Properties of seismic noise at the Virgo site

Details Properties of seismic noise at the Virgo site Properties of seismic noise at the Virgo site

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21s.433a&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 5, pp. S433-S440 (2004).

Physics

3

Scientific paper

We present the results of a study of the major low-frequency sources of seismic activity at the Virgo site. These sources are of natural and human origin: oceanic microseism (below 1 Hz), local traffic and human activity on site (below 10 Hz). Using data collected during the commissioning of the central Virgo interferometer (CITF) we have measured the seismic coupling to the interferometer, demonstrating that seismic noise contributed to the CITF dark fringe noise only below approximately 2 Hz.

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