Goldman A, Kyle T G, Murcray D G, Murcray F H, Williams W J
Appl Opt. 1970 Mar 1;9(3):565-80. doi: 10.1364/AO.9.000565.
A balloon-borne spectrometer was used to measure the atmospheric absorption of solar radiation in the 9-10-micro region as a function of altitude. Among the numerous spectra recorded, several were made with very long optical paths above the troposphere obtained from floating altitude (~30 km) while the sun set. When the experimental results are compared with calculated spectra, based on line by line parameters of the nu(3) and nu(1) fundamentals of ordinary ozone, (16)O(3), combined with the Curtis-Godson approximation, large discrepancies are found for the long path spectra. It is shown that the hot bands nu(3), + nu(2), - nu(2), and nu(3), + nu(3), - nu(3), of the (16)O(3), and the nu(3) fundamentals of the isotopic species (16)O(18)O(16)O and (16)O(16)O(18)O, can contribute significant absorption for long paths such as obtained in this experiment. Such long paths also give rise to significant absorptions by the nu(3) - nu(1) and the nu(3) - 2nu(2) degrees bands of CO(2). Including these weak bands in the calculated spectra leads to good agreement with the observed data.
一台气球携带光谱仪被用于测量9 - 10微米区域太阳辐射的大气吸收随高度的变化。在记录的众多光谱中,有几条是在日落时从浮空高度(约30千米)获得的对流层上方很长光程情况下测得的。当将实验结果与基于普通臭氧(¹⁶O₃)的ν(3)和ν(1)基频的逐线参数并结合柯蒂斯 - 戈德森近似计算出的光谱进行比较时,发现长光程光谱存在很大差异。结果表明,¹⁶O₃的热谱带ν(3) + ν(2) - ν(2)和ν(3) + ν(3) - ν(3),以及同位素物种¹⁶O¹⁸O¹⁶O和¹⁶O¹⁶O¹⁸O的ν(3)基频,对于本实验中获得的长光程可产生显著吸收。这样的长光程还会导致CO₂的ν(3) - ν(1)和ν(3) - 2ν(2)泛频带产生显著吸收。在计算光谱中包含这些弱谱带可使计算结果与观测数据达成良好吻合。