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dc.contributor.authorSenior, J.M.
dc.contributor.authorMoss, S.E.
dc.contributor.authorQiu, X.-Z.
dc.contributor.authorVandewege, J.
dc.identifier.citationSenior , J M , Moss , S E , Qiu , X-Z & Vandewege , J 1999 , ' Semiconductor optical amplifier cascade modeling for the PLANET SuperPON ' , Proceedings of SPIE , vol. 3843 , pp. 190-196 .
dc.identifier.otherPURE: 1364210
dc.identifier.otherPURE UUID: 30717a5a-bc7b-4b57-a916-7064708b0f63
dc.identifier.otherScopus: 0033329660
dc.descriptionCopyright 2004 Elsevier Science B.V., Amsterdam. All rights reserved.
dc.description.abstractThe next generation of optical communication networks should provide a significant role for large range high-splitting ratio high-speed passive optical networks (SuperPON). Optical amplification of both upstream and downstream traffic is necessary to sustain these configurations with several amplifiers in series throughout the network. The Photonic Local Access Network (PLANET), an EU-ACT project, is developed to operate at 2-5 Gbit/s in the downstream direction and at 311 Mbit/s in the upstream. The downstream utilized erbium-doped fiber amplifiers whereas in the upstream the use of burst-mode semiconductor optical amplifiers (SOA) minimized noise funneling effects. Results for the upstream SOA cascade are presented.en
dc.relation.ispartofProceedings of SPIE
dc.titleSemiconductor optical amplifier cascade modeling for the PLANET SuperPONen
dc.contributor.institutionOffice of the Vice-Chancellor
dc.contributor.institutionCentre for Computer Science and Informatics Research
dc.contributor.institutionOptical Networks
dc.contributor.institutionCentre for Engineering Research
dc.contributor.institutionCommunications and Intelligent Systems
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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