TEA-N2 laser with a high level of average radiation power

2021 ◽  
Author(s):  
Boris A. Kozlov ◽  
Dmitry S. Makhanko ◽  
Alexander Y. Payurov
2020 ◽  
Vol 24 (2) ◽  
pp. 22-27
Author(s):  
A.M. Gonopol'sky ◽  
S.G. Shashkovskiy ◽  
Y.A. Goldstein ◽  
S.G. Kireev ◽  
A.D. Volosatova ◽  
...  

Photochemical decomposition of phenol with a concentration of 5 to 24 mg/L using hydrogen peroxide and ultraviolet irradiation (UV/H2O2) was studied. Xenon flash lamp was chosen as a radiation source. It emits high-intensity continuous-spectrum radiation in a wide wavelength range from 200 to 1000 nm. The effect of the initial concentration of hydrogen peroxide and the source average radiation power on the phenol destruction rate were studied. An extremum in the dependence of the phenol decomposition rate constant on the initial concentration of hydrogen peroxide was found. Kinetic model of the process based on the obtained data was developed. It was tested by predicting phenol destruction rate with the different process parameters and gave good accuracy.


2000 ◽  
Vol 30 (12) ◽  
pp. 1107-1108 ◽  
Author(s):  
N F Andreev ◽  
O V Palashov ◽  
A K Potemkin ◽  
D H Reitze ◽  
Aleksandr M Sergeev ◽  
...  

2018 ◽  
Vol 61 (9) ◽  
pp. 926-931 ◽  
Author(s):  
M. L. Kozachenko ◽  
K. B. Savkin ◽  
N. P. Khatyrev

Author(s):  
K. N. Steshenko ◽  
D. D. Nikeev ◽  
A. Y. Kolomyschev ◽  
E. V. Gavrilov

The software model environment developed allows us to estimate the power characteristics of aircraft radiation at different observation angles. The method of implementation of this environment makes it possible to get results with an accuracy sufficient to determine the characteristics of the indicatrices of the aircraft under study. The high level of versatility of the model environment enables us to make calculations for any aircraft with different flight conditions in several spectral ranges


2011 ◽  
Vol 38 (4) ◽  
pp. 120-122 ◽  
Author(s):  
O. T. Loza ◽  
D. K. Ul’yanov ◽  
P. S. Strelkov ◽  
I. E. Ivanov ◽  
R. V. Baranov

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