Weekly Report for Week Ending August 3, 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  August 7, 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
 

Special Items:


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


No report this week.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


WBS 1.2 LIGO Operations--Administration


LIGO Weekly Site Telecon (Lindquist)


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. . .

 ACTIVITY HIGHLIGHTS

From: Cleveland Mak <mak_c@ligo.caltech.edu>
 
In Out
Packages 26 12
Faxes 27 30

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>

Finished up the lease agreement.  Have several subcontracts to do and need to set up the files on these.  Reconciled pcard transactions and placed new orders on the pcard.  Closed a few PO's out, but expect to start closing PO's again on Monday.

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 (Wood)

Dorothy Lloyd

Graphic provided by Cindy Akutagawa

Irene Baldon

Elizabeth K. Wood

Advanced LIGO (Frey, Petrac)

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

Progress Period from 7.28 to 8.3

Accomplishments:

Schedule: 8.4 to 8.10 Anticipated Challenges: Corrective Action: From: Irena Petrac <irena@ligo.caltech.edu>

WBS 1.4.1.2   Project Controls (LIGO Construction)

Reports (Lindquist)

I have distributed a second draft budget for FY 2001 Operations and already received some comments that will be incorporated.  Task managers are requested to provide substantive corrections by Friday, August 11, 2000.  I have also started the text portions of the submittal for FY 2001 Continuing Operations.  Everything related to the proposals continues to be a month or so behind schedule.


Change Control/Contingency (Lindquist)

A meeting of  LIGO Change Control Board, Tuesday, August 1, 2000 at 9:30 PDT in the Science Conference Room (SCR)

The following change requests were approved:
 

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 Controllers for Large Optics Suspensions 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
CR-000013 WBS 1.2.2 Redesign Controllers for Small Optics Suspensions D. Coyne

Minutes of the LIGO Change Control Board have been prepared and will be distributed (See LIGO-M000237-00-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)

From: Irena Petrac <irena@ligo.caltech.edu>

CO #7 was processed for a-cost extension of the REO contract to allow completion of ongoing coating and re-coating of LIGO I optics.

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

See above.


Quality/Safety (Tyler)

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

LIGO Hanford Observatory (LHO) Operations (Raab)


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

Activities are heating up related to installation as evidenced by the greater length of this report. An optic was scratched near its edge in handling, but a review of the situation indicates it should not adversely affect performance.
 

The Kamiakin SST team have gotten some nice measurements of ground vibrations from the present gravel mine in south Richland. They have collected field measurements at a number of sites at various distances from the plant, with plant operations on/off and with varying distance from the local highway. Analysis proceeds.
 

Bake Oven:
----------
(K. Ryan)
 

LHO Vacuum Bake Oven A load #98, consisting of misc. COS parts & fasteners and misc. small optics beam dump and mirror mount components, was released on 8-2-00.

Load #99, consisting of new OSEM bodies and misc. IOO (SOS top block) and COS parts, is to begin vacuum baking on the afternoon of 8/3/00- to be released on 8/7/00.
 

PreStabilized Laser:
--------------------
(R. Savage)
 

- Recently, a problem with the HVAC system in the LVEA caused a diurnal
temperature variation of several degrees Fahrenheit.   As a result, the PSL
output power varied by several percent.  The HVAC system has been patched
and the large PSL power fluctuations eliminated.  M. Guenther is using the
data from this accidental experiment in an effort to understand and
hopefully reduce the sensitivity of the PSL output power to ambient
temperature variations.  M. Lubinski has installed a temperature sensor
that is connected to the DAQ system in the 2k PSL chiller closet that
should help us assess the role of the closet temperature variations.
 

- We have received the acoustic insulation panels for the 2k PSL table
enclosure.  We ordered panels covered with PVF film rather than PVC film.
We don't notice any odor from the new panels as we did from the PVC-covered
panels.  G. Moreno is using the 4k PSL enclosure to investigate a method of
attaching the panels.
 

- T. Mahood has generated a new comprehensive optical layout of the 2k
IOO/PSL optical table using autocad.  The layout is to scale, +,- ~ 0.25
inch.  He is in the process of updating the optical component information
and is following the naming schemes devised by M. Guenther and the IOO group.
 

