Determination of Carbon Monoxide and Carbon Dioxide Concentrations at Temperatures between 295 and 1250 K Using Fourier Transform Infrared Absorption Spectroscopy

1992 ◽  
Vol 46 (12) ◽  
pp. 1887-1894 ◽  
Author(s):  
Patrick J. Medvecz ◽  
Kenneth M. Nichols

Fourier transform infrared absorption spectroscopy has been used for the determination of CO and CO2 gas concentrations in a high-temperature cell. The gas mixtures analyzed consisted of CO, CO2, and nitrogen; among the samples, the concentration of CO was varied between 0.5 and 4.7% and the CO2 ranged between 0.7 and 4.9%. The temperature of the gas cell was varied between 295 and 1250 K, while the pressure was maintained at atmospheric. Throughout this temperature range, 123 absorption spectra were recorded in the gas cell at a nominal instrument resolution of 0.25 cm−1. The absorption lines used for the concentration analysis consisted of 22 P-branch CO vibrational-rotational lines from the fundamental absorption band, and 19 R-branch CO2 vibrational-rotational lines from the v3 fundamental absorption band. All of the peak heights used for the concentration calculations were first numerically corrected for photometric errors resulting from the finite resolution of the FT-IR instrument. The corrected peak heights were assumed to follow the Bouguer-Lambert law at a constant furnace temperature. Fifty-one of the spectra were used to determine the temperature dependence of the line strength for each of the 41 lines. The experimentally obtained line strengths were then used to determine the gas concentrations of all 123 spectra. The calculated concentrations were compared to NDIR instrument measurements of the gas composition exiting the flow-through high-temperature gas cell. Comparison of the NDIR measured gas concentrations with the calculated concentrations from absorption spectra yielded an average accuracy of 3.6% for the CO spectra and 4.9% for the CO2 spectra.

2011 ◽  
Vol 50 ◽  
pp. 01BE03 ◽  
Author(s):  
Jun Shirahata ◽  
Tetsutaro Ohori ◽  
Hiroki Asami ◽  
Tsuneo Suzuki ◽  
Tadachika Nakayama ◽  
...  

1994 ◽  
Vol 48 (11) ◽  
pp. 1442-1450 ◽  
Author(s):  
Patrick J. Medvecz ◽  
Kenneth M. Nichols

Fourier transform infrared absorption spectroscopy has been used for the determination of the line strengths of 41 CO and CO2 absorption lines at temperatures between 295 and 1250 K. The CO vibrational-rotational lines were from the P branch of the fundamental absorption band (2150–1950 cm−1) while the CO2 vibrational-rotational lines were from the far wing of the R branch of the v3 fundamental band (2395–2380 cm−1). The intensities of the lines were measured from absorption spectra recorded in a high-temperature gas cell containing known concentrations of CO/CO2/N2 gas mixtures at atmospheric pressure. Absorption spectra were recorded through the cell with the use of a moderate-resolution Fourier transform infrared spectrometer. The absorption spectra were mathematically corrected for distortions resulting from the finite resolution of the spectrometer and for peak overlap. Line strength measurements were made from the corrected peaks by using the Bouguer-Lambert law and assuming a Lorenztian line profile. The experimentally obtained line strengths were evaluated (1) by statistical calculations, (2) by consideration of the validity of the Bouguer-Lambert assumption for these data, (3) by comparison with existing room-temperature and high-temperature data, and (4) by comparison with theoretical calculations. For CO, the statistical analysis suggests that the reported values have an uncertainty of ±10–12%, which is similar to the observed discrepancies with other reported values at room temperature. At high temperatures, the difference between these data and previously reported data and theoretical predictions is less than 10%. For CO2, the statistical uncertainty associated with the line strength calculations is less than 5%, which is also the approximate level of agreement with existing room-temperature data. For lines with m indicies of 65–89, at high temperatures, the values reported in this work agree within 5 to 10% of theoretical calculations.


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