Weekly Report for Week Ending January 18, 2001


 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  January 22, 2001 will be:

 (Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

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

Special Items:


Special Announcements:


Weekly Report Highlights

Another LHO commissioning advance - full recycling with gain


LSC Issues (Weiss)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


WBS 1.2 LIGO Operations--Administration


LIGO Weekly Site Telecon (Lindquist)

There was a site teleconference held on Thursday, January 18, 2001.  Discussion items included the financial reports for the end of Decvember 2000; total booked costs were slightly less than $21.9 million.  However, a number of large open commitments are still being booked, and the total for the fiscal year is expected to reach $21.8 million. Costs for FY 2001 are just beginning to roll in and December was a short month.  Other items on the agenda were procurement of a standby generator for Livingston, selection of an A&E contractor for the Hanford Support Building, and preparations for the NSF Operations Review at Hanford

The next site telecon is scheduled for Thursday, January 25, 2001.  The list of current actions revised to reflect open actions assigned through January 18, 2001 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

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


DOCUMENT CONTROL CENTER (Turner, Mak)

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

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

ACCOMPLISHMENTS

From: Cleveland Mak <mak_c@ligo.caltech.edu>
Packages Faxes
In 34 27
Out 16 32

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.


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

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

Press here for ACCOUNTS PAYABLE HISTORY DATA.

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

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

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

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

Support (Wood)
 
Irene Baldon
  • Twelve (12) new trips were started and I have fourteen (14) trips pending final approval before tickets can be issued.  Most of these trips required Advance Checks to be written as well as hotel and car authorization forms to be filled out and FAXed to the appropriate locations.
  • Reconciled fifty-six (56) items on my P-Card this week.
  • Worked on and completed twenty five (25) Expense Reports.  I have twenty-eight (28) Expense Reports to work on and I'm holding three (3) reports which need a check from the traveler before processing.
  • Please use the new Expense Report form, particularly if you are using the Pcard for your travels.  If you do not have a copy of the new expense report, please let me know and I’ll resend it immediately.
  • I would like to remind all travelers that if your flight is considerably delayed or completely canceled, and Gina or I are not available to personally assist you in rearranging your itinerary or notifying the hotels and car rentals of your delay (i.e., after working hours here in California or on the weekends), you as the traveler are responsible for calling either the number listed on your Itinerary, their 800 number, or even a local number (or airport desk) for the vendor.  Please let them know that you will either be late or a "No Show" otherwise you will be charged a "No Show Fee" and you could lose your reservation completely.
Rita Torres
  • Converted to MS Word the Attachments B, C, and D for Stanford to update for the next period.  Edits to the Advanced SEI Mechanical Structure RFP for G. Stapfer.  Obtained DCC numbers for 25 drawings to accompany the RFP, listed this numbers and titles in the document.
  • Arranged eye exams, and upcoming training session.  Obtained information to prepare requisition with IFR Americas.  Arranged for telecon on Friday for LIGO 2 systems.  Took a nice walk to Sponsored Research to obtain a signature.
  • Ongoing activity: Chased information associated with Pcard purchases.  No sooner do I reconcile a group in Passport when more appear to be done; reconciled 24 this period.  Completed the updates to PO log for D. Lloyd.
Dorothy Lloyd

Image by C. Akutagawa
  • Processed the usual requisitions, invoices and receiving on-line. For more detail, see "Cost Schedule Control Systems" report by Esther Cunningham.
  • Reviewed and recorded payments processed by Esther for the week of January 8, on contract summary sheets and LIGO database.
  • Continued to work with Florence and Ruth on transferring encumbrances to new fiscal period.
  • Continue to monitor contract and blanket order funding levels and notify task managers when supplements are needed.
  • Jim continues to do data entry in the LIGO database and help out in the DCC.
Elizabeth K. Wood
  • Submitted to the NSF the final report for the Amaldi conference.
  • Continuing with preparations for the NSF Review at the end of the month.
  • Along those same lines, at some point I will begin asking the presenters for the review to get me their transparencies so I can put them in binders for the reviewers.  Just thought I’d let you know about my nagging in advance.

