibrium Carbon Monoxide – Latitudinal trends and Meridional Transport

Ali Hyder1, Huazhi Ge2, Jeehyun Yang3 and Glenn Orton1, (1)NASA Jet Propulsion Laboratory, Pasadena, United States, (2)University of California Santa Cruz, Santa Cruz, United States, (3)University of Chicago, Chicago, United States