Signal to noise ratio in a satellite gravitational wave experiment

Details Signal to noise ratio in a satellite gravitational wave experiment Signal to noise ratio in a satellite gravitational wave experiment

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975acaau...2..535b&link_type=abstract

(International Academy of Astronautics, International Symposium on the Effects of Relativity in Present-Day Space Travel, 1st, B

Astronomy and Astrophysics

Astronomy

1

Gravitational Waves, Radiation Measurement, Rangefinding, Satellite Tracking, Signal To Noise Ratios, Velocity Measurement, Doppler Effect, Radio Tracking, Star Clusters, Stellar Radiation

Scientific paper

A system for detection of gravitational radiation is proposed which consists of a widely-separated pair of drag-free satellites. Variations in their relative velocity induced by gravitational waves would be detected by a Doppler-ranging system. It is shown that the sensitivity of such a system can be sufficient to allow detection of gravitational radiation from high-density star clusters near the galactic center.

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