Weekly Report for Week Ending June 5, 2003


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

The LIGO Executive Committee Agenda for Monday  June 9, 2003 will be:

 CANCELLED DUE TO NSF REVIEW PREPARATION


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Saulson)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


 
LIGO Weekly Site Telecon (Lindquist)
There was no site teleconference on Thursday, June 5, 2003 due to the Program Advisory Committee meeting.
 
PROPERTY MANAGEMENT (Chargois)
From: Ed Chargois <chargois_e@ligo.caltech.edu>
No report this week.
 
DOCUMENT CONTROL CENTER (Turner, Mak)
>From: Linda Turner - turner@ligo.caltech.edu>
No report this week.

> From: Cleveland Mak <mak_c@ligo.caltech.edu>
Processed and distributed 7 DCN's
 
DCC Activity
WE 06/5/03      Packages/Faxes
In                         20/36
Out                      13/47
 
COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman, Salone)

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
Completed the internal modification to CSRS, change order 3 and an internal modification for funds transfer to Star Service to re-do the Air Condition system. Completed change order 6 to Excel Group.  Working on change order 16 to Research Electro Optics and change order #14 to Crystal Systems.
Working with Ed Jasnow and Bill Tyler on the Raytheon work order.
Submitted the subcontract files on MIT, Northrop Grumman, and Butler to the PWC auditors for review.
Placing and reconciling pcard orders.
From: Gina Salone <gsalone@ligo.caltech.edu>
No report this week.

From: Florence Kaufman <fkaufman@ligo.caltech.edu>
Completed monthly financial reports which have been posted on the network.
Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
 SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

From: irena@ligo.caltech.edu (Irena Petrac)
AdLIGO Optics Coating RFP: The RFP package is out on the street. Proposals are due end of the month. Proposers Teleconference is planned.
Crystal Systems Inc.: CO No. 14, for the purchase of additional HEM sapphire test flats, was released to Purchasing.
Research Electro-Optics: CO No. 16, for coating of additional LIGO supplied test optics, was released to Purchasing.
From: Ed Jasnow <jasnow@ligo.caltech.edu>

CONSTRUCTION:

We continue to go down to the wire in spending out the remaining construction funds by June 30.  Computer deliveries, completion of the LLO pre-fabricated storage building, and resolution of retention issues for Chervenell at LHO are the big drivers at this point.

OPERATIONS:

P-cards for new employees at the sites remains an issue since they must be trained personally by the P-card team at Purchasing Services.  Arrangements are being made to have members of this team go to the sites to train multiple numbers of new employees
 
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Processed the paper work for Thirty (30) new/revised trips.  There are approximately fifteen (15) trips in various stages of completion before ticketing can be done and/or paper work completed.  And an additional seven (7) general inquiries.  Until further notice I will be doing travel for LHO travelers.
The 2003 SURF Program will be held from June 16th thru August 22nd.  LIGO/Caltech will have twenty (22) students, LIGO/Hanford will have seven (7), and LIGO/Livingston will have three (3), with four (4) going to Pisa, Italy.  I continue ticketing the thirty-two (32) coming to one of the three (3) LIGO sites and Pisa will be handling the four (4) going there as Passports and VISAs are confirmed.
Completed four (4) Expense Reports and there are seventeen (17) reports yet to be done.  I continue to contact travelers who have outstanding Expense Reports (more than one (1) month old) to ask for their cooperation in sending me their receipts so that they can be closed in a timely manner.  There  are six (6) reports more than 30 days old at this time.
Reconciled sixty-five (65) P-Card items which required numerous phone calls to hotels, car rentals, etc., in order to track down which traveler incurred which charge; and the pulling of each traveler's file to assure that charges are correct for each fee incurred.
I'm happy to report that the new EFT Program for Travel Reimbursement Direct Deposit continues to be functioning well and although there have been a couple of minor bugs Michelle and I are working on them.  Prospects are good for a successful implementation.  If you have any questions or problems with EFT please let me know so that we can address it promptly.  For those of you who have not as yet sent me your form for participation please send it to me as soon as possible and I'll get you signed up immediately.  Thanks for your cooperation and help on this one.
Worked on the preparation and distribution of the Travel/Vacation Itinerary for June 2, 2003.  Arranged three (3) new teleconferences and arranged five (5) new reservations on the LIGO Calendar.
I continue to do MIT's travel to the sites for installation activities and also to assist them wherever possible.
>Dorothy Lloyd
Processed the usual invoices for payment. Tracked and followed up on invoice problems. Reviewed and recorded payments processed by Esther the week of May 26.
Processed the usual requisitions, change orders and payment requests.
Continue to monitor contract and blanket order encumbrance and notify task managers when supplements are needed.
Jim continues with data entry in the LIGO database and helping out in the DCC.
>From: Ryan Tischler <rtischle@ligo.caltech.edu>
NSF Review -following up on details
Mayfield High School tour
 Advanced LIGO (Frey)
From: Thomas Frey <tfrey@ligo.caltech.edu>
 
Attended PAC meeting all day on Thursday the 5th.

