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Proceedings Paper

Modeling of laser beam propagation through turbulent medium
Author(s): Evgeni N. Terentiev; Fedor V. Shugaev; Ludmila S. Shtemenko; Olga I. Dokukina; Oksana A. Ignateva
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Paper Abstract

There are well known factors which provoke image distortions during the propagation of light in the atmosphere. We used the solution of the linear unsteady 3D Navier - Stokes equations in order to model turbulent fluctuations of the refractive index. Parabolic equation method has been used for the solution of the problem of laser propagation. Density distribution and structure function were determined as well as their temporal evolution. Distortions of the Gaussian beam due to the fluctuations of the refractive index are presented.

Paper Details

Date Published: 25 May 2005
PDF: 12 pages
Proc. SPIE 5793, Atmospheric Propagation II, (25 May 2005); doi: 10.1117/12.603598
Show Author Affiliations
Evgeni N. Terentiev, M.V. Lomonosov Moscow State Univ. (Russia)
Fedor V. Shugaev, M.V. Lomonosov Moscow State Univ. (Russia)
Ludmila S. Shtemenko, M.V. Lomonosov Moscow State Univ. (Russia)
Olga I. Dokukina, M.V. Lomonosov Moscow State Univ. (Russia)
Oksana A. Ignateva, M.V. Lomonosov Moscow State Univ. (Russia)


Published in SPIE Proceedings Vol. 5793:
Atmospheric Propagation II
Cynthia Y. Young; G. Charmaine Gilbreath, Editor(s)

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