Improved low frequency seismic noise isolation system for gravitational wave detectors

Details Improved low frequency seismic noise isolation system for gravitational wave detectors Improved low frequency seismic noise isolation system for gravitational wave detectors

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998rsci...69.2781z&link_type=abstract

Review of Scientific Instruments, Volume 69, Issue 7, pp. 2781-2784 (1998).

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3

Gravitational Wave Detectors And Experiments, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques, Surface Waves And Free Oscillations

Scientific paper

An improved three-stage low frequency seismic noise isolation system for gravitational wave detectors, based on the cantilever spring, is presented. The measurement results show that the vertical and horizontal displacements of the test mass, at 10 Hz, reach 7×10-13 m/Hz and 1×10-12 mHz, respectively, and the isolation ratios of the system come to about 60 dB vertically and over 50 dB horizontally.

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