This study reports the observation of magnetohydrodynamic (MHD) wave lensing in the solar corona, where a quasi-periodic wavefront from a solar flare converges at a specific point after passing through a coronal hole (CH). The process resembles electromagnetic wave lensing, with the CH acting as a convex lens. High-resolution observations from the Solar Dynamics Observatory (SDO) and numerical simulations confirm the lensing effect, showing that the wave energy is focused at a focal point. The lensing effect is attributed to the CH's geometry and enhanced Alfvén speed, which cause the wave to bend and converge. The study also demonstrates that the lensing process encodes information about the Alfvén speed, offering potential applications in coronal seismology. Numerical simulations using an idealized setup with a CH shape reproduce the observed lensing effect, showing that the density ratio and plasma beta determine the lensing characteristics. The results suggest that MHD lensing can effectively focus wave energy in magnetized plasma environments, with implications for understanding wave propagation in solar and astrophysical contexts. The study highlights the importance of geometric and density variations in determining the behavior of MHD waves in structured plasma environments.This study reports the observation of magnetohydrodynamic (MHD) wave lensing in the solar corona, where a quasi-periodic wavefront from a solar flare converges at a specific point after passing through a coronal hole (CH). The process resembles electromagnetic wave lensing, with the CH acting as a convex lens. High-resolution observations from the Solar Dynamics Observatory (SDO) and numerical simulations confirm the lensing effect, showing that the wave energy is focused at a focal point. The lensing effect is attributed to the CH's geometry and enhanced Alfvén speed, which cause the wave to bend and converge. The study also demonstrates that the lensing process encodes information about the Alfvén speed, offering potential applications in coronal seismology. Numerical simulations using an idealized setup with a CH shape reproduce the observed lensing effect, showing that the density ratio and plasma beta determine the lensing characteristics. The results suggest that MHD lensing can effectively focus wave energy in magnetized plasma environments, with implications for understanding wave propagation in solar and astrophysical contexts. The study highlights the importance of geometric and density variations in determining the behavior of MHD waves in structured plasma environments.