2.0 μm处CO2高温谱线参数测量研究

研究高温下待测气体的谱线属性, 如谱线强度、自加宽系数、空气加宽系数、温度系数等, 为高温环境中可调谐半导体激光吸收光谱技术反演温度、浓度、速度及其场分布提高精度和可靠性起着十分重要的作用. HITEMP数据库中的数据基本上是理论计算结果, 与实际情况存在相当的误差. 为了获得所选2.0 μm处的可用于燃烧诊断的CO₂谱线参数, 本文采用半导体激光器作为光源, 结合实验室的高温测量系统, 记录了700–1300 K温度范围内所选谱线的高温吸收光谱, 获得了各谱线在相应温度下的谱线强度、自展宽系数及温度系数等谱线参数. 测量得到CO₂的5006.978 cm^-1和5007.7874 cm^-1谱线强度与理论计算值相对误差小于11%; 获得了现有数据库缺少的温度系数和高温下自展宽系数数据. 所有各项参数对以后将要进行的燃烧诊断中的CO₂浓度检测有很大帮助. 关键词： 可调谐半导体激光吸收光谱 高温光谱 自展宽系数 温度系数     

SiH4激光等离子体内H谱线的线型研究

本工作利用光学多道分析仪(OMA Ⅲ)测量了脉冲TEA CO₂激光诱发的SiH₄等离子体内H Balmer系的H_α,H_σ和H_γ线的线型。结果表明,三条谱线的FWHM(半值全宽度)随跃迁上能级的主量子数的增加而增加,即△λ_1/2(H_α)<△λ_1/2(H_β)<△λ_1/2(H_γ)。通过对等离子体内各类加宽机制的讨论,得出等离子体内谱线的主要加宽机制为Stark加宽。由H_α线的实验线型与Stark加宽理论线型的拟合,得到等离子体的两个重要参量,平均电子密度N≈10¹⁷cm^-3,电子温度T≈40 000K。由H_β线的时间分辨测量得到等离子体的电子密度随时间的演变曲线。 关键词：     

基于非线性最小二乘法的多光谱拟合程序：应用于12CH4谱线参数分析

精确的甲烷分子实验光谱参数在大气科学和天文探测等领域有着广泛的应用,特别是谱线的展宽系数及其温度依赖系数对于甲烷分子浓度廓线的研究尤为重要。精密的实验测量是获得准确谱线参数的重要手段。采用实验测量获取谱线参数时,需要在已知实验条件（浓度,温度,总压力,吸收光程以及气体分子种类的混合比等）的情况下,多次扫描同一波段范围得到多组实验室吸收光谱,然后利用基于非线性最小二乘法的拟合程序处理这些光谱,反演获得所需要的光谱参数。然而,一般常用的单光谱拟合程序处理实验光谱既费时又容易引起拟合过程中的误差传递。针对此问题,采用最小二乘拟合技术和Levenberg-Marquardt迭代算法编写了一款适用于处理由可调谐半导体激光吸收光谱技术（TDLAS）所获得的吸收光谱的多光谱拟合程序。该程序可同时处理多张实验光谱,并基于全局拟合方法获得一套光谱参数。详细介绍了该程序的原理、使用方法及数据处理过程。利用多光谱拟合程序中的Voigt线型处理了2 958～2 959 cm-1波数内甲烷（12CH₄）分子6条跃迁谱线的实验光谱,获得了296.0,251.0,223.0,198.0和173.0 K共5组温度下12CH₄分子6条谱线的空气展宽系数。与之前文献报道的该波段内采用单光谱拟合程序得到的相应数据对比结果表明：获得的各温度下的空气展宽系数与参考文献中相应数据差值的百分比处在-4.97%~1.58%之间,两者数据整体符合较好,并且在30组对比数据中,有4组由单光谱拟合程序得到的空气展宽系数的误差值小于由多光谱拟合程序得到的相应数值,有2组数据显示由两种方法获得的误差值相等,其余24组由多光谱拟合程序获得的数据拟合误差小于由单光谱拟合程序获得的相应数值,表明多光谱拟合程序具有良好的可靠性,适用于气体分子吸收光谱的处理。     

