Microstrip yagi antenna for ALMA band 11 receiver

We present a planar Yagi antenna that has an end-fire beam characteristic and broad operational bandwidth. Two dipoles with different lengths are cascaded together to broaden the bandwidth. Printed directors and truncated ground plane are employed to achieve high front-to-back gain ratio. The double...

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Main Authors: Tan, B, Yassin, G, Whithington, S, Goldie, D
Format: Journal article
Published: 2019
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author Tan, B
Yassin, G
Whithington, S
Goldie, D
author_facet Tan, B
Yassin, G
Whithington, S
Goldie, D
author_sort Tan, B
collection OXFORD
description We present a planar Yagi antenna that has an end-fire beam characteristic and broad operational bandwidth. Two dipoles with different lengths are cascaded together to broaden the bandwidth. Printed directors and truncated ground plane are employed to achieve high front-to-back gain ratio. The double-dipole antenna is fed directly with a microstrip, and hence is readily adaptable to most of the millimetre and sub-millimetre detector circuits. In this paper, we present the antenna design in the context of designing a 1.05 THz Superconductor-Insulator-Superconductor (SIS) mixer that is suitable for Atacama Large Millimetre/Sub-millimetre Array (ALMA) Band 11 receiver. Detailed analysis of the antenna design is discussed, and simulated far field beam patterns and bandwidth performance is presented.
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spelling oxford-uuid:b9e9af9f-865f-40e4-839d-a6f9719025b12022-03-27T05:06:15ZMicrostrip yagi antenna for ALMA band 11 receiverJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:b9e9af9f-865f-40e4-839d-a6f9719025b1Symplectic Elements at Oxford2019Tan, BYassin, GWhithington, SGoldie, DWe present a planar Yagi antenna that has an end-fire beam characteristic and broad operational bandwidth. Two dipoles with different lengths are cascaded together to broaden the bandwidth. Printed directors and truncated ground plane are employed to achieve high front-to-back gain ratio. The double-dipole antenna is fed directly with a microstrip, and hence is readily adaptable to most of the millimetre and sub-millimetre detector circuits. In this paper, we present the antenna design in the context of designing a 1.05 THz Superconductor-Insulator-Superconductor (SIS) mixer that is suitable for Atacama Large Millimetre/Sub-millimetre Array (ALMA) Band 11 receiver. Detailed analysis of the antenna design is discussed, and simulated far field beam patterns and bandwidth performance is presented.
spellingShingle Tan, B
Yassin, G
Whithington, S
Goldie, D
Microstrip yagi antenna for ALMA band 11 receiver
title Microstrip yagi antenna for ALMA band 11 receiver
title_full Microstrip yagi antenna for ALMA band 11 receiver
title_fullStr Microstrip yagi antenna for ALMA band 11 receiver
title_full_unstemmed Microstrip yagi antenna for ALMA band 11 receiver
title_short Microstrip yagi antenna for ALMA band 11 receiver
title_sort microstrip yagi antenna for alma band 11 receiver
work_keys_str_mv AT tanb microstripyagiantennaforalmaband11receiver
AT yassing microstripyagiantennaforalmaband11receiver
AT whithingtons microstripyagiantennaforalmaband11receiver
AT goldied microstripyagiantennaforalmaband11receiver