The MSG model for cloudy sub-stellar atmospheres - A grid of self-consistent sub-stellar atmosphere models with microphysical cloud formation

Open Access

Fig. 3

Average cloud particle size, 〈a〉 (left), cloud particle number density, n_d (middle), and nucleation rate, J_⋆ (right), in the atmosphere for models with TiO₂ nucleation at T_eff = 2400 K, 2100 K, 1800 K, and 1500 K, and log(ɡ) = 4.0. The corresponding P_gas – T_gas profiles are shown in Fig. 2.

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