Differences between revisions 24 and 31 (spanning 7 versions)

Mirror Subsystem (MIR)

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

System definition

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)

Improve current KAGRA core optics

-  ⇤ ← Revision 24 as of 2020-12-30 19:30:35 → 
  Size: 743
  Editor: matteo.leonardi
  Comment:
+   ← Revision 31 as of 2021-01-11 19:56:40 → ⇥
  Size: 1069
  Editor: matteo.leonardi
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 5:
-||[[|Meetings]] ||[[|Optical Layout]] ||[[http://gwwiki.icrr.u-tokyo.ac.jp/optics/database.cgi|Old MIR database]] ||
||[[|Members]] ||[[LCGT/subgroup/ifo/MIF/OptParam|Optical Parameters (IOO)]] || ||
||[[|Task List]] ||[[|IOO Parameters]]  || ||
||[[|Budget]] ||[[|Arm Length Stabilization]] || ||
||[[|Interfaces]] ||[[|Noise Budget]]  || ||
|| || [[KAGRA/Subgroups/MIF/Simulation|Simulation]] || ||

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| JGWdoc MIR Document and Drawing Tree]] || [[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]] ||  || ||
-Line 19:
+Line 12:
+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)
Improve current KAGRA core optics