- T. Mahood, D. Cook and R. Savage have begun installing the
upgraded beam dumps on the PSL IOO optical table.  D. Cook has cut the beam
tubes (1" diameter Al. tubing) to length and they are out for anodizing.
 

- D. Ottaway and R. Savage plan to release a new draft of the LIGO II PSL
Conceptual Design Document (in the new Microsoft Word format) by early next
week.  It appears that the Design Requirements Review for the LIGO II PSL
will not take place during the LSC meeting next month as previously planned.
 
 

Optics:
---------------------
(D. Cook)
 

The ETMx-4k has its magnets/standoff glued and we will balance it Friday and
get it into the Vacuum bake on Tuesday. ETMy-4k will be have the guide rod
and wire standoff glued on Friday and the Magnets/standoffs and balance
hopefully in time to hit the same bake load on Tues. The ETM transmission
monitors are being installed after sorting through some minor confusions
and modifications. The optical levers will follow as parts are received.
The new OSEMs will come out of the bake and sent to MIT to be completed and
tested. The ETM optics HR surface yields ~ 1% reflectivity at 633 nm. This
is too low for our total station autocollimator. Upon its availability, we
will borrow the one from LLO which has been modified and is more sensitive
to weaker return signals. We will use ours for the balancing and wedge
angle measurements in the interim. Betsy continues to build up the COS
components as time allows.
 

Seismic Systems:
----------------------
(C. Gray, M. Guenther & H. Radkins)
 

Are seeing light at the end of the tunnel for the transfer function
measurements for a BSC Seismic Isolation Stack (at X-End).  Have performed
a few Swept Sine Measurements on the stack, but have had difficulties
producing coherence plots for these measurements.  Will now try to obtain
coherence data by using "white noise" as a source for our system.
 

Ribbon Cable Sag Test is still on going and Coarse Actuation System (CAS)
cabling installation is a background activity.
 

Controls:
---------
(D. Barker)
 

Replaced 50GB Cybernetics RAID with 18GB Sun and 36GB IBM disks on
hanford1. Waiting for RMAs to return Cybernetics RAID and Tape Robot for
repair. Using exabyte tape for CDS backups in the mean time, at a much
reduced rate.
 

Coding the next release of the DAQ ADCU code, which will run more
efficiently by using the DMA engines in both the onboard VIC64 chip on
the baja, and the DMA chips on the VMIC 5588 RFM modules. This will free
the baja CPU to perform digital filtering when decimating the data. Data
transmission to the RFM will be more closely monitored. In cases of
network collisions a "back off then retry" algorithm will be used. DCU
processing will be handled by three tasks instead of the current single
task, allowing for parallel processing of the tasks.
 

Completing the LHO EPICS save/restore system by forcing passive output
records to run at initialisation time to restore the saved setting.
 

Preparing for the CDS upgrade at Louisiana which will take place at the
end of the month.
 

Physics Environmental Monitoring:
---------------------------------
(M. Lubinski)
 

We are changing the gain setting in the Endevco accelerometer
chassis (Isotron power supply, model 2793) from X1(factory setting) to X10.
This will increase sensitivity of the instruments.  We are also working on
calibration of accelerometers to be able to correlate counts to acceleration.
 

We have developed a calibration method for the microphones using a Bruel
and Kjaer piston phone (model 4228) calibration unit with an attenuator unit
attached.  This calibration is in progress.  All of the data for the above
calibrations will be put on the CDS web page under "Installation files"
when completed.


LIGO Livingston Observatory (LLO) Operations (Coles)


The new Pre Mode Cleaner is running continuously with 5.4 Watts of output
with 7 Watts of input power. The cavity FWHM was measured to be 4.5 MHz.
The old pre mode cleaner was open to the atmosphere and the feedback
voltage on the PZT to keep it locked showed a strong correlation with
atmospheric pressure. The new pre mode cleaner is hermetically sealed. The
PZT voltage no longer shows any correlation with atmospheric pressure, but
rather strongly correlates with the table temperature.
 

Sany, Haisheng, and Dave R. worked on getting the mode cleaner and MMT
aligned.  We discovered that some of the cabling which carries the MC
alignment bias voltage into the controllers had been crossed. Cables are
now labeled and connected to the proper controllers. The MC has been
aligned to the point where flashes are coming through MC3. Beams are
centered on the mirrors to 1 mm or better. Pitch and Yaw biases for the MCs
are in the range |1 - 4| V. Reflected and transmitted MC beams are aligned
out of the chamber for IOT pickoff. MMT alignment - SM1 had to be shifted a
few mm to center the beam on the mirror. Faraday is aligned; MMT alignment
underway.