H2（V=3）+H2（He）碰撞中的转动能量转移

激发态Na₂与H₂碰撞,使H₂（V=3,J=3）得到布居,在H₂和He总气压为800 Pa及温度为700 K的条件下,利用相干反斯托克斯拉曼散射（CARS）光谱技术研究了H₂（3,3）与H₂（He）间转动能量转移过程.改变CARS激光束与激发Na₂的激光之间的延迟时间,测量He不同摩尔配比时H₂（3,J）态CARS谱强度的时间演化,得到H₂（3,3）的总弛豫速率系数分别为k_3,3^H₂=（21士5）×10^-3cm³·s^-1和k_3,3^H_e=（5.6士1.6）×10^-13cm³·s^-1.测量H₂（3,J）各转动态的相对CARS谱强度,由速率方程分析,得到H₂（3,3）+H₂→H₂（3,J）+H₂中,对于J=2,4,转移速率系数分别为（11±4）×10^-13cm³·s^-1和（8.2±3.1）×10^-13cm³·s_<sup>-1.在H₂（3,3）+He→H₂（3,J）+He中,对于J=2,4,转移速率系数分别为（3.1±1.2）×10^-13cm³·s^-1和（2.1士0.7）×10¹³cm³·s^-1.对于H₂（3,3）,单量子弛豫|△J|=1约占该态总弛豫率的90%.     

高位振动态RbH（X1∑+,v"≥15）与CO2碰撞转移中的能量相关性

研究了高位振动态RbH（X¹∑⁺,v″=15～21）与CO₂碰撞转移过程.脉冲激光激发RbH至高位态,利用激光感应荧光光谱（LIF）得到RbH（X¹∑⁺,v″）与CO₂的猝灭速率系数k_v″（CO₂）,k_v″=21（CO₂）=2.7k_vⁿ=15（CO₂）.利用激光泛频光谱技术,测量了CO₂（00⁰,J）高转动态分布,得到了转动温度,从而获得了平均转动能rot>和转动能的变化<△E_rot>,发现<△E_rot>_v″=21≈2.9<△E_rot>_v″=15.对于v″=16,证实了振动—振动能量转移的4-1近共振过程.在一次碰撞条件下,通过速率方程分析,得到RH（v″）-CO₂振转速率系数.对于v″=15,J=32-48,速率系数在1.25-0.33×10^-13cm³s^-1.之间;对于v″=21,速率系数在2.47-1.53×10^-13cm³s^-1之间,其能量相关性是明显的.     

K2分子23∏g—13∑u+漫射谱强度的碰撞诱导增强效应

用4415.6?CW激光线获得了5730?附近的K₂分子2³∏_g—1³∑_u⁺漫射荧光谱。实验研究了缓冲气体Ar气压强P对漫射谱峰值强度I_diff的碰撞诱导增强效应。用稳态碰撞模型描述了C¹∏_u—2³∏_g间的能量转移过程,推导出了I_diff-P函数关系,对实验数据进行了令人满意的拟合。这种拟合表明:适当变更实验装置,利用本文模型可以得到C¹∏_u—2³∏_g间的能级交叉速率和碰撞诱导转移速率。 关键词：     

1.39 μm附近H2O谱线参数测量及其在燃烧动力学中的应用

将可调谐半导体激光吸收光谱技术应用于高温气体浓度在线检测,谱线参数的准确性非常重要。为利用红外波段进行燃烧生成H₂O的浓度在线测量,需要实验校准H₂O的谱线参数,尤其是Ar加宽系数,该系数对燃烧反应速率测量和机理验证至关重要。采用半导体激光器作为光源,结合实验室搭建的谱线参数测量系统,采集了1.39 μm波段附近H₂O的4条吸收谱线信号,获得了谱线线强、自加宽系数和N₂加宽系数,与HITRAN数据库和文献结果进行了对比,均吻合较好。首次系统地获得了该波段谱线的Ar加宽系数。在谱线参数确定基础上,获得了在反射激波高温条件下H₂/O₂/Ar燃烧生成H₂O的浓度随时间的演变曲线,验证了相应燃烧动力学机理。结果为利用该波段进行含氢燃料燃烧过程H₂O浓度测量及相关高温燃烧动力学研究提供了可靠的实验依据。     

高气压直流辉光CH4/H2等离子体的气相过程诊断

对高气压(约100 Torr) 直流辉光碳氢等离子体的气相过程进行了光谱和质谱原位诊断. 在高气压下, 等离子体不同区域光发射特性存在明显差异. 正柱区存在着以C₂和CH为主的多个带状谱和分立谱线, 阳极区粒子发射谱线明显减少, 而在阴极区则出现大量复杂的光谱成分, 表明高气压情形下等离子体与阴极间强烈的相互作用将导致复杂的原子分子过程. 从低气压到高气压演变过程中, 电子激发温度降低而气体分子转动温度升高. 在高气压下, 高甲烷浓度导致C₂, C₂H₂及C₂H₄增多而C₂H₆减少. 表明在高气压条件下, 气体温度对气相过程的影响作用显著增强. 关键词： 高气压直流等离子体 光发射谱 质谱     

YVO4：Eu3+纳米微粒发射光谱与温度的关系

测量了非选择激发下YVO₄:Eu³⁺纳米微粒中Eu³⁺的⁵D₀→⁷F₂发射光谱随温度的变化.低温下的光谱是很多谱线叠加在一起形成的宽带;而室温下主要是与体材料相似的两条分离谱线.根据选择激发下YVO₄:Eu³⁺的发射光谱研究得到的结论,把发射光谱分解为两部分之和,一部分来自占据靠近纳米微粒中心的格位的Eu³⁺离子发射谱线具有与体材料相近峰值;另一部分来自占据靠近表面位置的Eu离子,发射分布在更大的光谱范围内.这两部分发光的相对强度随温度变化的分析表明,YVO₄:Eu³⁺纳米微粒发射光谱随温度的变化是由于靠近表面的Eu通过表面猝灭中心猝灭而引起的.     