Advanced LIGO (Frey, Petrac)

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

Progress Period from 01.12 to 01.18

Accomplishments:

Schedule 01.19 to 01.25:

WBS 1.4.1.2   Project Controls (LIGO Construction)



Reports (Lindquist)

Annual Report:  The Annual Progress Report for the LIGO Construction effort as of the end of November 2000 has been sent to the NSF.  An electronic version should appear shortly in the DCC under LIGO-M0100003-00-P.



Change Control/Contingency (Lindquist)

The following Change Requests have been submitted:
 

CR-000018 WBS 1.1.4 Curbing for Service Roads at Livingston G. Stapfer
CR-000019 WBS 1.2 Additional Lab Equipment D. Coyne
CR-000020 WBS 1.1.4 Staging Building and Renovations to Existing Building--Livigston F. Asiri

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> Reminder: An updated list of all OPEN LIGO account numbers has been posted on the LIGO internal bulletin board. Please use these lists when you need a LIGO account number (or make yourself a printed copy for quick references). Please note that the FY00 LIGO Operation account numbers expired on November 30, 2000, and that the new account numbers can be found at:

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

A visit to the third A/E candidate for the Hanford Support Building is scheduled for Wednesday, January 24, at the contractor's facility in Glendora, CA.  A decision on the selection is scheduled before the end of the month.

The letter to the NSF requesting approval for Phase I of the LDAS procurement has been completed in its first draft.  This is being reviewed and edited.  It will be submitted when the vendors have been selected for all of the different components comprising Phase I.

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


LIGO Hanford Observatory (LHO) Operations (Raab)


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

Our valiant commissars have made a major breakthrough in extending locking times
for the full 2-km configuration to one minute! (Undoubtedly there will be more
crowing about this elsewhere in this report, so I will say no more.) On another
front, we began installation of optics for the X End into the vacuum chamber.
Alignment was proceeding as of the afternoon of 18 Jan. A number of changes
have been made to controls and there are moves afoot to improve the acoustic
isoaltion of the PSL.

Controls
--------
(D. Barker)

Upgraded CDS main server hanford1. Replaced internal disk drives and
upgraded operating system to solaris 2.7.

Recabled CDS/GC ethernet and ATM networks in the control room and mass
storage room. Updated all cable labels and brought drawings up to
date.

Reorganised Sun workstations in the control room.

Worked on web server blue, trying to get apache to serve elog to all
hosts while keeping access control to other CGIs restricted to LIGO/LSC.

Fixed DAQ fibre optics problem with the 4k Y End station. EY ADCU now
keeps in sync with other 4k units. The failure of the 4k automatic bypass
board means that the 4k system is currently running on manual bypasses
only.

Worked with Hugh to setup an EPICS test stand for the PSL tidal
correction software.

Set up the 4k PSL EPICS system on an mv162.

Tested GEO's ADCU timing cards.

Bringing all CDS Rack, DAQ and networking drawings up to date.

Autoburt new feature programmed. PVs can be marked to be backed up, but
not restored to IOC.

Put FMCS controls pc onto CDS network, allows backup of fmcs data onto
hanford1 for archiving.
 


LIGO Livingston Observatory (LLO) Operations (Coles)


Commissioning (Joe Kovalik) LSC and ASC now work both in the LVEA and end
stations. The GDS excitation engine works in the end stations. Work is going
on in diagonalizing the actuators for the large optics.
 

Both ISCT1 (symmetric) and ISCT4 (anti-symmetric) are aligned. The
photodiodes are installed and the demodulated outputs are now operational.
 

LSC (Ed Daw and Szabi Marka)We added D.C. offsets at various points in the
LSC servo block diagram to do rudimentary tests of individual servo
components. We found every control we tested was working.
We measured the transfer functions of parts of the LSC digital servo and
associated analog pre and post digital signal conditioning. See LIGO
Livingston e-log entries, 17th Jan 2001.
We measured the dynamic range of the Lm LSC servo as a function of
frequency. We observed glitches in the output of the servo when saturating
below frequency of ~100Hz. See e-log entries, 18th Jan 2001.
 

Facilities (Gerry Stapfer) The Contractor (Brunt Construction Inc.) has
started work on the renovation of the Staging Building.


