dc.creator | Zorzi Avendaño, Pablo Ignacio | |
dc.creator | Granet, Christophe | |
dc.creator | Colleoni, Franco | |
dc.creator | Reyes, Nicolás | |
dc.creator | Pizarro Lucero, José | |
dc.creator | Mena Mena, Fausto Patricio | |
dc.creator | Bronfman Aguiló, Leonardo | |
dc.date.accessioned | 2013-12-26T14:22:05Z | |
dc.date.available | 2013-12-26T14:22:05Z | |
dc.date.created | 2013-12-26T14:22:05Z | |
dc.date.issued | 2012 | |
dc.identifier | J Infrared Milli Terahz Waves (2012) 33:17–24 | |
dc.identifier | DOI 10.1007/s10762-011-9834-1 | |
dc.identifier | https://repositorio.uchile.cl/handle/2250/125843 | |
dc.description.abstract | A 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.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Chile | |
dc.subject | Spline-profile | |
dc.title | Construction and Measurement of a 31.3–45 GHz Optimized Spline-profile Horn with Corrugations | |
dc.type | Artículo de revista | |