The effect of ground state population on the XeF laser performance

1980 ◽  
Vol 36 (4) ◽  
pp. 243-245 ◽  
Author(s):  
M. Rokni ◽  
J. H. Jacob ◽  
J. C. Hsia ◽  
D. W. Trainor
1989 ◽  
Vol 19 (6) ◽  
pp. 759-765 ◽  
Author(s):  
A A Isaev ◽  
V T Mikhkel'soo ◽  
G G Petrash ◽  
V É Peét ◽  
I V Ponomarev ◽  
...  

2018 ◽  
Vol 20 (2) ◽  
pp. 029501 ◽  
Author(s):  
F Gebert ◽  
Y Wan ◽  
F Wolf ◽  
Jan C Heip ◽  
Piet O Schmidt

1964 ◽  
Vol 4 (6) ◽  
pp. 102-104 ◽  
Author(s):  
R. L. Aagard ◽  
R. A. Dufault

2010 ◽  
Vol 81 (4) ◽  
Author(s):  
P. London ◽  
O. Firstenberg ◽  
M. Shuker ◽  
A. Ron

2010 ◽  
Vol 18 (18) ◽  
pp. 18832 ◽  
Author(s):  
Asif Sinay ◽  
Moshe Shuker ◽  
Ofer Firstenberg ◽  
Amnon Fisher ◽  
Amit Ben-Kish ◽  
...  

2016 ◽  
Vol 18 (1) ◽  
pp. 013037 ◽  
Author(s):  
F Gebert ◽  
Y Wan ◽  
F Wolf ◽  
Jan C Heip ◽  
Piet O Schmidt

1967 ◽  
Vol 22 (12) ◽  
pp. 1953-1959 ◽  
Author(s):  
W.L. Bohn

Steady-state population densities and electron densities are calculated in a non-equilibrium hydrogen plasma at constant pressure. The ratio of the temperatures of electrons and heavy particles is taken as a parameter. The radiation field of the LYMAN lines is included using a mean absorption coefficient for each transition. The deviations of densities of excited levels and electrons from equilibrium values are very large at low temperatures. The ground state population remains closer to equilibrium until the resonance radiation field vanishes with increasing temperature. Deviations from equilibrium are found to be present even at atmospheric pressure. Detailed results are shown in numerous diagrams for pressures from 0.01 to 1 atmosphere and electron temperatures from 5 × 103 to 4×104°K.


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