Weekly Report for Week Ending January 22, 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  January 26, 20043 will be:

(Meeting time: 10:30 am Pacific Time)

There will be no Executive Committee meeting scheduled.


Special Announcements:


Weekly Report Highlights
  [late breaking news:  LLO is now connected to LSU & the commercial Internet via gigabit--MZ.]


LSC Issues (Saulson)


No report this week.


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


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

Dominguez Hills:
GEO:
Northwestern Univ.:
Univ. of Michigan: Univ. of Oregon:

Met with the LSC Spokesperson to discuss LSC MOU updating, progress reporting, and web posting processes.


LIGO Weekly Site Telecon (Lindquist)

We held a site teleconference on Thursday, January 22, 2004.  The following issues were discussed:
The list of current actions revised to reflect the status of open actions assigned through January 8, 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

Packaged and shipped NSB packets to the NSF.
1/22/04
Packages
Faxes
In
22
33
Out
7
25

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)

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

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>
 

OUT of the Office on Friday the 16th and Monday the 19th.

 

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)

Nothing to report.


Change Control/Contingency (Lindquist)

Open Change Requests:

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

I believe that CR-040001 replaces CR-030015 and CR-030015 should be closed.  CR-030016 will be placed on the "watch" list.


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

Nothing significant to report.


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


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

Much of the Martin Luther King long weekend was devoted to DAQ studies, a search for the source of glitches observed during S3.  Recall the signature of the glitch is a random setting of some of the least significant bits of channels such as state vectors (at LHO) and REFL_Q (at LLO).  Barker et al. traced the problem to the sharing of a VME bus by the DAQ controller and the test point manager.  A new DAQ configuration will eliminate this conflict.  Read the summary elog here.

The workhouse  tool DTT was upgraded.

4K IFO
ISCT3 POY work was undertaken to compare POY and POB error signals.  The ports are redundant and thus should look very similar, which they do, with the exception of the bounce mode at 12Hz.

The coil driver range was shown to be unable to contend with large microseism, something that was learned empirically during S3.  Among many Saturday summaries, R. Schofield detailed how dust in ISCT4 causes glitches in AS_Q, particularly where the beam narrows.  Glitches observed in AS_Q were correlated in time with VCR images of dust passing through the beam.  Fred Raab points out that the steadily increasing range on H1 during S3 remains unexplained, and may be related to air cleanliness in ISCT4.

Acoustic coupling is worst at the REFL port.  1Hz sidebands on 60Hz can be seen in AS_Q, induced by HVAC system.

2K IFO
WFS work has been relaunched on the 2k.  The overarching goal is to increase the bandwidth on the WFS to ~3-4Hz.  Table mods are underway, as are digital filter construction - the un-optical lever filter that ameliorate the handoff between optical levers and the wavefront sensors.  WFS5 channels were observed to suffer from Pentek glitches, so the ADC was swapped out.

ASPD2 showed an apparent spontaneous 45 degree phase shift.


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



ANNOUNCEMENT:

LIGO and the LSU Physics Department are pleased to announce that Professor Joseph Giaime will take on a new role as Deputy Site Head for the Livingston Observatory. Joe's involvement with LIGO is long standing (certainly since his undergrad days with Rai Weiss at MIT), and for most of you he'll need no introduction. We are extremely fortunate to bring the benefit of his experience, knowledge and vision onto our management team.  We are grateful to
our colleagues in the LSU Physics Department and School of Science for helping to make this arrangement possible.

WELCOME ABOARD JOE!

L1 Interferometer

Continuing investigations on noise coupling mechanisms, characterization of interferometer optics, wavefront and sideband diagnostics, and "what really happens when the power goes up."

