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dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorCano de Diego, Juan Luis 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorVilla Benito, Enrique 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2015-11-11T16:22:17Z
dc.date.available2015-11-11T16:22:17Z
dc.date.issued2015-09
dc.identifier.urihttp://hdl.handle.net/10902/7638
dc.description.abstractCryogenic cooled very low noise amplifiers are critical components in radio astronomy receivers and other applications. A general description of these devices and their role in receivers is presented. Several examples of microwave and millimeter wave amplifiers covering bands from 4 GHz to 36 GHz are described. Noise temperatures of about 5 K in 4-12 GHz and 15 K in 25-34 GHz bands have been achieved in mHEMT technology based amplifiers.es_ES
dc.format.extent4 p.es_ES
dc.language.isospaes_ES
dc.rights© 2015 URSI Españaes_ES
dc.sourceURSI 2015, XXX Simposium Nacional de la Unión Científica Internacional de Radio, Pamplonaes_ES
dc.titleAmplificadores criogénicos de muy bajo ruido en microondas y ondas milimétricases_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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