Weekly Report for Week Ending December 11, 2003



 Exec. Comm. Agenda
Highlights
LSC
Administration
Hanford Observatory
Livingston Observatory
MIT
Caltech
Detector
40 Meter
TNI
LASTI
Data Analysis
Adv. LIGO Development
Past Weekly Reports

The LIGO Executive Committee Agenda for Monday  December 15, 2003 will be:

(Meeting time: 10:30 am Pacific Time)
The meeting Monday, December 15, 2003 will be a Staffing Committee meeting.  There will be no Executive Committee meeting scheduled.


Special Announcements:


Weekly Report Highlights


LSC Issues (Saulson)


No report.

LIGO I Construction/LIGO Laboratory Administration (Lindquist)


LIGO Weekly Site Telecon (Lindquist)

There was no site teleconference scheduled on Thursday, December 11, 2003.
The list of current actions revised to reflect the status of open actions assigned through December 4, 2003 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
Packaged and shipped PAC 15 binders to Hanford for Meeting
12/11/03 Packages Faxes
In 22 38
Out 19 28

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.


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

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

Press here for ACCOUNTS PAYABLE HISTORY DATA .

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

From: Gina Salone <gsalone@ligo.caltech.edu> From: Florence Kaufman <fkaufman@ligo.caltech.edu>
SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

LSC MOUs / Attachment Updates and Program Reports

ACIGA:
Draft-Attach. B for 08-15-03 to 02-15-04 / in LIGO review / Shoemaker
Draft-Attach. B for 08-15-03 to 02-15-04 / in process for web posting
Attach. C for 08-15-03 to 02-15-04 / in LIGO review / Barish
Draft-Attach. C for 08-15-03 to 02-15-04 / in process for web posting
Attach. D for 08-15-03 to 02-15-04 / in LIGO review / Barish
Draft-Attach. D for 08-15-03 to 02-15-04 / in process for web posting
Prog. report against Attach. B / in process for web posting
Prog. report against Attach. C / in process for web posting
Balearic:
Attach. A for 02-15-03 to 08-15-03 / to Prof. Sintes for signature
Attach. A for 08-15-03 to 02-15-04 / in LIGO review / Lazzarini
Draft-Attach. A for 08-15-03 to 02-15-04 / in process for web posting
Attach. Z for 08-15-03 to 02-15-04 / to Prof. Sintes for signature
Carleton:
Attach. A for 02-15-03 to 08-15-03 / in process for web posting
Attach. Z for 02-15-03 to 08-15-03 / in process for web posting
Attach. A for 08-15-03 to 02-15-04 / in LIGO review / Barish
Attach. Z for 02-15-03 to 08-15-03 / in process for web posting
Attach. Z for 08-15-03 to 02-15-04 / in process for web posting
Caltech Experimental Gravitational-Physics Group:
Attach. A for 02-15-03 to 02-15-04 / to Prof. Drever for sign-off
Attach. B for 02-15-03 to 02-15-04 / to Prof. Drever for sign-offf
Attach. Z for 02-15-03 to 02-15-04 / to Prof. Drever for sign-off
Institute of Applied Physics (IAP):
Attach. C for 08-15-03 to 02-15-04 / to Dr. Sergeev for sign-off
Attach. Z for 08-15-03 to 02-15-04 / to Dr. Sergeev for sign-off
Inter-University Centre for Astronomy and Astrophysics (IUCAA):
Attach. A for 02-15-03 to 08-15-03 / to Prof. Dhurandhar for sign-off
Attach. A for 08-15-03 to 02-15-04 / to Prof. Dhurandhar for sign-off
Attach. Z for 02-15-03 to 08-15-03 / to Prof. Dhurandhar for sign-off
Attach. Z for 08-15-03 to 02-15-04 / to Prof. Dhurandhar for sign-off
 
Loyola:
Attach. A for 02-15-03 to 08-15-03 / to Prof. McHugh for sign-off
Attach. A for 08-15-03 to 02-15-04 / in LIGO review / Lazzarini
Attach. Z for 08-15-03 to 02-15-04 / to Prof. McHugh for sign-off
Northwestern:
Draft-Attach. A for 02-15-03 to 08-15-03 / in process for web posting
Draft-Attach. A for 02-15-03 to 08-15-03 / in LIGO review / Lazzarini
Draft-Attach. A for 08-15-03 to 02-15-04 / in process for web posting
Draft-Attach. A for 08-15-03 to 02-15-04 / in LIGO review / Lazzarini and Riles
Draft-Attach. Z for 02-15-03 to 08-15-03 / in process for web posting
Draft-Attach. Z for 08-15-03 to 02-15-04 / in process for web posting
Prog. Report against Attach. A of February 15, 2003 / in process for web posting
Prog. Report against Attach. A of August 15, 2003 / / in process for web posting
 
