First locking of the Virgo central area interferometer with suspension hierarchical control

被引:13
作者
Acernese, F
Amico, P
Arnaud, N
Babusci, D
Barillé, R
Barone, F
Barsotti, L
Barsuglia, M
Beauville, F
Bizouard, MA
Boccara, C
Bondu, F
Bosi, L
Bradaschia, C
Bracci, L
Braccini, S
Brillet, A
Brisson, V
Brocco, L
Buskulic, D
Calamai, G
Calloni, E
Campagna, E
Cavalier, F
Cella, G
Chassande-Mottin, E
Cleva, F
Cokelaer, T
Confort, G
Corda, C
Coulon, JP
Cuoco, E
Dattilo, V
Davier, M
De Rosa, R
Di Fiore, L
Di Virgilio, A
Dujardin, B
Eleuteri, A
Enard, D
Ferrante, I
Fidecaro, F
Fiori, I
Flamino, R
Fournier, JD
Frasca, S
Frasconi, F
Gammaitoni, L
Gennai, A
Giazotto, A
机构
[1] EGO, I-56021 Cascina, PI, Italy
[2] Univ Naples Federico II, I-80126 Naples, Italy
[3] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[4] Univ Salerno, I-84084 Salerno, Italy
[5] Univ Perugia, I-06123 Perugia, Italy
[6] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[7] Univ Paris 11, CNRS, IN2P3, LAL, F-91898 Orsay, France
[8] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[9] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[10] Univ Pisa, I-56127 Pisa, Italy
[11] Lab Annecy Le Vieux Phys Particules Chemin Bellev, F-74941 Annecy Le Vieux, France
[12] ESPCI, F-75005 Paris, France
[13] Observ Cote Azur, Dept Fresnel Interferometrie Laser Gravitat & Ast, F-06304 Nice 4, France
[14] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy
[15] Univ Florence, I-50125 Florence, Italy
[16] Osserv Astrofis Arcetri, I-50125 Florence, Italy
[17] Univ Urbino, I-61029 Urbino, Italy
[18] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[19] Univ Roma La Sapienza, I-00185 Rome, Italy
[20] IPNL, SMA, F-69622 Villeurbanne, France
关键词
gravitational waves detectors; interferometer; control systems; servo and control equipment; vibration isolation;
D O I
10.1016/j.astropartphys.2003.10.003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Operation of the central portion of Virgo as a simple 6 in Michelson interferometer has given the first demonstration of the possibility to control an interferometer suspended from Virgo full scale multistage seismic attenuators using information derived from the interferometer locking signal. A special role in the control is played by the first stage of these suspensions, an inverted pendulum: besides its seismic preisolation action, this stage has positioning dynamics of several mm, and it allows to exert a very low frequency control at the tipper level of the suspension using the interferometer fringe signal. The application of this feedback to the top-stage of the suspension allows corrections of drifts, such as tidal ones, at a stage of the suspension where a large dynamic range in displacements is available, without introducing noise at the level of the mirror, resulting in a significant reduction of the lock keeping force applied directly on the mirror at the lowest stage of the attenuator. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:629 / 640
页数:12
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