用可调谐二极管激光光谱仪观测3657—3708cm~(-1)区域CO_2高分辨振转光谱

用可调谐二极管激光光谱仪观测到3657—3708cm~(-1)区域内CO_2各种同位素分子的9个振转谱带。首次观测到~(12)C~(16)O~(17)O的10011—00001谱带和~(12)C~(16)O~(18)O的11111—01101谱带,对其余7个谱带则扩充了其观测振转线的数目。用最小二乘方拟合法计算了各谱带的光谱常数,发现CO_2分子常数表中~(12)C~(16)O~(17)O的10011—00001谱带中心v的计算值比本实验观测值大0.287cm~(-1),而~(12)C~(16)O~(12)O的11111—01101谱带中心v_0的计算值则比本实验观测值小0.048cm~(-1)。     

采用多参考组态相互作用方法研究AsN( X1 Σ+ )自由基的光谱常数与分子常数

采用内收缩多参考组态相互作用方法和相关一致基对AsN(X ¹ Σ⁺)自由基的势能曲线进行了研究. 计算过程中对两原子分别采用不同基组,As原子为aug-cc-pV5Z基组,N原子为aug-cc-pV6Z基组. 通过最小二乘法将势能曲线拟合成Murrell-Sorbie函数,并进一步计算得到AsN(X ¹ Σ⁺)自由基的光谱常数.光谱常数分别为D_e=4.97 eV,R_e=0.16259 nm, ω_e=1061.14 cm^-1, ω_ex_e=5.4715 cm^-1, B_e=0.53919 cm^-1和α_e=0.003409 cm^-1. 通过比较发现它们与实验值符合非常好. 利用得到的解析势能函数, 求解双原子分子核运动的径向Schrödinger方程, 找到了J=0时该自由基存在的全部67个振动态. 对于每一振动态, 分别计算了振动能级、经典转折点、惯性转动常数和离心畸变常数. 与实验结果比较后发现,计算结果达到了很高的计算精度. 关键词： AsN 势能曲线 光谱常数 分子常数     

NO分子b~4Σ~-—a~4Π_i(4,0)带的吸收光谱

通过对NO与He流动混合气体放电,产生了激发态的NO(a⁴Ⅱ_ii)分子.利用光外差-浓度调制吸收光谱技术测量了NO分子在12530-12850 cm^-1波段内的吸收光谱,并标识出b⁴∑^--a⁴Ⅱ_i（4,0）带在该波段内的324条跃迁谱线.采用标准⁴∑^-—⁴Ⅱ_i哈密顿量模型,通过非线性最小二乘法拟合其中267条谱线,拟合残差(0.0071 cm^-1)接近实验系统测量误差(0.007 cm^-1).获得的主要分子常数与文献提供的常数符合,并且拟合得到了精细结构分子常数.     

15N16O的激光磁共振谱与同位素分子15N17O和15N18O的光谱分析

采用内腔式饱和吸收技术获得Lamb凹陷,使CO激光磁共振谱仪的灵敏度及分辨率大大提高.利用该技术对自然丰度下¹⁵N¹⁶O的X²Π(υ=1)←X²Π(υ=0)塞曼跃迁进行测量,实现了包括Λ双分裂在内的各种精细结构的谱分辨.结合已发表的¹⁵NO同位素分子光谱实验数据进行分析计算,拟合得到迄今最完备、最精确的各相关同位素分子¹⁵N^mO(m=16—18)的结构参 关键词：     

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.     