Southeastern Louisiana Univ.:
Attach. A for 02-15-03 to 08-15-03 / to Prof. Yoshida for sign-off
Attach. A for 08-15-03 to 02-15-04 / to Prof. Yoshida for sign-off
Univ. of Florida:
Attach. A for 08-15-03 to 02-15-04 / in LIGO review / Lazzarini
Attach. C for 08-15-03 to 02-15-04 / to Prof. Mitselmakher for sign-off
Attach. D for 08-15-03 to 02-15-04 / to Prof. Mitselmakher for sign-off
Attach. Z for 08-15-03 to 02-15-04 / to Prof. Mitselmakher for sign-off
Subcontracts:
From: Ed Jasnow <jasnow@ligo.caltech.edu>

SUPPORT (Baldon, Lloyd, Tischler)

>Irene Baldon

PLEASE NOTE:  This report covers a two (2) week period and includes a three (3) day trip to LHO to work with Terry Gunter and the Thanksgiving Holiday.
>Dorothy Lloyd >From: Ryan Tischler <rtischle@ligo.caltech.edu>

ADVANCED LIGO (Cost Schedule Control Systems) T. Frey
From: Thomas Frey <tfrey@ligo.caltech.edu>
 

Out of the office on 12/5 and 12/8.
 

 

For list of documents that are being used to develop Adv. LIGO Cost and Schedule, see http://www.ligo.caltech.edu/~tfrey/Cost_MTG_082002/
 

 

Continued development of a proposal for implementing Primavera Project Planner Enterprise.

Advanced LIGO Request
Cost Book Tool.
Development of the Advanced LIGO Project Controls Guidebook continues.

Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.


Reports (Lindquist)

The NSF caught up with the fact that we have yet to submit a final report for the Advanced R&D Grant (PHY-980158) when FastLane pointed the Knarly finger at LIGO and held up our FY 2004 funding.  We are working on it.  We may request some additional information from selected R&D task managers.

Reviews of the FY 2004 Operating budgets continue.


Change Control/Contingency (Lindquist)

The following change requests are open.
 
CR-030015 FY 2003 Livingston Observatory Detector Maintenance Expenses (Increment) R. Wooley July 14, 2003
CR-030016 Hanford Facilities 2.2--Divide the Large Equipment Access to Facilitate Movement of Large Items (currently assigned to FY 2004 liens list) J. Worden July 31, 2003


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

LIGO Hanford Observatory (LHO) and Interferometer Operations (Raab)


Summary of S3 Activities at LIGO Hanford Observatory  (compiled by M. Landry)

More conjecture about the microseism as an impediment to locking is given here.  Also in the same entry, a description is given of the clear correlation of lock losses and trucks passing on the bumpy route 10.  A follow-up report notes that, even if such truck passings don't unlock an ifo, up-conversion into the gw band is observed.  Seismic and wind impacts on locking are shown here.

After a testing phase, a GRB alarm is now running in the control room.  The diamond-shaped GRB widget now goes red on the site overview screen when notification of a GRB event is received.  The idea is to ensure that the IFOs remain in science mode if possible (e.g. no breaks for calibrations or injections, etc) for at least the hour following a GRB, in case there is some long-term GW activity associated with the burst.

Roughly 290 burst and inspiral waveforms were injected into H1 and H2.

The two day PAC15 meeting is underway at Hanford, 11-12 Dec.

DAQ

DAQ mysteries such as fb3 restarts and h1adcuex problems were observed.  Investigations into the low-bit flips (seen in data such as the 2k state vector and the 4k MC sensor channels) are ongoing: the DAQ controller cpu was vindicated.


