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

Super Lorentz vortex Gaussian beam (SLVGB) is propagated via the turbulent atmosphere parameters. The benefit key of SLVGB wave model that unlimited bandwidth and a spherical are involved. Additionally, Huygens Fresnel integral was used for schoolwork to study propagation in slant direction moderate medium. On other hand, applying crude international telecommunication union (ITU-R) possible. Moreover, Kolmogorov power spectrum applied, source field dispersed by zenith angle receiver plane. examine contour intensity. To investigate various parameters such as size, mode, scintillation index, topological charge, others associated with super entirely understood, outcomes were examined, obtained references build path turbulent; form constants especially comparison matching. Our graphical findings indicate happened randomly index intensity SLVGB, resulting novel technical configuration. summarize, this article advantageous remote sensing uses an optical communications system laser applications.