Weekly Report for Week Ending October 31, 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  November 4, 2002 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)

Field Change Orders/Contingency Liens/Change Requests
5. WBS 2 LIGO Lab Operations
Administration (Lindquist)
Sites (Raab, Coles, Shoemaker, Sanders)
Detector (Whitcomb, Coyne)
Campus Research Facilities (Weinstein (40 Meter), Libbrecht (TNI), Zucker(LASTI))
Data Analysis and Computing (Lazzarini)
6.WBS 3 and 4  Advanced R&D and LIGO II (Sanders)
7.CHANGE CONTROL BOARD/TECHNICAL REVIEW BOARD SESSION AS NEEDED Executive Committee only 11:30 - noon   Topics:

Special Items:


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


No report.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



LIGO Operations--Administration


LIGO Weekly Site Telecon (Lindquist)

There was a site teleconference held on Thursday, October 31, 2002. The following issues were among those discussed:

Budgets and Costs--The Office of Sponsored Research has reported that they have received an amendment to our Operations Cooperative Agreement adding $16.5 million in funding for the first half of FY 2003.  We have provided them the information required to generate a "resume" allocating the funds.

Livingston Staging Building--The contractor is still working punch list items.  He has been given until next Monday to complete the work.

Hanford Laboratory Building--Hanford personnel have moved in.  The contractor is working a few punch list items.

Hanford umbleweed Removal--the contractor for tumbleweed removal is going out of business.  The work will be transferred to Landscape Horizons, the current erosion control contractor for the new building.

Traffic Control--Hanford had no additional data.  Livingston has a quote for $11K to widen the road and put an island in the middle.  $14K is estimated for the hardware.

The list of current actions revised to reflect the status of open actions assigned through October 31, 2002 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

Contract
252
Drawings
5
Engineering
5
Graphics
126
Letters
244
Managemnent
54
Publications
185
Technical
145
TOTAL
1,016
> 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>

Working from home on Friday the 1st.  I will be checking email and voice mail.

Weekly Advanced LIGO Project Controls meeting was not held this week.

Advanced LIGO MRE Proposal (Highest Priority)

Cost Book Tool.

Continued assignment from Gary to develop material for the Project Science Seminar.

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)

Nothing to report.



Change Control/Contingency (Lindquist)

No change requests are currently open.
 


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) and Interferometer Operations (Raab)


From: Michael Landry <landry_m@apex.ligo-wa.caltech.edu>

2K IFO (H2)

2k efforts continue to be centered on IOO:  The MC remained highly unstable with IOO WFS engaged, still no solution for this.  The mode cleaner servo board was modified to bring it inline with that of the 4k.  The 2k MC2 has exhibited odd behaviour in which one sensor (LR) sees pitch and pendulum modes, but not yaw.  The optic does not appear to be mechanical coupled to stops, etc.

Optical lever servo filters were set up, similar to those of the 4k.

4K IFO (H1)


Work continued on the 4k AS port; investigations of the beam properties on and before the table, optic layout, and alignment of the EO shutter.  The resulting AS beamspot imaged on a CCD camera was highly elliptical.  While the culprit was initially thought to be the beam reducing telescope, unfortunately this is not the case: the aspect ratio of the beam emanating from HAM4 is roughly 1.5.

The ifo achieved arm, prm and state 3 locks, no full locking.

Frequency noise (Matone)


In the past few weeks, we've been measuring how frequency noise propagates through the system, from the PSL to the IFO. Using one of the long arms, we measured it out of the mode cleaner and we found that the simulated residual rms frequency (when the IFO is locked) is comparable to the common mode linewidth of ~1Hz.

Measurements of the residual rms frequency noise were then compared to the simulation results and were found to be in agreement. A dtt template will be set up to simulate the expected residual frequency noise and generating a figure of merit on the noise level.

It was observed that the 60 Hz power line contributes significantly to the rms and for this we plan to notch it out and hopefully make an impact on the rms level.

On the 2k, the MC settings have been adjusted so as to have a bandwidth of ~20kHz with the crossover at 50 Hz. We are, however, experiencing problems in engaging the WFS.