For list of documents that are being used to develop Adv. LIGO Cost and Schedule, see http://www.ligo.caltech.edu/~tfrey/Cost_MTG_082002/

Advanced LIGO MRE Proposal (Highest Priority)
Finished updating the top level schedule prepared by Dennis in MS Project.
Continued preparing revised budget sheet data.
Corrected issue with total cost summary report and generated subsystem cost summary reports as requested by David and Dennis.
Prepared a detailed cost sheet that shows only the costs included in the request for Outreach as requested by Phil for Gary and Fred.
The following is a summary of status by sub system:
COC - Still need completed WBS dictionary and BOE.  Garrilyn provided a minor change to a WBS definition.
PSL -  No action items pending.
AOS - Still need completed WBS dictionary and BOE.  Sent templates to David Ottaway.
IO -  Still need completed WBS dictionary and BOE.
SUS - No action items pending.
Attended meeting and answered questions related to SUS interface with LASTI.
SEI - Received revised (Version 3) data from Dennis and data input of WBS and BOE is in progress.  Completed WBS entries and will finish BOE by Monday AM.
SC - Still need completed WBS dictionary and BOE.  Issued WBS and BOE templates to Peter F. to complete input.
LDAS - No action required at this point in time.
INSTALL - Dennis provided a revision and data input is in progress.  Completed WBS entries and will finish BOE by Monday AM.
 DAQ - No action required at this point in time.
PM - No action required at this point in time.
FAC - No action required at this point in time.
SUP - No action required at this point in time.
Continue to update the LASTI Schedule and incorporate any changes.

Continue input of changes and comments from Mike Zucker.

Cost Book Tool.

ROSTER DATABASE:
BK is continuing work on action items.
Input of supervisor, dept., and specialty codes on hold until after review.
COST BOOK DATABASE:
BK is continuing work on action items.
Continued to work on preparing format for hard copy version to be submitted for NSF reviews.
Preparing reports requested by Dennis and David, required adding some reports and I made some changes to the cost database to accommodate other requested reports.
Development of the Advanced LIGO Project Controls Guidebook continues.

Reports (Lindquist)
No report this week.
 
Change Control/Contingency (Lindquist)
A change board was held during the Executive Committee Meeting on Monday, June 2.  Minutes will be prepared and distributed.
 
Human Resources (Akutagawa)
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Various personnel/payroll /HR related work.
 
Quality/Safety (Tyler)
>From: Bill Tyler <tyler@ligo.caltech.edu>
 Nothing significant to report this week.


LIGO Hanford Observatory (LHO) and Interferometer Operations (Raab)



 

Summary of Commissioning Activities at LIGO Hanford Observatory (Sigg/Landry)

Vent activities

The vent was successful as far as we can tell; more details here. Vent times were kept short: 11h40m for the 4K vertex, 9h17m for the 2K vertex and 11h27m for the X manifold (the Y manifold was kept under vacuum).
On Monday:
  • the 2K ITMX was replaced and its pointing restored; see here.
  • the 2K POY steering mirror was adjusted by the calculated angle. This was successful and we now have a Y pick-off beam on the ISCT10 table; see here.
  • beam baffles for the wire protection on 2K MC2 and 2K MMT2 were installed. The MMT2 beam baffle also serves as the RM beam dump.
  • a half disk baffle was installed at the bottom of the tube connecting HAM 8 to HAM 7 to protect the electric wiring.
  • some additional viewports were installed to give a better look at, for example, the output Faraday.

  • On Tuesday:
  • the 4K ITMX was translated along its axes by 28mm away from the BS to fix the asymmetry. Unfortunately its pointing was not maintained and the orientation is 0.45mrad off in yaw.
  • an inspection of the 4K BS reveled that one of the earthquake stops was touching the mirror; see here.
  • beam baffles for the wire protection on 4K MC2 and 4K MMT2 were installed. The MMT2 beam baffle also serves as the RM beam dump.
  • a steering mirror was installed that let's us look at the 4K MC baffle.
  • a half disk baffle was installed at the bottom of the tube connecting HAM 2 to HAM 1 to protect the electric wiring.
  • some additional viewports were installed to give a better look at, for example, the output Faraday.

  • On Wednesday:
  • the 4K ITMY was translated along its axes by 28mm towards the BS to fix the asymmetry. Its pointing was maintained.

  •  

     

    The 2K MC was locked and the pointing of the input train roughly restored. No one had time to look at the 4K MC as of yet. To fix the pointing of the 4K ITMX we are in the process to bring the coarse actuation system for BSC 3 back to live. There are no other optics mounted on this table so we should be able to rotate the table from the outside. The final word on the asymmetry fix and the ITMX replacement will of course have to wait until we have the arm cavities back.
     

    2K IFO (H2)

    Common mode running resumed on Saturday, after some modifications necessitated by an LSC code change to the CM script and the implementation of a 2nd ASI output channel, see here.

    In preparation for the vent, steering of the POY beam was dead reckoned; see here.
     

    4K IFO (H1)

    Bill Kells worked on data taken in May on H1 measuring HR surface scatter from each TM (scatterometer). The measurements are now absolutely calibrated (bench check of the PD at CIT performed). All the TMs show similar results (ITMx being somewhat an outlier). The average fit scatter loss in this regime is (extrapolated from the few view point measurements) ~ 70 ppm per HR surface.  The theta dependence of intensity scatter is closely theta^-2, which is a nominal expected dependence for surfaces of the type we have. Note that Bill's measurements of H1 arm visibilities gave a mean per mirror loss of ~70 ppm also.

