Weekly Report for Week Ending April 15, 2004


 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  April 19, 2004 will be:

(Meeting time: 10:30 am Pacific Time)

  1. Announcements
  2. LSC Issues (Saulson)
  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, Zucker, Shoemaker)
      • Detector (Whitcomb, Coyne)
      • Campus Research Facilities (Weinstein (40 Meter), Libbrecht (TNI), Ottoway (LASTI))
      • Data Analysis and Computing (Lazzarini)
  6. WBS 3 and 4  Advanced R&D and LIGO II (Shoemaker)
  7. CHANGE CONTROL BOARD/TECHNICAL REVIEW BOARD SESSION AS NEEDED


Special Announcements:


Weekly Report Highlights  


LSC Issues (Saulson)


No report this week.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


Status of LSC/MOU Research Updates and Program Reports (Petrac)

(LSC Research Updates through Aug. 2004,and Prog. Report through Feb. 2004)

Dom. Hills:
Univ. of Oregon:
Goddard:
LaTech:
Univ. of Texas at Brownsville:
Trinity Univ.
Nat. Observatory of Japan-TAMA Univ. of Washington:
Univ. of Syracuse:
Southeastern Louisiana Univ.:
Univ. Of Rochester:
GEO600:
AURIGA / proposed collaboration:
National Astronomical Observatory, Chinese Academy of Sciences (NAOC) / proposed collaboration:

LIGO Weekly Site Telecon (Lindquist)

There was a site teleconference Thursday, April 15, 2004.  The following issues were among those discussed:
The list of current actions revised to reflect the status of open actions assigned through the last update (March 4, 2004) 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

04/15/04
Packages
Faxes
In
27
32
Out
9
23

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>

No report (vacation). From: Gina Salone <gsalone@ligo.caltech.edu>
From: Florence Kaufman <fkaufman@ligo.caltech.edu>
Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport.

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

Goodrich: Final invoice was approved for payment.

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

We are waiting for a proposal from ASI to cover the removal of the Advanced LIGO seismic isolation system for the HAM chamber.  That decision was made by the CCB to defer that task until next fiscal year.  ASI will produce a set of full design and manufacturing drawings for the HAM system, but will not fabricate. This will result in a reduction of the target cost.

SUPPORT (Baldon, Lloyd, Tischler)

>Irene Baldon

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

ADVANCED LIGO (Cost Schedule Control Systems) T. Frey

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

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/


Assisted Carol with ACIGA cost and schedule data.  http://ligo.caltech.edu/~tfrey/ACIGA/

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


Reports (Lindquist)

LIGO Video--Tom Lucas (Lucas Productions) will be visiting Caltech April 21 through 23 to interview people.  Tom is building the "plot line" for a 20-25 minute NOVA type video on LIGO under a Grant from the NSF.  I will be arranging interviews with Caltech personnel for Tom.  Tom will be traveling from Caltech to the Hanford site to participate in the "star party" scheduled for April 24.


Change Control/Contingency (Lindquist)

There are no open change requests.  The minutes for the meeting of the LIGO Change Control Board  held on April 5 and April 8 have been published (LIGO-M04-107-00-P).  An electronic version is being circulated for electronic concurrence signatures.

Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

No report.


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


Summary of Commissioning Activities at LIGO Hanford Observatory (Sigg)

H1 activities

A new laser is being installed. This one giving up to 7.5W at the input to the mode cleaner. Details here, here. and here. and here.

An equalizer filter was tried in the LO path of the AS port photodetector, but strangely enough no effect could be observed. Details see here and here.

The mode cleaner board has yet another modification that prevents the signal from being attenuated first only to be amplified again. Details see here.

An additonal photodetector in the REFL path using the non-resonant sidebands has been installed and checked out. Details here, here, here, here, here and here. Currently trying to use the new diode in common mode.

Mode measurements of the RIN of the TCS have been performed. Details here and here.

Measurements of the beam profile on the AS table have been done in preperation of the installation of the OMC. Details here. and here.

