Structure of laminar sooting inverse diffusion flames

被引:61
|
作者
Mikofski, Mark A.
Williams, Timothy C.
Shaddix, Christopher R.
Fernandez-Pello, A. Carlos
Blevins, Linda G.
机构
[1] Univ Calif Berkeley, Micrograv Combust Lab, Berkeley, CA 94720 USA
[2] Sandia Natl Labs, Combust Res Facil, Livermore, CA 94550 USA
基金
美国国家航空航天局;
关键词
inverse diffusion flame; laminar; OH; PAH; laser-induced fluorescence; soot; laser-induced incandescence;
D O I
10.1016/j.combustflame.2007.01.006
中图分类号
O414.1 [热力学];
学科分类号
摘要
The flame structure of laminar inverse diffusion flames (IDFs) was studied to gain insight into soot formation and growth in underventilated combustion. Both ethylene-air and methane-air IDFs were examined, fuel flow rates were kept constant for all flames of each fuel type, and airflow rates were varied to observe the effect on flame structure and soot formation. Planar laser-inthiced fluorescence of hydroxyl radicals (OH PLIF) and polycyclic aromatic hydrocarbons (PAH PLIF), planar laser-induced incandescence of soot (soot PLII), and thermocoupledetermined gas temperatures were used to draw conclusions about flame structure and soot formation. Flickering, caused by buoyancy-induced vortices, was evident above and outside the flames. The distances between the OH, PAH, and soot zones were similar in IDFs and normal diffusion flames (NDFs), but the locations of those zones were inverted in IDFs relative to NDFs. Peak OH PLIF coincided with peak temperature and marked the flame front. Soot appeared outside the flame front, corresponding to temperatures around the minimum soot formation temperature of 1300 K. PAHs appeared outside the soot layer, with characteristic temperature depending on the wavelength detection band. PAHs and soot began to appear at a constant axial position for each fuel, independent of the rate of air flow. FAH formation either preceded or coincided with soot formation, indicating that PAHs are important components in soot formation. Soot growth continued for some time downstream of the flame, at temperatures below the inception temperature, probably through reaction with PAHs. (C) 2007 The Combustion Institute. Published by Elsevier Inc. All rights reserved.
引用
收藏
页码:463 / 478
页数:16
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