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== Minutes ==
 * Actuator noise modeling [Michimura]
  * Noise from heat links is one of the most interesting issues to be discussed
   * Ask people about the heat link vibration estimation status
 * bKAGRA Phase 1 initial alignment
  * Poke Akutsu for baffle PD for initial alignment use [Michimura]
 * IR/green steering mirrors
  * No objections for proposed mirror specs

ISC Meeting on 2017/7/3 14:00 - 15:00

Participants: (eZuce meeting)

Next meeting

2017/7/31 14:00 - 15:00 (July 17 is a holiday)

back to Meetings page

Agenda

  • PSL EOM Layout re-consideration [Enomoto] (JGW-T1706748)

    • Delay-line length decided to be 2.66 m (instead of 8.88 m)
    • Modulation phase between f1 AM and PM is always aligned (we need this to be aligned)
    • Modulation index needed at each EOM is less than measured maximum index by Uehera (JGW-T1605611)

    • Optickle simulation by Kohei Yamamoto
      • simulation on imperfections (MZ arm asymmetry, MZ lock, EOM phase difference control etc.)
      • start with hand calculation, simple setups, and then to full IFO simulation
      • meeting with him on June 6.
    • Requirement on carrier power loss?
    • Comment from Stefan Ballmer {*}

      • Similar calculation was done in LIGO in the past. Displacement noise requirement for MZ was tough (~1e-14 m/rtHz).
      • Any in-air interferometer suffer from jitter and frequency noise which cannot be suppressed.
  • OFI and OMC status? [Somiya]
    • look for OFI with larger aperture [Somiya]
    • output optics task sharing status?
    • OMC baseplate issue?
    • design review on June 26 at Titech {*}

  • Actuator noise modeling [Michimura,Miyamoto] (JGW-T1503453)

    • Updated magnet size for cryopayload marionette (ActuatorDesign wiki)

    • Updated lock acquisition section to derive velocity requirements for suspensions (see ISC Meeting minutes 20170410) [Michimura]

    • Needs to implement frequency noise, but FSS modeling with ALS is complicated [student!]
    • Discuss mirror vibration from heat link {*}

  • bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: JGW-T1605692

    • Fixed mirrors for AS port (including SR2)
    • Some comments from the Chief Meeting
      • Revised schedule seems compatible with PRMI. Why not?
        • PRMI is an option after achieving the Phase 1 goal, if it doesn't delay the final bKAGRA JGW-T1605595

      • Initial alignment does not interfere with ITM Type-A installation work?
      • Evacuation of IXC/IYC compatible with Type-A installation work?
      • Baffle PDs for initial alignment in vacuum
        • confirmed with Akutsu that he is thinking of putting PDs on narrow angle baffles
        • vibration isolation for baffle PDs necessary?
        • possibility of seeing beams with Tcam
  • IR/green steering mirrors [Michimura] (see [kagra-isc 01649]) {*}

    • for POP/POS and green steering in PR2/SR2 chamber, needs picomotors and ~40 cm pedestals
    • need this by the end of August 2017 (after PR2 installation on June, before IR initial alignment starts on September)
    • proposed mirror specs
      • HR reflectivity: more than 99% for both 1064nm and 532nm
      • AR refectivity: less than 0.3 % for 1064nm, similar for 532nm
      • incient angle: 20-45 deg, s-polarization
      • radius of curvature: flat
      • size: 2-inch
      • wedge: 1 deg
      • substrate: Fused Silica
      • surface quality: λ/20, 0.1 nm rms roughness

See this page for other agendas.

KAGRA/subgroup/ifo/MIF/Minutes20170703 (last edited 2017-07-03 15:20:11 by YutaMichimura)