H2 activities

An attempt was made to stabilize the beam jitter on WFS1 using a PZT controlled mirror. However, its range was not large enough.  

Site activities

No increase in LVEA temperature fluctuations noted after pulsed heating was shut off. Details here.

Dust not producing glitches at tables other than dark port. Details here.

Various problems with the new DAQ setup have been fixed. 


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


Announcement

Tomorrow is Jonathan Kern's last day at LLO. Jonathan was a founding member of the Livingston staff and played key roles in designing and commissioning the interferometers as a lead optical engineer and as our Laser Safety Officer. Most recently we were fortunate to have Jonathan leading our HEPI seismic retrofit effort, managing the design and continuing through much of the fabrication.

Jonathan now moves on to the Magdalena Ridge Observatory in New Mexico, where he will lead a design team to build a novel optical interferometer for astronomy. We at LIGO thank him, and wish him the best of luck in this exciting new endeavor.

Public Outreach (MZ)

Tom Lucas of Lucas Productions is here with a film crew to tape a HEPI actuator installation for an upcoming LIGO video. Gary and HarryO have been spotted on site wearing cool sunglasses.

L1 Commissioning

The move of the electronics at the X end station was accomplished successfully.  It is too early to do a complete EMC evaluation, but preliminary checks indicate dramatic reductions in local VME bus interference as well as 60 Hz hum. We have more cleanup to do, but are extremely pleased with the
way things look so far.

The timely completion of the X end electronics swap allowed us to run the interferometer over the weekend; this verifies that the electronics transplant was functionally successful. It also allowed resumption of ongoing commissioning.

The most interesting result was a probe of the sideband field amplitude and optical gain as a function of induced offsets in the PRC control path. This showed a clear peak well away from the nominal null; phase camera pictures also show the appearance of a ring structure in the sideband field. This behavior is qualitatively very similar to model predictions by E. D'Ambrosio. Follow up measurements are planned to make the comparison quantitative.

After this experiment the corner station gate valves were sealed to prepare for HEPI actuator installation in the LVEA.  We expect to be closed off for about 5-6 weeks to do this installation, finish hydraulic piping, install the TCS viewports, regenerate the cryos, and fix some IP valves. Rolf has also installed the latest version of the ASC code this week (along with the HEPI code) and is testing it with Chethan and Ash.  Meanwhile HEPI commissioning is in full swing at the end stations (see below).

LLO Seismic retrofit (MZ for Rich Abbott)

The X end HEPI electronics are now installed and wired.  All the pier modules are  checked out and powered up, and we expect to bring signals into the ADC's tomorrow. Meanwhile Pradeep, Brian and Rich Mittleman are testing the I/O and software. The system is wet and purged, and the pump speed control is now fully operational with closed-loop pressure regulation.

At the Y end we expect the last hoses to come in tomorrow so we can wet and purge the Y actuators over the weekend.

In the corner station, the acoustic enclosure was craned off ISCT4 and the table pivoted out of the way for installation of actuators on HAM4. The special lifting fixtures for gently lifting each leg of the HAM were load-tested. The first two actuators and piers have been staged to the LVEA  airlock. The HAM4 crossbeams have been instrumented with dial indicators to monitor the lifts.  We expect to begin HAM4 actuator installation tomorrow morning.

Meanwhile the LVEA hydraulic piping continues to progress rapidly; the HAM supply lines are almost complete, as well as one of the BSC sets.

Oddvar Spjeld adds:

Safety and security (Rich Riesen)

General Computing (Roddy)

Data Analysis (Yakushin)

LDAS admin:
Data analysis:

CDS Controls (Chethan Parameswariah)

Rolf visiting LLO this week. Working with him on installing the new ASC Code, Hepi code and the frame builder upgrade.

