Weekly Report for Week Ending March 2, 2000



 Exec. Committee Meeting 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  March 6, 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:    This is the first weekly report to cover activities broader than the LIGO I construction. The format and content will evolve over the next several weeks.


Weekly Report Highlights
 


LSC Issues (Weiss)


No report this week.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



LIGO Operations--Administration

LIGO Weekly Site Telecon (Jasnow)

There was a site telecon held on Thursday, March 2, 2000.   The list of current actions revised to reflect actions assigned during this meeting may be found at ACTION LIST.

LIGO II Proposal--It was noted that we will have a meeting Monday, March 6, 2000 to establish a proposal preparation schedule for LIGO II.  A proposal for continuing operations for FY 2002 through FY 2007 will have to be done in parallel with the LIGO II proposal.  The proposal for continuing operations should carefully address site needs.  Ed Jasnow suggested that Mark Coles, Gerry Stapfer, David Shoemaker, Otto Matherny, and Fred Raab be heavily involved in this proposal.  Mark Coles expressed an interest in being included in the meeting Monday afternoon.

Property Management--We have a long-open action regarding the proper identification of Caltech/Government Property which derives from an action assigned by Caltech Internal Audit almost a year ago.  The current status of the action is "waiting for Finance" to provide guidance and information.  Phil was assigned an action to prepare a memo for the new Controller, Al Horvath, summarizing the history and requesting some priority.

Funding--NSF previously instructed us to submit the Annual Report via FastLane and the Annual Work Plan via paper since the NSF system apparently does not provide a "place" for both.  We have submitted a Work Plan via paper requesting funds for FY 2000.  We are in the process of preparing the Annual Report in the FastLane format.  However, the NSF is apparently having second thoughts.  I think this means that the Annual Report will be via paper copy and the Annual Work Plan through FastLane.  I have asked Elizabeth Wood to start assembling a FastLane version of the Work Plan, and I am providing her with the necessary electronic files.  This may take a week or so.  Meanwhile, I would guess that we are going to have payments problems.  There are adequate funds in LIGO Contingency (this year!--as mentioned previously, this may not be true next  year), but Finance will be required to do much churning to put the funds in the work breakdown structure elements (accounts) incurring the costs!  This is necessary for ORACLE to be able to request funds from NSF.


PROPERTY MANAGEMENT (Chargois)

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

Assisted the System Administrator (L.Wallace) with the packing and shipping of a Computer and two Monitors to the LIGO Livingston Observatory (T.Evans).  Account Number LIGO.5N500 2.13 NSFLIGO.5N5000.

Assisted the Seimic Isolation R&D Group (R. DeSalvo) with the preparation of a Physical Plant Project Request Form for shipping of Hardware to the LIGO Hanford Observatory. Account Number LIGO.00002 3 NSFLIGO.5044800.


DOCUMENT CONTROL CENTER (Turner, Mak)

[We encountered the Y2k Leap Year Bug in the Document Control Center this week.  People who attempted to use the DCC Web page to get a document number Tuesday morning discovered that the default date provided on the Web page (02/29/00) would elicit a message indicating that the date couldn't get through the error checking routines.  Barbara K. provided a work around and a fix by lunch time.  We think that it was just a minor inconvenience.  --pel]

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. . .

ACTIVITY HIGHLIGHTS

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

Good news!  Learned how to "export data" from Oracle to an Excel spreadsheet to be able to print out the data on one spreadsheet versus multiple Oracle screen prints.  This data was requested on NYMA.  Kimmie Richardson provided the assistance on this.

We are still waiting to find out how to best obtain a list or report of "active encumbrances" on an open P.O.  Oracle support staff is working on this with Acquisitions management.

Acquistions has obtained folders to better organize the subcontracts internally and these were distributed a few days ago.  A folder was set up
for Lightwave Electronics which went to the Controller for signature.  Today, MIT C/O 6 and 7 were signed by the Controller.  The set up of the new folders is a little time-consuming, however, it pays later as it is easier to see the status of the subcontract at any given point in time.  I am working on finishing up the folder for MMR to take over for Acq's approval, and will also be creating a folder on Galli and Morelli to take over for the controller's signature today.  (The c/o's are done in the system, so payments have been going out.)  The folders will be prepared as change orders are submitted.

I checked with Tina yesterday about releasing encumbrances on subcontracts and she said it is okay to do this as an internal modification. I'll be trying this out today. [We have been trying to relieve old encumbrances.  If we strictly adhered to the rules, we would have to issue change orders to the subcontractors notifying them of a reduction in their contract value to reflect the elimination of the open encumbrances.  Some of these subcontracts are closed.  Some of the encumbrances relate to accounting processes that failed to relieve them when payments were made in the past.  Therefore, it makes no sense to issue a change order to the subcontractor.  I think that what Ruth is telling us is that they have decided on a process that allows us to make the necessary corrections without burdening the subcontractors (or the subcontract managers) with strange and unnecessary paperwork. --pel]

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

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

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

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

A contract is being issued directly to US West to provide telephone service to Hanford.  This is in lieu of this service being provided by DOE through their operations & maintenance contractor.  This contract will allow Hanford to pay their monthly telephone bills using the P-card.

