Baykal, Yahya Kemal

Baykal, Yahya Kemal

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https://hdl.handle.net/20.500.12416/8884

Name Variants

Bayka, Yahya
Baykal, Yahya K.
Baykal, Yahya Kemal
Baykal, Yahya
Baykal, Y. K.
Baykal, Yahya Kemal
Baykal, Y
Baykal, Y.
Baykal, Yahya
Baykal, Yahya
Baykal, Yahya Kemal
Baykal, Yahya
Baykal, Yahya Kemal

Job Title

Prof. Dr.

Email Address

y.baykal@cankaya.edu.tr

Main Affiliation

06.03. Elektrik-Elektronik Mühendisliği
06. Mühendislik Fakültesi
01. Çankaya Üniversitesi
06.03. Elektrik-Elektronik Mühendisliği
Elektrik-Elektronik Mühendisliği
06. Mühendislik Fakültesi
01. Çankaya Üniversitesi

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Current Staff

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This researcher does not have a Scopus ID.

Documents

132

Citations

4310

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Scholarly Output

286

Articles

232

Views / Downloads

3014/45

Supervised MSc Theses

10

Supervised PhD Theses

0

WoS Citation Count

6259

Scopus Citation Count

6755

WoS h-index

44

Scopus h-index

46

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0

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0

WoS Citations per Publication

21.88

Scopus Citations per Publication

23.62

Open Access Source

16

Supervised Theses

10

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Journal	Count
Journal of the Optical Society of America A	35
Optics Communications	34
Applied Optics	23
Applied Physics B	20
Journal of Modern Optics	15

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Scholarly Output Search Results