CDS support (Ash Khan)

E2E Suspension Modeling  (T. Findley and S. Yoshida)

We investigated the effect of asymmetric coil force on small optic's pitch and yaw motion using an e2e SOS box with a realistic table top motion given to its suspension point. To consider the coil force asymmetry, we gave different coil efficiencies (coil force per unit coil current) to the four OSEM actuators. The four coil efficiencies were randomly varied from the nominal value by 1% (i.e., two of the four coil have efficiencies higher than the nominal value and the other two coils have efficiencies lower than the nominal value). The SOS was facing normal to the beam direction (U-direction), and we looked at the height of the peak at 1.45 Hz in the pitch and yaw spectra of the optic's motion. Here 1.45 Hz is the HAM stack's U-U transfer resonance frequency. When the two top coil efficiencies were lower than the nominal value and the bottom two coil efficiencies were higher than the nominal value, the 1.45 Hz peak in the pitch spectrum increased by 18% and the 1.45 Hz peak in the yaw spectrum decreased by 9%. This can be interpreted as follows: When the HAM table moves, the OSEM actuators attached to the suspension tower pushes/pulls the optic via the magnetic force synchronously with the table motion. Under the given coil force asymmetry, horizontal HAM table motion in the U-direction results in a pitch motion of the optic because the difference between the top coil efficiency and the bottom coil efficiency is greater than the difference between the right coil efficiency and the left coil efficiency.  Therefore, the pitch motion of the optic tends to be enhanced, and consequently, less energy goes into the yaw motion of the optic. When the right two coil efficiencies were higher than the nominal value and the left two coil efficiencies were lower than the nominal value, the 1.45 peak in the pitch spectrum decreased by 11% and the 1.45 peak in the yaw spectrum increased by 10%. This effect can be explained in the same way as above.  With this second coil force asymmetry, we examined the effect on an LOS. When the coil force asymmetry is 1%, there was no substantial difference in either the pitch or yaw spectrum. When the coil asymmetry was increased to 10%, a similar effect as the SOS case (with 1% asymmetry) was observed.


Detector/Technical Support (Coyne)


Seismic Upgrade Project

see also:

Ken Mailand
Working on the task of organizing the HEPI materials and documentation, and sending drawing files to the DCC.  The development area in the CES building has been cleaned up and returned to its original condition (I thanked Mike Gerfen for letting us use the space.

CDS

see also CDS meeting minutes in the commissioning archives:

CDS Software

Rolf Bork reporting
At LLO this week: All of our EPICS code which runs on Linux PCs and all 2KHz/16KHz front end software has been put in a new CVS branch (cds/rts). This new branch allows for high level Makefiles and perl scripts to create all of the epics databases and sequencers and load them into target directories, which include the startup scripts and autoburt files. All of the front end code now resides in cds/rts/src/fe, with a single Makefile.

CDS Hardware

Jay Heefner reporting
Fiber Optic Timing Signal Link (Sander)


The oscillation problems reported on last meeting turned out to be a problem with the receiver itself. It appears as though the low frequency response of the receiver is limited to freq>100KHz. While this is fine for the 4MHz clock it is not OK for the 1pps signal. Sander is looking for different transmitters and receivers to use. He will have suggestions by next week's meeting.

Timing System Redesign (Flavio)
Anti-Image Filter (Mohana)

ISS (Flavio)

LSC PD Redesign (Ben)

EMI Upgrade (Jay)

Output Mode Cleaner (Jay)

HEPI (Ben)

Elect Shop (Todd)

PSL

PeterKing
Flavio and I have been working on the both the current shunt and the intensity stabilization board.  The electronics noise was measured in a number of places.  We believe we have a small improvement for the DAQ channel readouts.

OMC

PeterKing
Still more delays are being encountered with the machining of the vacuum chamber.  At last inspection, around 15:00 Wednesday, the only machining operations for the vacuum chamber were to tap two pipe threads, cut three access notches and drill four clearance holes.  Other miscellaneous hardware items have been cleaned and are ready for baking over the weekend.

Thermal Compensation System (TCS)

Mike Smith
Price and delivery quotations for 4 TCS installations plus spares are complete, pending a decision about the CO2 laser power.
A tentative installation and commissioning schedule for TCS systems at H2 and L1 was completed. Installation and commissioning would be occur during the months of July and August.

