Weekly Report for Week Ending June 29, 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  July 3, 2000 will be:

 CANCELLED DUE TO HOLIDAY

Special Items:


Special Announcements:


Weekly Report Highlights
 
 


LSC Issues (Weiss)


Minutes of the LSC Executive Committee meeting of June 16:

to: LSCexecutive committee
from: R. Weiss
concerning: Notes from June 16, 2000 committee meeting

1) We are planning a John A. Wheeler day at Hanford on August 14,
the Monday before the LSC meeting. This to be a celebration of
Wheeler who has multiple couplings to the Hanford site. During the
Second World War he was deeply involved in design and diagnosis of
the first production reactor at Hanford and, now, he is
responsible for many of the concepts in relativistic gravitation
which have motivated LIGO.

2) Meetings and events being planned

Workshop on r modes in neutron stars: L.Bildsten,
August 2 and 3 at Santa Barbara

Workshop on gravitational wave astrophysics: J. Centrella, in
late Oct - early November at Drexel Institute

GWDAW: December 14,15,16 in Louisiana at LIGO and LSU

Aspen to overlap the astrophysics and gravitation meetings in
February 2001.

3) Establish a writing committee for the second draft of the LSC
White Paper on Data Analysis. The committee to address the
analysis program and the long range needs for analysis.

People being asked to be on the committee:
     Stuart Anderson
     Al Lazzarini
     Tom Nash
     Keith Riles
     Allen Weinstein
     Alan Wiseman

One function of the committee is to take "testimony" from groups
who have asked for data analysis funds from the NSF.

4) Draft GEO/LIGO MOU on data analysis
Committee expressed caution in going forward with a bilateral
agreement with GEO without bringing the idea to GWIC. In particular,
to explore the type of bilateral (or hopefully multilateral)
agreements that would be useful to connect the data from LIGO,
GEO, VIRGO, TAMA and ACIGA as well as the neutrino, X-ray and
radio astronomy communities. A major concern was that an agreement
with GEO not prejudice an agreement with VIRGO.

The consensus of the meeting was not to present the GEO/LIGO
MOU to GWIC but rather to bring forward some talking points
(bullets) about the MOU which would become topics for discussion.
It was felt important to draw out the difficult
points in establishing agreements with the other gravitational wave
detection groups.
 


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


WBS 1.2 LIGO Operations--Administration


Finance, ORACLE, etc. (Lindquist)

We met with Arthur Anderson consultants on Tuesday.  Arthur Anderson has been retained by the Controller's Office to define a Project Accounting function for Caltech to replace the old Federal Accounting Department.  Their mission is to provide an organization, to partially staff this organization, and to develop some procedures all by the end of the calendar year.  They are currently interviewing the Caltech Divisions and major Projects to determine a requirements list for the function.

LIGO Weekly Site Telecon (Jasnow)

There was no site telecon on June 29, 2000 due to travel and the other distractions in progress at Hanford.  The list of current actions revised to reflect open actions assigned through June 22, 2000 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

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


DOCUMENT CONTROL CENTER (Turner, Mak)

From: the DCC <dcc@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. . .

From: Cleveland Mak <mak_c@ligo.caltech.edu>

 ACTIVITY HIGHLIGHTS

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.

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>

  • A meeting was held among Barry Barish, Donna Tomlinson, and Ed Jasnow, of the LIGO Project, with Sharon Borbon, of the Provost's office, for the purpose of discussing the processing of appointments of long-term visitors to the LIGO sites.  The issue was the length of time required to secure the appointments, which were necessary to establish affiliation and, therefore, insurance coverage for the visitors.  Sharon recommended that, if the visitors are receiving no reimbursement from Caltech, that they be categorized as "volunteers," with an official letter from Barry.  This will establish affiliation and insurance coverage, but will not require the appointment processing by Caltech.  It was also agreed that identification cards showing the term of the visit will be issued to long-term visitors.


  • Support (Wood)

    Rita Torres

    Irene Baldon Dorothy Lloyd Elizabeth K. Wood

    LIGO II (Frey)

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

    Progress Period from from 6.23 to 6.29

    Accomplishments:

    Schedule: 6.30 to 7.6 Anticipated Challenges: Corrective Action:

    WBS 1.4.1.2   Project Controls (LIGO Construction)

    Reports (Lindquist)

    The end-of-May Quarterly Progress Report is in progress.  Most material has been received with the exception of some figures.  "Strawman" budgets for LIGO I Operations and LIGO II Operations have been distributed.  Inputs are requested by Friday, June 30.  We have scheduled July 20, 2000 for the task managers to present and defend any increases to their proposed budgets over the current plan.

