We present the development and characterisation of a high frequency (500-750 GHz) corrugated horn based on stacked rings. A previous horn design, based on a Winston profile, has been adapted for the purpose of this manufacturing process without noticeable RF degradation. A subset of experimental results obtained using a vector network analyser are presented and compared to the predicted performance. These first results demonstrate that this technology is suitable for most commercial applications and also astronomical receivers in need of horn arrays at high frequencies.

High performance WR-1.5 corrugated horn based on stacked rings / Maffei, B.; Von Bieren, A.; De Rijk, E.; Ansermet, J. -P.; Pisano, G.; Legg, S.; Macor, A.. - 9153:(2014). (Intervento presentato al convegno Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII tenutosi a can) [10.1117/12.2056158].

High performance WR-1.5 corrugated horn based on stacked rings

Pisano G.;
2014

Abstract

We present the development and characterisation of a high frequency (500-750 GHz) corrugated horn based on stacked rings. A previous horn design, based on a Winston profile, has been adapted for the purpose of this manufacturing process without noticeable RF degradation. A subset of experimental results obtained using a vector network analyser are presented and compared to the predicted performance. These first results demonstrate that this technology is suitable for most commercial applications and also astronomical receivers in need of horn arrays at high frequencies.
2014
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Corrugated horns; quasi-optics
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
High performance WR-1.5 corrugated horn based on stacked rings / Maffei, B.; Von Bieren, A.; De Rijk, E.; Ansermet, J. -P.; Pisano, G.; Legg, S.; Macor, A.. - 9153:(2014). (Intervento presentato al convegno Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII tenutosi a can) [10.1117/12.2056158].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1557218
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