Machine learning spectral clustering techniques: Application to Jovian clouds from Juno/JIRAM and JWST/NIRSpec

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Table A.3

Physical parameters used to perform the NEMESIS simulations displayed in Fig. 12.

Parameter Name	Model 1 (Green)	Model 2 (Magenta)	Model 3 (Pink)
Base pressure (bar)	2.30	2.12	2.11
Optical depth at the base (τ_{2.73 µm})	21.3	17.2	14.8
Cumulative optical depth at 1.2 bar (τ_{2.73 µm})	1	1	1
Cloud fractional scale height (CFSH)	0.4	0.55	0.7
Cloud effective radius (µm)	2	2	2
Cloud composition	Imanaka et al. (2012)	Imanaka et al. (2012)	Imanaka et al. (2012)
NH₃ deep VMR (ppm)	230	230	230
PH₃ deep VMR (ppm)	0.8	0.8	0.8

Notes. τ_{2.73 µm} refers to optical depth normalized at the 2.73 µm wavelength, the center of the Jovian reflection peak.

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