    Change Control/Contingency (Lindquist)

    The following change requests have been submitted:
     

    CR-990028 WBS 1.1.3 Beam Tube Enclosure Closeout F. Asiri
    CR-000005 WBS 1.2.1 Upgrade Pre-stabilized Laser S. Whitcomb
    CR-000006 WBS 1.2.1 Re-polish Core Optics Components S. Whitcomb
    CR-000007 WBS 1.2.2 Replacement of Optical Lever Lasers S. Whitcomb
    CR-000008 WBS 1.1.4 Cameras and Projection System at LIGO Livingston Observatory F. Asiri
    CR-000009 WBS 1.1.4 Cameras and Projection System at LIGO Hanford Observatory F Asiri
    CR-000010 WBS 1.2.2 Redesign Suspension Controllers S. Whitcomb
    CR-000011 WBS 1.2.2 VME Development System and Spares S. Whitcomb
    CR-000012 WBS 1.2.2 ASC/LSC Rework S. Whitcomb

    Copies of these change requests have been distributed to memebers of the LIGO Change Control Board (See LIGO-M000176-00-P).

    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)

    Quality/Safety (Tyler)

    >From: Bill Tyler <tyler@ligo.caltech.edu>

    LIGO Hanford Observatory (LHO) Operations (Raab)


    FRED RAAB'S MAIL DESCRIPTION OF THE BRUSH FIRE AT HANFORD

    Last night the LIGO Hanford Observatory survived an intense brush fire
    without damage. The brush fire was started approximately 20 miles southwest
    of LIGO by a fatal car/truck collision on Tuesday. As of Wednesday
    afternoon it had jumped Highway 240 and was headed northwards, driven by
    high winds, toward the tank farms of the Hanford 200 area. At 6 pm, with
    the fire still about 10 miles west of LIGO and heading northerly I went
    home for dinner. Sometime after 7 pm I noticed the sky grow ominously dark
    over Richland and I began preparing to return to the observatory to check
    on conditions, suspecting the winds had shifted.  Richard McCarthy and I
    learned through Hanford emergency personnel that the fire was racing toward
    LIGO. Richard called the lab to tell people working inside and a touring
    Boy Scout group to evacuate the site. I drove in to ensure all personnel
    were out and Richard followed shortly to actuate our groundwater pumps and
    valves to recharge our firewater tanks.
     

    I found the site evacuated, except for Doug Cook, our laser safety officer,
    who had just completed a walk-through of all the labs and assured me that
    all personnel and visitors were gone. Hanford fire had set up a command
    post on the site, with a large number of fire engines, earth moving
    equipment attempting to trench firebreaks around the 10 mile perimeter of
    LIGO, and aircraft dropping fire retardant on the most threatened
    structures. By this time the winds had grown extremely strong with a wild
    fire out of control and bearing down on the observatory. For a time, the Y
    arm of LIGO served as a firebreak, but the winds eventually blew the fire
    over the arm and it raced further across the Hanford site. The fire started
    racing along the y arm past the mid and end stations. McCarthy and I went
    to the well (at the y end) to actuate the fire recharge system and were
    able to inspect those buildings at that time. The fire had burned out all
    the available fuel on the shrub-steppe surrounding these structures without
    damage to the structures. When we returned, the fire was challenging the
    corner station. I was able to inspect the site from the platform on the
    corner station roof and could see a line of fire advancing toward the x
    arm, but then a wall of smoke and high winds drove me off the roof. The
    combination of the extensive rock works we had installed surrounding our
    buildings and the firefighter's efforts prevailed as the fire burned down
    most of the grass and sage near the vertex, without placing significant
    heat loads on the buildings themselves. By this time I could see fire
    extending several miles to the east, about 15 miles to the west, about 10
    miles south and ascending Rattlesnake Mountain. The corner station was
    about the safest haven around, so we remained there.
     

    As the fire advanced along the Y arm burning away from the corner station,
    the firefighters rapidly left our site. I later found out that this was
    when the fire jumped the Yakima River, headed for populated areas of West
    Richland and Benton City, which were under evacuation orders. We remained,
    predominantly at the corner station, inspecting fire conditions with
    binoculars as the fire burned along the x arm toward the end station. The
    fire failed to jump the x arm and by midnight, it had burned past the x end
    station. We were able to drive out on the x arm at this time and inspect
    those buidlings, which looked OK. The winds were shifting and the fire
    started to advance northerly again. I expected it to start burning back
    toward the corner station along the north side of the x arm, but I knew our
    roads would provide adequate fire breaks. We decided conditions looked good
    enough to leave the observatory by driving north to the Wye barricade and
    then to Richland along Stevens Way.
     

