Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/32565
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | NANNI, Jacopo | en_US |
dc.contributor.author | Giovannini, Andrea | en_US |
dc.contributor.author | Hadi, Muhammad Usman | en_US |
dc.contributor.author | Lenzi, Enrico | en_US |
dc.contributor.author | RUSTICELLI, SIMONE | en_US |
dc.contributor.author | Wayth, Randall | en_US |
dc.contributor.author | PERINI, FEDERICO | en_US |
dc.contributor.author | MONARI, JADER | en_US |
dc.contributor.author | Tartarini, Giovanni | en_US |
dc.date.accessioned | 2022-09-12T12:40:13Z | - |
dc.date.available | 2022-09-12T12:40:13Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0733-8724 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32565 | - |
dc.description.abstract | Radio over Fiber (RoF) Systems exploiting a direct modulation of the laser source are presently utilized within important Radioastronomic scenarios. Due to the particular operating conditions of some of these realizations, the phenomena which typically generate nonlinearities in RoF links for telecommunications applications can be here regarded as substantially harmless. However, these same operating conditions can make the RoF systems vulnerable to different kinds of nonlinear effects, related to the influence of the Rayleigh Backscattered signal on the transmitted one. A rigorous description of the phenomenon is performed, and an effective countermeasure to the problem is proposed and demonstrated, both theoretically and experimentally. | en_US |
dc.language.iso | eng | en_US |
dc.title | Controlling Rayleigh-Backscattering-Induced Distortion in Radio Over Fiber Systems for Radioastronomic Applications | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1109/JLT.2020.2993203 | en_US |
dc.identifier.scopus | 2-s2.0-85091261577 | en_US |
dc.identifier.isi | WOS:000575409900019 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85091261577 | en_US |
dc.identifier.url | https://ieeexplore.ieee.org/abstract/document/9089231 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 38 | en_US |
dc.relation.issue | 19 | en_US |
dc.relation.firstpage | 5393 | en_US |
dc.relation.lastpage | 5405 | en_US |
dc.relation.numberofpages | 13 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 9 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | AUS | en_US |
dc.contributor.country | PAK | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF LIGHTWAVE TECHNOLOGY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_17 Instrumentation – telescopes, detectors and techniques | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0733-8724 | - |
crisitem.journal.ance | E092523 | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0003-3130-2514 | - |
crisitem.author.orcid | 0000-0002-8935-8142 | - |
crisitem.author.orcid | 0000-0001-6991-8651 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
FINAL_VERSION.pdf | postprint | 1.7 MB | Adobe PDF | Visualizza/apri |
JLT_38_19_2020.pdf | [Administrators only] | 2.15 MB | Adobe PDF |
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