Weekly Report for Week Ending February 5, 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  February 9, 2004 will be:

 (Meeting time: 10:30 am Pacific Time)
 

  1. STAFFING COMMITTEE


Special Items:


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Saulson)


no report


LIGO Laboratory Administration (Lindquist)


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

Univ. of Rochester Washington State GEO600 CaRT

LIGO Weekly Site Telecon (Lindquist)
There was no site teleconference scheduled on Thursday, February 5, 2004.
The list of current actions revised to reflect the status of open actions assigned through the last update (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


02/05/04 Packages Faxes
In 25 28
Out 4 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)
[pel] Univ. of Oregon: The contract for on-site support at LHO is under review. The payment for costs incurred to date is pending an agreement as to what is owed, consistent with the contract terms.  We are still waiting for University of Oregon information regarding amounts owed.
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>
 

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/
 

No report this week (vacation!)
 

 

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 has been 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>

Working with Ryan Tischler to negotiate and obtain approval of 2004 LIGO Renovation Requests with the PMA Administrator's office.  Presently, most of the LIGO safety related requests have been accepted and resolution/corrective action authorized by PMA.  One of the major renovation requests was for PMA to provide funding/assistance with space modifications required before work could start on major modifications of the LIGO server equipment room.  This request involved modifications required of the DCC work space to accommodate the LIGO "mail room".

During this reporting period, helped with the planning for the mail room relocation, coordinated and assisted with moving the main fax machine.  Also continuing to work with PMA to implement the "approved" LIGO renovation requests.


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



 

Summary of Commissioning Activities at LIGO Hanford Observatory  (compiled by L.Matone)

This week, we continued to work on H1's ASC system and we restored H1's Inpiral sensitivity
back to 2.5-3Mpc (see elog). Ring down one-arm measurements for H1 and H2's were
taken (see elog) which allowed to estimate the cavity poles and ITM trasmittivity.

In WFS land, we focused primarily on the WFSs on reflection. Currently, we have WFS4 that
behaves as expected (it sees mainly the cETM and cITM angular degrees of freedom). WFS3
sees a combination of cETM, cITM and RM and we'd like to see if we can get a better
separation (we'd like to have WFS3 that sees only the RM.) The goal is obtain an angular sensing
matrix with less cross-terms than before. If we succeed, we have a chance at stabilizing the
RF phase of WFS2 which we consider to be at the root of the bandwidth problem.

The NR sideband modulation depth was increased (see elog) by 10x therefore amplifying
the WFS signals by 10x. This however introduced a line in the AS_Q spectrum at 1442Hz
(difference between ASC sideband frequency and LSC sideband frequency (see elog)).

Auxiliary loop shaping (for l- and l+) was carried out this week in order to understand
where the excess noise in these loops is coming from (see elog).
 


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


LLO (Zucker et al)
---------------------------------------------------------------------
Special item: NSB Retreat at LLO
---------------------------------------------------------------------
We hosted a retreat of the U.S. National Science Board and NSF top brass
at LLO on Wednesday. This was a new experiment for the NSB: the first
time they have visited, as a group, one of the major U.S. science
facilities they voted into existence (ten years ago!).
 

By all accounts, the experiment was a resounding success. Thanks to all
the presenters, tour guides, operators, and support staff who
contributed time and energy. It's always hard to single any individual
out for special mention, but of course there's one name on everyone's
lips...
 

WAY TO GO BONNIE!
 

(OK now, about that LSC meeting next month...)

GHS note:  And Larry Wallace and Shannon Roddy did a great job on the technical elements of the presentations and video! Hoorah to them as well!
 

L1 commissioning (summary by Zucker)
--------------------------------------------------------------------
Commissioning work continued to concentrate on detecting and
understanding the effects of increased power in the interferometer.
After dealing with peripheral alignment effects due to radiation
pressure (reconfigured the optical lever filters) and debugging a
saturation issue in the RF sideband monitor (a.k.a. SPOB), a locked run
at 4 watts input power finally yielded clear evidence that thermal
lensing affected our sideband coupling. There is an intensive effort to
understand the results and correlate them with the modeled behavior.
 

Meanwhile we expect even more power will help clarify the parameters, so
Peter King and co. are working to improve the modematching into the PMC
and possibly boost the laser power proper. We hope to get something like
6 W with these steps.
 

Peter and Flavio Nocera also are revisiting the intensity stabilization
servo (ISS); this new version was commissioned before S3 but we want to
understand it better before we propagate it to H2 and H1.
 

Gregg Harry and others wrapped up an exhaustive round of test mass Q
measurements.  The coarse assessment was that the mirrors tested match
expectations, but further analysis continues (specifically to relate the
findings to projected losses in the coatings, of intense interest for
Advanced LIGO).
 

Gregg and Rupal also took joint video image and integrating
scatterometer data on the cavity mirrors, to follow up on the work by
Bill Kells and company at LHO.
 

We were interrupted a bit this week by some intense microseismic
activity due to stormy weather, and by an intermittent clock cable on
the main LSC realtime front end processor.
 
 

LLO Seismic retrofit (R. Abbott)
---------------------------------------------------------------------
1.  Things are still on track for the HEPI electronics to be in house
for the second half of February.  Almost all of the design work has been
done for the electronics and the majority of parts have been received.
A large part of the board stuffing was done this week by the online
board stuffing place.  Boards will be arriving next week in time for
Dave Grimmett to work with them.
 

2.  The HEPI piping contract was awarded.  The contractor, is to be on
site for a kick off meeting on Friday 6 February, and work is to begin
on the X end station on Monday.
 

3.  The valve calibration is finally converging.  We are anticipating
the first valve to be calibrated today (5 Feb).
 

4.  Preliminary AC wiring has begun to power the pump stations in the
corner and end stations.
 

5.  Next week, we are to review the installation procedure for the HEPI
system.  Hopefully, we will be able to bless this process by late next
week so that installation is free to begin thereafter.
 

6.  Fit check for the actuators and housings is progressing well.
Assembly of the tripods to the actuators is in progress.
 