MIT (Shoemaker)


All activity reported elsewhere.


Caltech (Sanders)


Kip Thorne has organized an association of the gravitation research projects at Caltech and JPL. An organizing meeting was held last Friday. Among other things, it was decided to combine and share the associations seminar series with the LIGO series, approximately equally. The time for the seminar series has been movedto a time convenient for the JPL attendees so they do not have to make a roundtrip. Thus, in the fall, the combined seminar series will meet on Fridays at 4 pm, not at the old Tuesday 11:00 am time.


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

Mike Zucker, Nergis Mavalvala, Rana Adhikari
Trying to obtain multichannel time series of single-arm lock attempt, with view toward comparison with E2E results and diagnosis of locking problems described last week. Got readouts working on internal recycling cavity pickoff light and got dark port wavefront sensor working, although control loop code seems to be broken and parts of both WFS demodulator boards on site turned out to be fried. Debugging and repairing software and hardware problems continues and hope springs eternal.

4km Suspensions

Janeen Romie, Phoenix Hoang, Paul Russell, Helena Armandula
Working procurement of new OSEM parts and fixtures. Fixture for mounting boards works; Physics machine shop is making 8 more sets by 8/8. Phoenix is assembling the circuit boards. Paul is making the PFA connectors. Helena is helping to write the assembly procedure. Working on design documentation.
During processing of the first 10 short and 10 long OSEMs, one short OSEM has broken. We will investigate why/how this occurred and determine a course of action.
Supporting LHO personnel with their processing/assembly of the ETM suspensions.

1.2 LLO INSTALLATION & COMMISSIONING

Input  Optics

Sany Yoshida, Haisheng Rong, Dave Reitze
MC alignment: We discovered that some of the cabling which carried the alignment bias voltage into the controllers had been crossed.  Cables are now labeled and connected to the proper controllers.  The MC has been aligned to the point where flashes are coming through MC3.  Beams are centered on the mirrors to 1 mm or better.  Pitch and Yaw biases for the MCs are in the range |1 - 4| V.  Reflected and transmitted MC beams are aligned out of the chamber for IOT pickoff.
MMT alignment: SM1 had to be shifted a few mm to center the beam on the mirror.  Faraday is aligned; MMT alignment underway.

ITMy

Gary Traylor, Joe Hanson, Harry Overmeyer
Completed reprocessing the ITMy (as a result of the failed rear face magnet, which was in turn a casualty of investigating why the aligment was drifting in pitch) and have installed the ITMy back into chamber LBSC1. Alignment to follow.

PEM Audit

Peter Saulson
The first phase of our PEM Audit, carried out with students from UT Brownsville, wrapped up with a final presentation by the teams working on the tiltmeters and on the accelerometers. They are leaving behind a written report of their work. It was a very successful student project, that will leave a genuine legacy for LIGO. We will have to develop a plan to continue the work with permanent LLO staff.

Core Optics Support (COS)

Lee Cardenas
  • Installed the (2) Black glass pieces missing in the Cavity Beam Dump in BSC2.
  • Gathered all the COS spare parts, which will be shipped to LHO.
  • Prepared and separated all the parts needed to complete installation and alignment for the PO telescope in HAM3.
  • PSL

    Peter King, Joe Kovalik
    The performance of the new pre-modecleaner is being monitored.  At one stage the visibility (1 - locked / unlocked) was tweaked to greater than 90%.  This was found to degrade during the installation of the pre-modecleaner for reasons unknown at the time.  Joe K has been monitoring the performance and concluded that the laser power was varying during the periods of observed visibility decay.
    A small analyzer cavity was fabricated to measure the PSL frequency noise. The analyzer cavity has a PZT at one end, otherwise it is the same as the reference cavity.

    Lee Cardenas

  • Gathered the old pre-mode cleaner (PMC) assembly and set it in the optic lab to be taken apart carefully.
  • Gathered and shipped all the equipment needed for assembly of a new PMC for the PSL at CIT.
  • Preparation for changing and flushing the heat exchanger cooling water for the Laser is on-going.
  • Contacted Class One Co. for the new Laser Enclosure with acoustic sound proof material.

