Exoplanet weather and climate regimes with clouds and thermal ionospheres - A model grid study in support of large-scale observational campaigns

Open Access

Fig. 18

Wavelength-dependent pressure levels, p_gas = p(τ_λ = 1), at which the optical depth due to cloud particles becomes unity, τ = 1, for a grid model planet with an F-type host star, at T_eff,P = 800, 1600 and 2400 K, log(ɡ) = 3 [cgs].

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