A new convective parameterization applied to Jupiter: implications for water abundance near the $24^\circ$ N region
Ramanakumar Sankar,
Csaba Palotai
Abstract:Jupiter's atmosphere features a variety of clouds that are formed from the interplay of chemistry and atmospheric dynamics, from the deep red color of the Great Red Spot to the high altitude white ammonia clouds present in the zones (bright bands in Jupiter's atmosphere). Beneath these upper level clouds, water condensation occurs, and sporadically leads to the formation of towering convective storms, driven by the release of large amounts of latent heat. These storms result in a widespread disruption of the c… Show more
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