Weekly Report for Week Ending May 30, 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  June 3, 2002:

 (Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

Executive Committee only 11:30 - noon   Topics:

Special Items:


Special Announcements:


Weekly Report Highlights

(Rai Weiss)

As a result of work at both Hanford (on the two-kilometer interferometer) and Livingston (four-kilometer interferometer) we achieved strain sensitivities during the last week a little better than that measured on the 40-meter system in 1994. This is the case over the entire gravitational wave band, from 100 Hz toward the higher frequencies. The sensitivity is better than has been achieved with any previous broad band detector.  And two of them, that is really a first.  Two interferometers at separated sites support coincidence techniques for the gravitational wave search.

Daniel Sigg and Rana Adhikari are the recent heroes standing on the shoulders of a lot of other people.


LSC Issues (Weiss)


no report.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



LIGO Weekly Site Telecon (Lindquist)

There was a site teleconference held on Thursday, May 30, 2002.  The following items were discussed:

Status of Commissioning: (See below.)

Action 106: Outfitting and Populating the Building at Livingston, Ed is planning a trip to Landover, MD (GSA collection point) on June 11 to check out some furniture.  The plan for population at Livingston has not been finalized; still looking at some options.  Gerry is on route to Pasadena and will be here next week.

Time line for spend out of construction funds: Gerry has identified up to $325,000 to be requested for completing the new facilities.  Some of this will be for outfitting the laboratory for MRE effort.  Air conditioning and fire suppression for LDAS room also included.  We have not yet seen a change request.  Phil to help Gerry prepare a Change Request next week.  Money for outfitting labs basically to be provided at time needed, especially since needs cannot be known at this time.

Livingston Staging Building: working on punch list (75 - 80 percent complete).  Some will drag on.

Building at Hanford:  Reported progress is good.  Getting PO today for audio/visual equipment.  $80,000 purchase order will include two projectors.

Property:  Ed is looking for 1) a good street sweeper for Otto, and 2) a small Bobcat for Gerry, kind of tough right now.

The list of current actions revised to reflect the status of open actions assigned through May 30, 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

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.

COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, 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>

CONSTRUCTION:

OPERATIONS:

SUPPORT (Baldon, Torres, Lloyd, Tischler)

>Irene Baldon

>Dorothy Lloyd >Rita Torres >From: Ryan Tischler <rtischle@ligo.caltech.edu>

Advanced LIGO (Frey)

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

Progress Period from 05.24 to 05.30

Accomplishments:

Schedule 05.31 to 06.06:

Reports (Lindquist)

August 1 we are scheduled to submit an annual work plan to the NSF for LIGO FY 2003 Operations.  We are modifying the first draft budget for FY 2003 based on the current staffing plan and information provided by group leads.



Change Control/Contingency (Lindquist)

The following additional change request has been submitted:

We are expecting an additional change request from G. Stapfer for effort to complete Livingston building.


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

LIGO Hanford Observatory (LHO) Operations (Raab)



Summary of Commissioning Activities at LIGO Hanford Observatory


(see elog for details - if it's not in the elog, it didn't happen...)

4k IFO investigations



Lots of activity to bring IFO back after software changes. Unfortunately this was complicated by a number of hardware problems that lost a lot of time. We have now been able to get all cavities to resonate separately and are setting up to test full locking as this is written. We still have a filter anomaly tofix in the software. Glitches in the PSL were traced to a range problem in the shunt actuator. Flavio is now working with Rick to get intensity stabilization working.

2k IFO investigations



Landry has released the autocalibration software so we can now easily (and more frequently) produce calibrated spectra to track stability. The spectra have been remarkably stable in the region of a few hundred Hz with amplitude falling like f-3 until Sunday night, May 26, when a change in loopology had the unintended effect of dropping this low-frequency noise by about a factor of 4. The background is that operation in common mode with higher ASPD light levels had improved the high frequency end of the spectrum as expected by getting us above dark noise. But the change was accompanied by a dramatic vertical bouncing of the spots on the end mirrors, caused by position to pitch coupling of ETMs with the large common mode drive. When the "bounce" was large, we would hear burst noise in the DARM_CTRL loop. In an attempt to alleviate this problem, Daniel tried to remove the CARM_CTRL drive to the ETMs by bringing all common mode feedback back to the input optics. The change was successful, and also caused changes in the displacement spectra, dropping the noise at low frequencies, but raising the noise around 1 kHz. This is not understood, which is bad. But it has produced the first warm clue on the origin of the low-f noise that we have had in long time. Investigation of this continues. The LSC front end code was also updated to utilize the new timing cards and reduce polling noise in the ADC.

