Jupiter's equatorial spectrum from visible to 5 μm is fit by three cloud layers — a thick 1–2 bar deck, a thin ~0.55-bar ammonia-ice-like layer, and deep chromophores — with a two-step ammonia profile and no detached photochemical haze.
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Cloud and ammonia vertical profiles in the equatorial atmosphere of Jupiter determined from visible to near-IR observations made by VLT/MUSE, Cassini/VIMS, IRTF/SpeX and Juno/JIRAM
Jupiter's equatorial spectrum from visible to 5 μm is fit by three cloud layers — a thick 1–2 bar deck, a thin ~0.55-bar ammonia-ice-like layer, and deep chromophores — with a two-step ammonia profile and no detached photochemical haze.