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dc.contributor.authorLim, Wansu
dc.contributor.authorYun, Changho
dc.contributor.authorKim, Kiseon
dc.date.accessioned2013-02-28T12:29:50Z
dc.date.available2013-02-28T12:29:50Z
dc.date.issued2009-03
dc.identifier.citationLim , W , Yun , C & Kim , K 2009 , ' BER performance analysis of radio over free-space optical systems considering laser phase noise under Gamma-Gamma turbulence channels ' , Optics Express , vol. 17 , no. 6 , pp. 4479-4484 . https://doi.org/10.1364/OE.17.004479
dc.identifier.otherPURE: 930718
dc.identifier.otherPURE UUID: e7ed0ba8-a5e2-48d0-a4f9-b3251297053a
dc.identifier.otherScopus: 62549135643
dc.identifier.urihttp://hdl.handle.net/2299/10115
dc.description.abstractThis paper analytically investigates a bit error rate (BER) performance of radio over free space optical (FSO) systems considering laser phase noise under Gamma-Gamma turbulence channels. An external modulation using a dual drive Mach-Zehnder modulator (DD-MZM) and a phase shifter is employed because a DD-MZM is robust against a laser chirp and provides high spectral efficiency. We derive a closed form average BER as a function of different turbulence strengths and laser diode (LD) linewidth, and investigate its analytical behavior under practical scenario. As a result, for a given average SNR with normalized perturbation, it is shown that the difference of average BER corresponding to two LDs (with linewidth of 624MHz and 10MHz) under weak turbulence is almost 3 times larger than that under strong turbulenceen
dc.language.isoeng
dc.relation.ispartofOptics Express
dc.titleBER performance analysis of radio over free-space optical systems considering laser phase noise under Gamma-Gamma turbulence channelsen
dc.contributor.institutionCentre for Computer Science and Informatics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1364/OE.17.004479
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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