  •  

     

    Rich Abbott
    Shipped a full set of frequency distribution components to LLO for installation in the near term on a trip to the site that I am planning.

    SUS Electronics

    Jay Heefner
    This week we have received 3 broken LOS controllers. Two have been repaired and sent back to LLO. One had a blown basic stamp. The other had a vaporized trace on a coil driver output.
    A blown satellite amplifier has been received and is being repaired. It appears as though the 24 volt input power had been reversed which blow up a capacitor and destroyed both regulators. In addition two of the PD monitors are blown, the result of being connected to a shorted cable. A second satellite received earlier also appears to have been reversed polarized and connected to shorted cables on the PD monitors. Both units will be repaired and sent back.

    LLO One Arm Test

    Jay Heefner
    The system drawing and cross connect lists for the one arm test have been completed and sent to Rusyl. He will begin building the cross connect harness and installation of equipment when he receives all the parts. The system should be ready for test some time in early Sept.

    Suspensions Controller Tuning

    Mark Barton
    This week I spent at LLO doing more suspension controller tuning R&D. There were a number of teething problems with the data acquisition system and the controllers so I started with a fair bit of debugging. The MC1 controller had to have its RS232 interface replaced and the SM1 needs the same fix. I ended up taking some good data on MC3 and developed a new chunk of the procedure: tuning the position component of the output matrix using the tuned input matrix as a reference (as opposed to using optical levers).

    2.0 Other Engineering and Scientific Activities

    2.1 Design/Analysis/Fab

    PSL

    Peter King, Rich Abbott, Todd Etzel
    A number of modifications to the FAST path of the frequency stabilization servo have been made and studied by Rich and Todd, to improve the robustness of lock and lock acquisition response.  The servo at present limits the FAST actuator dynamic range and places slightly more burden on the SLOW actuator.  In this configuration, with the FAST actuator centered, the servo recovered spontaneously at operational COMMON and FAST gains. With the FAST actuator voltage biased, recovery takes a little longer, since the SLOW actuator is adjusted to correct for offsets in the FAST actuator voltage.  Once the SLOW actuator is adjusted to bring the FAST actuator to within approximately 0.5 V of center, the servo recovers.  More investigations are continuing to see if this is a reproducible result on a different servo card (of the same rev. level).
    At present the SLOW actuator voltage is controlled by a simple deadband algorithm.  For better control, this will change to a EPICS PID record to remove the +/-0.5 V deadband.

    COC Metrology

    GariLynn Billingsley, Michael Hrynevych
    Michael Hrynevych's last day was Friday July 28, best of luck to him in his new job.
    Measurement of 4ITM06 is complete, measurement of 4ITM07 has started. 4ITM06 shows a Radius of curvature of 13.68 km, comfortably within the spec of 14.18 +140, -1000 The rms deviation from a perfect flat after subtraction of Tilt Power and Astigmatism over 80 mm is 0.79 nm. The requirement is that it be less than 0.8 nm rms.

    LSC Electronics

    Dale Ouimette, Mohana Mageswaram, Flavio Nocera
    Mohana is doing the re-design, including Cadence simulation for the gain requirements and the noise analysis, for the Mode Cleaner Servo Amp.

    Modulated OSEM  & Digital Suspension Controller Design

    Jay Heefner
  • The schematics for the suppressed carrier version of the AC OSEMs are 90% complete. Board layout will begin by 8/4.
  • The prototype for the amplitude stabilized oscillator version of the AC OSEMs is being tested. Initial tests show amplitude stabilization of 1e10-5 to 1e10-6. It is hoped that 10e-7 can be achieved.
  • The document describing the digital suspension controls has been released and a review has been scheduled for 8/2.
  • The PD whitening and interface boards for the LHO 4K SOS controls have been stuffed and will be tested next week.
  • GDS electronics

    Sander Liu, Paul Russell
    Placed an order with Bloss to fabricate the chassis faceplates. They should be back within the next couple of weeks. Circuit boards from TechniCircuits should be in sometime next week for us to begin assembling them.

    DMT

    John Zweizig
    This week I continued to debug and improve the DMT library software, including testing and fixing the inverse Fourier transform code, reorganizing frequency series storage to make it more obvious (although probably less efficient), writing a Perl script to display the DMT data manager status, and updating documentation.

