Differences between revisions 26 and 34 (spanning 8 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 26 as of 2020-12-30 19:34:49 → 
  Size: 670
  Editor: matteo.leonardi
  Comment:
+   ← Revision 34 as of 2021-01-11 22:56:40 → ⇥
  Size: 1131
  Editor: matteo.leonardi
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 5:
-|| [[|Meetings]] || [[LCGT/subgroup/ifo/MIF/OptParam|Optical Parameters (IOO)]] || [[http://gwwiki.icrr.u-tokyo.ac.jp/optics/database.cgi|Old MIR database]] ||
|| [[|Members]] || [[KAGRA/Subgroups/MIF/Simulation|Simulation]] ||  ||
|| [[|Task List]] ||  ||  ||
|| [[|Budget]] ||  || ||
|| [[|Interfaces]] ||  || ||
|| ||  || ||

Meetings

[[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4014| JGWdoc MIR Document and Drawing Tree]]
+|| [[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]] ||  || ||
-Line 19:
+Line 13:
+. 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