LIGO Livingston Observatory (LLO) and Interferometer Operations (Zucker)


 
S3 (or "What doesn't kill you, makes you stronger..." )
 Logging activity close to LLO continues to prevent useful locking during daylight hours. We also lost about 3 full nights of the last week to high microseismic activity from storm-related wave action in the Gulf of Mexico. Equipment troubles of various kinds are credited with further reducing the L1 duty factor.We have redoubled efforts to debug the equipment problems, with a view toward recovering duty factor (weather permitting) and stabilizing noise for the remaining few weeks of the run. So far this push has flushed but some nasty bugs: Safety/security (Rich Riesen) Replaced faulty proximity detector on machine shop exterior door. No more false alarms.Eliminated minor safety hazards. 1) trip hazard.  2) electrical concern.   Site tour found no other safety concerns.Pre HEPI installation work:  Getting the Toyota forklift, Genie lift and class 100 trailer ready for the end station.  Scheduled annual crane inspections for units that did not get inspected last go around.  Ensuring that "in chamber" and "class 100 area" apparel is ready on demand.Finishing up with the GSA sale equipment.Installed computer and printer in shipping & receiving to better facilitate contacting recipients of received packages, scheduling pick-ups, printing UPS and Fedex shipping labels.
S3 and detector optimization (V. Frolov)
 I worked on diagonalization of the test mass coil actuators. The coil drives were tuned to minimize the contribution of the angular drives to the ifo darm response. In the process of doing the tunning I found that three coils on the ITMX were not switched from the acquire state(high noise high dynamic range) to the run state(low noise) due to the undervoltage of the switching circuit.
HPLF, S3 Detector Studies, IO Faraday Upgrade (R. Amin)
 HPLF: No outstanding reports, except. Three weeks ago, US Laser misplaced our purchase order for a high power laser shutter ordered earlier in November. Two weeks ago LLO contacted them to both remind them of our purchase and reorder the product (thank you Bonnie!).  The shutter is due to arrive this week or early next week.Lock Loss: With respect to the growing interest in lock losses of the L1 detector, I have been compiling lock loss time series data for lock breaks that occur for both known and unknown reasons.  Last week I sorted through several lock loss data in hopes to find error signals that herald the onset of detector failure or mode cleaner failure.  So far data collected has been pointing towards the PSL and mode cleaner. However, enticing artifacts of data have generated inadequate evidence due to nonuniform sampling rates in the PSL.Faraday Isolator Upgrade: The proposal to replace the current Faraday isolator is nearing completion.  Basic designs, cost analysis, vacuum incursion plans, and a second draft proposal are complete.  Stray field analysis models have been constructed based on LIGO tech document LIGO_T970149-00-D by Sanichiro Yoshida et al and  are being debugged.  A final proposal is expected to be delivered by early next week.
CDS software (C. Parameswariah)
 Documenting the software robots Investigated the causes of the Y End seismic noise cycling in the 10 - 30 Hz band. Traced it to the chiller.Found the ascaux processor was/got rebooted last night. Burt restore was missing. Fixed the channel values with a burt restore.
LDAS (Yakushin)
 LDAS admin:
1) Disabled 'Fast Load' option for the tape robot.
LDAS data analysis:
1) Working on line removal algorithm in waveburst.
2) Produced and tested sine-gaussian burst MDC frames.
General Computing (Roddy)
The latest news on the Gigabit connection to the observatory is that Bell South will be ready by Dec 18th.  LSU will be ready by Dec 22nd.  This means that the Gigabit will not happen till I return from vacation on Jan 7th.  At some point after that we should be ready to go live.  LSU is going to provide us with the new router and also the interface cards for our firewall.Did a fresh windows install on a machine to put in the shipping and receiving area.  The usual windows/office/norton/etc.  Beware of Service Pack 4.  After a fresh install of Windows, SP4 crashed the OS.  Had to start over again.Have unplugged a machine on the network which I believe is infected with a virus.  Have not had a chance to check and see which one yet, but I was getting alerts from one of the IDSs.Coordinated with Rich to send our old E3000 to sun to receive a trade in credit towards a 280R purchase.  The "machine formerly known as Sirius" is no longer with us.  It was basically unused for the last year anyway.  The machine is terribly slow now and I am surprised Sun was willing to give us any kind of trade in value.Trying to work with the software.caltech.edu folks and improve the reliability of the software downloads.  They seem to not be very interested in the fact that it is nearly impossible for us to download site licensed software at the observatory.Patched several linux boxes with the kernel/rsync/etc. security patches.Once again I had to track down some invoices from Dell.  This is always a headache.Mounted the LDAS shares on touro at Igor's request.  People are complaining that decatur is too slow.  However, touro is not necessarily supposed to be used for analysis work in this manner.  This is something that should be looked at in the future.  Decatur desperately needs to be upgraded to Solaris 9 after the run, but more importantly, the hardware is showing its age.  Ideally decatur needs to be upgraded to an SF880, but that is around $40k if I remember correctly.  I do not like the idea of hard mounting the LDAS nfs shares to multiple GC machines and some sort of better solution needs to be found.
Burst analysis & S3 detector support (K. Franzen)
S3 Data Quality (Wang)
 I checked the S3 data segments every day. The lock loss for  segment L1:239 ( 754356088-754356736 ) was caused by a large seismic bump in the X end.
LLO Seismic Retrofit (Rich Abbott)
 Working exclusively on HEPI.  Ben has largely finished the assessment of the cabling and RFI feed through issues.  He anticipates being ready for the next task early next week.  I have sent out the first boards to the board house and ordered a bunch of parts.  I am working full bore on finishing more of the circuit boards.  Things are going well in general. Flavio is working on the pump speed controller to repackage it and incorporate a new isolation amplifier.Tasks completed so far include: Ordered all chassis parts and have started to receive them Ordered front panels for seismic interface chassis Ordered differential receiver boards for seismic interface chassis Am about 75% complete on the AA/Whitening board for the seismic interface chassis Ordered all parts for differential receiver board in seismic interface chassis Rear panel for VME crate RFI feed through has been designed and is ready to go to the panel house Excel has progressed well in completing the pump controller boxes and is almost complete.Much of the legwork to date allows rapid conclusion of the remaining tasks.  It takes a lot of time to research the proper parts, but once they are found and available the designs can progress much faster.
LLO Seismic retrofit (J. Kern)
 The shop manufacturing the machined parts for the hydraulic actuator ison target to deliver the balance of sets for 84 actuators this week.  Four actuators have been assembled and leak checked and 4 more are in assembly. These will be delivered to LLO next week for final assembly and shipment to MIT for installation on the BSC. HAM piers are completed and 4 will be shipped to MIT next week as well.  Springs are on track and 8 will be shipped to MIT before the 19th. 2 shops, manufacturing the HEPI housing and boot have fallen behind on production and it appears that the earliest we'll have parts to assemble for fit-check will be early January. A vendor has been selected to fabricate the pump station carts and assemble them.  Ken Mailand released drawings this afternoon and we'll begin fabrication immediately.  Ordered computer, daq cards and cables for the valve calibration pump cart.  Working on directing long-distance the assembly of the cart in Lafayette. Completed the mechanical Installation RFQ and statement of work.  Ed Jasnow is reviewing it. Marcel gave a familiarization to a few LLO staff members who will be involved in assembling and installing HEPI.