    More power at the AS port resulted in 10W over 10ms on the photodiode, killing it: don't look here.

    H1 arm cavity lengths were measured, yielding Yarm: L= 3995.04437 m +,- 0.08mm, Xarm: L= 3995.08418m +,- 0.08 mm, Arm length difference = 39.81 mm, Yarm shorter.  Details are here.

    A new optics train layout on the AS port appeared to improve the noise in the 100Hz region; look here.

    Potential beam clipping on the POX port was investigate, see the entry here.
     
     


    LIGO Livingston Observatory (LLO) and Interferometer Operations (Zucker)


    Dear Colleagues:
     

    I will be leaving LIGO later today to begin my new position at the NSF. Before I go, I want to let everyone know how much I have enjoyed working with all of you, and express the special privilege I have felt to be a part of the LIGO team. What we have accomplished together has been spectacular. It has truly been a grand adventure to be part of the effort that has transformed an arid stretch of tumble weeds and a snake infested swamp into gravitational wave antennae with extra-galactic reach. I'm confident that even more remarkable achievements are in store as LIGO continues to progress.
     

    I'd especially like to thank Barry Barish and Gary Sanders; for hiring me in the first place more than eight years ago, and for their kind and generous support as this opportunity at the NSF has evolved. And finally, I'd like to express my thanks and appreciation to the resident staff and LSC colleagues at LLO for all they have done: their countless hours of hard work, the camaraderie, and the shared enthusiasm that have made our efforts so worthwhile.
     

    I'm extremely pleased that a candidate as able as Mike Zucker will be taking over as the new LLO Observatory Head, and look forward to hearing of your continued successes.
     
     

    Mark
     

    GHS NOTE:   WE ALL WISH YOU WELL IN YOUR NEW CHALLENGING ROLE. GOOD LUCK MARK!
     


    Detector/Technical Support (Coyne)



     

    DETECTOR SCIENCE & ENGINEERING (Coyne)

    see also the Revision Technical Review Board (RTRB) status here

    D. Coyne note: This web page needs a number of revisions/updates. EPI and RFI change requests have been submitted to the CCB. A proposal for implementing an independent timing check system with atomic clocks has passed RTRB review and will be submitted to the CCB for evaluation as well. The low noise DAC effort is close to a point where the RTRB can review test results and a CCB request for funding a production order can be generated.

    Seismic Upgrade Project (External Pre-Isolation, EPI)

    see also the LASTI report for EPI work

    Awaiting a decision from LIGO management on which EPI system to pursue for deployment at LLO.

    Ken Mason has sent all EPI actuator/spring assembly parts out for multiple bids for production.

    HEPI Pump Station

    Ken Mailand

    ·I have received a quote on a contaminant characterization assessment for the LASTI pump station 3 micron filter.

    CDS

    see also 6/4 weekly CDS meeting minutes in the commissioning archives

    see also the 40m Lab report

    CDS Software

    Dennis Coyne reporting for Rolf Bork et. al.

    CDS Hardware

    Rich Abbott reporting
    ·Flavio is ready to manufacture the final version of the ISS cards.  The files will be sent out today.

    Dennis Coyne reporting for Jay Heefner et. al.

    PSL

    PeterKing

    The output noise of a voltage reference was measured before and afterfiltering by a 2-pole filter at 1 Hz.  The measured output noise was higher than the expected value by about a factor of 2.  This in turn was well above the noise floor of the dynamic signal analyzer.

    Some intermittent problems are being experienced with the 10-W laser at LLO.  In particular the problem is noticed with the frequency servo dropping out of lock -- for no apparent reason -- even if the control from the modecleaner to the VCO is disconnected.  The symptoms are if you monitor the FAST actuator voltage every now and then a level jump occurs. Looking at the trend data for the past 3 weeks, suggests that the problem started between 2 to 3 weeks ago.  On locking the laser to the reference cavity, the laser would lose lock after about a minute.

    In checking out the laser, the laser frequency was swept across the reference cavity resonance to display the discriminator signal from the frequency servo.  Ordinarily the discriminator signal can be displayed on an oscilloscope without any problems and that any drift in the relative position between the applied voltage ramp and the discriminator occurs on a time scale of tens of seconds.  What was observed was a movement on the order of a second.  The phase-correcting Pockels cell in the laser was checked for correct alignment and did not appear to be the problem.  The capacitance of the FAST actuator was measured and was consistent with the spare laser and an NPRO laser.

    This morning (Wednesday) Ken Watts and Mike Fyffe went out to check the power going to the rack because the fuse in the laser power supply has blown a number of times in the past week or so.  One problem found is that the PSL rack is not grounded with respect to the incoming mains power. When the rack was temporarily shorted to ground, I found that the frequency servo could lock and everything appeared to be normal.  The rack was then allowed to drift to see if the problem would return -- it did.  Temporarily grounding the rack again appeared to have cured the problem again but the test was interrupted.

    Tests on the laser are on-going, as are comparison measurements and cross checks with the spare 10-W laser.

    Errant Beam Blocks

    Mike Smith

    Errant beam baffles were installed in LHO HAM2 and HAM8.

