2017
DOI: 10.1016/j.ijleo.2017.03.009
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On the BER performance of FSO links with multiple receivers and spatial jitter over gamma-gamma or exponential turbulence channels

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Cited by 33 publications
(24 citation statements)
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“…The total simultaneous influence of the chromatic dispersion, time jitter and water turbulence effects on the performance of the UOWC link can be estimated, from (3) and (14), through the extraction of the corresponding joint PDF as [37,54,55]:…”
Section: The Joint Influence Of Gvd Time Jitter and Turbulencementioning
confidence: 99%
“…The total simultaneous influence of the chromatic dispersion, time jitter and water turbulence effects on the performance of the UOWC link can be estimated, from (3) and (14), through the extraction of the corresponding joint PDF as [37,54,55]:…”
Section: The Joint Influence Of Gvd Time Jitter and Turbulencementioning
confidence: 99%
“…denotes the Meijer function, (Equation (5) in [32]) that is a standard built in function which can be evaluated with most of the well known mathematical software packages and can be transformed to the familiar hypergeometric functions [32]. Similarly, for saturated turbulence conditions, by using (5), Equation (11) in [32] and by following the same analysis performed in [7], we obtain that (9) can be written according to [33], as…”
Section: Joint Turbulence and Pointing Errors Effectsmentioning
confidence: 99%
“…where P denotes the average signal power at the receiver's side and E[I {i,j} ] is the corresponding expected normalized irradiance value, [15,17,22] which for both G-G and NE turbulence distributions is given according to [33][34][35], as:…”
Section: Joint Turbulence and Pointing Errors Effectsmentioning
confidence: 99%
“…Many statistical distribution models have been proposed for the description of the intensity fluctuations which arise from the scintillation effect. Each properly describes the scintillation effect caused by different turbulence strength, i.e., weak, moderate or strong, [12,[14][15][16][17]. More precisely, lognormal and gamma statistical distributions are useful for describing the scintillations caused by weak turbulence, while GG, Malaga (M) and I-K are commonly used for a range from weak to strong turbulence conditions; finally, K and NE are suitable for strong and saturated conditions, respectively, [11,12,14,[18][19][20][21][22][23][24][25][26][27][28][29][30].…”
Section: Introductionmentioning
confidence: 99%