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Participants: (eZuce meeting) Participants: Hirose, Aso, Kokeyama, Michimura (eZuce meeting)
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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
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  * 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.
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  * design review on June 26   * design review on June 26 at Titech {*}
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  * Updated lock acquisition section to derive velocity requirements for suspensions (see [[KAGRA/subgroup/ifo/MIF/Minutes20170410|ISC Meeting minutes 20170410]]) [Michimura]
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  * Needs to update lock acquisition section (see [[KAGRA/subgroup/ifo/MIF/Minutes20170410|ISC Meeting minutes 20170410]]) [Michimura]   * Paper? {*}
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 * bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5692|JGW-T1605692]]
  * needs to be updated based on updated schedule
 * bKAGRA Phase 1 initial alignment / commissioning plan [Michimura]: [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5692|JGW-T1605692]] {*}
  * updated based on current schedule
   * ETMX and ETMY cryopayload installation almost at the same time
   * MICH lock at room temperature before cooling down (instead of cooling down ETMY first)
   * AS cannot be used for room temperature MICH lock (SR3 not ready)
   * SR2 won't be ready by the end of March 2018
  * 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 [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=5595|JGW-T1605595]]
   * Initial alignment does not interfere with ITM Type-A installation work?
   * Evacuation of IXC/IYC compatible with Type-A installation work?
   * Initial alignment compatible with Pcal setup at EXA/EYA?
    * Meeting with Inoue on June 15 {*}
     * PD at EXA/EYA compatible with Pcal setup
     * Don't we need something like aLIGO baffle PDs for initial alignment after evacuation? Use Tcam (Pcal camera)?

 * 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

ISC Meeting on 2017/6/19 14:00 - 15:00

Participants: Hirose, Aso, Kokeyama, Michimura (eZuce meeting)

Next meeting

2017/7/3 14:00 - 15:00

back to Meetings page

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

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!]
    • Paper? {*}

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

    • updated based on current schedule
      • ETMX and ETMY cryopayload installation almost at the same time
      • MICH lock at room temperature before cooling down (instead of cooling down ETMY first)
      • AS cannot be used for room temperature MICH lock (SR3 not ready)
      • SR2 won't be ready by the end of March 2018
    • 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?
      • Initial alignment compatible with Pcal setup at EXA/EYA?
        • Meeting with Inoue on June 15 {*}

          • PD at EXA/EYA compatible with Pcal setup
          • Don't we need something like aLIGO baffle PDs for initial alignment after evacuation? Use Tcam (Pcal camera)?
  • 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/Minutes20170619 (last edited 2017-06-20 12:28:33 by YutaMichimura)