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 |