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.