Laser spectroscopic study of ozone in the 100←000 band for the SWIFT instrument

Abstract

A complete spectroscopic study of 15 strong ozone lines in the 1132.5–1134.5 cm −1 spectral range has been undertaken in the framework of the development of the stratospheric wind interferometer for transport studies (SWIFT), led by the Canadian Space Agency. Measurements have been performed with an interferometrically stabilized tunable diode laser spectrometer. Absolute line positions and intensities have been determined with high accuracy (4×10 −5 cm −1 and 1–2% respectively). Self- and air-broadening coefficients at 296 K have been obtained with an accuracy of 1%. The air-shifting coefficient and its temperature dependence have also been measured for unblended lines together with the temperature dependence of the air-broadening. Line intensities have been calibrated by simultaneously performed UV absorption measurements at 253.7 nm. Our IR/UV comparison supports a previously reported inconsistency between recommended IR intensities (HITRAN08) and UV absorption cross-sections and indicates that current IR intensities are too small by ∼3%.