Mean global hydrodynamic and cloud properties as function of local gas pressure during ~60 Earth days of simulation. Top: kinetic energy density log ₁₀E_h,kin [erg cm^-3] (left) and global mean rms velocity v_rms [m s^-1] (right). Bottom: global mean cloud particle number density log ₁₀n_d [cm^-3] (Eq. (17), left) and drift velocity log ₁₀| v_dr | [m s^-1] (Eq. (13), right). Parallel contour lines indicate that the global properties of the chosen value in the atmosphere, at that pressure iso-bar, are not changing significantly with time. Note: there is no spin-up period since we use of a well converged continuation simulation of Dobbs-Dixon & Agol (2013) as initial conditions.