The IUPAC Database of Rotational-Vibrational Energy Levels and Transitions of Water Isotopologues from Experiment and Theory
- 1. MTA-ELTE Research Group on Complex Chemical Systems, H-1518 Budapest, P.O. Box 32, Hungary
- 2. Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, U.K.
- 3. Old Dominion University, Norfolk, VA, USA
- 4. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
- 5. Université Joseph Fourier/CNRS, Grenoble, France
- 6. Université de Reims Champagne-Ardenne, Reims, France
- 7. University of Massachusetts, Lowell, MA, USA
- 8. National Institute of Standards and Technology, Gaithersburg, MD, USA
- 9. Institute of Atmospheric Optics, Russian Academy of Sciences, Tomsk, Russia
- 10. Institute of Applied Physics, Russian Academy of Sciences, Nizhny Novgorod, Russia
- 11. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
- 12. Institut d’Aéronomie Spatiale de Belgique, Brussels, Belgium
Description
The results of an IUPAC Task Group formed in 2004 on “A Database of Water Transitions from Experiment and Theory” (Project No. 2004-035-1-100) are presented. Energy levels and recommended labels involving exact and approximate quantum numbers for the main isotopologues of water in the gas phase, H216O, H218O, H217O, HD16O, HD18O, HD17O, D216O, D218O, and D217O, are determined from measured transition wavenumbers. The transition wavenumbers and energy levels are validated using the MARVEL (measured active rotational–vibrational energy levels) approach and first-principles nuclear motion computations. The extensive data, e.g., more than 200,000 transitions have been handled for H216O, including lines and levels that are required for analysis and synthesis of spectra, thermochemical applications, the construction of theoretical models, and the removal of spectral contamination by ubiquitous water lines. These datasets can also be used to assess where measurements are lacking for each isotopologue and to provide accurate frequencies for many yet-to-be measured transitions. The lack of high-quality frequency calibration standards in the near infrared is identified as an issue that has hindered the determination of high-accuracy energy levels at higher frequencies. The generation of spectra using the MARVEL energy levels combined with transition intensities computed using high accuracy ab initio dipole moment surfaces are discussed.
Notes
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