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  * we had OFI telecon on June 24 [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5313|JGW-G1605313]]
   * reduce number of output steering mirrors from two to one?
   * move OFI postion?

ISC Meeting on 2016/6/27 14:00 - 15:00

eZuce:

Participants:

Adgenda

  • bKAGRA Phase 1 optical configuration study [Michimura]
    • HOM structure / LSC / ASC check [Michimura]
      • initiated Optickle 2 modeling: KAGRAOptickle SVN (login required)

      • Optickle (Optickle2) seminar on July 1 densuke

      • length sensing matrix is OK
    • continue checking dummy ETM availability [Hirose]
      • cost estimate arrived
    • check if reference spheres for PR mirrors are available at Caltech [Hirose]
    • check if IMC length stability and others are compatible with 3-km PRMI [Michimura]
    • check if dummy payload is quiet enough to make PRMI [Michimura]
  • bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: JGW-T1605274

    • we actually had only two months for room temperature PRMI with dummy payload
    • what should we do?
  • bKAGRA Phase 1 analog electronics request for AEL (Analog Electronics for ISC) [Michimura]

    • request for AEL [Michimura]
    • Quad IQ Demodulator heat-up issue
    • remake IQ Demodulator LSC to ASC temporarily for IMC WFS by 2016.10
      • confirmed with Miyakawa that AEL will take care
    • assemble RF Distribution Amplifier
      • MIF will take care of assembling and purchasing with AEL budget
      • in the process of ordering RF amp (Wenzel LNBA-10-23-CK or LNBA-11-23-CK)
      • in the process of ordering RF splitter (Mini-Circuits ZCSC-8-1+)
    • RF Patch Panel modification
  • RF generation scheme [Michimura]
    • f1 = 3/8*f2, f3 = 10/8*f2
    • we need 2*f1, 2*f2, f3-f1, f3-f2 as well
    • use harmonics generator (x2, x3, x6, x8, x10, x16 for f2/8 = 5.62698725 MHz)?
    • use multiple signal generators with frequency doubler and differential frequency generator?


  • bKAGRA optical layout around PRC [Aso]
  • iKAGRA post-run calibration mystery [Aso]
  • Requirement for the noise of watchdogs for coil drivers [Aso]
    • if watchdog resistance noise should be less than DAC noise, dR < 6e-8 Ohm/rtHz (High Power Coil Driver case), dR < 5e-6 Ohm/rtHz (Low Power Coil Driver case), both at 10 Hz

    • too meet actuator noise requirement, dR < 8e-5 Ohm/rtHz (for BS/SRs), dR < 6e-5 Ohm/rtHz (for PRs), both at 10 Hz

    • watchdog resistance fluctuation was measured to be dR < ~1e-6 Ohm (measurement noise limited) (JGW-E1605270)

    • see, also, VISMinutes20160603

  • Viewport quality for GV between SRM and OMMT [Akutsu]
  • BS baffle could make contract defect? (LIGO-T1000090) [Akutsu,Hiro]

  • bKAGRA ISC cabling [Michimura/Doi]
    • Doi-san said he will help.
  • Mirror absorption measurement status [Hirose]
  • Output optics status [Somiya]
    • suspensions for OMMT1/2 is same as IMMT1/2, ask Takahashi-san to add drivers to his list: JGW-L1605193

    • we have to make vacuum compatible PD/QPD for OMC by 2018.3
    • beam shutter: prototype done, AR coating and driver circuit design not yet
    • we had OFI telecon on June 24 JGW-G1605313

      • reduce number of output steering mirrors from two to one?
      • move OFI postion?
  • Magnetic noise, actuator noise calculation for cryogenic payload [Michimura]
  • Task list update (TaskList) [Michimura]

Next meeting

2016/7/11 14:00 - 15:00 (Michimura might be travelling)

back to Meetings page

KAGRA/subgroup/ifo/MIF/Minutes20160627 (last edited 2016-07-25 10:29:58 by YutaMichimura)