吡啶B1(nπ*)态(2+3)偏振共振多光子电离谱中6a10带型模拟及转动常量确定

通过模拟吡啶B₁(nπ^*)态(2+3)偏振共振多光子电离谱中转动结构可部分分辨的6a¹₀带型,获得了该态上吡啶分子的转动常量,分别为A′=0.21670cm^-1,B′=0.16758cm^-1,C′=0.09450cm^-1.表明氮原子上的一个孤对电子跃迁进入π^*轨道后氮原子自身电负性减弱,吡啶分子构架总体上张开.此外,比较6a^关键词：     

Ag离子注入非晶SiO2的光学吸收、拉曼谱和透射电镜研究

能量为200keV的Ag离子，以1×10¹⁶，5×10¹⁶，1×10¹⁷ cm^-2的剂量分别注入到非晶SiO₂玻璃，光学吸收谱显示：注入剂量为1×10¹⁶ cm^-2的样品的光吸收谱为洛伦兹曲线，与Mie理论模拟的曲线形状一致；注入剂量较大的5×10¹⁶，1×10¹⁷ cm^-2的谱线共振吸收增强，峰位红移并出现伴峰. 透射电镜观察分析表明，注入剂量不同的样品中形成的纳米颗粒的大小、形状、分布都不同，注入剂量较大的还会产生明显的表面溅射效应，这些因素都会影响共振吸收的峰形、峰位和峰强. 当注入剂量达到1×10¹⁷ cm^-2时，Ag纳米颗粒内部可能还形成了杂质团簇. 关键词： 离子注入 纳米颗粒 共振吸收 红移     

激光诱导NO2分子500—532nm区荧光激发谱的实验研究

用准分子激光抽运可调谐染料窄带激光测定了室温下NO₂分子500—532nm区高分辨荧光激发谱,在两个较强吸收区505—510nm和513—520nm范围内标识了25个振动带,并作了转动分析,得到了相应的带头位置、转动常数和旋-转偶合常数等分子光谱常数,在25个振动带中有5个谱带是新发现的,所有得到转动分析的谱线均属于平行跃迁X～ ² A₁—A～²Ｂ₂,对实验结果的分析表明电子激发态A～ 关键词： 激光诱导荧光激发谱 振动带 转动分析     

SiH4紫外多光子电离光谱的转动分析

本工作用激光扫描步长6×10^-4nm观测了SiH₄多光子电离光谱中363.52nm附近的精细结构。SiH₄被三光子共振激发后,作为略不对称陀螺处理。大多数转动谱线被论证为v₂振动垂直谱带的一个Q支,并推算出激发态转动常数B＇=3.04±0.01cm^-1。 关键词：     

MRCI方法研究CSe(X1Σ+)自由基的光谱常数和分子常数

采用内收缩多参考组态相互作用方法在0.08—2.5 nm的核间距范围内计算了CSe(X¹Σ⁺)自由基的势能曲线.为确保势能曲线的计算精度,C原子使用较大的相关一致基aug-cc-pV5Z,Se原子使用最大的相对论赝势基aug-cc-pV5Z-pp.对CSe(X¹Σ⁺)自由基的势能曲线进行了拟合,并进行了同位素识别,得到了该自由基6个主要同位素分子(¹²C^{74< 关键词： 同位素识别 势能曲线 光谱常数 分子常数}     

CO2 line intensity measurements around 1.6 μm

Using Fourier transform spectra and a multispectrum fitting procedure, 271 absolute line intensities of ¹²C¹⁶O₂ have been measured around 1.6 μm, for the three cold bands 30014-00001, 30013-00001, and 30012-00001, and for the two hot bands 31113-01101 and 31112-01101, extending from 6035 to 6380 cm⁻¹. Accuracies are on the average 3 and 5% for cold and hot bands, respectively. Vibrational transition dipole moments and Herman-Wallis coefficients are reported for each band. Comparisons are made with previous experimental results and with data available in the HITRAN database and the Carbon Dioxide Spectroscopic Databank (CDSD).     

