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26
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0007123209
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g symmetry are responsible for the predissociation of both systems. The weaker predissociation to the lower limit supports diabatic behavior at the avoided crossing between the two valence states.
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0001495571
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34
-
-
85034277755
-
-
note
-
a state is known, from absorption spectra, only for ν = 4-11.
-
-
-
-
35
-
-
0000882505
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D. L. Huestis, R. A. Copeland, K. Knutsen, T. G. Slanger, R. T. Jongma, M. G. H. Boogaarts, and G. Meijer, Can. J. Phys. 72, 1109 (1994).
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36
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0000411387
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K. Yoshino, J. R. Esmond, J. E. Murray, W. H. Parkinson, A. P. Thorne, R. C. M. Learner, and G. Cox, J. Chem. Phys. 103, 1243 (1995).
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Yoshino, K.1
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Cox, G.7
-
37
-
-
85034274631
-
-
note
-
Although the CRDS oscillator strengths for the A←X system are ∼40% lower than the UVFTS values, Huestis et al. (Ref. 35) use recommended values close to those of Yoshino et al. (Ref. 36) in estimating the Herzberg I cross-section branching ratio. CRDS oscillator strengths for the weaker A′←X and c←X systems are expected to be significantly more accurate than those for the A←X system.
-
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41
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0010819896
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A. S.-C. Cheung, K. Yoshino, W. H. Parkinson, S. L. Guberman, and D. E. Freeman, Planet. Space Sci. 34, 1007 (1986).
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Freeman, D.E.5
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44
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0013199235
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K. Yoshino, A. S.-C. Cheung, J. R. Esmond, W. H. Parkinson, D. E. Freeman, S. L. Guberman, A. Jenouvrier, B. Coquart, and M. F. Merienne, Planet. Space Sci. 36, 1469 (1988).
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Merienne, M.F.9
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45
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0001327491
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0000501605
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33745174354
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-
53
-
-
85034281843
-
-
note
-
- potential-energy curve.
-
-
-
-
54
-
-
85034307197
-
-
note
-
-1, respectively, for each of the A, A′, and c states.
-
-
-
-
55
-
-
85034286627
-
-
note
-
Extrapolation to ν=-0.5 was performed by fitting a low-order Dunham polynomial to the lowest four known vibrational levels.
-
-
-
-
58
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-
11744270172
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-
Ph.D. dissertation thesis, The Australian National University
-
S. S. Banerjee, Ph.D. dissertation thesis, The Australian National University, 1997.
-
(1997)
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Banerjee, S.S.1
-
60
-
-
85034298350
-
-
note
-
- symmetry.
-
-
-
-
62
-
-
85034303509
-
-
note
-
Subscripts in the transition-moment notation adopted in this work refer to the value of Ω′. Equalities between the moments arise because of symmetry considerations, leading to the need for only three independent moments in the case of the A←X transition.
-
-
-
-
63
-
-
85034300470
-
-
note
-
Expressions given in Ref. 61 have been simplified and corrected to obtain Eqs. (8) and (9).
-
-
-
-
65
-
-
11744263981
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-
edited by G. W. F. Drake AIP, New York
-
D. L. Huestis, in Atomic, Molecular, and Optical Physics Handbook, edited by G. W. F. Drake (AIP, New York, 1996), p. 403.
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-
-
Huestis, D.L.1
-
66
-
-
85034285671
-
-
note
-
ν′(R).
-
-
-
-
67
-
-
85034288907
-
-
note
-
The rotational line strengths employed by Kerr and Watson (Ref. 31) were taken from the photographically recorded spectra of Coquart and Ramsay (Ref. 30).
-
-
-
-
71
-
-
85034293386
-
-
note
-
In principle, it is possible to match the experimental cross section by making adjustments to the A-state potential-energy curve while retaining a smaller transition-moment slope. However, potential-energy curves determined in this way either exhibit anomalies in shape or are inconsistent with the known form in the Rydberg-valence region (Sec. IV B).
-
-
-
-
72
-
-
85034287576
-
-
note
-
-1 to allow for the effects of the lowest B←X hot bands.
-
-
-
-
74
-
-
0021631486
-
-
A. S.-C. Cheung, K. Yoshino, W. H. Parkinson, and D. E. Freeman, Can. J. Phys. 62, 1752 (1984).
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-
-
Cheung, A.S.-C.1
Yoshino, K.2
Parkinson, W.H.3
Freeman, D.E.4
-
78
-
-
85034294695
-
-
note
-
AX is calculated for J=0, the strong J-dependence of the A′←X transition moment leads to a small discrepancy (∼2%).
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-
-
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