TELKOMNIKA Telecommunication Computing Electronics and Control
An evaluation of scintillation index in atmospheric turbulent for new super Lorentz vortex Gaussian beam

TELKOMNIKA Telecommunication Computing Electronics and Control
An evaluation of scintillation index in atmospheric turbulent for new super Lorentz vortex Gaussian beam

Contour
ITU-R model
Kolmogorov
Scintillation
SLVGB
Topological charge
Turbulent

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

Hussein Thary Khamees, Ahmed Saad Hussein, Nadhir Ibrahim Abdulkhaleq

http://telkomnika.uad.ac.id

Nov 02, 2022

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