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


Interferometer Commissioning: After some diagnostic work on the coil controllers and balancing the output matrices at DC for the suspended masses, the interferometer is once again exhibiting stable locking behavior. We are now working on implementation of the common mode servo. (all)

All the WFS are now reinstalled, retuned and characterized. The only electronics work left is the end-to-end test of the WFS2 RF.  This was delayed because the demod board is still faulty and needs another visit to the EE lab.  We are just beginning to recommission WFS1 using interferometer light and will progress to the symmetric port as soon as the demod board is repaired.   Attention is also beginning to turn to the mode cleaner WFS which we are calling WFS M2 and WFS M2 to distinguish them from the other WFS.  The yaw picomoter stearing light into WFS M2 was broken and a new one should arrive tomorrow.  (Andri)

Continue testing and tuning the WFS electronics with Andri. Have verified that all electronics are functional but WFS2 demod board. Work on configuration tool (graphical interface to burt). Can read/write from/to epics a list of channels. More work needed to make the restoring safe for the optics. (Valera.)

Went to Inspiral Upper Limits group face-to-face in Penn State. Work is continuing on vibrational noise in the optical lever supports. We tried using lead-shot filled bags to weight the pier bases and see if this had any effect on the motion. Harry also tightened the floor bolts yesterday and Orlando is seeing if anything changed. Gaby has more accelerometers which we are going to get from LSU today (Thursday). (Brian)

CDS: LLOFb2 was hard down with boot problems. A sun tech support guy was called in to fix. Found memory problems that forced the memory testing at boot to look at a different location that was non-existent. Installed One Sun Blade 2000 in the control room as control 5 with 3 flat panel monitors. Solved problems with the projector interface when running with flat panel monitors. Fonts on new solaris 9 are giving us problems and I am looking into it. Also replaced control 0 in the control room with Sun Blade 1000 running 3 flat panel monitors. Tried the xinerama mode for the above machines. Of the 3 graphics card, one is a m64 - PGX graphics card and the other two are the powerful XVR-500's. In xinerama mode the XVR-500's take the least common configuration of the three graphics card. LLOFb0's minute-trend disk was 98% full. This data should stay forever. So moved some of the old channels that were not being acuired now to a safe place. With this change it is back down at 92% full. I have ordered a A1000 disk array and will put in place soon. Added the Optical Lever channels to the master.config file and reconfigured the DAQ. (Chethan)

LDAS data analysis: Visiting UFL for collaborating on WaveDSO with Sergei Klimenko. In the first approximation finished the whole data pipeline from TCL LDAS job script to LAL. (Igor)

HEPI / LASTI: We are still dealing with assembly problems with the HEPI actuator. We completed the second unit late last week and found after all our pains that we have a single, small leak. The bellows were individually tested in a fixture which permitted them to be pressurized to 90psi, and then immersed in water. Crude but effective in the shop. This time we took extra care to stagger the welds and use minimum heat. The unit looks beautiful but we ended up with a single, small leak at the actuator plate and as before it is leaking between the bellows and the weld assist band. All indications point to marginal welding performed by HYSPAN. With the probability of a weak weld that is thermally stressed by assembly we're proceeding down several paths. Gerry Stapfer suggested a low temperature tin-silver eutectic solder to repair the leaks. I've ordered the alloy and will attempt repair when it arrives. I've also sent some suspect bellows to a vacuum brazing firm, in the attempt to strengthen the weld joint with a braze alloy. They completed a first article this afternoon and are sending it for inspection tomorrow. The most promising solution is to replace the bellows with those of a different manufacturer. I've located a firm known as Ameriflex, who have been very helpful. We had a telecon with an engineer Monday afternoon and agreed upon an ring attachment that was acceptable to Stanford. Corwin Hardham in turn modeled it at Stanford and we (Marcel) checked it against our model and sent a drawing to Ameriflex on Tuesday. Within an hour I received a quote, and gave them the OK to proceed. I've heard from their production manager and they plan to ship our replacement bellows on Nov 8, 10 days after receipt. This is pretty unbelievable given our experience with the previous manufacturer. We plan to wait until receiving the new bellows and have both products in hand (brazed HYSPAN and new Ameriflex) before deciding which one to use. We are completing all of the assembly work on the 2 next units, sans bellows. By working over the weekend (and successfully leak testing) we should begin delivering actuators to MIT about Nov 12. Katrina Carter, Joe Langdale and Gary Traylor volunteered to help Marcel and me measure the constants on machines springs destined for LASTI. They completed 2 today, which are now enroute. We've yet to receive 4 additional springs which were promised Monday. ETD is now tomorrow (Thursday) and with help we will measure and ship by week's end. ETF / Advanced LIGO pod bases Still working on the simplified base and flexure to support the GS-13 geophone on the ETF without benefit of a pod. Marcel is detailing that and will supply to Joe Giaime for production in the LSU Physics shop. (Hammond,Kern)