块体金属玻璃Zr46.75Ti8.25Cu7.5Ni10Be27.5的超导与负电阻温度系数

测量了块体金属玻璃Zr_46.75Ti_8.25Cu_7.5Ni₁₀Be_27.5在退火前后其电阻值随温度的变化,测量的温度范围为1.5—300K.样品在退火前后都发现有超导现象.零磁场下其超导转变温度T_c分别为1.84和3.76K.在5—300K温度范围内,原始样品具有负的电阻温度系数.如果取Zr, Ti, Cu, Ni及Be分别贡献出1.5, 1.5, 0.5, 0.5及两个传导 关键词： 块体金属玻璃 超导 电阻温度系数     

Intensity measurements in the v4-Fundamental of CH4 at planetary atmospheric temperatures

Measurements of spectral transmittance have been performed in the v₄-fundamental band of ¹³CH₄ at low temperatures of planetary atmospheric interest with spectral resolution of 0.06 cm^-1. Comparison of observed and computed spectral transmittance on a line-by-line basis has yielded line strengths. Best agreement between measured and computed spectra was obtained when the absolute intensity of the band was taken as 123 cm^-2 atm^-1 at 296 K.     

A laboratory study of the 8.65 μm fundamental of CH3D at temperatures relevant to titan''s atmosphere

Spectral transmittance measurements have been performed in the v₆-fundamental of ¹²CH₃D at 153 K. Relevant to the studies of the emission spectra of Titan recorded by the IRIS instruments on board Voyagers 1 and 2, N₂ has been used as the broadening gas. Excellent agreement between experimental and theoretical spectral transmittance has been the result of using N₂-broadened line widths and their dependence upon temperature measured by us in the v₂-fundamental and S = 63.6 cm^-2 atm^-1 for the absolute intensity of the v₆-fundamental.     

Thermal infrared lines of methane broadened by nitrogen at low temperatures

Measurements of spectral transmittance in the v₄-fundamental band of ¹²CH₄ have been performed at low temperatures using a Fourier transform spectrometer with apodized spectral resolution of 0.06 cm^-1. With applications to lines formed in the atmospheres of Titan and Earth in mind, N₂ has been used as the broadening gas. Comparisons of observed and computed spectral transmittances on a line-by-line basis have yielded line strengths, N₂-broadened half-widths and their variation with temperature. Best agreement between measured and computed spectra was obtained when the absolute intensity of the band was taken as 128 cm^-2-atm^-1 at 296 K. Line widths were found to vary as Tⁿ with n = -1.0 for lines of the F-species and 0.63 for the A-species. Our measured line widths are considerably larger than those used in the AFGL compilation.     

H2-broadening coefficients in the ν3 band of CH3D at low temperatures

Using a diode-laser spectrometer, we have measured H₂-broadening coefficients of CH₃D at low temperatures (153.5, 183.5, and 223.5 K) for four lines in the ν₃ band. The collisional widths are obtained by fitting each absorption line with three lineshape models: the Voigt, Rautian, and Galatry profiles. The broadening coefficients are also calculated on the basis of a semiclassical model of interacting linear molecules by considering an atom-atom Lennard-Jones potential in addition to electrostatic contributions. By comparing the broadening coefficients at room and low temperatures the temperature dependence of these broadenings has been determined both experimentally and theoretically.     

Infrared absorption by acetylene in the 12–14 μm region at low temperatures

Spectral transmittance measurements have been performed on N₂-broadened lines of ¹²C₂H₂ and ¹²C¹³CH₂ in the 13.7 μm region at 153,200, and 296 K. From line-by-line comparison of observed and computed spectral transmittance, line strengths, half-widths, and their dependence on temperature have been deduced for conditions relevant to the atmospheres of Jupiter, Saturn, Titan, and Earth.     

