A receiver intensity for Super Lorentz Gaussian beam (SLG) propagation via the moderate turbulent atmosphere using a novelty mathematical model

Abstract

First of all, the beam propagation of Super Lorentz Gaussian (SLG) profile is propagated via space, the recent research dealt extensively with the investigation of the propagation of SLG in a level of specified atmospheric. In a turbulent atmosphere of intensity and receiver field, models were derived from a new mathematical expression of intensity and analyzed. Also, to find the power scintillation indicators for the SLG beam in a random turbulence of receiver plane. The equations are obtained for the average receiver-aperture. The new beam of SLG systems generated a modified model when compared with the receiver-aperture averaging. When we revisions the parameters, firstly is started the factor source size, this affected the profile for the power propagation and the analysis proved that the average of the aperture is affected by increasing the distance of propagation length. The enhancement of the average power of the aperture effect reliably with the source size of the initial beam source depends on several factors, including the structure constant, the beam order and static value of source size. Finally, the target of this article is detected a novel of mathematical expression of the receiver intensity is applied in the system of optical communications.

Propagation of Vortex Gaussian Beam in Atmospheric Blustery and Evaluation of the BER for Laser gradient Launching

“…Besides, Eqs. (1,3,7). Our contemporary starts are verified, and evaluations are terminated using the current setting of the topologic charge records at M =1, 2, 3, 4 also the number of repetitions is 100, the wavelength setting is 1.35 μ m, also, the size of the source used it is 2 cm.…”

“…In this case, scattering waves from above Earth's atmosphere, and the oscillation of the horizontal wave is likely to rise mainly as expected in ref. [1].…”

An evaluation of scintillation index in atmospheric turbulent for new super Lorentz vortex Gaussian beam

“…The elevation plane ℎ = 5 km. Moreover, the SLVGB is used to characterize the elements that influence beam order (00, 10,21,22,33). While the factors of SLVGB are divided into two parts, the middle of the part Gaussian is more diverse than the source sizes of the super Lorentz part.…”

“…The Lorentz-Gauss beam model is the best compared with the original beam for designing a laser of the photodetector [19]. Super Lorentz beam [20], therefore a super Lorentz Gaussian beam is produced solid atmospheric turbulence, and it's evaluated in higher-order mode [21]. Without turbulence, the Lorentz-Gauss beam is propagated in a vacuum [22].…”

“…2 ) (9) in [7], [20], [21] explains how to describe the on-axis of the SLVGB scintillation index in a gradient route explosive environment.…”