Highlights:
Safety/security (Rich Riesen)
LLO, a Community Resource (Bonnie Wooley)
L1 Studies (Valera Frolov)

I worked on increasing input power into the interferometer.  The input power was increased by a factor of 2 from 1.8W to 3.6W.  The loop gains and the mode cleaner reflected port light level were adjusted to compensate for the increased optical gains.  The carrier power in the interferometer scaled with the input power but the sideband power did not. The sideband power is  between 25% and 75% of what is expected from the input power increase. The maximum of 75% was achieved by realigning the input beam into the ifo after the power increase. The radiation pressure on the interferomter and mode cleaner mirrors, electronics saturations and RF phase shift are among possible causes that are being investigated to understand and recover the loss of the sideband power. Two ~20 min long data stretches were taken to look for effects of thermal lensing on the interferometer. No large effect(no more than 10-20%) was seen in carrier and sideband power build up or the optical gain after running the ifo at twice the nominal input power for ~20 min.

LDAS (Yakushin)

LDAS admin: Archived PEM injections segment 758175814-758177713 per Peter Saulson's request

LDAS data analysis:
General Computing (Roddy)
L1 Research and Community Enrichment (O'Reilly)
LLO Seismic retrofit (R. Abbott)
MZ Note: We have received four responsive bids for the HEPI hydraulic piping installation and are meeting to expedite the selection process.

HPLF and Burst Analysis (Franzen, Amin)
CDS support (Ash Khan)


Detector/Technical Support (Coyne)


Seismic Upgrade Project

see also:

Dennis Coyne reporting

Ken Mailand

The seven LLO pump station sub-assemblies are complete.  The pump station frames were rejected and the purchase order cancelled (poor QC). The frames are being made another shop (Southern Enterprises). The assembly of the pump stations was moved from a contractor's location to on-site at LLO for a cleaner and better controlled environment. Two of the seven frames should be complete 1-27, the remaining 5 frames by 2-4.  The 7 inlet tube assemblies should be complete 1-23, the frame drip pans should be complete 2-2.  The fluid biological growth test is showing nothing after 56 weeks. [12 weeks dark environment, seven weeks with the following materials added] I have added aluminum, copper, brass, and iron to the fluid to represent the materials in the system, and moved it to the light.

CDS

see also CDS meeting minutes in the commissioning archives:

CDS Software

Rolf Bork reporting

CDS Hardware

Rich Abbott reporting

Working to get loose ends tied up for HEPI.  Dave Grimmett has been here this week and has accomplished a great deal of work.  He was able to kit up and inventory all parts for the seismic interface chassis and even did a dry fit to be sure things line up.  Various people are putting together cable assemblies for the sensors used on the pump cart and in HEPI proper.  I have finished the schematics for the STS2 interface box, and am in the process of laying out the board.  Parts continue to come in on a daily basis and are piling up here and there. We are still on schedule for delivery of electronics in the second half of February, but there isn't a moment to spare.

Ben Abbott

HEPI electronics:

Jay Heefner reporting

Frequency Devices DAC:

EMI  Upgrade:

Thermal Compensation: Two PCs have been received from LHO. The memory in the machines needed to be upgraded prior to installation of Linux and EPICS. Both machines now have Linux installed and should be ready to ship back to LHO by 1/30.

Sander Liu

(HEPI) Since F. Mann was unable to start designing the optical link circuit boards I have taken over the designing task myself. The transmitter board should be ready by tomorrow and the receiver board sometime next week.

Thermal Compensation

Mike Smith

The magnification ratio of the projected annulus mask pattern was measured to be approx. 25X; the ASAP and MathCad models predicted a magnification of 21X. The difference may be due to dimensional tolerances of the actual purchased optical elements. A new annular mask, central beam mask, and Bessel aperture mask were designed compatible with the actual magnification ratio.

The Edmund Sci. gold coated elliptical mirrors for the compensation bench periscope are out of stock. Uncoated mirrors were ordered and a protected gold coating will be applied by a local coating vendor.

The lenses for the redesigned central heating beam/mask illumination optical system will be ordered after Dave O. tests the new design. The optical layout of the thermal compensation bench was revised to incorporate the latest changes.

PSL

Peter King

After pumping down for the better part of a week, the pre-modecleaner pieces have started baking.