Detector/Technical Support (Coyne)


DETECTOR SCIENCE & ENGINEERING

Seismic Upgrade Project

Hydraulic External Pre-Isolation (HEPI)

(Jonathan Kern)
We received the first vacuum brazed bellows from Solar Atmospheres
yesterday.  We checked to see if any relaxation of the convolutions happened since the bellows were heated vertically, but none occurred. We do see a slight bowing along the axis, but it is no more than one of theothers that has not been heated.  The braze joint looks good all around.  The areas where the bellows and ring were in contact have a small fillet of braze alloy (Brazed 1).  More typical is the meniscus seen in the other views where a small opening existed between the bellows and the ring.  The engineer at Solar told us to expect this, and is confident that the braze allow has penetrated the gap around and fully wetted the area down to the weld.  Before brazing the remaining bellows we're going to hydro-test this one first. The amount of work hardening that occurred in rolling the bellows is unknown, but the brazing process has resulted in a fully annealed structure.

We had a meeting Monday with an engineer from Ameriflex, and Corwin.  Corwin proposed several weld designs, and the one we selected is seen on the 2 final images on the webpage. I've placed an order for 24 bellows, and Ameriflex has assured me they will ship no later that next Friday, Nov. 8. 

My plan is to assemble the remaining actuators using Ameriflex bellows.  We should be able to deliver the first units to MIT ~Tues, Nov. 12. As a fallback, assuming the Hyspan bellows pass a hydro-test we can use the vacuum brazed Hyspan bellows.  A third option is using the lo-temp tin-silver eutectic solder, which has been ordered.  I should receive it soon and we will experiment with it as well.
http://www.ligo-la.caltech.edu/~jkern/Actuator_Bellows_VacBraze_Oct_31/

We are completing all of the assembly work on the 2 next units, sans bellows.  By working over the weekend (and successfully leak testing) we should begin delivering actuators to MIT about Nov 12.

Katrina Carter, Joe Langdale and Gary Traylor volunteered to help Marcel and me measure the constants on machines springs destined for LASTI. They completed 2 today, which are now enroute.  We've yet to receive 4 additional springs which were promised Monday.  ETD is now tomorrow (Thursday) and with help we will measure and ship by week's end.

(Rich Abbott)
EMI filters were designed and tested on the hydraulic pump stand motor control unit.  The filters are effective in removing the switching noise from the pump servo interface.  More work needs to be done to filter the AC output to the pump motor for switching noise.  We are anticipating shipping the motor speed control electronics this Friday to MIT.

(Ben Abbott)
The Dspace whitening interface and interface boards (for the seismic external pre-isolator) were finished and were sent to PCB Express last week.

(Ken Mailand)
Assembly of the second resistor internal parts and packaging of a parts / tools kit the week of 10-28.

New screw pump arrived 10-29.

Pump station shipped to LASTI  MIT 10-25, est. 5 days to delivery. On going communication with Ken Mason  re.the re-assembly of the pump station at MIT, arrangements made for facilities / staging and tools.

Will make the final viscosity tests on the alternate fluid mixture of alcohol and glycerin, as soon as a tantalum material ball arrives for the viscosity tester. This material allows the instrument to measure more accurately in our range.

