Fundamental factors affecting the optimum frequency range for SETI

Details Fundamental factors affecting the optimum frequency range for SETI Fundamental factors affecting the optimum frequency range for SETI

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1867...66o&link_type=abstract

Proc. SPIE Vol. 1867, p. 66-74, The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum, Stuart A. Kingsley;

Physics

Scientific paper

There is little doubt that confirmation of the existence of extraterrestrial intelligent life will be obtained from electromagnetic waves generated by our counterparts. The best frequency regions in which to expect such signals depends upon the free-space loss, the background noise, the spectral purity obtainable, and the power required as a function of frequency. This paper will discuss the rationale that led to the selection of the microwave window for the NASA SETI Program.

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