    By morning the fire was mostly contained on the Hanford site, but was
    burning near populated areas. The population of these areas was evacuated
    to emergency shelters. According to radio reports, about 500-1000
    firefighters were on the fire, which had by now burned about 150 square
    miles of land. We instructed staff to remain at home while a few of us
    drove out to do an inspection under daylight conditions and to attend to
    checking systems. A power surge around midnight had taken down our turbo
    pumps (without any danger to the vacuum system) and we began a restart
    procedure. We drove the full 10 mile perimeter of the buildings and beam
    tube and found no discernible damage. We met with Rex Jordan and other
    officials of Hanford Fire and other DOE contractors who came out to inspect
    conditions at LIGO. The x end station was partially covered with fire
    retardant compound, whose sticky surface had a layer of ash glued onto it.
    I think the worst damage we may have is if the fire retardant damages the
    underlying paint. Otto Matherny is trying to get a contractor out as soon
    as possible to wash this down. The ventilation systems prevented smoke
    damage within the critical experimental areas although there is a slight
    smoke smell and dust levels were exceeded in the clean areas during the
    fire. None of the critical optics were exposed. Vacuum system operation has
    been restored to normal.
     

    The DOE contractors, especially Hanford Fire and Hanford Patrol, were
    exemplary in their efforts to keep us informed, to let key people into the
    affected areas while providing for public safety, and most importantly to
    bring tremendous resources to bear on protecting our structures. As of
    approximately 10:30 am PDT today, the state of emergency surrounding the
    LIGO area was lifted and roads into the area were opened. Some personnel
    are returning to resume installation/commissioning work.
     

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

    Some photos have been collected by Doug Cook, Richard McCarthy and Tom
    Mahood and I have them posted at

    http://www.ligo-wa.caltech.edu/wildfire/

    We will post more photos as we collect them.

    One of the noticeable oddities is the existence of small islands of unburnt
    shrub-steppe visible in the panoramas. Nightfire.jpg could have been taken
    in any direction last night.

    GHS NOTE:   We were very lucky. Fred and his colleagues did a very admirable job of stewardship at the site. The DOE earned our gratitude in this event. After the smoke clears, during the next month, we will have a lessons-learned meeting to review this experience and to capture insights for the next time.
     


    LIGO Livingston Observatory (LLO) Operations (Coles)



     

    OPTICS/COC INSTALLATION: Standoffs, guide rods and magnets were removed from our Beamsplitter, replaced, balanced and vacuum baked this week. BS returned to BSC-2 yesterday and we'll realign today. Used the time while the optic was in the oven to straighten the lab and shop areas. Small vacuum bake oven back online using an RGA Allen loaned us. Final COS bakeload completed; Kapton ground cables are now being baked. (Jonathan Kern)

    PSL: We replaced the main output laser beam periscope with a fixed one, non-adjustable one. All the fixed mounts for the PSL are in place. There was no difficulty attaining alignment with these fixed mounts. We will replace the few adjustable mounts that are necessary next week with Optosigma ultra-stable mounts. (Joe Kovalik)

    SMALL OPTICS: Three optics came out of the vacuum bake oven. We re-hung MC1 using the current suspension tower (i.e., the suspension tower that was on the HAM table before the door was opened). The new balancing angle is 0.18 mrad (the designed balancing angle of MC1 is 0 mrad, i.e., the new balancing angle is within the spec of +/-0.5 mrad). MC1 has been reinstalled on the HAM1 table. Before taking MC1 out of the HAM table, we checked the new alignment fixture using the PSL beam in HAM1 and HAM2. All fixtures work properly. (Sany Yoshida)

    LLO seismic array: We are gathering price information for the vault components to finalize the design and array layout. It appears that there is some confusion at PASSCAL regarding the delivery of the seismometers as the original request from Louisiana Tech seems to have gotten misplaced. Noel Bartow of PASSCAL said that she is working to straighten out the mess, but this probably means that our seismometers will dribble in rather than all arrive July 1 as originally requested.

    Community relations: Groups of 20-30 teachers from Livingston Parish public schools have been LLO for each of the three past Thursdays. This visit is part of in-service training for them. Many have expressed interest in coming for a return visit with their classes during the next academic year.


    MIT (Shoemaker)


    All activity reported in other categories


    Caltech (Sanders)


    All activity reported in other categories


    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

    Nergis Mavalvala, David Ottaway, Rana Adhikari, Doug Cook, Stan Whitcomb
    We have begun installation and testing of all analog modules in the LSC rack.

    We have moved IOT7 back to its location at HAM7 following flooring work. All light paths on the table have been aligned and the mode cleaner was locked.