Electro-Magnetic External Pre-Isolator (MEPI)

See LASTI report

CDS Software

(Rolf Bork)

CDS Hardware

(Rich Abbott)

Progress was made on the ISS testing at the 40m lab.  A test was performed of a single loop control with sufficient gain to achieve the specified noise suppression using a single loop topology.  The new loop achieved ~80kHz bandwidth and 45 degrees of phase margin,  with a preliminary measurement of suppression, out of the loop, at 10 kHz of about 16 dB.  Lower frequency measurements are being performed, and will be posted when available.  The single loop approach seems robust as tested before the MC, but could not function if sensed after the MC due to large AM fluctuations associated with ground noise. Flavio Nocera is making new cables that will work with the electronic pressure sensor readout box.

(Mohana Mageswaran)

I have sent two tested CM Mode Servo boards to Rana with the DCN change and documentation. I am testing the Variable Delay timing boards. I am also helping Rich with testing his Pump Servo and ordering the correct filter for the driver.

 (Jay Heefner)

FPGA Timing Module

Adv LIGO Suspension Prototype (which has potential applicability for initial LIGO):

(Mike Zucker)

Completed draft requirements spec for the LOS Coil DAQ readout filter & distributed for preliminary review.

With Jay and Sander Liu (also visiting this week) went through rack locations and cable run options for LASTI SUS and SEI installations.

RFI Mitigation

(Mike Zucker)

Detector electronics (Zucker):

With Jay Heefner (visiting MIT this week) and Rich Abbott (by phone) reviewed plans for our upcoming EMC upgrade review, distributed invitations to outside reviewers (from NRAO Greenbank and Los Alamos), and tuned up technical design features of the plan. Comments and questions are welcome on the current drafts of our core documents, now posted at E020966-00.pdf and E020350-08.pdf

The design review will be held 22 November starting at 09:30 Pacific.

PSL

(PeterKing)

The slow loop code was compiled for a Motorola processor, so that it could be run on the LASTI PSL.  An EPICS database required for the code to run was copied over to the m1psl target area. 

A coarse PSpice model for an Hamamatsu photodiode was written and the part created in Capture.  Of the 14 parameters required, only 5 have been figured out.  Some of the remaining parameters are probably not important for circuit modeling.

Optical Contamination Cavities

(Lee Cardenas, Liyuan Zhang)

OTF Lab. (Bridge)

Contamination Cavity # 1

Cavity has the new test sample--65 % Glycerin and 35% Ethyl.   We encountered an alignment situation with the new mirrors.  So we have replaced the cavity with the old cleaned  mirrors.  Now the cavity is aligned and LOCKED.  We are getting 83% beam visibility so far.  We RGA scan the cavity and one can see clearly the Ethyl is outgasing as the Ethyl partial pressure peak is larger than before.

We took ringdown and beat frequency measurements for absorption, ringdown and cavity thermal lensing measurements.

New OTF Lab at Lauritsen ROOM 38

Cavity #3 Reference Cavity still pumping down. Optical train ready.  Continue taking RGA measurements.  Beam visibility is low ~ 65%, we may have to open the cavity to change the mirrors.

Cavity #2 Test cavity

This cavity still pumping, optical alignment and installation in progress.  Continue taking RGA measurements.

Ray Tracing for Errant Beams

(Mike Smith)

Working with Dennis Rose to analyze all potential stray laser beams in the 2K and 4K IFOs that might damage the COC suspension wires and/or electronic cables.

Earthquake Stops & OSEMs

(Janeen Romie)

Received comments on Earthquake Stop Design Requirements document and will incorporate this week. I'll submit this to the DCC & the Revision Technical Review Board (RTRB) after that. Coordinating with Gregg Harry and Dave Ottaway at MIT about getting a spare SOS, from Dave Reitze, and a spare SOS optic (not sure where it will come from yet). Doug Cook has been designing and buying materials for prototypes.

Right this minute, the new osems are somewhere on campus. I'll inspect them upon delivery and send them to the coil winders after that. (These OSEMs are for Gin Gin, 40m, and spares for the observatories).

