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首页> 外文期刊>International Journal of Heat and Mass Transfer >Effects of radiation on the uncertainty of flame speed determination using spherically propagating flames with CO/CO_2/H_2O dilutions at elevated pressures
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Effects of radiation on the uncertainty of flame speed determination using spherically propagating flames with CO/CO_2/H_2O dilutions at elevated pressures

机译:辐射对球形传播火焰稀释的CO / CO_2 / H_2O稀释气体的火焰速度不确定度的影响。

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This work investigates numerically the effects of spectral dependent radiation on laminar flame speed determination using spherically propagating CH_4/air and H_2/air flames with CO/CO_2/H_2O dilutions at elevated pressures. Three different models, adiabatic, optically thin radiation, and fitted statistically narrow band correlated k (FSNB-CK) models, are employed. The effects of radiation-induced negative burned gas velocity, increased density ratio, and chamber confinement induced flow compression are investigated. It is found that compared to the FSNB-CK model, the adiabatic flame model over-predicts the flame speed by 7% and the optically thin model makes more significant under-prediction. Moreover, this discrepancy increases with pressure. The results also show that a large negative velocity in the burned gas is induced by radiative heat loss and magnified further by the flow compression in a small combustion chamber. The radiation-induced negative burned gas velocity causes an under-estimation of flame speed. Moreover, radiation also increases the density ratio between the burned and the unburned gases. The use of the density ratio of adiabatic flame also causes under-prediction of flame speed. Two radiation corrections taking into account of the negative burned gas velocity and the increased density ratio are recommended for flame speed determination using propagating spherical flame for radiative mixtures. The corrections proposed in this study reduce the uncertainty of flame speed due to radiation.
机译:这项工作使用球形传播的CH_4 /空气和H_2 /空气火焰在CO / CO_2 / H_2O稀释液中在升高的压力下,数值研究了光谱相关辐射对层流火焰速度测定的影响。使用了三种不同的模型,即绝热,光学薄辐射和拟合的统计窄带相关k(FSNB-CK)模型。研究了辐射引起的负燃烧气体速度,增加的密度比和腔室限制引起的流动压缩的影响。结果发现,与FSNB-CK模型相比,绝热火焰模型将火焰速度高估了7%,而光学薄模型则使预测值显着降低。而且,这种差异随着压力而增加。结果还表明,辐射热损失在燃烧气体中产生很大的负速度,而在小燃烧室中的流动压缩进一步放大了该速度。辐射引起的负燃烧气体速度导致火焰速度的低估。此外,辐射还增加了燃烧气体和未燃烧气体之间的密度比。绝热火焰密度比的使用也会导致火焰速度的预测不足。建议使用考虑燃烧气体负速度和增加的密度比的两种辐射校正来确定火焰速度,方法是使用球形球形火焰传播辐射混合物。这项研究中提出的修正减少了由于辐射引起的火焰速度的不确定性。

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