dc.contributor.author | Cano de Diego, Juan Luis | |
dc.contributor.author | Villa Benito, Enrique | |
dc.contributor.author | Terán Collantes, José Vicente | |
dc.contributor.author | González Mariscal, Elena | |
dc.contributor.author | Fuente Rodríguez, Luisa María de la | |
dc.contributor.author | Artal Latorre, Eduardo | |
dc.contributor.author | Mediavilla Sánchez, Ángel | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2015-11-11T14:15:11Z | |
dc.date.available | 2015-11-11T14:15:11Z | |
dc.date.issued | 2015-09 | |
dc.identifier.uri | http://hdl.handle.net/10902/7627 | |
dc.description.abstract | This contribution presents and analyzes a polarimeter scheme for radio astronomy applications in W-band. The scheme is based on a sub-harmonic mixer thus enabling the reduction of W-band hardware design. The receiver functionality is analyzed theoretically and the design of some subsystems such as the feed-horn, the polarizer and the orthomode transducer is shown in detail. Finally, the whole scheme is simulated in an ideal way and then realistic data files are introduced in order to check the receiver functionality and the expected performance. | es_ES |
dc.format.extent | 4 p. | es_ES |
dc.language.iso | spa | es_ES |
dc.rights | © 2015 URSI España | es_ES |
dc.source | URSI 2015, XXX Simposium Nacional de la Unión Científica Internacional de Radio, Pamplona | es_ES |
dc.title | Polarímetro en banda W para aplicaciones de radioastronomía: diseño y simulación | es_ES |
dc.type | info:eu-repo/semantics/conferenceObject | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.type.version | publishedVersion | es_ES |