CO2及其碳同位素比值高精度检测研究

改进了一种基于傅里叶变换红外光谱法测量CO₂气体的装置, 改进后的装置能够提高CO₂检测精度, 并能同时测量CO₂碳同位素比值. 研究了温度和压力对CO₂浓度值和CO₂碳同位素比值测量的影响规律. 利用该装置连续测量了标准CO₂气体和环境大气, 对标准CO₂气体测量得到的CO₂浓度值及其碳同位素比值进行温度和压力影响修正, 获得了较好的精度和准确度. 关键词： 光谱学 同位素比值 傅里叶变换红外光谱 二氧化碳     

A multispectrum analysis of the ν2 band of HCN: Part I. Intensities, broadening, and shift coefficients

Absolute intensities, self- and air-broadening coefficients, self- and air-induced shift coefficients and their temperature dependences have been determined for lines belonging to the P- and R-branches of the ν₂ band of H¹²C¹⁴N centered near 712 cm⁻¹. Infrared spectra of HCN in the 14-μm region were obtained at high resolution (0.002-0.008 cm⁻¹) using two different Fourier transform spectrometers (FTS), the McMath-Pierce FTS at the National Solar Observatory on Kitt Peak and the Bruker IFS 120HR FTS at the Pacific Northwest National Laboratory. Spectra were recorded with 99.8% pure HCN as well as lean mixtures of HCN in air at various temperatures ranging between +26 and −60 °C. A multispectrum nonlinear least squares technique was used to fit selected intervals of 36 spectra simultaneously to obtain the line positions, intensities, broadening, and shift parameters. The measured line intensities were analyzed to determine the vibrational band intensity and the Herman-Wallis coefficients. The measured self-broadening coefficients vary between 0.2 and 1.2 cm⁻¹ atm⁻¹ at 296 K, and the air-broadening coefficients range from 0.08 to 0.14 cm⁻¹ atm⁻¹ at 296 K. The temperature dependence exponents of self-broadening range from 1.46 to −0.12 while the corresponding exponents for air broadening vary between 0.58 and 0.86. The present measurements are the first known determination of negative values for the temperature dependence exponents of HCN-broadening coefficients. We were able to support our self-broadening measurements with appropriate theoretical calculations. Our present measurements are compared, where possible, with previous measurements for this and other HCN bands, as well as the parameters that are included in the 2000 and 2004 editions of the high-resolution transmission (HITRAN) database.     

N2-broadening coefficients in the ν2 and ν4 bands of PH3 at low temperature

N₂-broadening coefficients have been measured for 41 transitions of PH₃ at −100 °C in the ^QR branch of the ν₂ band and the ^PP, ^RP, and ^SP branches of the ν₄ band, using a tunable diode-laser spectrometer. The recorded lines with J values ranging from 1 to 13 and K from 0 to 10 are located between 1026 and 1093 cm⁻¹. The collisional widths are determined by fitting each spectral line with a Voigt profile, a Rautian profile, and a speed-dependent Rautian profile. The latter models provide larger broadening coefficients than the Voigt model. These coefficients have also been calculated on the basis of a semiclassical model of interacting linear molecules by considering an atom-atom Lennard-Jones potential in addition to the electrostatic contributions. By comparing broadening coefficients at room and low temperatures, the temperature dependence of these broadenings has been determined both experimentally and theoretically.     

Ar-Broadening of isotropic Raman lines in the ν2 band of acetylene

Using a high resolution Raman spectrometer, we have measured Ar-broadening coefficients in the ν₂Q branch of C₂H₂ for 22 lines at 295 K, 20 lines at 174 K, and 16 lines at 134 K. These lines with J values ranging from 1 to 23 are located in the spectral range 1970.9-1974.3 cm⁻¹. The collisional widths are obtained by fitting each spectral line with a Rautian profile. The resulting broadening coefficients are compared with theoretical values arising from close coupling and coupled states calculations. A satisfactory agreement is obtained at room as well as at low temperatures, especially for odd J lines. By comparing broadening coefficients at 295, 174, and 134 K from a simple power law, the temperature dependence of these broadenings has been determined both experimentally, and theoretically.     

Argon-broadening coefficients in the ν5 band of acetylene at room and low temperatures

Ar-broadening coefficients have been measured in the P- and R-branches of the ν₅ fundamental band of C₂H₂ for 30 lines at room temperature and 8 lines at −100 °C, using a tunable diode-laser spectrometer. These lines with J values ranging from 2 to 27 are located in the spectral range 665-795 cm⁻¹. The collisional widths are obtained by fitting each absorption line with three lineshape models: the Voigt profile, the Rautian profile accounting for the Dicke narrowing effect, and a general Rautian profile including the absorber speed-dependent collisional broadening. The latter model provides significantly larger broadening coefficients than the Voigt model. These coefficients are also calculated from a semiclassical theory performed by using a simple intermolecular potential with two adjustable parameters. Finally, the temperature dependence of the broadening coefficients has been determined both experimentally and theoretically.