On April 18, the Hanford observatory will be visited by representatives of the Washington State Department of Revenue to determine whether LIGO is subject to paying their B & O tax.



Support (Wood)

Rita Torres

For I. Petrac formatted, from Oregon's email, the 6-month LSC report for University of Oregon; submitted electronically for DCC posting after review. Distributed letter Re: University of FL invoice error. Obtained an Oracle requisition number, then distributed signed PO with Crystal Systems. Did change order No. 2 to Dynamic Light, and change order No. 8 to MIT, obtained Oracle requisition numbers for both. Helped to close contracts with SORL, and Conejo Industries.

I'm near closure on a credit that I've been chasing for over two weeks. MWS Wire Industries does not issue credit on credit card purchases, instead they issue a check for the amount, and that check was mailed to the wrong mail stop on campus. The company finally agreed to stop payment on that check and issue another to Caltech at M/S 18-34. Hope to close this next week.

Dorothy Lloyd

Continue to process receiving, requisitions, and invoices on-line. For more detail see "Cost Schedule Control Systems" report by Esther Cunningham.

Monitoring contract and blanket order funding levels continues, and requests for supplements from task managers when needed.

Reviewed payments processed by Esther for the period Jan 17 through Feb 29. Payments were entered on contract summary sheets by myself, while Jim entered the payments made on standard purchase orders in the LIGO database.

Managed to start filing away POs processed (since the switch-over last July to Oracle) in PO Log books using the new POETAs.

Graph provided by Cindy A.

Irene Baldon

Attended a meeting on the possibility of LIGO becoming the prototype for using P-Cards for travel. I will be attending 2 days of passport/travel demonstrations on the 13th and 14th. I will keep you informed as I soon as I know anything.

Worked on preparing the paper work for 15 new trips taken recently or upcoming (15 Payment Requests and 11 Advance Requests). In addition, there are approximately 15 new trips in preparation.

Completed 17 Expense Reports. There are 41 Expense Reports still to be done. I'm holding 1 completed Expense Report which requires a check from the Traveler before sending to Travel Audit to clear.

I'm seeing some improvement in the time lag for receiving checks from Disbursement Audit. Disbursement Audit has been moved to an address on South Hill thus making it very difficult to walk over to pickup a check that I'm particularly looking for. I now seem to be receiving TR numbers on somewhat of a regular basis.

Elizabeth K. Wood

Livingston is making offers and hiring people. Gary Traylor started March 1. Another offer will be going out soon with a possible third hire in the very near future.


LIGO II (Lindquist)

We have scheduled a meeting next Monday afternoon to prepare a schedule for preparation of the LIGO II Proposal.  The Continuing Operations (FY 2002-2007) must be prepared in parallel.
 



Project Controls (LIGO Construction)


Reports (Lindquist)

Change Control/Contingency (Lindquist)

The following change requests have been submitted:
 

CR-990028 WBS 1.1.3 Beam Tube Enclosure Closeout F. Asiri
CR-000001 WBS 1.1.4 Fencing Road at Livingston (Info Only) G. Stapfer
CR-000002 WBS 1.4 Project Office Close Out K. Duncan

Press for the latest Contingency Needs Projection.


COST SCHEDULE CONTROL SYSTEMS (Duncan, Akutagawa, Kaufman)

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

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



LIGO Hanford Observatory (LHO) Operations (Raab)


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

Thanks to the good work by team PSL, we now have a temperature stabilized
reference cavity. Earlier measurements indicated that the observed 2K arm
length drifts were much larger than the expected earth tide and stabilizing
the reference cavity temperature has increased lock times by roughly a factor
of two. We now regularly observe lock times of order 1 hour. We compared
drifts observed in Monday night's data run to the earth tide. It is hard
to make a lot of such a short data set. The predicted tide was within a
few microns per hour of the observed drift, but the prediction is
systematically smaller and shows a sign reversal not present in the
observed drift.

Mike Landry and David Ottoway have completed a compendium of mechanical
resonances in the current LHO 2k hardware. It is document number
LIGO-T000020-00-W. The 23-page document lists resonances by hardware
element in the body of the document and includes an appendix with
resonances listed by frequency. This provides a "fingerprint file" that
will be useful for identifying features in power spectra.

This week the focus is on implementing autoalignment on the 2K arm.

Bake Oven:
----------
(K. Ryan)

LHO vacuum bake oven load #79, consisting of two ETM telescope assemblies,
was released earlier this week.  This load did not include the pieces of
LLO and LHO 4k pick off mirror assemblies as was reported last week.

I discovered this week that we have not been abiding by the "3%" dilution
that is specified in LIGO-E960022 but rather have been using a much higher
concentration of PROTEX. Considering that the only LHO load to have
"failed" an RGA scan was one in which PROTEX had been utilized, I decided
to separate the mirror assembly parts from the telescope parts and bake
them as independent loads.  Hopefully, the "PROTEXed" parts will have a
normal scan, but if there is a link I wanted to use the mirror parts,
which are representative of a typical PROTEX load, to help establish this.
We will be observing the 3% dilution in the future, regardless.
 
