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dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorPascual Gutiérrez, Juan Pablo 
dc.contributor.authorMediavilla Sánchez, Ángel 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2013-09-23T07:06:59Z
dc.date.available2013-09-23T07:06:59Z
dc.date.issued2005-09
dc.identifier.urihttp://hdl.handle.net/10902/3359
dc.description.abstractThis communication deals with the implemented assemblies and characterisation test results of several Back End Modules at 44 GHz for the Planck Mission of the European Space Agency (ESA), which are low noise and broadband (20%) receivers having direct conversion to DC. They are parts of the 44 GHz radiometers. In order to perform integration tests, before the integration of Flight Model units, some representative demonstrators have been manufactured and tested. These demonstrators will be integrated in Jodrell Bank Observatory (Manchester, England) with the Front End Modules made there. Main magnitudes tested are effective bandwidth, RF to DC response, noise temperature, linearity, input matching, video bandwidth and knee frequency of low frequency 1/f noise at the output.es_ES
dc.format.extent4 p.es_ES
dc.language.isospaes_ES
dc.rights© 2005 URSI Españaes_ES
dc.sourceURSI 2005, XX Simposium Nacional de la Unión Científica Internacional de Radio, Gandíaes_ES
dc.titleDemostradores de los módulos posteriores de 44 GHz para la misión Planckes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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