EM developments for a radio astronomy polarimeter: The QUIJOTE experiment

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URI: https://hdl.handle.net/10902/38422
ISBN: 978-1-4673-5706-7
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Autoría
Artal Latorre, EduardoAutoridad Unican; Cano de Diego, Juan LuisAutoridad Unican; Mediavilla Sánchez, ÁngelAutoridad Unican; Villa Benito, EnriqueAutoridad Unican; Aja Abelán, BeatrizAutoridad Unican; Fuente Rodríguez, Luisa María de laAutoridad Unican; Cagigas Ibañez, JaimeAutoridad Unican
Fecha
2013
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© 2013 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.
Publicado en
International Conference on Electromagnetics in Advanced Applications (ICEAA), Torino, Italy, 2013, 250-253
Editorial
Institute of Electrical and Electronics Engineers, Inc.
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Resumen/Abstract
A comparison between simulated and measured results in different subsystems of a radio astronomy polarimeter receiver at 26–36 GHz band is presented. This comparison underlines the importance of careful simulation with different electromagnetic software tools in order to predict the receiver behavior. The receiver obtains three (Q, U and I) Stokes parameters simultaneously.
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