L1 Commissioning (Frolov)
---------------------------------------------------------------------
I worked with Rai and Andri on thermal lensing studies.
The POB electronics chain was checked for RF saturations during the power
increase. The FR levels are below saturation even for the maximum current
input power. The ITM angular motion was stabilized using the DC coupled
optical levers by increasing the oplev DC gain. The thermal lensing effect
on the interferometer power build up and optical gains was investigated.
The effect is small for current power levels ~<10%. Work is underway to
improve the accuracy of the measurements.
 
 

LDAS (Yakushin)
---------------------------------------------------------------------
Preparing for burst F2F meeting at UF.
 

General Computing (Roddy)
---------------------------------------------------------------------
Since Mydoom.A came out on 1/27 the anti virus software on the mail
server has stopped well over 1,100 mydoom.A infected emails.  We only
had one user get infected by the virus shortly before the new virus
definitions came out.  I estimate that RAV has stopped over 5,000
infected emails since we started using it if you include sobig, klez and
the other major viruses over the last two years.
 

I upgraded the software on the PIX firewall to version 6.2 from 5.3.
Hopefully this will fix a few problems that we were experiencing.  There
are numerous bug fixes between these releases.  Within the next couple
of weeks I plan to start modifying some of the PIX configuration to take
advantage of some of the features that we are not currently using.
 

Spent a lot of time preparing for and then supporting the NSB meeting
this week.
 

Looked into a problem on the Solaris to Linux file server backups.
Turns out that using NFS v2 increases performance, but breaks ufsdump
backups via NFS.  Had to revert back to NFS v3 for the time being.  I
will have to dig a bit deeper into this problem to figure out what is
going on.
 

Contacted Solsoft to determine how well they support the Cisco 3550
series since that is now our router for our internet connection.  Turns
out that I may be able to use the PIX strictly for internal networking
and use the 3550 for public address space.  This may improve performance
of the new connection.  This will take some time to look into and
possibly implement.
 

Ordered a copper GigE switch to provide copper GigE connections to the
GC servers.  Waiting on a quote from Sun for NICs.
 
 
 
 

HPLF and L1 commissioning (R. Amin)
---------------------------------------------------------------------
 

HPLF: Earlier this week, both the Laser Midwest technician and ELS
telephoned.  They mentioned that a new fiber optic had been sent to
replace the fiber optic damaged in last week's test.  Even though ELS
has been informed that the fiber catastrophically failed while inside
the diode chamber, they believe that the diode pump bank will continue
to run correctly.  We have aired our concerns regarding debris remaining
in the pump chamber.  The new fiber should be here by early next week,
pending on US Customs.
 

Further inquires intot the status of the 100 W device are uninspiring at
best. One of ELS's engineers has indicated that neither the contracted
power nor the planned lasing efficiency has been achieved. The laser
currently is capable of ~80 W with rapidly decaying beam qualities. They
clarificatied that the working 100 W device was constructed and is run
by the University of Stuttgart, and that a comparison is being made
between their commercial laser and the academic device to find out what
is amiss.  No set deadline on delivery exists.  More information
regarding the laser will be known by Friday.
 

Oscillator phase noise: With several megajoules of assistance from Rich
Abbott and Peter Fritschel, I have taken noise spectra of the two spare
IFR 2023A oscillators in the electronics shop.  Rai Weiss will be
working with me when we document the amount of phase noise being
transmitted from the 24.5 MHz oscillator.
 

Scatterometers: I have also calibrated the LHO scatterometer photodiode
used to measure the ETMy.  These numbers have been  posted in the e-log.
 

New Faraday Isolator Hardware for LHO: The first pieces of the LHO 2k FI
have begun arriving.  All 20mm FI hardware will be kept in the LLO
Optics lab until assembly begins.  Additionally, a spare 20 mm TGG
crystal is being sent from LHO to UF for absorption analysis.  Should
this crystal pass UF absorption criteria, we will incorporate this
crystal into a second replacement input FI.
 
 

Burst data analysis (Ken Yoshiki Franzen)
---------------------------------------------------------------------
Preparing data and presentation for the f2f Burst group meeting in
Gainesville. Florida.
 

ISS and PSL (Peter King)
---------------------------------------------------------------------
 

1.2 LLO
=======
    Flavio and I have been taking data on the intensity stabilization
servo, characterizing its performance with the photodetector in its current
location after the pre-modecleaner.  A broad peak between 300 Hz and 1 kHz
was observed in the noise spectrum that was not present at the time of the
initial installation.
 

    Ashfaq has completed a test sequence for communicating with the laser
power supply and fooling it into thinking that a chiller is connected.
After sorting out a relatively minor problem with the format of the chiller
response, the sequence works up to the point of putting the laser into
standby.  So far so good.  The next test will be to communicate with the
new chiller.
 

2.2 PSL
=======
    During the course of re-aligning the 10-W laser, it was observed that
the output windows on both the main and sample beam distort the beam shape
by more than what would be expected from a planar window.  The reason could
be that the center of the windows does not coincide with the optical height
and as a result the beam exits the windows near the edge of the window.
The edge of the window is a little distorted from being epoxied, or sealed,
into its metal holder.  As a result the beam gets distorted.  The output
windows were subsequently removed.
 
 

CDS support (Ash Khan)
---------------------------------------------------------------------
1) Developed a communication interface between the laser power supply and
the Chiller, to be used as a replacement for the old Chiller.
 

2) Created a new RedBook Web page showing the list of the CDS controllers in
Alphabatical order, as well as, location and desction and added a procedure
for the Burtgooey.
 

3) Rebooted l1lscl0 nearly 10 times in the last 5 days.
 


Detector/Technical Support (Coyne)



 

DETECTOR SCIENCE & ENGINEERING

Seismic Upgrade Project

see also:

Rich Abbott

1.  Things are still on track for the HEPI electronics to be in house for the second half of February.  Almost all of the design work has been done for the electronics and the majority of parts have been received.  A large part of the board stuffing was done this week by the online board stuffing place.  Boards will be arriving next week in time for Dave Grimmett to work with them.

2.  The HEPI piping contract was awarded.  The contractor, is to be on site for a kick off meeting on Friday 6 February, and work is to begin on the X end station on Monday.

3.  The valve calibration is finally converging.  We are anticipating the first valve to be calibrated today (5 Feb).

4.  Preliminary AC wiring has begun to power the pump stations in the corner and end stations.

5.  Next week, we are to review the installation procedure for the HEPI system.  Hopefully, we will be able to bless this process by late next week so that installation is free to begin thereafter.

