Weekly Report for Week Ending January 17, 2002



 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 21, 2002 will be:

There will be no Executive Committee Meeting on Monday, January 21 because of the holiday.


Special Announcements:


Weekly Report Highlights

The E7 data collection was stopped at noon CST this Monday.


LSC Issues (Weiss)


No report.

Next LSC Executive Committee meeting
-------------------------------------
Friday Jan 25, 2002 at 11:00AM ET (Please note change of day)


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



LIGO Weekly Site Telecon (Lindquist)

A Site Teleconference was held on Thursday, January 17, 2002.  Discussion centered on the status FY 2002 costs-to-date, of NSF funding and the Cooperative Agreement, the establishment and budgeting of FY 2002 accounts, the FY 2002 Financial Reporting format, as well as the status of the construction at the two sites.  Administration is moving towards restructuring the overhead application for fabricated equipment.  The biggest effect for LIGO will probably be for facilities fabricated for intended eventual Government ownership.  Florence will be assessing the impact of the changes as best she can given that the information available is limited.

A review of the recent E7 Engineering Run is scheduled for February 4 in place of the Executive Committee Meeting.  Mark Coles and Fred Raab will be requested to summarize lessons learned.

The list of current actions revised to reflect the status of open actions assigned through January 17, 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>

ACTIVITY

Click the link to access the DOCUMENT CONTROL CENTER WEB PAGE.


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

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>

CONSTRUCTION:

OPERATIONS:

SUPPORT

Irene Baldon

Dorothy Lloyd Rita Torres

Advanced LIGO (Frey)

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

Progress Period from 01.11 to 01.17

Accomplishments:

Schedule 01.18 to 01.24:

Reports (Lindquist)

We are doing a standard Annual Report for the Construction Project as of the end of November.  I have received all expected contributions and am working on the report.  This effort has been interrupted to work on responses to DCAA Audit requests.



Change Control/Contingency (Lindquist)

The following change request has been submitted:
 


CR-010012 
Revision B
WBS 1.4.4.1 Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites P. Lindquist

Press for the latest Contingency Needs Projection



Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

No report this week.


LIGO Hanford Observatory (LHO) Operations (Raab)


2K PSL: (Doug & Rick) We are making preparations to increase the 2K PSL power into the IFO from 1 Watt to 6 Watts. We peaked up the laser alignments, Reference Cavity and pre-mode cleaner visibilities. We are installing added attenuation to the ISC/IO tables to maintain the same light levels on WFSs and to set light levels to the trigger  PDs etc. We are placing the light pipes back over the beam path on the 2k PSL . We have added a BNC bulkhead terminal strip to the 2K PSL table and terminated all the CCD cameras and PDs outputs.  This gives a central point for measurements without the risk of changing alignments when connecting/disconnecting cables. We have cleaned up some of the wire routing on the tables as well.

I will be installing the laser safety shutters on the PSL tables and wiring in the PSL shutters soon to complete the laser safety hardware installation. We will do a final walk through, approve the new SOP, begin training and final commissioning as time allows.

Facility: (Otto) Only the slopped portion of the auditorium floor is not concreted. All the other floors for the building have the slab on grade. There is only a very minor work left on all the utilities. All the pipes, wires and conduits are in the ground and back filled only a few connections need to be made. We are expecting structural steel to arrive on site the 11th of February.


LIGO Livingston Observatory (LLO) Operations (Coles)



Interferometer: Immediately following the conclusion of the E7 run, the laser was shut off and electrically disconnected so that the acoustic isolation chamber could be installed around the PSL table. The chamber erection is nearing completion and should be completely finished this week.

CDS: Upgrading the control room machines to Solaris 8. Working on the CDS Red book for Livingston. Also today we are working to change the time server back to the True Time Server in the mass storage room. I will also look into changing the bad disk on the Frame Builder. Downloaded a software patch for london to deal with latest security issue with the CDE desktop on solaris. Completed the CDS diagnostics medm screens and epics interface for the mass storage room machines. This needs to be added to the checklist. (Cheithan)

GC: We are working with LSU to put the final touches on the installation of our new router and firewall.We are doing some maintenance and upgrading on our servers, which had been on hold over the E7 run.