    ITMy,2k PO Mirror Re-Alignment

    Mike Smith

    ITMY PO mirror was re-aligned by rotating the mirror 1.5 mrad ccw in the yaw direction, as viewed from the plan view of the IFO. This rotation of the PO mirror rotates the input to the ITMY PO telescope by 3.0 mrad, which was determined to be the correct PO beam alignment by measuring the rotation of the FMY mirror required to direct the ITMY PO beam out the center of the output viewport.

    Optics Analysis

    Erika D’Ambrosio

    I had previously done some simulations when the recycling cavity is only locked.Including the arms the sideband power is basically the same and having a 3% loss through the two internal test mass mirrors does not affect the gain much. 

    My personal interpretation is that the sidebands might be so large in transverse distribution that they are basically lost after crossing the two ITM mirrors and energy is not conserved. The effective reflectivity of the ITM keeps on being ~97% instead of jumping to 1. The gain of the carrier is high though as we expect since the impact of thermal lensing is only a second order effect for it. Were the interferometer matched the sideband gain should be roughly half the one of the carrier.

    CR                 SB+                   SB-

    61.42              7.57                  7.14

    CR TEM00           SB+ TEM00             SB- TEM00 

    61.17              2.83                  2.76

    With no arm:       SB+                   SB-

                       6.91                  7.26

                       SB+ TEM00             SB- TEM00

                       3.03                  3.13

    Optical Contamination Cavities

    Lee Cardenas, Liyuan Zhang

    OTF Lab. (W. Bridge)
    Contamination Cavity # 1
    New test sample a 10mm Capacitance position sensor (given By: Rich Abbott)
    which consist of a sma cable and a ceramic connector at the end. The whole cabling it has been introduced
    and tested. The chamber is pumping down and cavity is locked and we are taking ring down and beat frequency every day.
    Please see Dr. Zhang graphs for absorption, ring down and thermal lensing.

    Absorption Test Measurement prototype in progress

    Scatterometer system is in STANDBY for measurements.
    We are taking more absorption measurements for the 6 inches in diameter by ~ 3 inches thick Sapphire mirror.
    We will be measuring the scattering of the this mirror.  As a result, We have made a base holder specifically for this mirror to accommodate into the scatterometer system.

    OTF Lab at Lauritsen ROOM 38
    Cavity #3
    This cavity has 70  ppm mirrors and hung with one end at 1.8 degree higher that the other end.
    Cavity is locked and we have 147 mw of power with a 95% ! visibility. We are taking ring down and beat frequency every day.

    Cavity #2 Test cavity STILL in STANDBY.
    Optical train upgrading is in progress.
    New cavity assembly is in progress for this chamber.

    Misc. tasks..  placing orders to modify the scatterometer system to accommodate the new sapphire mirrors for the advance Ligo.


    40 Meter Interferometer (Weinstein)




    Thermal Noise Interferometer (Libbrecht)


    no report


    LASTI (Zucker)


    MEPI (Myron, Ken, Rich, Dave, Bill)
     

    We ran a sensor correction measurement cycle over the weekend and got a
    full set of data on all three directions (X,Y,Z). This was done by
    locking up 7 modal loops, varying the sensor correction coefficient and
    recording the ground and witness seismometers. The transfer functions
    were then calculated and the effects of varying the sensor correction
    could then be evaluated. Some of the data from this run can be seen on
    the ilog for Tuesday June 3. Their resolution (in terms of sensor
    correction coefficient) is limited due to the low loop gain at low
    frequencies. Plots of the loop gain are also in the June 3rd ilog entry.
    We reworked the control laws to get more low frequency gain and reran
    the measurement; some of these data have been entered into the ilog, on
    June 5.
     

    HEPI (Myron, Ken, Rich, Dave, Bill)
     

    After installing the new pump and motor we remeasured the hydraulic
    pressure spectrum. This spectrum along with a spectrum for the old pump
    can be found on the June 3rd ilog.
     

    LLO EPI Installation (Ken Mason)
    Bid packages have been delivered to 5 suppliers for all fabrication and machined parts (excluding actuator) for the EPI systems to be installed at Livingston. Three bidders have already completed quotes.
     
     

    ISC TELESCOPE IMPROVEMENT (Ken Mason)
    An ISC telescope has been designed with a very high stiffness, the first mode being at 415 Hz. Also included are provisions for acoustic isolation. Fabrication drawings are now being created for building a prototype.
     
     

    Thermal Compensation Advanced LIGO (Dave)
     

    Spent time preparing for NSF Review.
     

    Thermal Compensation Initial LIGO (Dave, Dan Mason)
     

    Dan Mason is coming up to speed on the CO2 laser that will be used as the actuator.
     

    LASTI Optics
     

    Waseem Bakr (UROP student) has started a trade study to determine whether it is feasible to increase the g factor of the LASTI cavities given the expected excellent seismic isolation that LASTI will have.
     
     


    Data Analysis and Computing (Lazzarini)


    SIMULATIONS AND MODELING (BHAWAL)
     

    _______________
     

    E2E MODELLING:
    _______________
     

    e2e weekly Physics meeting
    ---------------------------
    Luca, Matt, Malik, Virginio, Hiro, Biplab discussed the new optical model
    code and WFS issues in hardware and e2e-model.
     

    e2e in Japan
    -------------
    Dr. Hayakawa of the Institute of Cosmic Ray Research, working with
    Prof.Kuroda and Prof.Ohashi, raised a question regarding the use of e2e and
    presentation of the work using e2e. Barry and Gary endorsed that e2e is a
    freeware copyrighted by LIGO/Caltech and that people/groups with a proper
    MOU/attachment exchanged with LIGO can present and publish their works
    so long as they quote e2e/LIGO/Caltech properly.
     

