Characterization of the Virgo seismic environment
The Virgo gravitational wave detector is an interferometer (ITF) with 3 km arms located in Pisa, Italy. From July to October 2010, Virgo performed its third science run (VSR3) in coincidence with the LIGO detectors. Despite several techniques adopted to isolate the ITF from the environment, seismic noise remains an important issue for Virgo. Vibrations produced by the detector infrastructure (such as air conditioning units, water chillers/heaters, pumps) are found to affect Virgos sensitivity,...[Show more]
|Collections||ANU Research Publications|
|Source:||Classical and Quantum Gravity|
|01_Rabeling_Characterization_of_the_Virgo_2012.pdf||1.13 MB||Adobe PDF||Request a copy|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.