dc.contributor.author | Artal Latorre, Eduardo | |
dc.contributor.author | Aja Abelán, Beatriz | |
dc.contributor.author | Cagigas Ibañez, Jaime | |
dc.contributor.author | Cano de Diego, Juan Luis | |
dc.contributor.author | Fuente Rodríguez, Luisa María de la | |
dc.contributor.author | Mediavilla Sánchez, Ángel | |
dc.contributor.author | Terán Collantes, José Vicente | |
dc.contributor.author | Villa Benito, Enrique | |
dc.contributor.author | Hoyland, Roger J. | |
dc.contributor.author | Casas Reinares, Francisco Javier | |
dc.contributor.author | Ortiz García, David | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2013-09-13T12:18:56Z | |
dc.date.available | 2013-09-13T12:18:56Z | |
dc.date.issued | 2012-09 | |
dc.identifier.uri | http://hdl.handle.net/10902/3268 | |
dc.description.abstract | This 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.extent | 4 p. | es_ES |
dc.language.iso | spa | es_ES |
dc.rights | © 2012 URSI España | es_ES |
dc.source | URSI 2012, XXVII Simposium Nacional de la Unión Científica Internacional de Radio, Elche | es_ES |
dc.title | Receptor de polarización a 31 GHz para radioastronomía | es_ES |
dc.type | info:eu-repo/semantics/conferenceObject | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.type.version | publishedVersion | es_ES |