Weekly Report for Week Ending December 14, 2000


 Exec. Comm. Agenda
Highlights
LSC
Administration
Hanford Observatory
Livingston Observatory
MIT
Caltech
Detector
40 Meter
TNI
LASTI
Data Analysis
LIGO II/Adv. R&D
Past Weekly Reports

The LIGO Executive Committee Agenda for Monday  December 18, 2000 will be:
 (Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

  1. Announcements
  2. LSC Issues (Weiss)
  3. Comments on Weekly Report
  4. WBS 1 LIGO I Construction (Lindquist)
  5. WBS 2 LIGO Lab Operations
  6. WBS 3 and 4  Advanced R&D and LIGO II (Sanders)
Executive Committee only 11:30 - noon   Topics:
 

Special Items:  PAC 9 and GWDAW reprise


Special Announcements:


Weekly Report Highlights

The TNI arm test cavity lock has been achieved!
 


LSC Issues (Weiss)


No report.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


WBS 1.2 LIGO Operations--Administration


LIGO Weekly Site Telecon (Lindquist)

No Report this week.

PROPERTY MANAGEMENT (Chargois)

From: Ed Chargois <chargois_e@ligo.caltech.edu>


DOCUMENT CONTROL CENTER (Turner, Mak)

>From: Linda Turner - turner@ligo.caltech.edu>

Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
 

ACCOMPLISHMENTS

REMINDER to all LIGO-ites
From: Cleveland Mak <mak_c@ligo.caltech.edu>
Packages Faxes
In 58 34
Out 16 32

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.


COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Akutagawa, Kaufman)

From: Esther Cunningham <esther@ligo.caltech.edu>

Press here for ACCOUNTS PAYABLE HISTORY DATA.
 
 
Date Incoming Invoices And Receivers Wires Large Contract Invoices
December 8, 2000 10 0 0
December 11, 2000 12 0 0
December 12, 2000 12 1 0
December 13, 2000 3 0 0
December 14, 2000 11 0 0
Totals 48 1 0

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>

From: Florence Kaufman <fkaufman@ligo.caltech.edu>

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

From: irena@ligo.caltech.edu (Irena Petrac)

From: Ed Jasnow <jasnow@ligo.caltech.edu>


Support (Elizabeth Wood) <ewood@ligo.caltech.edu>

Dorothy Lloyd

Irene Baldon Rita Torres Elizabeth K. Wood

Advanced LIGO (Frey, Petrac)

From: Thomas Frey <tfrey@ligo.caltech.edu>

Progress Period from 12.8 to 12.14

Accomplishments:

Schedule 12.15 to 12.21:
From: irena@ligo.caltech.edu (Irena Petrac)



WBS 1.4.1.2   Project Controls (LIGO Construction)



Reports (Lindquist)

Annual Report:  There will be an Annual Report due as of the end of November.  I will be requesting inputs from the usual bunch mid-December after the dust from the proposal has a chance to settle a bit.  I propose to keep this report moderate in size, about the size and complexity of a Quarterly Report, to minimize the burden.



Change Control/Contingency (Lindquist)

The following Change Requests have been submitted:
 

CR-000018 WBS 1.1.4 Curbing for Service Roads at Livingston G. Stapfer
CR-000019 WBS 1.2 Additional Lab Equipment D. Coyne

Press for the latest Contingency Needs Projection.


COST SCHEDULE CONTROL SYSTEMS (Duncan, Akutagawa)

From: Kris Duncan <kris@ligo.caltech.edu>

From: Cindy Akutagawa <cindy@ligo.caltech.edu>

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

From: Ed Jasnow <jasnow@ligo.caltech.edu>

From: irena@ligo.caltech.edu (Irena Petrac)

LIGO Hanford Observatory (LHO) Operations (Raab)


General Items:
--------------
(F. Raab)
 

Work is continuing on a number of fronts, most of which are either unremarkable
or reported elsewhere. We had a meeting with Peter Fritschel, Rolf Bork, Dave
Barker, Dennis Coyne, Hugh Radkins and Fred Raab to discuss implementation of
tidal feedforward compensation and how it might interact with plans for possible
tidal feedback and for compensation of microseism. We agreed the tidal actuator
on the PSL did not interact with the microseism. An interesting question will be
whether feedforward alone might suffice for this actuator. Tidal and microseism
signals potentially interact at the SEI fine actuators. We resolved to separate
these two problems, because of great differences in signal sizes and signal time-
scales, using separate DACs to feed an analog summing point. Rolf and Dave favored
using an EPICs sandbox sequencer to provide the tidal signals for both PSL and
SEI. An analog lo-pass filter before the summing junction for the SEI fine actuator
should provide additional equipment safety on equipment reboots and will help with
noise suppression. Rick Savage and Hugh are working the PSL side of the problem,
Dave is working on the EPICs implementation, and Fred is continuing to work the
issues on the predictor code.


