Fig. 3: CO mole fraction profiles calculated using the hydrodynamic model with various timescale scaling factors for the ×0.3 water enrichment case. | Nature Astronomy

Fig. 3: CO mole fraction profiles calculated using the hydrodynamic model with various timescale scaling factors for the ×0.3 water enrichment case.

From: A supersolar oxygen abundance supported by hydrodynamic modelling of Jupiter’s atmosphere

Fig. 3

The different colours signify the corresponding scaling factors. The variation in the profile due to timescale changes is substantial. However, the nominal value estimated by Cavalié et al.12 is unlikely to fit the observed CO abundance near the LCL.

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