Vibration-rotation interactions between overtone and combination levels of asymmetric-top molecules: Application to the infrared spectroscopy of formaldehyde and ketene

2005 ◽  
Vol 122 (3) ◽  
pp. 034307 ◽  
Author(s):  
David M. Smith
1980 ◽  
Vol 87 ◽  
pp. 515-524 ◽  
Author(s):  
Donald N. B. Hall

High resolution spectra of red giants and long period variables exhibit lines of infrared CO vibration-rotation bands arising in circumstellar material. In the few such stars so far observed at very high resolution (≲ 1 km/s) the circumstellar material appears localized in 3 distinct regimes with temperatures of 800K, 200K and 75K and expansion velocities of 0, 10 and 16 km/s rather than being uniformly distributed.


1984 ◽  
Vol 62 (12) ◽  
pp. 1300-1305 ◽  
Author(s):  
L. O. Halonen ◽  
C. M. Deeley ◽  
I. M. Mills ◽  
V.-M. Horneman

High-resolution Fourier transform infrared spectra have been recorded and analyzed for the ν3, ν4, ν5, and ν6 fundamental bands of trans-DONO, and for the ν4 fundamental of cis-DONO. The spectral resolution was better than 0.01 cm−1, and the bands have been fitted using an asymmetric top Hamiltonian with a standard deviation of around 0.0006 cm−1.


1963 ◽  
Vol 38 (1) ◽  
pp. 8-17 ◽  
Author(s):  
K. T. Chung ◽  
Paul M. Parker

1970 ◽  
Vol 24 (2) ◽  
pp. 161-174 ◽  
Author(s):  
Philip L. Hanst

The use of spectroscopic methods in the analysis of the atmosphere is discussed. The special advantages of infrared vibration-rotation spectra for identification and measurement of air pollutants are emphasized. The capabilities of lasers in atmospheric work are reviewed, with particular attention being given to proposed methods of detecting pollutants by absorption of selected ir laser lines. Some commentary is presented on current and future atmospheric studies.


In the last few years, the specificities of millimetre-wave spectroscopy coupled with active developments in other fields ( ab initio calculation, radioastronomy and infrared spectroscopy) have led to an impressive increase in our knowledge of the spectral characteristics of molecular ions. The advances to be reviewed in this paper are a result of the development of highly sensitive spectrometers and of efficient methods of production. Some specific examples, including ions with large-amplitude motion (H 3 0 + ), weakly polar ions (HCNH + ), asymmetric-top ions (HCO+2, HON+2) and ionic clusters (Ar • H+3), will be used to illustrate the potentialities of millimetre- and submillimetre-wave spectroscopy.


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