LIGO Livingston Observatory (LLO) Operations (Coles)


Hosted the PAC meeting, December 12-13, 2000.  Members of the PAC attended
programmatic sessions and presented status and proposal summaries.
 

OPTICS/COC/SEI INSTALLATION: Calibration of optical levers, and installation
of cameras and illuminators has consumed the bulk of our time this week. We
found an open OSEM driver coil on the BS, which explains the damping
difficulties we experienced last week. We've prepared a lab at the X-end for
the U of F hi-power laser, and have been helping set things up there. The
last 2 BSC bellows for LASTI have passed RGA, and Joe Hanson will be crating
and shipping them soon. Continuing to move the machine shop as opportunities
present themselves. (Jonathan Kern)
 

Operations/Control Room:  We have developed a protocol for tracking and
controlling commissioning activities. This includes informing the lead
operator of any changes to Epic settings or configurations.  This enables
coordinated work efforts with all parties being informed on other parallel
activities.  An LLO Operations I-log site has be established that will
include all pertinent control room activities. Control room staffing has
increased to accommodate extended work hours for
the LLO staff and visitors.  (Rich Riesen)
 

Administrative:  We have been working with our vendors which currently do
not accept Master Card. So far, we have added seven vendors to accept the
card.  Results probably will not become apparent until January-February
because we need to allow time for them to receive the equipment and
installed it.
To ensure better phone coverage for the 3100 extension, we have
re-programmed our telephone system to allow calls to roll over to the
control room if the front office does not answer. If the control room is
either busy or does not answer, then the calls will be forwarded to the main
voice-mail box. We have also set up our phone with a holiday greeting during
this season.
Have provided administrative assistance to PAC attendees as needed and made
sure everyone had plenty of good food to eat during the last couple of days.
(Bonnie Wascom)
 


Detector/Technical Support (Whitcomb, Coyne)


 
Installation & Commissioning:
Hanford
Livingston
Other Science/Engineering Activities:
Design/Analysis/Fab
Issues/Concerns
See also the Installation web page

1.1 LHO INSTALLATION & COMMISSIONING

2km Commissioning


Peter Fritschel, Matt Evans, Rolf Bork, Nergis Mavalvala, Dick Gustafson, Stan Whitcomb

Work on locking the full interferometer continues with moderate progress. We implemented optical lever based damping of the beamsplitter and the two fold mirrors, as had been done previously with the input test masses. This helped dramatically to stabilize the fluctuations in power buildup in the power recycling cavity, which in turn has allowed us to make better measurements on the system. We also moved the feedback for the power recycled michelson (PRM) from acting on the four test masses (moving the cavities as a whole) to acting on the fold mirrors, which also resulted in a more stable PRM lock.

We continue to have brief lock stretches of the full interferometer, with longer lock stretches for lower power buildup cases (we continue to exercise some control over the latter by clipping the beams with the gate valves). The largest buildup seen corresponds to a recycling gain of about 10, but lasting only ~1/10 second.

Bill Kells
Brought back a raft of lock stretches from last week at LHO.  Am trying to come to some insight as to their characteristic nature (with eye on improving the situation).
 

E2 Run

John Zweizig
This week I set up for and ran the E2 two-arm data through a finalized set of monitors. The idea behind this run was to get a consistent set of triggers, trends and other data products for use in the E2 analysis. It also provided a means to run monitors that had not been completed at the time of the E2 run. The data rerun proceeded with only minor snags over last weekend. Since then Mary Lei and I verified that all the triggers generated during the run were in fact inserted into the metaDatabase. We found that 103 of the 211477 triggers were not inserted because of two independent errors. These errors will be prevented in the future by adding handshaking and error recovery to the script used to submit data insertion jobs to the ldas manager. The files containing the 103 missing triggers were resubmitted to ldas by hand so now ALL generated triggers are in the database.

The remaining E2 data (one-arm running) will be run through the same set of monitors soon.

COS

Mike Smith, Ken Mailand, Lee Cardenas, Betsy Weaver
APS Telescope are awaiting pre-alignment. ETM telescopes need a slight rework of a mounting bracket. Two telescopes were focussed. The COS autocollimators will be evaluated for focus alignment at CIT prior to being sent to Davidson for repair.