Load #80, consisting of LLO and LHO 4k pick off mirror assemblies, is
vacuum baking and should be released by 3.6.00.

Computing:
----------
(C. Patton)

Spent most of this week helping my new helper Oudone Voraphaychith, a
WSU EE student, get settled in to his new job.  Oudone will be helping
to upgrade all the site PCs to Windows98 as well as helping with user
problems and any misc. jobs that come up.

So far Oudone has upgraded two PCs to Win98 and moved one of the
upgraded PCs out to the MidX station.  The other is having some
additional software installed on it so that it can become the Guest
computer in the Common area of the Offices.

I have also followed up on a PO for the Exceed license upgrades,
followed up on getting Norton Antivirus software from the Caltech site
license.  Continued network security maintenance, did the weekly
backups, helped setup a new Unix workstation for Michael Landry, helped
users with several printer and PC problems and kept the GC accounting
paper work up to date.

Controls:
---------

CDS
D.Barker

Built ADCU test stand in MSR for testing next release of ADCU code.

Updated dust monitor screens to include new monitors, and allow dynamic
alarm level changing.

Reconfigured control room alarms, new PSL alarms added. DAQ alarms
removed while DAQS configuration manager has socket problems.

Supported CDS installation at LLO. Built the LLO jdclient machine as
dual ported apache web server (control2/nashville). A. Ivanov installed
latest jdclient on this.

Replaced all Hanford ADCU timing cards with the latest version. This
allows all ADCUs to record the GDS ramp and 1PPS signals. The cards
which were released by this will be used for ASC in MY, and Excitation
engines in LVEA and MX.

Reorganizing LHO source code for inclusion into the LDAS CVS
configuration management system.

Reviewing all Hanford EPICS systems, will release all systems currently
running in test or dev mode.

Performed routine daily tasks; add channels to DAQ, add channels to
Backup, check daily backups, add new accounts, add new MEDM screens to
site overview, fix sofware problems/hang ups in control room,  release
EPICS code for software development, etc.
 

Vacuum Controls
C. Patton

Modified the annulus ion pump summary on the site overview medm screen
so that the pumps in each building are grouped and labeled for that
building.

Modified the Gate Valve detail medm screens so that the gate valve open
and close buttons now call a Tk/TCL program which brings up a
confirmation window.  This way it requires a two step process to open or
close a gate valve.

Started changes to the cold cathode on/off buttons to call the Tk/TCL
confirmation program.
--


LIGO Livingston Observatory (LLO) Operations (Coles)



 

This is the first LLO weekly report written in the spirit of Gary's new guidelines. This initial report is consequentally very brief because normal discussions of routine installation progress have not been included, however items of project wide interest are listed below. I expect the amount of information will grow in the upcoming weeks as we learn how to utilize the new format to communicate information of project wide interest and to air issues and concerns which would benefit from discussion in this forum. - Mark Coles

Installation work: The Faraday isolator was re-aligned in the optics lab using the 700 mW NPRO YAG laser. This time, we measured the double pass isolation ratio (the isolation for the returning beam) by reflecting the forward going beam by a reflector. When the second (downstream) halfwave plate was optimized, the
isolation ratio and transmission for the returning beam were 37.4 dB and 88%, respectively. Because the total Faraday rotation angle depends on the laser power (due to the temperature dependence of the Verdet constant), it will be necessary to adjust the orientation of the second halfwave plate on the optical table in the vacuum chamber at nominal PSL power.

The ETM-x telescope and transmission monitor have been successfully installed and aligned. ETM-x mirror installation and alignment continues.

PSL: We are still struggling to understand and correct the sever power throughput defecit of the new pre mode cleaner. As of 7:30 Thursday evening, an inexplicable loss of 50% within the mode cleaner is observed. Investigation continues.

Beam tube bakeout: The beam tube temperature has returned to ambient on Y1. RGA data are being collected as this report is being written and will be reviewed by Rai Weiss and Allen Sibley.

GDS: The LVEA GDS Excitation Engine is now accesible over the net (gdslvea1). It is now being configured.

CAS training: Coarse actuator training was conducted Monday-Thursday at LLO. Mark Guenther and Hugh Radkins attended from LHO along with Rich Riesen and Joe Kovalik from LLO. It was agreed that Mark will be the software librarian for the CAS control software.

LIGO-TriNet Station: (Caltech remote seismic monitoring station at the LLO site). Preliminary site surveying is underway. One area of possible interest is the small triangular parcel of property along the south arm on the opposite side of the borrow pit. This has been measured using a seismometer on battery power and observed to have somewhat smaller levels of seismic noise as it is furthest away from structures, roads, and general site activity. Data was also collected from 11 other candidate spots.
 


MIT (Shoemaker)


All activities for this week are covered in other categories.


Caltech (Sanders)


No report this week.