Line positions and strengths of OCO, OCO and OCO between 2200 and 7000 cm

Line positions and strengths of ¹⁶O¹²C¹⁸O (628), ¹⁸O¹²C¹⁸O (828) and ¹⁷O¹²C¹⁸O (728) were measured between 2200 and 7000 cm⁻¹ using 22 near infrared (NIR) absorption spectra recorded at 0.01-0.013 cm⁻¹ resolution with the McMath-Pierce Fourier transform spectrometer located at the National Solar Observatory on Kitt Peak, Arizona. These data were obtained at room temperature using absorption cells with optical path lengths ranging from 2.4 to 385 m; the cells were filled with natural and ¹⁸O-enriched samples of CO₂ at pressures ranging from 0.54 to 252 torr. The observed line positions were analyzed to obtain the upper state band centers and rotational constants for 17 bands of ¹⁶O¹²C¹⁸O, 19 bands of ¹⁸O¹²C¹⁸O and 8 bands of ¹⁷O¹²C¹⁸O. The majority of the ¹⁸O¹²C¹⁸O and ¹⁷O¹²C¹⁸O bands were measured for the first time. In addition, the rotational constants for the lower states 00001, 01101e and 01101f were derived for all three species using the method of combination differences in which the averaged values obtained from the line positions of two or more bands were least-squares-fitted. Rovibrational parameters were also obtained for the 02201e, 02201f, 10002 and 10001 states of ¹⁸O¹²C¹⁸O. The line position analysis revealed that transitions of the levels 38 ? J′ ? 46 of the 11111f ← 01101f band of ¹⁸O¹²C¹⁸O are perturbed. Perturbed transitions were also observed for the 12212 ← 02201 band and in the high-J transitions (J′ ? 49) of the 20012 ← 00001 band of ¹⁸O¹²C¹⁸O. Band strengths and Herman-Wallis-like F-factor coefficients were determined for 21 bands of ¹⁶O¹²C¹⁸O, 25 bands of ¹⁸O¹²C¹⁸O and 8 bands of ¹⁷O¹²C¹⁸O from least-squares fits to more than 3700 measured transition intensities; band strengths and line positions for 34 of these bands were obtained for the first time.     

CO2 line intensity FTS measurements with 1% assumed accuracy in the 1.5-1.6 μm spectral range

Using Fourier-transform spectra and a multispectrum fitting procedure, 124 absolute line intensities of ¹²C¹⁶O₂ are obtained for the cold band 30011-00001 and the hot band 01131-01101 between 6460 and 6950 cm⁻¹. Vibrational transition dipole moments squared and Herman-Wallis coefficients are reported for each band. Cross comparisons made with previous experimental results and with data available in the HITRAN and Carbon Dioxide Spectroscopic Databank (CDSD), bring some confidence on the good level of accuracy of the present results. Motivated by the demanding needs of some atmospheric experiments dedicated to the survey of the carbon cycle, an additional evaluation of potential absolute line intensity measurement limit is also performed on recently published carbon dioxide absolute line intensity independent measurements. These are obtained in two different laboratories on the bands 30013-00001 and 30012-00001 both located in the 1.6 μm spectral window. It is shown that Fourier-transform experimental CO₂ line intensity determination is approaching the challenging required figure of about 0.3% accuracy needed for the survey of the atmospheric carbon cycle.     

Infrared spectroscopy of CO2 isotopologues from 2200 to 7000 cm−1: I—Characterizing experimental uncertainties of positions and intensities

Fourier transform spectra of carbon dioxide enriched in ¹⁷O and ¹⁸O have been recorded in LADIR (Paris, France) with the Bruker IFS 125-HR between 2000 and 9000 cm^?1 at an unapodized resolution of 0.0056 cm^?1. In this contribution we present a total of 1861 line positions and intensities retrieved for 46 bands of ¹²CO₂ isotopologues between 2000 and 7000 cm^?1 including the ¹⁶O¹²C¹⁶O, ¹⁷O¹²C¹⁷O, ¹⁸O¹²C¹⁸O, ¹⁶O¹²C¹⁸O, ¹⁶O¹²C¹⁷O, and ¹⁷O¹²C¹⁸O species. The objective of this first part of work was to examine the absolute concentrations of various CO₂ isotopologues in the sample by comparing our measurements of the line intensities to those available in literature and in HITRAN 2008. The accuracy of the determined abundances of the various isotopologues in our sample could be estimated to be about 2–7% for all above listed isotopologues except for ¹⁷O¹²C¹⁷O for which the accuracy on abundance is estimated to be around 20%. The accuracy of the line positions retrieval is better than 0.1×10^?3 cm^?1. We estimate the relative uncertainty of the line intensities retrieval to be around 1–2% (except for very weak lines), whereas the absolute accuracy to be around 3–15% depending mainly on the accuracy of the determination of the partial pressures for the various isotopologues in our sample, but also on the line strengths and on the spectral region. The estimation of the partial pressures of the various CO₂ isotopologues is crucial for retrieving absolute values of line intensities, but this is not an easy task because there are no absolute calibration standards for CO₂ intensities. Among the results obtained in this work, measurements are obtained for the first time for the 10011–00001 band of ¹⁷O¹²C¹⁷O, ¹⁶O¹²C¹⁷O, ¹⁶O¹²C¹⁸O, and ¹⁸O¹²C¹⁸O species, for the 00011–00001 band of ¹⁷O¹²C¹⁸O, and for the 2001i–00001 (i=1, 2, and 3) bands of the ¹⁶O¹²C¹⁷O isotopologue.     

