FT spectroscopy of the Comet-Tail system in 12C17O+: Deperturbation analysis of the A2Πi(v=0) level

IF 1.9 3区 物理与天体物理 Q2 OPTICS
Izabela Piotrowska , Rafał Hakalla , Wojciech Szajna , Ryszard Kȩpa , Stanisław Ryzner , Marzena I. Malicka , Aleksandra Stasik
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引用次数: 0

Abstract

The first recording of the 0v progression (v=0,1,2,3) in the emission spectrum of the Comet-Tail (A2ΠiX2Σ+) system in the 12C17O+ molecule was performed. Using a high-resolution Fourier-transform spectrometer, in the region of 12 880 – 20 500 cm−1 nearly 1900 lines were measured with an accuracy of 0.02 cm−1. As a result of the spectral analysis, 20 molecular parameters of the A(v=0) and X(v=0,1,2,3) levels were determined, including the parameters of the A2Πi(v=0)X2Σ+(v=10) perturbation of a complex, spin–orbit, spin-electronic and rotation-electronic (Luncoupling) nature. In addition, the values of the rovibronic terms of the A2Πi(v=0) level were also determined and the fractional 2Π character of the A2Πi(v=0) and X2Σ+(v=10) levels was examined.

Abstract Image

[公式省略]中彗星-彗尾系统的FT光谱:[公式省略]能级的摄动分析
在Comet-Tail (A2Πi→X2Σ+)系统的发射光谱中首次记录了12C17O+分子的0−v“级数(v”=0,1,2,3)。利用高分辨率傅立叶变换光谱仪,在12 880 ~ 20 500 cm−1范围内测量了近1900条谱线,精度为0.02 cm−1。作为光谱分析的结果,确定了a (v=0)和X(v=0,1,2,3)能级的20个分子参数,包括A2Πi(v=0) ~ X2Σ+(v=10)复合扰动、自旋-轨道、自旋-电子和自旋-电子(L−解耦)性质的参数。此外,还确定了A2Πi(v=0)能级的振动项值,并检验了A2Πi(v=0)和X2Σ+(v=10)能级的分数级2Π特征。
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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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