Spectrum of 13 CO 2 at 3420-3680 cm−1 (2.8 μm)

C. Rinsland, A. Baldacci, M. Smith, K. Rao
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Abstract

The 2.8 μm region is useful for the sounding of atmosphere pressure since it contains a number of weak and strong CO2 lines allowing a range of altitudes be sensed (1). This region has been selected for the measurement of pressure in the Halogen Occultation Experiment (HALOE, 2). To aid in the identification of spectral lines within this bandpass, we have recorded the absorption spectrum of 13CO2 in the laboratory. The data were obtained in the spectral interval 3420 to 3680 cm−1 with a vacuum grating spectrometer equipped with a 40 cm × 20 cm Harrison-ruled echelle and a 13C-enriched sample of carbon dioxide. The spectra were recorded both at room temperature and at 160°C. In the high temperature data, it was possible to observe transitions from high rotational levels and moderately high vibrational states. Measurements in this single spectral region provided information on 29 vibrational levels, 4 of which have been studied for the first time. Twenty-one bands have been identified, and about 80 percent of the 2000 lines recorded have been given assignments. The spectral resolution was about 0.03 cm−1.
13co2在3420 ~ 3680 cm−1 (2.8 μm)处的光谱
2.8 μm区域对于大气压力的探测是有用的,因为它包含许多弱和强CO2线,允许在一定高度范围内被探测(1)。在卤素掩星实验(HALOE, 2)中,该区域被选择用于测量压力。为了帮助识别该带通内的光谱线,我们在实验室中记录了13CO2的吸收光谱。数据在3420 ~ 3680 cm−1的光谱区间用40cm × 20cm哈里森直尺梯级的真空光栅光谱仪和富含13c的二氧化碳样品获得。在室温和160℃下分别记录了光谱。在高温数据中,可以观察到高旋转水平和中高振动状态的转变。在这一单一光谱区域的测量提供了29个振动水平的信息,其中4个是首次研究。21个谱带已被识别,2000个谱线中约80%已被分配。光谱分辨率约为0.03 cm−1。
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