Simulation of the iMZ response with the ELT pupil in closed-loop to ten different atmospheric turbulence sequences corresponding to very good seeing (0.4 arcseconds) and flux conditions (m = 5). Upper part: evolution of the residual phase variance for one second of turbulence, generated with HCIPy (Por et al. 2018). Each of the ten curves correspond to a different turbulence sequence with r₀ = 15 cm (42 cm at 1.2 µm) and L₀ = 25 m. Bottom part: residual phase maps and corresponding PSFs at the last iteration for three of the ten sequences, representing three typical cases.