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Sensitive detection of narrowband pulses.
1SETI Institute, Moffett Field, CA 94035, USA.
Acta Astronautica
|January 1, 1986
Summary
This study demonstrates a new method for detecting low-duty-cycle pulsed signals, improving sensitivity by 7 dB. This technique is ideal for identifying potential extraterrestrial beacons in the Search for Extraterrestrial Intelligence (SETI).
Area of Science:
- Astrophysics
- Signal Processing
- Electrical Engineering
Background:
- Highly monochromatic signals are typically detected using narrow filters and power accumulation.
- Low-duty-cycle pulsed signals present a unique detection challenge compared to continuous signals.
Purpose of the Study:
- To develop a more sensitive method for detecting low-duty-cycle pulsed signals.
- To assess the suitability of pulsed signals as potential extraterrestrial beacons for SETI.
Main Methods:
- Utilized a square law device followed by thresholding and a novel algorithm.
- Compared the sensitivity of the new method against traditional narrow-band filtering for pulsed signals.
Main Results:
- The proposed method achieved approximately 7 dB greater sensitivity for low-duty-cycle pulsed signals compared to continuous monochromatic signals.
- Identified pulsed signals from rotating beacons as strong candidates for extraterrestrial communication.
Conclusions:
- The developed signal detection algorithm offers enhanced sensitivity for pulsed signals.
- This method is promising for SETI applications, particularly for detecting extraterrestrial beacons.
- Software is ready for field testing with the NASA Multichannel Spectrum Analyzer (MCSA).