IF 0.3 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR
A. M. Molchanov, D. S. Yanyshev, L. V. Bykov, A. S. Kovalenko
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引用次数: 0

摘要

提出了一种计算 3200 至 5400 cm-1 范围内二氧化碳吸收和发射特性的方法,并考虑了热不平衡的影响。在不同的压力、光谱区域、层厚度、温度和二氧化碳摩尔分数条件下,使用逐行(LBL)和统计窄带(SNB)模型进行了一系列计算。所开发的方法显示 LBL 模型和 SNB 模型之间具有良好的一致性,在计算传输容量时与实验数据的一致性也令人满意。在所考虑的范围内,非平衡旋转温度对辐射特性几乎没有影响,这与平移和振动温度不同,后者对非平衡普朗克函数有显著影响。由此得出的方法可用于研究全球变暖问题时的计算。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Calculation of the Emission Characteristics of Thermally Nonequilibrium CO2 Gas in the Range of 3200–5400 cm–1 Using the Line-by-Line and Statistical Narrow-Band Models

Calculation of the Emission Characteristics of Thermally Nonequilibrium CO2 Gas in the Range of 3200–5400 cm–1 Using the Line-by-Line and Statistical Narrow-Band Models

A method for calculating the absorption and emission characteristics of CO2 in the range from 3200 to 5400 cm–1 with allowance for the effect of thermal nonequilibrium has been presented. A series of calculations using line-by-line (LBL) and statistical narrow-band (SNB) models has been performed at various pressures, spectral regions, layer thicknesses, temperatures, and molar fractions of CO2. The developed method shows good agreement between the LBL and SNB models and satisfactorily agrees with experimental data when calculating the transmission capacity. In the considered range, the nonequilibrium in rotational temperature has virtually no effect on the radiative characteristics, unlike translational and vibrational temperatures, which have a significant effect on the nonequilibrium Planck function. The resulting methodology can be used for calculations when studying the problem of global warming.

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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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