Detector/Technical Support (Whitcomb, Coyne)



 

Installation& Commissioning:
Hanford
Livingston
Other Science/Engineering Activities:
Design/Analysis/Fab
Issues/Concerns
Seealso the Installationweb page

1.1 LHO INSTALLATION & COMMISSIONING

2km Commissioning

Matt Evans, Nergis Mavalavala, Bill Kells, Richard McCarthy, Dave Barker, Stan Whitcomb
We continued with our attempts to lock the 2 km ilnterferometer this week.  The eary part of the week was spent trying to understand and remove the apparent offset that had been observed in locking the sidebands to the power recycled Michelson.  We made a number of tests, did a major realignment in the corner station and were unable to significantly change the offset.  In the end, a series of FFT rune by Bill Kells convinced us that the apparent offset is a real effect from the (slightly) unstable recycling cavity, and thus it is a good thing not to be able to eliminate it.

With that under our belts we tackled locking.  We measured the lock acquisition parameters for Matt Evans code, getting similar numbers to what we had gotten in the past.  The rf phase for the reflected port ended up about 7 degrees different (and in my opinion, better), but most other numbers did not seem to be changed by much.

The interferometer locked robustly in all of the subconfigurations (including a new one: one arm and a half-Michelson).  The we tried the full interferometer.  Initially the results were similar to what had been achieved in the past: buildups in the arms indicative of "recycling gains of 7-10, but durations typically 0.1 second.  One striking feature of these brief locks was the similarity of the signals from attempt to attempt; one frequently had to really examine traces in detail to see that two printouts of the timetraces were from different events.  This lead us to believe that the action was dominated by what we were doing to the optics via the servos and not by random forces or initial conditions.

At that point we turned off the angular suspension damping from the OSEMs; it had been turned way down when the optical lever damping was implemented, but typically left on at a low level for those occasional times when the optlev goes out of range (typically during the alignment process).  Lock duration immediately leaped to 0.3 seconds. After a good night's rest, the interferometer was ready to go for 2.5 seconds and encouraged by the occasional passerby, these locked stretches gradually extended to more than one minute.  Slight improvements to the alignment have brought the recycling factor up to about 15.  We had to reduce power on a couple of photodiodes to eliminate saturation.

The figure below shows key images from four locations in the interferometer: on top the two transmitted beams through the two arms, below, the "dark port" and a pickoff inside the recycling cavity.  These are more or less the same ones as in background of the first lock photo of Rai on the webpage, but note that the saturated nature of the images indicates the increase in power in the interferometer (of order 500 for the transmitted beams).

First Lock image
 

Core Optics

Doug Cook, Mark Lubinski, Hugh Radkins, Betsy Weaver, Rick Graff, John Worden, Kyle Ryan, Gerardo Moreno
Installation of the 4 km ETMX started.  The vacuum volume was vented. The door and spool piece were removed.  The tooling was installed and the alignment equipment inserted into the chamber.  The ETM telescope was installed and rough aligned. The assembly of the arm cavity baffle was started.  The ETM has been installed and aligned.  So far it looks like we have a pretty good chance to finish this week, but may not get the end station pumped down until the beginning of next week.

COS

Mike Smith, Ken Mailand , Doug Cook, Dennis Coyne
The ETMx telescope was installed and aligned roughly in preparation for final alignment with the COS autocollimator.
The arm cavity baffle is in process of being assembled.
 

IOO

Jay Heefner
Drawings and cross connect lists for the "new" mode cleaner length controls are complete. R. McCarthy is building the cross connects for both the 2K and 4K. We still need to change the database and the operator screens prior to running the system.
 
 
 

1.2LLO INSTALLATION & COMMISSIONING

Commissioning

Rai Weiss, Mike Zucker and everyoneat LLO
The short term goal of the commissioning at Livingston is to individually lock the 4 km arm cavities. In order to achieve this, the commissioning effort in the past two weeks has concentrated: Visitors to the site have been Rolf Bork, Jay Heefner, Rich Abbott and David Shoemaker.
 

ISC

Rich Abbott
Helped with the troubleshooting of the ETMY LOS suspension controller that had two coil driver channels inoperative.

Performed functional checks of all I&Q demodulator boards due to poor detection linearity.  Problem was found to be an improperly set LO drive level.  Fixed the problem and now all channels have I relative to Q phase of 90 +/- 0.5 degrees, and I relative to Q magnitude balance of better than 0.5 %

Changed all elements of the frequency distribution system to incorporate the RF decoupling capacitors.  This should improve RF leakage from the cabling.  A measurement is to be performed today to check the field strength against the numbers obtained by Rai.