6.  Fit check for the actuators and housings is progressing well.  Assembly of the tripods to the actuators is in progress.

Ken Mailand

All 7 pump stations are mechanically complete and pumped to 110 PSI for a

leak down test.

We will require one pump station at the X end first. Distribution

manifolds need to be 

designed and manufactured for the end station[s] X and Y should be the

same.

A reservoir common to the vertex and both end stations also needs to be

designed and manufactured.

The local fluid re-circulation circuit, and passive pressure relief

circuits designed,

the valves and other parts purchased.

I have done preliminary work on these tasks today.

CDS

see also CDS meeting minutes in the commissioning archives:

CDS Software

Rolf Bork reporting

- All realtime front ends have now been modified to connect to the new DAQ 

networks using standard libraries. In the process of modifying the ADCU code to 

do the same.

- Still no definitive word on when the HEPI processors will arrive. I called 

yesterday, but was told production is still awaiting something from R&D (doesn't 

sound good). Someone is supposed to get back to me with more details.

- Framebuilder code almost ready with latest upgrades. A header file still needs 

modification for the Framebuilder to read in the new configuration files.

- Alex is working in his "spare" time on modifying the LSC code for lock 

acquisition in the 40m lab.

- Started writing up documentation on the new DAQ layout. Includes descriptions 

of all code changes, installation and test plan, and how to operate the new 

system. Hope to have this out early next week prior to installation starting on 

Feb. 17in advance.

CDS Hardware

Rich Abbott reporting

Jay Heefner reporting

ETM Transmission PD

- The circuit boards for the ETM PD filter are due back on 2/9.

RFI Retrofit

- Panels for the VME crates and end racks have been received.

- All cables are on order and are due within 2 weeks.

Thermal Compensation

The two EPICS PCs are operational and ready to ship. Initial control databases have been installed and are ready for test with the hardware.

Frequency Devices Low Noise DAC Modules

- One module has been received and is to be tested as HEPI code development allows.

- FDI thinks they have found the source of the glitches and are in the process of modifying saveral modules for an integrated test. They should have results by 2/6.

Ben Abbott

a.  Another Conec order has arrived, with the remainder expected next week.

b.  The XYCOMM 212 Interface boards and the XYCOMM 220 interface boards have come back from PCB Express, and they look fine.

c.  I have finished work on the 8-Channel Valve Driver Board, It is at PCB Express, and should be back in the next few days for examination.  Once I'm satisfied that it is healthy, I will send it on to Screaming Circuits.

d. The Power distribution boards are back from PCB Express, and they look fine.  I need to stuff them, and get them ready for shipping.

e. The front and back panels are drawn for the ICS Interface Chassis and the XY220 Interface Chassis.  The Rack panels are also drawn, as are their panel blanks for 9-pin, 15-pin, 50-pin and a special blank to allow timing, ethernet, and reflective memory through.  All of these will go out shortly.  Panels remain to be made for the 8ch Valve driver chassis, but those will be done as soon as the circuit boards are back from PCB express so I can double check the fit.

f. Phoenix changed out all the 15V caps that were on the ISS PD that failed.  I have begun to check it out, and it does not draw the high currents that it used to.  I will continue to test it until I am convinced that it is reasonably robust.

Sander Liu

Proof reading of  both the electro-optical transmitter and receiver circuit board design is now complete. Will place an  order for a couple of boards as well as components for testing today.

PSL

PeterKing

During the course of re-aligning the 10-W laser, it was observed that

the output windows on both the main and sample beam distort the beam shape

by more than what would be expected from a planar window.  The reason could

be that the center of the windows does not coincide with the optical height

and as a result the beam exits the windows near the edge of the window.

The edge of the window is a little distorted from being epoxied, or sealed,

into its metal holder.  As a result the beam gets distorted.  The output

windows were subsequently removed.

The bug I reported last week in the power supply software was wrong and was

the result of the bath temperature being coincidentally the same as the

default standby temperature.  At the time this led me to wonder which

temperature probe was being engaged.

 

Thermal Compensation

Mike Smith

All of the remaining parts have been ordered, and will be received at LHO either this week or the week of 2/9.

I updated the optical layout to incorporate the changes that have occurred during the last week. I updated the parts list. Made an integrated layout drawing and sent it to Doug Cook showing the plan view of the LHO thermal compensation installation and proposed external alignment location in the LVEA. Wrote a component alignment procedure for the thermal compensation bench: LIGO-T040014-00. Made travel plans to be at LHO from 2/9 to 2/27.

Optics Analysis

Erika D’Ambrosio

I am analyzing the results of several FFT simulations 

for LIGO I, in preparation to the meeting on the thermal compensation system. 

This work is instrumental for comparing the images of the phase cameras

with the power distribution predicted by the paraxial model.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)

The (21) pieces of the new twisted, shielded, teflon cables are under test.

Cavity locked and we are taking ring down and beat frequency measurements 

as well as the RGA of the chamber every day. 

Please see Dr. Zhang's report.

Absorption Test Measurement prototype in progress 

Testing of thenew sapphire mirror 25 mm Dia. X 50 mm thick for

absorption measurement has been completed.

we replaced the 1mw He-Ne laser for the 4mw of power. 

A new absorption test scan at different depths (Z ~ 2.25"& 3.875" inches) for the Lyon, France 

(314 mm Dia. X 131mm thick.) Sapphire mirror has been completed. 

basically, the patterns are consistent and measurement is relative.

Please see Dr. Zhang's report. 

Scatterometer system in standby

OTF Lab at Lauritsen ROOM 38

Cavity #3 

The cavity is locked and we are taking ring down and beat frequency measurements every

day as well asthe RGA for the chamber.

Cavity #2 Test cavity optical set up in standby

PSL LAB.

The (4) PMC bodies are under vacuum and RGA is in progress.

Alignment and mode match of the 10 watt laser into the PMC ring laser is in progress.

Misc... tasks 

ordering of mirror mounts and optical mounts for the absorption test. 

The new enclosure design for the 60 watt laser is in progress.

New design of an enclosure for the chopper(to reduce noise) has been completed and

fabrication is underway.


