Determining the location and size of potential magma reservoirs is crucial to constrain the size of future eruptions or eruptive frequency. Magma accumulation and melt migration have been the focus of extensive research at Mt. Etna volcano. Recent geophysical imaging of Mt. Etna has shown the growing importance of several geological bodies in explaining the migration of eruptive materials inside the volcano. One such body, known as the High Velocity Body (HVB), is a highly consolidated structure located below the central-southern part of the volcano. The HVB has been observed in several tomography studies (Giampiccolo et al., 2020 and references therein) and is interpreted as a massive accumulation of intrusions within the sedimentary basement. In addition, new structural elements have been identified tomographically to the west and southwest of the main volcanic edifice (e.g., Díaz-Moreno et al., 2018 and references therein). Despite not being widely discussed and interpreted in studies based on travel time tomography, these bodies have been well resolved using other techniques. In addition, recent studies (Alparone et al., 2015;Barberi et al., 2016) have found a strong association between deep seismicity beneath Mt. Etna and these geological objects, indicating the need for further study. Apparent contradictions between older and newer tomographic images possibly reflect the increased sensitivity of new tomography techniques to rock heterogeneity