Rolf Bork
Finished up at LLO Friday.  The intermittent problem withthe ASC/LSC front ends turned out to be a bad Pentium CPU in the ASC crate.  This was the problem that I had been looking for since the first installationand appeared to be a problem with the X end station, as system would crashdue to non-numeric data (0xffff everywhere) randomly showing up in the Xend reflected memory. This would cause one or more of the three CPUs on thisnet to crash.  Finally found the problem Thursday night while monitoringall three CPU on my laptop from the hotel.  With no software running, suddenly0xffff ate thru the memory of the ASC processor reflected memory board.  Replaced that CPU on Friday, and problem has not reappeared.
 

Jay Heefner
A new set of schematics showing the LSC wiring and cross connects has been generated. The previous version had many mistakes, was hard to follow and did not incorporate changes needed for lock acquisition. Once the drawings are checked the new version will be released.

All modules, wiring and software for the ASC and LSC systems are installed and operational. This does not include any additions that may come from the lock acquisition studies at LHO.
 

2.0 OtherEngineering and Scientific Activities

2.1 Design/Analysis/Fab

Optical Metrology

Helena Armandula, GariLynn Billingsley
Given the marked temperature fluctuations testing of 2ITM03 is "on hold"
 

Optics Modelling

EriKa d'Ambrosio
Testing how stable is a cavity supporting a flattopped beam as an eigenstate
I created the maps for the hypothetical mirrors by making thebeam propagate and catching the constant phase surfaces as border conditionsfor reflection. Those were put inside the FFT-code and after relaxation isreached the field grid of the resonating beam was picked up for post-checkthat the eigenmode is the one we want. Comparisons were made by using "perfectspherical mirrors" and the curve of power gain versus tilt for the "reshapedmirrors" decreases with a slope that is ~thirty times larger.
 

PSL

Peter King
Ben, PR and I have been testing out the newly fabricated frequency stabilization servo, 80 MHz VCO and 21.5 MHz RF photodiode down in the PSL Lab.  Both the VCO and the photodiode passed without modification.  After the addition of an external capacitor, the frequency servo functioned as usual.

A prototype board for the high power photodiode was fabricated and stuffed.  After some bemusement about the circuit's behavior, the cutting of a few traces ... the photodiode was placed in the laser beam.  The output of the photodiode was consistent with there being about 115 mA of photocurrent. Unfortunately the photodiode bandwidth was not as high as hoped for.  The measured bandwidth was only 70 kHz, compared to the hoped for 70 MHz. Measurements of the feedback resistor and capacitor confirmed that they were the proper values, so I don't quite understand where all the bandwidth went.

Lee Cardenas
Work on the Laser. Complete re-alignment and Beam scan for both lasers, the npro as well as the amplifier is on going.  Since we are replacing the mount for the EOM with a goniometer.

Preparing an station to mount the reference cavity so we can be able to do optical contacting on the new reference cavities.

General lab task ( placing orders, paper work, drawings etc...)

Rick Karwoski, Paul Russell, Ben Abbott
All four boards composing the Frequency stabilization sub-system have been bench tested, system-tested at Lauritsen, and shipped to Hanford for installation.
Modulated OSEM DesignJay Heefne r
Five stabilized oscillator satellite amps are operational and in final test. The boxes for the boards are late from the vendor. We can ship the boards and test them with no boxes if the LHO commissioning team needs them. Richard McCarthy is checking with Stan.
 
 

New OSEM Heads

Peter Fritschel, Myron McInnis, Fred Miller
We're continuing production of new osems for the LHO 4k installation. We have had more problems of poor bonding of the device boards to the cylindrical forms. We have thus moved to a different ceramabond adhesive. This one is based on alumina (rather than magnesium oxide) which is a better match to the alumina parts; it is also much easier to work with as it is less viscous than the previous adhesive. Early results indicate that it is giving better bonds. We expect to finish all LHO 4k osems in a couple of days.

Janeen Romie
Helena and I cleaned the 120 acid etched heads from Orbit Technology. Rapid Prototyping will receive them tomorrow morning for metallization. The assembly specification is being updated.

