High Temperature Absorption Spectrum of 4.3 Micron CO2†

M. Esplin, H. Sakai
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Abstract

The importance of CO2 as an atmospheric molecule makes the obtaining of high precision band parameters for a great number of bands a significant contribution to both theoretical and experimental studies of our atmosphere. Very accurate parameters on the (00011-00001) band of 12C16O2 have been obtained by Pine and Guelachvili. Their measurment was accomplished by combining two spectra, a room temperature Fourier transform spectrum, and a high temperature tunable laser spectrum.1 There have been numerous measurements of other bands of CO2,2,3 but they were made either with lower resolution spectrometers, or near room temperature where fewer rotational lines were excited, resulting in a less accurate determination of band parameters. In this work a high resolution Michelson interferometer was coupled with a high temperature absorption cell4 heated to 800 K to obtain a high resolution (0.007 cm−1), high temperature spectrum of CO2 in the 4.3 micron region.
4.3微米CO2†的高温吸收光谱
CO2作为大气分子的重要性使得获得大量波段的高精度波段参数对我们大气的理论和实验研究都有重大贡献。Pine和Guelachvili在12C16O2(00011-00001)波段上获得了非常精确的参数。他们的测量是通过结合两个光谱来完成的,一个是室温傅里叶变换光谱,一个是高温可调激光光谱对CO2,2,3的其他波段进行了大量测量,但它们要么是用较低分辨率的光谱仪进行的,要么是在接近室温的地方进行的,在那里激发的旋转谱线较少,导致波段参数的测定不太准确。在这项工作中,高分辨率迈克尔逊干涉仪与加热到800 K的高温吸收池4耦合,在4.3微米区域获得了高分辨率(0.007 cm−1)的CO2高温光谱。
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