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[[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=7654|OMC report]] (Somiya)  * Next meeting: 2/19

Monday Meeting 0129

Participants

Kokeyama, Izumi, Nagano, Uehara, Moriwaki,Matsushima, Furuhata, Yokogawa, Yoshioka

Updates from projects

  • Tiltsensor installation o

=== Memo related to tilt sensor===

  • The tilt sensor is supported by JSPS Core-to-core.
  • The sensor can measure d\theta directly.
  • The principle is Mach-Zhender interferometer.
  • One tilt sensor was installed to MCE. For other two, no space for install.
  • A difference between OptLev and tilt sensor will be checked.

  • There are three tilt sensors; one installed.
  • No phase wrapping(Probably)
  • Absolute tilt angle can be measured
  • Dina mic range (5 mrad) is bigger than OptLev's(<1 mrad).

  • Install is not easy comparing to OptLev install, because there are 4 beam lines.

=== Memo related to RFAM in EOM===

  • AC/DC < 0.0001.

Plan for this week

Kamioka

  • 1/30 ISS work
  • 1/31-2/2 PMC commissioning

Topic of this week

  • Next meeting: 2/19

KAGRA/Subgroups/IOO/Meeting/Meeting20180129 (last edited 2018-01-29 13:10:14 by TomoyukiUehara)