Beyond monoculture: Polydisperse moment methods for sub-stellar atmosphere cloud microphysics - I. Examining properties of the exponential distribution

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Fig. 2

Example of the settling velocity tanh smooth interpolation scheme. The blue line shows the Stokes law values (Eq. (92)), the orange line the Epstein law values (Eq. (93)), and the dashed black line the interpolation function (Eq. (94)). The background gas is assumed to be T = 500 K, p = 10⁻³ bar, $\log g = 3.25, \bar{μ} = 2.33 g {m o l}^{- 1}$ $\[\log ~\mathrm{g}=3.25, \bar{\mu}=2.33 \mathrm{~g} \mathrm{~mol}^{-1}\]$ , and 100% H₂.

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