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 * bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=5274|JGW-T1605274]]  * bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5595|JGW-T1605595]]
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   * Nov 1, 2017: ETMY CRYp installation done
   * Nov 21, 2017: ETMY cool down starts
   * Feb 2, 2018: ETMX CRYp installation done
   * Feb 19, 2018: ETMY cool down starts
   * Oct 31, 2017: ETMY CRYp installation done
   * Dec 8, 2017: ETMY cool down starts
   * Feb 13, 2018: ETMX CRYp installation done
   * Mar 2, 2018: ETMY cool down starts

ISC Meeting on 2016/9/20 14:00 - 15:00

Participants:

Next meeting

2016/10/17 14:00 - 15:00 ??

back to Meetings page

Agenda

  • bKAGRA Phase 1 optical configuration study [Michimura]
    • summary: JGW-T1605595

      • UPDATE: no PR-related adjustments before Michelson operation
    • ASC [Enomoto]
      • noise study by NoiseBudget [Enomoto]

        • Enomoto volunteered to do ASC NoiseBudget; meeting on Sept 27

      • effect on WFS from RF HOMs [who?]
    • check if reference spheres for PR mirrors are available at Caltech [Hirose]
      • 9.0m (CC), 11.5m (CC), 6.5m (CC), 5.0m (CC), 34m (CX), 36m (CX) were available
      • PR2/SR2 is -3.0764m/-2.9872m and PR3/SR3 is 24.9165m. Maybe 5.0m TS can be used for PR2/SR2.
      • what about PR3/SR3, PRM/SRM?
    • check if IMC length stability and others are compatible with 3-km PRMI [Michimura]
  • bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: JGW-T1605595

    • beam profiling plan should be compatible with vacuum plan; MIF will lead the planning
      • not only PR2-PR3 but also IMMT1-IMMT2
    • how to extract AS beam should be fixed by MIF
    • according to CRYp current schedule;
      • Oct 31, 2017: ETMY CRYp installation done
      • Dec 8, 2017: ETMY cool down starts
      • Feb 13, 2018: ETMX CRYp installation done
      • Mar 2, 2018: ETMY cool down starts
    • we need more time for PR-ETMY cavity

      • no more PR-ETMY cavity before Michelson operation
    • do we have enough time for TMS measurement and PR2-PR3 adjustment?
    • initial alignment plan including green is taken cared by MIF [confirmed with Kawamura, Moriwaki on Aug 30]
  • bKAGRA Phase 1 analog electronics (Analog Electronics for ISC) [Michimura]

    • Quad IQ Demodulator heat-up issue
      • 1st stage amp is heating up
      • we have to decide if we need 1st stage amp or not

    • remake of Quad IQ Demodulator LSC to ASC [Michimura->Niigata students?; by 2016.10]

      • MIF will take care instead of AEL
      • mass production will be taken care by AEL
      • 4-way splitter (Mini-Circuits ZFSC-4-1-S+) arrived at Kamioka -> Mozumi office loft

    • RF Distribution Amplifier [Michimura->Niigata students?; by 2016.10]

      • we will omit RF monitor for now, and add them later
      • Nakano found front/rear panels -> Mozumi office loft

      • ordered RF amp (Wenzel LNBA-11-23-CK-100-15)
      • 8-way splitter (Mini-Circuits ZCSC-8-1+), coupler (Mini-Circuits ZX30-20-4) arrived at Kamioka -> Mozumi office loft

      • cables and connectors to assemble one chassis by hand arrived at Kamioka -> Kokeyama's desk

      • basically copy of LIGO-D1000124, but we will omit Interface for the first stage

      • asked AEL to make RF amplifier interface board (which is also used for Frequency Doubler) [Michimura]
    • RF Patch Panel modification [Michimura->Niigata students?]

      • one by one by hand is tough; outsource?
    • Electronics request meeting with Miyakawa/Kamiizumi on Aug 24
      • photos of the assembled chassis are helpful for AEL
        • does anyone have a photo of Frequeny Doubler? LIGO-D1002178

          • asked Izumi and Kokeyama
  • RF PDs and RF QPDs
    • RF PD / RF QPD noise and transimpedance characterization [who?]
    • RF PD modification [who?]
      • fix DC path
      • solve single supply issue (RF PDs easily break when accidentally supplied with single)
      • fix plugs so that Dsub 9pin cable fixes better
  • Output optical tables [Michimura] (OutputTables wiki)

    • Kawamura suggested to move this task from IOO to MIF

    • vacuum optics to extract beams for each port (except for REFL and AS DC) and related beam shutters will also be MIF task
    • MIF and IOO agreed, SEO agreed, next step is budget migration
  • 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 (FSR for IMC))
      • seeking for vendors
    • MIF and IOO agreed to use 13.78 MHz (~= f2/8*2.45) for IMC sideband (JGW-T1605493)

    • MIF agreed to use 32 MHz and 33 MHz for ALS sidebands JGW-T1605626

    • may be IMC sideband (and ALS sidebands) should also needs to be phase locked with f1/f2/f3 to avoid "whistling noise"
  • Arm Length Stabilization plan (JGW-T1605353)

    • NoiseBudget [Kambara]

      • results agreed with Tatsumi Simulink model
      • include fiber noise (fiber setup is different from Tatsumi model)
        • fiber length? how to do the wiring?
      • include phase noise from mirror vibration for IR beat setup (it is one of the limiting noise source for aLIGO)
      • schedule and plan for the procurement of circuits should be fixed soon
        • keep in touch with AEL group


  • Aperture of sapphire test mass
    • recoil mass aperture is OK for diffraction loss and scattering noise
    • what is the baffle aperture?
  • bKAGRA optical layout around PRC
    • POY clipping issue will be solved by modifying PR3 optical bench suspension [Shoda]
    • we need layout CAD for POY pickoff mirror, POP pickoff mirror to design baffles
      • budget for baffles around POY and POP were shifted to next FY [SEO]
  • iKAGRA post-run calibration mystery [Aso]
  • Requirement for the noise of watchdogs for coil drivers [Aso]
    • recent result show dR < 1e-7 Ohm/rtHz, so it may meet the requirement

    • slow (~20 min) drift at dR ~ 5e-4 Ohm -> this should be negligible

  • Viewport quality for GV between SRM and OMMT [Akutsu]
    • aLIGO case: SRM-OFI-viewport, KAGRA case: SRM-viewport-OMMT-OFI
    • aLIGO viewport is always closed
    • if we need super quality viewport, we have to decide soon

  • BS baffle could make contract defect? (LIGO-T1000090)

    • ask Akutsu and Hiro
    • BS has 370 mm dia and beam at BS is 2*36 mm dia. So, it should be in principle OK. But recoil mass aperture should be considered.
  • bKAGRA ISC cabling [Michimura/Doi]
    • announced to IOO mailing list
    • need to update the cabling diagram
  • Mirror absorption measurement status [Hirose]
  • Output optics status [Somiya]
    • suspensions for OMMT1/2 is same as IMMT1/2 (driver list for now: JGW-L1605334)

    • 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
    • OMC suspension requirement cross check [Somiya]

    • OFI, OMMT, OMC meeting on 2016.9.14
      • design suspended table similar to TMS?
  • Magnetic noise, actuator noise calculation for cryogenic payload [Michimura]
    • Ask Tomaru about the parameters and actuator design, range

  • Task list update (TaskList) [Michimura]

KAGRA/subgroup/ifo/MIF/Minutes20160920 (last edited 2016-09-20 21:05:18 by YutaMichimura)