RF Distribution

Rich Abbott
The RF Distribution system has been shipped to LHO, and we are awaiting the swap to retrofit the old units for the 4K

PSL

Lee Cardenas
I have suspended the 4K  Ref. Cavity which it is awaiting inside the chamber to be closed up as soon as Robert and Mark finished the vibration test for the optic table.

We (Mark G. & I) started the RGA unit on the pump station destined to pump the 4K Ref. Cavity chamber. So far, the sum of the elements (amu 16, 18, 40, 41,43, 53, 55, and 57 ) are below 1E-9 torrs.

I have completely flushed and cleaned the Neslab chiller for the 4k Laser. tomorrow will fill the chiller with new and fresh cooling (mixture of 20% Ethylene Glycol, and 80 % of Distilled water.  (1 gram/gal of water ) of Chloramine-T as an Algae inhibitor.

Input Optics

David Ottaway, Betsy Weaver, Corey Gray
Corey and Dave are laying out the IO components on the PSL table.

1.2 LLO INSTALLATION & COMMISSIONING

Commissioning

David Shoemaker, Rai Weiss, Joe Kovalik, Dave Reitze, Szabi Marka, Jay Heefner, Jonathon Kern, Russ Wooley, Peter Saulson, Stan Whitcomb, ++++
The big push has bee to get ready to check the initial pointing of the laser beam down the Xarm.  We have gotten all the suspensions working (we think!), though the residual motion on some of them seems a little larger than it should be.  The most problematic was the beamsplitter, which tirns out to have an open coil.  The sensing and actuation matrices were adjusted to compensate and it seems to be damping pretty well.

The optical levers seem to be in good shape, though the power may be low on one or two of them.  The ASC biases are working in the corner station.  All illuminaters are functioning and the camera feed are available in the control room. We need to re-verify the initial alignment relative to the ITMs, but we are not far from opening the gate valves.

#SEW# This is Peter Saulson's last week of sabbatical at LLO.  We should all give him a big thanks for his leadership in the LLO commissioning.  His successor will have big shoes to fill.

Fortunately, Rai Weiss has agreed to serve as commissioing director at LLO, starting immediately.  Rai will concentrate his travel on LLO and will be on site more than half time. I hope that everyone will give all possible help to Rai in this new role.

Jay Heefner
Various problems have been fixed in recent days The summary is as follows:

  • ETMX suspension controls database had apparently been changed from the original version that was installed and tested several months ago. The channel mapping was incorrect so there were no control or monitoring capablities or the suspension. This has been fixed and the controller is fully operational.
  • There are continuing problems with the restore functions killing the sequencers in the suspension IOC. We are not sure of the fix.

  • #SEW# Replacing the processor on the three LOS's in the LVEA seems to have helped (solved?) the problem, but we are continuing to monitor it
  • The DAQ system has been reconfigured to add the PEM microphone channels in the LVEA.
  • The ETMX optical lever is now functional.
  • The ASC bias adjust controls for the suspensions are operational with the exception of MMT3 and ETMX. It should be operational by the end of the week.
  • Input Optics

    Dave Reitze, Sanny Yoshida, Warren Johnson, etc
    Mode cleaner work:
  • we noticed that the MC was misbehaving over the past two weeks (fragile lock, frequent loss of lock).  We investigated how the local damping gains affect the lock stability by looking at the MC_F and MC_L signals vs gain.  Both L and F were dominated by stack motion at 1.5 Hz. Initially, all gains (P/Y/Pos/S) were set to 9.  Reducing the gain of MC1 to 2 significantly improved the robustness of the lock; the MC_L amplitude reduced by 3X. The lock stability was insensitive to gain changes in MC2,3
  • power dependence of the lock was also looked at in anticipation of the long arm beam hunt by looking at the MC_F control signal vs. power in the MC.  We were able to keep the MC locked (albeit barely) with 2 W going in.  The maximum stable operating power was ~1 W, above that we saw increased pointing fluctuations and degradation of the MC_F signal.
  • MC transmission (power transmitted through the MC/power into the HAM) was measured to be ~ 90.5%.  This was done without the WFS operating and with no attempt to improve the mode matching (the character of the reflected spot indicates that the mode matching could be improved).

  •  

     

    Initial measurements of dynamic RFAM were made; we demodulated the output of the New Focus 1811 PD (2 mW power) at the resonant side band frequency and looked for low frequency noise above shot noise in the 0-1 KHz range.  These measurements are ongoing, but preliminary data shows some resonances in the spectrum (34 Hz), but no significant noise above shot noise.

