DF Relayed Subcarrier FSO Links over Malaga Turbulence Channels with Phase Noise and Non-Zero Boresight Pointing Errors

被引:18
|
作者
Varotsos, George K. [1 ]
Nistazakis, Hector E. [1 ]
Gappmair, Wilfried [2 ]
Sandalidis, Harilaos G. [3 ]
Tombras, George S. [1 ]
机构
[1] Univ Athens, Fac Phys, Dept Elect Comp Telecommun & Control, Athens 15784, Greece
[2] Graz Univ Technol, Inst Commun Networks & Satellite Commun, A-8010 Graz, Austria
[3] Univ Thessaly, Dept Comp Sci & Biomed Informat, Papasiopoulou 2-4, Lamia 35131, Greece
来源
APPLIED SCIENCES-BASEL | 2018年 / 8卷 / 05期
关键词
free-space optics (FSO); multi-hop transmission; atmospheric turbulence; pointing errors; phase noise; SPACE OPTICAL COMMUNICATION; GAMMA-GAMMA; PERFORMANCE;
D O I
10.3390/app8050664
中图分类号
O6 [化学];
学科分类号
0703 ;
摘要
Subcarrier free-space optical (FSO) systems using coherent recovery techniques at the receiver have acquired growing research interest in recent times. However, their optimal performance is diminished by the non-perfect synchronization of carrier frequency and phase, which is mainly due to phase noise problems. Moreover, turbulence and pointing error effects further deteriorate the overall performance. However, relay transmission schemes can extend the coverage distance and offer substantial improvements over fading conditions. In this respect, we consider a serially relayed network using decode-and-forward relays, and investigate its performance by means of average symbol error probability and mean outage duration. Turbulence is modeled by the recently unified M(alaga) distribution, which constitutes a very general statistical model that accurately describes the irradiance fluctuations from weak-to-strong turbulence conditions. Additionally, the presence of non-zero boresight pointing errors due to misalignment between the transmitter-receiver pair is considered, while the effect of phase noise is specified by a Tikhonov distribution. A comparison between single line-of-sight and serially relayed FSO configurations is provided as well. Novel approximated mathematical expressions are deduced, which are proved to be accurate enough over a wide range of turbulence strengths and signal-to-noise values. Finally, proper numerical results are presented and validated by Monte Carlo simulations.
引用
收藏
页数:15
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