2005
DOI: 10.1016/j.jms.2004.12.001
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Water line parameters for weak lines in the range 7400–9600cm−1

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Cited by 37 publications
(57 citation statements)
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References 19 publications
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“…There are many applications involving water molecule in which the knowledge of a reliable potential energy surface is required. Selected examples of such applications include the spectrum of the water vapor, which is important for the understanding of the absorption and retention of sunlight in Earth's atmosphere and physics of other planets and stars [103][104][105][106][107][108][109][110][111][112], and combustion studies involving hot steam. For example, the…”
Section: Methodsmentioning
confidence: 99%
“…There are many applications involving water molecule in which the knowledge of a reliable potential energy surface is required. Selected examples of such applications include the spectrum of the water vapor, which is important for the understanding of the absorption and retention of sunlight in Earth's atmosphere and physics of other planets and stars [103][104][105][106][107][108][109][110][111][112], and combustion studies involving hot steam. For example, the…”
Section: Methodsmentioning
confidence: 99%
“…Table 3 summarises the results of analysis in each of these regions. The region below 11 190 cm À1 has been the subject of studies [6,18,19,[28][29][30] which actually probe deeper than the BR results. The results for this region are therefore of less significance.…”
Section: Line Assignmentsmentioning
confidence: 99%
“…Detailed comparison of our energy levels set with compilation [6] has shown that the levels from both sets agree within 0.0012 cm À1 on average. We did not confirm 18 energy levels derived in [3][4][5]. Full set of the obtained energy levels is presented in the electronic archive attached to the paper.…”
Section: Energy Levels Derivationmentioning
confidence: 93%
“…The spectrum under present study is formed by transitions coming on the first hexad upper vibrational states: (101), (200), (002), (120), (021), and (040), it occupies 6000-7940 cm À1 spectral region and has been investigated, since 1986 in a number of papers [1][2][3][4][5]. Chevillard et al [1] presented first consistent study of the first hexad energy levels and line intensities.…”
Section: Introductionmentioning
confidence: 99%
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