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Authordc.contributor.authorReyes Guzmán, Nicolás 
Authordc.contributor.authorGüsten, Rolf 
Authordc.contributor.authorGraf, Urs 
Authordc.contributor.authorRisacher, Christophe 
Authordc.contributor.authorRicken, Oliver 
Admission datedc.date.accessioned2019-05-29T13:41:12Z
Available datedc.date.available2019-05-29T13:41:12Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationISSTT 2017 - 28th International Symposium on Space Terahertz Technology, Volumen 2017-March
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/169089
Abstractdc.description.abstractThe Low Frequency Array instrument at SOFIA is a heterodyne array designed to observe in the complete range between 1.9 and 2.5 THz. It is a 14 pixel instrument, working in a dual polarization configuration. To provide enough LO power for the 14 HEB mixers a cryogenic solid state LO source is used. It consists of two identical set of millimeter wave amplification and multiplication chains, one per polarization. The frequency coverage is limited to 1.830 to 2.070 GHz, centered on one of the main scientific target of the instrument, the CII at 158mm. We present an overview of the design of this LO source and present the experimental results obtained.
Lenguagedc.language.isoen
Publisherdc.publisherISSTT
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Sourcedc.sourceISSTT 2017 - 28th International Symposium on Space Terahertz Technology
Keywordsdc.subjectAtomic and Molecular Physics, and Optics
Keywordsdc.subjectComputer Networks and Communications
Keywordsdc.subjectSpace and Planetary Science
Keywordsdc.subjectRadiation
Keywordsdc.subjectElectrical and Electronic Engineering
Títulodc.titleA cryogenic solid state LO source at 1.9THz
Document typedc.typeArtículo de revista
dcterms.accessRightsdcterms.accessRightsAcceso a solo metadatos
Catalogueruchile.catalogadorlaj
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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