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作 者:杨斌[1] 郭浩然[1] 桂欣扬 刘鑫[2] 王志新[2] 陈晓龙 刘佩进[2] YANG Bin;GUO Hao-ran;GUI Xin-yang;LIU Xin;WANG Zhi-xin;CHEN Xiao-long;LIU Pei-jin(Institute of Particle and Two-Phase Flow Measurement, University of Shanghai for Science and Technology, Shanghai 200093, China;Science and Technology on Combustion, Internal Flow and Thermal-Structure Laboratory, Northwestern Polytechnical University, Xi’an 710072, China;Shanghai Space Propulsion Technology Research Institute, Shanghai 201109, China)
机构地区:[1]上海理工大学颗粒与两相流测量研究所,上海200093 [2]西北工业大学燃烧热结构与内流场重点实验室,陕西西安710072 [3]上海航天动力技术研究所,上海201109
出 处:《光谱学与光谱分析》2018年第6期1958-1962,共5页Spectroscopy and Spectral Analysis
基 金:the National Key Research and Development Program of China(2016YFB0600601);the National Natural Science Foundation of China(NSFC)(51327803);Shanghai Academy of Spaceflight Technology(SAST2016099)
摘 要:针对固体火箭发动机恶劣环境下的高温燃烧测量问题,提出了利用辐射光谱法来开展固体火箭推进剂燃烧温度在线测量的方法,采用200~1 100nm光纤光谱仪测量了高压实验燃烧器下固体火箭推进剂燃烧火焰辐射光谱,总结了其光谱特性,并基于普朗克定律和光谱拟合方法获得了相应的推进剂燃烧温度,这对固体火箭推进剂燃烧诊断与燃烧机理研究具有重要的参考价值。For the high combustion temperature measurement in harsh environment,the radiation spectroscopy method was proposed to realize the online measurement of combustion temperature of solid rocket propellant.The radiation spectrums in the range of 200~1 100 nm of solid rocket propellant flame in high pressure experimental combustor were obtained by fiber-optic spectrometer.Their representative characteristics were summarized,and the corresponding combustion temperature was determined by the Planck radiation law and the spectral fitting method.The paper provides important reference for combustion diagnostics and mechanism of solid rocket propellant.
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