渐近非对称陀螺分子H122C16O的高温光谱

在直接计算分子配分函数的基础上,将无转动跃迁偶极矩平方近似为一常数,计算了渐近非对称陀螺分子H122C16O 100000-000000跃迁在中等温度和高温下的线强度.计算结果在500K时与HITRAN数据库的结果吻合相当好.在温度高达3000K时与HITRAN数据库的结果仍符合较好,表明分子配分函数和线强度的高温计算是可靠的.在此基础上,进一步计算了渐近非对称陀螺分子H122C16O 100000-000000跃迁带在极端高温4000和5000K的线强度并报道其模拟光谱.计算结果对大气分子高温光谱的实验测量和理论研究均有一定的参考价值.     

对称陀螺分子NH3的高温谱线强度研究

在直接计算分子配分函数的基础上,将无转动跃迁偶极矩平方近似为一常数,计算了对称陀螺分子NH₃ 0300 a—0000 s跃迁在高温下的线强度.在296K,计算的分子总配分函数与HITRAN数据库的结果符合很好,只有0.19%的百分误差.计算的跃迁线强度在2000 K和3000K的高温与HITRAN数据库的结果也符合相当好,最大百分误差分别为-0.65%和-1.77%.这就表明分子配分函数和线强度的高温计算是可靠的.在此基础上,计算被扩展到更高温度,报道了对称陀螺分子NH_{3< 关键词： 高温光谱 对称陀螺分子 配分函数 氨}     

臭氧分子同位素16O18O16O的高温光谱研究

在直接计算分子配分函数的基础上,将无转动跃迁偶极矩平方近似为一常数,计算了非对称陀螺臭氧分子同位素16O18O16O 001-000跃迁在中等温度和高温下的线强度.计算结果在1000 K时与HITRAN数据库的结果吻合相当好.在温度高达3000 K时与HITRAN数据库的结果仍符合较好(最大百分误差为5.48%),表明分子配分函数和线强度的高温计算是可靠的.在此基础上,进一步计算了非对称陀螺分子16O18O16O 001-000跃迁带在极端高温4000和5000 K的线强度并报道其模拟光谱.计算结果对大气分子高温光谱的实验测量和理论研究均有一定的参考价值.     

对称陀螺分子NH3的高温谱线强度研究

在直接计算分子配分函数的基础上,将无转动跃迁偶极矩平方近似为一常数,计算了对称陀螺分子NH3,0300a-0000 s跃迁在高温下的线强度.在296 K,计算的分子总配分函数与HITRAN数据库的结果符合很好,只有O.19%的百分误差.计算的跃迁线强度在2000 K和3000 K的高温与HITRAN数据库的结果也符合相当好,最大百分误差分别为-0.65%和-1.77%.这就表明分子配分函数和线强度的高温计算是可靠的.在此基础上,计算被扩展到更高温度,报道了对称陀螺分子NH30300 a-0000 s跃迁在极端高温4000和5000 K的模拟光谱.计算结果对大气分子高温光谱的实验测量和理论研究均有一定的参考价值.     

对称陀螺分子PH30010-0000跃迁带的高温线强度计算

通过直接计算分子配分函数并将常温下的无转动跃迁偶极矩平方近似为一常数应用到高温，计算了对称陀螺分子PH3 0010-0000跃迁的高温线强度。在296K，计算的分子总配分函数与HITRAN数据库的结果符合很好，只有-0.075%的百分误差。计算的跃迁线强度在2000 K和3000 K的高温与HITRAN数据库的结果也吻合较好，表明分子配分函数和线强度的高温计算是可靠的。在此基础上，进一步计算了更高温度4000和5000 K的跃迁线强度，报道了对称陀螺分子PH3 0010-0000跃迁在极端高温4000和5000 K的模拟光谱。计算结果对大气分子高温光谱的实验测量和理论研究均有一定的参考价值。     

对称陀螺分子PH30010-0000跃迁带的高温线强度计算

通过直接计算分子配分函数并将常温下的无转动跃迁偶极矩平方近似为一常数应用到高温,计算了对称陀螺分子PH3 0010-0000跃迁的高温线强度。在296K,计算的分子总配分函数与HITRAN数据库的结果符合很好,只有-0.075%的百分误差。计算的跃迁线强度在2000 K和3000 K的高温与HITRAN数据库的结果也吻合较好,表明分子配分函数和线强度的高温计算是可靠的。在此基础上,进一步计算了更高温度4000和5000 K的跃迁线强度,报道了对称陀螺分子PH3 0010-0000跃迁在极端高温4000和5000 K的模拟光谱。计算结果对大气分子高温光谱的实验测量和理论研究均有一定的参考价值。     

二氧化碳非对称同位素16O12C17O 00011～00001跃迁带的高温谱线强度

利用本文计算所得配分函数和实验振动跃迁矩平方及Herman-Wallis因子系数,我们计算了二氧化碳同位素16O12C17O分子00011～00001跃迁在296 K和3000 K的线强度.结果显示,在296 K和3000 K时,计算所得线强度与HITRAN数据库提供的数据均符合较好.表明高温下的分子配分函数和线强度的计算是可靠的.从而进一步计算了二氧化碳同位素16O12C17O的000011～00001跃迁在4000 K和5000 K高温下的线强度及模拟光谱.     