    PSL

    Peter King
    Well after the 9500 hours indicated on the laser power supply, the master oscillator for the 10-W laser (SN #103a) is only producing about 25% of the delivered output power.  The spare PSL NPRO (SN #238) from LHO has been requested, ready to be installed at an opportune moment when the PSL output power delivered to IO becomes an issue.

    It was noticed that the pre-modecleaner (PMC) regularly dropped out of lock overnight.  Re-acquiring lock was not as easy as previously recalled.  A check of the PMC servo mixer output indicated that not enough RF was being applied.  The RF level was increased and this appears to have solved the problem of the PMC dropping out of lock.

    The PSL generic DAQ card was modified to permit monitoring of the AC component of the PMC PZT voltage (above 0.1 Hz) after some consulting with RichA.

    I spent some time trying to figure out the connections for the modecleaner generic DAQ card since it was mentioned that two of the channels were either noisy or saturated.  As it turned out, these channels were not connected.  A few wire wraps later, things were (hopefully) sorted out.  The signals now appear on the dataviewer okay.

    2.0 Other Engineering and Scientific Activities

    2.1 Design/Analysis/Fab

    Optical Metrology

    GariLynn Billingsley
    Veeco representative Sen Han visited this week to inspect the WYKO 6000 interferometer in the metrology lab.  He was able to witness one of the various quirks that the instrument sometimes exhibits, a feature which appears to be related to the ground glass screen.  While the behavior itself doesn't appear to take the instrument "out of spec" it is at least a symptom of something strange going on.  Many of the instruments strange symptoms come and go at various times.  Some of these, we believe, are attributable to the ground glass screen.  We would love to see the motor replaced at minimum.  It will be interesting to see if Veeco grabs onto on the "not out of spec" point.

    PSL

    Peter King
    Rick Karwoski, Paul Russell
  • All three boards for the PMC servo have been tested in our lab and delivered to LHO
  • Schematics for all three boards have been updated and delivered to LHO
  • The RFPD for the Frequency stabilization subsystem has been tested at our lab and is ready for shipment to LHO
  • The schematic for this board has been updated
  • We are currently testing the Frequency Ref card for the FreqStab subsystem
  • We are wrestling with parts shortages on the Frequency Servo board which is mostly stuffed. We anticipate resolution shortly and start of test by early next week.
  • We are awaiting the approval of two additional work benches and cabinets for our lab.  They will be needed in short order for stuffing and testing of LASTI and 40m. electronics.

  •  

    ISC

    Mike Zucker
    Working with Rana, Rich Abbott and Rick Karwoski on photodetector problems found in LLO 4k length sensing detectors.  We found three (apparently unrelated) problems; 1) detectors can be destroyed by improper power supply hookup, 2) due to an oversight in a late design change, DC readout amplifiers are vulnerable to saturation, allowing overpowering of the detector without an external indication, and 3) the PD bias circuit seems to oscillate at 500 kHz in the dark (not an issue under normal operating circumstances, but potentially confusing for calibration and dark tests).  Working on fixes/workarounds for all three; also checking to find out if problems 2 and 3 afflict installed LHO diodes.

    Rich Abbott, Flavio Nocera, Mohana Mageswaran
    All daughter boards for the new modecleaner servo have been ordered.  We are working through the board trying to get the noise performance within specification.  All transfer functions are verified to be correct.  We are building additional timing boards and I&Q demodulator boards.  We have also been working towards understanding the recent issues with the RFPD's.

    Modulated OSEM Design

    Jay Heefner
  • Stabilized oscillator satellite amp boards are due this week and should

  • be available for test in a few weeks.
  • Suppressed carrier satellite amps are being held in reserve.
  • New OSEM Heads

    Janeen Romie, Peter Fritschel, Myron McInnis
    All of the new osem heads have now been plated/metallized and received at MIT. Quality is inconsistent: many are of good quality, and are now in the coil winding stage; but many have poor quality coatings and will need to be reworked (in progress). We do have enough good quality units for the LHO 4k ifo though, so we are still on the schedule of completing new osems for this first installation in the first two weeks of January.

    Mark Barton
    This week I set up an experiment to check the thermal performance of the OSEMs in vacuum. I've been practicing on one of the old OSEMs, trying to replicate the results of Miyoki as a sanity check. I'm checking the heating effect of both the LED and the coil. I'll be ready to test the new design as soon as I get the ZnN coated prototype from Peter.

