Construction and Measurement of a 31.3–45 GHz Optimized Spline-profile Horn with Corrugations
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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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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.
General note
Artículo de publicación ISI
Patrocinador
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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J Infrared Milli Terahz Waves (2012) 33:17–24
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