    ISCT7 and ISCT9 have also been moved to their nominal positions by HAM7 and HAM9. We are in the process of aligning the tables with 1.06 um beam out of the viewports, after which we will complete the field cabling on the tables.

    Rana is testing/tuning the LSC photodetectors and has gotten at least one fully tuned for use on ISCT7.

    Suspension Tuning

    Mark Barton, Betsy Weaver
    This week we've been at LHO working on suspension controller tuning. We started working through the procedure (T000003) with the RM2K to refresh both our memories. There were a few places where the behaviour of the software was not quite as implied by the writeup, and as well as correcting those we ended up making a lot of other small changes to the software and the writeup to make the procedure easier. We tuned the input matrix for RM2K without incident. We attempted to tune the position component of the output matrix but got somewhat strange results - very different gain settings for the four actuators. It turns out that the UR actuator was dead. Richard and Josh measured the resistance of the coil at the vacuum feedthrough - it was around 5 ohms instead of the usual 18 ohms, suggesting that the coil is shorted at the end of the kapton cable. To fix it properly will require a vent but we may well be able to live with it until a scheduled vent for 4K installation. The software has already made a good effort at compensating in the position output matrix, and we can make analogous changes in the pitch and yaw matrices. We switched to working on the BS2K and already have the input matrix tuned.

    ###SEW adds
    The shorted coil on the RM will need to be fixed eventually, but should not prevent us from making significant progress bringing the LSC system up and beginning tests of its performance.  We will defer any action to fix this problem until a later date, possibly in conjunction with 4 km installation.

    ASC/LSC/SUS Electronics

    Rolf Bork
    I have primarily been trying to find a bug in the data acquisition system at Hanford which prevents us from pulling up GDS test points and excitation signals from the framebuilder.  Everything worked fine up thru June 18, but not since.  At first I thought it was something in my LSC code, which I was working on at the time, but it turns out that ASC test signals and GDS direct signals are not working either.  The last DAQ code change at Hanford was back in early May.  Only difference we know of is the configuration files, which were modified to add new channels.  We can find nothing obviously wrong with them, but I plan to load them onto the test system here at Caltech tonight and put in some extra diagnostics to try and track down the problem.  All channels other than TP and excitation seem to be ok.  The major impact of this problem is that it prevents us from running swept sine tests on the LSC digital filters as part of the LSC system testing.

    Mike Zucker, Rana Adhikari, Richard McCarthy
    Diagnosed and patched a high-frequency oscillation in the MC servo demod board.  This may have caused the wandering DC offset problem which sporadically impaired mode cleaner operation.

    Began measuring cable delays and wiring up the new (beautifully engineered!) RF reference distribution system for the three 2k modulation frequencies.

    Dale Ouimette, Mohana Mageswaram, Flavio Nocera
    We shipped to Hanford the following LSC boards this week:

  • 7 I&Q Demodulators
  • 4 Differential Driver/Receivers
  • 2 LSC Whitening Filters
  • 2 LSC Anti Alias Filters

  • We have started building another complete set of LSC electronics for Livingston.

    LIGO-Trinet Seismic Stations

    Szabi Marka, Hugh Radkins, Corey Gray
    The Preliminary survey results are posted at http://www.ligo.caltech.edu/~smarka/sne/LHO_survey.html with a link to the drawing of the planned LHO vault.

    1.2 LLO INSTALLATION & COMMISSIONING

    Core Optics Alignment

    Ken Mason
    The delay in the initial alignment schedule due to the beamsplitter made it possible to spend time preparing LLO personal for performing the alignments.  Monuments have been placed for completing the beamsplitter and aligning the ITM's.

    Core Optics Support (COS) Assembly

    Lee Cardenas, Ken Mailand, Joe Hansen, Mike Smith, et. al.
    Arm Cavity Baffle ITM- X & Y completely assembled including the beam dump black glass. These are wrapped and waiting for installation. The remained parts for the other two AC Baffle end station completely, staged , labeled and storage in the gray cabinets including the hardware, ready to be assembled later.

    Elliptical baffle staged and assembly in process.

    APS/PO Telescope: Four telescopes were pre-aligned and focussed and are awaiting installation.

    APS/PO Telescope Optical Train: Optical train parts are awaiting assembly.

    HAM2/HAM3 Beam dumps: The HAM2/HAM3 beam dump assemblies are in process.

    ASC/LSC Electronics

    Rich Abbott
    The frequency distribution system components that were sent back from LHO are being updated ready to be shipped to LLO

    Global Diagnostics System

    Szabi, Keisha Williams (SURF)
    Keisha is in the "overhead phase" working on her programming skills while also studying background materials for her project.