Detector/Technical Support (Whitcomb, Coyne)


 

Commissioning:
Hanford
Livingston
Science & Engineering Support
See also the daily electronic logs for the installation and commissioning activities:
Hanford Detector Log
Livingston Detector Log

E7 Run

Szabi Marka, Daniel Sigg
The E7 data collection was stopped at noon CST this Monday. We received feedback from several people, all very positive and encouraging. We should all be very happy with the results! The end of the data collection is the start of the intensified data analysis effort, which should be our focus for the weeks to come. We would like to express the gratitude of the collaboration to the people who made it possible to have such a successful run! A great "Thank You" is due to everybody who participated in the building and commissioning effort to get us to this point of operation; especially to the observatory staff.

Lock statistics for the E7 Run, based on a preliminary report from Gaby Gonzalez, are below; More data is available in the report and will become available as the GEO and ALEGRO availability is compared to the LIGO instruments.

Single:

L1

Total locked time: 284 hrs
Duty cycle: 70.7 %
Total time locked with locks longer than 15min: 249 hrs

Duty cycle for long locks: 62 %

H1

Total locked time: 294 hrs
Duty cycle:      72 %
Total time locked with locks longer than 15min: 231 hrs

Duty cycle for long locks: 56.6 %

H2

Total locked time: 214 hrs
Duty cycle: 52.5 %
Total time locked with locks longer than 15min: 157 hrs

Duty cycle for long locks: 38.5 %

Double:

H1 and H2

Total locked time: 180 hrs
Duty cycle: 44.1 %
Total time locked with locks longer than 15min: 111 hrs

Duty cycle for long locks: 27.3 %

L1 and H2

Total locked time: 160 hrs
Duty cycle: 39.3 %
Total time locked with locks longer than 15min: 98.8 hrs

Duty cycle for long locks: 24.2 %

L1 and H1

Total locked time: 227 hrs
Duty cycle: 55.6 %
Total time locked with locks longer than 15min: 154 hrs

Duty cycle for long locks: 37.8 %

Triple:

L1, H1 and H2

Total locked time: 140 hrs
Duty cycle: 34.5 %
Total time locked with locks longer than 15min: 71.5 hrs

Duty cycle for long locks: 17.6 %

LHO COMMISSIONING

Rolf Bork
Alex made a number of changes to the DAQS controller. One primary change was to prevent the controller from being overloaded when framebuilders make requests for configuration updates, which could cause the controller to go into a synch fault. This was also needed to support the new multi-CPU Epics Data Collection Unit (EDCU). The new code is now running and being tested at LHO.

2km Commissioning

Jay Heefner
We have discovered that the noise seen on the 2k ASC bias inputs to the suspension controllers is caused by ground bounce during VME polling of the penteks. The noise can be reduced by appropriate grounding and filtering, but we should consider a LIGO wide solution as part of the EMI/noise investigations. See the LHO 1/15/02 elog entry for a description of the noise (user: reader, password: readonly).

4km Commissioning

Rolf Bork
1) Fixed problem on 4k DAQ where the two LVEA data acq units were limited to only acquiring a few (8) channels before experiencing VME bus errors. These units are now operating at their intended capacity of 55 and 97 channels. This adds approx. another 0.5MByte/sec of data collection at LHO above that recorded for E7.
2) Problem with Digital Suspension Control (DSC) test points was a mismatch in TP names between GDS and DAQ. This has been corrected and we will reload and test this tomorrow AM.

3) Loaded new DSC code in end stations, which incorporates the new filters and other changes requested last month (same as LVEA large optics, previously installed prior to E7).

LLO COMMISSIONING

Rai Weiss reporting


The commissioning group at Livingston has not had an organizational meeting since the end of the E7 run so the plans described last week have not changed. Currently, the acoustic isolation chamber around the PSL is being installed and there is a good chance that the laser will again be on by Friday Jan 18. While the laser has been off, noise, saturation and the transfer functions of electronics is being characterized and measured by Mike Zucker, Rana Adhikari, Szabi Marka and others.