Digital Suspensions

Rolf Bork
This week, returned to code development for the digital suspension system.  Some early testing indicates we might be able to run all suspensions with two CPU in the LVEA, one performing all servo calcs and SOS coil drives and the other performing final LOS calculations (add in ASC/LSC inputs) and LOS coil drives. I'm in the process of adding in the sensor input / coil output filters now (for a total of up to 39 user definable digital filters per suspension) and hope to get performance numbers by Friday.  We need this info to complete the system layout and begin the system wiring diagrams.

Jay Heefner

GDS

Daniel Sigg
Started with the new client interface for the DTT which should be able to read frame files and which can get data directly from the archive with the help of the data flow manager.

Helped tracking down two problems with mini-nds and the rds writer. The reduced data set writer can now be started and stopped from the control room. It has an internal buffer to store frames for several seconds. This made it possible to implement a snap shot feature which saves frame files to disk around the time someone presses the rds snapshot button. For example, if the operator sees an interesting feature with the data viewer, the event can be saved to fortress by taking a snap shot.

DMT

John Zweizig
This week I am attending the GEO data analysis conference. They aregetting all sorts of good(?) advice on how to run their experiment.

Data Acquisition

Sander Liu
SoCal ValueAdded delivered the first 16 channel data cable they built for us for testing. Continuity check was ok and it looks good. They were authorized to proceed building the rest of the cables for us per our purchase order.

In the process of testing a +/- 5V, 25 Amp power supply for the 40 meter.

2.2 IssuesConcerns

nothing new

40 Meter Interferometer (Weinstein)



 
  • Mike Smith continues to add detail to the optical layout of the 40m IFO. Six of the 9 output beams now go to tables to the south of the PSL table, close to 7 electronics racks. Jay Heefner, Mike, Ben, and Steve have gone over the layout of the tables and electronics racks, and think there's (barely) enough room for the required equipment. Some rework of our brand new electrical wiring may be required. The integrated layout of the 40 meter interferometer, which combines the building layout, electrical layout, and opto-mechanical layout, is being revised to incorporate the planned locations of the electronic racks, and the as-build configuration of the cable trays.
  • PSL, from Peter King: following last week's report stating that the vibration isolation stacks arrived, some parts were discovered to be missing. Nor-Cal have been contacted and the parts should arrive sometime in the next two weeks. Somehow fabrication of the parts was overlooked.
  • PSL, from Rick Karwoski: Plan to begin moving pieces of the 40m PSL to the 40m lab in February is still on track.
  • Ben Abbott will update his plan for the control room layout, including furniture, computer locations, PSL cooling location, etc, and will begin the process of ordering the furniture.
  • Larry Jones reports a series of mishaps where parts for the 40m mode cleaner vacuum chamber were not ordered when they were supposed to be, things weren't shipped to LLO for cleaning when they were supposed to, other parts are on back order, etc. Nonetheless, we can still hope to begin assembly of the mode cleaner vacuum enveloped in February.
  • As you can tell from the above, February and March will be a very busy time at the lab: installation of the output optic chamber and it's new seismic isolation stacks; installation of the 12 meter mode cleaner; begin installation of the PSL; installation of 9 electronics racks and the beginnings of populating them with VME crates, DAQ electronics, etc; setting up of the control room (furniture, computers, networking); regeneration and re-installation of the ion pumps; commissioning of the new vacuum control system; finish up items on the building rehab punch list; etc. Wow! A very preliminary but detailed schedule is here.
  • AJW met very briefly with Tom Frey to go over the Primevera-based WBS for the 40m program. Unfortunately, AJW is battling the flu, but promises to give Tom detailed comments when he returns to sentience.
  • Similarly, AJW was too zonked to prepare for or attend the dry run for the NSF review on Friday, but promises transparencies ASAP.


  • Thermal Noise Interferometer (Libbrecht)


    We are currently in the process of characterizing and experimenting with
    our successfully locked test cavity, and we are debugging and repairing the
    fast inputs on two of our OSEM controllers. Shanti is also working on
    materials for his candidacy exam next week.
     


    LASTI (Zucker)


    no report


    Data Analysis and Computing (Lazzarini)



     
     

    Simulation and Modeling (Yamamoto)


    * physics analysis :

    Biplab kept working on the systematic study of the effect
    of angular fluctuation on the lock acquisition process.

