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Intensity Correlations of General Type Beam in Weakly Turbulent Atmosphere

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Date

2011

Journal Title

Journal ISSN

Volume Title

Publisher

Elsevier Sci Ltd

Open Access Color

Green Open Access

No

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Abstract

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.

Description

Keywords

Intensity Correlations, Weakly Turbulent Atmosphere, General Type Beam

Fields of Science

0103 physical sciences, 01 natural sciences, 0104 chemical sciences

Citation

Baykal, Y. (2011). Intensity correlations of general type beam in weakly turbulent atmosphere. Optics and Laser Technology, 43(7), 1237-1242. http://dx.doi.org/10.1016/j.optlastec.2011.03.016

WoS Q

Q1

Scopus Q

Q1
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OpenCitations Citation Count
12

Source

Optics & Laser Technology

Volume

43

Issue

7

Start Page

1237

End Page

1242
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CrossRef : 10

Scopus : 15

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Mendeley Readers : 2

SCOPUS™ Citations

15

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Web of Science™ Citations

14

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Page Views

5

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1.41889443

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