Dec 1st, 2011 Meeting of the 40m Technical Advisory Committee

Link to the slides https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=76382

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I. Personnel

  1. Current members
  2. Joe B gone to Louisiana...
  3. A new grad student Den joined
  4. Long visit by Mirko(AEI), Katrin(AEI), Keiko(LSU), and Anamaria (LSU)
  5. Current crew: Kiwamu Izumi (GS - March), Jenne Driggers (GS), Denis Martynov (GS), Jamie Rolllins (PD), Suresh Doravari (PD-April), Steve Vass, Koji, Rana

II. Overview of the presentation

III. Current Status / Recent and Ongoing Work for each subsystem

  1. Optics and Suspensions
    • An overview of the new optical layout (high lighting the differences from the previous plan)
      • ITMs and ETMs are dichroic, mass/finesse chosen such that the radiation pressure effects are enhanced
      • PRC is resonant with 11 MHz, 55 MHz and the carrier (PSL)
      • SRC is resonant with 55 MHz
      • Small Schnupp asymmetry
      • Additional optics installed to route the green beam from the end tables to the PSL table
      • Tip-tilts (with blades) are installed with new suspensions: some characterization done (SURF project)
    • Status:
      • All optics suspended and installed according to the new plan in the vacuum chamber
      • The chamber has been evacuated and has reached operational vacuum pressure
      • Arm lengths have been readjusted
      • Rearrangement of the green optics done
      • Rearrangement of pick off optics done (POX/POY/POP are now available)
      • A new procedure to diagonalize the suspension input matrix has been developed (link to poster in DCC)
  2. Length Sensing and Control
    • An overview of the Current status
      1. PSL locked to MC length (in IR) w/ HV. No feedback to MC length!
      2. X-end and Y-end laser frequency locked to each arm length (in 532nm)
      3. Single-mode fiber brings X-end / Y-end NPRO light to the PSL table for IR beat
      4. Handing off of the single-arm ALS was demonstrated
      5. Refinement of the LSC model and screens done
    • Work in progress:
      1. Y arm Green noise budget and handing off test
      2. automation/sequencing of single arm ALS acquisition
  3. Alignment Sensing and Control
    • An overview of the Current status
      1. MC alignment is controlled by WFS / IOO-WFS model w/ lockins, matrices, scripts, etc.
      2. Dither beam alignment system installed: uses suspension A2L to measure/maintain spot positions
    • Work in progress:
      1. Study of optimal WFS-ASC control in MC (incorporating the MC_TRANS_QPD for slow centering control)
  4. Electronics (RF system)
    • An overview of the new RF system
      • The layout and the measurement scheme
    • Status
      • Done: Multiple frequency RF generator to preserve the phase noise performance of the oscillator
      • Done: RF signal distribution (oscillators, splitters, amplifiers, etc.)
      • Done: Triple-Resonant EOM (New Focus KTP + resonant circuit) prototype installed
      • Ongoing: Finish the PDs / Install the photodiodes on the tables; characterization of all the PDs underway
      • Done: RFAM monitor installed
    • Work in progress:
      • Reduction of RFAM using a heater on the EOM crystal
  5. Control and Data Systems
    • Done: All of the new CDS hardware installed
      1. All 5 IO chassis and computers installed: c1lsc, c1sus, c1ioo, c1iscex, c1iscey
      2. New frame builder computer and code running, recording, and serving data
    • Done: Local damping has been achieved on all suspended optics with the new CDS system
    • Done: Have working reflected memory networks communicating between computers
      1. Both old GE Fanuc and the new Dolphin PCIE reflected memory networks installed
    • 1/2 Done: "Simulated plant" taken by JoeB to LLO
      1. virtual suspension can be controlled by the actual realtime controller

IV. Future Projects

  1. Comparison of the 40m and the LHO/LLO instruments
  2. Length Sensing and Control
    • Deterministic full lock acquisition through auxiliary green laser locking
    • Locking sequences: successively increasing the length of the primary length reference
    • Coherent lock of the three lasers (PSL and two auxiliary lasers)
  3. Adaptive seismic noise cancellation
    • seismometers are back in action installed near the 40m arms
    • determination of the transfer function matrices
    • closing the feedforward loops to arm cavities
    • implementing the algorithms in CDS
  4. What is the future of the 40m?
    • What to prototype (if anything) for LIGO 3G?
    • Dual-carrier / local readout schemes ?
    • Any use to speedmeter, variational readout schemes? (SQZ cav happening at MIT)

V. End


Previous TAC Meetings

TAC_Meeting-Dec_11 (last edited 2012-01-03 23:02:38 by localhost)