Snapshots of transversal velocity V_iz (color map), expressed in the units of km s⁻¹, and velocity vectors (arrows) at t = 100 s (a) and t = 135 s (b) for B = [0, 10, 2] Gs. This configuration leads to the generation of MAWs waves which are coupled to Alfvén waves. Here, the spatial profile of V_iz (color map) represents the presence of both Alfvén and MAWs in the chromosphere (0.5 ≤ y ≤ 2 Mm) and in the higher layers of the solar atmosphere. The black arrows indicate the direction of the plasma flow.