North tube of Virgo

The 3-km long building of Virgo hosts a vacuum tube of 1.3 m of diameter. The laser beam propagates back and forth inside this tube.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Infrastructures
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The 3-km long building of Virgo hosts a vacuum tube of 1.3 m of diameter. The laser beam propagates back and forth inside this tube.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Infrastructures
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Three racks hosting the electronics to control the superattenuator where a bench used to acquire the interference pattern is suspended and the electronics to control the optical elements installed on this bench.
On the background, vacuum enclosure of superattenuators are visible.
Credits: The Virgo collaboration/LAPP
Album: Instruments – Computing/Electronics
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The researcher is tuning the position of a mirror on an optical bench. For Advanced Virgo, new optical benches have been suspended and put in vacuum. The mechanics of the suspension is visible on the top part still opened. On-board electronics is attached below the suspended bench to reduce the number of (white) electrical cables going along the suspension.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Laser&Optics
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The Virgo infrared laser beam propagates back and forth inside the 3-km long vacuum tube.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Infrastructures
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The Virgo infrared laser beam propagates back and forth inside the 3-km long vacuum tube.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Infrastructures
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Superattenuators are used to suspend the main interferometer mirrors and benches to isolate them from the seismic ground vibrations. Here, a mechanical attenuator, part of a superattenuator, is being installed. The attenuator is then enclose in a vacuum tower.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Payloads/Suspensions/Mirrors
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Superattenuators are used to suspend the main interferometer mirrors and benches to isolate them from the seismic ground vibrations. Here, a superattenuator, surrounded by a scaffolding, is being installed. The attenuator is then enclose in a vacuum tower.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Payloads/Suspensions/Mirrors
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The Advanced Virgo central building hosts the laser, five suspended mirrors and five suspended benches in vacuum.
Credits: Cyril Frésillon/Virgo/Photothèque CNRS
Album: Instruments – Infrastructures
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The two 3-km arms of the interferometer meet the central building where the laser is generated, and five mirrors, including the beam-splitter mirror, are hosted. Optical benches used to acquire the interference pattern are also hosted in this building. On the left part, the other buildings host EGO offices.
Credits: the Virgo Collaboration/N. Baldocchi
Album: Instruments – Infrastructures
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