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dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorCagigas Ibáñez, Jaime 
dc.contributor.authorCano de Diego, Juan Luis 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorMediavilla Sánchez, Ángel 
dc.contributor.authorTerán Collantes, José Vicente 
dc.contributor.authorVilla Benito, Enrique 
dc.contributor.authorHoyland, Roger J.
dc.contributor.authorCasas Reinares, Francisco Javier
dc.contributor.authorOrtiz García, David
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2013-09-13T12:18:56Z
dc.date.available2013-09-13T12:18:56Z
dc.date.issued2012-09
dc.identifier.urihttp://hdl.handle.net/10902/3268
dc.description.abstractThis document describes the scheme and prototype test results of a broadband radioastronomy receiver aimed to obtain polarisation data of Cosmic Microwave Background (CMB) radiation from the sky. Nominal receiver bandwidth is 26 to 36 GHz. The radiometer will work as a polarimeter to obtain the polarisation Stokes parameters (Q, U and I) of the incoming electromagnetic signal to the feed-horns. Prototype tests have demonstrated the receiver concept based on electronic phase switching in two balanced branches. The correlation between signals is performed directly at 31 GHz by a broadband 3 dB/180º hybrid coupler.es_ES
dc.format.extent4 p.es_ES
dc.language.isospaes_ES
dc.rights© 2012 URSI Españaes_ES
dc.sourceURSI 2012, XXVII Simposium Nacional de la Unión Científica Internacional de Radio, Elchees_ES
dc.titleReceptor de polarización a 31 GHz para radioastronomíaes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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