    New Optical Model
    ------------------
    (Matt & Hiro) Matt revisited the new optical model code, adding and updating
     comments and writing a new test program. This has new implementation of the
     modal model for the next generation of the optics/field simulation in e2e.
     This object oriented implementation makes it easier to model complicated
     objects (mirror with wedge and thickness). Hiro received the package and
     started playing with it.
     

    FFT modeling
    ------------
     Hiro started (again) to prepare the mirror phasemap for the FFT
     simulation to study the as-built LIGO performance using the measured
     phasemap. This work will be used later for the calculation of the mode
     decomposition matrix to be used in e2e so that mirror aberration effect
     can be included in the time domain simulation.
     

    WFS signals in presence of mode mismatch
    -----------------------------------------
    (Biplab) Started calculation of dynamical misalignments in presence of
     mode-mismatch using as-built parameters in order to see how the signals
     may change in a not-so-hot IFO.
     

    Code development and maintenance
    ---------------------------------
    (Ed Maros) Work was completed on the  CVS repository for the e2e. The
      JAlfi directory has been removed and a new directory called alfi
      now appears at the same level as e2e. This allows the simulator
      and the alfi editor to have different release cycles.
     

    (Melody) Figuring out the reasons for the differences in the results
      generated by the different versions of gcc in different platforms
      (Linux and Sun) using different optimization levels.
     

    Alfi
    -----
    (Bruce)
     - Fixed copy/paste problem regarding adding of some ports (PR 404).
     - Completed new port reposition interface for internal and external
       movement of ports on nodes (PR 380).
     - Working on Copy/Paste problems with Macro and settings not being
       copied into the new nodes properly (PRs 394 and 413).
     
     

    -------------------------------------------------------------------------------
     

    LIGO DATA ANALYSIS SYSTEM
     

    SOFTWARE SYSTEMS (BLACKBURN)
    ----------------------------
     

    The 0.7.0 Release of LDAS went out this week. It was installed onto the
    Caltech systems on Wedesday and being installed at LLO, LHO, and MIT as
    of today (Thursday). This release includes an enhanced "createRDS" command
    to support merging LLO and LHO channels into a single RDS frame. It also
    fixes the issues seen during the science run. Most of the effort over the
    past week has gone into testing and packaging up this release. It requires
    a new LDCG and that LAL and LALwrapper be compiled with GCC 3.2.3 under
    Redhat Linux 7.3. However, the wrapperAPI's binarys will run successfully
    under Redhat 9.
     

    We grabbed the S2 locked segments from LHO and LLO and inserted them
    into the database at CIT. A Burst script is now running on CIT,
    "walking" along the S2 RDS frames.  It is running three burst jobs
    analyzing H1:LSC-AS_Q.  There was a small problem with one of the
    ligotools (lwtprint) which the script uses.  The attributes in the XML
    entities are in a different order which confused the ligotool.  Philip
    fixed it temporarily for me so that The Burst script works again. Results
    of these pipelines are going into the TEST database on LDAS-CIT.
     

    Modified waveburst table in database, and added new table "sngl_block"
    to support the BlockNormal search code being developed at Penn State.
    Modified guild to work with the new table.
     

    Traced the problem with using NDAS frames in stochastic searches to an
    issue in the generation of the NDAS frames. The DMT tool used to create
    these frames was occasionally dropping out data. It was reported that
    about one NDAS frame per day per IFO had this problem. These problematic
    NDAS frames are being regenerated by the DMT group.
     

    In order to trace the problem with the NDAS frames, the frame file utility
    programs such as frverify and frdump6 had to be enhanced to isolate the
    problem and make sure it wasn't a bug in LDAS. These now provide much more
    diagnostic information than previous version.
     

    Work continued on the porting of LDAS to the new GCC 3.3 compiler. The
    Sun port continues to be a problem. We have developed simple test programs
    that clearly show the problem on the sun but the same test programs run
    without fault under Redhat Linux 9. We have found GCC patches that we
    will be testing out this week. Unfortunately, every rebuild of the GCC
    compiler on our current Solaris test platform takes 7 hours. We hope to
    have faster boxes next week to increase the turnaround time as we look
    for a solution to the issues of this compiler under Solaris.
     
     

    HARDWARE SYSTEMS (ANDERSON)
    ---------------------------
     

    Caltech
    -------
    (Dan Kozak)
     

    * Got bad 9940 drive (wouldn't mount tapes) replaced.
     

    * Provided some assistance to LHO vis a vis their bad T3 (t3-4).
     

    * Staged NDAS data to support Szabolcs Marka's effort to find the bad frames.
     

    * Began re-archiving data (specifically NDAS frames) to 9940B drives.
      9940A drives are now switched off.  Am trying to figure out why the first
      few tapes were written with small block sizes (16k).  Subsequent tapes
      are being written with the correct blocksize (256k).
     

    * Leaned on StorageTek to clean up the mess in Powell-Booth left over from
      the silo upgrade.  Finally successful (today).  Am also leaning on STK
      to get correct power supplies for our two new 9940B drives.
     