40 Meter Interferometer (Weinstein)




Thermal Noise Interferometer (Libbrecht)


This week we carefully measured the shot noise in differential mode and confirmed our earlier estimate. We find our shot noise limit to be 3.7e-19m/rHz. This is below our previous electronic-noise limit of 5e-19m/rHz, but not by much. It does make our thermal noise measurement a little clearer, though, at high frequencies.
 

We also measured the power transmitted out the back of the cavities and found it to be 25 mW, a factor of four lower than the 100 mW we had assumed for our initial shot-noise estimates. This, along with a very rough estimate of the effect of less-than-perfect visibility, gives us a shot noise estimate of about 1.3e-19 m/rHz, much closer to our observed level than before but still somewhat low. This still assumes that we are getting the full 1e4 finesse in the arm cavities, which we have not yet measured.
 

We also fit our newest noise curves to a combination of coating thermal noise and our measured shot noise limit. We find that the thermal noise floor is slightly different from what we observed before the mirrors were removed and reinstalled, but the difference is not great. Attached is the latest noise curve along with a fit.


LASTI (Ottaway)


We spent most of this week installing the BSC hydrualic actuators and
working out a procedure for the Livingston installation.
 

A new revised LASTI schedule for the next two years was done taking into
account the new Lab budget.


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)
LinLIGO
------------
(Matt) Finished work on update to LinLIGO's optical model. Comparison
 between this version and the "Readout and Control" paper is good,
 though the paper addresses only some of the matrix elements and is
 limited to a small set of symmetric optical configurations.
 

Matlab tools for FFT studies
-------------------------------
(Biplab) Matlab tools for calculating signals from FFT's grid outputs
 for fields are now ready. Accuracy limits of these are understood.
 [Related to that: Hiro and I detected a bug in an E2E code that
  determines if two numbers are same within the accuracy of resolution.
  This bug was responsible for creating some major confusions in
  validation tests of these Matlab tools. Fortunately, this didnot
affect
  our previous e2e results including those from SimLIGO.]
 

FFT files for as-built LIGO
-------------------------------
(Biplab) Gave as-built input files and phase maps (that we used last
 summer to study effects of phase-maps on LIGO sensitivity) to
 Kenneth Ganezer of UC Dominguez Hills for use in his studies of
 thermal effects.
 

Mechanical Simulation
-----------------------
(Virginio)
Calculated a state space representation of the LIGO suspension including
the violin modes.The representation is obtained on a  model of the
suspension
which represent the wires using a finite partition. Some asymmetries on
the wires are also introduced. Dissipation mechanisms are simulated
considering the usual viscous damping ( time domain model) .
Derivation of the Lagrangian, the stiff mass damping (et cetera )
matrices
has been done using a library of routines developed in the maple 9.01
framework. Providing the Lagrangian and the set of generalized
coordinates
the library is able to compute the proper matrices in numerical and
analytical form.
 

The aim of this work is to better understand the excitation mechanisms
of
the violin modes.
 

Debugging and Validation of the representation will be done using the
new
state space primitive for LTI system implemented on e2e.
 

Code development and maintenance
----------------------------------
(Hiro) modeler code:
 Modification of modeler to support a simulation of systems described by
 State Space Model using ABCD matrix is completed.
 A new primitive, statespace, has been added. It is possible to use quad
 precision internally to achieve a better accuracy, just like the
 digital_filter primitive.
 Old matrix class is replaced by a new template based matrix class.
 The gcc compiler requirement will be 3.3.1 or newer from this release
 on.
 A new version of modeler package (1.8.3) will be released soon.
 

 The matrix class can use expression template method, but, for now, the
 code generated is too slow compared with the primitive implementation.
 Hiro gave several articles and a simple example implementation to
 Melody, asking to look into this issue. For now, the version used in
 modeler does not use expression template.
 

(Melody)
 C++ FUNC:
 Finalized code development.  Currently writing a technical document
 to describe dynamic linking and how it is being used in E2E.
 

 Examining performance issues with our implementation of a Matrix class
 using expression templates
 

(Ed Maros)
   1. Completed work on e2e code to support 3.3.x compilers.
   2. Fixed minor issue in documentation generation that
      prevented compilation of FlatTex tool.
 

Alfi
-----------
(Bruce)
        - Work on stabilizing and improving bundlers.
        - Added new E2E/Alfi data types.
        - Fixing box file parser semi-colon handling(PR 441).
 

LIGO Data Analysis System
 

Software Systems (Blackburn)
 

The new diskcacheAPI has now been well tested with this past weekend's
test runs on LDAS-DEV adn LDAS-TEST. With this new diskCachAPI we are
now able to bump up the job rate through LDAS by about 30%. The LDAS-DEV
system was able to run at 2000 jobs per hour all night and we think we
have a bit more head room before hitting another bottleneck.
 

A pre-release version of LDAS has now been built and the full suite of
system tests performed against it. Several minor issues with the new
diskCacheAPI have been found and 4 out of 6 of these have already been
fixed. Of the two remaining, one is certain to be fixed and the other
needs a more thorough investigation before determining if it requires
fixing for this release. We are currently targeting Thursday Feb 12th
for the release assuming no new issues are discoverd in system tests.
 

The memory leak reported for the frameAPI over the last two weeks has
shown a new and unusual behavior. At 1500 jobs per hour the system can
go for 12 to 36 hours without leaking memory. At the newly acheived
2000  jobs per hour the memory leak is immediate and about 5.7 KB/job.
We are using the public domain leak checker, valgrind, to look for
causes of these leaks in mini-standalone processes based on the frameCPP
and frameAPI code. A few very minor issues with the code have been
found with valgrind, but nothing that points to the full memory leak.
 

A new test script has been developed to use the inspiral DSO to look
at all the S2 data as part of a long running system test. A couple of
minor issues still remain (such as missing sensemon frames) before it
will be possible to run this test against all S2 data for LHO and LLO.
 

Began putting together a skeleton of the configuration scripts for the
TCL/Globus project. This skeleton will allow our TCL/Globus wrapping to
integrate easily with other scripting language wrappers over Globus.
We have made arrangement to visit with the developers of the PyGlobus
package at LBL on the 24th of February. There we plan to identify common
grounds for making TCL/Globus and PyGlobus an integrated solution.
 

