Design of an L-Band Dual Feedhorn for the Purposes of Microwave Search for ExtraTerrensial Intelligence
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Horowitz, P.
Gimersky, M.
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Mark
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Společnost pro radioelektronické inženýrství
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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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Radioengineering. 1994, vol. 3, č. 2, s. 1-4. ISSN 1210-2512
http://www.radioeng.cz/fulltexts/1994/94_02_01.pdf
http://www.radioeng.cz/fulltexts/1994/94_02_01.pdf
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en
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Except where otherwised noted, this item's license is described as Creative Commons Attribution 3.0 Unported License