Detector/Technical Support (Whitcomb, Coyne)


 

Installation:
Hanford
Livingston
Commisioning:
Hanford
Livingston
Other Science/Engineering
Activities
 

1.0 Installation (including fabrication and subsystem test)

1.1 LHO

Since the previous reporting period, the temperature stabilization hardware for the 2k IFO PSL has been installed and the PID controller that regulates the temperature of the reference cavity has been programmed with an initial set of parameters. The parameters entered represents a "best guess" at the desired values and may require future tweaking. An offset to the PID controller settings is available under EPICS and is a setting that should not be toyed with lightly, due to the long temperature ringdown of the reference cavity. Presently this input is limited to a maximum of ~1 degree C. The hardware installed was the hardware that was used to obtain initial information about the tidal actuator. The final version of the hardware is scheduled to be installed in April.
The new VCO has been installed. The difference between the new one and the previous one is the addition of a 1.6 Hz pole and a 40 Hzzero in the input to the 800 MHz VCO. The measured phase noise of the newVCO is ~6mHz per Sqrt[Hz].
Installation was completed on the transmission monitoring pier at X end station.We're having difficulty with stainless bolts galling on the SEI Fine Stage unit assemblies, even after chasing the threads. We'll be resorting to careful use of Krytox lubricant in these sensitive areas, as well as leaving one bolt uninstalled in a joint with eight bolts, two places, and the use of one or two flexures from the prototype fine stage assemblies.
SEI Fine Stages and air bearings have been installed at WBSC 10 (Y end).
An inspection was made of the ribbon cables inside WBSC 6 (Y mid) as part of the incursion for baffle replacement and ETMy realignment. Two areas of cable touching were noted: between the support table and the bottom leg element (touching the table) and between the top leg element and the down tube (cables touching each other). A riser was added to the in-chamber work stool to allow work access, and the latter touching was corrected. The former touching, which is much less critical, was found to be much more difficult to correct, and was left in a touching condition. Digital photos were taken to document the configurations, and actions are being taken to better understand whether the touchings are due to cable saggings or improper installation.
A ladder platform has been fabricated and installed at the X arm 80K pump/optical lever table in the corner station. This will allow convenient access to the optical lever laser and the gate valve mechanical lock, which should prevent future stepping on the optical lever table.
Large parts are being cleaned by Allied and will be shipped to LHO. Small parts have been shipped to LHO for cleaning and baking.
Made some progress on the Common Mode servo detailed design. I hope to have it completed by the end of this weekend and ready to start the PCB layout. We are prototyping the 16 step variable gain amplifier in our lab now and with Paul's help we hope to have results by end of this week. This is a low noise (3nV/rt-Hz) 15 volt amplifier that (if it works) will be used in four places in the CM Servo and eight places in the LSC Whitening filter. Mohana has begun laying out the LSC Antialias filter board. Flavio, our visiting Italian engineer, is helping me get five more LSC Notch filters tested and out the door. Thanks, Gary.
We shipped 5 more GPS Clock Drivers this week to Hanford. Three more are waiting for a delay chip that is back ordered from the factory.
- The two controllers that were destroyed on LHO FMY have been repaired and are being tested. They should be ready to ship by 3/3.
- The modulated version of the satellite amplifers have been assembled and are being tested. It has been decided to reduce the modulation frequency to ~1KHz for the tests to be conducted at LHO. This will reduce to offsets induced by the vacuum cabling. The local sensor bandwidth will thus be limited to ~100Hz for the tests. Future system designs will have to address this offset and cross talk problem. The amplifiers should be ready to ship to LHO by 3/8.

1.2 LLO

The newest version of the frequency stabilization servo (Rev. C) has been installed. After correcting for an incorrectly soldered part and a PEM nut that contacted more than one plane in the circuit board, the servo is now functional.
Previous reported problems associated with the PSL MEDM screens were partly the result of the incorrect screens being called up. Old versions of the MEDM screens will be removed by week's end.
Data from the LLO PSL temperature stabilization scheme will be obtained and compared with LHO data. Any differences should be due to the hardware differences.
- realigned the Faraday isolator in optics lab
- measured the double pass isolation ratio (the isolation for the returning beam); the isolation ratio and transmission for the returning beam were 37.4 dB and 88% (which is a little low), respectively. Because the total angle of Faraday rotation depends on the laser power (due to temperature dependence of the Verdet constant), it is necessary to adjust the orientation of the second halfwave plate on the optical table in the vacuum chamber at the nominal PSL power when it is available.
Last week Rana was in Livingston to help install and align LIOT1. The physical installation, wiring termination and checkout went well. Problems related to swapping the premodecleaner on the PSL (burned out PMC amplifier) left insufficient time to complete the alignment of the table to the MC reflection beam. In addition Rana found that the ISC chamber video camera on LHAM1 does not provide an adequate view of the MC1 and MC3 mirrors; a workaround using a viewport on top of the HAM connecting nozzle is under consideration for next week's scheduled vent.
The ETMy telescope was assembled, pre-aligned, focussed, installed in BSC4 at the x-end and positioned laterally by means of the ISC theodolyte. Final alignment of the telescope pointing orientation and steering of the output beam is scheduled to be completed by the end of the week (2/3/00). The ETM beam dump has been assembled and is ready for installation and positioning by the end of the week (2/3/00).
The ETMx has been installed and accurately positioned in the Livingston X-end station. We were only able to obtain a 1% reflectivity on the HR surface which was not enough to align it in pitch and yaw. We were able to autoreflect off the HR surface with the theodolite. Three calibration runs were made to determine the accuracy. By comparing this method to the laser autocollimator on an optical flat we found we could be accurate and repeatable to within 15 microradians. Currently we are on hold due to controller and signal problems
- LLO ETMX suspension system is ready for installation of the optic starting 3/1

