Equatorial transit asymmetry calculations for planets around diverse host stars from different cloud scenarios for MIRI. Results are shown for observations in the integrated wavelength range between 5 −8 μm for tidally locked planets with T_global = 800 K… 2600 K. Colored stripes indicate the range for cloud scenarios (with cloud mass load, ρ_g/ρ_d(z) for atmospheric layers, where 〈a〉 < 0.1 μm is scaled by values between 1 and 10⁻³) around different main sequence host stars.