在2300 nm范围内,大气压增宽的CH4吸收谱线参数

IF 0.9 Q4 OPTICS
T. M. Petrova, A. M. Solodov, A. A. Solodov, V. M. Deichuli, T. Yu. Chesnokova
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引用次数: 0

摘要

甲烷是主要的温室气体之一,其浓度近几十年来一直在增加,从而提高了地球表面的温度。为了监测大气中甲烷的含量,需要准确了解甲烷分子的吸收光谱。在4345-4360 cm−1的光谱区域,甲烷吸收谱线的参数被大气压力展宽。数据来源于布鲁克IFS 125HR傅立叶光谱仪记录的光谱,光谱分辨率为0.005-0.01 cm−1,室温下,缓冲气体压力为5个值。利用HITRAN和GEISA光谱数据库的导出结果和谱线参数对大气传输进行了模拟。与实测大气太阳光谱的比较表明,本研究所得的CH4吸收谱线参数在均方根偏差方面吻合最好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Parameters of CH4 Absorption Lines Broadened by Atmospheric Air Pressure in the 2300 nm Region

Parameters of CH4 Absorption Lines Broadened by Atmospheric Air Pressure in the 2300 nm Region

Methane is one of key greenhouse gases, whose concentration has been increasing in recent decades, thus increasing the Earth’s surface temperature. To monitor the methane content in the atmosphere the accurate knowledge of the absorption spectrum of CH4 molecule is required. In this work, the parameters of methane absorption lines broadened by atmospheric air pressure are presented in the spectral region 4345–4360 cm−1. Data were derived from spectra recorded at a Bruker IFS 125HR Fourier spectrometer with a spectral resolution of 0.005–0.01 cm−1 at room temperature and five values of buffer gas pressure. Atmospheric transmission was simulated using the derived results and line parameters from HITRAN and GEISA spectroscopic databases. The comparison with measured atmospheric solar spectra shows the CH4 absorption line parameters found in this work to coincide the best in terms of root-mean-square deviation.

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来源期刊
CiteScore
2.40
自引率
42.90%
发文量
84
期刊介绍: Atmospheric and Oceanic Optics  is an international peer reviewed journal that presents experimental and theoretical articles relevant to a wide range of problems of atmospheric and oceanic optics, ecology, and climate. The journal coverage includes: scattering and transfer of optical waves, spectroscopy of atmospheric gases, turbulent and nonlinear optical phenomena, adaptive optics, remote (ground-based, airborne, and spaceborne) sensing of the atmosphere and the surface, methods for solving of inverse problems, new equipment for optical investigations, development of computer programs and databases for optical studies. Thematic issues are devoted to the studies of atmospheric ozone, adaptive, nonlinear, and coherent optics, regional climate and environmental monitoring, and other subjects.
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