Baffles

Ken Mailand, Mike Smith
I'm working with Mike Smith on the Baffle project layouts for the next few days to complete and check the work before Mikes vacation.

COS Papers

Mike Smith
An abstract was submitted for a talk to be given at the GR17 conference in Dublin on 4-18.

Revising the scattered light calculations and editing the paper to be submitted on "Direct Measurement of Scattered Light Effect on the Sensitivity in TAMA300", by Takahashi, Arai, Kawamura, and Smith.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)

The (21) pieces of the new twisted, shielded, teflon cables are under test.  We are taking ring down and beat frequency measurements
as well as the RGA of the chamber every day.   NO CHANGE

Absorption Test Measurement prototype in progress

The sapphire substrate PINK color from Lyon, France. (314 mm Dia. X 131mm thick.) still inside the enclosure and it is in standby for further measurements.  The 80mm sapphire cube is waiting for cleaning.  The aluminum support for this cube has been fabricated and tested to hold the cube in place.  We'll scan this cube for absorption test and compared with the sapphire rod (~50ppm/cm in loss).  This cube will be our STANDARD for measuring absorption.  The fabrication of the rods for the enclosure still in progress.

Scatterometer system in standby

OTF Lab at Lauritsen ROOM 38 NO CHANGE.

Cavity #3
The cavity is locked and we are taking ring down and beat frequency measurements every day as well as the RGA for the chamber.

Cavity #2 Test cavity optical set up in standby.
We need to mount back the NPRO and re-align it on the loop.

PSL LAB.
The 10 watt ND:YAG laser is undergoing for a complete and new alignment which is in progress.  We are waiting on the OMC parts from the shop.  We made a ring adapter to align the PZT and the mirror in place to glue it together.  We are baking the OMC body and mirror support.

Misc... tasks
Spacer to increase the height of the mirror holder at the imaging lab has been completed.  Ken Mailand and I, have disassembled the wooden frame for the HEPI assembly and cleaned the area from the shop.


40 Meter Interferometer (Weinstein)


Commissioning (Miyakawa, Vass, Ward, Kawamura):
PSL (Miyakawa, Vass, Ward):
Optical sensing (Kawazoe, Sakata, Ward):
Electronics (B. Abbott, Heefner, Taylor, Mageswaran):
Dual-recycling lock acquisition (Kawamura, Miyakawa): Seiji and Osamu have settled on two lock acquisition sequences (using double demod) that they think will work robustly. Seiji's involves dither-locking MICH then locking the PRC and then SRC with double demodulation at the SP and PO, respectively. Osamu's replaces the first step with an alternative scheme for MICH. We will work towards implementing these schemes. This is a perfect thing to test with e2e... new visitors are arriving in May who may want to work on this.

Facility (Vass) and South Annex Bake Ovens (Taylor):

Thermal Noise Interferometer (Libbrecht)



No report.


LASTI (Ottoway)


LASTI Weekly (Allen, McInnes, Mason, Mittleman, Ottaway, Sarin, Smith)

No report.


Data Analysis and Computing (Lazzarini)



Simulation and Modeling (Yamamoto)

Weekly Physics meeting
We discussed current status of H1 and H2 and problems of WFS, especially noise in WFS1 and low bandwidth in WFS2b loop, with Luca (at LHO). Matt (at MIT) described plans to improve lock acquisition procedure for LIGO I and developing this procedure for Advanced LIGO.

Dual Recycling Cavity
(Hiro) finished the calculation of the scalar case field evolution in a Dual Recycling Cavity.  The LIGO document (T040062), matlab code, validation note and e2e box files using primitive modules are placed in www.ligo.caltech.edu/~e2e/drm.  Next is to extend this to include the modal model.