Hardware Systems (Anderson)
Caltech
-------
(Hari Pulapaka)
 

* Installed the new RH9 ldas-grid.
* Moved all user accounts on ldas-grid from group based to individual
  user based accounts on NIS.
* Modified the Condor configuration on the nodes so that jobs are not
  pre-emptively killed, maximum number of jobs increased, jobs run with
a
  nice level of 10 and always start on the nodes immediately.
* Also learning about SWIG and building a small prototype for ftp-ing a
  directory using pyGlobus.
 

(Al Wilson)
 

* Moved the new RH9 ldas-grid machine into the live system.
* Changed limits of BB for cit. Set warning level for /usr1 to 95% and
danger
  to 97%.
* Repaired one of the new dual-Xeon 1RU machines on 6th floor. Now
running
  memtest. If all goes well Burntest over the weekend.
* Swapped node128 and node8 (test) The old node128 will not boot.
Continuing
  to troubleshoot
* Node128 (old node8) has been set to hyper-treading off for performance
  testing of the Inspiral search code.
* Replaced disk3 in datacache6.
 

(Stuart Anderson)
 

* Help testing LADS-1.0.0 release due in 1-2 weeks.
* Worked with Foundry to solve a major problem with the core Ethernet
switch
  for the LDAS-CIT cluster.
* Started working on evaluation of the next Operating system to use for
  the Intel clusters in the post Red Hat Linux era, e.g., Fedora,
  Red Hat Enterprise Linux, ...
 

MIT
---
(Keith Bayer)
 

* Syncing data off of pcraid2 so I can do final board swap.
* Pcraid6 passed burntest.
* Copied MDC data via LDR (impressive 6-9MB/s bandwidth from Caltech!).
 

Hanford
-------
(Greg Mendell)
* I have verfied that the S3 pemCRoss RDS frames reported on last week
  (and under /samrds/S3/pemCross/HL-RDS_R_L2-75[15-77], visible to
  fortress, at LHO) contain no gaps other than those due to times when
the
  DAQ system failed to produce raw frame data.  The
LDAS/createrdsGUI.tcl
  RDS generation process was very successful.
* The LDAS beowulf cluster at LHO has been running waveburst DSO jobs
  at capacity for the last week. This raised the room temperature
several
  degrees F. I have set up independent temperature monitors on gateway
and
  dataserver. See:
 
http://www.ldas.ligo-wa.caltech.edu/ldas_outgoing/tempmonitor/ gateway.txt
  and
 
http://www.ldas.ligo-wa.caltech.edu/ldas_outgoing/tempmonitor/ dataserver.txt.
  These are useful for viewing trends, and as a backup to the CDS
  temperature alarm system. (The CDS temperature alarm for the LDAS room
  is currently broken. Ben is working to replace/repair it.)
(Ben Johnson)
 

* The air filter was finally re-installed in the 5-ton AC unit on Jan
30 2004.
   It was removed long ago while for the move to its current location.
* /backups filesystem (t3-26) now available on all servers via NFS, at
LHO.
* Worked on SAMFS@dataserver stall on Feb 2 2004. It was similar to the
  incident in mid January and required a reboot of gateway and
dataserver.
  Ping tests between the hosts are now running.
* Continued work on the data glitch problem with Vern Sandberg and Dave
Barker.
 

Data Analysis Activities (Lazzarini)
Mendell/LAndry:
Mike Landry and I are continuing to work on the StackSlide code.
Currently we are focused, in parallel, on three main issues: validation
of the code, benchmarking it to learn what parameter space we can
realistically run on with available computational resources, and the
analysis pipeline. This week I am writing code to organize results in
xml files.
 

Shawhan:
* Ran the inspiral search code on the S2 playground data from H1 and H2,
in order to take a look at correlated glitches which may look like
coincident inspiral candidates.
* Updated the LIGOtools 'segments package', including the 'segwizard'
utility.
* Preparing several LIGOtools packages for release.
 

Lazzarini:
Formatted and posted official S3 h[f] curves to DCC. see S3 section:
http://www.ligo.caltech.edu/~lazz/distribution/LSC_Data/  -> S3
 

Working with Joe Romano and Stan to complete the draft of our H1-H2
combined
channel paper.
 

General Computing (Wallace)
MIT:
(Keith)
-Building replacement wireless router for NW17
-Finished upgrading new mailserver - will make
 swap next week
Installed replacement cheapo inkjet for color 11x17 prints
-Trying to find replacement hp4550 duplexer (they don't
 make them anymore) for NW22
 

Livingston:
(Shannon)
-Since Mydoom.A came out on 1/27 the anti virus software on the mail
server has stopped well over 1,100 mydoom.A infected emails.  We only
had one user get infected by the virus shortly before the new virus
definitions came out.  I estimate that RAV has stopped over 5,000
infected emails since we started using it if you include sobig, klez
and the other major viruses over the last two years.
-Upgraded the software on the PIX firewall to version 6.2 from 5.3.
Hopefully this will fix a few problems that we were experiencing.
There are numerous bug fixes between these releases.  Within the next
couple of weeks I plan to start modifying some of the PIX
configuration to take advantage of some of the features that we are
not currently using.
-Spent a lot of time preparing for and then supporting the NSB meeting
this
week.
-Looked into a problem on the Solaris to Linux file server backups.
Turns out that using NFS v2 increases performance, but breaks ufsdump
backups via NFS.  Had to revert back to NFS v3 for the time being.  I
will have to dig a bit deeper into this problem to figure out what is
going on.
-Contacted Solsoft to determine how well they support the Cisco 3550
series since that is now our router for our internet connection.
Turns out that I may be able to use the PIX strictly for internal
networking and use the 3550 for public address space.  This may
improve performance of the new connection.  This will take some time
to look into and possibly implement.
-Ordered a copper GigE switch to provide copper GigE connections to the
GC servers.  Waiting on a quote from Sun for NICs.
 

(Larry)
-Assisted Shannon in debugging a couple of network problems. We still
have a few
minor items we did not get to on this trip. Mostly documentation
related tasks.
-Overall the setup/presentation for the NSB conference went well. We
learned a
number of things from this setup.
There were issues with the different presentations being loaded on a
single box.
Since a few of the presentations had special features developed on a
certain
level of s/w they did not work properly on a different version of the
s/w.  We
did get everything working on a single box but there was some time spent
debugging the issues. We did find that the Windows OS and different
video
drivers to be our biggest problem.
We are now looking into a video hub/switch so speakers can use their own
computer if needed without removing the main presentation computer. We
are also
looking into a video booster because of the long video cable run.
More work is also needed on audio setups for the teleconferencing that
was used.
 