2.0 Commissioning (incl. diagnostics and characterization)

2.1 LHO

There have been two 2km cavity (X arm) locking runs made in the last week. The first run saw locking stretches of ~20 minute duration, limited by a combination of linear drift, excitation of a 32kHz test mass mode, and a broadband frequency noise in the several kHz region (the sum of these would eventually saturate the coil drivers). During this run the input beam was better centered on the input test mass; this apparently reduced the clipping loss on this mirror so that the cavity resonant reflectivity went up to 96% (still not as high as expected, but better than the previous measurement of 94.5%).
For the second run, the linear drift component was reduced with the temperature stabilization servo of the PSL reference cavity, which was installed and turned on by Rich and Peter K. The 32 kHz mode was greatly reduced by adding an additional low-pass filter in the servo chain. We also had hopes of reducing the frequency noise component with a better VCO-MC servo configuration, but that doesn't seem to have worked, and needs more debugging. Nonetheless, the second run achieved lock stretches of ~1 hr duration. A summary of this run is posted in the 2-29 LHO Elog. Unfortunately, the full-bandwidth archived data for this run appears to have been mostly contaminated with 16Hz data alignment problems.
The focus now is to get the wavefront-sensor based alignment system running on the cavity. Both WFS heads are now functioning, and RF test signals injected into the demod boards come out as expected at the output end of the digital servos. We also intend to archive some data of a long lock stretch with no interventions, so that it can be analyzed for things like microseismic correlations.
For this week I have been preparing for LHO 2K arm commissioning. Reviewing the significant recent results and focusing on a [final] effort to really pin down the "true" visibility and hence arm cavity optics losses. It sould be possible to simultaneously fit the real time cavity reflected and transmitted intensity to determine the relative mismatch and intrinsic loss components. (Bill Kells)
Recent MC linewidth measurement data have been partially analyzed. By fitting the data from the transfer function measurements we obtained cavity pole frequency of 3.54 (2) kHz. Using the same method to fit the data from the previous x-function measurements (last Sept.) the cavity pole frequency was found to be 3.63 (3) kHz. It seems that the MC cavity Q increases slightly although the difference between the two measurements is still within 3 standard deviations. A set of data from the ringdown measurements will be analyzed soon and we will compare the results.
Dave Reitze is looking into possible telescope misalignments that could accunt for the the ~ 5 cm vertical shift on the ITMx.
- Rev B ASC whitening board are being stuffed and should be ready for test by 3/10. When they are ready they will be shipped to LHO where they will replace the Rev A boards in the system. This replacement will fix the polarity flip problem that occurs when the filters are bypassed.
- Pentek is sending us a low distortion version of the 6102 DAC module so that we can measure the output noise voltage. Hopefully it will be lower than the current 7uV/rtHz. Any reductions will make the design of the universal dewhitening filter easier.

2.2 LLO

Saulson worked on developing a commissioning plan for LLO, through discussions with LLO staff and LIGO experts.
Loaded the diagnostics test software onto the LLO CDS server, compiled it and run some of the command line utilities to make sure everything is recognized. Successfully loaded and started the testpoint manager software on Baja in the DAC controller crate.

3.0 Other Engineering and Scientific Activities

A three flat calibration test continues in the Metrology lab. The current test takes advantage of a more stable thermal environment than we had for the last test which was done a year ago.

3.1 Issues Concerns

SDRC IDEAS Master Series 7 is still a troublesome installation. Larry Wallace hopes to address this soon. There is no simulation package and the 2D translators do not work well. (Janeen Romie)
The LHO ETMy realignment task had to be repeated due to the fact that its controller was in the wrong mode during adjustments. Although this was covered by procedure and originally set up properly, it defaulted to the wrong mode when a blown fuse was replaced and the operator was not aware of this feature. A training session on the functions and use of the controllers should minimize reoccurances of this type. (Larry Jones)
A technician who had taken a radio to the X end station for listening during work noticed a strong RF signal during tuning. Turning the volume down to zero revealed a local acoustical noise of the same pitch. This should be checked and the source eliminated or shielded if it's a potentialdetector problem. (Larry Jones)

3.2 Site Support

COS needs site support at LLO. A significant volume of large COS parts will begin to arrive during the next several months; some of the parts will need cleaning and baking, others will arrive cleaned and will only require baking, all of the parts will need a suitably large staging area for assembly and subsequent clean storage. (Mike Smith)

40 Meter Interferometer (Weinstein)


Two weeks are included below - GHS

March 2, 2000

Feb 25, 2000


From Mike Smith March 2

I am working on getting the 40 meter layout drawing files, which at the
present are drawn using the Ideas drawing package, translated into ACAD format.


