Numerical simulation for echo characteristics of laser beams reflected by retro-reflectors in atmospheric turbulence

Optik ◽  
2019 ◽  
Vol 179 ◽  
pp. 244-251 ◽  
Author(s):  
Ya-Qing Li ◽  
Li-Guo Wang ◽  
Zhen-Sen Wu
2020 ◽  
Vol 44 (1) ◽  
pp. 53-59
Author(s):  
S.N. Khonina ◽  
S.G. Volotovskiy ◽  
M.S. Kirilenko

It is proposed to use the random field generation in the numerical simulation of the propagation of radiation through a random medium using method based on the Karhunen–Loeve expansion with various types of correlation operators to describe turbulence simulators. The properties of the calculated simulators of a random medium with a Gaussian correlation function were investigated in modeling the propagation of Laguerre-Gaussian vortex beams. The simulation results showed that an increase in the order of the optical vortex leads, as in the experiment, to lower stability of the phase singularity of the beams to random optical fluctuations. The similarity of the simulation results and the optical experiments indicates the promise of the proposed approach for the synthesis of random environment simulators.


Photonics ◽  
2021 ◽  
Vol 8 (10) ◽  
pp. 445
Author(s):  
Alexey A. Kovalev ◽  
Victor V. Kotlyar ◽  
Anton G. Nalimov

It is well known that the orbital angular momentum (OAM) of a light field is conserved on propagation. In this work, in contrast to the OAM, we analytically study conservation of the topological charge (TC), which is often confused with OAM, but has quite different physical meaning. To this end, we propose a huge-ring approximation of the Huygens–Fresnel principle, when the observation point is located on an infinite-radius ring. Based on this approximation, our proof of TC conservation reveals that there exist other quantities that are also propagation-invariant, and the number of these invariants is theoretically infinite. Numerical simulation confirms the conservation of two such invariants for two light fields. The results of this work can find applications in optical data transmission to identify optical signals.


2001 ◽  
Vol 24 (3) ◽  
pp. 230-230
Author(s):  
Lyes Lakhal

Diameter measurements performed with the solar astrolabe are affected by atmospheric effects. In order to deduce significant astrophysical results, it is necessary to know how these effects contribute to the error of diameter measurement. For this purpose, a numerical simulation was developed leading to a law of error behaviour with observing conditions. In order to validate these results, recorded data obtained at the Calern observatory astrolabe (France) during the period 1996 – 1997 are used. A good agreement is observed with the simulation, which permit salso to give access to daily atmospheric time constants. (Co-author is A. Irbah, Algeria.)


2017 ◽  
Vol 30 (2) ◽  
pp. 191-197
Author(s):  
V. A. Bogachev ◽  
S. G. Garanin ◽  
F. A. Starikov ◽  
R. A. Shnyagin

2019 ◽  
Vol 26 (2) ◽  
pp. 022902 ◽  
Author(s):  
Y. Lu ◽  
P. Tzeferacos ◽  
E. Liang ◽  
R. K. Follett ◽  
L. Gao ◽  
...  

2012 ◽  
Vol 59 (13) ◽  
pp. 1168-1179 ◽  
Author(s):  
Xiaoqing Li ◽  
Xiaoling Ji ◽  
Wenyue Zhu

2013 ◽  
Vol 31 (3) ◽  
pp. 403-410 ◽  
Author(s):  
Ashutosh Sharma ◽  
Mahendra Singh Sodha ◽  
Shikha Misra ◽  
S.K. Mishra

AbstractIn this paper, the authors have presented a paraxial theory for propagation of (1) Gaussian (2) dark hollow Gaussian high power laser beams in the atmosphere, considering the nonlinearity arising from the temperature variation along the wave-front. Specifically, the focusing parameter for both beams has been evaluated as a function of distance and initial beam power and width (corresponding to radiation of wavelengths 1.045 µ, 1.625 µ, and 2.141 µ in the water absorption window) for the maritime, desert, rural, and urban environments as modeled at NRL; the results have been presented in the dimensionless form. It is seen that in all four environments a dark hollow beam defocuses less than the corresponding Gaussian beam of same radius and power. It is suggested that this conclusion based on the paraxial theory be verified by numerical simulation.


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