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Extinction characteristics of ammonia/air counterflow premixed flames at various pressures

机译:不同压力下氨/空气逆流预混火焰的消光特性

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Ammonia has promising features as a carbon-free fuel without greenhouse gas emission. However, due to its low combustion intensity, the combustion characteristics of ammonia have been rarely investigated. The design of ammonia based industrial applications requires the development of effective turbulent ammonia combustion models. Thus, a study of the flame stretch effect in ammonia/air premixed combustion is necessary. The objective of this research was to study the ammonia flame extinction stretch rate both experimentally and numerically and to investigate the effects of pressure on its extinction characteristics. Experiments were conducted using a counterflow flame burner. Numerical simulations were run on CHEMKIN-PRO, using the PREMIX opposedflow model, for various detailed chemistry mechanisms. The effects of pressure on the extinction stretch rate of ammonia/air premixed flame were compared with that of methane/air flame, and the effects of pressure on the detailed reaction paths were clarified. It was found that the extinction stretch rate of ammonia/air flame is low compared with that of methane/air flame, as could be expected from its low laminar burning velocity. However, the increase of extinction stretch rate with pressure was found to be greater in the case of ammonia/air flame. From detailed chemistry analysis, it was found that the different dependence on pressure of the reaction path of the two fuels could explain this difference. Indeed, the heat release process and flame strength are affected by a greater dependence on pressure of the reactions contributing the most to heat released in the case of methane/air flame. For methane/air flame, CH_(3) is consumed in the main heat releasing reactions, and they experience competition by the third body recombination, 2CH_(3)+M?C_(2)H_(6)+M at high pressure. In the case of ammonia/air flame, the heat release process is mainly related to NH_(3)+OH ? NH_(2)+H_(2)O, NH_(2)+OH ? NH+H_(2)O and NH_(2)+NO?N_(2)+H_(2)O, which remain preponderant when pressure increases. Thus, the decrease of characteristic reaction time with pressure was found to be greater in the case of ammonia/air flame, explaining a larger increase in extinction stretch rate when pressure increases.
机译:氨具有无温室气体排放的无碳燃料的广阔前景。然而,由于其低燃烧强度,很少研究氨的燃烧特性。基于氨的工业应用的设计要求开发有效的湍流氨燃烧模型。因此,有必要研究氨/空气预混燃烧中的火焰拉伸效应。这项研究的目的是通过实验和数值研究氨火焰的消光拉伸速率,并研究压力对其消光特性的影响。使用逆流火焰燃烧器进行实验。使用PREMIX对流模型在CHEMKIN-PRO上进行了数值模拟,用于各种详细的化学机理。比较了压力对氨/空气预混火焰和甲烷/空气火焰消光拉伸速率的影响,并阐明了压力对详细反应路径的影响。已经发现,与甲烷/空气火焰相比,氨/空气火焰的消光拉伸速率低,这可以从其低层燃烧速度来预期。然而,在氨/空气火焰的情况下,发现消光拉伸速率随压力的增加更大。通过详细的化学分析,发现两种燃料对反应路径压力的不同依赖性可以解释这种差异。实际上,在甲烷/空气火焰的情况下,放热过程和火焰强度受到对反应压力的更大依赖性的影响,所述反应对最大释放热量的贡献最大。对于甲烷/空气火焰,CH_(3)在主要的放热反应中被消耗,并且它们在高压下受到第三体重组2CH_(3)+ M?C_(2)H_(6)+ M的竞争。在氨/空气火焰的情况下,放热过程主要与NH_(3)+ OH? NH_(2)+ H_(2)O,NH_(2)+ OH? NH + H_(2)O和NH_(2)+ NO3N_(2)+ H_(2)O在压力增加时仍然占优势。因此,发现在氨/空气火焰的情况下,特征性反应时间随压力的减少更大,这解释了当压力增加时消光拉伸速率的更大增加。

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