Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/24234
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Clivati, Cecilia | en_US |
dc.contributor.author | Costanzo, Giovanni A. | en_US |
dc.contributor.author | Frittelli, Matteo | en_US |
dc.contributor.author | Levi, Filippo | en_US |
dc.contributor.author | Mura, Alberto | en_US |
dc.contributor.author | Zucco, Massimo | en_US |
dc.contributor.author | AMBROSINI, ROBERTO | en_US |
dc.contributor.author | BORTOLOTTI, CLAUDIO | en_US |
dc.contributor.author | PERINI, FEDERICO | en_US |
dc.contributor.author | ROMA, MAURO | en_US |
dc.contributor.author | Calonico, Davide | en_US |
dc.date.accessioned | 2020-04-24T16:42:35Z | - |
dc.date.available | 2020-04-24T16:42:35Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0885-3010 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24234 | - |
dc.description.abstract | We realize a coherent fiber link for application in very long baseline interferometry (VLBI) for radio astronomy and geodesy. A 550-km optical fiber connects the Italian National Metrological Institute (INRIM) to a radio telescope in Italy and is used for the primary Cs fountain clock stability and accuracy dissemination. We use an ultrastable laser frequency- referenced to the primary standard as a transfer oscillator; at the radio telescope, an RF signal is generated from the laser by using an optical frequency comb. This scheme now provides the traceability of the local maser to the SI second, realized by the Cs fountain at the 1.7×10^-16 accuracy. The fiber link never limits the experiment and is robust enough to sustain radio astronomical campaigns. This experiment opens the possibility of replacing the local hydrogen masers at the VLBI sites with optically-synthesized RF signals. This could improve VLBI resolution by providing more accurate and stable frequency references and, in perspective, by enabling common- clock VLBI based on a network of telescopes connected by fiber links. | en_US |
dc.language.iso | eng | en_US |
dc.title | A coherent fiber link for very long baseline interferometry | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1109/TUFFC.2015.007221 | en_US |
dc.identifier.scopus | 2-s2.0-84959465365 | en_US |
dc.identifier.isi | 000367010200001 | en_US |
dc.identifier.url | https://ieeexplore.ieee.org/document/7321699 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 62 | en_US |
dc.relation.issue | 11 | en_US |
dc.relation.firstpage | 1907 | en_US |
dc.relation.lastpage | 1912 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 11 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | IEEE TRANSACTIONS ON ULTRASONICS FERROELECTRICS AND FREQUENCY CONTROL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE2 Fundamental constituents of matter: particle, nuclear, plasma, atomic, molecular, gas, and optical plasma::PE2_17 Metrology and measurement | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0885-3010 | - |
crisitem.journal.ance | E079963 | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0002-6480-4564 | - |
crisitem.author.orcid | 0000-0002-8935-8142 | - |
crisitem.author.orcid | 0000-0003-4142-3897 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
LIFTforRadioastronomy-2.pdf | 1.17 MB | Adobe PDF | Visualizza/apri | |
07321699.pdf | [administrators only] | 2.41 MB | Adobe PDF |
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