    Lock acquisition with misalignments: studying tolerance
    of various stages of the lock-acquisition procedure towards
    levels of angular fluctuations in mirrors.
    Studying power fluctuations at desired states of various stages.

    Although it may sound obvious, it has been observed from
    simulation runs that the statistical quantity
    "average lock-acquisition time" increases with the level
    of angular fluctuations.

    Hiro worked in the noise modeling. In order to simplify
    the PSD analysis, primitives calculating psd and some
    low pass filters will be provided.

    * LIGO II mechanics modeling

    Virginio has reassembled and completed the first version of the
    quad suspension model for LIGO II, based on the work done by
    Akiteru and himself using MSE by G.Cella. The top blade is not
    implemented yet, and he will discuss with Peter Fritschel and
    Giancarlo Cella to find out the most effective way of implementing
    the blade. Hiro is working to complete the interface between MSE
    and e2e.

    * parallelization effort

    Having the thread-safe queue and a looping algorithm completed,
    Tavio and Hiro designed the testbed which has an interface identical
    to the real simulation program as to the module arrangement and
    execution. Future effort will be concentrated to the algorithm
    development to arrange the module execution using optimal number
    of thread in this testbed.

    Tavio and Hiro tried semaphore synch mechanism under the assumption
    that it's being simple and  (probably) having a kernel implementation
    would make it faster that mutexes &  cond variables.  Unfortunately,
    same long delay (~50 micro seconds) was observed as was the case
    using mutextes & cond variables.

    * alfi / GUI :

    A new released has been installed at CIT and LHO, and a tarball is
    made available from the webpage. Copy&Paste and new setting front
    end is coming.

    In order to simplify using remote computers (like CACR) as computation
    engine, a program will be written to merge all box files keeping only
    minimal information in it.

    LIGO Data Analysis System

  • Software Systems (Blackburn)

  •  

     
     
     

    LDAS released version 0.0.13 late on Friday of last week. The release was
    tagged in the CVS repository, extracted and a distribution built and added
    to the LDAS webpage. It was also re-built and compiled from the distribution
    over the weekend in preparation for the begin of the MPI Mock Data Challenge.

    The remainder of the week has been dominated with activities in support of
    the MPI MDC. Several of the staff worked on the MPI MDC Plan documentation
    and prepared TCL test scripts to exercise each aspect of required functionality
    being evaluated during the MDC. So far we have tested the mpiAPI, wrapperAPI,
    LAL, LALwrapper, and mpi-wrapper interface. Testing of the details of the
    individual search libraries is actively underway. It looks like there is a
    very good chance that the week will end with a very successful completion of
    this MDC.

    Other areas that have been worked on this week include closing out a large
    number of lingering open problem reports. The documentation has also been
    greatly improved in areas of the frameAPI, controlMonitorAPI and the
    dataConditionAPI.

    Very good progress is being made towards recasting the dataConditionAPI
    classes to use the new UDT with significant support from UTB, PSU, and ANU.
    The completion of data ingestion has been given a very high priority this
    week in hopes that we might be able to do a couple of tests during the MDC
    of the mpiAPI, wrapperAPI "and the dataConditionAPI" before everyone packs
    up and heads back to their home institutions.

  • Hardware Systems (Anderson)

  •  

     
     
     

            Work in support of the LDAS MPI MDC, including the installation
    of a 16 processor Beowulf cluster in the ldas-test system (AltaCluster).

            Continuing negotiations with several vendors in preparation for the
    major LDAS Phase I purchase.

  • Data Analysis Activities

  •  

    General Computing (Wallace)

    MIT:
    Nothing to report.

    Livingston:
    -Working on a number of system maintenance items. Discussed reconfiguring the
    Big Brother program to accommodate a few other tasks.
    -Larry has sent another message to Bellsouth to try and get the information that
    they promised to deliver by the first of the year.

    Hanford:
    -Getting elog mirrored to the Observatories main web server.
    -Larry is working on the procurement for the FORE cards to connect the
    Observatory with PNL using an ATM link.
    This is part of the project to get the OC3 connection going at the Observatory.