    Digital Suspensions

    Jay Heefner
  • SOS Dewhitening board layout on hold until next week. (Jay is at LLO this week)
  • SOS coil driver design needs to be started
  • GDS

    Daniel Sigg
    The problems encountered on raid2 of fortress (data loss & SCSI error) finally have been fixed by a new set of SCSI cables.

    A backup of the E2 data was done with the data stored on fortress. The backup was checked with a separate verify cycle. A set of tapes was assembled for MIT, another tape was sent to LSU. Greg's tape control software proved to be very useful.

    More memory (+1GB) was orderer for all DMT machines.

    Fantom (frame multiplexer software) can now access tar archives. This makes it possible to read backups from AIT-2 tapes without transferring the data to disk first. The next feature will be to interface the DMT shared memory partitions. All together, this will allow to run DMT monitor programs directly from tapes.

    A couple of dtt bugs reported during the E2 run have been tracked down and fixed.

    Data acquisition

    Sander Liu
    In the process of purchasing components to build couple of +/- 5Vdc power supplies.  Still waiting for long lead time components to arrive before we can proceed to build more antialiasing filter chassis.
     


    40 Meter Interferometer (Weinstein)



     



    Thermal Noise Interferometer (Libbrecht)


    TNI Weekly Report
    (Eric Black, Luca Matone, Shanti Rao, Kevin Schulz, Ken Libbrecht, with
    help from Seiji Kawamura)
     

    TNI test cavity locked!
     

            We spent a considerable amount of time this week trying to get our
    mode-cleaner to lock well, but without a great deal of success.  After
    solving a few assembly problems (a wire brushing against one of the
    mirrors, a bad electrical contact), we still could not achieve an
    acceptable lock.  The symptoms included some unusual high-frequency
    oscillations, and we suspect that the laser PZT is not functioning
    properly.  We observed additional odd behavior when locking the laser to
    our fixed-length reference cavity, which seems to support our hypothesis
    that the laser is at fault.  The easiest way to check this is to swap in
    another laser, and this will be done shortly.
            We also found a low-frequency oscillation in the mode cleaner lock that
    goes away when the laser power is reduced, suggesting that scattered light
    from the cavity may be getting into our OSEM sensors.  We need to nail down
    our lock much better before we can investigate this problem further.
     

            Rather than swapping lasers right away, and having to realign the works,
    we decided to first route around the mode cleaner cavity and try locking a
    test cavity.  We expected lock acquisition might not be straightforward,
    since the test cavity finesse is high (the mirrors were coated for
    F=100000, and a quick measurement gave F>55000).  We first locked the laser
    to a reference cavity, and tried locking the test cavity to the laser using
    a broad-band Pockels cell to increase the servo bandwidth. This didn't work
    for some rather uninteresting reasons.  First the electronic gain required
    for the PC path was too high.  Also, we were using one power supply for the
    laser PZT driver and the PC driver, and saturation of the PC driver tended
    to push the reference cavity out of lock.
            Finally we tried to lock the test cavity and laser by actuating on the
    laser PZT and the test mass, without a reference cavity and without the
    Pockels cell.  This worked well.  The lock was robust and stable for at
    least 10s of minutes at a time.  The system is still far from its final
    configuration, but we are now fairly confident that lock acquisition for
    the test cavities will not be a serious problem.
     


    LASTI (Zucker)


    No report received.


    Data Analysis and Computing (Lazzarini)


    No report received. Must be the GWDAW meeting ?


    LIGO II/Advanced R&D (Sanders)


    From Bill Kells:

    2. Going over some loose ends with Jordan on the work we have
    done on Sapphire mirror birefringence. In particular it seems
    that we have observed very much lower Rayleigh scatter in the
    sapphire mirror we used than has previously been thought.

    3. More work on getting the FFT code running revved up. Have executed
    my first run on the new CACR supercomputer!
     
     

    From Peter King

    3.2 LASTI
    The reference cavities for the LASTI PSL have arrived on campus.

    3.3 40m Lab
    The reference cavities for the 40m Lab PSL have arrived on campus. The
    vacuum chambers should arrive some time next week.

    From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>

    The Core Optics Development plan has been circulated.  Until it finds a permanent home in the DCC, you can obtain a copy of LIGO- T000098-00-D at DCC\OUT\ or at http://ligo.caltech.edu/~gari/LIGOII/index.htm
     
     


    For additional information about this report, contact sanders@ligo.caltech.edu