Hanford:
(Christine)
- Installed new labview software on the unix license server.
- Fixed some ssh problems on the Control Room GC unix computer.
- Took care of some sendmail error messages and some offsite use of our
mail server.
- Finished installing the new wireless access points.  Have noticed big
fluctuations in signal strength on all the access points.  I'm
investigating why this is happening.
- Updating the support license for my backup software.
- Misc. user support.
 

CIT:
(Mike)
-Backed up all NTSRV's; end of month ghost backups.
-Helped DCC relocate a few workstations to make room for new mail room
setup.
-Working on an Ansys 8.0 issue, trying to get a new feature called
workbench to run on multiple clients with our current license. This is
looking like a licensing issue that Ansys tech people will have to
correct.
They claim that it should work. I have tried every which to get this
work
but (no luck)
-Worked with Irena Petrac, regarding a Microsoft Office issue. (Very
time
consuming) but resolved the problem.
-Called Dell's tech support to get a loaner laptop fixed. I spent a lot
of
time on the phone going through a diagnostics with Dell's tech support.
This required a motherboard replacement.  Dell has come out to replace
the
motherboard. I am finishing up loading this laptop with GC software, to
put
back into the loaner pool.
-I worked on Ruth Brambila's computer. She is complaining about it
being to
slow. I am loading a more updated PC for her.
-This week I updated the following ghost images: Cindy A., Florence
Kaufman, Dot Lloyd, Gina Salone, and Donna Tomlinson.
 

(Larry)
-Worked a few procurement issues. It looks like I have a number of
items to work
on when I return to Caltech.
-Assisted the group in a few minor items. Some disk clean, user account
setup
and modifications.
-Most of this week was spent working on the NSB meeting. From my point
of view
everyone involved handled things really well and there was a large group
involved. Kudos to Bonnie and the Livingston group, those attending the
conference/mtg gave out a number of compliments on how well things went
and were
appreciative of all the work they put in.

GHS:  I AGREE. EVERYONE DID A GREAT JOB!
 

(Lisa)
- Did monthly backups.
- Swapped hardware for betelgeuse and jump-started it to Solaris 9.
- Installed AP2000's on the 6th floor of Millikan.  There was a lot of
user
support following this.
- Troubleshooting on wireless connection for Peter Shawhan.  Determined
that he
needed to have his card replaced.  It looks like notebooks that run
particularly
hot are prone to have their wireless cards die in the 1-2yr age range.
There is
another notebook besides Peter's that I suspect is having early
symptoms of
hardware failure.
- Created a half dozen mailman mailing lists for advanced ligo use.
 

(Veronica)
- LIGO website: Updates to various pages.
Compressed a set of mpeg movies for Riccardo's SWG presentation.
- LSC website: Updating MOUs. Working on the GWDAW webpage. Posting
updates to the LSC March meeting website as they arrive. Working on the
repair of the progress report submittal web application. This starts
with getting closely familiar with WeBase documentation. Finished an
image of a map of the LSC Collaboration; continue working on the online
version of the map.
- CaJAGWR website: Updates to the website and user support.
 


Advanced LIGO Development (Shoemaker)


Advanced LIGO and supporting R&D

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. They have added two design personnel to the task, part of a planned rampup. They have completed the FEA model of HAM Stages 1 and 2.

LIGO has sent ASI data to close one of the three outstanding Action Items, the location of the CG for the STS-2 seismometer.  ASI has notified LIGO that their deadline for information required for the other two Action Items, Payload Mass Properties and Stiffness Matrix, is 5 February. If not received by then, assumptions will be made by ASI for the missing data, and the LIGO Project may bear more cost if revisions are necessary. LIGO personnel are attempting to meet this deadline.

The Configuration Intermediate Design Review for the BSC and HAM structure is scheduled by plan to be held on 17 Feb.
 

Actuator Testing and Redesign:

Still awaiting requests for quotations.
 

Position Sensor Probe Development:

Ordered and received an additional 20M of position sensor cable for testing. This will be processed with bake temperature increased to 200C for a new RGA scan in an attempt to meet its proposed AdLIGO outgassing allocation.

Plans for replacing/upgrading a vacuum bake oven in the 40M lab continue, to better provide us the capability of qualifying materials for AdvLIGO outgassing levels. In the meantime, testing will be conducted by Kyle Ryan at LHO.
 

Seismometer Procurement:

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

Galling/Dusting Test:

Testing of the 10 tapped aluminum plates has been completed, with 50 Stainless Steel (SS) screws and 50 Electropolished Stainless Steel (EP) screws. Reduced galling and dusting was noted on 0.005" oversize tapped holes and with EP screws (possibly because the EP screws has pitch diameters that were 0.001" smaller than the SS screws). One of the SS screws froze in position in a standard size tapped hole.

Testing of the 2 aluminum plates with Heli-Coils was completed, with 10 Nitronic 60 (N6) and 10 Silver Plated Stainless Steel (SP) screws. One plate had Heli-Coils of N6 material, and the other used standard SS Heli-Coils. All N6 screws were extremely smooth with every insertion and removal. Dust generation was very light with both screw materials, with possibly more particles seen from the SP screws. N6 screws are expensive (58 X SS!), and no one stocks the 1/4-20 size. N6 Heli-Coils' cost is 2 X SS. The N6 Heli-Coil test plate will be retested with SS screws, which is a more likely configuration for LIGO.

The fabrication of Stainless Steel plates has been completed; these will be cleaned and baked in preparation for testing.

Suspension

From: Janeen Romie <romie_j@ligo.caltech.edu>


Advanced LIGO Suspensions
Working with Calum and Mike on organizing the quad design work and the progressive prototyping plan. Working with Larry and the others on a surrogate BSC chamber and table into and upon which we can do quad assembly and installation tests.

We will have the first of our weekly design meetings on Monday at 8am Pacific. We are looking forward to an informal setting to discuss quad design issues. Highlights, actions and decisions will be distributed to the aligo_sus mailing list weekly. Issues with physics implications will be brought to the weekly suspension meeting.