Because the new M-150 laser chiller does not have the same instruction set as the original RTE-140M chiller, I have been trying to get at the chiller instructions issued by the laser power supply.  The current strategy being to use a software translator to translate RTE-140M commands from the laser power supply into M-150 commands and then respond to the laser power supply.  Hopefully this will hoodwink the laser power supply into thinking that the RTE-140M chiller is connected.  This way the controls to the laser temperature can still be executed from the dial, if need be, with the M-150 chiller doing the work without need for the RTE-140M "answering machine".

Errant Beam Baffles

Ken Mailand

The baffles, mounts, and hardware have been received at LHO.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)

Contamination Cavity # 1

A total test of 1700 hrs for the solder sample for the OSEM assembly has been completed.we got a result for the absorption= -0.1+/-0.1 ppm/year and total loss = -0.7+/-0.8 ppm/yr, this result meets the advance LIGO requirement. Please see Dr. Zhang's report.

We have introduced a new sample in this chamber. (21) pieces of  the new twisted, shielded, kapton cables.  Each is 106" inches long cables. Chamber is pumping and laser alignment is in progress.

Absorption Test Measurement prototype in progress

A linear scan along the x-axis of the new sapphire mirror that came from Lyon, France 314 mm Dia. X 131mm thick.  The absorption scan test has been completed.  A bulk absorption measurement completed.  To compare with Lyon I SMA's result, the map was  made with the same coordinate.  The measurement was done at the depth Z= -58mm and with an interaction length of about 8mm, we may compare our results with  SMA's map at Z=-57 mm with main absorption ~ 91ppm/cm at 1mm steps.  Basically, the patterns are consistent, measurement is relative.

Please see Dr. Zhang's report. as well as the attachment at:  http://www.ligo.caltech.edu/~gari/LIGOII/Downselect/SapAbsLyon.ppt

Scatterometer system in standby

OTF Lab at Lauritsen ROOM 38

Cavity #3

The cavity was recovered and it is locked again.  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

PSL LAB.


40 Meter Interferometer (Weinstein)



Rob Ward has joined the 40 meter team as a graduate research assistant. Welcome!

Commissioning (Miyakawa, Kawamura, Sakura): Electronics (B. Abbott, Heefner, Taylor, Nocera, Mageswaran) Digital suspension controllers (Sakata, Goggin, B. Abbott, Heefner) Optical sensing: Safety (all): Following up on the action items from the safety inspection of 1/13/04: South Annex Bake Ovens (Taylor):

Thermal Noise Interferometer (Libbrecht)


This week we have been addressing the electronic noise in our photodetectors. By breaking the signal path at different points, we have identified which stage inside the RF photodetectors is responsible for the excess noise. The noise appears to be coming from the last op-amp stage at the RF-out port, and is present even when this stage is disconnected from the rest of the electronic path. This op-amp is a MAX4107ESA, and its data sheet quotes an input-referred noise of 0.75 nV/rHz. In our detectors, we saw 130 nV/rHz in SAC and 200 nV/rHz in NAC at the outputs of the mixers, which corresponds to 13 and 20 nV/rHz at the inputs of the MAX4107's. We consulted Ben Abbott, who suggested simply replacing the op-amps and supplied us with new ones. Apparently, MAX4107's can sometimes sustain damage that increases their noise floor but does not affect their transfer function. We replaced both NAC's and SAC's op-amps, and we saw the noise come down. However, it did not come down far enough to meet the 0.75 nV/rHz spec.

Next, we looked at the cables connecting the RF outputs to the mixers. Apparently, MAX4107's do not like to drive capacitive loads, so we removed the cables and attached the mixers directly to the RF-out ports, using BNC barrel adapters. This brought the noise down by a considerable amount in SAC. NAC's noise came down as well, but not by as much as SAC's.

With the op-amps replaced and the output cables removed, the electronic noise in SAC is now 40 nV/rHz and in NAC, 80 nV/rHz at the outputs of the mixers. Even though this noise floor is still not quite to spec for the MAX4107's, it is still a significant improvement, and our preliminary measurements indicate that it will be below the shot noise limit for the TNI.


