High Resolution Microwave Survey
From Infogalactic: the planetary knowledge core
The High Resolution Microwave Survey was a NASA project that was to scan ten million frequencies using radio telescopes. A decade in the making, the objective was to find transmissions from alien intelligences. The primary point of observation for the project was the Arecibo Ionaspheric Observatory in Puerto Rico. The project began in October 1992 with SETI researcher Jill Tarter on board. However, a year later, first-term Nevada Senator Richard Bryan succeeded in shutting down the project.[1]
References
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External links
- The NASA High Resolution Microwave Survey
- BEACON eSpace at Jet Propulsion Laboratory: NASA's High Resolution Microwave Survey: The first Year of the Sky Survey
- Social implications of NASA’s high resolution microwave survey
- The Current State of Target Selection for NASA's High Resolution Microwave Survey
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