2014
DOI: 10.1016/j.jqsrt.2014.01.019
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Efficient representation of the absorption line blackbody distribution function for H2O, CO2, and CO at variable temperature, mole fraction, and total pressure

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Cited by 99 publications
(58 citation statements)
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“…The line width γ i depends on temperature T, the total pressure P, and the partial pressure of the radiating species P s as [25,26] γ i ðT; P; P s Þ ¼…”
Section: Line-by-line (Lbl) Modelmentioning
confidence: 99%
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“…The line width γ i depends on temperature T, the total pressure P, and the partial pressure of the radiating species P s as [25,26] γ i ðT; P; P s Þ ¼…”
Section: Line-by-line (Lbl) Modelmentioning
confidence: 99%
“…The only few relevant studies are perhaps those of Denison and Webb [22], Badinand and Fransson [23], Pal and Modest [24], and Pearson et al [25,26]. Denison and Webb [22] made the first attempt to study the effects of total pressure on the absorption-line blackbody distribution function (ALBDF).…”
Section: Introductionmentioning
confidence: 99%
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“…Generally, the values of k T, i φ ( ) and a T T , i 0 ( ) are obtained from the absorption distribution function (ADF) [20][21][22][23]. Thus, the weight function a T T ,…”
Section: Spectral-line-based Weighted-sum-of-gray-gasesmentioning
confidence: 99%
“…This has prompted the development of simple correlation formulas for individual species at atmospheric pressure [15][16][17][18][19][20], from which kdistributions can be efficiently obtained; however, their accuracy are rarely satisfactory and sometimes may lead to serious errors [14]. Recently, Pearson et al [21,22] use absorption cross-sections instead of absorption coefficients) for CO 2 , H 2 O and CO over the full spectrum as a tool used in the SLW method, providing an alternative to solve the radiative property of nongray gas with excellent accuracy. However, this tabulation does not include gas mixtures and is relatively coarse, making it difficult to use for mixtures.…”
Section: Introductionmentioning
confidence: 99%