LASTI (Ottoway)


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

HEPI Installation
The first five housing assemblies are on schedule for completion of the finish machining at Southbridge Sheet Metal (SSM) on 1/30. Oddvar and Joe Lacour are scheduled to come assist with a fit check at SSM on 2/4.  Should everything fit fine, five housings will be painted and shipped to Livingston. Lavallee Machine has completed all smaller machined parts and shipped them to SSM for paint and eventual shipment to Livingston. Arland Tool has one operation left. They will ship the first boot to SSM on 1/28 for the fit check. The next four will be shipped to SSM on 2/4 for paint and eventual shipment to Livingston.

We have stopped the installation of the hydraulic acyuators on the BSC chamber and waiting for calibrated Parker control valves.

We stiffened up the attachment area of the crossbeam stiffeners in an attempt to improve the response of the stiffeners.

BSC Chamber

We are reinstalling hydraulic actuators onto the BSC. We hope thatthis will be done by the end of next week.

HAM Chamber

After examining last week's system id, with the aluminum stiffening beams(see LASIT ilog 1/15/04) we decided to try and stiffen the joint between the beams and support table.  The problem is the enhanced tilt in the Y-mode, which can be seen by the zero in the Y-mode transfer function at ~0.25Hz. We changed  the attachment point of the stiffening beams (see LASTI ilog 1/21/04) and are now reexaming the control transfer functions.

Thermal Compensation

Final test were performed on the CO2 projector in preparation for it being shipped to the sites next week


Data Analysis and Computing (Lazzarini)



Simulation and Modeling (Yamamoto)

*** Commissioning ***
*** Modeler Code ***
Melody completed the design and implementation of the C++ FUNC. Her report summarizes as:
 Added code to get the compile/link options from the system's configuration and use them in building the shared library.  Finalizing code development and updating the install document to remove unneeded setup instructions.  Also creating a technical document to describe dynamic linking and how it is being used in E2E.  As soon as her clean up is completed, this will be tested by Hiro and will merge in the cvs.  This will be a major upgrade.
Virginio and Hiro have tested the RungeKutta integrator with SS front-end. With the time step less than 0.1 ms, the error is dominated by the numerical precision. With the double precision, the accuracy is limited at 10-11, while with the quad precision, it goes down to 10-15. The state space module will have an option to choose double or quad precision for the internal calculation, just as the digital filter support the same option.

For the implementation of SS, matrix class is replaced by a version developed by Matt which supports the expression template. This will allow to write codes very cleanly, without sacrificing the speed.

*** thread ***
LIGO Data Analysis System

Software Systems (Blackburn)
Added extra error handling conditions to genericAPI to improve the quality of error messages from job control. This fixed a problem occasionally seen in the controlMonitorAPI logs.

The database table creation scripts have been updated and checked into CVS.

Fixed the problem report on the lightWeightAPI concerning bad or corrupt XML files which were insufficiently being reported as bad items in data bucket.

Added logging of the number of iterations necessary to complete a transaction in the metaDataAPI. Previously the logs didn't reflect the number of retries necessary due to table locks, etc. which can be useful in tracing anomalously large transaction times.

Added additional metadata to the histogram plots in the control-MonitorAPI which provide mean, median, and standard deviation for the y-values plotted in the histogram.

Performance testing of the new buffered/memorymap options continue on the LDAS development system. Preliminary results on a standalone system gave mixed results when the number of threads exceeded the number of CPUs available to the frameAPI.

Added support for using different buffer/memorymap options on different filesystems in the event that NFS, SAM/QFS/Local file-systems have different behavior and require unique tuning to optimize performance.

Removed the annoying system error number message which were never correct.

Enhanced reliability of data structure reads in the frameCPP library to solve a problem associated with corrupt data object lengths that exceed size of frame.

Updated LDAS software documentation to reflect new dependency on the version 3.0.1 release of FFTW.

Work continues on implementing the necessary diskCacheAPI C++ functionality. The I/O components are now complete and the focus is now on supporting excluded directories and one second resolution timing issues on timestamps in Unix.

Polished up the ssh-agent script used in remote process control. More testing is necessary before it is integrated into LDAS.