Thermal Noise Interferometer (Libbrecht)


We are in the process of installing our triangular mode cleaner, and this
week we glued magnets onto both of the diagonal, flat mirrors.  We also
glued fixtures and a side magnet to one of the mirrors.  We are using a
single side magnet per mirror, so the first flat mirror will be ready to
suspend as soon as the vac-seal epoxy has cured to our
satisfaction.  When we glued the magnets onto the first flat mirror, last
week, we kept a small sample of epoxy from that procedure, and we found
that the sample needed nearly a week to completely cure. (Later samples
showed the same behavior, so we do not believe that this is a function of
poor mixing.)  Our back, curved mirror already has magnets and fixtures, so
when we are finished preparing the flats, we will have a complete set to
make a triangular cavity.
 

This past Tuesday, Feb. 29, was the last day Eric accepted comments on his
"Thermal noise in coupled harmonic oscillators" paper, and all of the
comments received came in on that day.  Eric have been assimilating those
comments, as well as improving Proposition 3 in Appendix B, an estimate of
the accuracy of the high-frequency asymptotic formula.
 

Also on Tuesday, Eric did some community outreach by participating in
"Futures Day" at John Muir High School, here in Pasadena.  Speakers from a
wide range of professions gave presentations to students about what they
did for a living, why they liked it, and what preparation was necessary.
Most of the students had never heard of neutron stars, black holes, or
gravitational waves, and they were very interested and asked a lot of good
questions.
 


LASTI (Zucker)


LASTI (Zucker, Shoemaker, Burgess, Kruzel)
-----------------------------------------
Vacuum envelope:
Continued installation of annulus pumps & control hardware.

Installed and tested main valve control interlock panel; permanent
wiring installation in progress.

Procured reducers for RGA nipple & built up vacuum controls relay
racks.

Mechanical internals:
The weather (snow & ice) has cleared up enough to rig the internal
seismic isolation components (received in January from Allied
Engineering) into the LASTI high bay.  We've scheduled the Plasma
Fusion Center's 20 ton forklift & crew for Thursday 3/2.

Interferometer:
DHS is drafting technical & strategic plan for our initial interferometer
implementation to support of LIGO II SEI/SUS testing. This will be
distributed prior to the LSC meeting for discussion at the technical
advisory panel meeting.


Data Analysis and Computing (Lazzarini)


Simulation and Modeling


Lock Acquisition study (Matt Evans)

The servo design leading to step 1 to step 2 (Michelson locked)
and step 4 (all mirroed placed at locked position, but the arm
power is not filled yet) to step 5 (all locked and power fully filled)
have been done. The recorded ground motion has been parametrized
and the e2e module of the stack has been made based on Ed Daw's
parametrization.

Mechanics simulation & PSL (Giancarlo Cella, Hiro Yamamoto)

Giancarlo calculated transfer functions of the PSL reference cavity
based on MSE (Mechanical Simulation Engine). Hiro calculated the
frequency noise caused by the cavity motion.

Giancarlo gave a talk at LHO on Feb.25 about MSE and the modeling
of the PSL reference cavity using MSE.

Giancarlo, Hiro, Rick, Michael and David had a meeting at LHO how to
proceed to assist the design of the PSL reference cavity. LHO member
measured the motion of the PSL table and the data is now reviewed by
Giancarlo. Rick proposed a several modifications of the cavity,
and Giancarlo will generate the mirror motion using the measured table
motion with difference configurations of the cavity propsoed by Rick.
This will include the deformation of the cavity as well to generate
the distance change of the two mirrors. When this is provided, Hiro will

feed this mirror motion into e2e and generate the frequency noise.

Ringdown data analysis (Hiro Yamamoto)

Hiro obtained more data from Haisheng about the MC ringdown and the
detector
response used at the FP ringdown experiment analyzed last week.
With the detector response taken into account, the model calculation of
the
FP ringdown power spectrum tallied with the measurement well.

Adlib basic improvements (Biplab Bhawal)

Biplab is working to implement the load/save (stop the simulation and
resume again later time) feature. Various problems found when using e2e
for PSL was looked into account. The frequency noise is proportional to
the frequency (~10^14) and the simualtion of the cavity with a tilt of
10^-6~8 needs to be done correctly.
 

Biplab, Matt and Hiro discussed about the planning of the first e2e
paper.

LIGO Data Analysis System (Kent)


This week was primarily spent testing the performance of the new
LDAS release 0.0.9 software. These tests were carried out in two
main areas:

 - Socket Based Communications: It was learned that the tests of
   LDAS lstrings were skewed in last weeks tests. This was corrected
   by making the tests consistent in size with 2,4 and 8 byte data
   types. Early results showed much more consistent transmission
   rates for lstrings when compared with integers and floats but
   there is something still unusual about the test so new tests are
   being performed to account for instantaneous fluctuations in the
   measured performance.

