JWST observations of exogenic species on Jupiter: HCN, H2O, and CO2

Open Access

Fig. 2

Left column: different vertical profiles used in this work for the three molecules (HCN, CO₂, and H₂ O) analysed in this work. Right column: contribution functions for the different profiles of each molecule. For CO₂ and H₂O, the contribution functions correspond to a mean latitude of 60^∘S, while for HCN they correspond to a mean latitude of 60^∘S for the blue profile, and 75^∘S for the red profile.

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