Scintillation index of a multi-Gaussian Schell-model beam in turbulent atmosphere
dc.authorid | Chen, Yahong/0000-0003-3258-8032 | |
dc.authorscopusid | 55474912600 | |
dc.authorscopusid | 45961232200 | |
dc.authorscopusid | 56188482100 | |
dc.authorscopusid | 55312406900 | |
dc.authorscopusid | 7401750425 | |
dc.authorscopusid | 7201534947 | |
dc.authorscopusid | 7201534947 | |
dc.authorwosid | Cai, Yangjian/E-9745-2012 | |
dc.authorwosid | Chen, Yahong/Aag-8122-2021 | |
dc.authorwosid | Liu, Xianlong/Aid-2781-2022 | |
dc.contributor.author | Yuan, Yangsheng | |
dc.contributor.author | Liu, Xianlong | |
dc.contributor.author | Wang, Fei | |
dc.contributor.author | Chen, Yahong | |
dc.contributor.author | Cai, Yangjian | |
dc.contributor.author | Qu, Jun | |
dc.contributor.author | Eyyuboglu, Halil T. | |
dc.contributor.authorID | 7688 | tr_TR |
dc.contributor.other | Elektronik ve Haberleşme Mühendisliği | |
dc.date.accessioned | 2017-03-02T10:54:28Z | |
dc.date.available | 2017-03-02T10:54:28Z | |
dc.date.issued | 2013 | |
dc.department | Çankaya University | en_US |
dc.department-temp | [Yuan, Yangsheng; Qu, Jun] Anhui Normal Univ, Dept Phys, Wuhu 241000, Peoples R China; [Yuan, Yangsheng; Liu, Xianlong; Wang, Fei; Chen, Yahong; Cai, Yangjian] Soochow Univ, Sch Phys Sci & Technol, Suzhou 215006, Peoples R China; [Eyyuboglu, Halil T.] Cankaya Univ, Dept Elect & Commun Engn, TR-06530 Bulger Ankara, Turkey | en_US |
dc.description | Chen, Yahong/0000-0003-3258-8032 | en_US |
dc.description.abstract | Multi-Gaussian Schell-model (MGSM) beam was introduced recently [Sahin and Korotkova, Opt. Lett. 37 (2012) 2970; Korotkova et al., J. Opt. Soc. Am. A 29 (2012) 2159]. In this paper, an explicit expression for the scintillation index of a multi-Gaussian Schell-model (MGSM) beam in weakly or extremely strong turbulent atmosphere is derived with the help of a tensor method. Applying the derived formulae, the scintillation properties of a MGSM beam and a GSM beam in weakly or extremely strong turbulent atmosphere are studied numerically and comparatively. Our results show that a MGSM beam has advantage over a GSM beam for reducing turbulence-induced scintillation, which will be useful for long-distance free-space optical communications. (C) 2013 Elsevier B.V. All rights reserved. | en_US |
dc.description.publishedMonth | 9 | |
dc.description.sponsorship | National Natural Science Foundation of China [11274005, 11104195]; Huo Ying Dong Education Foundation of China [121009]; Key Project of Chinese Ministry of Education [210081]; Priority Academic Program Development of Jiangsu Higher Education Institutions; Universities Natural Science Research Project of Jiangsu Province [11KJB140007]; Innovation Plan for Graduate Students in the Universities of Jiangsu Province [CXZZ11_0088]; National College Students Innovation Experiment Program [111028510]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry | en_US |
dc.description.sponsorship | This work was supported by the National Natural Science Foundation of China under Grant nos. 11274005 and 11104195, the Huo Ying Dong Education Foundation of China under Grant no. 121009, the Key Project of Chinese Ministry of Education under Grant no. 210081, the Project Funded by the Priority Academic Program Development of Jiangsu Higher Education Institutions, the Universities Natural Science Research Project of Jiangsu Province under grant 11KJB140007, the Innovation Plan for Graduate Students in the Universities of Jiangsu Province under Grant no. CXZZ11_0088, the National College Students Innovation Experiment Program under Grant no. 111028510, and the Project Sponsored by the Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry. | en_US |
dc.description.woscitationindex | Science Citation Index Expanded | |
dc.identifier.citation | Yuan, Y...et al. (2013). Scintillation index of a multi-Gaussian Schell-model beam in turbulent atmosphere. Optics Communications, 305, 57-65. http://dx.doi.org/10.1016/j.optcom.2013.04.076 | en_US |
dc.identifier.doi | 10.1016/j.optcom.2013.04.076 | |
dc.identifier.endpage | 65 | en_US |
dc.identifier.issn | 0030-4018 | |
dc.identifier.issn | 1873-0310 | |
dc.identifier.scopus | 2-s2.0-84878552113 | |
dc.identifier.scopusquality | Q2 | |
dc.identifier.startpage | 57 | en_US |
dc.identifier.uri | https://doi.org/10.1016/j.optcom.2013.04.076 | |
dc.identifier.volume | 305 | en_US |
dc.identifier.wos | WOS:000328524900011 | |
dc.identifier.wosquality | Q3 | |
dc.institutionauthor | Eyyuboğlu, Halil Tanyer | |
dc.language.iso | en | en_US |
dc.publisher | Elsevier | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/closedAccess | en_US |
dc.scopus.citedbyCount | 93 | |
dc.subject | Multi-Gaussian Schell-Model Beam | en_US |
dc.subject | Turbulent Atmosphere | en_US |
dc.subject | Scintillation | en_US |
dc.title | Scintillation index of a multi-Gaussian Schell-model beam in turbulent atmosphere | tr_TR |
dc.title | Scintillation Index of a Multi-Gaussian Schell-Model Beam in Turbulent Atmosphere | en_US |
dc.type | Article | en_US |
dc.wos.citedbyCount | 86 | |
dspace.entity.type | Publication | |
relation.isAuthorOfPublication | 71977731-6d7b-42a5-81b1-f2681bf655b6 | |
relation.isAuthorOfPublication.latestForDiscovery | 71977731-6d7b-42a5-81b1-f2681bf655b6 | |
relation.isOrgUnitOfPublication | 3f3f4ac0-1357-4a67-a7c4-465451ea38db | |
relation.isOrgUnitOfPublication.latestForDiscovery | 3f3f4ac0-1357-4a67-a7c4-465451ea38db |
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