     

    (Al Wilson)
     

    * Setting up systemimager for cloning of nodes at CIT, LHO, LLO.
     

    * Setting up nodes 41-56 on the LDAS-CIT system.
     

    * Preparing the old nodes 1-16 from LDAS-CIT for use in LDAS-DEV.
     
     

    (Stuart Anderson)
     

    * Worked with Albert and Al to install the first full rack (40 units)
      of the new LDAS-CIT Beowulf nodes. Two units developed problems
      during the weekend burn test. The failures where combined into
      one node and sent back to ASA (power supply and memory). The remaining
      39 nodes have passed the memory stress test.
     

    * Installed new 224-port copper GigE switch which has been successfully
      used by Al to start cloning the new Beowulf nodes for LDAS-CIT.
     

    * Started installing new Sun 280R server to replace ldas-sw.
     

    * Identified incorrect disk drive size in recent Sun order and initiated
      remedial action with Sun.
     

    * Received notification from Shipping and Receiving that 14 pallets of
      computers from ASA have arrived at Caltech.
     

    * Decomissioned a rack full of old 4GB drives that would not die but
      where taking up too much space in Millikan.
     

    * Transferred one dual- and one quad-processor Intel machine to General
      Computing at Caltech to make room for newer LDAS servers.
     
     

    MIT
    ---
    (Keith Bayer)
     

    * Configured Gigabit card in pcraid2 (using reiserfs).
     

    * Moved S1 data to make room for S2 rds triple coincidence data.
     

    * Running burn-test with RH7.3 of new 3GHz datacon/beowulf boxes.
     

    * Electrical work on ldas lab scheduled to begin June 5/6.
     
     

    Livingston
    ----------
    (Igor Yakushin)
     

    * Set up a test replication configuration from LHO's LHO_TEST database
      and LLO:'s H_TEST_R. At first it worked fine but later H_TEST_R
      completely lost replicated data. My guess, is that some kind of overflow
      happened (not enough primary logs, insufficient buffer pool or something
      like that). I increased the number and size of primary logs, turned on
      logging both for capture and apply programs and restarted replication.
     

    * Experimenting with multipage_alloc configuration parameter of a
      database. According to the documentation, turning it on should speed up
      the insertion rate.
     

    * Got all the remaining hardware from SUN.
     

    * Upgraded kernel on both IDE RAID boxes.
     

    * Restored /frame21 after multiple disk failure.
     

    * Since it turned out that currently LDAS cannot work with NDAS frames,
      I generated AS_Q only RDS frames both at LHO and LLO to exchange them
      between sites.
     

    * Wrote a perl script to set up creator_db differently for different sites.
     

    * Backed up the databases at MIT before LDAS upgrade.
     
     

    Hanford
    -------
    (Greg Mendell)
     

    * Assisting Ben Johnson with installations of the new LDAS beowulf
      cluster, new L700 tape library system, new switches, and recabling the
      room to work with the new switches.
     

    * Assisting Ben Johnson with T3 problems: t3-4 has a firmware/hardware
      problem.  Ben has been working with Sun to fix the problem.
     

    * Assisting Igor Yakushin with creating and writing to tape H1H2 AS_Q
      only S2 RDS frames to be sent from LHO to LLO.  The reverse will be done
      for L1 AS_Q.
     

    (Ben Johnson)
     

    * Continuing work with Sun about t3-4. I have updated the firmware
      level on u1d4 of t3-4 to revision 1204. Problems still persist...
     

    * Configured StorEdge 3510 FC RAID with 11 disks as one RAID 5, with
      one hot spare disk.
     

    * LDAS room temperature monitor is sending data into the CDS network
      for testing. It has not been fully put into the EPICS, i.e. the
      operators won't know if the room gets too hot yet.
     

    * New beowulf and datacon boxes have passed memtest86.
     
     

    DATA ANALYSIS ACTIVITIES (LAZZARINI)
    ------------------------------------
     

    Greg Mendell:
     

    1) Assisted the PULG group on the final draft of its S1 paper.
     

    2) Continuing to work on a proposal with Mike Landry for the PULG group
    to start writing a stackslide DSO to run under LDAS, in preparation for
    the PULG face-to-face meeting June 16-17.
     

    3) Continuing to prepare my SURF student project, which is to study
    various methods of parameter estimation for continuous wave sources.
     

    4) Found memory leaks in LALIndependentTestDetResponse.c, the
    independent test of the beam pattern response functions that Malik
    Rakhmanov and I are working on.  The problem does not seem to invalidate
    the simple test the code currently does, but these need to be fixed
    before we can expand the tests.
     

    Philip Charlton:
     

    The only thing I have to report this week is that I looked into Isaac
    Salzman's observation that running LDAS pipelines with NDAS frames
    produced slightly different results from the same pipelines using
    RDS or raw data. The differences were very small (order 10^-6).
     

    I found that the raw NDAS and RDS/raw data were identical, however the
    downsampled data had a few tiny differences (order 10^-7 to 10^-6).
    Downsampling of data is done on frame-sized chunks. Although the
    algorithm is designed so that (as much as possible) downsampling a long
    data set in chunks should give the same result as downsampling the entire
    data set in one operation, there are necessarily some differences,
    due to the slightly different ways that data must be processed when
    downsampling in chunks vs a continuous data stream.
     

