The manuscript presents a detailed, multi-diagnostic analysis of a single 3D radiation-hydrodynamics Athena++ snapshot of a red-supergiant donor undergoing Roche-lobe overflow. The authors (i) reconstruct an effective Roche potential and mask material outside the L1 equipotential (Sec. 2.1–2.2), (ii) quantify the morphology and intermittency of the mass-flux field and show a strongly filamentary, bursty outflow rather than a smooth stream (Sec. 3.1–3.2, Table 2, Fig. 2), (iii) apply the Q-criterion to assess flow topology and argue the L1 stream is shear-dominated without large coherent vortices (Sec. 2.3, Sec. 3.3, Fig. 4), and (iv) introduce an upstream “source fingerprinting” procedure tracing stream cells back to a photospheric surface and comparing the resulting footprint’s properties to the global surface (Sec. 2.5, Sec. 3.4, Table 3, Fig. 5). The headline interpretation is that localized convective upwellings (lower density/pressure, higher outward radiation flux, more positive radial velocity) preferentially supply material to the L1 stream. The overall narrative is compelling and the analysis toolkit is potentially valuable, but several conclusions are currently overextended given the reliance on a single snapshot and the under-specification/validation of key threshold-based steps (Roche masking, Q-structure identification, and source tracing). The paper would be substantially strengthened by (a) clearer documentation of the underlying simulation and gravity/potential consistency, (b) robustness checks across nearby snapshots and parameter/threshold choices, and (c) quantitative presentation of the force/work decomposition that underpins the “driving engine” claims (Sec. 2.4, Sec. 3.4, Sec. 4).