Transit asymmetry calculations from different cloud scenarios for MIRI. Differences between the individual evening and morning transit depths (transit asymmetries) for tidally locked planets with T_global = 800 K … 2600 K orbiting G main sequence stars (all latitudes are used). Results for clear atmosphere calculations are indicated by circles. Cloudy scenarios with different cloud mass loads, ρ_g/ρ_d(z), in atmospheric layers where 〈a〉 < 0.1 μm are denoted by different markers (crosses: 10⁻³ρ_g/ρ_d(z), diamonds: 10⁻²ρ_g/ρ_d(z), squares: 0.1ρ_g/ρ_d(z)). Triangles denote Fe-free results with full ρ_g/ρ_d(z). Colors denote values integrated between 5-8 μm (black) and 8-10 μm (golden).