NASA NTRS · 19920065599
Improved spectroscopic line parameters for the ozone molecule
Abstract
Recently the authors made a comprehensive compilation of improved line positions, intensities, and lower state energies of ozone between 0 and 3400/cm. Examples of improvement brought by these data and progress achieved in remote sensing using them are given. Areas for future study include hot bands in the higher wavenumber range, spectral regions above 3400/cm, the O-17 isotopic variants of ozone, broadening coefficients, and emission from high-lying vibrational levels of ozone in the upper atmosphere.
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Flaud, J. M., Rinsland, C. P.. 1991-06-01. Improved spectroscopic line parameters for the ozone molecule. https://ntrs.nasa.gov/citations/19920065599
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