Transit asymmetry calculations for planets around diverse host stars for MIRI. Differences between the individual evening and morning transit depths (transit asymmetries) of cloudy atmosphere scenarios for observation in the integrated wavelength range between 5 and 8 μm for tidally locked planets with T_global = 800 K… 2600 K (left: only equatorial information is used, right: all latitudes are used). 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 (purple: A, dark blue: F, golden: G, orange: K, gray: M). Circles denote the maximum values for clarity.