2005
DOI: 10.1016/j.proci.2004.08.078
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A technique for extrapolating absorption coefficient measurements to high temperatures

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Cited by 21 publications
(16 citation statements)
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“…The averaged temperatures and species concentrations were used for calculating the spectrally resolved absorption coefficient needed in the radiative transport equation which was integrated from the flame location back to the pool surface. For these calculations, a semi-empirical correlation based on a three-parameter fit [25] of the quantum molecular line intensity equation for each wavenumber provided a means for calculating each j m as a function of T. Figure 5 shows that H 2 O and CO 2 are the principle emitting species near and outside of the actual flame. The methanol mole fraction only becomes significant below a height of 0.3 m (or 0.26 m above the liquid surface).…”
Section: Resultsmentioning
confidence: 99%
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“…The averaged temperatures and species concentrations were used for calculating the spectrally resolved absorption coefficient needed in the radiative transport equation which was integrated from the flame location back to the pool surface. For these calculations, a semi-empirical correlation based on a three-parameter fit [25] of the quantum molecular line intensity equation for each wavenumber provided a means for calculating each j m as a function of T. Figure 5 shows that H 2 O and CO 2 are the principle emitting species near and outside of the actual flame. The methanol mole fraction only becomes significant below a height of 0.3 m (or 0.26 m above the liquid surface).…”
Section: Resultsmentioning
confidence: 99%
“…For the high temperature measurements, the ZnSe windows were externally cooled to maintain high spectral transmissivity. Further details of the setup are provided elsewhere [25,26].…”
Section: Approachmentioning
confidence: 99%
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“…Using the semi-quantitative technique developed in Ref. [36] where the experimental absorption coefficient is adjusted with empirical parameters, the database has been extended to 1400 K and interpolated in 50 K increments. A sample of this database is provided in Fig.…”
Section: Spectral Featuresmentioning
confidence: 99%
“…So absorption coefficient ) (λ α ∑ can be described as [13] ) 6 ( 296 Therefore, absorption coefficient is proportional to the gas pressure P theoretically. Based on database HITRAN2008, the influence of pressure on peak absorption coefficient of gas absorption line of the C 2 H 2 , CH 4 and CO 2 in the same order of magnitude at 296K can be counted out using Voigt line theory [14][15][16].…”
Section: Theoretical Derivation To Gas Pressure Characteristics Omentioning
confidence: 99%