Abstract

This is the third of a series of articles reporting critically evaluated rotational–vibrational line positions, transition intensities, and energy levels, with associated critically reviewed labels and uncertainties, for all the main isotopologues of water. This paper presents experimental line positions, experimental-quality energy levels, and validated labels for rotational–vibrational transitions of the most abundant isotopologue of water, H216O. The latest version of the MARVEL (Measured Active Rotational–Vibrational Energy Levels) line-inversion procedure is used to determine the rovibrational energy levels of the electronic ground state of H216O from experimentally measured lines, together with their self-consistent uncertainties, for the spectral region up to the first dissociation limit. The spectroscopic network of H216O containstwo components, an ortho (o) and a para (p) one. For o-H216O and p-H216O, experimentally measured, assigned, and labeled transitions were analyzed from more than 100 sources. The measured lines come from one-photon spectra recorded at room temperature in absorption, from hot samples with temperatures up to 3000K recorded in emission, and from multiresonance excitation spectra which sample levels up to dissociation. The total number of transitions considered is 184667 of which 182156 are validated: 68027 between para states and 114129 ortho ones. These transitions give rise to 18486 validated energy levels, of which 10446 and 8040 belong to o-H216O and p-H216O, respectively. The energy levels, including their labeling with approximate normal-mode and rigid-rotor quantum numbers, have been checked against ones determined from accurate variational nuclear motion computations employing exact kinetic energy operators as well as against previous compilations of energy levels. The extensive list of MARVEL lines and levels obtained are deposited in the supplementary data of this paper, as well as in a distributed information system applied to water, W@DIS, where they can easily be retrieved.

Highlights

  • Water is the most abundant polyatomic molecule in the universe and it is responsible for the majority of the greenhouse effect on Earth [1]

  • (2bb) 83Guelachv [81]. 1181 lines of H216O were measured in the 1066–2296 cmÀ1 spectral range with an Fourier transform spectroscopy (FTS) under room temperature conditions and natural abundance

  • This paper reports lines obtained from FTS measurements of water vapor at low pressure is in the spectral range of 2903–4255 cmÀ1

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Summary

Introduction

Water is the most abundant polyatomic molecule in the universe and it is responsible for the majority of the greenhouse effect on Earth [1]. As emphasized already in Parts I and II, a distinguishing feature of the present series of IUPAC-sponsored spectroscopic studies is the joint utilization of all available experimental and the best theoretical line (transition) and energy-level data, with a long-term aim of creating complete linelists for all water isotopologues. Emission spectra for water are available over a extensive range of temperatures, the hottest being spectra recorded in an oxy-acetylene flame at about 3000 K [174] These spectra provide a rich source of information on states both with significant bending excitation [175], which are normally not probed in standard absorption spectra, and with high levels of rotational excitation. Sunspots provide a very rich source of spectroscopic data on water [168] and many lines, which are almost certainly due to hot water, still need to be assigned

Pre-MARVEL validation
Uncertainties
Hot transitions
Multiphoton transitions
Recalibration
Comments on the data sources
Variational validation
Post-MARVEL validation
MARVEL energy levels
Status of highly accurate transitions
Comparison with previous sets of energy levels
A comparison with HITRAN and HITEMP
Conclusions
Findings
O lines as frequency standards in the
Full Text
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