    2.0 Other Engineering and Scientific Activities

    2.1 Design/Analysis/Fab

    PSL

    Peter King
    In the last reporting period, it was reported that there was a peak in the modified current shunt transfer function and that it was suspected to be related to the relaxation oscillation.  As it turns out this was not the case, as the relaxation oscillation occurred at around 600 kHz and the "noise eater" was operational.   The reason for the peak is not clear.

    Orders for beam dumps and monitoring equipment for the 40m Lab PSL and LASTI laser have been ordered.

    Rich Abbott
    Prototype of new pockels cell driver for the frequency servo is being constructed with the goal of extending the useful bandwidth of the PA-85 output driver.

    Beginning the ordering of new items for the 40 meter and MIT PSLs.  All of the documentation is being reviewed with the goal of matching to "as builts" from the sites.  New release wiring diagrams and point to point wiring lists are being prepared.

    Beginning to plan the photodiode and servo for the intensity servo using the current shunt actuator that was retrofitted during my last visit to LHO.  This was chosen as the next item to finish as reports from LHO by Peter F.  indicate that the ISS is the next most desired item.

    ISC fab

    Mike Zucker, Ken Mason
    Working out video camera and lens deployment for shipment to LLO and LHO to complete the 4k's. Except for a few filters we now have all the video equipment in house.

    The ISC layer showing all ISC supplied equipment supplied to LLO has been completed and sent to Caltech to add to the integration drawing. Work has started on the LHO supplied equipment.

    Computing A new version of MSC Nastran finite element analysis 4.5.1 has been recieved and installed on several pc's.

    COC Metrology

    GariLynn Billingsley, Michael Hrynevych
    Metrology continues on ETM01.  We are currently performing the second of 6 measurements.  With fine tuning the thermal control system is becoming more robust.

    Suspensions/OSEM Head Re-Design

    Janeen Romie
    Working procurement of new osem parts.

    Data monitoring Tool

    John Zweizig
    This week I continued work on the DMT software. I added software contributed by LSC members, notably a operation status class that Keith Riles wrote. I have started to incorporate this into the designer dataset writer so that the designer datasets can be triggered on certain events, e.g. when an IFO or a cavity is locked.

    I also modified the name server to handle nodes that are connected to more than one network. Before this modification a client process would only be able to contact a given process through the network from which it registered. This change will allow monitors or servers running on the DMT machines to be contacted from either the CDS consoles or the GC network machines.

    Finally I worked with LDAS to verify that the Hanford LDAS system was receiving triggers properly from the DMT.

    Electronics

    Sander Liu
    EO shutter Controller - Completed building four (4) new EO Shutter Controllers. Expect to finish building the other three (3) by the end of this week and start testing them after the holidays.

    Global Diagnostic System Signal Processor - Printed Citcuit Board design is in progress.

    Electronics Shop

    Paul Russell
    I'm busy ordering new tools and equipment for the CDS Bridge lab. Coordinating with Ed Chargois about getting lab benches, chairs,etc.  working with Jo Ann the PMA administrator to re-plaster and paint the room and get phone and net hook-ups in there.

    2.2 Issues Concerns

    COS/Photon Calibrator interference

    Mike Smith
    Photon Calibrator Port for the X-end and Y-end is G2, and the reflected beam from the ETM will hit the ETM arm cavity baffle.
    Photon Calibrator Port for the X-mid and Y-mid is G5; there is no arm cavity baffle at the midstation to block the reflected beam.

    Optical Lever Lasers

    Mike Zucker
    We have been unable to obtain lifetime test data for 650 nm wavelength replacement lasers.  This wavelength appears to be somewhat better suited to our core optics coatings than the "certified" long-life 670 nm lasers (for which our 1064 HR turns out to be a good AR). We are assured they will be "significantly" longer-lived than our current 635 nm units however.  We are now discussing a pilot order for trial and installation in the Hanford 4k, with complete replacement contingent on our experience.


    40 Meter Interferometer (Weinstein)




    Thermal Noise Interferometer (Libbrecht)


    While working on the test cavity assemblies for the TNI, we also started
    installing a new version of our photothermal experiment, with which we
    intend to measure one of the thermal noise sources predicted by Braginsky,
    et al. (Phys. Lett. A 264, 1-10 (1999)).  We laid out a new optical setup,
    mode matched to the test cavity, and aligned one of the two beams we will
    be using to make the measurement.  We now have a nice TEM00 mode resonating
    in the cavity, and should be able to lock the system and get a preliminary
    signal in the next few days.
     

