Advanced LIGO subsystems
are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem.
Auxiliary Optics | Core Optics |
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Data Acquisition | Data and Computing Systems |
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Facilities Modifications |
Input Optics |
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Interferometer Control |
Pre-Stabilized Laser |
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Seismic Isolation |
Suspensions |
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Advanced LIGO News
New Laser Enclosures Take Shape
February 2011
Prior to entering the vacuum system, LIGO's laser light passes from the main lasers through a number of additional optical components on long optical tables. The contents of these tables, including the lasers themselves, comprise the "Pre-Stabilized Laser" subsystem, or PSL. The Advanced LIGO (aLIGO) PSL makes up the only portion of a detector that will reside outside the vacuum once the detector reaches "science mode," its most sensitive operating state. In order for the PSL to deliver ultra-stable light into the vacuum, aLIGO will employ PSL enclosures of far greater size and thickness than their Initial LIGO predecessors. The iLIGO enclosures were cabinet-like structures on legs. The aLIGO enclosures are walled-in rooms with ceilings up to 13 feet in height that will offer improved acoustic shielding and a higher level of contamination control. The PSL tables are those from Initial LIGO but the tables will rest on new legs (hollow and filled with tiny glass beads) that reduce table vibrations.
Readers can easily imagine that the construction of small houses inside LIGO's Laser and Vacuum Equipment Areas (LVEA's) limits the extent of sensitive work that can occur in other areas of the LVEA's. aLIGO schedulers must factor the impacts of PSL enclosure production into their overall work flows. Surgery wouldn't seem desirable on a day when bolt holes were being drilled in the operating room floor. Similarly, LIGO needs to segregate noisy construction tasks from sensitive alignment and installation activities in the project schedule.
Image 1: PSL table moving from temporary storage to final location.
Image 2: Landing the table on new aLIGO legs.
Image 3: The acoustic enclosure.
Image 4: Additional space for clean prep.
Image 5: The door is on.
Image 6: Nearing completion with HEPA filtering undergoing installation.
aLIGO News Archive
August 2016 -- LIGO Reports O1 Results
June 2016 -- Another Black Hole Merger
Feburary 2016 -- First Gravitational Wave Detection
November 2015 -- O1 Progress Report
August 2015 -- Final Preparations for the O1 Run
February 2015 -- Hanford's H1 Achieves Two-Hour Lock
July 2014 -- Livingston Commissioning Progress
June 2014 -- Livingston Locks the L1 Interferometer
December 2013 -- Livingston Installs End Station Payloads
September 2013 -- Half-interferometer Test Closes
June 2013 -- DRMI Test at Livingston
May 2013 -- Arm Length Stabilization
November 2012 -- One-arm Test at Hanford
September 2012 -- LIGO Begins Locking Optical Cavities
August 2012 -- Installation of Stray Light Controls
July 2012 -- Small Optic Suspenions Enter L1
April 2012 -- First Cartridges Enter the Vacuum
November 2011 -- Glass Fiber Suspensions in Production
October 2011 -- Continued Suspension Development
July 2011 -- Hanford's H2 Becomes a 4K
May 2011 -- LLO Laser Installation Completed
March 2011 -- Input and Output Tubes Undergo Removal
February 2011 -- New Laser Enclosure Takes Shape
December 2010 -- Initial LIGO Comes Out of the Vacuum
October 2010 -- S6 Yields to Advanced LIGO
Explore Advanced LIGO
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Instrumentation and Astrophysics
An Overview of the Upgrades
The International Partnership
Science Impacts
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