氧化亚氮3000—0200和1001—0110跃迁带在高温下的线强度

采用乘积近似法计算了氧化亚氮分子的总配分函数，其中转动配分函数考虑了离心扭曲修正，振动配分函数采用谐振子近似. 利用计算所得的配分函数和实验振动跃迁矩平方及Herman-Wallis因子系数，计算了氧化亚氮3000—0200和1001—0110跃迁带在常温和高温下的线强度. 结果显示，当温度高达3000K时，计算所得线强度与实验值及HITRAN数据库提供的结果仍符合较好. 这表明高温下的分子配分函数和线强度的计算是可靠的. 还进一步计算了氧化亚氮3000—0200和1001—0110跃迁带在更高温度(40 关键词： 氧化亚氮 配分函数 线强度 高温     

烟道气体SO2光谱辐射强度和吸收系数的研究

采用乘积近似法构建配分函数合理模型,计算了SO₂分子的总配分函数.利用所得的配分函数、将常温下的无转动跃迁矩平方近似为一常数并应用于高温及Herman-Wallis因子系数,编制光谱程序,计算了烟道气体SO₂分子三个主要跃迁带100-000、001-000和101-000不同温度段的光谱强度和吸收系数.结果表明,计算所得的配分函数和谱线强度与数据库相比,不管是常温296 K还是高温3000 K,都吻合较好,相对偏差都在3%以下,这说明构建的配分函数模型和编制的程序是可靠的,在此基础上,进一步计算了各跃迁带在不同温度的吸收系数.从模拟光谱图可看出,强度随着温度升高明显减小,谱带带心没变,峰值波数向两边偏移;吸收系数随着温度升高也减少,其中在3000 K以下吸收峰位置增宽,到高达4000 K以上基本不再变换,这为监测烟道气体环境污染提供实验和理论参考.     

H12C14N分子v2垂直带的高温谱线强度及随温度的变化规律

采用乘积近似法计算了氰化氢分子H12C14N的总配分函数,其中转动配分函数考虑了离心扭曲修正,振动配分函数采用谐振子近似.利用计算所得配分函数和文献提供的实验振动跃迁矩平方及HermanWallis因子系数,计算了氰化氢分子H12C14Nv2垂直带,即0110-0000跃迁在常温和高温下的线强度,并与HITRAN数据库的数据进行了比较.结果显示,在296 K及温度高达3 000 K时,计算所得谱线强度与HI-TRAN数据库提供的结果均符合较好.表明对氰化氢分子H12C14N高温下的分子配分函数和线强度的计算是可靠的.进一步计算了0110-0000跃迁带在更高温度4 000和5 000 K的线强度及模拟光谱,并总结了该跃迁带中的谱线强度随温度的变化规律:对于转动量子数J≥32的跃迁谱线(包括P支、Q支和R支),当温度从296.K逐渐增加时,其线强度迅速增加,到1 000 K附近达到最大值,然后迅速减弱.对于转动量子数J<32的跃迁谱线(同样包括P支、Q支和R支),线强度在296 K时最大,然后随温度的升高迅速减弱.     

Study on High-Temperature Spectra of Asymptotic Asymmetric-Top Molecule O3

The line intensities of 001-000 transition of the asymptotic asymmetric-top O₃ molecule at several temperatures are calculated by directly calculating the partition functions and regarding the rotationless transition dipole moment squared as a constant. The calculated values of the total internal partition sums (TIPS) are consistent with the data of HITRAN database with -0.61% at 296 K. The calculated line intensity data at 500 K and 3000 K are also in excellent agreement with the data in HITRAN database with less than 0.659% and 5.458% at 500 K and 3000 K, which provide a strong support for the calculations of partition function and line intensity at high temperature. Then we extend the calculation to higher temperatures. The line intensities and simulated spectra of ν₃ band of the asymptotic asymmetric-top O₃ molecule at 4000 and 5000 K are reported. The results are of significance for the studying of the molecular high-temperature spectrum including experimental measurements and theoretical calculations.     

Temperature dependence of the absorption spectrum of CH4 by high resolution spectroscopy at 81 K: (I) The region of the 2ν3 band at 1.66 μm