Continued working on developing a new set of tests to challenge all the data from a particular science run within a particular LDAS release candidate.

Hardware Systems (Anderson)
Caltech

(Dan Kozak)
(Hari Pulapaka) (Al Wilson)
(Stuart Anderson)
MIT

(Keith Bayer)
Livingston

(Igor Yakushin)

Hanford

(Greg Mendell)
H2:LSC-AS_Q!8
H1:LSC-AS_Q!8
H0:PEM-BSC1_MAG1X
H0:PEM-BSC1_MAG1Y
H0:PEM-BSC1_MAG1Z
H0:PEM-BSC5_MAGX
H0:PEM-BSC5_MAGY
H0:PEM-BSC5_MAGZ
H0:PEM-BSC6_MAGX
H0:PEM-BSC6_MAGY
H0:PEM-BSC6_MAGZ
H0:PEM-BSC9_MAGX
H0:PEM-BSC9_MAGY
H0:PEM-BSC9_MAGZ
H0:PEM-BSC10_MAGX
H0:PEM-BSC10_MAGY
H0:PEM-BSC10_MAGZ
H0:PEM-LVEA_SEISZ
H0:PEM-MX_SEISZ
H0:PEM-MY_SEISZ
H0:PEM-EX_SEISZ
H0:PEM-EY_SEISZ
H0:PEM-LVEA2_V1
H0:PEM-LVEA2_V2
H0:PEM-LVEA2_V3
H0:PEM-MX_V1
H0:PEM-MY_V1
H0:PEM-EY_V1
H0:PEM-EX_V1
H0:PEM-RADIO_LVEA
H0:PEM-RADIO_CS_1
H0:PEM-RADIO_CS_2
H0:PEM-COIL_MAGX
H0:PEM-COIL_MAGZ
L1:LSC-AS_Q!8
L0:PEM-LVEA_MAGX
L0:PEM-LVEA_MAGY
L0:PEM-LVEA_MAGZ
L0:PEM-EX_MAGX
L0:PEM-EX_MAGY
L0:PEM-EX_MAGZ
L0:PEM-EY_MAGX
L0:PEM-EY_MAGY
L0:PEM-EY_MAGZ
L0:PEM-LVEA_SEISZ
L0:PEM-EY_SEISZ
L0:PEM-EX_SEISZ
L0:PEM-LVEA_V1
L0:PEM-EX_V1
L0:PEM-EY_V1
L0:PEM-RADIO_LVEA
L0:PEM-COIL_MAGX
L0:PEM-COIL_MAGZ

(Ben Johnson)
Data Analysis Activities (Lazzarini)
Mendell:

Mike Landry and I continue to work on the stackslide search. Some of the coding and debugging is taking longer that we had hoped, though this is par for the course. We hope to post some test results by next week.

Shawhan:
LDAS data analysis:

1) Improved precision with which central time and frequency of events are computed in waveburst;
2) Running waveburst simulations on S2 in preparation for face-to-face burst meeting.

General Computing (Wallace)
MIT:
(Keith)
Livingston:
(Shannon)
Hanford:
(Christine)
CIT:
(Mike)
(Lisa) (Veronica) (Larry)


Advanced LIGO and Supporting R&D (Shoemaker)


Seismic Isolation

From: Larry Jones <ljones@ligo.caltech.edu>
 
Advanced LIGO Seismic Structure

SEI Structure Design/Fab contract:

ASI is applying fewer hours than expected, but progress made to date is still on plan. There are no significant risks or technical issues identified. Total costs to 19 Jan were 10% of contract total cost.

ASI has submitted its design concept for modifying the GS-13 by converting its manual locker function to remote by adding an internal dc micromotor/gearbox unit with gear drive to the existing mass lock shaft with two small brackets. They also provided a quotation for completing the design and building a prototype.

An Intermediate Design Review will be held for the structure configuration on 17 Feb.

Actuator Testing and Redesign:

I'm still having difficulties communicating with BEI/Kimco; I've added e-mail attempts as well as the voice messages I'm leaving, requesting a quote for two standard small actuators (to be used as forcers in modal testing), in addition to the quote for ultrahigh vacuum modifications they had promised since 18 Dec.

