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氧分子(O₂)赫茨伯格谱带的傅里叶变换光谱学。III. 碰撞诱导谱带和赫茨伯格连续谱的吸收截面。

Fourier Transform Spectroscopy of the O(2) Herzberg Bands. III. Absorption Cross Sections of the Collision-Induced Bands and of the Herzberg Continuum.

作者信息

Fally S, Vandaele AC, Carleer M, Hermans C, Jenouvrier A, Mérienne M, Coquart B, Colin R

机构信息

Laboratoire de Chimie Physique Moléculaire, CP160/09, Université Libre de Bruxelles, 50 Av. F. D. Roosevelt, Brussels, B-1050, Belgium

出版信息

J Mol Spectrosc. 2000 Nov;204(1):10-20. doi: 10.1006/jmsp.2000.8204.

DOI:10.1006/jmsp.2000.8204
PMID:11034837
Abstract

Absorption spectra of molecular oxygen were measured in the laboratory under temperature and pressure conditions prevailing in the Earth's atmosphere. Spectra of pure O(2), O(2) + N(2), and O(2) + Ar were recorded in the 41 700 to 33 000 cm(-1) region (240-300 nm) at a maximal optical path difference of 0.45 cm using a Fourier transform spectrometer and a multiple reflection gas cell. The different components of the spectra, namely the discrete bands of the three Herzberg systems, the Herzberg continuum, and the collision-induced diffuse Wulf bands, were separated. The contribution of the Herzberg bands was first subtracted using the line parameters determined previously [A. Jenouvrier, M.-F. Mérienne, B. Coquart, M. Carleer, S. Fally, A. C. Vandaele, C. Hermans, and R. Colin, J. Mol. Spectrosc. 198, 136-162 (1999)] from high-resolution data. Spectra recorded at various pressures then made it possible to determine by linear regression the intensity of the Wulf bands and the Herzberg continuum. The characteristics of the Wulf bands have been investigated in details: vibrational analysis, pressure effect, foreign gas effect, and a simulated spectrum are reported. The Herzberg continuum cross section is determined below the dissociation limit. A comparison with literature data is given. The new O(2) absorption cross sections and O(2)-O(2) collision-induced absorption cross sections are useful in connection with atmospheric measurements of ozone and other trace gases in the UV spectral region. Copyright 2000 Academic Press.

摘要

在实验室中,在地球大气中普遍存在的温度和压力条件下测量了分子氧的吸收光谱。使用傅里叶变换光谱仪和多反射气室,在41700至33000cm⁻¹区域(240 - 300nm)记录了纯O₂、O₂ + N₂和O₂ + Ar的光谱,最大光程差为0.45cm。光谱的不同成分,即三个赫兹伯格体系的离散带、赫兹伯格连续谱和碰撞诱导的弥散伍尔夫带,被分离出来。首先使用先前从高分辨率数据中确定的谱线参数[A. 热努维耶、M.-F. 梅里安、B. 科夸尔、M. 卡勒尔、S. 法利、A.C. 万代勒、C. 赫尔曼斯和R. 科林,《分子光谱学杂志》198, 136 - 162 (1999)]减去赫兹伯格带的贡献。然后,在不同压力下记录的光谱使得通过线性回归确定伍尔夫带和赫兹伯格连续谱的强度成为可能。对伍尔夫带的特性进行了详细研究:报告了振动分析、压力效应、外来气体效应和模拟光谱。确定了低于解离极限的赫兹伯格连续谱截面。并与文献数据进行了比较。新的O₂吸收截面和O₂ - O₂碰撞诱导吸收截面对于紫外光谱区域中臭氧和其他痕量气体的大气测量很有用。版权所有2000年,学术出版社。

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