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Soot volume fraction measurement in low-pressure methane flames by combining laser-induced incandescence and cavity ring-down spectroscopy: Effect of pressure on soot formation

机译:结合激光诱导白炽和腔衰荡光谱技术测量低压甲烷火焰中的烟尘体积分数:压力对烟尘形成的影响

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Soot volume fraction (f_v) profiles are recorded in low-pressure methane/oxygenitrogen flat flames using laser-induced incandescence (LII). Experiments are performed from 20 to 28 kPa in flames having the same equivalence ratio (2.32). Calibration is performed by cavity ring-down spectroscopy (CRDS) and indicates a very weak soot volume fraction (0.066 ppb at 21.33 kPa and 0.8 ppb at 26.66 kPa in the burnt gases). Soot volume fraction is found to increase continuously after a given distance above the burner (HAB) and tends to level off in the burnt gases. The reaction time resolution available in low-pressure flames makes it possible to examine the early steps of soot formation. The variation of the LII signal with laser energy before the LII "plateau" region is much weaker at the beginning of soot formation than after a given reaction time. The LII time decays are nearly constant within the first millimetres, whereas an increase in the decay, correlated with the growth of the primary soot particle, is observed later. The growth of soot volume fraction is then analysed by considering the variation of the derivative function df_v/dt with f_v. Three regimes having respectively a positive slope, a constant slope, and a negative slope are observed and are interpreted with respect to the soot inception process. Finally, a very important sensitivity of f_v with pressure P (at 30 mm HAB) is observed, leading to a power law, f_v = K P~(11), confirmed by extinction measurements (by CRDS). The observed dependence of f_v with pressure could be a result of the prominence of the early soot inception process in the investigated low-pressure flames.
机译:使用激光诱导的白炽灯(LII)在低压甲烷/氧气/氮气平焰中记录烟灰体积分数(f_v)曲线。在具有相同当量比(2.32)的火焰中进行20至28 kPa的实验。校准是通过腔衰荡光谱法(CRDS)进行的,表明烟灰体积分数非常弱(燃烧气体中21.33 kPa时为0.066 ppb,26.66 kPa时为0.8 ppb)。发现烟灰体积分数在燃烧器(HAB)上方一定距离后连续增加,并趋于稳定在燃烧气体中。低压火焰中可用的反应时间分辨率使检查烟灰形成的早期步骤成为可能。与在给定的反应时间之后相比,在烟灰形成开始时,LII“高原”区域之前的LII信号随激光能量的变化要弱得多。在最初的毫米内,LII时间衰减几乎是恒定的,而与初级烟灰颗粒的生长相关的衰减的增加则在稍后被观察到。然后通过考虑导数函数df_v / dt随f_v的变化来分析烟灰体积分数的增长。观察到分别具有正斜率,恒定斜率和负斜率的三种状态,并相对于烟灰起始过程进行了解释。最后,观察到非常重要的灵敏度f_v与压力P(在30 mm HAB时),导致幂定律f_v = K P〜(11),由消光测量(通过CRDS)证实。观察到的f_v对压力的依赖性可能是在研究的低压火焰中早期烟灰开始过程突出的结果。

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