Note on Thermal effect on WFS
(Biplab) Wrote a technical note on "The Effects of Thermal Lensing on Wave-Front Sensor Signals" (T040066-00-E) and submitted to DCC. Currently it's available at http://www.ligo.caltech.edu/~bbhawal/T040066-00-E.pdf

Code development and maintenance
(Hiro) Getting ready for the release of e2e-2.0.0: Melody and Hiro have been working to finish the simulation engine code release for the next release of e2e, version 2.0.0. This will be released by next Monday. Big thing is the FUNC_X, replacement of FUNC, which uses c++ compiler and dynamic linking.

(Melody)
Modeler:
Modified the build scripts to change some default options and provide more user feedback.

Alfi
(Bruce)
(Melody)
LIGO Data Analysis System

Software Systems (Blackburn)

The weekend tests of LDAS revealed memory leaks in the frameAPI and the metaDataAPI. Both of these have had recent code changes and the authors of these code changes are reviewing their code in an effort to track down the source of the memory leaks. The standing memory leak in the dataConditionAPI is still there, but we now have an idea where to look to fix these.

The DASWG group has requested that LDAS delay its release until final decisions can be made regarding database table changes. The inspiral group has finalized its table changes and the GDS group will be making a proposal for a change early next week. We will probably have a one week delay to accommodate these changes.

Several issues within the controlMonitorAPI regarding backwards compatibility and standardization of the widgets between releases have been resolved this week.

The decision was made this week to upgrade to the IBM DB2 version 8.1 with fixpac level 5 after two weeks of testing revealed no incompatibilities with Redhat 9 and showed performance boosts as much as 5.5x. This decision was also facilitated by the delay in the release proposed by the DASWG. It will also set the stage for bringing online the federated/replicated database services.

Much of the documentation has now been cleaned up in preparation for the next release of LDAS. New versions of dependencies on tools and added functionality has been the focus.

We have a new programmer on staff; Mark Turner will be taking on half of the C++ development associated with LDAS in conjunction with Ed Maros. Mark spent the week reviewing the LDAS architecture and learning how to build LDAS and maintain the nightly builds on the LDAS-Dev system. He has also spent some time studying the diskCacheAPI interfaces with TCL code.

A set of temporary patches have been made to the lightWeightAPI and the eventMonitorAPI to address thread wake-up issues seen under RH Linux (note: these issues have also been seen by the Globus Project).  Eventually, we would like to implement a common solution for all APIs that can reside in the genericAPI instead of patching each API for which the problem is seen.

Several problem reports for the frameAPI, eventMonitorAPI, lightWeightAPI and controlMonitorAPI were closed out this week also. Another 4 seconds of delay were shaved off of jobs that use cURL to move data via URL addresses. This was accomplished with a few lines of code changes in the managerAPI.

The full suite of system and integration tests were completed this week and results were posted on the web. This pass through validated the use of the GCC 3.3.3 CC compiler on our tools sets. We are also verifying that the DB2 7.2 -> 8.1 upgrade will be database compatible and that backup restore functionality translates across version.

Hardware Systems (Anderson)

Caltech
(Dan Kozak)
(Al Wilson) (Stuart Anderson) MIT
(Keith Bayer)
Livingston
(Igor Yakushin)
Hanford
(Greg Mendell)
(Ben Johnson)
Data Analysis Activities (Lazzarini)

Creighton:
This has been a week of cross-checking: I have been looking at the precision of radio pulsar timing data for the known pulsar analysis, examining changes between old and ``official'' versions of the F-statistic code for the GriPhyN pulsar area search, and checking some calculations for seismic noise reduction in subterranean interferometers.

Mendell:
The StackSlide code now has the option to use LALSRunningMedian to normalized the power in the SFTs using the running median estimate of the power spectral density.  We continue to work on comparisons of our code with the Hough code, and improve our estimated upper limits.  We will soon start working on the code needed to run the Monte Carlo simulations needed to get the final results.

Shawhan:
Sutton:
I divided my time this week between working on the new DMT code for calibrations, processing TFClusters events for the LIGO-TAMA analydid, and editing the LIGO-TAMA paper for the GWDAW proceedings.