Position Sensor Probe Development:

The cabling bake/scan (60M, equivalent to 20 probes) was completed with discouraging results. Subtracting the oven background levels, outgassing rate of the cable per probe unit was 10-10 torr l/s, compared with 1.1x10-12 torr l/s allocated for this for AdLIGO in the proposed document, "Vacuum Hydrocarbon Outgassing Requirements", LIGO-T040001. The SRS RGA head from the 40M was sent back for repairs, and plans are underway to replace Oven C with a 12" ID electropolished nipple, with an extra turbopump and valves so that the RGA head can be islolated during a bake.

Seismometer Procurement:

This task is on hold pending management approval for SEI structure prototype fabrication.

Galling/Dusting Test:

The CES shop has completed fabricating all of the aluminum plates, and is tapping the stainless plates now. They ran into difficulties (binding, breaking taps) in tapping stainless with the prescribed water soluble cutting fluids, both in the machine and with hand tapping, and will be tapping all of the stainless plates with Redi-Tap fluid. They will hopefully finish this week. We need to re-think our restrictions on cutting fluids, on tapped holes at least, to get quality threads. We currently have no controls over coolant used to machine catalog products, such as screws.

Suspension

From: Janeen Romie <romie_j@ligo.caltech.edu>
 
AdLIGO Suspensions
Running an fea on the quad model in Ideas. Had some problems with the conversion from Solidworks but cleared that up. Continuing to model stiffenening concepts on the MC models to compare with the experimental results. This will more thoroughly prepare us for quad structure design in a week or so. Have worked with Calum & Caroline on a list of tasks to finish up this research and the paper detailing the research.

Participated in a telecon with Justin and others on quad work and, primarily, schedule. Again, good progress was made. Carol Wilkinson will be at Caltech next week to finalize schedules with Thomas and I and others.

In the weekly SUS meeting we talked about a possible May/June MC installation test at LASTI. At present, Helena is working on background tasks required to facilitate this. We are waiting for Mark's finalized travel plans to pin down a possible delivery date. Larry mentioned a problem with the 14 cables bought for SUS prototype testing at LASTI. He feels that there is enough time before May to deal with this problem. Doug Cook and I will talk this week about any work we need to do to prepare for the installation test.

Melles Griot sent us some alignment HeNe lasers that were supposed to be Class 3A. They were labeled Class 3B. I sent them back to Melles Griot on an RMA for retesting and relabeling. One came back on Tuesday with the Class 3B label. A call to customer service provided this information - the lasers we bought are class 3A for eye safety criteria specified by CDRH and class 3B for the electronics specified by IEC. I forwarded this to Bill Tyler for advice. After all, we only use these for alignment.

The upgraded ANSYS software with 4X node capability is finally working - we've been given a 12 day extension. Additional software called Workbench was provided but we can't find how to access it. Customer Service has generally been helpful. Calum came in over the holiday to take advantage of this evaluation copy and give it a test drive.

The small sheet of maraging steel Rutherford Appleton requested has been stuck on the roof of a building near the So. Annex. Bob Taylor called Transportation again this morning to get them over with a forklift to take one sheet off and bring it to Mike in CES for cutting. As soon as it is cut, Ed Chargois is ready to ship it to England.

PDMWorks software for design/drawing management seems to be working well. I'm crossing my fingers that it will be a big time saver while still providing the security we need. We will continue to tests it's capabilities.

Core Optics

From: "Erika D'Ambrosio" <ambrosio@ligo.caltech.edu>
 
Caltech prototype for flat topped beam: I run the FFT code for several values of the Finesse to observe the amount of input Gaussian beam that is admixed to the flat topped beam.

We decided that F=100 provides enough suppression of the input Gaussian beam, since in this case it only contributes 10^(-4) of the total power built up inside the cavity. Unfortunately the cavity length has been changed and I will have to design the mirror profile again and start a new set of  numerical simulations. I wrote a document on our first choices in order to discuss it with our collaborators in Lyon.


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