SCIENCE & ENGINEERING SUPPORT

Improved Digital to Analog Converter (DAC) Module

Jay Heefner
The letters to vendors for the RFI should go out this week. We have asked for responses by the first week of February.

2 Omega I&Q Demod Board

Jay Heefner
Two boards have been stuffed and tested. One was sent to each site. The remaining modules are stuffed and awaiting test.

RF Photodiodes

Rich Abbott
Finished characterization of all RF photo-diodes in our inventory. Data has been transmitted to Perkin Elmer for their investigation into the failure mechanisms & causes. Measured series resistance and capacitance at nominal bias. Preparing a diode at 29.5 MHz for shipment to LHO today. Continuing research into RFPD's and trying to get the last remaining diodes tested and out of the shop.

MC Servo

Rich Abbott
Completed CAD of prototype variable gain amplifier for use in the MC length path in the MC servo.  It will go to the board house today (01/17)

Timing System, Clock Driver Boards

Rich Abbott
In the process of checking the boards out for the new timing system clock driver boards. The boards have some stuffing errors and will require testing. Several are going through an accelerated test for immediate shipment to Rolf/Stan at LHO.

EO Shutter Controller

Sander Liu
Three new controllers are in various stage of completion. One should be ready for delivery sometime next week.

LEMO version Anti-aliasing Filter Chassis

Sander Liu
10 housings were received last week. We are waiting for the circuit boards and electronic components to make kits for Accu-Asembly to assemble. 20 each of the 16 channel data cables were on order but not received. A quotation for 200 each D68L8EX-850 Hz lowpass filter modules were received and an order will be placed next week.

Seismic Signal Conditioning

Sander Liu
In the process of finalizing the conceptual design document. The document will be sent out to the CDS weekly meeting group for comment and review.

GEO PSL Boards

Rick Karwoski, Paul Russell
The three main PSL boards (FSS, 80MHz VCO and 21.5 MHz Frequency Reference modules ) have all been tested and burned in. The Freq Ref and FSS have been boxed up with the appropriate traveler paperwork. The 80MHz VCO will have its paperwork completed tomorrow. It will be boxed up and ready for delivery.

Optical contamination testing cavities (OTF)

Lee Cardenas
Preparing the optical contamination cavities for advanced LIGO materials testing. The first optical contamination testing chamber is in standby and waiting on Jordan's visit this Friday. Jordan will advise and be able to provide some other information needed to continue. Another contamination chamber has been prepared, optics have been aligned (with exception of a needed 1/4 wave plate), mode matching is in progress.

Data Viewer

Rolf Bork
Hongyu Ding is working on updating dataviewer to allow it to directly read new 16sec frame files such that it can read archived E7 data

ASC Code

Rofl Bork
Lori has begun modifying ASC code such that it is similar to LSC w/configurable filters, etc.

DMT

John Zweizig


Writing code to emulate the LSC on-line software. Comparing the emulated results to the results of the on-line software recoded in the data frames will demonstrate that the on-line software is functioning correctly. Any discrepancies could point out occasional failures such as precision errors or timing errors if they exist

Seismic Isolation Improvement

Dennis Coyne reporting
·Much of the team will be meeting at MIT 12/28 through 2/6 to review progress, design and complete planning. A requirements & preliminary design review will be held in February
·Rai Weiss and Joe Giaime are preparing requirements definition. Robert Schofield has prepared some Hanford wind induced seismic noise data that is being reviewed.

·Ken Mason has nearly completed the mechanical design and detailing for the structure which integrates the actuators into an assembled pair atop each pier. A set of drawings will be generated in the next couple of weeks for review by the team.

·Marcel Hammond has designed a spring tester for the large custom helical springs and is working with the fabricator. The springs should be delivered for testing at LLO next week.

·Ken Mailand spent last week at Stanford to get up to speed on the hydraulic pump station design and components. He is gathering together a complete parts lists and will soon be ordering all of the parts to build up a complete pump station (includes the motor, pump, accumulator, flow resistors, active diverter valve and controls and transmission line, filters, pressure transducers, etc.) Plan to design, assemble and test within 3 months at CIT.

