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1943
DOI: 10.1103/physrev.64.207
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Absorption Spectrum ofN2in the Extreme Ultraviolet

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Cited by 107 publications
(32 citation statements)
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“…The new fit of the vibrational data is simply a straight line fit to the AG(S) of Verma and Jois Also shown in the figures are new fits to the data, and curves computed using the deperturbed constants of Leoni (1972) and Leoni and Dressler (1972), which are tabulated in both Huber and Herzberg (1979) and Lofthus and Krupenie (1977). Similar data not plotted in Figure 25 can be found in Worley (1943), Gaydon (1944), Lofthus (1957), Tilford and Wilkinson (1964), Yoshino and Tanaka (1977), Yoshino et al (1979) …”
Section: N 2 Dsupporting
confidence: 49%
“…The new fit of the vibrational data is simply a straight line fit to the AG(S) of Verma and Jois Also shown in the figures are new fits to the data, and curves computed using the deperturbed constants of Leoni (1972) and Leoni and Dressler (1972), which are tabulated in both Huber and Herzberg (1979) and Lofthus and Krupenie (1977). Similar data not plotted in Figure 25 can be found in Worley (1943), Gaydon (1944), Lofthus (1957), Tilford and Wilkinson (1964), Yoshino and Tanaka (1977), Yoshino et al (1979) …”
Section: N 2 Dsupporting
confidence: 49%
“…Furthermore, it is possible that the lowest rotational level is not discerned, which also may lead to equivocalities. Based on this scheme, three 1 The rotational level energies of the unperturbed ⌺ states are fitted to the following formula:…”
Section: Resultsmentioning
confidence: 99%
“…The only two states suitable for such an extrapolation are the y 1 ⌸ g , and the k 1 ⌸ g states. Both the a 1 ⌸ g and aЉ 1 ⌺ g ϩ states have vibrational levels in the energy re- Some interactions have been taken explicitly into account. As is clear from the avoided crossings in Fig.…”
Section: Resultsmentioning
confidence: 99%
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