Spectroscopic lineshape study of the self-perturbed oxygen A-band

This paper reports accurate line positions, intensities, self-broadening, -shift and -line mixing coefficients for 56 rotational transitions from multispectrum fits of low noise, high-resolution Fourier-transform spectra. The measured line intensities are within the statistical spread of the previous measurements available in the literature—thus contributing to the efforts to measure the oxygen A-band intensities with an accuracy better than 1%. We determined the integrated band strength and Einstein A coefficient. Using our spectrum calibration method we could clearly show for the first time that there is a meaningful statistical discrepancy in the frequency standards used in spectroscopic studies for the oxygen A-band. We were able to explain how this discrepancy leads to two different sets of shifts reported in the literature and demonstrate the need for precise frequency-type transition wavenumber measurements of the oxygen A-band transitions. We observed deviations from the conventional Voigt profile due to speed-dependent broadening and line mixing effects. Dicke narrowing was observed on a selected group of spectra recorded at pressures between 98 and 337 Torr. The Dicke narrowed lineshapes were best modeled using a Galatry profile implemented using a fixed value for the velocity-changing collision rate. The weak line mixing coefficients were determined from fits using the speed-dependent models. Exponential Power Gap (EPG) and Energy Corrected Sudden (ECS) scaling laws were used to calculate the self-broadening and self-line mixing coefficients.     

Einstein A coefficients and absolute line intensities for the E2Π–X2Σ+ transition of CaH

Einstein A coefficients and absolute line intensities have been calculated for the E²Π–X²Σ⁺ transition of CaH. Using wavefunctions derived from the Rydberg–Klein–Rees (RKR) method and electronic transition dipole moment functions obtained from high-level ab initio calculations, rotationless transition dipole moment matrix elements have been calculated for all 10 bands involving v′=0,1 of the E²Π state and v″=0,1,2,3,4 of the X²Σ state. The rotational line strength factors (Hönl–London factors) are derived for the intermediate coupling case between Hund's case (a) and (b) for the E²Π–X²Σ⁺ transition. The computed transition dipole moments and the spectroscopic constants from a recent study [Ram et al., Journal of Molecular Spectroscopy 2011;266:86–91] have been combined to generate line lists containing Einstein A coefficients and absolute line intensities for 10 bands of the E²Π–X²Σ⁺ transition of CaH for J-values up to 50.5. The absolute line intensities have been used to determine a rotational temperature of 778±3 °C for the CaH sample in the recent study.     

2 μm附近CO2谱线参数测量及应用

吸收光谱技术用于痕量气体浓度监测,特别是在气体分子稳定同位素丰度探测中,吸收谱线参数的准确性非常重要,目前普遍使用的HITRAN数据库中给出的各项参数具有一定的不确定性。为利用2.0 μm激光波段进行CO₂浓度及其同位素丰度探测,需要对该波段的CO₂吸收谱线参数进行校准,采用窄线宽分布反馈式二极管激光器作为光源,结合自行搭建的谱线参数测量系统,采集了2.0 μm波段10条CO₂吸收谱线,获得了各谱线的位置、强度、自加宽系数和N₂加宽系数,并与HITRAN2012数据库中相应的数据进行对比发现两者之间吻合较好,CO₂谱线强度和自加宽系数相对偏差均小于2%。实测实验室大气的CO₂浓度为440 ppm,13CO₂的丰度值δ为-9‰。测量结果为该波段应用于CO₂浓度及13CO₂同位素丰度的实时在线探测提供了重要参考依据。     

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     

Vibrational-rotational Einstein coefficients for HF/DF and HCl/DCl

The RKR potential functions have been combined with the best experimentally based dipole functions to calculate the Einstein coefficients for HF/DF and HCl/DCl. Calculations were done for the Δν = 1,2,3 transitions for a wide range of ν′ (?15 for HF/DF and ?8 for HCl/ DCl) and J′ (?25). Experimental tests involving comparison of P- and R-branch line intensities for high-J′ transitions of the HF (ν₁ → ν₀, ν₂ → ν₁ and ν₃ → ν₂ bands) and the Δν = 2 and Δν = 1 transitions for HF/DF and HCl are done to examine the reliability of the Einstein coefficients for the rotational and vibrational levels, respectively. Good agreement is obtained for HF/DF even for the high-J′ R-branch intensities which vary markedly with J′. But the data suggest improvement is needed in the dipole functions for HCl (and DCl).     