    Our test cavity is L-shaped, with a beamsplitter at the fold, and we
    observed an interesting effect while aligning it.  When misaligned, the
    cavity resonates in a "necklace-shaped" mode, much like a Herriott delay
    line.  The effect is not really surprising, once you think about it, but
    the spot pattern is quite pretty!
     


    LASTI (Zucker)


    No report received


    Data Analysis and Computing (Lazzarini)


    Simulation and Modeling

    LHO and PSL model

    Biplab visited LHO last week. He continued the work initiated at LHO.
    He worked with Rick and his SURF student, Brad on PSL noises.
    For those noise study of PSL, he introduced 'beam-wiggler' module.
    Kept working together with Brad on the shot noise in the error signal
    of the reference cavity when the mode is not matched.
    He introduced E2E to Rana Adhikari and David Ottaway. Rana wants to
    use it for Michelson runs.
    He sorted out differences among all latest versions of PSL and
    finally settled on a new version 0600.0_std_config  which is not
    much different from 08.0_std_config

    Adlib

    Hiro wrote the code to parse a text expressing equations.
    The code development is almost over and modeler code
    will be modified so that users can use expressions in the
    settings and can embed formulas in the box file using
    a new primitive.

    MSE

    G.Cella has committed his delivered software, including example codes and documents,
    in our CVS repository. Ed is working to modify so that MSE is fully
    integrated with e2e from the code management point of view.

    LIGO Data Analysis System

    LDAS Software

    The problems found with the managerAPI and genericAPI last week have been
    fixed and much of the week was spent retesting the LDAS system with these
    new patches. A run of the DMT trigger ingestion into the LDAS system early
    this week was fully successful at entering all 7120 triggers into the LDAS
    tables. ILWD socket test, database table insertion tests and frame to ILWD
    translation tests are currently underway. Preliminary results are looking
    great. The new tester has worked closely with the TCL staff during these
    tests as he prepares to take over these activities. We will meet later
    this week to determine the readiness of the LDAS software for a new release.
    All indications are that the system is in the most reliable state ever.
    There are still a few known problems, including a small memory leak in the
    frameAPI (most likely the TCL layer) which amounts to a few hundred bytes
    per gigabyte of data processed. And this is cleanly handled by the LDAS
    system managerAPI by having the frameAPI cleanly shutdown and restart during
    an idle period after a threshold memory leak has been detected.

    GUILD has been getting a lot of attention this week with new functionality
    being added to this user interface to support requests for frame data. The
    GUI will also display a list of channels in the frame and allow frame data
    from consecutive frames to be concatenated into a result set (frame/ilwd/xml).

    The work on the wrapperAPI has moved away from the MPI code development to
    modifications to the LAL library build process to support shared objects. The
    wrapperAPI itself had a bug discovered late last week in which data sent from
    the master to the slaves usually fails. This will need to be fixed before a
    test of the wrapperAPI with the LAL code from UWM can be made. The build of
    the MPI library and the wrapperAPI will also need to be repeated with several
    configuration modifications before the test to support shared objects.

    A meeting was held here at CIT to outline the user command that will drive
    the dataConditionAPI during its MDC. Two proposals were on the table. One
    with an OOP look and feel interface and the other with a scripting language
    look and feel. It was determined that the scripting language look and feel
    was adequate and easier on users and easier to implement. The code to handle
    pushing chains of commands down into the C++ layer and into threads is near
    to completion but much testing is still needed.

    Also this week, the FFTW development team finally responded to our weeks of
    notices concerning huge memory usage within this package. The FFTW teams
    now agrees with us that there is a problem and has made a commitment to have
    this fixed in the next release. But there is no commitment as to when that
    release will take place.

    We have a lot of work on the dataConditionAPI, mpiAPI, wrapperAPI, and the
    controlMonitorAPI still ahead of us. The debugging of the new release of
    LDAS has interfered with new development on these APIs but this is expected
    to shift in favor of new code development after the release.

    Lazzarini: I met with Eric Katsavanitas several times to go over LDAS with him as he starts
    to ponder his MIT involvement.

    General Computing

    MIT:
    Nothing to report.

    Livingston:
    We are in the process of surveying our software and hardware to
    determine what is in need of upgrade.

    Hanford:
    Working on the network expansion and s/w upgrades.

