Average Intensity of SLVGB for Slant Path Propagation in Atmospheric Turbulent

The physical meaning of propagation characteristics of an (SLVGB) Super Lorentz vortex Gauss beam in a turbulent atmosphere is studied and analyzed. To use the method of Huygens-Fresnel integral. Likewise, to apply the ITU-R turbulence structure constant model and calculate the mean intensity of SLVGB in slant path beam propagation with different speared distances, and then used a random phase screen method to analyzing the scintillation index and investigated the turbulent in receiver plane, furthermore, the impact of the source size, and beam order factors of an SLVGB beam are checked into atmospheric blustery. The distribution belongings of an SLVGB beam via atmospheric turbulence are arithmetically computed and investigated. Additionally, the Kolmogorov atmospheric turbulence power spectrum model is used to find the propagation distance of an SLVGB beam in the turbulent atmosphere. To sum up, to set a value of normalized intensity is increased gradually in the turbulent atmosphere and finally, this work is creating a new beam propagation and its epitomized original article.