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CO+分子离子彗尾带系在近红外区域的光谱研究
引用本文:李伟,杨晓华,甘雨洁,吴玲,郭迎春,刘煜炎,陈扬骎. CO+分子离子彗尾带系在近红外区域的光谱研究[J]. 光谱学与光谱分析, 2005, 25(8): 1250-1252
作者姓名:李伟  杨晓华  甘雨洁  吴玲  郭迎春  刘煜炎  陈扬骎
作者单位:华东师范大学物理系,光谱学与波谱学教育部重点实验室,上海,200062;波谱与原子分子物理国家重点实验室,中国科学院武汉物理与数学研究所,湖北,武汉,430071
基金项目:国家自然科学基金(10174020和10204007)和上海市重点学科资助项目
摘    要:
CO 分子离子是一种重要的瞬态自由基分子,许多研究者对该带系进行了大量的研究。文章采用光外差-磁旋转-速度调制光谱技术测量了12C16O 分子离子彗尾带系(A2Πi-X2Σ )在近红外区域的3个支带(0,3),(1,4)和(3,6)的振转吸收光谱。利用最小二乘法拟合,得到了上态A2Πi(ν′=0,1,3)的精确的分子常数。进一步验证了光外差-磁旋转-速度调制光谱技术在吸收光谱测量中的优越性。

关 键 词:CO+离子  彗尾带系  近红外  分子常数
文章编号:1000-0593(2005)08-1250-03
收稿时间:2004-03-16
修稿时间:2004-07-31

Study on the Comet-Tail System of 12C16O+ in the Near-Infrared Region
LI Wei,YANG Xiao-hua,GAN Yu-jie,WU Ling,GUO Ying-chun,LIU Yu-yan,CHEN Yang-qin. Study on the Comet-Tail System of 12C16O+ in the Near-Infrared Region[J]. Spectroscopy and Spectral Analysis, 2005, 25(8): 1250-1252
Authors:LI Wei  YANG Xiao-hua  GAN Yu-jie  WU Ling  GUO Ying-chun  LIU Yu-yan  CHEN Yang-qin
Affiliation:Key Laboratory of Optical and Magnetic Resonance Spectroscopy, Department of Physics, East China Normal University, Shanghai 200062, China
Abstract:
The molecular cation CO+ is a very important transient molecular radical, and the spectra of the ion has been investigated by numerous researchers. Optical-heterodyne-magnetic-rotation-enhanced velocity modulation spectroscopy(OH-MR-VMS) was employed to measure the comet-tail system (A2 pi(i)-X2 sigma+) of 12C16O+ molecular ion. The vibrationalrotation absorption spectra wereobserved in the near-infrared region, including three bands of (0, 3), (1, 4) and (3, 6). A set of precise molecular constants for the A2 pi(i) (v' = 0, 1, 3) were determined using the least-squares fit. This experiment has further proved that OH-MR-VMS is very valuable in measuring absorption spectra of molecular ions.
Keywords:CO ion  Comet-tail system  Near-infrared  Molecular constants
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