    CIT:

    Samantha (still on crutches) sshed into every sun and linux box and ran the sun
    script that detectspatches.
    Worked with screen savers.
    Called and chatted with Gateway personal multiple times, in a vain attempt to
    get the gateway box sitting on my desk fixed. They finally concluded that the
    hard drive is bad, just as Larry said it was weeks ago.
    Worked on a CD Rom that was not working quite right, I believe the
    problem is fixed, but will not know until the user gets back to me.
    Learned all sorts of new and cool stuff all unix related.
    Burned a number of CD's.
    Futzed with my desktop computer, vainly attempting to make it back into
    an even semi-stable system, but alas it is not to be.  Lookinginto different
    options to keep it stable in the future.
    Aquired mad crutching skills.  I can now walk to work.  It takes over
    fifteen minutes, but I do eventually make it:+)

    Barbara reworked the CostBook database and web forms for a different Activity
    Sheet identifier.
    Continued efforts on web forms for next LSC reporting period.  Purchased
    2 remaining license upgrades for WebBase.  Installed Office 2000 on my NT
    box.  The existing LSC reports database will not open in Access 2000; I'm
    trying to figure out why.
    Continued updating LSC web pages.  Added more reports and attachments.
    Set up new institutions.  Updated the Council page using latest Z attachments.
    Worked with Larry changing the setup on the Primavera NT server in attempts
    to improve the performance of the unit.

    Lisa performed a demo network installation of StarOffice 5.2 on graffias.  The
    installation procedure went well but it still needs a round of client testing
    before it is deployed on sirius.
    Replicated the samba problem that Jay was experiencing using Protel98 on Luna
    (but not on sirius).  This indicated that it was a problem in either samba or
    the network connection to luna.  I installed version 1.9.17p3 of samba on luna.
    Initial testing looks like this might firm up the connection, but we won't be
    sure until after Jay has a chance to run the connection during a
    high load of traffic.
    Installed ssh2 on luna.  Now that this is working we need to make sure that
    F-secure is running on all the PCs and that everyone is trained on how to use it
    with Exceed.
    Installed the 6/23/00 jumbo patch cluster on luna.
    Began working with Rolf on how the VME crates boot from luna/kater.
    Got a tutorial on monthly backups from Suresh.  Sam and I are jointly running
    the monthly backups for June.
    Got a tutorial on managing user accounts.
    Worked with Sam on running patchdiag to determine the patch level of all the
    Solaris boxes.
    Began looking into the problems Todd Etzel (Wilson house) is having on Cheetah.
    These include:
    - file locking errors in his email (fixed)
    - NIS+ password problems
    - SSH daemon has fatal errors when it starts.  This looks like a shared library
    problem.  Cheetah is running OS 5.5.1.  A recent set of patches will probably
    fix this, but Todd would prefer to have cheetah swapped out for a PC instead.
    He needs StarOffice.

    (Suresh)Installed GPIB-SCSI-A driver in system named tiger after loading solaris
    2.5.1 in RSE Lab in Lauritsen. This would enable to display output from spectrum
    analyser by using Labview.
    Put system named bala (Ultra 1) in 131.215.120 network and made a client of
    LIGO domain in Synchrotron Lab for use by SAS (Ricardo's) group.
    Demonstrated how monthly backups of LIGO servers are done to Samantha and
    Lisa.

    (Larry) Resolved a number of PC issues. There are a number of utilities such as
    crash guard that cause more problems than they prevent. The best things is to
    run the utilities once a week or at bootup but don't have them running in the
    background, this takes away resources the computer can use for other programs.
    Worked a number of procurement issues including the SUN order. It looks like the
    order is now with SUN and we are trying to get a partial part of the order
    expedited.
    Working on some of the logistics and costs to get the Observatories network
    connections upgraded. Both Larry and Albert have been making contacts to try and
    get more information on what needs to be done.
    Evaluating a problem tracking s/w pkg. that LDAS is using to see if it would
    work with the GC group.
     


    LIGO II/Advanced R&D (Sanders)


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

    I am requesting a quote for Suprasil 311 SV glass in the shapes of rods and "microscope slides" from Heraeus Amersil.  These are for Phil Willems and Gregg Harry (Syracuse.)

    Veeco has still not responded with a quote for upgrading the IR Metrology interferometer.

    The first 15 cm diameter sapphire blank shipped to CSIRO, they are to measure the homogeneity of two pieces.

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

    Attended CleanTech 2000, an International Cleaning Technology Conference and Exposition.
    The most positive outcome from the Conference, was to be able to identify and contact some vendors that could supply equipment needed for LIGO II.
    As an example: an ergonomic arm to perform mirror lifting and positioning in fixtures during substrate/mirror characterization, cleaning, and assembly. And a customized cleaning and drying system for mirrors.

