Radiofrequency, Microwave, Submillimeter-Wave, and High-Resolution Infrared Spectra of thev6= 1 Vibrational State of CDF3

1997 ◽  
Vol 182 (1) ◽  
pp. 34-49 ◽  
Author(s):  
H. Bürger ◽  
J. Cosléou ◽  
J. Demaison ◽  
C. Gerke ◽  
H. Harder ◽  
...  
Keyword(s):  
High Resolution ◽  
Infrared Spectra ◽  
Vibrational State ◽  
Submillimeter Wave

High-Resolution Infrared Spectra of the ν1 Fundamental Bands of Mono-Substituted 13C Propyne Isotopologues

2018 ◽  
Vol 122 (2) ◽  
pp. 582-589 ◽  
Author(s):  
Kirstin D. Doney ◽  
Dongfeng Zhao ◽  
Harold Linnartz
Keyword(s):  
High Resolution ◽  
Infrared Spectra

High resolution infrared spectra of water vapor

1969 ◽  
Vol 29 (1-3) ◽  
pp. 312-347 ◽  
Author(s):  
Phillip E. Fraley ◽  
K. Narahari Rao ◽  
L.H. Jones
Keyword(s):  
Water Vapor ◽  
High Resolution ◽  
Infrared Spectra

Erratum: High resolution infrared spectra of the ν2 and 2ν1 bands of 14N16O2

1976 ◽  
Vol 54 (10) ◽  
pp. 1087-1087
Author(s):  
Aldée Cabana ◽  
Michel Laurin ◽  
Walter J. Lafferty ◽  
Robert L. Sams
Keyword(s):  
High Resolution ◽  
Infrared Spectra

High Resolution Infrared Spectra of the ν2 and 2ν1 Bands of 14N16O2

1975 ◽  
Vol 53 (19) ◽  
pp. 1902-1926 ◽  
Author(s):  
Aldée Cabana ◽  
Michel Laurin ◽  
Walter J. Lafferty ◽  
Robert L. Sams
Keyword(s):  
High Resolution ◽  
Infrared Spectra ◽  
Ground State ◽  
Equilibrium Structure ◽  
Coriolis Interaction ◽  
Rotational Constants ◽  
Average Structures

The infrared spectra of two B type bands, ν2 and 2ν1, of 14N16O2 have been recorded under high resolution. Ground state combination differences from these bands have been combined with combination differences obtained in previous studies and eight pure rotational microwave transitions to yield improved ground state rotational constants. Upper state constants and band centers for the ν2 and 2ν1 bands are also reported. The 2ν1 band contains internal intensity anomalies believed to arise from a weak Coriolis interaction with the much stronger ν1 + ν3 band. Equilibrium rotational constants have been calculated. The equilibrium structure of the molecule is: rc = 1.1945 ± 0.0005 Å and Θc = 133.85 ± 0.10°. For the sake of comparison, effective, substitution, and average structures are also reported.

High-resolution infrared spectra of jet-cooled allyl radical (CH2–CH–CH2): ν2, ν3, and ν14 C–H stretch vibrations

2002 ◽  
Vol 116 (15) ◽  
pp. 6505-6512 ◽  
Author(s):  
Jia-xiang Han ◽  
Yu. G. Utkin ◽  
Hong-bing Chen ◽  
Neil T. Hunt ◽  
R. F. Curl
Keyword(s):  
High Resolution ◽  
Infrared Spectra ◽  
Allyl Radical

High-resolution infrared spectra of spiropentane, C5H8

2011 ◽  
Vol 269 (1) ◽  
pp. 129-136 ◽  
Author(s):  
J.E. Price ◽  
K.A. Coulterpark ◽  
T. Masiello ◽  
J.W. Nibler ◽  
A. Weber ◽  
...  
Keyword(s):  
High Resolution ◽  
Infrared Spectra

scholarly journals New Infrared Spectra of the Jovian Planets: Study of Jupiter and Saturn in the 3v3 Methane Band by Fourier Transform Spectroscopy

1974 ◽  
Vol 65 ◽  
pp. 357-358
Author(s):  
C. De Bergh ◽  
M. Combes ◽  
Th. Encrenaz ◽  
J. Lecacheux ◽  
M. Vion ◽  
...  
Keyword(s):  
Fourier Transform ◽  
High Resolution ◽  
Infrared Spectra ◽  
Rotational Temperature ◽  
Michelson Interferometer ◽  
Fourier Transform Spectroscopy ◽  
Half Width ◽  
Layer Model ◽  
Jovian Planets

High resolution spectra of Jupiter and Saturn were obtained with a Fourier Transform Michelson interferometer. A comparison of the observed spectra, after elimination of the solar and terrestrial contributions to absorption, with synthetic profiles for the reflecting layer model has permitted new determinations of the Lorentz half-width, the methane abundance, the rotational temperature and the pressure at the level of formation of the methane lines for both Jupiter and Saturn.

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