FACILITIES



The siding, with exception of the stainless steel panels is installed. The Stainless steel panels are ordered and will be here in a few weeks. HVAC, plumbing, electrical and insulation work is ongoing. The outside area was seeded and mulched to keep the wind from blowing the sand away. Additional landscaping will be done in September when the building contract is complete.


LIGO Livingston Observatory (LLO) Operations (Coles)



Higher power on the anti-symmetric photodetector and further refinements in the common mode servo have resulted in strain sensitivity improvements on the interferometer sufficient to be somewhat better than the strain performance of the 40 meter system in 1994. The improvements have been made in the band above 100Hz. Preliminary measurements of the amplitude spectrum of the anti-symmetric error signal, the signal that contains the gravitational wave information, exhibits Gaussian behaviour to approximately 5 sigma in a data stream with high pass filtering above 100 Hz. Command scripts have been written to engage the common mode servo through the many gain and filter changes required to bring it into operation. A script has also been written to increase the light power incident on the antisymmetric photo detector which increases the shutter transmission while reducing the digital gain in the DARM control loop. An important finding has been that the alignment servo using wavefront sensor 1 keeps the ASI signal (which is not controlled directly by any servo) bounded so that the saturation does not occur in the RF amplifiers as the light power is increased. Work has been done in closing the servo loop from the wavefront sensor at the symmetric port (WFS2). The pitch servo on the recycling mirror works while the yaw servo does not. We have traced the problem to the software.

We will freeze changes in the hardware after Friday June 7 to prepare for the S1 run at the end of the month. The improvements we anticipate before S1, other than clean up and improvements in operating procedures, are:

Active Seismic Isolation

We've redrawn ~80% the Stanford model of the Hydraulic Actuator on LIGO templates and issued DCC numbers. Detail checking and tolerancing are in progress. Five machine shops have been contacted, which are preparing preliminary estimates for the production of 12 sets for the LASTI instillation. Most shops are slow right now and several can begin work immediately. A quantity of Stanford's modified nozzles was ordered 5/21, ~ 3 wk delivery. Ordered 12 DPY2S Parker differential proportional valves on 5/28, ~ 1 mo delivery (These are the standard valves. Special testing and calibration using our procedure will increase the price and delay delivery). Provided Hyspan with drawings for the revised details of the weld-assist/shield rings on 5/28. They will reply soon with a price for the LASTI units. Returned to Stanford Wednesday and am meeting with Dennis and the group here today and tomorrow. Goal here is to learn more of the test and qualification procedure for the valve, and to document the procedure for LIGO. (Jonathan)

I have made arrangements to start the heat treat-coating-joining process for the machined spring pathfinder. I will meet with Metal improvement Inc. tomorrow (Friday) to have them start the heat treat efforts and discuss with them a greater quantity of springs. I have also made arrangements with the LSU Civil Engineering department Materials lab to perform the materials test on the machined spring. I will meet with Dr. Vojyadtis to show him the pathfinder before I bring it to Lafayette to have it heat-treated I along with Jonathan Kern have been working to get the pre-isolator hydraulic actuator fabricated in time to support the current schedule. Preliminary outlook looks promising, and we hope to be able to down select a fabricator and start cutting by next week. I am also looking very closely at ways to assemble and properly tension the springs, and I have come up with a design that piggy backs the current design that uses a load cell to give proper tension indication. I have been assessing potential interferences with the digital model to help ensure an expedient installation . The work continues on implementing the pre-isolator design into the BSC and HAM stacks then utilizing techniques to successfully produce a finite element model that reflects the physical model. This is still part of the effort to refine the 6x6 stiffness matrix that I have been working on. (Marcel)

LDAS

Performing extensive tests for metadatabase replication from sites.
Tested various 2,3 node configurations.

RET Program

Two teachers will participate in this summer's RET program. One is a returning teacher and the other is from the New Orleans Public Schools.


SCIENCE & ENGINEERING SUPPORT (Coyne)


Seismic Upgrade Project

Hydraulic External Pre-Isolation (HEPI)
Electro-Magnetic External Pre-Isolator (MEPI)
Greg Harry is measuring the magnetic field strength generated by the electro-magnetic actuators as part of an effort to determine the coupling factor to the test mass magnets and assure ourselves that it is acceptable.