Detector/Technical Support (Coyne)


see also the Revision Technical Review Board (RTRB) status here

Seismic Upgrade Project

see also the LASTI report for HEPI experimental progress

Jonathan Kern reporting

Ken Mailand

CDS

see also 12/10 weekly CDS meeting minutes in the commissioning archives:

DMT

John Zweizig

With much invaluable assistance from Dan Kozak, Stuart Anderson and Al Wilson, I was able to bring up a cluster of 4 Linux nodes for use in offline detector characterization using the DMT. The cluster has access to the Caltech data archive and has all the necessary software for running DMT applications and monitors.

Several modifications to the DMT software were necessary to allow coexistence of the Linux code with the Solaris code in the same directory tree. I have also been making changes to the DMT software to facilitate its use in offline batch environment for e.g. trigger generation.

CDS Software

Rolf Bork reporting

12/4 report:

12/11 report:

CDS Hardware

Rich Abbott reporting

Working exclusively on HEPI.  Ben has largely finished the assessment of the cabling and RFI feed through issues.  He anticipates being ready for the next task early next week.  I have sent out the first boards to the board house and ordered a bunch of parts.  I am working full bore on finishing more of the circuit boards.  Things are going well in general.  Flavio is working on the pump speed controller to repackage it and incorporate a new isolation amplifier.

Tasks completed so far include:

Much of the legwork to date allows rapid conclusion of the remaining tasks.  It takes a lot of time to research the proper parts, but once they are found and available the designs can progress much faster.