Fourier transform spectroscopy of CO2 and OCO in the 3800-8500 cm region and the global modeling of the absorption spectrum of CO2

The absorption spectrum of the ¹⁸O enriched carbon dioxide has been recorded at Doppler limited resolution with a Fourier transform spectrometer in the spectral range 3800-8500 cm⁻¹. Seventeen cold bands (14Σ-Σ and 3Σ-Π) and nine hot bands (9Π-Π) of ¹²C¹⁸O₂, nineteen cold bands (18Σ-Σ and 1Σ-Π) and eighteen hot bands (6Σ-Σ, 9Π-Π and 3Δ-Δ) of ¹⁶O¹²C¹⁸O have been observed. Among them, 14 ¹²C¹⁸O₂ bands and 12 ¹⁶O¹²C¹⁸O bands are observed for the first time. The spectroscopic parameters G_v, B_v, and centrifugal distortion constants, have been determined for all observed bands. Effective Hamiltonian parameters for the ¹²C¹⁸O₂ isotopic species are retrieved from the global fitting of the observed line positions presented in this paper and collected from the literature. As the result, 65 obtained effective Hamiltonian parameters reproduce 5443 observed line positions of 73 ¹²C¹⁸O₂ bands with RMS = 0.00145 cm⁻¹.     

Line strengths of CO2: 4550-7000 cm

Line positions and strengths of ¹²C¹⁶O₂ were measured between 4550 and 7000 cm⁻¹ using near infrared absorption spectra recorded at 0.01-0.013 cm⁻¹ resolution with the McMath-Pierce Fourier transform spectrometer located at the National Solar Observatory at Kitt Peak, Arizona. These were retrieved from 42 laboratory spectra obtained at room temperature with five absorption cells having various optical path lengths (from 0.1 to 409 m) filled with natural and enriched samples of CO₂ at pressures ranging from 2 to 581 Torr. In all, band strengths and Herman-Wallis-like F-factor coefficients were determined for 58 vibration-rotation bands from the least-squares fits of over 2100 unblended line strengths; strengths of 34 of these bands had not been previously reported. Band strengths in natural abundance generally ranged from 3.30 × 10⁻²⁰ to 2.8 × 10⁻²⁵ cm⁻¹/molecule cm⁻² at 296 K. It was found that the high J transitions (J′ ? 61) of the 20012 ← 00001 band centered at 4977.8347 cm⁻¹ are perturbed, affecting both measured positions and strengths. Two other interacting bands, 21113e ← 01101e and 40002e ← 01101e, were also analyzed using degenerate perturbation theory. Comparisons with corresponding values from the literature indicate that absolute accuracies better than 1% and precisions of 0.5% were achieved for the strongest bands.     

