Distribution of oscillation frequencies, detected with Auto-NUWT at each height, z, from the synthesised 171 Å line emissions. The colour bars correspond to the normalised amplitude of the oscillation for each detected frequency. As in Fig. 4, the left, middle, and right columns correspond to SDO/AIA, Solar Orbiter/HRI_EUV, and MUSE/SG resolution, while the top, middle, and bottom panels correspond to the simulations with the broadband driver, symmetric pulse, and asymmetric pulse, respectively.