    For this reason, I believe the observed differences are due to the fact
    that the NDAS frame files are downsampled in 1-second chunks while the
    the RDS and raw frames are downsampled in 16-second chunks.
     

    Peter Shawhan:
     

    1) Worked on S1 inspiral paper
     

    2) Organized face-to-face meeting of the inspiral group, to be held
    at Caltech on June 20-22.  Primary goal is to get analysis of the
    S2 data going.
     

    Kaice Reilly:
     

    I prepared the stochastic scripts to produced the necessary intermediate
    data products. I didn't run them yet becuase of disk space logistics. Worked
    with Stuart and the group to setup a work area at Caltech for the stochastic
    group and to move the stochastic cvs to Caltech (ldas-sw).  Most of my other
    time has been dedicated to preparing for PAC 14.  Computer problems
    and getting locked out of the building have made this interesting.
     

    Teviet Creighton:
     

    Prepared a talk on the S1 pulsar analysis for the PAC.
     
     

    -------------------------------------------------------------------------------
    GENERAL COMPUTING (WALLACE)
     

    MIT:
    (Keith)
    -Rebuilt Ultra 1 workstation guinevere with new harddrive
    -Investigating tryplesync software package to sync with
     calcium calendar service
    -General support for summer students
     

    Livingston:
    (Shannon)
    -Added three hard drives to the GC File server.  Spent most of Tuesday
    working with Sun tech support on an issue with the Solaris Management
    Center.  This software has been causing problems on both NIS+ tables and
    Logical Volume Management.  Installed the recommended patch cluster to
    the file server on Monday.  Sun had me roll back one of the patches as a
    result of the call support call.  The issues are still unresolved.
    -Pricing various options for a new backup system.  I am considering a
    RAID similar to what LDAS has for backups.  This would be periodically
    backed up to tape.  We have significantly outgrown our tape library for
    backups.  I am also considering different software options that would
    allow me to use the RAID instead of the library for daily/weekly backups.
    -Set up a new computer for Allen.  His old computer will be wiped and
    given to one of the summer students.
    -Working with ASA on a computer that has been having problems.  This is
    the second time the computer has been back for service.
    -Still working with Bonnie to restore most of her software.  It had been
    upgraded from Windows 98 to Windows 2000 a while back and it just
    finally died.  She lost some e-mail when it did die, however most of her
    files are intact.
    -Setting up computers for the SURF students and teachers today and
    tomorrow.
    -Worked on a couple configuration issues on some of the Sun servers.
    Turning of various services and ssh configurations, etc.
    -Planning on how to upgrade the web server/ilog files, since the order
    has gone through for the hardware.  I am beginning to think that perhaps
    the ilog server should be a separate server.  Also, the database
    functions on the web server should be moved to a separate machine.  The
    web server upgrade will probably take several days to a week to do
    everything I believe should be done.
     
     

    Hanford:
    (Christine)
    - Writing the PR to buy the GigE network equipment.
    - Started setting up the new Cisco router.
    - Various user support.
     

    CIT:
    (Lisa)
    - An incredibly large pile of spam blocks
    - Did monthly's and root dumps of all servers
    - Did a couple of small scripts for users
    - Went to a Sun seminar on core dump analysis
    - Worked on an ntp sync problem for the 40meter
     

    (Mike)
    -Worked on loading two PC's for up coming surf students.
    -Worked on loading a laptop for the loaner pool.
    -The Scanner up on the 3rd floor went out. After troubleshooting it I ended
    up replacing this with a backup scanner we had in storage.
    -Finished up loading Pro/Engineer for Calum. This installation took many
    hours due to loading this software on win 2000.
    -Ran end of the month ghost backups on all NTSRV's.
    -Called in a laptop to Dell tech support.
    -Backed up Lori Robison's computer by getting a ghost image of her
    workstation. Then I set this computer up for a visitor that is going to
    work from this computer.
    -Loading a laptop with an OS for testing for a Dell technician to test with
    after he replaces parts.
    -Larry and I setup SCR for the PAC meeting that included setting up
    additional network connections and rearranging furniture to allow adequate
    seating.
    -Worked on Ken Mailand's computer due to some OS problems and installed
    zone alarm.
     

    (Veronica)
    - LIGO website: worked with George Stokes on troubleshooting of the DCC
    databases. Helped him understand the d/b architecture and the workflow.
    Provided support files and information. Working with him on possible
    immediate and long-term solutions.
    Worked with Larry on DVD burning issues. Contacting Caltech Digital Media
    Ctr for help in converting a set of files to a format suitable for our
    software, in response to Phil's request for a backup copy of a DVD.
    Posted several updates to various parts of the LIGO website.
    - CaJAGWR website: user support. Updated the website in several places.
    Vote count for the Executive Committee elections.
    - Project Science: user support.
    - LSC website: posted a stray talk from the last LSC meeting.
     