Line mixing and speed dependence in CO2 at 6227.9 cm: Constrained multispectrum analysis of intensities and line shapes in the 30013 ← 00001 band

Line position, intensity and line shape parameters (Lorentz widths, pressure shifts, line mixing, speed dependence) are reported for transitions of the 30013 ← 00001 band of ¹⁶O¹²C¹⁶O (ν₀ = 6227.9 cm⁻¹). The results are determined from 26 high-resolution, high signal-to-noise ratio spectra recorded at room temperature with the McMath-Pierce Fourier transform spectrometer. To minimize the systematic errors of the retrieved parameters, we constrained the multispectrum nonlinear least squares retrieval technique to use quantum mechanical expressions for the rovibrational energies and intensities rather than retrieving the individual positions and intensities line by line. Self- and air-broadened Lorentz width and pressure-induced shift, speed dependence and line mixing (off-diagonal relaxation matrix elements) coefficients were adjusted individually. Errors were further reduced by simultaneously fitting the interfering absorptions from the weak 30012 ← 00001 band of ¹⁶O¹³C¹⁶O as well as the weak hot bands 31113 ← 01101, 32213 ← 02201, 40014 ← 10002 and 40013 ← 10001 of ¹⁶O¹²C¹⁶O in this spectral window. This study complements our previous work on line mixing and speed dependence in the 30012 ← 00001 band (ν₀ = 6347.8 cm⁻¹) [V.M. Devi, D.C. Benner, L.R. Brown, C.E. Miller, R.A. Toth, J. Mol. Spectrosc. 242 (2007) 90-117] and provides key data needed to improve atmospheric remote sensing of CO₂.     

Infrared spectrum of isotopic carbon dioxide in the region of bending fundamental ν2

Infrared absorption spectra of ¹³C¹⁶O₂, ¹³C¹⁸O₂, ¹⁶O¹³C¹⁷O, ¹⁶O¹³C¹⁸O, and ¹⁶O¹²C¹⁸O have been measured in the wavenumber region 570–780 cm^?1 with a spectral resolution of about 0.005 cm^?1. The data were recorded at room temperature with a Fourier transform spectrometer using a ¹³C-enriched sample of carbon dioxide. The fundamentals ν₂ and several “hot” bands have been identified and effective molecular constants have been derived.     

Infrared spectrum of CO2 in the region of the bending fundamental ν2

The infrared spectrum of CO₂ in the region 540–830 cm^?1 has been studied with a Fourier spectrometer at a resolution of 0.010 cm^?1. In addition to the fundamental ν₂, more than 10 “hot” band transitions of ¹²C¹⁶O₂ have been identified. The rotational constants involved have been derived. Special care has been taken in obtaining accurate constants for the level 01¹0. The ν₂ fundamentals of the isotopic molecules ¹³C¹⁶O₂, ¹⁶O¹²C¹⁸O, and ¹⁶O¹²C¹⁷O have also been observed in a natural sample.     

Air-broadened halfwidth and pressure shift coefficients of CO2 bands: 4750-7000 cm

Previously we obtained self-broadened halfwidth and self-induced shift coefficients at room temperature for 15 near infrared CO₂ bands between 4750 and 7000 cm⁻¹ [R.A. Toth, L.R. Brown, C.E. Miller, V.M. Devi, D.C. Benner, J. Mol. Spectrosc., 239 (2006) 243-271]. The present study expands our work on the near infrared line parameters of CO₂ to include air broadening coefficients. Here we report nearly 400 air-broadened half width and air-induced pressure shift coefficients spanning 11 different CO₂ vibrational bands in the 4750-7000 cm⁻¹ region. Retrievals have been performed using Voigt line profiles over three distinct spectral intervals: (a) 4750-5200 cm⁻¹, covering the 20011 ← 00001, 20012 ← 00001, and 20013 ← 00001 Fermi Triad and three associated hot bands 21111 ← 01101, 21112 ← 01101, 21113 ← 01101; (b) 6100-7000 cm⁻¹, covering the 30011 ← 00001, 30012 ← 00001, 30013 ← 00001 and 30014 ← 00001 Fermi Tetrad; (c) near 6950 cm⁻¹ for the 00031 ← 00001 overtone band. The air-broadened halfwidth and air-induced pressure shift coefficients have been modeled with empirical expressions and compared to other measurements available in the literature.