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Scintillation behavior of Laguerre Gaussian beams in strong turbulence

dc.authoridFalits, Andrey/0000-0003-1417-8080
dc.authorscopusid35614168400
dc.authorscopusid7004576489
dc.authorscopusid6507260332
dc.authorwosidFalits, Andrey/Jkj-4949-2023
dc.contributor.authorEyyuboglu, H. T.
dc.contributor.authorBaykal, Y.
dc.contributor.authorFalits, A.
dc.contributor.authorID7688tr_TR
dc.contributor.authorID7812tr_TR
dc.date.accessioned2016-08-11T13:18:20Z
dc.date.available2016-08-11T13:18:20Z
dc.date.issued2011
dc.departmentÇankaya Universityen_US
dc.department-temp[Eyyuboglu, H. T.; Baykal, Y.] Cankaya Univ, Dept Elect & Commun Engn, TR-06530 Ankara, Turkey; [Falits, A.] Zuev Inst Atmospher Opt, Tomsk, Russiaen_US
dc.descriptionFalits, Andrey/0000-0003-1417-8080en_US
dc.description.abstractIn strong atmospheric turbulence, the asymptotic on-axis scintillation behaviors of Laguerre Gaussian (LG) beams are examined. To arrive at the strong-turbulence solution, we utilize the existing filtering approach for weak-turbulence solutions and our recently reported weak-turbulence scintillation index formula for LG beams. In the limiting case, our solution correctly predicts the asymptotic strong-turbulence behavior of Gaussian beam wave scintillation. Investigation of the scintillations versus the propagation distance, source size, wavelength and refractive index structure parameter lead to the conclusion that the LG beams with higher order radial modes can provide less scintillation. The results are applicable to long-haul atmospheric optical communication links.en_US
dc.description.publishedMonth9
dc.description.sponsorshipScientific and Technological Research Council of Turkey (Tubitak); Russian Foundation for Basic Research (RFBR)en_US
dc.description.sponsorshipThis study was performed within the framework of the joint research project between The Scientific and Technological Research Council of Turkey (Tubitak) and The Russian Foundation for Basic Research (RFBR) entitled, "Effects of source beam types on optical wave propagation in turbulent atmosphere". The authors would like to express their gratitude to Tubitak and RFBR and the hosting institutions, Cankaya University and Zuev Institute of Atmospheric Optics (IAO SB RAS). We would also like to thank Dr. Emre Sermutlu for the original design and the revision of the double quadruple routine that was used in the numeric evaluation of (6).en_US
dc.description.woscitationindexScience Citation Index Expanded
dc.identifier.citationEyyuboğlu, H.T., Baykal, Y., Falits, A. (2011). Scintillation behavior of Laguerre Gaussian beams in strong turbulence. Applied Physisc B-Lasers And Optics, 104(4), 1001-1006. http://dx.doi.org/10.1007/s00340-011-4588-yen_US
dc.identifier.doi10.1007/s00340-011-4588-y
dc.identifier.endpage1006en_US
dc.identifier.issn0946-2171
dc.identifier.issn1432-0649
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-80053569004
dc.identifier.scopusqualityQ2
dc.identifier.startpage1001en_US
dc.identifier.urihttps://doi.org/10.1007/s00340-011-4588-y
dc.identifier.volume104en_US
dc.identifier.wosWOS:000295611800038
dc.identifier.wosqualityQ3
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleScintillation behavior of Laguerre Gaussian beams in strong turbulencetr_TR
dc.titleScintillation Behavior of Laguerre Gaussian Beams in Strong Turbulenceen_US
dc.typeArticleen_US
dspace.entity.typePublication

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