Jay Heefner reporting

Suspension: Week before last, discovered an oscillation in the bypass path for the sus pd whitening interface board. It is caused by the choice of resistor values in the circuit. It is cured by putting a 10pF cap in the feedback path of the circuit, per the datasheet. A DCN will be issued to upgrade all boards in the system.

RFI Upgrade: Week before last, received a quote for the EMI racks that we recently tested. It is significantly lower than any quote received to date. Since the performance is essentially the same as the best rack tested, we (Rusyl Wooley) will order Knurr racks. A request for a revised quote (with relatively minor changes) has been made.

Thermal Compensation: Alex and I succeeded in getting EPICS to run on a linux pc with a Measurement Computing PCI-DAS-1002 IO card. The card has 8 differential analog inputs, 2 analog outputs, 16 binary inputs and 8 binary outputs. One card should support the controls required for each of the systems to installed at LHO.

Lower Noise Anti-Image Boards: Looking at design alternatives for an anti-image board to be used with our new low noise DACs.

Sander Liu

Working on the optical link for the GPS clock distribution system. (Note this will be needed for HEPI since we are imposing the new RFI standards and we need a different means of connection of the clock signal than the current 4-oin lemo connector.)

PSL

PeterKing

Week before last: I have been troubleshooting my high voltage amplifier that is to beused in the beam pointing control experiment.  A number of things were tested out on the circuit.  The monitor port is truly a monitor port now, without some excess noise that was experienced with the previous version. A broadband peak around 85 kHz was traced to a faulty regulator.  The high voltage offset was trimmed down to 100 uV and it was found that the offset trimming circuit added some noise to the output of the high voltage stage. This was remedied.  The output voltage noise is less than a factor of 2 off from a noise model.

Further to last weeks' high voltage amplifier troubleshooting, theamplifier was tested with a dummy load of 0.7 uF.  This mimics a PZT in the steering mirror mount.  The output current limit had to be increased in order to maintain a bandwidth of 500 Hz but the limitation seems to be the slew rate of the amplifier.  The output voltage noise of the amplifier remained the same.  Initially part of the problems were due ringing in the output of the function generator used in testing.  Full power testing also revealed a slew rate problem with the OP-37 based monitor.

A relatively minor change will be made to the laser enclosure in the PSL Lab to activate the panic button.  This is one of the outcomes of the recent lab safety inspection.

Active Thermal Compensation

see also report from Dave Ottaway (MIT)

Mike Smith

CO2 Telescope Projector:

Several re-designs of the thermal compensation optical bench were made to accommodate the availability of vendor components.  Parts are arriving at MIT for two thermal compensation optical bench assemblies. The parabolic mirrors from Edmund are delayed until 1/9/04. The CO2 laser periscope from Thorlabs will not arrive until 12/18/03. Most of the mechanical parts being made by CIT will arrive on 12/15; one bracket may be delayed until 12/16.  Phone and e-mail discussions are being held with Daniel S., Doug C., Ken M., Dave O., and Mike S. to finalize the installation configuration of the thermal compensation bench and periscope steering mirror at LHO 4K. Mike Smith has made travel arrangements to be at MIT during the week of 12/15 to assemble the CO2 laser mask projector. He will return to MIT the week of 1/12/04 for alignment and testing of the projector.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)

Contamination Cavity # 1

OTF Lab at Lauritsen ROOM 38

Cavity #3

Cavity #2


40 Meter Interferometer (Weinstein)


Commissioning (Miyakawa, Kawamura, Sakura):
Computing:
Electronics (B. Abbott, Heefner, Taylor, Nocera, Mageswaran)
PSL (Miyakawa, Kawamura, Abbott, Nocera):
Digital suspension controllers (Sakata, Goggin, B. Abbott, Heefner)
Optical sensing (Smith, Kawazoe):
South Annex Bake Ovens (Taylor):
AJW compiled an equipment budget for the 40m for FY04, with input from Jay, Steve, and Bob. There has been some re-alignment of the budget in order to relieve the pressure on the overall LIGO budget.


Thermal Noise Interferometer (Libbrecht)


This week we shipped the Sapphire masses back to REO for recoating, and we finished re-installing the fused-silica masses.  We are now in the process of aligning the South Arm Cavity (SAC). NAC was not removed and does not need realignment.

