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||[[LCGT/subgroup/ifo/MIF/AuxOpticsLists|Auxiliary optics list from MIF's point of view]]||[[KAGRA/Subgroups/VAC|Layout Meeting]]|| ||[[LCGT/subgroup/ifo/MIF/OptParam|Optical Parameters]]||[[LCGT/subgroup/OCG/parametermeeting|Interface Parameter Meeting]]|| |
||[[LCGT/subgroup/ifo/MIF/AuxOpticsLists|Auxiliary optics list from MIF's point of view]]|| ||[[KAGRA/Subgroups/VAC|Layout Meeting]]||[[LCGT/subgroup/OCG/parametermeeting|Interface Parameter Meeting]]|| ||[[LCGT/subgroup/ifo/MIF/OptParam|Optical Parameters]]|| |
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|| [[LCGT/iLCGT/Subgroup/DiscussionRana2010|Discussion with Rana (2010)]]|| || [[LCGT/Meeting/RoadMap|Roadmap]] || |
||[[LCGT/iLCGT/Subgroup/DiscussionRana2010|Discussion with Rana (2010)]]||[[LCGT/Meeting/RoadMap|Roadmap]] || |
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||<#FF8080> ''''' Subsystems ''''' ||<#FF8080> ''''' Related subgroups '''''||<#FF8080> ''''' Notes ''''' || || [[LCGT/subgroup/AOS/StrayLight1|Stray Light Control]] || IOO, MIF, VAC, CRY, VIS || || || [[LCGT/subgroup/AOS/BeamReduceTelescope1|Beam Reducing Telescopes]] || IOO, MIF, VAC, CRY, VIS|| || || [[LCGT/subgroup/AOS/OptLev1|Optical Lever]] || IOO, MIF, VAC, CRY, VIS || || || [[LCGT/subgroup/AOS/CCD1|Imagers and Light Sources ]] || ISC, IOO || including CCD Monitors or equivalent|| || [[LCGT/subgroup/AOS/Viewport1|Viewports]] ||IOO, MIF, VAC, CRY, VIS, MIR || at room temperature || || [[LCGT/subgroup/AOS/BeamTarget1|Automatic Target System]] ||MIF, VAC, DGS || || || [[LCGT/subgroup/AOS/BeamModeProfiler1|Beam Profilers for large beams]] || IOO, MIF, VAC || || |
* [[LCGT/subgroup/AOS/StrayLight1|Stray Light Control]] * [[LCGT/subgroup/AOS/BeamReduceTelescope1|Beam Reducing Telescopes]] * [[LCGT/subgroup/AOS/OptLev1|Optical Lever]] * [[LCGT/subgroup/AOS/CCD1|Imagers and Light Sources ]] including CCD Monitors or equivalent * [[LCGT/subgroup/AOS/Viewport1|Viewports]] at room temperature * [[LCGT/subgroup/AOS/BeamTarget1|Automatic Target System]] * [[LCGT/subgroup/AOS/BeamModeProfiler1|Beam Profilers for large beams]] |
KAGRA Auxiliary Optics System
Contents
Objectives
The objectives of the subgroup "Auxiliary Optics System" (AOS) is to design and complete the auxiliary optics that physically, logically and consistently glue the main parts of the KAGRA interferometer together.
General Description
- Most of the AOS shall be fit to the vacuum chambers that had been already determined when the AOS group was established.
- Even if the vacuum chamber was not designed considering the space allocated for AOS, AOS are required for fully operating KAGRA, so we shall, by any means, pack them into the vacuum chambers if required.
References
Subsystems
Major subsystems
Imagers and Light Sources including CCD Monitors or equivalent
Viewports at room temperature
Other subsystems
- Squeezing? Squeezer optics
Local Sensors and Actuators LIGO's OSEM-like things utilized in vibration isolation system
Violine mode sensors or Wire position sensors utilized in vibration isolation system or in noise-hunting phase
Meetings