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Автор The VIRGO Collaboration (presented by Giovanni Losurdo)
Дата выпуска 2002-04-07
dc.description The VIRGO superattenuator (SA) is effective in suppressing seismic noise below the expected thermal noise level above 4 Hz. However, the residual mirror motion associated with the SA normal modes can saturate the interferometer control system. This motion is reduced by implementing a wideband (DC–5 Hz) multidimensional active control (the so-called inertial damping) which makes use of both accelerometers and position sensors and of a digital signal processing (DSP) system. Feedback forces are exerted by coil–magnet actuators on the top of an inverted pendulum pre-isolator stage. The residual root mean square motion of the mirror in 10 s is less than 0.1 μm.
Формат application.pdf
Издатель Institute of Physics Publishing
Название The inertial damping of the VIRGO superattenuator and the residual motion of the mirror
Тип paper
DOI 10.1088/0264-9381/19/7/354
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 19
Первая страница 1631
Последняя страница 1637
Аффилиация The VIRGO Collaboration (presented by Giovanni Losurdo); Istituto Nazionale di Fisica Nucleare—Sezione di Firenze, Lgo E Fermi, 2, Firenze, Italy
Выпуск 7

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