Differences between revisions 2 and 29 (spanning 27 versions)

Output Mode-cleaner

Meetings

Shot noise increase due to the signal reduction by the OMC and residual spatial higher order modes after the OMC should be less than 5%.

TBD

TBD

-  ⇤ ← Revision 2 as of 2014-01-05 00:46:52 → 
  Size: 290
  Editor: KentaroSomiya
  Comment:
+   ← Revision 29 as of 2018-03-13 14:39:34 → ⇥
  Size: 1188
  Editor: KentaroSomiya
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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-[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1875|Report by Kumeta]]
+== Meetings ==
 * [[KAGRA/Subgroups/IOO/OMC/meeting2016|2016]]
 * [[KAGRA/Subgroups/IOO/OMC/meeting2017|2017]]
 * [[KAGRA/Subgroups/IOO/OMC/meeting2018|2018]]
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+Line 8:
-=== Requirement ===
+== Task List ==
 * [[KAGRA/Subgroups/IOO/OMC/Tasks|here]]

== Reports ==

 * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8043|OMC Design Document]]

== Requirement ==
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+Line 18:
+== Optical Design (updated 17/11/14) ==
||item||RoC||Beam Raidus||
||OMMT1||13.16m||4.46mm||
||OMMT2||44.39m||2.68mm||
||OSTM||flat||TBA||
||OMC1||flat||444um||
||OMC2||flat||444um(X)/447um(Y)||
||OMC3||1.80m||604um||
||OMC4||1.80m||604um||
||DCPD||--||562um||

||Space||Distance||AOI||
||SRM-OMMT1||5.63m||3.07deg||
||OMMT1-OMMT2||2.60m||3.07deg||
||OMMT2-OSTM||2.97m||90deg||
||OSTM-OBS1||0.30m||90deg||
||OBS1-OMC1||0.03m||0.078deg||
||OMC1-OMC2||0.357m||3.00deg||
||OMC2-OMC3||0.359m||3.00deg||
||OMC3-OMC4||0.357m||3.00deg||
||OMC4-OMC1||0.359m||3.00deg||

== Suspension Design ==

TBD

== Control Scheme ==

TBD