scholarly journals Absorption Coefficients and Hydrogen Line Intensities.⋆

1936 ◽  
Vol 96 (3) ◽  
pp. 268-268 ◽  
Author(s):  
D. H. Menzel ◽  
C. L. Pekeris
Astrophysics ◽  
1970 ◽  
Vol 4 (4) ◽  
pp. 276-278
Author(s):  
T. I. Kuznetsova

1994 ◽  
Vol 154 ◽  
pp. 365-370
Author(s):  
R. T. Boreiko ◽  
T. A. Clark ◽  
D. A. Naylor ◽  
J. R. Busler

This paper reports the observation of high-n lines in emission from n = 12-11, 13-12, 14-13 and 16-15 Rydberg transitions in H, Mg and Si in solar far IR spectra taken from balloon altitudes, in which the H I line intensities are found to exceed those from the heavier elements. Tentative identification is also made of the n = 8-7 hydrogen line in emission on 20 μm spectra taken from Mauna Kea. The characteristics of the hydrogen lines are compared with lower-n transitions seen in the Space Shuttle ATMOS spectra, in which Brackett, Pfund and n = 6 lines with Δn = 1, 2, 3 and 4 are seen as broad absorption features, while the n = 7-6 line shows a small emission peak within a broader absorption line and the n = 9-7, and possibly the 11-8, transitions appear as weak emission lines. These results indicate that the transformation from absorption to emission occurs at longer wavelengths for hydrogen lines than for those of heavier elements.


1988 ◽  
Vol 334 ◽  
pp. L103 ◽  
Author(s):  
P. W. J. L. Brand ◽  
A. Moorhouse ◽  
M. G. Burton ◽  
T. R. Geballe ◽  
M. Bird ◽  
...  

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