In other news, Dave Crooks has been helping us analyze our data on thermal noise in silica-tantala coatings on the fused-silica mirrors. Based on the most recent estimates of coating loss angle from ringdown measurements, our observed thermal noise falls below the minimum predicted noise level by about 30%. This difference is greater than the uncertainties in both the prediction and the measurement. Many thanks to Gregg Harry for pointing out that the initially-reported coating phi of 10-4, the initial reported result from the ringdown experiments and the one we used in our initial analysis, was in error. The corrected value, as reported in Penn, et al., Class. Quantum Grav. 20, 2917 (2003), is 5.2x10-4.


LASTI (Ottoway)


No report


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)

Nothing to report.

LIGO Data Analysis System

Software Systems (Blackburn)

a) a buffering issue in C++ that doesn't exist in C which can easily be coded around
b) the LDAS version was doing a deeper checksum, evaluating both the individual frame structure and the entire file; the VIRGO version only evaluated the file checksum
c) the LDAS version read the bytes twice when it is only needed to read once.
After correcting these three differences (evening the playing field),the two version are within 10% of each other.
(Peter Shawhan)A web page is being set up to provide information about database tables, such as the current table definitions and procedures for modifying themor adding new tables.  For now, at least, the URL is: http://www.ligo.caltech.edu/~pshawhan/dbwg/


Hardware Systems (Anderson)
 

Caltech
(Dan Kozak) (Hari Pulapaka) (Al Wilson) (Stuart Anderson) MIT(Keith Bayer) Hanford(Ben Johnson) Data Analysis Activities (Lazzarini)

(Greg Mendell)The first version of the StackSlide driver code to run under Condor and the Grid has been completed.  The code currently has been run on test data only.  Our next step is get set up to run the code on a Condor cluster.  The stackslide algorithm (which will be the same LAL code for the Condor/Grid and LDAS versions) needs to be refined and debugged, using test data and the injections into the S2/E10/S3 data.  This of course, will be an ongoing process over the next few weeks.(Peter Shawhan)

(Patrick Sutton) 
Lazzarini and Sutton travelled to Osaka and had extensive discussions with Nobuyuki Kanda of TAMA regarding the LIGO-TAMA joint burst search for S2.  Sutton is currently in Tokyo meeting with Masaki Ando, the TAMA leader for burst investigations.  They are planning the simulations and coincidence procedures necessary for combining LIGO and TAMA data.(Igor Yakushin) (Alan Weinstein) General Computing (Wallace)
MIT:(Keith) Livingston:(Shannon) (Yakushin) Hanford:(Christine) CIT:(Mike) (Veronica) (Lisa) (Bruce) (Larry)

Advanced LIGO and Supporting R&D (Shoemaker)


Seismic Isolation

From: Larry Jones <ljones@ligo.caltech.edu>

Advanced LIGO Seismic Structure (Larry Jones)

Actuator Testing and Redesign:

I met with BEI/Kimco representatives on 12/4 and showed them the reworked small actuator and told them of the thermal vacuum testing of the large actuator. We discussed each of the changes desired by LIGO to meet UHV requirements. They offered to supply anodized coupons and neodimium-iron magnets for RGA and contamination testing. They are working on a quote to provide design and prototyping of one unit each, which they feel will take 12 weeks. With LIGO testing required after that and 8-10 weeks estimated for producing units for the LIGO prototypes, we will be hard pressed to have units ready for the start of ASI's assembly phase. ASI's design review is currently scheduled for 3/16/04, and the BSC assembly fit check is scheduled to be complete on 6/9/04.

Position Sensor Probe Testing:

Cabling, connectors, epoxy and solder were received from ADE Technologies and the cabling has been cleaned to prepare it for a vacuum bake/RGA scan, which is scheduled for next week at the 40M lab. After that is complete, the cabling will be tested in the optical contamination cavity.

Suspension

From: JaneenRomie <romie_j@ligo.caltech.edu>

Continuing to work with CalumTorrie on getting more data points for the MC modal testing. This work will provide confidence in future fea work. Mike in the machine shop machined a set of stiffening plates that we bolted to the structure but there were not enough attachment points to provide enough stiffening. I'm sending new prints to Mike this week. He'll make up new plates and rework the structure. This stiffening approach may be used for the RM also.
Worked on some Solidworks/PDMWorks issues.Ongoing.
Working on schedule and labor estimates for the next few months.Reviewed Thomas's updated cost and labor data.