基于可调谐半导体激光吸收光谱的H2O分子光谱参数测量研究

气体分子吸收谱线的光谱参数是影响吸收光谱测量精度的重要因素,分子光谱数据库中收录的光谱参数大都具有较大的不确定度,用以测量气体温度等参数时会产生较大的测量误差。为了获得可用于燃烧场诊断的H₂O谱线的光谱参数,采用时分复用技术,在温度、压强和H₂O组分浓度可控的环境中对1.4 μm附近的吸收光谱开展了研究。对7 185.60和7 454.45 cm-1两条H₂O谱线的线强度、展宽系数及其温度指数等光谱参数进行测量,实验结果表明,两条谱线的线强度测量值与数据库中的值偏差分别小于2.61%和4.65%,不确定度都小于4%。     

Time-resolved spectroscopy for 5s~('4)D_(7/2) state transitions undergoing electron–ion recombination in femtosecond laser-produced copper plasma

In the femtosecond laser-produced Cu-plasma, the transient transition dynamics that the excited state 5s~('4)D_(7/2) via electron–ion recombination transfers to 4p~('4)F_(9/2)~0(465.11 nm, Λ1 line) and 4p~('4)D_(7/2)~0(529.25 nm, Λ_2 line) states are investigated by using the time-resolved spectroscopy. The occupation number and relevant lifetime of the excited state 5s~('4)D_(7/2),the temporal evolutions of spectral intensities for Λ_1 line and Λ_2 line emissions are demonstrated to be in direct proportion to the employed laser intensity, which reveals the transient features of transition dynamics clearly differing from that resulted in the traditional collision excitation. Furthermore, some unique characteristics for Λ_1 and Λ_2 transitions stemming from electron–ion recombination are examined in detail.     

HBr分子的爱因斯坦自发辐射系数的计算

本文从第一性原理出发,计算了ＨＢｒ分子ｖ≤７,Ｊ≤１４,Δｖ＝１,Ｒ,Ｐ支谱线的爱因斯坦自发辐射系数Ａ＾ｖ‘Ｊ’ｖ＾ｎＪ＾ｎ。测量了ＨＢｒ红外发射的振转谱线强度,证实由理论计算获得的Ａ＾ｖＪ’Ｖ＾ｎＪ＾ｎ系数是可靠的。     

0.35μm激光与金靶耦合发射X光能谱分析

 利用改进后的More模型计算Au等离子体各电离度离子的Einstein系数和线发射强度。在0.35μm激光与金平面靶耦合产生晕区等离子体条件下,求解离子模型定态速率方程组得到离子布居概率,从而求出X光线发射能谱。将此能谱与JB19程序计算得到的出系统外边界光子能谱进行了比较。     

Experimental Line Parameters of the Oxygen A Band at 760 nm

To support atmospheric remote sensing applications, line positions, intensities, self- and nitrogen-broadened linewidths and their temperature dependences and pressure-induced shifts in line positions at room temperature were measured up to J' and N' = 22 for the oxygen A band at 13 122 cm(-1). Line intensities were obtained with 1% precisions and 2% absolute accuracies using absorption spectra recorded at Doppler-limited (0.02 cm(-1)) resolution with the McMath Fourier transform spectrometer (FTS) located at Kitt Peak National Observatory/National Solar Observatory in Arizona. The oxygen line positions were calibrated using near-infrared transitions of the 2-0 and 3-0 bands of CO as secondary standards. The intensities and positions of seven H(2)O lines near 13 900 cm(-1) were also remeasured to validate the FTS performance. The O(2) intensities fell within 1% of the values currently assumed for the molecular databases, but it was found that broadening coefficients and line positions should be revised for the A band of molecular oxygen. Copyright 2000 Academic Press.     