·Joshua Phinney is finishing a report on the transmission line modeling and testing that he performed at MIT.

·Peter Fritschel and Rich Abbott are preparing an electronics requirements document for the hydraulic pre-isolation system.

·David Shoemaker has been exploring linear electric motor and solenoid alternatives to the hydraulic actuator. The intent is that they be “plug & replace” compatible with the integrated actuation assembly that Ken Mason has designed.

Optical Modeling

Erika D’Ambrosio
I studied the formalism of complex-valued Hermite-Gaussians to understand how operators are supposed to be transformed when biorthogonality must be applied. Doing so I finally tackled the last puzzle William Kells and I have been left with: how to switch from an initial TEM basis to the basis of modes defined by the symmetric combination of the two perturbed arms. This issue is a "matter of principle" since in reality we have to deal with the feeding beam basis and we have already explored the consequences of this on the "sidebands imbalance". The problem of understanding whether the imbalance is an intrinsic physical effect or the result of using a driving beam that breaks the symmetry was important. I still have to discuss my results with Bill but they clearly show that there is an intrinsic balance of the two sidebands if the basis is chosen according to the eigenmodes of the common perturbation plus (since the Guoy phase of the eigenmodes is redefined) the beamsplitter must be moved in such a way that the eigenmode we choose to be the resonating one has no loss out of the dark port.

These two ingredients are not independent of course and the analysis has been pretty complicated but roughly speaking there is a maximization procedure for one eigenvalue that I can use for choosing the "differential length" and then I formally evaluate the eigenmode for the corresponding common perturbation and tune the common length. This basically corresponds to having only the mode orthogonal to the resonating one at the dark port. If the feeding beam exactly matches that resonating mode everything is trivial and this choice corresponds to the minimum power of the carrier at the dark port and all our intuitions are reconciled with formalism.
 


40 Meter Interferometer (Weinstein)


Bill Tyler et al have completed a draft of the 40m Annual LIGO Safety Audit Report. We have already acted on their primary recommendations, and will act on them all before long. A response (to questions, etc) is being formulated.

PSL (Abbott, Ugolini, Vass, Smith, King): Our PSL 126MOPA laser power is now down to 2.5 watts. We hope to swap it for a newly refurbished 700 mW NPRO, early next week, with Peter King's help. Soon thereafter, we will re-layout our PSL table, with new mode matching lenses and new layout for the beam diagnostics.

Suspensions (Romie): The mechanical parts for the SOS suspensions have been cleaned and baked at LHO, and are now back at our lab.

Mode cleaner sensing and control:

Suspension controllers (Ben Abbott, Jay Heefner): South Annex Bake oven chambers (Vass, Taylor, Cardenas): Facilities (Vass, Jones, Smith, AJW): Dennis is up at LHO (back next week). He continues his studies of correlated noise with CorrMon, helped Rolf and Dave Barker reconfigure the DAQ to solve a PEM problem, helped diagnose misalignment in the 2K X-arm, and assisted or observed in many other tasks.


Thermal Noise Interferometer (Libbrecht)


Since our last report we have made progress in a number of different areas.  We have ruled out two candidate noise sources in the North Arm cavity: OSEM controller electronic noise and "defocus" noise in the photodetector.  We received the fourth and final sapphire optic from Crystal Systems and shipped all of the optics off to REO to be coated.  Flavio Nocera was kind enough to build us three more notch filters for the South cavity.  And we further reduced the laser frequency noise by increasing the gain of the mode-cleaner servo, with the result that we now see a noise floor in the South cavity that scales as f^-0.5 over an additional kilohertz at high frequencies.

