Special features of the periodic-pulse-train laser radiation confinement in doped gallium arsenide and zinc selenide

2002 ◽  
Vol 28 (1) ◽  
pp. 48-49 ◽  
Author(s):  
O. P. Mikheeva ◽  
A. I. Sidorov ◽  
A. S. Khaiikina ◽  
E. V. Chuguevets
2008 ◽  
Vol 77 (4) ◽  
Author(s):  
Ken-ichi Hino ◽  
Xiao Min Tong ◽  
Nobuyuki Toshima
Keyword(s):  

2001 ◽  
Vol 46 (1) ◽  
pp. 59-62 ◽  
Author(s):  
S. P. Zhvavyi ◽  
G. D. Ivlev ◽  
O. L. Sadovskaya

1998 ◽  
Vol 16 (1) ◽  
pp. 61-70 ◽  
Author(s):  
A. Magunov ◽  
A. Faenov ◽  
I. Skobelev ◽  
T. Pikuz ◽  
D. Batani ◽  
...  

Time- and space-integrated emission spectra measurements have been performed in plasma produced by 308 nm wavelength XeCl laser radiation (IL = (4–10)·1012 W/cm2, τ = 10 ns) and by 248 nm wavelength KrF laser pulse train radiation (IL = 5·1015 W/cm2, τ = 7 ps, 16 pulses in train) on CF2 plane target. Theoretical modelling of Lyman series and He-like ion resonance series of fluorine and its fit of experimental data show considerable differences in the absorption of laser radiation in the two plasmas.


1994 ◽  
Author(s):  
Yuri A. Zagoruiko ◽  
Vitaliy K. Komar ◽  
V. P. Migal ◽  
O. N. Chugai

1978 ◽  
Vol 3 (3) ◽  
pp. 200-205 ◽  
Author(s):  
R. N. Manchester

Pulsars are unique astronomical objects in that their emission is in the form of a periodic pulse train. For most pulsars the pulse duty cycle is small, only a few per cent of the period. The shapes and intensities of individual pulses are in general quite variable. This is illustrated in Figure 1 which shows a series of individual pulses from PSR 1133 + 16. Despite this variation in shape of individual pulses, it is found that the mean or integrated pulse profile obtained by adding many pulses synchronously with the period is in most cases stable in shape.


2020 ◽  
Vol 2 (3) ◽  
pp. 034009
Author(s):  
Shen Huang ◽  
Guodong Shao ◽  
Yufeng Song ◽  
Luming Zhao ◽  
Deyuan Shen ◽  
...  

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