Absolute line intensities measurements and calculations for the 5.7 and 3.6 μm bands of formaldehyde

The goal of this study is to achieve absolute line intensities for the strong 5.7 and 3.6 mu m bands of formaldehyde and to generate, for both spectral regions, an accurate list of line positions and intensities. Both bands are now used for the infrared measurements of this molecule in the atmosphere. However, in the common access spectroscopic databases there exists, up to now, no line parameters for the 5.7 mu m region, while, at 3.6 mu m, the quality of the line parameters is quite unsatisfactory. High-resolution Fourier transform spectra were recorded for the whole 1600-3200 cm(-1) spectral range and for different path-length-pressure products conditions. Using these spectra, a large set of H2CO individual line intensities was measured simultaneously in both the 5.7 and 3.6 mu m spectral regions. From this set of experimental line strength which involve, at 5.7 mu m the nu(2) band and, at 3.6 mu m, the nu(1) and nu(5) bands together with nine dark bands, it has been possible to derive a consistent set of line intensity parameters for both the 5.7 and 3.6 mu m spectral regions. These parameters were used to generate a line list in both regions. For this task, we used the line positions generated in [Margules L, Perrin A, Janeckova R, Bailleux S, Endres CR Giesen TF, et al. Can J Phys, accepted] and [Perrin A, Valentin A, Daumont L, J Mol Struct 2006;780-782:28-42] for the 5.7 and 3.6 mu m, respectively. The calculated band intensities derived for the 5.7 and 3.6 mu m bands are in excellent agreement with the values achieved recently by medium resolution band intensity measurements. It has to be mentioned that intensities in the 3.6 mu m achieved in this work are on the average about 28% stronger than those quoted in the HITRAN or GEISA databases. Finally, at 3.6 mu m the quality of the intensities was significantly improved even on the relative scale, as compared to our previous study performed in 2006. (c) 2008 Elsevier Ltd. All rights reserved.