    (Larry)
    -Went through a number of purchases. Most were minor items for various people
    and LDAS. Started going through where things are at financially this year on the
    GC budget.
    Discussing the pros & cons people have had with the IDE raid systems. We need
    more disc space and just checking on the best way to get it now that we have a
    few more options.
    -Worked with a number of users going over their setups, adding and modifying
    their accounts. We've spent a great deal of time going over logistical issues to
    get a computer up and going for all of the summer visitors and SURF students.
    With the surplus units coming in from LDAS we should have enough equipment for
    everyone.
    -In between all of the distractions for user needs and going over different
    issues for the PAC and NSF meetings, I have been able to start working on the
    Livingston GC audit report. So far it appears that most of the problem items
    were already identified and being worked on.
    -Worked on the server room. It looks like the air-conditioning will not handle
    any more equipment, I plan on talking to the PMA group to see what some of our
    options may be.
     
     


    Advanced LIGO Development (Shoemaker)



     

    Advanced LIGO and supporting R&D

    Seismic Isolation

    No report

    Suspensions


    From: ctorrie <ctorrie@ligo.caltech.edu>

    Mode Cleaner

    Several attempts have been made to damp all of the degrees of freedom in the new mode cleaner suspension. Shake down of the electronics by Jay Heefner revealed that everything was working. I am currently working on testing the different degrees of freedom one at a time.
    The current situation is that I believe the pitch, vertical and transverse modes can be excited and damped within 10 seconds. More work is required. 2 of the OSEMs which were accepted that did not meet the specifications, in E030084-00-D
    are back with Bob Taylor. More OSEMS are expected to arrive from Glasgow in the next day or so.

    Eddy Current Damping

    I have created drawings of the various light weight arrays that we plan to test on a single pendulum. This will allow us determine if this new design could be incorporated on an upper mass like the one proposed fro the ETM.

    Blades
    Mike Plissi and I have been gathering information and previous experimental work done here at Caltech on cantilever blades. We hope to have several technical notes finished by later this week and posted on the DCC.

    Visit
    10 girls and 3 members of staff from MayfieldHigh School in Pasadena visited us on Tuesday for 2 hours. Pictures of the visit can be found at http://www.ligo.caltech.edu/~ctorrie/. Several of the girls have expressed an interest in during summer work at Mayfield so if anyone is interested you can let me know.


    From: JaneenRomie <romie_j@ligo.caltech.edu>

    AdLIGO Suspensions
    Preparing for the NSF Review.
    Local control hybrid osems are installed on a MC triple suspension in the Synchrotron. As Mark is on vacation, Jay and Calum are working on tweeking thedSPACE  system to damp the suspension.
    CES is manufacturing some tablecloth brackets that will allow for more vertical adjustment of the upper mass, and therefore, the test mass. They are also working on a prototype of a low-mass eddy current magnet holder.
    Calum and I worked on comparing the cost estimates for the triple suspensions.
    In the weekly suspension meeting, we discussed the suspension schedule. We will continue that talk next week.


    Pre-stabilized Laser

    From: Peter King <pking@ligo.caltech.edu>


    2.2 AdvLIGO PSL
    ===============
        In between working on problems with the 10-W laser at LLO, I have been
    trying to go through the IO material for the NSF Review.  In addition, some
    standby viewgraphs have been worked on.
    .

    Input Optics

    No report.

    Core Optics

    From: Bill Kells <kells@ligo.caltech.edu>


    I have been looking into the impact of polarization
    rotation of beams passing through sapphire itms.
    we really have no data at all on this. The phase plate
    inhomogeneities (for one, measurement polarization) we
    DO measure for exisiting samples has
    been large and assumed to be associated with opitcal
    axis migration in the bulk. This would imply also polarization
    rotation. The inhomogeneity is to be ameliorated by
    comp. polish of the AR surface. However any scatter to the
    wrong polarization would not be affected by this comp. So it
    should be directly measured. I have started a thread to have
    this initially done one a handy sample here in our OTF, and
    am working on that and the analysis.

    From: Helena Armandula <ahelena@ligo.caltech.edu>

    Advanced LIGO Coatings

    The RFP for the coating development work was FEDEXed to the vendors today, Wednesday!


    Auxiliary Optics

    From: Michael Smith <smith@ligo.caltech.edu>


    ADVANCED LIGO
    Am in the process of procuring a 0.5 W laser from MIT and a laser driver board from CDS to be used for the photon actuation experiment.


    Interferometer Sensing and Controls

    No report

    Data Acquisition, Diagnostics, Network & Supervisory Control

    No report

    Other Laboratory R&D

    From: YouichiAso<aso@granite.phys.s.u-tokyo.ac.jp>


     Eric
       melted and x-ray'd new candidates.  Seem to be slowly lifting the glassy
    percentage and lowering crystalline contamination. baby steps forward, but
    still steps forward.
     

    Greg

      - X-rayed samples. Still Noisy.
      - Talked to Bill about ways to filter out Fe fluoresence from x-ray
    spectra.  25-40 micron Cr filter should help.
      - Designed new mold to be made which better fits ideal Q-factor
    measurement dimensions.

    Enrico

    I finished the code for calculating inspiral NS range with the system of
    the 2 IFOs together but I'm trying to solve a bug I found for heavy masses.
    I did some test with different last stage lengths.
    I started looking at Kenji's work on thermal noise and Youichi's work on blades.
     

    Youichi

    Compared the results of my MGAS design program with the Virginio's
    paper.  The results almost agree with the paper, but I found a small
    discrepancy. Trying to figure out the reason.
    Tested wire clamp pins. Found that they hold only a little load. Will
    test pins with bigger bulge.

     

     



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