Control System Design for the LIGO Pre-stabilized Laser

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dc.creatorAbbott, R.
dc.creatorKing, P.
dc.date2001-11-20
dc.date.accessioned2026-07-07T05:46:42Z
dc.date.available2026-07-07T05:46:42Z
dc.descriptionTo meet the strain sensitivity requirements [1], [2] of the Laser Interferometer Gravitational Wave Observatory (LIGO), the laser frequency and amplitude noise must initially be reduced by a factor of 1000 in the pre-stabilized portion of the interferometer [3]. A control system was implemented to provide laser noise suppression, data acquisition interfaces, diagnostics, and operator control inputs. This paper describes the VME-based analog and digital controls used in the LIGO Pre-stabilized Laser (PSL).
dc.description3 Pages, 3 figures, ICALEPCS Conference
dc.identifierhttps://arxiv.org/abs/physics/0111155
dc.identifierhttp://arxiv.org/abs/physics/0111155
dc.identifiereConf C011127 (2001) WEAP038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/84431
dc.subjectInstrumentation and Detectors
dc.titleControl System Design for the LIGO Pre-stabilized Laser
dc.typetext

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