dc.creatorZorzi Avendaño, Pablo Ignacio
dc.creatorGranet, Christophe
dc.creatorColleoni, Franco
dc.creatorReyes, Nicolás
dc.creatorPizarro Lucero, José
dc.creatorMena Mena, Fausto Patricio
dc.creatorBronfman Aguiló, Leonardo
dc.date.accessioned2012-07-31T21:32:32Z
dc.date.available2012-07-31T21:32:32Z
dc.date.created2012-07-31T21:32:32Z
dc.date.issued2012
dc.identifierJ Infrared Milli Terahz Waves (2012) 33:17–24
dc.identifierDOI 10.1007/s10762-011-9834-1
dc.identifierhttps://repositorio.uchile.cl/handle/2250/125675
dc.description.abstractA corrugated spline-profile horn has been designed to meet the stringent specifications and constraints of a receiver for Band 1 (31.3–45 GHz) of the Atacama Large Millimeter Array (ALMA). Given the physical restrictions of the receiver, the horn will be located behind a focusing lens placed 191 mm over its aperture. After this first focusing stage, the horn must have a reflection coefficient less than −20 dB and the cross-polarization not exceeding the −30 dB level in the entire frequency range. The side-lobes should be less than −25 dB at all frequencies and its half power beamwidth must be approximately 24◦ at 31.3 GHz and 16◦ at 45 GHz. The horn has been constructed using the split-block technique and characterized in a near-field scanner setup. The results show an excellent performance complying with all the requirements.
dc.languageen
dc.publisherSpringer
dc.subjectSpline-profile
dc.titleConstruction and Measurement of a 31.3–45 GHz Optimized Spline-profile Horn with Corrugations
dc.typeArtículo de revista


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