The paper describes strategies, tradeoffs, instrumentation, and overall objectives for the SETI Radio Observation Project. Novel approaches have been formulated in order to achieve coverage of the desirable frequency and spatial regimes (about 80% of the sky and in the frequency range of 1.4-25 GHz). A mixed strategy has been developed which uses the survey capability of small antennas and the sensitivity of modern maser amplifiers to achieve sensitivities comparable to those reached by previous observers, but with as much as 10,000 times the scope of both the frequency and spatial coverage possible to those experimenters.
The SETI Radio Observational Project - Strategy, instrumentation, and objectives
International Astronautical Federation, International Astronautical Congress ; 1978 ; Dubrovnik, Yugoslavia
01.10.1978
Aufsatz (Konferenz)
Keine Angabe
Englisch
The SERENDIP SETI Project: New Instrumentation for SETI and Results of Recent Observations
British Library Conference Proceedings | 1995
|The SERENDIP piggyback SETI project
NTRS | 1992
|New SETI sky surveys for radio pulses
Online Contents | 2010
|The Radio Hazard for Astronomy and SETI
British Library Conference Proceedings | 2000
|