Differences between revisions 18 and 35 (spanning 17 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 18 as of 2020-06-18 11:25:16 → 
  Size: 239
  Editor: matteo.leonardi
  Comment:
+   ← Revision 35 as of 2021-01-11 23:29:23 → ⇥
  Size: 1168
  Editor: matteo.leonardi
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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-= Mirror =
+= Mirror Subsystem (MIR) =
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-[[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4014| JGWdoc MIR Document and Drawing Tree]]
+||<#E08030 style="text-align:center; ">'''Beaurocracy''' ||<style="text-align:center">'''Interferometer''' ||'''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]] ||  || ||
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-http://gwwiki.icrr.u-tokyo.ac.jp/optics/database.cgi
+== 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