CDS Hardware

Rich Abbott and Peter King reporting
Installed the VME based intensity servo board and newly designed differential photo-detectors (designed by Ben Abbott) at LLO last week.  After getting everything installed, the system was quickly put online by Flavio, Peter King and Rich A.  The suppressed RIN level was measured "outside the loop" to be about 2 x 10-7 at about 150 Hz rising to 3.0 x 10-7 at 10 kHz.  The suppression was consistent with the available loop gain in the servo.  An attempt was made to close the outer loop, but due to large MC power fluctuations resulting from the daytime ground motion, the loop had insufficient dynamic range.  The PSL generic DAQ interface was re-wired to accommodate the signals available from the intensity servo.  Whilst the signals were the same, namely the servo error point and the actuator signal, where the signals came from on the P2 connector was different.

Flavio continued on to LHO for installation on both interferometers there this week.

Sander Liu

LEMO Antialiasing Filter Chassis: Prepared DCN No.E020580 to correct output signal polarity for channels 3, 19 and 32 on new builds using PCB D990147 Rev B circuit boards.

Seismic Signal Processor:

PSL

PeterKing
Rack mountable power supplies for the PSL rack arrived this week and will be installed.  These will replace the 5 units that are delicately balanced already there.

Optics Analysis

Erika D’Ambrosio
Sadly it took a considerable amount of time for me and Ray Beausoleil to make the paper on Melody successfully submitted because the fonts and the versions embedded for the compilation of our draft failed to work when uploaded on the electronic system that was not able to generate any postscript file. Anyway we succeeded at last! The other paper I am having troubles with is the one on the sidebands imbalance. I generated much more graphs trying to include only those that are useful for the "theme" that is making clear statements on the physical causes for the imbalance.

I am still interested in understanding the coupling with the oscillator phase noise and I talked with Guido Mueller who happened to be in Caltech. He looked at my analytical calculations and said he is going to spend some time on this problem. I started to think on how to measure the "oscillator phase noise" since it should be possible by inducing an artificial time-delay. Those measurements have not been done and in the Ligo documents I only found the "required" values.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang
OTF Lab: continuing measurements on both cavities everyday.

Cavity#1: Ring down is 24.7742 microseconds and its Beat frequency is 86.0815 MHz.

Cavity #2 with mineral oil test sample in it: Ring Down is 31.2098 microseconds. Its Beat Frequency is 74.4012 MHz.
In cavity 2 containing the mineral oil sample, the surface absorption keeps at a saturated level of ~2ppm, and its ringdown measurements show a big fluctuation, which is probably due to a big change of the room temperature since the cavity system is very close to the air condition port.

We have this situation with the room temperature as it changes overnight about 20F.  This causes the cavity to go out of lock. We are monitoring the room temperature daily.

P.King made good suggestion as to have control with the computer the slow actuator voltage of the NPRO to compensate temperature changes in the cavity.  We will look into this possibility (Lab view program).

I have sent the NPRO S/N 256 (Not functional from RSE LAB/CIT) to Lightwave for repair.  This laser is only 100mw of power. I would like to use this laser for the transmission test set up once it is repaired and the new NPRO S/N 415 to be used for the third contamination cavity.
Misc Tasks: 12.5 MHZ, 5watts power amplifier are being fixed.  Placed orders, etc.

40 Meter Interferometer (Weinstein)


Suspended mass mode cleaner (Ugolini, Miyakawa, Vass):

Suspension Controllers and Mode Cleaner length controls (B. Abbott, Heefner, Taylor, Ugolini, Miyakawa): DAQ (Rolf, Ivanov): There haven't been any DAQ frame logging interruptions in the last week, ever since Alex rebuilt the RAID array.

PSL:

Optics (Billingsley, Armandula): GariLynn, Helena, and Alan met to go over the status of the polished core optics. Most optics have visible scratches, but mostly within tolerance. A scratch in the central 10 mm of SRM01 brings it out of tolerance, and we discussed sending it back to CSIRO to polish it out before coating. Since then, GariLynn has determined that the scratch is very small (20 um by 2 um), so we will live with it. All core optics go out for polishing by REO on July 8, and Helena will be there to observe. It will take approximately 3 weeks to coat all the parts.

Computing:

STACIS seismic isolation system (Ugolini): Two bad STACIS isolators were shipped back to TMC for repair. They have been repaired, and have been shipped back to us. We expect them any day now.

Facilities and vacuum envelope (Vass, Jones):

South Annex Bake Ovens (Taylor, Cardenas):

Thermal Noise Interferometer (Libbrecht)



This week we began looking at ways to reduce the electronic noise in the TNI. As a first step, we looked at where the electronic noise came from in the current configuration. As it turns out, most of our noise comes from the first SR560 in our servo filter, and with our present setup there is no way to substantially reduce this noise.