Now showing 1 - 10 of 286

Citation - Scopus: 2
Effect of Partial Coherence on Miso Fso Systems
(Ieee, 2015) Baykal, Yahya; Uysal, Murat; Gokce, Muhsin Caner
Multiple-input single-output (MISO) techniques are employed in free space optical (FSO) systems to mitigate the degrading effects of atmospheric turbulence and therefore the link reliability is improved. In this paper, we consider an incoherent radial array beams and a finite sized slow detector for MISO FSO systems. We have derived the average power and power correlation formulas on the finite sized slow detector using the Huygens Fresnel principle in weak atmospheric turbulence. This helps us to find the system performance, such as power scintillation and aperture averaging factor. Effect of system parameters such as the source size, the ring radius, the degree of coherence, the link distance, the structure constant and the receiver aperture radius are analyzed on the performance of MISO FSO systems.
Su Altı Türbülanslı Ortamda Uyarlanabilir Optik Kullanarak Görüntü Düzeltmesi
(2025) Turan, Mehmet Furkan; Baykal, Yahya Kemal; Arpali, Çağlar
Optik haberleşme yöntemleri veri iletim hızından dolayı ve gecikmenin az olmasından dolayı önemli bir haberleşme yöntemidir. Optik haberleşme yöntemlerinden su altı optik haberleşme önemli bir haberleşme yöntemidir ancak su altı ortamında görüntüleme bozulmaktadır. Bu bozulmanın önemli nedenlerinden biri türbülanstır ve su altı haberleşmenin performansını etkilemektedir. Bu tezde, uyarlanabilir optik yöntemi ile su altı ortamında bozulan görüntülerin düzeltilmesi incelenmiştir. Bilinen ve yeni geliştirilen kaynak profillerinin kullanılarak tanımlanmasıyla rastgele optik ışınların yayılımı su altı ortamında incelenmiş ve ortalama yoğunlukları elde edilerek sunulmuştur. Su altı türbülanslı ortamda rastgele optik ışınlarının, alıcıdaki yoğunluğu bulunarak analiz edilmiştir. Rastgele optik ışınların kaynak alan profilleri kaynak alanının piksellere bölünmesi ve piksellere faz ve genlik bilgisinin eklenmesiyle elde edilmiştir. Işın yoğunluklarının su altı türbülanslı ortamda alıcı düzleminde dağılımları gösterilirken, bilinen Gauss ışını, satranç tahtası şeklinde olan rastgele ışınlar ve Çankaya Üniversitesi baş harflerinin kısaltmasından oluşan Ç.Ü. ışını gibi farklı ışın tipleri kullanılmıştır. Dalga boyu, bağlantı uzunluğu, ortalama kare sıcaklığın dağılma oranı, sıcaklık ve tuzluluğun kırılma indisi spektrumuna katkı oranı, sıvı birim kütlesi başına kinetik enerjinin dağılma oranı, iç ölçek, alıcı açıklık çapı ve kaynak boyutu gibi su altı türbülans parametrelerinin ışın şiddetine olan etkisi incelenmiştir. Optik ışınlarının su altı türbülansı sonucunda bozulan görüntülerinin düzeltilmesinde, uyarlanabilir optik düzeltmesinin piston, eğim ve astigmatizma bileşenleri kullanılmıştır. Türbülans sonucu oluşan bozulma, uyarlanabilir optik yöntemi kullanılarak ve kullanılmayarak etkinliği karşılaştırılmıştır. MATLAB programı kullanılarak hesaplamalar yapılmış ve grafikler elde edilmiştir. Su altı türbülansının neden olduğu görüntü bozulmasının düzeltilmesi için kalite ölçütü belirlenmiş ve düzeltme miktarı incelenerek, uyarlanabilir optik yardımıyla ne kadar görüntü düzeltmesi sağlandığı incelenmiştir. Bu tezde, uyarlanabilir optik düzeltme yöntemi ile su altı ortamında türbülansın neden olduğu görüntü bozulmasının etkisinin en aza indirilmesi amaçlanmıştır. Bu tezde yapılan çalışma, su altı optik görüntüleme sistemleri, su altı kablosuz optik haberleşme ve elektro optik sistemlerin su altı performanslarının artırılması gibi alanlarda kullanılabilir.
Citation - WoS: 24
Citation - Scopus: 23
Scintillation Index of Flat-Topped Gaussian Laser Beam in Strongly Turbulent Medium
(Optical Soc Amer, 2011) Gercekcioglu, Hamza; Baykal, Yahya
In a strongly turbulent medium, the scintillation index of flat-topped Gaussian beams is derived and evaluated. In the formulation, unified solution of Rytov method is utilized. Our results correctly reduce to the existing strong turbulence scintillation index of the Gaussian beam, and naturally to spherical and plane wave scintillations. Another checkpoint of our result is the scintillation index of flat-topped Gaussian beams in weak turbulence. Regardless of the order of flatness, scintillations of flat-topped Gaussian beams in strong turbulence are found to be determined mainly by the small-scale effects. For large-sized beams in moderate and strongly turbulent medium, flatter beams exhibit smaller scintillations. (C) 2011 Optical Society of America
Citation - WoS: 14
Citation - Scopus: 15
Intensity Correlations of General Type Beam in Weakly Turbulent Atmosphere
(Elsevier Sci Ltd, 2011) Baykal, Yahya
In weakly turbulent atmosphere, intensity correlations at the receiver plane are formulated for a general type optical beam. Evaluating our formula at the appropriate source parameters versus the diagonal distance, intensity correlations for cos Gaussian, cosh Gaussian, annular and flat-topped Gaussian beams are obtained. As compared to Gaussian beam, intensity correlations are found smaller for cos Gaussian and larger for cosh Gaussian beams. Intensity correlations of cos Gaussian, cosh Gaussian and flat-topped Gaussian beams become larger at large source sizes. Thicker annular beams and flatter flat-topped Gaussian beams show larger intensity correlations. Without generalizing, intensity correlations tend to increase when the link length and the structure constant decrease and the wavelength increases. Our results show that the intensity correlations are not only built up using random medium effects, but also using the diffraction pattern formed at the receiver plane for the specific incidence investigated. As a check point, for all source types and medium parameters, our evaluations indicate that intensity correlations approach zero at sufficiently large diagonal distances. (C) 2011 Elsevier Ltd. All rights reserved.
Citation - WoS: 50
Citation - Scopus: 55
Expressing Oceanic Turbulence Parameters by Atmospheric Turbulence Structure Constant
(Optical Soc Amer, 2016) Baykal, Yahya
