On the combined effects of compositional inhomogeneity and ammonia addition to turbulent flames of ethylene
Macfarlane, Andrew R.W.
Dunn, Matt J.
Roberts, William L.
Masri, Assaad R.
KAUST DepartmentClean Combustion Research Center
Physical Science and Engineering (PSE) Division
Mechanical Engineering Program
Embargo End Date2025-02-04
Permanent link to this recordhttp://hdl.handle.net/10754/687540
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AbstractThis paper is part of a broader program aimed at investigating the effects of co-firing clean fuels such as ammonia or hydrogen with hydrocarbons. The focus is on soot formation as well as flame stability in turbulent mixed-mode combustion, which is highly relevant in practical combustors. Ammonia substitution for nitrogen results in reduced flame stability, and this is correlated to differences in flame speed and extinction strain rate. While it is known that the addition of ammonia suppresses soot, visual inspection of compositionally inhomogeneous flames of ethylene-ammonia indicates a reduction in ammonia's ability to suppress soot formation. Measurements of soot volume fraction and laser-induced fluorescence in selected UV and visible bands are made along the centreline in selected flames to test this hypothesis. Experimental results are then compared to simulations in laminar diffusion flames, stratified counterflow flames, and partially premixed flames. All results confirm the soot-inhibiting ability of ammonia. Increasing inhomogeneity, leading to higher centreline mixture fractions, enhances soot formation, and the level of enhancement is greater for flames with ammonia than without. Moreover, it is found that partial premixing is ultimately responsible for determining the amount of soot formed as opposed to stratification of fuel mixtures near the pilot.
CitationBoyette, W. R., Macfarlane, A. R. W., Steinmetz, S. A., Dunn, M. J., Roberts, W. L., & Masri, A. R. (2023). On the combined effects of compositional inhomogeneity and ammonia addition to turbulent flames of ethylene. Proceedings of the Combustion Institute. https://doi.org/10.1016/j.proci.2022.08.092
SponsorsThis work is supported by the Australian Research Council and by King Abdullah University of Science and Technology (KAUST).