Dry Entry

(Larry Jones)

The outlet port of the canister was enlarged from 1/4" NPT to 1" NPT and flow checks were conducted with full face mask/mask mounted blower and with half face mask/belt mounted blower, blowing through an empty canister. The full face system had more than sufficient flow, and the half face system was barely sufficient. Silica gel was added to the canister and the full face system was again tested, this time with insufficient flow indicated. Samples of four variations of size of molecular sieve and activated alumina beads were ordered in an attempt to find a system setup that will provide sufficient flow rate for safety; these desiccants should work nearly as well as silica gel, and are more readily available in the larger bead sizes desired for lower pressure drop. 


40 Meter Interferometer (Weinstein)


Suspended mass mode cleaner (Ugolini, Miyakawa, Vass, Abbott, Benna, Bonfield, Berdnikov):
Intensity stabilization (B. Abbott, R. Abbott, F. Nocera, D. Ugolini): Electronics (B. Abbott, Taylor): Optical sensing (Smith): Optics (Billingsley, Armandula), suspensions (Romie), OSEMs (Bob): Facilities and vacuum envelope (Ugolini, Vass, Jones): South Annex Bake Ovens (Taylor, Cardenas):


Thermal Noise Interferometer (Libbrecht)


Since our last report, we have opened the vacuum chamber and removed two collimating lenses from the output paths, the in-vacuo broadband Pockels cell, and a number of extra mirrors from the output paths just before the RF photodetectors. All of this is an attempt, based on a similar experience in TAMA, to reduce scattered light noise in the TNI.

After removing these optics, we then realigned each of the cavities to improve the shot noise limit and to generally clean things up. We now have the best visibilities yet seen in the TNI in all three cavities, 75% for the mode cleaner, 69% for the South Arm Cavity, and 78% for the North Arm Cavity.

Early this week we closed the vacuum chamber and started pumping out.  Closing the chamber perturbed the alignment some, but the visibilities quoted above were easy to recover with minor adjustments to the mode cleaner's input periscope and the pitch of the mode cleaner's back mirror. The error signals and reflected powers are not as symmetric as we expected, and not a symmetric as they were with the chamber open. We are now in the process of tracking down the reasons for these differences.


LASTI (Adhikari, Coyne, Hammond, Kern, Mason, MacInnis, McKenzie, Mittleman, Ottaway, Rollins, Shoemaker, Zucker)

PSL (Adhikariu, McKenzie, Rollins, Ottaway)

Found the PMC control was flaky, and traced it to a blown demodulator.  Replacement with a spare appeared to affect operation of the new FSS; investigation is in progress. 

EPI design and installation (Mason, MacInnis)

The plumbing continues for the HEPI pre-isolators. Tubing has been run from the pump room to the large manifold below the BSC chamber.

Myron has lifted one side of the BSC crossbeams for fit checking a housing assembly. If everything looks good we will bring it down and attach the springs. Mike Hennessey from Stanford will be visiting next week to help with the installation of the HEPI assemblies on the remaining piers.

Additional FEA stiffness modeling was done on the MEPI housing assembly to help Rich and Dennis with the overall model.

MEPI Characterization and Test (Ottaway, Coyne, Mittleman)

We upgraded one the dSpace memory from 256K to 1M, this should enable us to take long swept sine data segments.  Upgrading the other memory would allow us to run more complicated or higher sampling rate simulink programs.

We also retrofitted a 1 micro-farad capacitor onto all of the current driver boards (following Rich Abbotts instructions) which should now make the current monitors operate correctly.

The control effort hasn't accomplished as much as we would have like last week due to the NSF and thermal lensing reviews.

HEPI Fabrication (Kern, Hammond)


We're still dealing with assembly problems if the HEPI actuator.  We completed the second unit late last week and found after all our pains that we have a single, small leak. The bellows were individually tested in a fixture which permitted them to be pressurized to 90psi, and then immersed in water.  Crude but effective in the shop.  This time we took extra care to stagger the welds and use minimum heat.  The unit looks beautiful but we ended up with a single, small leak at the actuator plate and as before it is leaking between the bellows and the weld assist band. All indications point to marginal welding performed by HYSPAN. With the probability of a weak weld that is thermally stressed by assembly we're proceeding down several paths.