Our spec requires that the input noise of our servo filter be 30nV/rHz or less to give an equivalent length noise of 10-19 m/rHz. Our chain of passive circuits and SR560's, while allowing us to lock during the day, does not meet this requirement. Jay Heefner offered some advice on how to achieve this in a custom-built circuit, and we have started, with his help, designing a unit to replace our SR560-based prototype electronics.

We also measured the noise in our active notch filters directly and got approximately 5nV/rHz, punctuated by a number of peaks at 60Hz and its harmonics. Fortunately, these filters can meet our noise requirements and can be retained when we replace the rest of the servo filters. We are working on ways to eliminate the 60Hz harmonics.

Kyle Barbary, the first TNI SURF student for this summer, started work this week.


LASTI (Zucker)



LASTI (MacInnis, Mason, Mittleman, Ottaway, Rollins, Shoemaker, Zucker)

No report.


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)

SimLIGO


 (Matt) Continuing work on the common mode servo.

Mechanical simulation



(Virginio) FFT and E2E for Mode Mismatch


(Biplab)

E2E runs (including upto 4th order modes) and FFT runs match each other quite well for carrier fields in various cases of mismatch. For sidebands, the order of magnitude of power in various modes agree in most cases.  One important point is 06 or 60 power comes out to be more than 04 or 40 in FFT. Trying to understand if this is a real physical effect or some artefact.

Alfi



(Bruce) (Melody) LIGO Data Analysis System

Software Systems (Blackburn)

Work continues on improving the reliability of the LDAS software reliability in preparation for this next release. The phenomenal performance from three weeks ago has yet to be reproduced as needed functionality has introduced stability issues along the way. At one point this week the system was approximately a thousand times less stable. We have worked very hard and almost recovered two of those three orders of magnitude. A primary source of trouble has been in the form of memory leaks introduced in new code that wasn't adequately unit tested before being committed to the system repository. Everyone is now more aware of the importance of unit testing and progress is once again being made.

A new interface to the data socket allowing "linger" parameters to be set on LDAS APIs that write through the client socket was incorrectly being used.  This has now been removed from client side writers.  New log files were added to the system to allow graphically monitoring of memory usage for each of the APIs. The recent rash of memory leaks discovered in the system necessitated this.

The job status web pages now capture the particular dynamically loaded shared object being loaded in the dataPipeline.

We've had a rather large number of core files to contend with from the system this week. These were primarily due to the large memory leaks and the incorrect usage of the linger option in the client side data sockets. It was also discovered that the objectSpace C++ socket library was not recompiled when we rebuilt our C++ compiler on May 9th. Several problems with exceptions were seen in these core files which lead us to this discovery.  Since the recompile, this problem has not been seen.

Work continues on the development of the cgi web pages for managing LSC requests for LDAS usernames and passwords. The interface now communicates with LDAS using various security steps (including encryption techniques).  The ParaSoft company has finally come through with our new license for the Insure++ software development tool we use for debugging various aspects of our C++ code.

Hardware Systems (Anderson)

Caltech



(Dan Kozak) (Al Wilson) MIT


(Keith Bayer) Livingston


(Igor Yakushin) Hanford


(Greg Mendell) Data Analysis Activities (Lazzarini)

Mendell:

Shawhan: Lazzarini: General Computing (Wallace)

MIT:



(Keith) Livingston:


(Shannon) Hanford:


(Christine) (Larry) CIT:


(Lisa) (Veronica) (Mike) (Larry)

LIGO II/Advanced R&D (Sanders)


>From: Janeen Romie

AdLIGO Suspensions

Nothing to report.



>From: ctorrie

Advanced LIGO Suspensions

Mode Cleaner:  Working on the comments collected from both LIGO and GEO on the drawings. Larry Jones is helping to implement new ideas to some of the designs. Russell Jones and I are trying to migrate all of the drawings to SOLIDWORKS and incorporate the new templates and notation. (Previously the drawings were a mixture of AutoCAD and SOLIDWORKS.)

Prototypes for SURFS:  Workshop has almost completed the parts that are required for the tests planned for the 2 SURF students.  I accepted the majority of these parts this week and have checked through them.

Coil Assembly:  Russell Jones and I have finished the drawings and assembly for the coil former and clamp. These have now been sent to get 3 sets made at a local machine shop in Glasgow.  The plan is to follow these 3 assemblies through to the point where they have the LED, PD's, cabling etc.. installed.


>From: Riccardo DeSalvo (prepared by Hareem Tariq)

Mike

Hareem Szabi, Alessandro, Akiteru and Riccardo, in Elba.

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