De Natale P, Lorini L, Inguscio M, Nolt I G, Park J H, Di Lonardo G, Fusina L, Ade P A, Murray A G
Appl Opt. 1997 Nov 20;36(33):8526-32. doi: 10.1364/ao.36.008526.
We report frequency measurements for relatively weak H(2)O and (16)O(3) rotational transitions in the ground state and in the nu(2) = 1 vibrationally excited state. We obtained the frequency measurements by using the laboratory technique of tunable far-infrared spectroscopy with the objective of improving H(2)O and O(3) line parameters required for modeling the important atmospheric spectral window near 119 cm(-1). New sets of molecular constants are calculated from the (16)O(3) data, and improved values are reported for the frequencies of the H(2)O lines. The improvement in atmospheric simulations obtained with the new results is illustrated by comparison with recent high-resolution balloon-based atmospheric measurements. These new data significantly improve simulations of high-resolution atmospheric emission spectra.
我们报告了基态和ν₂ = 1振动激发态下相对较弱的H₂O和¹⁶O₃转动跃迁的频率测量结果。我们采用可调谐远红外光谱的实验室技术获得频率测量结果,目的是改进模拟119 cm⁻¹附近重要大气光谱窗口所需的H₂O和O₃谱线参数。根据¹⁶O₃数据计算了新的分子常数集,并报告了H₂O谱线频率的改进值。通过与最近基于气球的高分辨率大气测量结果进行比较,说明了利用新结果在大气模拟方面取得的改进。这些新数据显著改进了高分辨率大气发射光谱的模拟。