The parameters composing oceanic turbulence are the wavelength, link length, rate of dissipation of kinetic energy per unit mass of fluid, rate of dissipation of mean-squared temperature, Kolmogorov microscale, and the ratio of temperature to salinity contributions to the refractive index spectrum. The required physical entities such as the average intensity and the scintillation index in the oceanic medium are formulated by using the power spectrum of oceanic turbulence, which is described by oceanic turbulence parameters. On the other hand, there exists a rich archive of formulations and results for the above-mentioned physical entities in atmospheric turbulence, where the parameters describing the turbulence are the wavelength, the link length, and the structure constant. In this paper, by equating the spherical wave scintillation index solutions in the oceanic and atmospheric turbulences, we have expressed the oceanic turbulence parameters by an equivalent structure constant used in turbulent atmosphere. Such equivalent structure constant will help ease reaching solutions of similar entities in an oceanic turbulent medium by employing the corresponding existing solutions, which are valid in an atmospheric turbulent medium. (C) 2016 Optical Society of America
Citation - WoS: 21
Citation - Scopus: 27
Scintillations of Led Sources in Oceanic Turbulence
(Optical Soc Amer, 2016) Baykal, Yahya
The scintillation index of light emitting diode (LED) sources is evaluated when such sources are employed in oceanic wireless optical communication (UWOC) links. In the formulation, LED source radiation is taken to be perfectly incoherent with a Gaussian field distribution. We have utilized the scintillation index solution of an incoherent source in atmospheric turbulence, together with our recently obtained expression that expresses the structure constant of atmospheric turbulence in terms of the oceanic turbulence and UWOC link parameters. Oceanic turbulence parameters of interest are the ratio of temperature to salinity contributions to the refractive index spectrum, rate of dissipation of kinetic energy per unit mass of fluid, rate of dissipation of mean-squared temperature, and viscosity. UWOC link parameters are the LED source size, link length, and the wavelength. Scintillation index results are presented for various variations of the oceanic turbulence and UWOC link parameters. (C) 2016 Optical Society of America
Citation - WoS: 5
Citation - Scopus: 6
Propagation of Optical Flat-Topped Gaussian Beams in Satellite Links
(Ieee, 2009) Kamacioglu, Canan; Arpali, Serap A.; Baykal, Yahya; Yazgan, Erdem
Propagation of optical flat-topped Gaussian beams in earth-satellite optical communication links is investigated where part of the link is turbulent atmosphere. Flat-topped Gaussian source field is obtained by superposing many Gaussian beams of different source size. Starting with the flat-topped Gaussian incidence at the earth surface, the average intensity at the satellite is formulated by using the extended Huygens Fresnel principle. For the structure constant variation versus height, Hufnagel-Valley model is employed in the vertical and slant paths. The received average intensity is numerically calculated and the effects of the source and medium parameters on the received average intensity profile are examined for different zenith angles. In earth-satellite optical communications links, the advantages of using flat-topped Gaussian beams as compared to Gaussian beams are scrutinized.
Citation - WoS: 69
Citation - Scopus: 74
Equivalence of Structure Constants in Non-Kolmogorov and Kolmogorov Spectra
(Optical Soc Amer, 2011) Baykal, Yahya; Gercekcioglu, Hamza
We find the equivalence of the structure constants in non-Kolmogorov and Kolmogorov spectra in a turbulent atmosphere. As the reference point, the spherical wave scintillation index in a non-Kolmogorov medium is used. Relations of the structure constants are found to be functions of the power law of the turbulence spectrum and the Fresnel zone. It will be useful to employ the equivalence of the structure constants in making performance comparisons found with non-Kolmogorov and Kolmogorov spectra. (C) 2011 Optical Society of America
Citation - WoS: 1
Citation - Scopus: 1
Speckle Contrast for Flat-Topped Field Profiles
(Elsevier Sci Ltd, 2013) Baykal, Yahya
Speckle contrast is evaluated for flat-topped field profiles where the characterization and evaluation of speckle contrast are based on mathematical formulation and theoretical parameter variation. The speckle field which is represented by the random phase shift and the random phase tilt is multiplied by the flat-topped shaped field. The increase in the source size of the flat-topped field first causes the speckle contrast to increase, then reaches saturation. Increase in the variance of the phase shift of a flat-topped field causes an appreciable increase in the speckle contrast. Depending on the diffraction characteristics of the finite sized flat-topped field distribution, upon changing the variance of the phase shift, the speckle contrast exhibits different behavior at short and long propagation distances. However, especially for small variances of phase tilts, the speckle contrast seems to monotonically increase as the propagation distance becomes larger. The effect of the order of flatness on the speckle contrast is small at short propagation distances which can be appreciable at long propagation distances. (C) 2012 Elsevier Ltd. All rights reserved.
Citation - WoS: 3
Citation - Scopus: 3
Laser Beam Scintillations of Lidar Operating in Weak Oceanic Turbulence
(Optica Publishing Group, 2022) Baykal, Yahya; Gercekcioglu, Hamza
The formulation of light detection and ranging (LIDAR) systems is derived and examined for the scintillation index, evaluated on-axis, of laser beams in horizontal links in the ocean with weak turbulence by utilizing the Rytov method. These scintillation indices, obtained for the Gaussian beam which is collimated, the limits of plane and spherical waves, are depicted versus the source size, target size, and parameter of the normalized reflector size. It is found that the source size, target size, and normalized reflector size parameter, lessening the scintilla-tion index evaluated on-axis, are approximately 0.44 cm, 56 x 10-4 cm, and 2.2, respectively. Additionally, by using these values that minimize the scintillation index, the variation of the scintillations is shown against the propagation distance, radius of reflector, temperature and salinity fluctuation effects, mean squared temperature, and turbulent kinetic energy dissipation rate per unit mass of fluid at various selected source size and radius of reflector values. (c) 2022 Optica Publishing Group

Baykal, Yahya Kemal

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8

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