(3-0)泛音带自展宽CO跃迁的线形参数

IF 2.3 3区 物理与天体物理 Q2 OPTICS
Q. Huang , J. Wang , J.-K. Li , Z.-L. Nie , A.-W. Liu , Y. Tan , S.-M. Hu
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引用次数: 0

摘要

本研究采用激光锁腔衰荡光谱研究了近红外中15个弱12C16O跃迁,对应于(3-0)波段的P和R分支,旋转量子数J在25 ~ 35之间。大多数光谱记录在低压(1333 Pa以下),其中多普勒展宽占主导地位,碰撞展宽主要由速度依赖的相互作用驱动。这种环境可以精确地确定碰撞线的形状参数。利用pad近似和多项式拟合来估计速度相关的Voigt (SDV)展宽参数,将数据扩展到更高的旋转量子数。得到了CO的精确自展宽参数,这对研究其他大气气体的压力展宽具有重要意义。这些结果将支持该光谱区域地球大气的高精度辐射传输模型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Line shape parameters of self-broadened CO transitions in the (3-0) overtone band
This study employs laser-locked cavity ring-down spectroscopy to investigate 15 weak 12C16O transitions in the near-infrared, corresponding to the P and R branches of the (3-0) band with rotational quantum numbers J ranging from 25 to 35. Most spectra were recorded at low pressures (below 1333 Pa), where Doppler broadening dominates, and collision broadening is mainly driven by speed-dependent interactions. This environment enables precise determination of collisional line shape parameters. The Padé approximation and polynomial fit were used to estimate speed-dependent Voigt (SDV) broadening parameters, extending the data to higher rotational quantum numbers. Accurate self-broadening parameters for CO were obtained, which are essential for studying pressure broadening by other atmospheric gases. These results will support high-precision radiative transfer models for Earth’s atmosphere in this spectral region.
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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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