UV and VUV high resolution Fourier transform spectroscopy: laboratory atomic and molecular spectroscopy for astrophysics and atmospheric physics applications

Author(s):  
Juliet C. Pickering ◽  
Darren G. Smillie ◽  
Richard Blackwell-Whitehead ◽  
Anne P. Thorne ◽  
Jonathan E. Murray ◽  
...  
1987 ◽  
Vol 122 (2) ◽  
pp. 462-476 ◽  
Author(s):  
Kuniaki Nakagawa ◽  
R.H. Schwendeman ◽  
J.W.C. Johns

1974 ◽  
Vol 65 ◽  
pp. 357-358
Author(s):  
C. De Bergh ◽  
M. Combes ◽  
Th. Encrenaz ◽  
J. Lecacheux ◽  
M. Vion ◽  
...  

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.


1988 ◽  
Vol 43 (8-9) ◽  
pp. 755-757 ◽  
Author(s):  
N. Heineking ◽  
M. Andolfatto ◽  
C. Kruse ◽  
W. Eberstein ◽  
H. Dreizler

Abstract Employing the high resolution of microwave Fourier transform spectroscopy, we investigated the lowest rotational transitions of fluoro-, bromo-, and iodoacetylene-d. Along with the rotational, centrifugal distortion, halogen nuclear quadrupole, and halogen spin-rotation coupling constants, we determined the deuterium quadrupole coupling constants of bromo-and iodoacetylene-d. For fluoroacetylene-d, we redetermined the deuterium nuclear quadrupole coupling constants with higher accuracy.


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