    2.2 Issues Concerns

    Better MTBF Optical Lever Lasers

    Mike Zucker, Ken Mason
    Placed order for 30 new optical lever lasers with Point Source ltd. These units have been engineered for reliability and tested by the manufacturers; projected MTTF indicates 2 or fewer failures expected during LIGO I observation & commissioning period. They will be integrated initially at H4k and then retrofitted to H2k and L4k machines.

    PSL Laser Supply Trip-out problem solved

    Peter King
    I have been told that Lightwave have "fixed" the problem with the laser power supply tripping out -- something which occurs more frequently at LHO than at LLO.  The problem being that the diode protection circuitry was too sensitive to transients.  This has been apparently fixed by removing the protection circuitry. After an engineering review, Lightwave Electronics decided to remove this diode protection circuit from all their products, not just the 10-W LIGO Laser.

    40 Meter Interferometer (Weinstein)




    Thermal Noise Interferometer (Libbrecht)


    This week, still with Seiji's considerable help, we have been studying the
    noise in our mode cleaner frequency-stabilization servo.  We measured both
    the electronic noise and the shot noise in our frequency measurement system
    (photodiode, demodulator, etc.) and found them to be comparable.  We have
    also been moving components in the feedback loop around to improve its
    noise performance and to replace as many active components as possible with
    passive ones.
     

    We have successfully glued magnets and guide rods to two test masses, and
    we plan to begin installing one test cavity in a few days.  There's a fair
    bit of electronics that needs to be built before we will have a working
    suspended test cavity, but we have decided to take advantage of Seiji's
    expertise while he is here and install the mirrors anyway, clamp the masses
    down with their earthquake stops and look at the finesse and throughput of
    the cavity.  The mirrors will remain under vacuum during these tests and
    while the electronics are being finished.


    LASTI (Zucker)


    LASTI: Continued work on documentation for LASTI program discussion and review
    for week of 8/15.

    LIGO II ISC: Continued work on WBS dictionary.  Circulated "fanciful" hybrid
    block diagram of sensing & control scheme, incorporating elements of all major
    modulation/readout schemes under current consideration, to act as a strawman
    for hardware & software cost effort.

    HAM Installation

    All parts and tooling for the installation of the first HAM seismic
    isolation system has been located with the exception of an adapter plate
    and hardware. These items are short lead and will be ordered early next
    week if not found before then.

    Installation is scheduled to begin 9/11. LLO will be sending 2 people
    for two weeks to get us started.

    Recieved and installed Algor analysis software to assist Stanford with
    STIFF prototype design.
     


    Data Analysis and Computing (Lazzarini)


    Simulation and Modeling


    Lock Acquisition

    Matt is working to implement a better logic for Jim's RSE.
    He is also working to find a better robust locking of LHO Michelson.

    PSL

    Rick, Brad and Biplab kept working to study the noise sources of
    PSL using e2e. The result will be summarized in the SURF report.
    (possibly LIGO note, or better yet publication?)

    adlib

    Biplab worked hard to trace bugs which were found when the mis aligment
    effect for the lock acquisition was studied. The bug fix release will be
    very
    soon.

    alfi / GUI

    A new version, 4.0.13, was released. New features in this release are
    (1) better support of multiple directories
    (2) better information feedback to the user
    in addition to the fixes of some of the known bugs.
    A few problems were found after the release and Bruce worked to trace
    the cause. A new revised version is expected to be released very soon.
    After that revised version goes through basic QA, it will be installed
    at
    LHO.

    Improvement works are going on as well. Bruce is working to implement
    a better interface to edit the settings. He is also working to implement

    a semi-automatized ALFI test suite so that ALFI can be tested more
    reliably after changes are made in maintenance and features are added.

    LIGO Data Analysis System

  • Software Systems (Blackburn)

  • (Lazzarini for Kent)
    This week has been consumed by an intense effort to perform the first LDAS Mock Data Challenge. More will be provided next week. PSU, UTB and ANU visitors have been working around the clock with LIGO people to complete the challenge.
     
