Plasma turbulence is a complex phenomenon in ionized gases characterized by chaotic, nonlinear fluctuations across a wide range of spatial and temporal scales. This academic concept investigates the collective behavior of charged particles and electromagnetic fields under conditions where instabilities drive disordered flows, leading to enhanced transport of energy, momentum, and particles. Its significance lies in governing fundamental processes in astrophysical plasmas, such as stellar atmospheres and the interstellar medium, and in terrestrial applications like magnetic confinement fusion, where it critically impacts plasma performance and confinement efficiency.