In a recent contribution, (Gao B, Kassi S, Campargue A. Empirical low energy values for methane transitions in the 5852-6181 cm⁻¹ region by absorption spectroscopy at 81 K. J Mol Spectrosc 2009;253:55-63.), the low energy values of methane transitions between 1.71 and 1.62 μm were derived from the variation of the line intensities between 296 and 81 K. The line intensities at 81 K were retrieved from the high resolution absorption spectrum of methane recorded at liquid nitrogen temperature by direct absorption spectroscopy using a cryogenic cell and a series of distributed feed back (DFB) diode lasers. For the line intensities at 296 K, the values provided by the HITRAN database were used. As a consequence of the relatively high intensity cut off (4×10⁻²⁴ cm/molecule) of the HITRAN line list in the considered region, the lower energy values were derived for only 845 of the 2187 transitions measured at 81 K. In the present work, our line list was extended by the retrieval of many weak line intensities leading to a set of 3251 transitions. The minimum value of the measured line intensities (at 81 K) is on the order of 10⁻²⁶ cm/molecule. In relation with the project “Greenhouse Gases Observing Satellite” (GOSAT), a much more complete line list for CH₄ at 296 K has become available (intensity cut off of 4×10⁻²⁶ cm/molecule). By applying the two temperature method to our line intensities at 81 K and GOSAT intensities at 296 K, the lower energy values of 2297 transitions could be derived. These transitions represent 99.1% and 90.8% of the total absorbance in the region, at 81 and 296 K respectively. This line list provided as Supplementary Material allows then accounting for the temperature dependence of CH₄ absorption below 300 K. The investigated spectral range is dominated by the 2ν₃ band near 6005 cm⁻¹ which is of particular interest for atmospheric retrievals. The factor 2 narrowing of the Doppler linewidth from room temperature down to 81 K has allowed the resolution of a number of 2ν₃ multiplets and improving the line intensity retrievals. A detailed comparison with GOSAT and HITRAN line lists has revealed a number of possible improvements.     

Collisional broadening and line intensities in the ν2 and ν4 bands of PH3

Using a tunable diode-laser spectrometer self-broadening coefficients and absolute intensities have been measured for 26 lines of PH₃ at 298 K in the QR branch of the ν₂ band and the PP and RP branches of the ν₄ band. The recorded lines with J values ranging from 2 to 14 and K from 0 to 11 are located in the spectral range 995-1093 cm⁻¹. Self-broadening coefficients have also been measured at 173.4 K for nine of these lines. The collisional widths and line strengths are obtained by fitting each spectral line with different theoretical profiles. The results obtained for the line intensities are in good agreement with recent measurements [J. Mol. Spectrosc. 215 (2002) 178]. The self-broadening coefficients are also calculated on the basis of a simple semiclassical model involving only the electrostatic interactions. A satisfactory agreement is obtained except for high J values or K values equal to J, for which the calculated results are notably underestimated. By comparing broadening coefficients at room and low temperatures, the temperature dependence of these broadenings has been determined both experimentally and theoretically.     

Calculation of absorption coefficient for the ν2 and ν3 bands of sulfur dioxide

Absorption coefficients S/d of sulfur dioxide were calculated in the ν₂ and ν₃ bands for a temperature range from 300 to 1200°K. Calculations were carried out for such vibrational transitions that their integrated absorption coefficients α at T°K are greater than 0.1% of the total integrated absorption coefficients α^obs observed at 300°K. Rotational lines with intensities greater than 10^-6 cm^-2 atm^-1 STP were included in the calculation. The line intensities were averaged over small wavenumber intervals of Δω = 10 cm^-1 throughout the bands to obtain the absorption coefficients S/d. They were compared with the experimental values of other investigators and good agreement was obtained.     

New infrared integrated band intensities for HC3N and extensive line list for the ν5 and ν6 bending modes

The infrared spectrum of cyanoacetylene (also called propynenitrile) has been investigated from 400 to 4000 cm⁻¹ at a resolution of 0.5 cm⁻¹. Integrated intensities of the main bands and a number of weaker bands have been obtained with an uncertainty better than 5%. Inaccurate values in previous studies have been identified in particular concerning the intensity of the strong ν₅ stretching band at 663.2 cm⁻¹. Former results on the temperature dependence of integrated intensities have also been revisited.Synthetic spectra calculation has been performed for the ν₅ and ν₆ bands on the basis of the best available high resolution data. It has been shown that the GEISA line parameters for HC₃N are not sufficient to reproduce the band intensities and some hot band features observed in our experimental spectra at room temperature. As a first step, the model spectra has been improved by including a number of missing hot subbands and by calculating accurately the hot band relative intensities. Finally, a perfect agreement between calculated and observed spectra was achieved on the basis of a global analysis of HC₃N levels up to 2000 cm⁻¹ combined with the new integrated intensity measurements. A new extensive line list for the ν₅ and ν₆ bending modes of HC₃N has been compiled.     

Study on high-temperature spectra of asymptotic asymmetric-top radical SiO2

Total internal partition sums are calculated in the product approximation at temperatures up to 6000 K for the asymptotic asymmetric-top SiO2 molecule.The rotational partition function and the vibrational partition function are calculated with the rigid-top model and in the harmonic oscillator approximation,respectively.Our values of the total internal partition sums are consistent with the calculated value in the Gaussian program within 0.137% at 296 K.Using the calculated partition functions and the rotationless transition dipole moment squared as a constant,we calculate the line intensities of 001-000 band of SiO2 at normal,medium and high temperatures.Simulated spectra of the 001-000 band of the asymptotic asymmetric-top SiO2 molecule at 2000,5000 and 6000 K are also obtained.