Scintillation Index of Higher-Order Cos-Gaussian, Cosh-Gaussian and Annular Beams
| dc.contributor.author | Arpali, Serap Altay | |
| dc.contributor.author | Eyyuboglu, Halil T. | |
| dc.contributor.author | Baykal, Yahya | |
| dc.contributor.authorID | 51304 | tr_TR |
| dc.contributor.authorID | 7688 | tr_TR |
| dc.contributor.authorID | 7812 | tr_TR |
| dc.contributor.other | 06.02. Elektronik ve Haberleşme Mühendisliği | |
| dc.contributor.other | 06.03. Elektrik-Elektronik Mühendisliği | |
| dc.contributor.other | 06. Mühendislik Fakültesi | |
| dc.contributor.other | 01. Çankaya Üniversitesi | |
| dc.date.accessioned | 2020-04-07T10:41:07Z | |
| dc.date.accessioned | 2025-09-18T14:08:48Z | |
| dc.date.available | 2020-04-07T10:41:07Z | |
| dc.date.available | 2025-09-18T14:08:48Z | |
| dc.date.issued | 2008 | |
| dc.description.abstract | In this paper, via the generalized beam formulation, we evaluate the scintillation index for higher-order general beams propagating through the weak atmospheric turbulence. The investigated higher-order beam types are cos-Gaussian, cosh-Gaussian and annular beams. The scintillation indices of these beams are plotted with respect to propagation length, source size and order of the beam. According to our graphical outputs, higher-order beams have less on-axis scintillation index than zero-order beams at longer propagation distances. The on-axis scintillation exhibits a slight increase when the order of even-ordered beams is made higher. Moreover, our study on the source size variation shows that, for most of the source size range, cos-Gaussian beams have a lower scintillation index than the other beams. | en_US |
| dc.identifier.citation | Arpali, Serap Altay; Eyyuboğlu, Halil Tanyer; Baykal, Yahya, "Scintillation index of higher-order cos-Gaussian, cosh-Gaussian and annular beams" Journal Of Modern Optics, Vol.55, No.2, pp.227-239, (2008). | en_US |
| dc.identifier.doi | 10.1080/09500340701374221 | |
| dc.identifier.issn | 0950-0340 | |
| dc.identifier.scopus | 2-s2.0-36949002286 | |
| dc.identifier.uri | https://doi.org/10.1080/09500340701374221 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12416/13215 | |
| dc.language.iso | en | en_US |
| dc.publisher | Taylor & Francis Ltd | en_US |
| dc.rights | info:eu-repo/semantics/closedAccess | en_US |
| dc.subject | Scintillation Index | en_US |
| dc.subject | Turbulence | en_US |
| dc.subject | Higher-Order Beams | en_US |
| dc.subject | Gaussian Beam | en_US |
| dc.subject | Cosh-Gaussian Beam | en_US |
| dc.subject | Annular Beam Vs Beam Propagation | en_US |
| dc.title | Scintillation Index of Higher-Order Cos-Gaussian, Cosh-Gaussian and Annular Beams | en_US |
| dc.title | Scintillation index of higher-order cos-Gaussian, cosh-Gaussian and annular beams | tr_TR |
| dc.type | Article | en_US |
| dspace.entity.type | Publication | |
| gdc.author.institutional | Arpali, Serap | |
| gdc.author.institutional | Eyyuboğlu, Halil Tanyer | |
| gdc.author.institutional | Baykal, Yahya Kemal | |
| gdc.author.scopusid | 14826627400 | |
| gdc.author.scopusid | 35614168400 | |
| gdc.author.scopusid | 7004576489 | |
| gdc.description.department | Çankaya University | en_US |
| gdc.description.departmenttemp | Cankaya Univ, Elect & Commun Engn Dept, TR-06530 Balgat Ankara, Turkey | en_US |
| gdc.description.endpage | 239 | en_US |
| gdc.description.issue | 2 | en_US |
| gdc.description.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
| gdc.description.scopusquality | Q3 | |
| gdc.description.startpage | 227 | en_US |
| gdc.description.volume | 55 | en_US |
| gdc.description.woscitationindex | Science Citation Index Expanded | |
| gdc.description.wosquality | Q4 | |
| gdc.identifier.openalex | W1968630853 | |
| gdc.identifier.wos | WOS:000251515300002 | |
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| gdc.openalex.normalizedpercentile | 0.94 | |
| gdc.openalex.toppercent | TOP 10% | |
| gdc.opencitations.count | 45 | |
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