Time-resolved infrared emission spectra of naphthalene under gas phase laboratory and astrophysical conditions

2012 ◽  
Vol 990 ◽  
pp. 112-118 ◽  
Author(s):  
P. Parneix ◽  
M. Basire ◽  
F. Calvo
2009 ◽  
Vol 113 (15) ◽  
pp. 3431-3437 ◽  
Author(s):  
Hui-Fen Chen ◽  
Hung-Chu Chiang ◽  
Hiroyuki Matsui ◽  
Soji Tsuchiya ◽  
Yuan-Pern Lee

Science ◽  
1996 ◽  
Vol 274 (5287) ◽  
pp. 582-583 ◽  
Author(s):  
K. Zhang ◽  
B. Guo ◽  
P. Colarusso ◽  
P. F. Bernath

1994 ◽  
Vol 218 (4) ◽  
pp. 295-303 ◽  
Author(s):  
Laszlo Nemes ◽  
Ram S. Ram ◽  
Peter F. Bernath ◽  
Frank A. Tinker ◽  
Michael C. Zumwalt ◽  
...  

2012 ◽  
Vol 136 (4) ◽  
pp. 044302 ◽  
Author(s):  
Yu-Ying Yeh ◽  
Meng-Hsuan Chao ◽  
Po-Yu Tsai ◽  
Yuan-Bin Chang ◽  
Ming-Tsang Tsai ◽  
...  

1975 ◽  
Vol 29 (6) ◽  
pp. 496-500 ◽  
Author(s):  
D. Kember ◽  
N. Sheppard

Infrared emission spectra from metal samples with oxide surface layers are shown to be very advantageously studied using the spectrum-ratioing facility of a recording infrared interferometer. The emission from a given sample is ratioed against that from a black-body emitter at the same temperature so as to give emittance as a function of wavenumber directly. This method has very useful application to irregularly shaped metal emitters. In the absence of selective reflection there is a direct correspondence between emission and absorption spectra for thin layers of an emitting substance. However, the presence of selective reflection leads to reduced emission and to considerable differences in the appearance of “absorption” and emission spectra in regions of strong absorption. Emission spectra obtained from copper plates heated, above 150°C, for different periods in air are shown clearly to indicate the presence of cuprous, Cu(I), and cupric, Cu(II), oxides in the surface layer.


2021 ◽  
Vol 768 ◽  
pp. 138403
Author(s):  
Kendall D. Hughey ◽  
Russell G. Tonkyn ◽  
Warren W. Harper ◽  
Valerie L. Young ◽  
Tanya L. Myers ◽  
...  

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