2002
DOI: 10.1109/tcomm.2002.800829
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Free-space optical communication through atmospheric turbulence channels

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Cited by 1,274 publications
(93 citation statements)
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“…The GG distribution model is widely accepted for characterising the weak, moderate and strong turbulence conditions because results achieved match closely with experimental results [1,9,21]. The GG probability density function (pdf) is given as [1,2,6]   a mean value of 1, and in the turbulent free limit, this mean value is attained at all times. With a plane wave assumption at the receiver, the parameters  and  are defined as [2]     where  is the optical wavelength [2].…”
Section: Channel Statisticsmentioning
confidence: 62%
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“…The GG distribution model is widely accepted for characterising the weak, moderate and strong turbulence conditions because results achieved match closely with experimental results [1,9,21]. The GG probability density function (pdf) is given as [1,2,6]   a mean value of 1, and in the turbulent free limit, this mean value is attained at all times. With a plane wave assumption at the receiver, the parameters  and  are defined as [2]     where  is the optical wavelength [2].…”
Section: Channel Statisticsmentioning
confidence: 62%
“…(6) where the mean signal level at the sampling instant with OA input power . This emerges from the binary symmetric channel assumption and there is a corresponding formula for the threshold which would be almost optimal if the noise was truly Gaussian.…”
Section: Adaptive Decision Thresholdmentioning
confidence: 99%
“…Following the approach adopted in (Zhu and Kahn, 2002), the error probabilities of the DPSK modulated coherent system in the absence and presence of the turbulence channel is given as Eq. 31a-b:…”
Section: Resultsmentioning
confidence: 99%
“…The log-normal distribution is commonly used to model the weak turbulence condition and has been embraced in many calculations for the turbulence channel [28,29]. The distribution of the light intensity fading induced by weak turbulence can be described by log-normal distribution as where 2 is the scintillation index and for a weak turbulence regime is found to be proportional to Rytov variance 2 , which can be calculated as A plane wave model is used for starlight and other exoatmospheric sources while spherical wave model is used for a small-aperture source within or near the turbulent atmosphere.…”
Section: Log-normal Turbulence Modelmentioning
confidence: 99%
“…Figure 10 presents the predicted BER performance for a FSO link between Tx and Rx using Eqs. (29) and (32) for weak and strong turbulence conditions, respectively, and the simulated BER performance of TWR-FSO PNC in terms of ⁄ for a range of Rytov variance. In this model, the end-to-end link in TWR-FSO PNC was considered, where the RN performed PNC demapping on the superimposed received signal, which reduces the system complexity but at the cost of performance degradation at the destination nodes due to un-corrected errors at the RN.…”
Section: Btwr-fso Pnc Modelmentioning
confidence: 99%