Preprint Article Version 1 This version is not peer-reviewed

Nonturbulent troposphere of Supper Lorentz Gaussian Seed ‎Mathematically of Receiver Field and Intensity Fluctuation

Version 1 : Received: 27 June 2024 / Approved: 28 June 2024 / Online: 1 July 2024 (09:23:31 CEST)

How to cite: Khamees, H. T. Nonturbulent troposphere of Supper Lorentz Gaussian Seed ‎Mathematically of Receiver Field and Intensity Fluctuation. Preprints 2024, 2024070013. https://doi.org/10.20944/preprints202407.0013.v1 Khamees, H. T. Nonturbulent troposphere of Supper Lorentz Gaussian Seed ‎Mathematically of Receiver Field and Intensity Fluctuation. Preprints 2024, 2024070013. https://doi.org/10.20944/preprints202407.0013.v1

Abstract

In recent studies, the circulation of a (SLG) super-Lorentz-Gaussian beam in a non-turbulent ‎troposphere has been investigated and used for laser applications. This method uses the extended ‎Huygens-Fresnel integral technique and refers to the multiplication of the Gaussian beam by the ‎Lorentz function. Formulas are derived for the normal density and approximate field of the Lo-‎Rentz-Gaussian beam in a non-turbulent troposphere. The average density power and the propagation characteristics of the SLG jet in the non-turbulent troposphere are numerically represented. ‎The characteristics of the beam boundaries at atmospheric non-turbulence for the propagation ‎distance of an SLG beam in a non-turbulent troposphere are also discussed in detail. They are ‎practical in an optical communication system used in lasers.

Keywords

SLG; Nonturbulent troposphere; Huygens-Fresnel Integral; Intensity; Receiver Field

Subject

Engineering, Electrical and Electronic Engineering

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