Gerry Stapfer suggested a low temperature tin-silver eutectic solder to repair the leaks.  I've ordered the alloy and will attempt repair when it arrives. I've also sent some suspect bellows to a vacuum brazing firm, in the attempt to strengthen the weld joint with a braze alloy.  They completed a first article this afternoon and are sending it for inspection tomorrow.  The most promising solution is to replace the bellows with those of a different manufacturer.  I've located a firm known as Ameriflex, who have been very helpful.  We had a telecon with an engineer Monday afternoon and agreed upon an ring attachment that was acceptable to Stanford.  Corwin Hardham in turn modeled it at Stanford and we (Marcel) checked it against our model and sent a drawing to Ameriflex on Tuesday.  Within an hour I received a quote, and gave them the OK to proceed.  I've heard from their production manager and they plan to ship our replacement bellows on Nov 8, 10 days after receipt. 

This is pretty unbelievable given our experience with the previous manufacturer.  We plan to wait until receiving the new bellows and have both products in hand (brazed HYSPAN and new Ameriflex) before deciding which one to use.

We are completing all of the assembly work on the 2 next units, sans bellows.  By working over the weekend (and successfully leak testing) we should begin delivering actuators to MIT about Nov 12.

Katrina Carter, Joe Langdale and Gary Traylor volunteered to help Marcel and me measure the constants on machines springs destined for LASTI.  They completed 2 today, which are now enroute.  We've yet to receive 4 additional springs which were promised Monday.  ETD is now tomorrow (Thursday) and with help we will measure and ship by week's end. 


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)

Weekly meeting

Luca explained the frequency noise characterization of the LHO 4k IFO. He wants to start using e2e to understand the effect of the seismic noise to the frequency noise induced by the mode cleaner.

Hiro and Virginio are talking to simulate the LLO 4k IFO with the  measured seismic noise by the train and logging, in order to set the requirement
on the improvement of the seismic isolation in order to LLO IFO insensitive (locking-lock breaking, and the noise level) to these noises.


Mirror motion - simulation vs data

Virginio is working to compare the simulated table top and suspended mirror motion with the data. He is using a HAM table which has several suspenbded mirror on top of it. This is a approach similar to the one by S.Yoshida and his stundent at SLU.

SimLIGO development (M.Evans)

Released SimLIGO_021020 which includes functional wavefront sensors (WFS), and associated control loops, for all degrees of freedom of the COC (except the BS, which is not controlled by WFS in the LIGO design).  WFS control has been observed in SimLIGO to stabilize the IFO power and reduce the AS port noise relative to optical lever control.

Version 021020 also includes an improved intensity noise model (more accurate in the 0-10 Hz region), and variable amplitude line harmonics in the coil driver output.  Both of these noise source are important for many bilinear noise couplings.

Of interest in the SimLIGO noise curve is the contribution of DAC timing jitter noise (which results from having the DACs clocked at 1 MHz rather than 16 kHz).  I believe the plan is to reclock the DACs, but until this change is made, I expect this noise source to dominate other actuation noise sources.

New field model development (M.Evans)
Work on the E2E field model continues.  Most recently I have compiled, and tested, albeit very superficially, the highest level operator component (AmpOp) and one of the low level optical building blocks (Interface).

Simulation code development

Melody is working on the input part of the modeler (C++ program) to read the revised file format and to implement optimizations using caching.

Hiro is working on debugging based on the findings by Matt and Bill Kells, both of which are related to frequency modulation of the input field.

alfi5 development

Bruce completed the implementation of the copy and paste. A few bugs were fixed and a minor interface change were done based on the feedback.

Melody Araya continued working on the automated tester for alfi5.

