We investigate the magnetic fabrics of Impact melt breccia at the Dhala impact structure to understand its emplacement mechanism. Our results show that the pseudo-single domains of Ti-poor magnetite and Ti-hematite are the prime magnetic carriers in the impact melt breccia. The magnetic fabrics from most sites reveal a general westward flow of impact melt breccia (IMB), with magnetic lineations of individual specimens trending between NW and SW. This indicates the emplacement of IMB in a semi-molten state with temperatures below c. 1500°C, which is the melting point of Ti-magnetite. Occurrence of poorly sorted clasts implies that IMB was emplaced as surficial flow rather than aerial. The variation in the dips of magnetic fabrics among individual specimens from a site resembles a pyroclastic flow rather than a ground-hugging volatile- and melt-rich flow. We, therefore, suggest that the IMB at Dhala was ballistically ejected and then moved in a semi-molten state as surficial pyroclastic-like flow with temperatures below c. 1500°C. Most flow vectors aligned between NW-SW, may represent a dominant westward excavation flow of the IMB (rather than radially outward flow), which may be activated by an east-to-west directed impactor striking at an impact angle below 50°.