  • Hardware Systems (Anderson)

  • ----- Forwarded message from Omar Rashad (LDAS SysAdmin) -----

    Applied slight tweaks to LDAS servers requested for MDC
    Resurrected muscida from temp storage for usage by visitors for MDC

    Gnats:
    Added MDC visitors to edit access for ldas-bugs database
    Created associations from newly utilized mdc categories to responsible
      email addresses
    Corrected associations in the ldas_procurrements db to use alias groups
      and migrated references in existing problem reports
    Similar corrections should be applied to GC database

    Installs/reinstalls:
    Resurrected apache on ldas-wa after server hardware replacement
    Reinstalling Linux OS on kitalpha and all 8 beowulf nodes to bring them up
      to must current official release
    Helping with Linux install on users laptops

    ----- End of forwarded message from Omar Rashad (LDAS SysAdmin) -----

    For Omar add,
    Fixed hardware problem with ldas-pcdev1 that prevented it from using
    both CPU's.
     

    P.S. Should we consider opening up the GNATS ldas_procurement table to
    perusal by interested LSC members? I can imagine that some of them
    will be interested to know when certain computational resources
    will be made avilable.

     
  • Data Analysis Activities
  • New LIGO visitors to LDAS:
    Sathya is here from GEO to work for one month with Tom, Jeff Edlund, and myself one understanding how to integrate the Fast Chirp Transform (FCT) approach with the standard template based optimal filtering approach -- e.g., finding regions in the parameter space where there is complementarity, etc.

    Also, Beoit Mours has arrived for his year-long sabbatical visit from VIRGO. He will likely work in two areas: user interfaces to LDAS (with Peter Shawhan); multiple interferometer analysis (with Sam Finn and other GWIC researchers in this area).
     

    LIGO-SNEWS: (K. Ganezer, A Lazzarini, Sz. Marka)
    We welcome Albert Lazzarini in our group. Albert helped us along the
    way to draft our proposal and plans to participate in the development of
    our coincidence system.
    We sheduled our introductory SNEW talk for the 08/2000 LSC Meeting in
    Hanford. We would like to use the opportunity discuss the project with
    interested LSC members especially experts already working on burst
    detection algorithms.

    Jeff Edlund (summer student):

    I modified the code for the Fast Chirp Transform (FCT) so that it
    automatically corrects for phase functions that are not 0 at x=0 and 1 at
    x=1.  Phase functions are now only required to be monotonically
    increasing.

    I started a small web page to keep track of my progress.

    I completed my comparison of the 2D FFT FCT method and our new method that
    does the FFTs of the columns by inspection. I showed that the results at
    powers of 2 were consistent with the change in order.

    I'm currently working on understanding how to apply the FCT to
    gravitational chirps from the binary inspiral of neutron stars.
     
     

    General Computing


    MIT:
    Has received most of the SUN equipment from the special SUN order.
    Larry will be traveling to MIT the third week of August to assist in setting the
    new computers up.
     

    Livingston:
    Nothing to report from General Computing. Bellsouth and LSC did have some
    network problems but they did not adversly affect the Observatory.

    Hanford:
    Preparing for the LSC meeting.

    CIT:
    (Barbara)
    - Continued work on the web reports for the CostBook.
    - Helped Irena with the LSC progress reports and research plans.  Made some
    minor changes to the Access application.

    (Sam)
    Finished up a new PC build. Worked on documentation.

    (Lisa)
    - Finished monthly backups.  This included centralizing the backup scripts and
    changing them to use hardware compression.  We are still only getting about 10G
    per tape.I want to look into it a bit more to see if I can get closer to the
    14G mark.
    - Added users to the dial up access. Will add an entry to the FAQ
    on how to configure a user for dial-up. Will work on DHCP configuration for
    dial-up services.
    - Changed (with Larry's help) the automaps on sirius and sadal.  Both servers
    still had remnants of maps from kater and puma which was affecting my ability to
    install the new cadence software.
    - Cadence installation has begun.
    - Worked with Larry on moving the home accounts on home8 to a larger disk array.
    - Provided user support to Wilson House. Worked with Larry on installing the
    Multi-mode to Single-mode signal converter. The first test did not pass on the
    single mode connection so there will have to be some tweaking done.

    (Suresh)
    Still in Nepal visiting family.