CO分子振转光谱的理论研究

采用从头算的多参考组态相互作用(MRCI)方法并结合基组aug-cc-pCVQZ计算了CO分子基态(X1Σ+)的势能曲线和偶极矩曲线,得到的势能曲线、偶极矩曲线分别与RKR势、文献的偶极矩曲线吻合较好。利用所得的势能,求解双原子分子核运动的Schrdinger方程找到了CO分子X1Σ+态转动量子数J=0时的70个振动态,对于每一振动态,分别计算了其振动能级G(v)、转动惯性常数B_v和离心畸变常数D_v,并把计算结果与已知的42个实验值做了详细比较,结果表明,计算的振动能级G(v)、转动惯性常数B_v、离心畸变常数D_v与实验值符合较好。利用G(v),B_v导出的光谱常数[谐振频率ω_e(2 160.1 cm-1)、非谐振频率ω_eχ_e(13.1 cm-1)、转动常数B_e(1.918 cm-1)、振转耦合常数α_e(0.017 3 cm-1)]也与实验值的光谱常数[ω_e(2 169.8 cm-1),ω_eχ_e(13.3 cm-1),B_e(1.931 cm-1),α_e(0.017 5 cm-1)]较为符合,这在一定程度上证明了方法MRCI/Aug-cc-pCVQZ对CO分子基态性质的计算是合适而可靠的。利用乘积近似方法计算了CO分子在常温、中温、高温时的配分函数,在此基础上,计算了CO分子在T=296 K时的1-0跃迁带的谱线强度,通过比较发现,计算所得的线强度与HITRAN数据库符合较好。进一步计算的CO分子X1Σ+态1-0,2-0,3-0,4-0,2-1,3-1和4-1跃迁带的带强度也与实验值较为吻合,同时首次计算了CO分子X1Σ+态3-2跃迁带、4-2跃迁带的线强度及带强度。     

Infrared radiation modeling of NO,OH, CO,H2O,and CO2 for emissivity/radiance prediction at high temperature

In the present study, infrared radiation modeling of NO, OH, CO, H₂O, and CO₂ molecules was devised based on a line-by-line method by utilizing a structured radiation analysis package, SPRADIAN07, coupled with up-to-date spectroscopic parameters and recent high-resolution radiation databases. An infrared calculation module was newly implemented in SPRADIAN07 for simulating the emissivity/radiance of NO and OH. The line positions of NO and OH molecules were determined by diagonalizing the Hamiltonian matrices of each molecule. The Einstein coefficients were obtained from either radiation databases or available calculated temperature-related line intensities. H₂O, CO₂, and CO were also modeled based on the high-resolution radiation databases, HITEMP2010 and CDSD-4000. When the line-by-line calculations were performed using the radiation databases, a parallel computing technique based on PC clusters was adopted for fast and efficient evaluation. The line-by-line model devised in the present study was validated by comparing the results with existing measurements. The simulations with room air absorption composed of H₂O and CO₂ were also carried out. The spectra taken from a plasma torch and those from a rocket plume were calculated by utilizing the present radiation model. It was shown that the calculated spectra are in good agreement with observed ones.     

Einstein A-coefficients and statistical weights for molecular absorption transitions in the HITRAN database

This paper describes the calculation of the statistical weights and the Einstein A-coefficients for the 39 molecules and their associated isotopologues/isotopomers currently present in the line-by-line portion of the HITRAN database. Calculation of the Einstein A-coefficients was carried out using the HITRAN line intensities and the necessary statistical weights. The Einstein A-coefficient and the statistical weights of the upper and lower levels of the transition were added in the new format of the line parameters for the most recent edition of the HITRAN database.     

基于可调谐激光吸收光谱技术的脱硝过程中微量逃逸氨气检测实验研究

为了对电厂脱硝过程中逃逸的微量氨气进行在线检测,实验室采用可调谐激光吸收光谱技术对常温常压下以及不同温度下的低浓度氨气进行了测量试验,其中电厂逃逸氨气检测处温度约为650 K。通过分析近红外波段的氨气吸收谱线,并考虑实际测量环境H₂O和CO₂等浓度很大的气体吸收谱线的干扰,实验选取2.25 μm附近的ν₂+ν₃谱线作为浓度检测谱线。为了验证所选谱线对低浓度NH₃的测量能力,实验对H₂O,CO₂和NH₃的吸收谱线进行模拟,发现低浓度NH₃受较大浓度的H₂O和CO₂谱线的干扰较小,尤其是CO₂谱线的干扰可以忽略不计,且2.25 μm处谱线强度远远大于通讯波段1.53 μm处的谱线。基于新型Herriott池以及高温管式炉,结合可调谐激光吸收光谱中的直接吸收技术和波长调制技术,实现了对不同温度下超低浓度NH₃的高分辨率快速检测。常温常压下其线型函数可以利用洛伦兹线型来近似描述,直接吸收测量技术可以使探测极限降低到0.225×10-6。通过采用简单降噪处理技术如多次平均、简单小波分析等,得到不同温度下的谐波信号与浓度具有良好的线性关系,为采用可调谐激光吸收光谱技术进行现场低浓度逃逸氨气检测提供了很好的依据。     