LIGO Data Analysis System

Software Systems (Blackburn)

A schedule was distributed for the next LDAS release this week. It outlines a code freeze late this week with the release late next week. This release  of LDAS will be used to carry out the LIGO/GriPhyN Applications demonstration at the Super Computing 2002 Conference in the middle of this month. It also incorporates the first release of LDAS based on the new version 6 frame specification.

The bulk of software development this week has been focused on getting all of LDAS to work coherently with the new frameCPP I/O library and to support the new metadata associated with the greatly enhanced FrProc structure in that specification. This has also involved developing frame handlers for LDAS that are based on the frame specification's table of contents.

Several issues with the new dataStandalone and putStandAlone user commands which will be at the core of the LDAS contribution to the LIGO/GriPhyN  Applications demo were discovered this week. They are being addressed and we hope to have all the bugs worked out in a couple of days; This would put the finishing touches on the new functionality for the next LDAS release.

The current performance of LDAS with the new frameCPP is about 50% of the maximum achieved in earlier pre-release code based on the old frameCPP. It is known that this is all contained within the frameAPI and mostlikely the new "table-of-contents" handlers which are very inefficient in memory management. There is not sufficient time in the schedule to rework these handlers so the performance will be somewhat less than desired in this release of LDAS.

Two minor changes were made in the wrapperAPI so that in its stand-alone configuration (remoteAPI) it would more easily integrate with the Grid tools being used for the Super Computing 2002 demo.

Hardware Systems (Anderson)

Caltech
(Dan Kozak) (Al Wilson)
(Stuart Anderson)
MIT
(Keith Bayer)
Livingston
(Shannon Roddy)
Hanford
(Greg Mendell)
Data Analysis Activities (Lazzarini)
(Shawhan)
(Weinstein)
(Yakushin)
(Mendell)

General Computing (Wallace)

MIT:
(Keith)

Livingston:
(Shannon)
Hanford:
(Christine) Caltech:
(Mike) (Veronica) (Lisa) (Larry)

LIGO II/Advanced R&D (Sanders)


Core Optics
(From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>)

No report this week.

Advanced LIGO Coatings
(From: Helena Armandula <ahelena@ligo.caltech.edu>)

After receiving an invitation from Ramin Lalezari, formerly the Vice-President of REO, to visit his new company, Advanced Thin Films, I was there last Tuesday.  The State of Colorado has created the Colorado Advanced Photonics Technology (CAPT) Center on the Higher Education Advanced Technology (HEAT) Center Campus at Lowry.  Ramin's lab is in the CAPT Center.  Actually this facility was designed and built by REO during their expansion days, and they never got to use it. The university took over the facility and equipped with state-of-the-art characterization equipment left behind by many companies from the failed telecommunication business.  Ramin's company acquired a large IBS coating chamber with simple rotation that he has already characterized and is producing coatings.  At this time they are manufacturing a planetary rotator that should be finished by the end of the year.  One of his active partners is an ex REO coating engineer. He has other two silent partners with extensive experience, more than 30 years, in the coating field.  They rent clean room space from the university as well as access to the available equipment at the center.  They have a variety of good ovens and microscopes including an Atomic Force Microscope; an ellipsometer, an interferometer, spectrophotometers, they are in the process of building a ring down cavity. Besides they have numerous clean benches, general DI water and point of use DI water units under clean benches.  They have excellent potential to provide good coatings; they are mainly interested in R and D work, and of course, they are looking for business.  http://www.captcenter.org/about/Default.htm

MLD
Received two SiO2/Al2O3 coated substrates, one thin and one thick. The parts have been shipped to Glasgow and MIT.  The coating has not been annealed. "Q" measurements will be taken before and after annealing.

SMA
We have planned a meeting, tentatively for Nov. 7th, with Jean-Marie Mackowski at Stanford.  Jean-Marie will be in the States attending a conference.  During the meeting we'll be discussing possibilities for future coating development work. 

Adv LIGO Core Optics:
(Erika D’Ambrosio)

No report this week.

Advanced LIGO Suspensions
(From: Janeen Romie <romie_j@ligo.caltech.edu>)

 Mode Cleaner:
(From: ctorrie <ctorrie@ligo.caltech.edu> )

 Electronics:

(Jay Heefner)
No report.

