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| Indexado |
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| DOI | 10.1007/S10762-011-9834-1 | ||||
| Año | 2012 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
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 24A degrees at 31.3 GHz and 16A degrees 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.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | ZORZI-AVENDANO, PABLO IGNACIO | Hombre |
Universidad de Chile - Chile
|
| 2 | Granet, Christophe | Hombre |
BAE Syst Australia Pty Ltd - Australia
BAE International Inc. Sdn. Bhd. - Malasia |
| 3 | COLLEONI-VILLAGRAN, FRANCO ANTONIO | Hombre |
Universidad de Chile - Chile
|
| 4 | REYES-MENESES, NICOLAS | Hombre |
Universidad de Chile - Chile
|
| 5 | Pizarro, Jose | Hombre |
Universidad de Chile - Chile
|
| 6 | MENA, FAUSTO-PATRICIO | Hombre |
Universidad de Chile - Chile
|
| 7 | BRONFMAN-AGUILO, MIGUEL LEONARDO | Hombre |
Universidad de Chile - Chile
|
| Fuente |
|---|
| ALMA-CONICYT |
| ALMA-CONICYT Fund for the Development of Chilean Astronomy |
| Chilean Center of Excellence in Astrophysics and Associated Technologies |
| Agradecimiento |
|---|
| This work was supported by the Chilean Center of Excellence in Astrophysics and Associated Technologies (PBF 06), and by the ALMA-CONICYT Fund for the Development of Chilean Astronomy (Projects 31080003 and 31080004). |
| Acknowledgements This work was supported by the Chilean Center of Excellence in Astrophysics and Associated Technologies (PBF 06), and by the ALMA-CONICYT Fund for the Development of Chilean Astronomy (Projects 31080003 and 31080004). |