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Analysis of wave structure functions

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dc.contributor.author Eyyuboğlu, Halil T.
dc.date.accessioned 2020-04-07T11:23:07Z
dc.date.available 2020-04-07T11:23:07Z
dc.date.issued 2008
dc.identifier.citation Eyyuboğlu, Halil Tanyer, 'Analysis of wave structure functions' LFNM 2008: Proceedings Of The 9th International Conference On Laser And Fiber-Optical Network Modeling, pp.107-109, (2008). tr_TR
dc.identifier.isbn 978-1-4244-2526-6
dc.identifier.uri http://hdl.handle.net/20.500.12416/2951
dc.description.abstract Wave structure function (WSF) of spherical wave is used in extended Huygens-Fresnel integral to induce the effect of turbulent atmosphere on the propagating laser beam. Depending on the approximation made and the choice of the spatial power spectral density of refractive index fluctuation function, different forms of WSFs become available. In this study, five different WSFs are numerically evaluated for pure Gaussian, cosh-Gaussian, sinh-Gaussian, cos-Gaussian and sine-Gaussian types of source plane beams. In the range of adapted source and propagation parameters, namely under weak fluctuation conditions, no substantial deviations are found to occur with respect to the WSF selection. Our results are offered in terms of graphical illustrations showing the differences in the receiver intensity profiles against the varying propagation distance. tr_TR
dc.language.iso eng tr_TR
dc.publisher IEEE tr_TR
dc.relation.isversionof 10.1109/LFNM.2008.4670354 tr_TR
dc.rights info:eu-repo/semantics/closedAccess tr_TR
dc.subject Laser Beam Propagation tr_TR
dc.subject Turbulence tr_TR
dc.title Analysis of wave structure functions tr_TR
dc.type workingPaper tr_TR
dc.relation.journal LFNM 2008: Proceedings Of The 9th International Conference On Laser And Fiber-Optical Network Modeling tr_TR
dc.contributor.authorID 7688 tr_TR
dc.identifier.startpage 107 tr_TR
dc.identifier.endpage 109 tr_TR
dc.contributor.department Çankaya Üniversitesi, Mühendislik Fakültesi, Elektronik ve Haberleşme Mühendisliği Bölümü tr_TR


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