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Testing the 3–18 GHz Ultra-Wideband Feed Prototype

A. A. Roev, V. Chernov

Transactions of IAA RAS, issue 36, 61–67 (2016)

Keywords: VGOS, radio telescope, ultra-wideband feed, development, parameters

About the paper

Abstract

A research prototype of an ultra-wideband feed was designed and built based on our calculations. Measurements are presented for the following main feed parameters: phase and amplitude radiation pattern in E-, H-, and D- planes, gain, voltage standing-wave ratio, and isolation between the orthogonal channels. Channel isolation across the operating range is not worse than 16 dB, VSWR is less than 1.8: 1 in the range from 5 GHz to 14 GHz; it is less than 2.5: 1 in the range from 3 GHz to 16 GHz. The measured radiation patterns in E-plane and H-plane are close to the calculation and simulation results

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A. A. Roev, V. Chernov. Testing the 3–18 GHz Ultra-Wideband Feed Prototype // Transactions of IAA RAS. — 2016. — Issue 36. — P. 61–67. @article{roev2016, abstract = {A research prototype of an ultra-wideband feed was designed and built based on our calculations. Measurements are presented for the following main feed parameters: phase and amplitude radiation pattern in E-, H-, and D- planes, gain, voltage standing-wave ratio, and isolation between the orthogonal channels. Channel isolation across the operating range is not worse than 16 dB, VSWR is less than 1.8: 1 in the range from 5 GHz to 14 GHz; it is less than 2.5: 1 in the range from 3 GHz to 16 GHz. The measured radiation patterns in E-plane and H-plane are close to the calculation and simulation results}, author = {A.~A. Roev and V. Chernov}, issue = {36}, journal = {Transactions of IAA RAS}, keyword = {VGOS, radio telescope, ultra-wideband feed, development, parameters}, pages = {61--67}, title = {Testing the 3–18 GHz Ultra-Wideband Feed Prototype}, url = {http://iaaras.ru/en/library/paper/1081/}, year = {2016} } TY - JOUR TI - Testing the 3–18 GHz Ultra-Wideband Feed Prototype AU - Roev, A. A. AU - Chernov, V. PY - 2016 T2 - Transactions of IAA RAS IS - 36 SP - 61 AB - A research prototype of an ultra-wideband feed was designed and built based on our calculations. Measurements are presented for the following main feed parameters: phase and amplitude radiation pattern in E-, H-, and D- planes, gain, voltage standing-wave ratio, and isolation between the orthogonal channels. Channel isolation across the operating range is not worse than 16 dB, VSWR is less than 1.8: 1 in the range from 5 GHz to 14 GHz; it is less than 2.5: 1 in the range from 3 GHz to 16 GHz. The measured radiation patterns in E-plane and H-plane are close to the calculation and simulation results UR - http://iaaras.ru/en/library/paper/1081/ ER -