Direct measurements of N2 broadened linewidths in the CO fundamental at low temperatures

1983 ◽  
Vol 61 (2) ◽  
pp. 192-197 ◽  
Author(s):  
J.-P. Bouanich ◽  
R. Farrenq ◽  
C. Brodbeck
Keyword(s):  
High Resolution ◽  
Temperature Dependence ◽  
Low Temperatures ◽  
Variable Temperature ◽  
Absorption Cell ◽  
Fundamental Band ◽  
Direct Measurements ◽  
High Resolution Spectrometer ◽  
Vibration Rotation ◽  
Resolution Spectrometer

The halfwidths of CO vibration–rotation lines, pressure-broadened by N2 have been measured in the fundamental band at −83, −148, and −180 °C, using a variable temperature absorption cell and a high resolution spectrometer. The temperature dependence of linewidths has been calculated from the Anderson–Tsao–Curnutte theory and compared to the experimental determinations.

Nuclear analysis of the DEMO divertor survey visible high-resolution spectrometer

2021 ◽  
Vol 169 ◽  
pp. 112460
Author(s):  
R. Luís ◽  
Y. Nietiadi ◽  
A. Silva ◽  
B. Gonçalves ◽  
T. Franke ◽  
...  
Keyword(s):  
High Resolution ◽  
Nuclear Analysis ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

Low pressure spark chambers — high resolution spectrometer for 1 GeV protons

1967 ◽  
Vol 54 (1) ◽  
pp. 71-76 ◽  
Author(s):  
R.J. Sutter ◽  
G. Bennett ◽  
J. Fischer ◽  
J.L. Friedes ◽  
H. Palevsky ◽  
...  
Keyword(s):  
High Resolution ◽  
Low Pressure ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

scholarly journals HERMES – An instrument of the future

2009 ◽  
Vol 5 (S262) ◽  
pp. 448-449 ◽  
Author(s):  
Elizabeth Wylie-de Boer ◽  
Kenneth Freeman
Keyword(s):  
Star Formation ◽  
High Resolution ◽  
Resolving Power ◽  
Individual Stars ◽  
Elemental Abundances ◽  
The Future ◽  
The Galaxy ◽  
History Of ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer

AbstractHERMES is a new, multi-object high resolution spectrometer for the 3.9m Anglo Australian Telescope, using the existing 2dF positioner. The primary goal of the HERMES survey is to unravel the history of the Galaxy from detailed elemental abundances for about 1.2 million individual stars. The HERMES chemical tagging survey concentrates on the 5000 to 8000 Å window at a resolving power of 30,000 in order to identify dissolved star formation aggregates and ascertain the importance of mergers throughout the history of the Galaxy.

Application of a High-Resolution Spectrometer in a Broadband Optical Monitor for Film Coating

2008 ◽  
Vol 53 (9(4)) ◽  
pp. 2307-2311
Author(s):  
Yun-Fei Wu ◽  
Qing-Yuan Cai ◽  
Yu-Xiang Zheng ◽  
Rong-Jun Zhang ◽  
Liang-Yao Chen
Keyword(s):  
High Resolution ◽  
Film Coating ◽  
High Resolution Spectrometer ◽  
Resolution Spectrometer
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