Sylvestre:
Weinstein: Yakushin: Lazzarini: General Computing (Wallace)

MIT:
(Keith)
Livingston:
(Shannon)
Hanford:
(Christine)
CIT:
(Bruce Sears)
Ilog/Enote:                                           (3.0 days)

(Mike)
(Lisa) Mail Stats 4/1/04 - 4/7/04
Messages Accepted:      18188
Spam Rejected:          10044
Viruses Rejected:       1131
False Positives:        12
Total Mail Thru:        29363

Mail Stats 4/8/04 - 4/14/04
Messages Accepted:      18043
Spam Rejected:          9448
Viruses Rejected:       1130
False Positives:        24
Total Mail Thru:        28645

(Veronica)

(Larry)


Advanced LIGO and Supporting R&D (Shoemaker)


Seismic Isolation

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

Advanced LIGO Seismic Structure

SEI Structure:

ASI has completed a NASTRAN finite element model of what they call Stage -1: the BSC crossbeams, clamps and support tubes. The first resonant mode is at 21 Hz, with 7 modes below 100 Hz. They are performing analyses to determine the phase of the stage-to-stage transfer function. The BSC configuration development is on plan.

LIGO has directed that the BSC optical table be lowered in elevation by 10 cm, to accommodate an overall quad height of 200.5 cm.

LIGO has directed that both optical tables have nitronic-60 Heli-Coil inserts installed in all of the 1/4-20 tapped holes, to greatly reduce the amount of particles generated by fasteners.

ASI has released a process specification for fabrication of the SEI structure, and issued a draft process specification for precision packaging of the SEI structure and pods.

We have requested copies of drawings and fabrication quotations as structure design progresses, and have enlisted Mike Gerfens and Rick Paniagua, supervisors of Caltech machine shops, to assist in making independent estimates of fabrication costs. Quotations and estimates will be tracked and compared in an effort to understand and control costs.

The Design Review meeting for the BSC structure is now scheduled for May 18, 2004. The HAM structure Design Review is scheduled for July 30, 2004. Delivery at LASTI of the BSC prototype is expected to be in November, 2004.

Actuators:

A contract was signed with Planning Systems Inc. (PSI) for the design and fabrication of voice coil actuators for the SEI prototype BSC structure for LASTI. Planned deliveries are as follows:

29 April 2004: interface drawings, small and large actuators
24 June 2004: production drawings and prototype units, one each, small and large actuators
30 September 2004: production units, 6 each, small and large actuators

Having production drawings will permit LIGO to competitively bid the production quantities of the actuators, likely to be over one million dollars.

A teleconference was held between PSI and ASI (SEI structure contractor) to clarify design requirements and to make sure that all known design issues were understood. PSI's thermal analysis had assumed a four point mounting at the bobbin instead of our planned two point mounting. The four point mounting provides higher heat transfer, for lower outgassing; this has now been incorporated in the SEI structure design plans. It will likely be implemented by two mounting points and two copper cold straps. Bobbin wall thickness and top and bottom flange thickness are increased (compared with the actuators previously used) which will also result in a cooler bobbin coil. Lateral coil gap has been increased slightly to allow for more convenient assembly. The capability of having the actuators custom designed is a big benefit to LIGO.

Position Sensors:

Refinements were made in the design requirements for the position sensors. Jay Heefner will be directing the procurement of the sensor probes and modules.

Seismometers:

Nothing new.

Galling/Dusting Test:

Nothing new.

Suspension

From: Janeen Romie <romie_j@ligo.caltech.edu>
 
AdLIGO Suspensions
Quad FEA
Working with Dennis and Calum on Quad/SEI fea. I'm currently working on the heavy mass/high first mode model to remove enough mass to meet the mass budget Dennis has provided. I've gone from 214 kg to 189kg with a goal of 175kg. I hope to get that done this afternoon. I'll run an analysis to make sure that the changes have not drastically changed the 1st mode.