Collision-induced emission of singlet oxygen in the visible spectral region at temperatures of 90–315 K

Collision-induced emission of singlet oxygen molecules is studied using spectrometers calibrated for absolute spectral sensitivity. The collision-induced emission-rate constants at wavelengths of 479, 514, 577, 634, and 703 nm are determined within the temperature range 90–315 K. It is found that the intensities of the emission bands increase with decreasing temperature below 100 K. The interrelation between the collision-induced emission-rate constants and the intensities of the collision-induced absorption bands is discussed. The Einstein coefficients for spontaneous emission of excited free O₂: O₂ complexes are estimated.     

Absorption intensities for vibration-rotation bands and the dipole-moment expansion of HBr

Line intensities in the four 0–2, 0–3, 0–4, 0–5 vibration-rotation bands of HBr were measured. The electric dipole matrix elements 〈0|M|ν'〉 for vibrational transitions with ν'?5 have been calculated by using a Dunham potential and the analytical solution of the Schrödinger equation described by R.H. Tipping. A dipole-moment expansion accurate to M₅ was determined by fitting these matrix elements to the available experimental data on line intensities. The experimental results were also used to calculate the Einstein coefficients of the R₀ lines for the bands ν' → ν′' with ? ν' ? 5.     

Cumulative "roof effect" in high-resolution in vivo 31P NMR spectra of human calf muscle and the Clebsch-Gordan coefficients of ATP at 1.5 T

NMR spectra of non-weakly coupled spin systems exhibit asymmetries in line intensities known as "roof effect" in 1D spectroscopy. Due to limited spectral resolution, this effect has not been paid much attention so far in in vivo spectroscopy. But when high-quality spectra are obtained, this effect should be taken into account to explain the quantum-mechanical fine structure of the system. Adenosine 5'-triphosphate (ATP) represents a 31P spin system with multiple line splittings which are caused by J-couplings of medium strength at 1.5 T. We analyzed the ATP roof effect in vivo, especially for the beta-ATP multiplet. The intensities of its outer resonances deviate by ca. 12.5% from a symmetrical triplet. As this asymmetry reflects the transition from Paschen-Back to Zeeman effect with total spin that is largely broken up, the Clebsch-Gordan coefficients of the system can be indicated in analogy to the hyperfine structure of hydrogen. Taking the roof effect into account, the chi2 of fitting in vivo ATP resonances is reduced by ca. 9% (p<0.005).     

13CH4分子v3振动带空气和氮气加宽系数温度依赖性研究

采用中红外波段连续可调谐二极管激光器和自行研制的低温吸收池, 测量了温度为296 K, 252 K, 213 K, 173 K时, 3.38 μm附近¹³CH₄分子的四条跃迁谱线的氮气和空气加宽光谱; 首次通过实验获得空气和氮气对¹³CH₄分子的碰撞加宽系数, 以及谱线加宽系数的温度依赖系数. 实验过程中, 利用Voigt线型对所测量的光谱进行拟合. 实验结果表明, 氮气和空气对¹³CH₄分子的碰撞诱导加宽系数随温度的降低而增大; 相同温度下, 氮气对¹³CH₄分子的碰撞加宽系数普遍大于空气加宽系数. 实验数据为地球和外星体大气遥感探测提供了依据.     

Line positions and intensities of acetylene in the 2.2-μm region

More than 440 line positions and intensities of 8 bands of acetylene are measured in the 2.2-μm spectral region. A multispectrum fitting procedure has been applied to retrieve line parameters. The average absolute accuracy of the line parameters obtained in this work is estimated to be ±0.0005 cm⁻¹ for the line positions, and ±5% for the line intensities. Vibrational transition dipole moment and Herman-Wallis coefficients are determined for two of the studied bands. An unusual rotational dependence of the vibrational-rotational transition dipole moment of remaining bands has been found. All measured line intensities are treated simultaneously within the framework of the effective operators approach. The sets of effective dipole moment parameters obtained reproduce the observed line intensities within the experimental uncertainty.