DocumentCode
1137196
Title
A comparison of rare-gas flashlamps
Author
Oliver, John R. ; Barnes, Frank S.
Author_Institution
Univ. of Colorado, Boudler, CO, USA
Volume
5
Issue
5
fYear
1969
fDate
5/1/1969 12:00:00 AM
Firstpage
232
Lastpage
237
Abstract
Spectral data for argon, krypton, xenon, and neon flashlamps are presented for the region of lamp operation in which the line radiation makes up a substantial portion of the total radiant energy. The spectral charateristics are presented in terms of both power flux and emitted quanta per unit area per second, the latter being appropriate for the characterization of illumination and laser pumping efficiencies. The emission spectra show strong line radiation peculiar to each gas superimposed on a low emissivity background continuum. The electrical resistance coefficient
is presented for each gas and is shown to increase with increasing gas atomic weight and pressure. An analysis of lamp radiative efficiency indicates that through proper optimization of the gas pressure, the efficiency and overall output of the lighter rare gases will be comparable to those for optimized xenon lamps with optimum pressures increasing with decreasing gas atomic weight. Overall lamp efficiencies are shown to be as high as 40 percent in the
region.
is presented for each gas and is shown to increase with increasing gas atomic weight and pressure. An analysis of lamp radiative efficiency indicates that through proper optimization of the gas pressure, the efficiency and overall output of the lighter rare gases will be comparable to those for optimized xenon lamps with optimum pressures increasing with decreasing gas atomic weight. Overall lamp efficiencies are shown to be as high as 40 percent in the
region.Keywords
Argon; Atomic measurements; Electric resistance; Gas lasers; Lamps; Laser excitation; Lighting; Power lasers; Pump lasers; Xenon;
fLanguage
English
Journal_Title
Quantum Electronics, IEEE Journal of
Publisher
ieee
ISSN
0018-9197
Type
jour
DOI
10.1109/JQE.1969.1075765
Filename
1075765
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