    LIGO II coatings:
    A preliminary talk (for costing purposes) with Ramin from REO, reinforces the fact that REO took a "real commercial"  business path during the last year.
    Each ion beam sputtering chamber, they have around 10 by now, produces $100,000.00 a day.
    Research and development of coatings implies tying a coating chamber for extended periods of time.
    LIGO II optics would require coating development to achieve uniformity on the larger substrates and to achieve lower absorption.
    To accommodate the larger substrates the chamber would require mayor re-tooling.
    A ball park figure for these tasks is between $1.5 M and $2 M. (Does not include the coating of the LIGO II mirrors).
    Also, the possibility exist, that when the time comes for the LIGO II coatings to materialize, REO could be on a different business tempo.
    We discussed different possibilities, I think that a meeting is required to develop a plan to ensure we can procure coated optics in time, within specs. and budget.
     

    From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>

    Welcome Susha and Paolo

    Started lab removal,  big mess but will get better.
    Due to removal slowdown and 4th of July festivities next week no group
    meeting and no weekly report.
    Virginio will run group meeting of July 12th and write status report.

    Hareem, Paolo, Riccardo
    Started oil bearing, shortly followed by recycling pump breakdown,
    despite specs the pump lining was not oil compatible, an oil bath
    ensued.  Tested second set of oil pump, this one was not compatible with
    the bubbles in the recovery oil.  Finally tested pumps from C&H surplus
    store;  these pumps seem to work, The oil bearing and IP testing
    facility should be finally up and running by the 4th of July.

    Hareem, Akiteru
    Measured thermal drift of GASF and MGASF at 230 mHz.  This time it is a
    stable 1 mm/degree.  Proven that the Akiteru-Tatsuo measurement was
    transient dominated.
    Start designing a simple bi-metal spring compensator to passively null
    the filter vertical load point thermal sensitivity.

    Hareem
    Changed load disk in GASF, obtained 170 mHz, going to extend Quality
    factor and thermal stability measurements in this frequency range.

    Hareem, Virginio
    Writing GASF paper.

    Brett
    Component acquisition for stepper motor controllers, e.t.a. this week.
    Finished and tested hand wired driver boards, will make PCB version in
    background priority with Flavio’s assistance.

    James
    Learning Transfer function measurement techniques.
    Populated an LVDT board, built some coils.

    Erik.
    Reported on suspension fiber TNI feasibility and on related discussions
    with Vladimir.

    Susha
    Started working/learning MSE
    Studying static profile of blades in MGASF plus dynamic range behaviour
    around w.p..

    Chenyang
    Starting up Marconi AC electrostatic actuator demonstrator.

    Akiteru, Kenji
    Confirmed 50 dB performance of 1.5 mm MGASF; The 70 dB were faked by a
    miscalibration in connecting two different frequency ranges.  Result now
    qualitatively agrees with expectation that less stressed blades produce
    worse attenuation plateau.

    Akiteru
    TAMA suspension design.

    Alessandro
    Advancing in accelerometer circuit construction.
    Accelerometer item one construction delayed by lack of special end
    mills.
    Present accelerometer item one e.t.a. is Monday or Tuesday.

    Soy
    LVDT driver work.
    Tooling up a stand for acoustic emission measurements in stressed
    blades.

    Virginio, Riccardo
    Continuing heavy duty supervision work.
     

    Virginio
    Re-diagonalization of Ip controls for new load and new LVDT
    positionings.  Wrapping up for removal of IP.
    Remaining some accelerometer testing with Akiteru before removal.

    Virginio, Akiteru
    IP long term drift measurement. Found no correlation with temperature.
    Only floor tilting (within 5 micro rad/day) observed occasional sudden
    shifts of tens of nano-rads.
    Tilting compatible to known building stability.

    Gilberto
    LVDT calibrations for creep measurement. 4 made, found some glitch,
    probably in measurement technique.

    Lisa
    Running thermal stability measurement. Found problems in including LVDTs
    in the DAQ, may be simpler to change existing card.

    Szabi
    Remotely assisting in solving DAQ problems.

    Paolo
    Starting compilation of transfer function, sensitivities and seismic
    activities.

    Data acquisition status report (from Virginio).
    Three PC computers in the lab.
    C1 reserved for creep with K. DAQ
    C2 running IP controls and thermal measurements with DSP and NI DAQ
    C3 general purpose use

    Receiving a work station from Suresh.

    Need to run thermal stability stand, TAMA SAS stand and acoustic
    emission stand.
    Filter transfer functions generally run on spectrum analyser.

    Need at least another PC and two DAQ cards.

    Waiting for the return of the second broken DSP card (shipped today).
    We will need another one for the lab plus need to order all the TAMA
    ones.
    Waiting for a second DSP crate, late on e.t.a..

    For those who enquired, the report order is given by the sitting
    position of the people coming to the meeting, starting clockwise from my
    chair.


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