Properties of seismic noise at the Virgo site

被引：24

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

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 ^{[1
]}

Flaminio, R

Fournier, JD

Frasca, S

Frasconi, F

Gammaitoni, L

Gennai, A

Giazotto, A

Giordano, G

机构：

[1] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy

[2] Univ Naples Federico II, I-80126 Naples, Italy

[3] Univ Salerno, I-84084 Salerno, Italy

[4] Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France

[5] European Gravitat Observ, Pisa, Italy

[6] Ist Nazl Fis Nucl, Sez Firenze, I-50125 Florence, Italy

[7] Univ Florence, Dipartimento Fis, I-50019 Florence, Italy

[8] Osservatorio Arcetri, I-51125 Florence, Italy

[9] Univ Urbino, Ist Fis, I-51019 Urbino, Italy

[10] Ist Nazl Fis Nucl, Sez Lab Nazl Frascati, I-00044 Frascati, Italy

[11] Inst Phys Nucl, F-69622 Villeurbanne, France

[12] Observ Cote Azur, F-06034 Nice, France

[13] LAL, F-91898 Orsay, France

[14] CNRS, IN2P3, F-91898 Orsay, France

[15] Univ Paris 11, F-91898 Orsay, France

[16] Ecole Super Phys & Chim Ind Ville Paris, F-75005 Paris, France

[17] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[18] Univ Perugia, I-06123 Perugia, Italy

[19] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[20] Univ Pisa, I-56127 Pisa, Italy

[21] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[22] Univ Roma La Sapienza, I-00185 Rome, Italy

来源：

CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 05期

关键词：

D O I：

10.1088/0264-9381/21/5/008

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of a study of the major low-frequency sources of seismic activity at the Virgo site. These sources are of natural and human origin: oceanic microseism (below 1 Hz), local traffic and human activity on site (below 10 Hz). Using data collected during the commissioning of the central Virgo interferometer (CITF) we have measured the seismic coupling to the interferometer, demonstrating that seismic noise contributed to the CITF dark fringe noise only below approximately 2 Hz.

引用

页码：S433 / S440

页数：8

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