MC to LASTI in June
Coordinating with many key folks on preparing for the mode cleaner triple suspension to go to LASTI in June.
The long poles are osems, so far, along with working around personnel travel schedules. We will discuss this in more detail at the Tuesday SUS telecon.

Hybrid Osems
I've requested a quote and delivery schedule from a coil winding house in Corona - Corona Magnetics - which may be do the coil winding for the hybrid osems. Russell reports that 20 hybrid osem heads/formers should make it to Caltech (barring Customs problems) by April 30. We have the Kapton magnet wire ready to go.

Suspension Gazebo
Minitec in New York has provided us a faxed drawing of the suspension gazebo. We chose a rectangular structure, made of 90mm x 90mm Bosch-like aluminum extrusions. I've asked Minitec to quote for a kit, so that we can assemble the structure here in the Synchrotron. Hopefully, they will provide answers to some more questions in the next day, along with providing us a firm price and delivery schedule.

Suspensions Controls Prototype Testing Plan
I've received input and comments from almost everyone on the Suspensions Controls Prototype Testing Plan. I've incorporate all changes and am just waiting for clarification on a few issues from Mark Barton and Caroline Cantley. As soon as that is done, I'll make any more changes necessary and send it around to the aligo_sus mailing list.

Primavera
I've been working on assigning Primavera task numbers to the Quad task list such that Primavera updates and task scheduling/priorities may be done more easily. I will try to get this done as soon as possible as Primavera % completes are due to Thomas. I'll schedule a meeting with the Primavera reporting personnel to make the appropriate updates as soon as Thomas, Calum and I have checked the interfaces.

Core Optics

From: Bill Kells <kells@ligo.caltech.edu>
 
As the downselect issue heats up now, I've been spending more time re-considering the entire situation and doing some related studies. What more can we conclude, near term about sapphire? How much better will it indeed be functionally? A lot is related to the thermal issues, and so this has been in close contact with P. Willems. Also whetehr some further OTF measurements on the samples we have can give some further clues. An immediate need I'm pursuing are the outstanding DRR "action items" in this regard.

Auxiliary Optics

From: "Mark Barton" mbarton@ligo.caltech.edu

This week Bram Slagmolen of the AIGO facility at Gingin and I reached a major milestone in the work that I had come to Australia to help with. We had prepared and suspended two BK7 test optics, an ETM and an ITM, and in the last few days we finished installing them in the vacuum system and aligning them. (See attached photos.) Thanks to Janeen and Helena for all the prep work that made it possible.  The whole process went without major incident except that we had to do a number of workarounds because the practice optics weren't quite the same size as the sapphire optics that the fixtures had been designed for. In the remaining week and a half of my time here we'll see how far we get towards locking an 80 m cavity. 

Other Laboratory R&D

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

Simoni
We have cleaned and reorganized the OTF laboratory to begin the constuction of the cavity.  Probably lost five ponds in the process.
We received the suspension maraging components and we built a support to constrain the shape of the maraging blades and wires during the bake. Yesterday we  started the bake, at the beginning of the next week we will have the blade and the suspending wire ready to use. We also received and are preparing most components of the cavity structures, in the next week we will probably be able to finish the assembling of the internal part of the cavity mechanics . We  received the initial optics but we forgot ordering the mirror micrometric screws.  As soon as we get the screws we will start to mount the optics in the cavity. The delayed vacuum tanks should be done in 10 days.

Mantovani
I  almost finished the modifications of the control circuit, adding the thermal compensation part. In the next week I'm going to take transfer function measurements to reach lower resonance frequencies (so far stoppped at 60 mHz vertical frequency due to thermal instabilities. I have also calibrated the magnetic actuator and modified the magnetic circuit to improve its performance increasing the flatness of the working region.

Agresti, D'Ambrosio
Considering the possibility of converting the MHM interferometer from co-palnar to confocal, like the new baseline Adv-LIGO.  We calculated the corrective coating profile needed to produce M-H mirror for this confocal configuration starting from spherical mirrors of different focal lengths.  The best starting mirror seems to be a 8500 mm focal length mirror.

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