I've just got to fix one node in the huge (1 million + nodes) IDEAS quad model for the analysis to go through, I hope.

Working with various team members on updating Thomas's Primavera data. As we have not done this since October and because of the replan, this involves lots of work.

Starting to coordinate talks/discussion topics for the Suspension Summit.

Mike P-L and Calum will be giving a tutorial on their Solidworks design tools this week which I look forward to very much.

I talked to Bill Tyler about the Melles Griot lasers. He will provide me a part number for an appropriate filter to make these lasers class IIIa.
 

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

Advanced LIGO Suspensions - Caltech Quad

Vault - PDMWorks
PDMWorks now up and running and being used by SUS team. All CAD and related documents will be stored here for the quad work. this will replace the /engmech/

Quad Tasks
Janeen, Michael and I have created a Quad tasks list. This will be passed by other members of the SUS team before being distributed to a wider group.

Pitch Adjuster prototype in lab
Michael and I tested a pitch adjuster on the MC triple pendulum. Theoretical calculations have been created that have now been backed up experimentally. This will allow us to more easily design a pitch adjuster for the Quad upper mass.

40kg Test mass Prototype
Single Pendulum drawings to workshop. Should be assembled by Feb 25th.

FEM
Quad structure (repeating analysis by Dennis Coyne in T030044), a test structure and static example of an optic for Ricardo de Salvo have been modelled this week using Ansys Workbench 8.0. It is hoped to set up all of the licences with Workbench 8.0 and also have at least 5 copies of the translator used to load SolidWorks files.

Suspension/Isolation Group quasi-Monthly Summaries


 
  6 
February 05, 2004. 17:17 CST
Janeen Romie 
Periodic Summary 
Suspensions 
Caltech Suspension Work 
Calum, Mark, Russell, Caroline and Janeen have been working on finite 
element and experimental analyses on the MC, RM and quad. To support this 
and other areas, Russell joined us here at Caltech for 2 weeks in November. 
A report summarizing the preliminary work shall be published soon under 
document number T030278. The primary work involved the mode cleaner 
suspension. Frequency analysis was performed and experimental data was 
taken on three different configurations of the mode cleaner suspension. 
Finite element modeling was done in ANSYS and IDEAS. All three methods 
compare favorably. A second set of data was compiled which compares modeled 
and experimental results of various methods of clamping and concepts for 
stiffening the structure. The paper also outlines several more concepts 
that may be used to stiffen the MC and RM designs. It is assumed that those 
concepts may be used to stiffen the quad structure. A sub-group of the SUS 
team has been established to carry forward the work for a quad. Mike P-L is 
here now for a month to work on quad development.
 
Because of the 2004 Plan Update, much of our work on the MC and RM has 
stopped as we transition to the quad prototype design work. One suspension 
will remain assembled here at Caltech while the other will be prepared for 
cleaning and baking. Mark hopes to double-check the local controls and 
check the global controls sometime this week. The only work left on the MC 
shall be the preparation work to ship the MC to LASTI in the May/June 
timeframe for an installation test. Helena is coordinating this work now. 
We are coordinating with Doug at LHO and Dave Ottaway at LASTI on an 
alignment plan.
 
RAL has agreed to support the quad controls prototype design work. With 
this support, along with support from the other UK groups – the University 
of Glasgow, the University of Birmingham and Strathclyde University – the 
suspension team hopes to have a quad prototype to LASTI in a year from now. 
 
A progressive prototyping plan has been created to lead up to a full quad 
prototype in the fall. We’ve also been working on categorizing and 
organizing the design work required to complete this design. Weekly design 
meetings, starting this Monday, will improve the efficiency of the 
organization.
 
A sampling of modeling work to support the quad may be found at these links:
Investigation of Wire Lengths in Advanced LIGO Quadruple Pendulum Design 
for ETM/ITM by Norna Robertson
Investigation of Spacing of Silica Fibres in Advanced LIGO Quadruple 
Pendulum Design for ETM/ITM by Norna Robertson 
Effects of Asymmetries in the Suspension on Cross Couplings by Mark Barton
 
 
Calum and many others are working on CAD data management issues. They are 
testing software called PDMWorks, which members of the SEI group have been 
using with Solidworks. It will be used in conjunction with the DCC.  
PDMWorks will store and support control of files of almost any flavor – CAD 
model and drawing, word processing, translation, and Acrobat. The PDMWorks 
vault and a web based access for non-CAD users is now set up and running at 
Caltech. Several members of the SUS team are already using it to store 
files, templates etc., related to the quad prototype work.
 
Calum and Mike Perreur-Lloyd have created various Solidworks tools to 
support and streamline the design process including tools to create a bill 
of materials, a drawing tree and a materials list. They’ve created smart 
CAD and data templates and have customized the Solidworks toolbox for our 
needs. Sometime this week, they will give a tutorial on how to use these 
tools. Associated documents on this are T030143, D030382, D030383 and 
D030384. If you’re interested in these tools, please contact Calum or Mike 
P-L as all up-to-date templates, etc., are on the Caltech PDMWorks vault.
 
Suspension weekly meetings have proved invaluable. Meetings are every 
Tuesday at 9am Pacific/5pm UK and instructions may be found at this link. 
Notes from previous meetings may also be found at this site.
 
In eddy current damping news, Mark used Mathematica to do the theory for 
the case of a finite-sized cylindrical magnet (as opposed to an idealized 
zero-size dipole) in a cylindrically symmetrical cavity. As he suspected, 
this showed that most of the eddy current damping was being produced in a 
small volume of copper near the shoulders of the magnet, and that copper 
elsewhere could be cut away to save weight. Calum produced a design for a 
2x2 array that incorporated these ideas, and we measured the damping 
performance of it and some older designs on a single pendulum at Caltech. 
We got fairly good agreement between the Mathematica theory and the Caltech 
measurement, but both of these were about a factor of four higher than 
expected based on earlier work at Glasgow. After some debugging it turned 
out that the high values were indeed correct, which means it might just be 
possible to use eddy current damping on a quad pendulum.
  7 
February 05, 2004. 17:43 CST
Helena Armandula 
Periodic Summary 
Suspensions 
Ribbon / Fibers / Bonding Issues 
Started monthly meetings on Ribbon / Fibers / Bonding issues.
As result of the first meetings we have a partial AdvLIGO “ear” design.
K. Strain remarked on the need to evaluate the impact of the bonded area / 
ears (on sapphire and silica masses) on noise performance.  
Since there is a practical parameter that needs to be maintained in order 
to accommodate the welding of the ribbons/ fibers, it was strongly 
suggested to formalize the calculations in case that the thermal noise goes 
over the allocated budget, then, the issue would have to be raised to the 
Systems level.  
For the next meeting:
Calum – Will perform some modeling to ensure that wires, as they are 
positioned on the preliminary ear design, clear the penultimate mass.
Caroline – Will continue the development of ear design for sapphire and 
silica masses, calculate how the bonded area impacts on thermal noise. 
She’ll also start looking into a parallel ear design to accommodate fibers.
 