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

1) Eddy Current Dampers
Mark Barton and I are working with Mike Plissi, Caroline and Norna on a paper summarizing the recent work on eddy current dampers at both Glasgow and Caltech. We have a setup that includes a 2x2 array at Caltech on a single pendulum.

2) Galling and Dust
Larry Jones and I have been working with Mike Gerfin to come up with a plan for testing galling and the production of dust particles for fasteners and tapped holes. Work should start on this in the new year. See report from Larry Jones for more detail.

3) PDMWorks and SolidWorks
Caltech now has PDMWorks 2004 and a sever that acts as our vault. Tests are ongoing and are about to be expanded to include hopefully MIT and the UK.
The suspension team has now updated to SolidWorks 2003 service Pack 4.0. We also have a copy of SolidWorks 2004 on the visitor machine to allow communication with the Seismic team.

4) RM Suspension
MPL and I are continuing to tie up various aspects of the RM suspension including a +/- 500 g mass adjuster for the intermediate stage and a pitch adjuster that better meets the requirements from Betsy Blade.

5) Structure analysis
JaneenRomie, Russell and I are gathering together al of the data we have collected both experimentally and through FEA. This is divided into 2 sections. Section 1 includes several data points such that we are able to compare FEA directly to experiment. This has proved fairly successful so far. Section 2 includes various conceits for stiffening the structure and highlights the importance of the non-suspended components in the analysis. Ideas are being gathered from various people and these include increasing the footprint for the RM as well as several stiffening concepts. All of which we hope to test on the existing MC structure.

6) MATLAB
Norna Robertson and I have been looking at the prospect of increasing the separation of the ribbons in the ETM. This is ongoing but looks promising.
Other updates to the existing quad model are ongoing and it is hoped a version of the MC< RM and ETM can be sent to the DCC before Christmas.

7) VISIT
I plan to visit the IGR at Glasgow for 1/2 a day during my vacation in Scotland, probably the morning of the 23rd. I have a small experiment to carry out and a meeting with Jim, Harry and Caroline.

8) Mode Cleaner Suspension
Both Mode Cleaner suspensions have been prepared and stored again in the containers as they were for the Caltech Workshop in October. New parts for the local control osems, all made from 6061-T6-Al, are due from Glasgow in the new year. At present Russell Jones is ordering 80 to cover the 1 RM, 2 ETM and 2 MC. Perhaps this needs to be reviewed?

CalumTorrie (with input from Norna Robertson)

Core Optics

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

Advanced LIGO Coatings -

CSIRO
Received a 3"dia. fused silica substrate with a 30 layer (Ta2O5/SiO2) coating.
This was a trial run to allow them to tune their coating parameters and measurement techniques.
By their calculations, a (HL)^15 coating design should have a transmittance of 75ppm, we measured ~162 ppm on the delivered parts; this means that they need to revise their calculations to incorporate the refractive indexes they are actually getting on the materials.
Coating thickness uniformity was not very good, CSIRO knew there was a problem with the uniformity on the SiO2 layers, they calculated it to be ~1% on a single layer, we see ~10% on the 3" dia. sample. It is assumed that, as the layer count increases, so does the thickness non-uniformity.
CSIRO also coated four 1"dia. fused silica substrates that were sent toRoger Route for absorption measurements. Roger received the parts and he expects Vlad to measure them after some problems with their laser are solved.

MLD
The coating on the 3" dia. sapphire substrates blistered after annealing them at 350 degrees C.
On a previous occasion MLD had tried to anneal 1" dia. witness pieces at 450 and then 400 deg. C  and they had all blistered.
For the 350 deg anneal test they had none of the 1" pieces that we supplied, so they used sapphire witnesses that MLD supplied and coated with our parts.
The test anneal at 350 degrees was successful, so, our 3" diameter pieces were loaded and annealed using the same protocol that had been tested. For some reason that they do not understand, both 3"dia. pieces blistered in the 350 deg C anneal process. They suggest that it may be that our substrates were polished using a different process than the 1" sapphire witnesses that MLD had provided and the difference in the surfaces was the reason that the coating adherence to our parts failed.
I suspect that contamination on the surface may be the cause; those parts were originally coated more than 7 mo. ago. I suggested to clean the parts before annealing, however, I do not know if the suggestion was followed.
After they make some interferograms, they expect to ship the parts next week.

Auxiliary Optics

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

PHOTON DRIVE R&D
Awaiting replacement of the 500 mW laser.


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