Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/68712
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Type: Journal article
Title: The Seismic Attenuation System (SAS) for the Advanced LIGO gravitational wave interferometric detectors
Author: Stochino, A.
Abbot, B.
Aso, Y.
Barton, M.
Bertolini, A.
Boschi, V.
Coyne, D.
DeSalvo, R.
Galli, C.
Huang, Y.
Ivanov, A.
Marka, S.
Ottaway, D.
Sannibale, V.
Vanni, C.
Yamamoto, H.
Yoshida, S.
Citation: Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment, 2009; 598(3):737-753
Publisher: Elsevier Science BV
Issue Date: 2009
ISSN: 0168-9002
Statement of
Responsibility: 
Alberto Stochino, Benjamin Abbot, Yoichi Aso, Mark Barton, Alessandro Bertolini, Valerio Boschi, Dennis Coyne, Riccardo DeSalvo, Carlo Galli, Yumei Huang, Alex Ivanov, Szabolcs Marka, David Ottaway, Virginio Sannibale, Chiara Vanni, Hiroaki Yamamoto, Sanichiro Yoshid
Abstract: New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave interferometers of Advanced LIGO as part of the strategy to increase the sensitivity in the entire frequency range. In this perspective the LIGO Seismic Attenuation System (SAS) Group designed a new kind of seismic attenuation platforms for the Horizontal Access Module (HAM) and Basic Symmetric Chamber (BSC) vacuum chambers of the interferometers. HAM-SAS, a specific prototype for the HAM chambers, was constructed and installed in a test-bench laboratory. At the end of the commissioning time the prototype achieved many of the Advanced LIGO requirements about seismic isolation, stability and reliability. The lab experience also enabled us to finalize the design and indicated SAS as a solution worth considering for the seismic isolation of the advanced detectors.
Keywords: Gravitational waves interferometers; Seismic noise; Seismic isolation
Rights: Copyright status unknown
RMID: 0020112881
DOI: 10.1016/j.nima.2008.10.023
Appears in Collections:Chemistry and Physics publications

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