    (Larry)
    - Still working procurement issues most dealing with LDAS but still have a
    number of items for the GC.
    - Resolved a number of PC issues, most dealing with incorrect installations of
    s/w. Just a reminder for everyone to keep their virus-scan up to date, we've had
    a number of hits this past week and so far no major problems and the virus-scan
    s/w has helped in keeping the problems to a minimum.
    - Installed a few more hubs and ran some more cable for the network.
    - Working with Ed C. on getting some of the old equipment moved out.
    - Started installation of equipment into a new rack.
    - Working with Liz to get an area set aside for people to use the scanner and CD
    burner. Presently, looking at location on the third floor of Bridge.
     


    LIGO II/Advanced R&D (Sanders)


    From: Janeen Hazel <romie_j@ligo.caltech.edu>
    Suspensions - Wednesday August 2, 2000

    Working on LIGO II Proposal. Updated the Development Plan and the Table
    listing which optic with which type of suspension (on the L2 Proposal
    Suspension page.)

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

    A preliminary cost estimate has been received from CSIRO for polishing a Pathfinder II piece.  I will discuss this with them in depth when I visit next week to take part in sapphire homogeneity measurements.

    A SUS-COC interface meeting was held to try and find the dotted line between the subsystems and to decide what type of requirements SUS might put on COC.  More in depth questions to follow, but it was a good start.
     

    From: Jordan Camp <jordan@ligo.caltech.edu>

    Worked on LIGO-II PSL and COC proposal chapters.

    Measured total loss and absorption of a 1" MLD mirror coating (MLD is the Oregon
    coating company founded by one of the co-inventors of the ion beam sputtered
    coating process.) The mirror appears to be in the supermirror category, with
    total loss (transmission+scatter+absorption) ~30 ppm, and with absorption ~1
    ppm (comparable to the absorption of an REO mirror coating). At
    present, MLD has no facilities for coating of LIGO size large optics, but they
    have expressed interest in the LIGO program and have asked for a copy of our
    coating specifications.
     

    From: Virginio Sannibale <vsanni@ligo.caltech.edu>
    Caltech SAS Seismic Group Short Report.

    Akiteru

     TAMA-IP transverse mode tuned at ~ 67mHz.
     TAMA- IP Counter weight tunning: Coupling with the yaw mode fixed by
     using 2 accelerometers. Model to fit experimental data improved by
     considering an effective counter weight arm.

    Brett and Virginio

      Still working on the software to control the VME board to drive the stepping
      motor.

    Lisa

      finishing the cabling of the LVDT and testing the last 3 LVDT drivers.
      First run of the 3 reference LVDT placed into the oven seems not to correlate
      quite well with the temperature fluctuation. A better data analisys is
      needed

    James and Akiteru

      Transfer function measurement of the MGASF with different working point under
      progress.

    Giovanni Lo Surdo

      Remounting and re-wiring the IP sensors and actuators.

    Soy and Francesco Fidecaro

      Working on a Labview program to trigger the creak/creep noise of a
      loaded triangular blade.

    Chenyang

      improved the Q factor for the LC actuator circuit.

    Virginio

      Supervising the work of the LIGO-SAS surf students.
      Working on fixing a bug on the DSP control program.

    Hareem

      Finishing the characterization of the MSGAF and GASF working point
      and Q factor of the vertical mode.

    Susha Giancarlo Virginio

      Found a better agreement on the simulation of the MGASF and the
      experimental data for the blade working point. Fit of the blade shape
      under progress.
     
     [1] From Peter King:3.1 LIGO II PSL        Quotations for various PSL-related components continue totricklein.  Currently the second draft of the PSL WBS Dictionary is beingworkedon, after some guidance from the meeting held on Monday.
     > LIGO II coatings> During a teleconference, REO reaffirmed their intention to be involved with> the LIGO project.> They mentioned the possibility of getting a dedicated chamber and staff to> support LIGO II coatings; previous commitment ($$) from CALTECH is expected.>> Also, JM Mackowski, from the Virgo coating laboratory, visited Caltech.> He also expressed interest in making  LIGO II coatings.> He had a very impressive presentation about their capabilities. They have a> very complete characterization facility, a coating chamber capable to fit> very large substrates, a very sophisticated rotation / mask system capable> of correcting the surface wavefront in a mirror.> However, they do not have cleaning or coating procedures in place yet. They> just made some single coating layers.>>> A mirror from MLD was tested, see Jordan's report. Maybe they can become a> good supplier for coatings other than COC's.



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