The fact that, by reducing the laser frequency noise, we can uncover more of a noise spectrum that looks like thermal noise is encouraging.  Our baseline goal for the TNI was to have a fused-silica-based, thermal-noise-limited interferometer by Dec. 18, 2001.  We first began to see this f^-0.5 noise spectrum on Dec. 3, and its level is approximately that predicted by the fluctuation-dissipation theorem, based on the measured Q of the South Output mirror.  There is an additional factor of 2 or 3 that might be accounted for by coating thermal noise (Gregg Harry, private communication).  Moreover, the noise level in the North cavity is substantially higher than its predicted thermal noise, and it does not exhibit an f^-0.5 spectrum anywhere, so a spurious source of f^-0.5 noise does not seem likely.  It is still too early to positively identify our data as thermal noise, but the tests we have performed since Dec. 3 have strengthened the case for thermal noise rather than weakened it.

Now about the North Cavity.  Its noise level is higher than that of the South cavity, and we would like to know why.  We have listed a number of potential candidates for this excess noise and are in the process of systematically eliminating them.  One of the first things we noticed was that the error signal for the North Cavity is approximately a factor of 100 smaller than that of the South Cavity.  We thought at first that the beam falling on the photodetector was defocused, and that that might be causing the discrepancy.  As it turns out, both beams are tightly focused on their respective photodetectors, so that at least is not a problem.  Next we will check the intensities of each beam using an independent photodetector and, if those are the same, we will check the response of each RF photodetector.

Another difference between the North and South cavities is their OSEM controllers.  We have seen evidence in the past that not all of our controllers have the same noise level, and we suspected that one of the North Cavity's controllers might be introducing a significant amount of noise.  The most reliable way to check this, if not the most elegant, is to simply swap the controllers, putting the North Cavity controllers on the South Cavity and vice versa.  We did this, and observed no change in the noise levels of either cavity.  All four controllers give us a nice, low noise level on the South Cavity and a fairly high level on the North, so we conclude that controller noise is not the problem in the
North Cavity.

Our models suggest that the noise level in the South Cavity may already be low enough to observe Braginsky noise in Sapphire mirrors, but we are still trying to reduce the noise level in our all-fused-silica interferometer in preparation for sapphire.  We would very much like to have the North Cavity's noise comparable to the South's, so that we might have two separate measures of displacement noise in sapphire.



Over winter break, we ran a 700 mW LightWave 126-1064-700 laser and an InnoLight Mephisto 800E laser near the center of their operating ranges, as indicated by the manufacturer's calibration sheet. The intensities of both lasers were measured with New Focus photodiodes, and recorded with a SR785 spectrum analyzer. No lenses or mirrors were between the lasers and the photodiodes. Consequently, the voltages measured in the two channels are slightly different, because of the different spot sizes of the two beams.

Before and after the 3-week period, we recorded time series and frequency spectra of both lasers. At the beginning, the Mephisto laser appeared to have slightly less intensity noise. At the end, the LightWave laser was dead, and the Mephisto laser looked much as it had before.


LASTI (Zucker)



LASTI (Bayer, Fritschel, Goda, Harry, Laliberty, MacInnis, Mason, Mason, Miller, Mittleman, Ottaway, Phinney, Rollins, Shoemaker, Zucker)


VACUUM ENVELOPE: Still leak checking after R&R of the leaking bellows seal last week.

HYDRAULIC ACTUATORS: (10) Fabrication drawings have been completed. (2) are partially completed, waiting for final results of FEA.

A finite element model of the weldment which sits on the pier holding the springs and actuators has been completed. A modal and deflection analysis is running. Results should be available thursday.

CDS/DAQ/GDS: No problems to report.

PSL: This week we continued with our efforts to shake down the FSS servo. Jamie has started to modify the spare FSS board to test candidate design improvements. Once the vacuum system leak check is completed we will commence locking the one meter test cavity.


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)



Weekly Physics meeting: Luca Matone talked about "Calibration procedures: e2e and observations" focussing on DC calibrations of ITMs using two methods: (i) counting of fringes (ii) toggling control loop signals. Comparison with results using e2e model was presented.  Details available at http://www.ligo.caltech.edu/~e2e

Lazzarini note: I thought it was an excellent exposition in how Luca has been reconciling measurement with models.

Locking LIGO in presence of mode mismatch: (Biplab) Using the E2E model of LIGO 2km with all its spatial mode mismatches (coming from the as-built, measured differences in radii of curvature of the corresponding mirrors in two arms and from recycling mirror curvature designed to be matching in the hot state but not in cold) it was shown that  model would achieve lock.