 - Data Base Ingestion: The ingestion rates for data into LDAS
   tables was re-evaluates with the new 0.0.9 release. Early results
   indicate that speed for tables which do not have blobs has
   increased by roughly 50%. There is a bug in the blob ingestion
   code which prevents tests on tables with blobs. This will need
   to be debugged before further testing is possible.

LDAS was also busy preparing for implementation of several new APIs
this week. Documentation for the mpiAPI, wrapperAPI and dataConditionAPI
neared completion. Work has already begun on the mpiAPI and wrapperAPI,
but weekly meetings with the LSC have kept a steady but minor flow of
new thoughts in the documentation for these two. The documentation for
the controlMonitorAPI was only distributed this week and a kick-off meeting
with programming staff was held to outline the relationships between these
3 LDAS APIs. It was proposed at the meeting that the controlMonitorAPI
should be split into a server/client implementation allowing the GUI
component to be used anywhere. These APIs play an important role in the
operations of the LDAS beowulf cluster. Another key component to the
beowulf cluster's software is MPI. LDAS has choosen the public domain
standard for Linux clusters - MPICH. The new version release in December
of last year has proven to be buggy and not fully supporting some of the
standard. This week a major memory leak was discovered. LDAS reported the
bug to MPICH but never heard back so we patched the leak ourselfs. This
means that for the time being, we will be using a "custom" MPI implementation.

A milestone in the development of the version 4 FrameCPP I/O library was
reached this week. The software still lacks support for the "table of
contents" structure. However, since this structure is optional, it means
that we could start to write frames based on version 4 of the frame spec
and read the with the fully functional FrameCPP library once complete. It
is worth noting that frames written with a "table of contents" will support
much faster read access so implementing the full frame specificaition is
still a high priority.

Stuart:
A re-write of the frame archive monitoring script to parse the
ftp logs and generate statistics on LIGO usage of HPSS.
Initiated discusions with CACR on the possibility of purchasing
a second 6,000 tape slot silo to hold the main LIGO data archive.

LIGO 40m/TAMA300 coincidence analysis (Mike Zucker, Julien Sylvestre)
----------------------------------------------------------------------------
JS found significant correlations between transients in strain, magnetometer
and seismometer channels from the 40m '99 run using an efficient statistical
time-frequency technique. Details at

        http://space.mit.edu/LIGO/Research/julien/40mTAMA/bursts.html

MZ continued prototype development of "classical" matched-filter pulse height
analysis for canonical (Gaussian-envelope sinusoid) pulse templates
on '99 40m data using Matlab. Scripts and some preliminary findings
posted at

        http://www.ligo.caltech.edu/~wmajid/40m+tama/

Walid:

I have started to work on the fast Chirp Transform technique. I have
implemented a not so efficient but exact method to do an acceleration
search for pulsars. I am now trying to get a better feel for 2D transforms
and use it to check my results.

I have put together a draft of an LSC proposal to carry out a coincidence
search using the 40m and TAMA data. Work in this group is continuing. For
an update, please have a look at:

http://www.ligo.caltech.edu/~wmajid/40m+tama
 

General Computing


Lazzarini: We have received a large database from Battelle (PNNL) which documents our use of the T1 link from LHO over most of past year
on a resolution of 5 minutes(!). I have filtered the data with an excel spreadsheet and created set of plots (NOTE: pdf file size is 4MB):

http://www.ligo.caltech.edu/~lazz/distribution/ESNetUsage1999.pdf

The data are plotted modulo 24 hours to see time-of-day trends and modulo 31 days to see day-of-month trends. Integrated usage statistics results in volumes
which seem too large and I am tracking this down. The data usage trends are total flux to and from LHO, with no visibility into the destinations.
Peak BW usage is appraoching 0.65 T1 which we have confirmed is the saturation level of single-socket  transmission
over TCP/IP ethernet (2-sockets in parallel appoach the full T1 bandwidth). We have asked for continued data from PNNL to allow us to watch the usage trend.
We have talked to PNNL about opening up a second T1 line for LHO if and when it is needed.
 

MIT:
Nothing to report.

Livingston:
Preparing for LSC and usual maintenance.
 

Hanford: (Christine)
Spent most of this week helping my new helper Oudone Voraphaychith, a
WSU EE student, get settled in to his new job.Oudone will be helping
to upgrade all the site PCs to Windows98 as well as helping with user
problems and any misc. jobs that come up.

So far Oudone has upgraded two PCs to Win98 and moved one of the
upgraded PCs out to the MidX station.  The other is having some
additional software installed on it so that it can become the Guest
computer in the Common area of the Offices.

I have also followed up on a PO for the Exceed license upgrades,
followed up on getting Norton Antivirus software from the Caltech site
license.  Continued network security maintenance, did the weekly
backups, helped setup a new Unix workstation for Michael Landry, helped
users with several printer and PC problems and kept the GC accounting
paper work up to date.
 

