Design of an L-Band Dual Feedhorn for the Purposes of Microwave Search for ExtraTerrensial Intelligence
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.
Keywords
SETI, radio astronomy antennasPersistent identifier
http://hdl.handle.net/11012/58485Document type
Peer reviewedDocument version
Final PDFSource
Radioengineering. 1994, vol. 3, č. 2, s. 1-4. ISSN 1210-2512http://www.radioeng.cz/fulltexts/1994/94_02_01.pdf
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- 1994/2 [6]
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