New quantum assignments and analysis of high-resolution H212CO spectra in the range 3700–4450 cm-1

IF 2.3 3区 物理与天体物理 Q2 OPTICS
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引用次数: 0

Abstract

Four spectra of formaldehyde in natural isotopic abundance in the 3700–5200 cm-1 region were recorded at low temperature 160–166 K at Synchrotron SOLEIL for various pressures. Line positions and intensities were retrieved by non-linear least-squares curve-fitting procedures in the range 3700–4450 cm-1 and analyzed using ab initio based effective Hamiltonian and line intensities computed using new ab initio dipole moment surface. A new measured line list contains positions and intensities for 6177 features. Refined parameters of effective Hamiltonian were fitted to all assigned line positions with the RMS deviations of 0.001 cm-1. Updated line lists include intensity values based on ab initio variational calculations which were subsequently empirically optimized. Comparison of our theoretical simulation with previously available data as well as with high-resolution and low-resolution experimental spectra are reported.

3700-4450 cm-1 范围内高分辨率 H212CO 光谱的新量子赋值和分析
在同步加速器 SOLEIL 的 160-166 K 低温条件下,记录了不同压力下 3700-5200 cm-1 区域自然同位素丰度的四条甲醛光谱。在 3700-4450 cm-1 范围内,通过非线性最小二乘曲线拟合程序检索了线的位置和强度,并使用基于非初始有效哈密顿的方法进行了分析,还使用新的非初始偶极矩表面计算了线的强度。新的测量线列表包含 6177 个特征的位置和强度。经过改进的有效哈密顿参数被拟合到所有指定的谱线位置,均方根偏差为 0.001 厘米-1。更新后的谱线列表包含了基于非初始变分计算的强度值,这些强度值随后根据经验进行了优化。报告了我们的理论模拟与先前可用数据以及高分辨率和低分辨率实验光谱的比较。
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来源期刊
CiteScore
5.30
自引率
21.70%
发文量
273
审稿时长
58 days
期刊介绍: Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer: - Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas. - Spectral lineshape studies including models and computational algorithms. - Atmospheric spectroscopy. - Theoretical and experimental aspects of light scattering. - Application of light scattering in particle characterization and remote sensing. - Application of light scattering in biological sciences and medicine. - Radiative transfer in absorbing, emitting, and scattering media. - Radiative transfer in stochastic media.
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