    CIT:
    (Larry)
    -Working on getting things started with the DCC in preparation for the upcoming
    LSC meeting. Mainly working on equipment and software purchases they will be
    needing.
    -Cleaned out a number of defunct aliases on the e-mail server.
    -A number of hours spent with procurement related issues. Includes resolving
    problems with existing procurements as well as placing more orders.
    -Working on a number of LDAS related issues.
    -Just as a note to remind everyone to be careful on any programs they download
    or install on their computers. Be sure they are virus free. Please, download
    only what is necessary and if you find it is a junk program be sure to remove
    it.

    (Lisa)
    - Created users in the new modem pool.  I am only a day or two away from
    switching to the new pool.  I still need to get a free block of IP numbers on
    the 125 subnet and chase down a couple of more people who need accounts created.
    - Updated an ultra1 on the 6th floor of Milliken to solaris 8
    - Rebuilt Paul Russell's pc with a new hard disk.
    - Swapped in a new ultra 10 for Hongyu in Wilson House.
    - Have been dealing with lots of little laptop issues that have cropped up as a
    byproduct of the modem pool upgrade.

    (Barbara)
    - Completed and installed changes to CostBook system for equipment line
    items, contingency override, and subcontract overhead calculations.
    - Updated LDAS database links and the green-map images.
    - Tried several possibilities for a DCC report for David Shoemaker.
    - Worked with Lisa on executing jobs when TimeTarget is installed as a
    service.
    - Attended roster meeting with Liz and Gary.
    - Made a number of web site changes to Publications and Talks pages.

    (Suresh)
    -Resolved the network connection in one of the cubicles in third floor west
    bridge.
    -Fixed Erika's mailserver connection problem from her workstation. Helped Paul
    Russel with some applications.
    -Worked on some printer maintenance.
    -Working on new PC set up for Ken Mainland.

    (Sam)
    -Talked with Phil about his computer difficulties.
    -Did some ip stuff
    -Answered a few random questions
     


    LIGO II/Advanced R&D (Sanders)


    From Peter King:
     

    LIGO II PSL
    I am still working on a new costing for the PSL. Mostly incorporating
    updates for the cost of fabrication of the 200-W laser.

    From: Peter Fritschel <pf@ligo.mit.edu>

    Completed the design requirements document for the seismic isolation
    system, and sent it out to the committee which will be reviewing it next
    week (Wednesday, 24 Jan).

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

    Silicate bonding
    We may have an answer for the "ferns" seen in most of the bonds.
    There is a well studied model for pattern formation, "diffusion-limited aggregation", that explains this phenomena.
    The "fern" patterns, called "fjords" in the literature, form when colloidal particles undergoing Brownian motion adhere on contact with one another.
    If the density of the particles is quite low, the aggregation process occurs one particle at the time, and explains why we do not see these formations right away but maybe hours after the bonding took place.
    In our case, we observed that the cleaner the substrate is before bonding, the more faint is the pattern seen.
    Now, the bonding solution, which is a mild etchant, may dislodge some loosely attached fused silica particles coming from the top "superpolished" layer of the substrate. This may explain the changing bonding behavior on different substrates.
    Surface tension also plays an important role in this pattern formation.

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

    Fred is sick, will be out for several weeks.  Best wishes from
    everybody.

    Digital Electronics (IDED)
    Digital cards coming along
    DME crates available
    NIM crates still late

    Alessandro
    Accelerometers I n construction, 6 for the 2 IP, 2 for Szabi and 2
    spares.
    Coils shipped
    Linear electronics waiting for NIM boxes

    Virginio, Akiteru
    Testing Alessandro’s new accelerometers on old IP (3 for controls and 1
    for monitor).
    Testing introducing asymmetry with parasitic springs.

    Kenji, Akiteru
    Counterweight validation started on 3 meter units.

    Galli&Morelli
    The weak IP joints remade within 8 hours, they are cooking since Friday
    together with the filters new blades. End of cooking and shipping on
    Wednesday the 17th.
    Hexawire half shells shipped.

    Kenji.
    Tuning F0, bystable with original blades, stabilized by shortening
    blades and adding tuning parasitic springs.

    Edwin
    measuring mini-GASF blades to select them and install in top mass of
    multiple pendulum.

    Virginio
    GASF paper approved by Dennis with few comments, send out next week.

    Ric
    Preparing shipping crates.


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