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Fuel-rich n-heptane oxidation: A shock tube and laser absorption study

机译:富含燃料的正庚烷氧化:激波管和激光吸收研究

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The chemical kinetics of n-heptane (n-C-7-H-16) - an important reference compound for real fuels - oxidation are well studied at stoichiometric and lean conditions. However, there is only limited information on the n-heptane chemical kinetics in fuel-rich combustion. In order to verify the accuracy of chemical kinetic models at these conditions, the oxidation of rich n-heptane mixtures has been investigated. Combustion of n-C2H16/O-2/Ar mixtures at equivalence ratios, phi, of 2.0 and 3.0 behind reflected shock waves has been studied at temperatures ranging from 1066 to 1502 K and at pressures ranging from 1.4 to 6.2 atm. Reaction progress was monitored by recording pressure and absorption time-histories of ethylene (C2H4) and n-heptane at a location 2 cm from the endwall of a 14-cm inner diameter shock tube. Ethylene and n-heptane absorption time-histories were measured, respectively, using absorption spectroscopy at 10.532 mu m from a tunable CO2 laser and at around 3.4 mu m from a continuous wave distributed feedback interband cascade laser (ICL). The measured absorption time-histories were compared with modeled predictions from the Lawrence Livermore National Lab (LLNL) detailed n-heptane reaction mechanism. To the best of our knowledge, current data are the first time-resolved n-heptane and ethylene concentration measurements conducted in a shock tube at these conditions. (C) 2017 The Combustion Institute. Published by Elsevier Inc. All rights reserved.
机译:对正庚烷(n-C-7-H-16)(一种用于真实燃料的重要参考化合物)的化学动力学在化学计量和稀薄条件下进行了很好的研究。但是,关于富燃料燃烧中正庚烷化学动力学的信息很少。为了验证在这些条件下化学动力学模型的准确性,已经研究了富正庚烷混合物的氧化。研究了n-C2H16 / O-2 / Ar混合物在反射冲击波之后的当量比phi为2.0和3.0时的燃烧,其温度范围为1066至1502 K,压力范围为1.4至6.2 atm。通过记录乙烯(C2H4)和正庚烷在距14厘米内径减震管的端壁2厘米处的压力和吸收时间历程来监测反应进程。乙烯和正庚烷的吸收时程分别使用可调光谱CO2激光器在10.532μm处和连续波分布反馈带间级联激光器(ICL)在约3.4μm处的吸收光谱法测量。将测得的吸收时程与劳伦斯·利弗莫尔国家实验室(LLNL)详细的正庚烷反应机理的模拟预测值进行了比较。据我们所知,当前数据是在这些条件下,在冲击管中首次进行的时间分辨的正庚烷和乙烯浓度测量。 (C)2017燃烧研究所。由Elsevier Inc.出版。保留所有权利。

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