Chemiluminescent NiO* emissions: band systems and spectral simulation

2011 ◽  
Vol 89 (8) ◽  
pp. 869-874 ◽  
Author(s):  
R.L. Gattinger ◽  
W.F.J. Evans ◽  
E.J. Llewellyn

Following the renewed interest in metal oxide emissions in the night airglow, high-resolution laboratory observations of NiO* in the visible and near-infrared regions of the spectrum are reviewed, and approximate spectroscopic constants are derived to augment those already available in the literature. A preliminary spectral band simulation model is developed for the relevant NiO systems. Franck–Condon factors, calculated using the preliminary spectroscopic constants, are used in the model to conduct an iterative comparison with low-resolution NiO* chemiluminescent emissions observed in the laboratory. Relative vibrational level populations are estimated, and shortcomings of the model are noted. The existence of a new NiO band system is also suggested.

1979 ◽  
Vol 57 (3) ◽  
pp. 496-504 ◽  
Author(s):  
B. R. Yadav ◽  
S. B. Rai ◽  
D. K. Rai

The electronic spectrum of the GaO molecule has been re-investigated in the region 3600–4200 Å The use of high resolution and dispersion permitted clear resolution of the rotational structure and the formation of head of heads in Δν = + 1 and + 2 sequences is clearly visible. The rotational analyses of the (0,0) and the (1,0) bands have been performed and more reliable molecular constants have been obtained. Intensity anomalies in the bands have been explained on the basis of the true potential energy curves and the associated Franck–Condon factors.


Author(s):  
Adil Nameh Ayaash

The present work concerns by study of spectroscopic properties for Beryllium monobromide BeBr. Franck Condon Factor of BeBr molecule had been calculated theoretically for ground state X2Σ+ and excited state A2Π by special integrals by depending on spectroscopic constants for this molecule. The Dissociation energy and potential curves of this molecule is studied in this work by using Hua potential function, the results of potential curves and Franck Condon Factors converge with other researchers results.


2021 ◽  
Vol 923 (2) ◽  
pp. 234
Author(s):  
Jason J. Sorensen ◽  
Peter F. Bernath

Abstract The ZrO B1Π—X1Σ+ transition is an important opacity source in the near-infrared and optical spectrum of S-type stars. The 0–0, 0–1, 0–2, 1–0, 1–2, 1–3, 2–0, 2–1, 2–3, 2–4, 3–1, 3–4, and 4–2 bands of the 90Zr16O B1Π—X1Σ+ transition are reanalyzed using a high-temperature (2390 K) high-resolution (0.04 cm−1) emission spectrum collected at the National Solar Observatory (Kitt Peak). A modern spectroscopic analysis was performed using the PGOPHER program to provide updated spectroscopic constants and to produce a high-precision line list with line strengths based on an ab initio calculation of the transition dipole moment.


1979 ◽  
Vol 57 (8) ◽  
pp. 1178-1184 ◽  
Author(s):  
M. L. Sink ◽  
A. D. Bandrauk

Ab initio Cl calculations of the transition moment for the B′2Σ+–X2Σ+ transition in MgH are reported. Theoretical values for the Franck–Condon factors, band strengths, band oscillator strengths, and transition probabilities have been computed for MgH and MgD. An analysis of our results for this system predicts many bands to be observable which have not yet been identified. Dipole moment functions and vibrationally averaged dipole moments are given for the X2Σ+, A2Π, and B′2Σ+ electronic states.


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