LIGO I simulation system: (Matt) Working on the LIGO1 simulation system (upgrade from Han2k). I have decided upon and implemented a top level design and am currently working on subsystem design.

LSC characterization: (Luca) Prepared and verified a new version of Han2kControl.box, compatible to Matt's original Han2k model, containing all the new filtering measured in the past few months.

Mechanical Simulation: (Virginio)

Code Maintenance: (Ed Maros) Started work on porting e2e code to GCC 3.0.3. This is preliminary work.

Alfi: (Bruce) Implementing various menu item options.

LIGO Data Analysis System



Software Systems (Blackburn)

A job submission summary has now been added to the controlMonitorAPI. It has a graphical interface which includes the statistics (number submited, number failed) and a graph of the GPS time vs the total jobs submitted in the user specified time interval for any LDAS user (including all). It even has color coding, showing the jobs that failed on the graph in red along the total curve.

The problem reported during the engineering run in the metadataAPI whereby slave interpreters were being killed by users without properly removing the threads within the slave interpreter has been fixed.

The issue of having more than 5 pending socket connections for the server in the eventMonitorAPI which was causing some wrapperAPI jobs to terminate has been resolved by adding more servers to the eventMonitorAPI and by adding several re-tries to the wrapperAPI to increase robustness.

Work continues on the separation of the disk caching functionality found in the frameAPI for previous releases into the new separated diskCacheAPI. Some minor testing has begun, but there is still a weeks worth of effort here.

The problem that was discovered during the engineering run whereby the job resultant subdirectories were filling up and not allowing any more results to be written to disk has been fixed in the development version of LDAS by implementing a hierarchical subdirectory naming system.

LDAS now compiles with the new GCC 3.0.3 compiler, but it has yet to be tested with this new build. This effort began today with pressing urgency on a one CPU Linux Box. Hope to know how well it does by tomorrow.

Several modifications to the rules for building packages used by LDAS have been made to make LDAS more inline with the more ANSI/ISO compliant compiler.

Made several modifications to LDAS to support Beowulf clusters with 100 or more nodes.

Hardware Systems (Anderson)

Caltech:

(Dan Kozak)

(Al Wilson) (Stuart Anderson)

Met with Sun Microsystems to discuss there near-term plans for new Fiber Channel equipment. The most important update is that the firmware to support the desired LDAS storage network topology is now available.

Ingesting E7 data into the HPSS archive.

Wasted a day due to a "planned" power outage in Millikan library tracking down a bug in the Solaris network table management on multi-homed machines.

Replicated a few hours of "standard" E6 and E7 test data to all Lab LDAS systems and working to make it available on LSC LDAS systems as well.

Investigated and reported bug to gcc related to Solaris file I/O performance degradation in the latest version of the compiler (gcc-3.0.3).

Installed new AMD Athlon 1900+ Linux machine to evaluate next generation platforms for LDAS.

Enabled web access to all CVS software repositories on ldas-sw, i.e., CDS, GDS, E2E, DSO, as well as the already accessable LDAS. To browse see http://www.ldas-sw.ligo.caltech.edu/cvsweb.cgi.

MIT:

(Keith Bayer)

Livingston:

(Igor Yakushin)

(Shannon Roddy)

Ordered the UPS for the SF880.

The Cybernetics tape library came back from repairs and is in the Mass Storage Room.  After the run is over, I will reinstall the unit, return the GC unit to decatur, and test the LDAS unit.

Igor and I installed the UPS for the new SF880 in the Mass Storage room.

Hanford:

(Greg Mendell)

1) Two shipments of tapes with the LHO full frame E7 data have been or are about to be sent to Caltech.  These contain about the first 250 hours of the run.

2) The process writing data from the fb3 framebuilder T3 disk cache to tape at LHO is falling behind.  It will need to be switched to write data from the archived E7 T3 disk cache to tape to get the last 3-4 days of the run.  This is not a major problem for this run, and no data will be lost.  However, the disk to tape write speed will need to be increased for future runs.  The archiving of E7 data to tape is keeping up with the data at LLO.

