This study systematically investigates the effects of multi-jet interaction and gravity on soot formation in methane/air multi-jet diffusion flames through both experimental and numerical approaches. The particle and microcrystalline size, as well as the deposition morphology of soot, of different heights and gravities were detected by Field Emission Scanning Electron Microscopy (FESEM) and High-Resolution Transmission Electron Microscopy (HRTEM). The experimental results showed that both jet interaction and buoyancy effects significantly affect the soot nanostructure. Many large luminous spots named soot ‘meteor’ appeared in methane diffusion flames under microgravity. This phenomenon results from the combined effects of jets interaction and gravity variation. The period fluctuation of the flame tip with a frequency of 12 Hz was observed at normal gravity, but disappeared under microgravity conditions. Reduced gravity enhanced soot formation, with soot particles under microgravity reaching sizes approximately three times larger than those under normal gravity. Moreover, soot generated under microgravity exhibited a higher degree of graphitization, characterized by longer fringe lengths, smaller fringe tortuosity, and a higher C/H ratio. The soot generated from the side tube exhibited a higher degree of maturity compared to that of the center tube under both normal and microgravity conditions. Furthermore, A 3D laminar flame model was built to analyze the soot formation. The simulation results manifested that the soot-related reaction rates of side tubes were higher than those in the center tube, indicating that the combustion performance of the side tubes played more important roles in soot formation and combustion efficiency.
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