Design of an L-Band Dual Feedhorn for the Purposes of Microwave Search for ExtraTerrensial Intelligence

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Date
1994-07
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Referee
Mark
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Společnost pro radioelektronické inženýrství
Abstract
Logic behind the design of a dual feedhorn for the 26-meter Cassegrainian antenna of the Agassiz Station-Harvard-Smithsonian Observatory is presented in the paper. Theoretically predicted arid measured results in the "waterhole" band (1.4-1.7 GHz) are presented. The antenna has been utilized in the Harvard Wide-Bandwidth HighResolution Microwave Search for ExtraTerrestrial Intelligence (SETI) Program, with the Observatory as a SETI-dedicated facility.
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Citation
Radioengineering. 1994, vol. 3, č. 2, s. 1-4. ISSN 1210-2512
http://www.radioeng.cz/fulltexts/1994/94_02_01.pdf
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Peer-reviewed
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en
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Creative Commons Attribution 3.0 Unported License
http://creativecommons.org/licenses/by/3.0/
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