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dc.contributor.authorMalcoci, Andrei
dc.date.accessioned2010-10-12T18:25:29Z
dc.date.available2010-10-12T18:25:29Z
dc.date.issued2006
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-30F6-B
dc.description.abstractPhotonic Local Oscillators (PLOs) operating at optical wavelengths around 1550 nm have a major importance especially for radio astronomic THz Antenna arrays like the "Atacama Large Millimeter/Submillimeter Array" (ALMA) in Chile. The PLO-Technique allows the distribution of a centrally generated Local Oscillator signal over more than ten kilometres to the Antennas, by using the optical Window for long distance communications where loss in glass fibres is lowest...
dc.format.extent165 S.
dc.format.mimetypeapplication/pdf
dc.language.isodeu
dc.publisherUniv. Duisburg
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc522
dc.subject.gokTBC 000
dc.titlePhotonische Lokaloszillatoren für Anwendungen in der Terahertz-Radioastronomie
dc.typemonograph
dc.subject.gokverbalRadioastronomie
dc.identifier.doi10.23689/fidgeo-110
dc.identifier.ppn517856050
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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