This paper investigates the interpretation of helioseismic data in local helioseismology using diverse methodologies, including the Fourier transform, Time-Distance helioseismology, and Ring diagram analysis. In this study, frequency components, spatial features, and surface phenomena are analyzed to better understand the complex dynamics of the sun’s interior. Key findings reveal significant insights into the dynamic and structural complexity of the Sun. This research contributes to the field by providing a comprehensive analysis of solar dynamics through advanced analytical techniques.