CIT:
  Suresh completed monthly full backup of LIGO servers.
  Setup a PC with Windows NT workstation for Thomas Frey. Installed couple of
applications (Microsoft Office, Eudora, Exceed, Secured Shell 2 etc ) required.
  Installed a2ps (ascii to postscrit print) utility on sirius.
  Resolved some of the networking problem of printers. Setup one new user
account.

  Barbara continued work on the web videos.  I'm trying to fix some clips with
single-channel audio and clips where the video freezes.  Scanned the photos
of the Nov 11 speakers.(Barbara actually resolved the video freeze problem
today).

  Made a large number of web site changes.  Updated links to Donna's pages
(again); updated LSC pages with meeting, MOU, attachment, and report links;
 changed all the LSC links to point to public document directories.

  Updated the VB program that generates pages for the as-built drawings via
the DCC database.  Created pages for approximately 300 facilities and BTE
drawings.  A couple of drawings still have to be processed and then the
pages will be published.

  Met with Linda Turner again about changes to the DCC system for version
control.  The current plan will track different versions of drawings for pc
boards.  The DCC can track individual boards via serial number using the
child table/form for serial numbers.

  Larry worked a number of PC issues. Assisted in a build and resetting of a
laptop. One of the lessons learned is that installing AOL can cause a lot of
problems. Users should be sure to limit their installation and say no to most of
the questions.
  A number of PC's were having problems with things locking up and dropping out.
After running Norton Utilities for Windows (from the CD) the problems no longer
appeared on the systems. Loading Norton on a system and leaving it on presents
its own set of problems and running it from the CD has eliminated that issue.
Worked on the Amaldi server. It has a number of problems and will need to be
completely gone over again.
  Found the problem with the Simulation pkg. on IDEAS. A number of patches and
libraries need to be installed on any machine running the SDRC s/w pkg. locally.
Presently, sirius is the only machine that pkg. can run on. We will be
installing the necessary items on the machines of the main users over the next
few days. The DWG converter on IDEAS needs to be re-installed which will take
some time and hopefully can be done in the next few days.
  Worked a number of DCC issues. Resolved some problems with files and setup a
few programs to help automate a few of Linda T.'s procedures in moving documents
around.
  Fixed a number of printer problems. All were paper jams or the user forgot to
put in the correct media for the print job.
  Helped Ed C. setup a number containers for shipping the E3000 and a couple of
monitors to Livingston. Also, did some work in preparing the units themselves
for shipping.
  Assisted a number of people via telephone for s/w installations and
work-throughs on their PC's. I am working on a web page to get more information
out on how certain pkgs. like ssh work.
  Continued working on a number of procurement issues.
  Worked with the SRL group in dealing with a few Cadence issues they were
having.
  Assisted Barbara in working through some of the LSC web setup issues so that
Jennifer H. of MIT can perform her tasks dealing with the LSC WEB pages.
 


LIGO II/Advanced R&D (Sanders)


Thomas Frey joined the LIGO II effort this past week to provide additional support to R&D/LIGO II schedule and cost estimate preparation.

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

I attended the Aspen 2000 Gravity Wave conference and presented some
recommendations for scattered light control in Advanced LIGO interferometers.

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

Specifications for a LIGO 2 pathfinder polish are nearing completion.

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

>Placed RFQ with REO for the coating of sapphire test pieces.
>At the same time requested REO to schedule a coating run for the last week
>of March to coat the test pieces.

>From: Sam Richman <srichman@ligo.mit.edu>
>stiff isolation system report
>
>Fabrication of  ~95% of mechanical parts for the double active stage
>prototype was completed by the main contractor, High Precision Devices, of
>Boulder, CO.  The blade springs, flexures, and clamps are in production,
>with all parts expected to arrive at MIT on Wednesday 8 March.  The vacuum
>chamber to house the prototype was successfully pumped down.  The noise of
>the commercial inductive proximity sensors (to be used for very low
>frequency regime of the servos) was measured to be 10^-7 m/rtHz at 0.01
>Hz.  Production of readout electronics for seismometers and cabling continues.

>From: "Ryan C. Lawrence" <rclawren@ligo.mit.edu>
>
>I got the CO2 laser on tuesday, and am working on installing it next to the tank
>and instituting safety procedures in the high bay (signs, lights, goggles,
>etc.).  The shielded ring analysis is nearing completion, and I'm working on a
>double ring and shield solution.  Rob Bennett (ugrad) is working on instituting an adaptive
>meshing scheme into his finite element model of the scanning laser method.  Dave van Stroh (ugrad)
>is working on measuring the intensity distribution of the new ring heater  with
>the pyroelectric sensor.

From: kells@ligo.caltech.edu (Bill Kells)

>For last week I was preoccupied at the Aspen mtg which
>had mostly to do with Adv. R&D.
>I had/have been studying the the GW band "scintillation" noise
>which any material must have at finite temperature and with
>a dn/dT coefficient. This was inspired by the recent revelation
>of "Braginsky noise" which is closely related.


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