New seismic attenuation system (SAS) for the advanced LIGO configurations (LIGO2)

Details New seismic attenuation system (SAS) for the advanced LIGO configurations (LIGO2) New seismic attenuation system (SAS) for the advanced LIGO configurations (LIGO2)

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..523..320b&link_type=abstract

GRAVITATIONAL WAVES: Third Edoardo Amaldi Conference. AIP Conference Proceedings, Volume 523, pp. 320-324 (2000).

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Gravitational Wave Detectors And Experiments, Vibration Isolation

Scientific paper

A new passive seismic attenuation system is being developed to replace the current passive attenuation stacks in LIGO 2, it is expected to drive the seismic contribution to the interferometer noise below any other noise source. The SAS will be effective completely starting at about 5 Hz, well inside the (uncompensated) gravity gradient noise wall. .

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