Differences between revisions 1 and 37 (spanning 36 versions)

Mirror Subsystem (MIR)

Beaurocracy	Interferometer	Old pages
Meetings	MIR Document and Drawing Tree (JGWdoc)	Old MIR database
Members	Optical Parameters (IOO)
Task List	Simulation (IOO)
Interfaces
Papers

System definition

1. Procurement and preparation of KAGRA core optics:

sapphire optics (Input and End Test Masses – ITMs & ETMs) and
large fused silica optics (Input Mode Cleaner mirrors, Power Recycling and Signal Recycling Cavities mirrors, Input and Output Mode Matching Telescopes Mirrors and Beam Splitter)

2. Improve current KAGRA core optics

-  ⇤ ← Revision 1 as of 2010-11-08 12:03:16 → 
  Size: 37
  Editor: KentaroSomiya
  Comment:
+   ← Revision 37 as of 2021-01-11 23:31:01 → ⇥
  Size: 1211
  Editor: matteo.leonardi
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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-= Mirror =
+## page was renamed from LCGT/subgroup/mirror
= Mirror Subsystem (MIR) =
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-Under construction...
+||<#3090e0 style="text-align:center; ">'''Beaurocracy''' ||<#3090e0 style="text-align:center">'''Interferometer''' ||<#3090e0 style="text-align:center">'''Old pages''' ||
|| [[KAGRA/Subgroups/MIR/Meetings|Meetings]] || [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4014| MIR Document and Drawing Tree (JGWdoc)]] || [[http://gwwiki.icrr.u-tokyo.ac.jp/optics/database.cgi|Old MIR database]] ||
|| [[KAGRA/Subgroups/MIR/Members|Members]] || [[LCGT/subgroup/ifo/MIF/OptParam|Optical Parameters (IOO)]] ||  ||
|| [[KAGRA/Subgroups/MIR/TaskList|Task List]] || [[KAGRA/Subgroups/MIF/Simulation|Simulation (IOO)]] ||  ||
|| [[KAGRA/Subgroups/MIR/Interfaces|Interfaces]] ||  || ||
|| [[KAGRA/Subgroups/MIR/Papers|Papers]] ||  || ||


== System definition ==
1. Procurement and preparation of KAGRA core optics:
  * sapphire optics (Input and End Test Masses – ITMs & ETMs) and 
  * large fused silica optics (Input Mode Cleaner mirrors, Power Recycling and Signal Recycling Cavities mirrors, Input and Output Mode Matching Telescopes Mirrors and Beam Splitter)
2. Improve current KAGRA core optics