40m Suspensions:
(From: Janeen Romie <romie_j@ligo.caltech.edu>)

Prestabilized Laser (PSL):
(From: Peter King <pking@ligo.caltech.edu>)

Software:
(From: "Mark Barton" <mbarton@ligo.caltech.edu> )

This week I worked on reconfiguring Mal Gray's interferometric position sensor to use a corner reflector as a sensing target instead of a simple mirror. The sensor is a Michelson interferometer in which one arm is internal to the sensor and the other extends to a mirror on the object whose position is to be sensed. The end mirror of the internal arm is servoed to keep the arm lengths matched, and the feedback signal is a measure of position. The defect of the original design that we're trying to address is excessive sensitivity to angular motion of the target. We get around this by folding the external arm using a corner cube on the target and a static end mirror on the outside of the sensor housing. I've set up the new configuration and with the help of Phil Willems I got it aligned well enough to produce interference fringes using an external laser, but not yet with the internal LED source (which has a much poorer coherence length of only about 30 microns).

Low Frequency Seismic Isolation:
(From: Hareem Tariq <htariq@ligo.caltech.edu>)

(Charles)
Received the load frame back from the material science but the power supply broken and voltage regulator not in working conditioner. New setup prepared with two LVDTs and drivers this time and a new gauge (~100 lb). Can modify gain now through a separate amplifier (amplification up to 2000 if LVDTs put in series configuration). Ready to calibrate the LVDTs.

LabView: Working on modifying the LabView programme to incorporate the LVDTs. It is now ready to be tested.
Braze: Made the AuSn braze. Looking for an evaporator, consulting Axel regarding it.

(Stoyan)
ANSYS: Voodoo mystery solved in 3-D as well and now can bend and flex naturally the flex joint. ANSYS limited number of nodes causing trouble again. Had problems with incorporating 2-D autocad design in ANSYS, solved it by importing simpler models.
Furnace: Received the gate valve. Ready to put it in.
X-ray: X-rayed B17 (multiple samples) which would be used for annealing tests.
Splat Quencher: Working on converting the mechanical valves to electric ones. Placed an order for more sample holders and coils.

(Alison)
Hardness: Measured more samples for hardness including B16.5. Getting lower values than previously measured by Maddalena.

(Xavier)
TTO: Conductivity analysis continues. Verified that QD values are indeed are inconsistent, completely relying on our own data analysis. Now can control almost all parameters independently of QD software. Ready to test a multiple MoRuB sample.
ANSYS: Almost done with the monoflex model and would soon have results.

Valerie (Xavier):
TTO: Finished almost all radiation loss data and will now have our own measurement for the radiation losses.

(Xavier/ Stoyan/ Charles)
Splatted a night and produced B16, B16.5, B20, B21 and B22. Discovered B22 was contaminated.

(Akiteru and Riccardo in Hongo)
Received repaired vacuum extension rings and mounted on the towers, the vacuum was better but unfortunately there was a residual leak in one of the two extensions that was sent back for repair.  Met with other people in TAMA to discuss the design improvements for the production run of TAMA-SAS.

(Alessandro and Riccardo in Pisa)
Looked with the SEM at the failed braze joint, it is not clear yet if it separated between MoRuB and NiP or between NiP and AuSn.  We will need chemical analysis of the surface with scattering x-ray analisys, but need liquid Nitrogen to do that.  Will do it next week.  The braze still may be sufficiently good as is for most measurements, especially if we manage to improve it by better cleaning and more agressive etching, but it looks more likely that we will have to resort to spattering deposition to get a more intimate bonding of the layers for mirror suspensions and ultimate low noise operation.  Met with G&M and others to discuss details of the TAMA-SAS production run for Florence and Naples, and later for TAMA.

(Akiteru)
I can happily announce that the vacuum envelope for the 3m is fixed this time.  We achieved the best vacuum level of 10-3 Torr and it remains below 2 Torr after left for a day. Certainly there is still some leak but within an acceptable level.


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