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Strong turbulence analysis of sinusoidal and hyperbolic Gaussian beams

dc.contributor.authorEyyüboğlu, Halil Tanyer
dc.contributor.authorID7688tr_TR
dc.date.accessioned2023-01-16T07:54:06Z
dc.date.available2023-01-16T07:54:06Z
dc.date.issued2010
dc.departmentÇankaya Üniversitesi, Mühendislik Fakültesi, Elektrik Elektronik Mühendisliği Bölümüen_US
dc.description.abstractWe formulate the on-axis asymptotic scintillations of sinusoidal and hyperbolic Gaussian beams, namely cos and cosh Gaussian beam, under strong turbulence conditions. Our results are displayed in the form of plots of the scintillation index against propagation distance and wavelength at several source and propagation parameters. It is revealed that at small source sizes, cosh Gaussian beams will exhibit the lowest scintillations, but at large source sizes, this will reverse and cos Gaussian beams will attain such characteristics. It is further found that in strong turbulence, longer wavelengths will offer less scintillations, a behavior similar to the one, encountered in weak scintillation conditions.en_US
dc.identifier.citationEyyüboğlu, Halil Tanyer (2010). "Strong turbulence analysis of sinusoidal and hyperbolic Gaussian beams", Conference Proceedings - 5th International Conference on Advanced Optoelectronics and Lasers, CAOL' 2010, 10 September 2010through 14 September 2010, pp. 15-17.en_US
dc.identifier.doi10.1109/CAOL.2010.5634277
dc.identifier.endpage17en_US
dc.identifier.isbn9781424470464
dc.identifier.startpage15en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12416/6064
dc.language.isoenen_US
dc.relation.ispartofConference Proceedings - 5th International Conference on Advanced Optoelectronics and Lasers, CAOL' 2010en_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleStrong turbulence analysis of sinusoidal and hyperbolic Gaussian beamstr_TR
dc.titleStrong Turbulence Analysis of Sinusoidal and Hyperbolic Gaussian Beamsen_US
dc.typeConference Objecten_US
dspace.entity.typePublication

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