3) The copying of E7 data from the framebuilders' disk cache to the archived E7 T3 disk cache has proceeded without problems since the beginning of the run.

4) Worked two shifts in the control room.

5) Performed daily monitoring of the ldas systems at LHO and assisted in solving problems as they arose.

Data Analysis Activities: (Lazzarini)

Worked through the properties of the LSC servo in order to understand (with Luca's help) the conceptual foundation of the calibration procedure.

Worked on software to automate the discovery of clean locked segments, by scanning the 'conlog' logs.  This function will be added to the conlog web interface, so that it can be done on demand.  (It was done manually by scientists on shift during the E7 run.)

Operations support activities: (Lazzarini)

General Computing (Wallace)


MIT: (Keith) Livingston:

(Tom)

(Shannon) Hanford: (Christine) CIT:

(Veronica)

(Mike) To download the VNC software without installing VRVS here is the URL http://www.uk.research.att.com/vnc/ then precede to download.

To setup a server all you have to do is click on the icon that is located on your tool bar
(WinVNC: Current User Properties) will open; then just put a check mark in the (Accept Socket Connections)
(Display Number) you can limit the amount of connections or put a check mark in the (auto) option.
(password:) you must put in a password, make sure you disable remote keyboard & pointer remote and local.

(UPDATE Handling) I have everything checked, this seems to work for me; you can play with these settings if you like.
APPLY settings and click OKAY.
Done deal.

(Lisa) (Larry)

LIGO II/Advanced R&D (Sanders)


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

Silicate Bonding: We performed an experiment to observe the stress distribution on the bonded surface of a prism (ear) using a polariscope.  We silicate bonded a prism, made from an old Glasgow design, to a flat polished on a fused silica disk. Welded fibers to the prism and suspended weights to the fibers.  One of the fibers broke while being loaded.  With the other fiber loaded with a few grams, we saw the stress distribution on the bond.  As the weight increased, we observed several stress points where stress was expected from the design analysis.  A few seconds after reaching 2.5 kg of load, one part of the prism's leg broke matching the shape of the stress distribution seen at the time.  The experiment will be repeated again to be able to determine if the leg broke because of stress induced during welding fibers, a flaw on the glass or a design problem.

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

CSI:  Gari B and I visited Crystal Systems on 16 Jan to review the status of the sapphire development. The most significant development is that they have produced the first sapphire boule from their 15" diameter furnace (ie, the boule is 15" diam). Their intent is to develop production capability of this size, from which the AdLIGO test masses would be made (their current largest production size is 13.5" diam, a bit too small for our desired 40kg test masses). They haven't yet done any quality characterization of this piece, but at least they were able to produce this size without cracks/fracture in the bulk. They plan on growing 4-5 more 'experimental' boules of this size over the next ~6 months to tune the process. We agreed that they should grow these pieces along the a-axis, as our limited data indicate its homogeneity is better than m-axis material (the first boule is actually m-axis, but the second one underway is a-axis). There are no real developments on their end regarding absorption (they are waiting for samples from Stanford).

>From: Phil Willems <willems@ligo.caltech.edu>

Fused silica fiber research: We have submitted for LSC review a paper entitled, "Investigations of the Dynamics and Mechanical Dissipation of a Fused Silica Suspension," summarizing the last two years of such research at Caltech.  The main results we report are:

The coauthors of this paper are Virginio Sannibale, Valery Mitrofanov, Phil Willems, and Jaap Weel.  Jaap is a SURF student who is seeing his work published, and who just might transfer to Caltech thanks to the experience.

Based in part on the work in this paper, we are composing a database of fused silica properties relevant to thermal noise, in an effort to unify the ranges of values we currently use.  This will be a joint effort of Moscow, Glasgow, Syracuse, and Caltech, and we intend to present our findings at the 2002 Livingston LSC meeting.  All those with data to share please contact Phil Willems.

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

No report.

>From: Rich Abbott <abbott@ligo.caltech.edu>

>From: Janeen Hazel Romie <romie_j@ligo.caltech.edu>

No report.

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

No report.


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