2017
DOI: 10.1364/jocn.9.000498
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BER Performance of an Optically Pre-amplified FSO System Under Turbulence and Pointing Errors With ASE Noise

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Cited by 60 publications
(30 citation statements)
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“…The analytical results for the considered system with EDFA are obtained for parameters M 1 = 2, E = 4 and y th = 0.5. Note that, in this paper we utilize the same set of parameters for EDFA that were used and validated in [20], [25]. Further, the choice of the AT parameter α i for non-identical links in the rest part of this section can be verified from the AT parameters of the reported results in [39].…”
Section: Numerical Results and Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The analytical results for the considered system with EDFA are obtained for parameters M 1 = 2, E = 4 and y th = 0.5. Note that, in this paper we utilize the same set of parameters for EDFA that were used and validated in [20], [25]. Further, the choice of the AT parameter α i for non-identical links in the rest part of this section can be verified from the AT parameters of the reported results in [39].…”
Section: Numerical Results and Discussionmentioning
confidence: 99%
“…Here h is Planck's constant, ν is the optical center frequency, G is the amplifier gain, and N sp is spontaneous emission factor [20], [42]. It is assumed that, the optical gain is sufficiently high such that the ASE noise is the dominant source compared with the shot and thermal noise sources at the Rx [20], [22], [25], [42]. Prior to square law detection, the received optical signal with noise is passing through a band-pass filter in order to improve the SNR (i.e., reduce the noise).…”
Section: B Ber Of Rc Over Correlated γ γ At With Edfa Pre-amplifier mentioning
confidence: 99%
“…From (16) and (18), it can be seen that the optimal weighting scheme does not depend on R. For simplicity, we assume that R = 1 and hence we have w 1 = cos θ and w 2 = sin θ. Theorem 1: The solution of the optimisation problem (18) is given by…”
Section: System Model and Problem Formulationmentioning
confidence: 99%
“…Pointing errors which are generated by misalignment of the laser beam at the receiver is the second challenge towards FSO deployment [17,18]. The Málaga channel model can cover a wide range of channel conditions from weak to strong as well the effect of the pointing errors [16].…”
Section: Introductionmentioning
confidence: 99%
“…Although intensity modulation with direct detection (IM/DD) is widely used in LEO-StG optical communications due to its simplicity, especially on-off keying (OOK) and pulse-position modulation (PPM), the received signal photons per bit is limited which results in difficulties to establish a high capacity LEO-StG links [4]. Besides, atmospheric attenuation, pointing error and turbulence due to the atmospheric stochastic volatility may lead the fluctuations at the received signal power [5], [6], resulting in received signal power drop below the receiver's sensitivity threshold and deteriorating the system performance, especially for IMDD systems with limited transmit power and receiver sensitivity. Therefore, an advanced modulation technique is urgent for LEO-StG optical communications.…”
Section: Introductionmentioning
confidence: 99%