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Construction and Measurement of a 31.3–45 GHz Optimized Spline-profile Horn with Corrugations

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2012
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Zorzi Avendaño, Pablo Ignacio
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Construction and Measurement of a 31.3–45 GHz Optimized Spline-profile Horn with Corrugations
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Author
  • Zorzi Avendaño, Pablo Ignacio;
  • Granet, Christophe;
  • Colleoni, Franco;
  • Reyes, Nicolás;
  • Pizarro Lucero, José;
  • Mena Mena, Fausto Patricio;
  • Bronfman Aguiló, Leonardo;
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.
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Artículo de publicación ISI
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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).
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URI: https://repositorio.uchile.cl/handle/2250/125675
DOI: 10.1007/s10762-011-9834-1
Quote Item
J Infrared Milli Terahz Waves (2012) 33:17–24
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