The next meeting is scheduled for February 24th.
 
Helena
  8 
February 05, 2004. 19:55 CST
Norna Robertson 
Periodic Summary 
Suspensions 
Update 
Work on Suspensions at Stanford (Norna Robertson)
 
Test mass (ETM/ITM) Suspensions
a)      Analysis carried out of length changes i) to increase space for catcher structure supporting penultimate and test mass, and ii) to ease 
installation at LASTI. Work written up: "Investigation of Wire Lengths in Advanced LIGO Quadruple Pendulum Design for ETM/ITM" NAR, 26 Jan 
2004, and submitted to SUS group for discussion (decision pending).
b)      Analysis carried out of effect of increasing spacing of ribbons/fibres in lowest stage of quad pendulum to allow exploration of different 
designs of ears used to attach the fibres to the penultimate and test masses and to ease space for the welding process. Work written up: 
"Investigation of Spacing of Silica Fibres in Advanced LIGO Quadruple Pendulum Design for ETM/ITM" NAR 26 Jan 2004, and distributed to 
Ribbon/Fibre/Bonding subcommittee of SUS for discussion (ongoing). The major effect of increasing this spacing is to increase pitch thermal 
noise. Estimates of this noise level as a function of fibre spacing and loss in fibre (using a simplified analysis at present) have been produced to 
aid further consideration of design.
 
Beamsplitter Suspension.
Analysis is ongoing on a preliminary design of a triple pendulum suspension for the beamsplitter (which hangs in a BSC chamber, and thus has 
nominally been considered to be a quad). Draft document has been prepared and will be released to the SUS group shortly for consideration.
A RODA (record of agreement/decision) has been made that the folding mirrors (FMs) required at Hanford for the second interferometer will be the 
same size and mass as the beamsplitter - thus the above design work will be applicable to the FMs as well. 
 
Eddy Current Damping Work
        Work done in collaboration with colleagues at Glasgow and Caltech.
Experimental results on GEO prototype at Glasgow have been compared to theory using MATLAB model. Application of ECD to various 
suspensions (MC, RM, ETM) has been considered: (looking at level of damping to meet settling time requirements and checking thermal noise 
levels). A paper summarizing ECD work is well underway.
  9 
February 06, 2004. 05:34 CST
Caroline Cantley 
Periodic Summary 
Suspensions 
Suspensions Update Glasgow Feb 04 
QUAD SUSPENSION DEVELOPMENT
As a result of the 2004 LIGO plan update development of the triple RM has
been postponed and design effort is being focused on the quad suspensions.
MPL is currently at Caltech for one month to assist in the quad suspension
development. RAL also hopes to assist with the quad controls prototype
development. The aim is to enable the overall suspension development plan to
synchronise with the UK programme requirements for noise prototype
development. (Caltech/Glasgow/RAL suspension teams + NAR (Stanford))
Sensitivity studies have been carried out to determine the effects of quad
suspension parameter changes on noise performance. These investigations are
being driven by other design developments such as ear design (e.g. ribbon
separation). (NAR (Stanford))
 
QUAD MASS CATCHER/ASSEMBLY JIG DESIGN
Over the last six months the GEO triple mass catcher/assembly jig has been
under review to allow development and optimisation of the design for
application to the AdvLIGO triple suspensions. A replica mass
catcher/assembly jig has been manufactured with the help of our colleagues
in MPQ. Due to the 2004 LIGO plan update the work on development of the
triple suspensions has been suspended to enable the quad suspension
development to be progressed more quickly. For this reason our design
efforts have recently been focused on the quad mass catcher/assembly jig
development. The first and current stage of the development plan is to lift
the experience and lessons learned from the GEO triple mass catcher/assembly
jig and use this as a baseline. The design of the mass catcher/assembly jig
must interface with the overall requirements for assembly, installation and
repair of the quad final suspension stage and detailed discussions have
already begun to address these interfaces. (RJ/CAC/GC/CIT/JR/HA + S.
Gosler(MPQ) ++)
 
SUSPENSION SUPPORT STRUCTURES 
Development of support structures for triple and quad suspensions commenced
several months ago. The main challenge is to design structures stiff enough
that they will meet the requirement for a minimum structural resonant
frequency of 150Hz. This has involved FE analysis and basic experimental
modal analysis and is ongoing. RJ visited Caltech for 2 weeks last November
and assisted with this work (CIT/MB/RJ/CAC).
 
CANTILEVER BLADE DEVELOPMENT
Detailed modelling and testing of cantilever blades for application to the
AdvLIGO suspensions has been carried out based on GEO designs. Deflections
within 2% of prediction have been achieved for triple pendulums similar to
AdvLIGO triples. The grinding/lapping/bending process for blade manufacture
has been found to be optimum achieving tolerances in blade thickness of less
than 1%. This work is being continued by RAL under the UK AdvLIGO Project
(MP/MPL/RJ/CAC/RJSG/IW ++)
Preliminary work has also started on the development of silica blades for
improved vertical thermal noise performance in the final pendulum stage.
Preliminary loading tests have been carried out on small silica blades and a
mass of 540g has been suspended using a blade of length 65mm with root width
10mm. Protective abrasion resistant coatings for the blades and improved
attachment methods are currently being investigated. (GC/AH/CAC + G. Losurdo)
 
EDDY CURRENT DAMPING
Investigation of eddy current damping of multi-stage pendulum suspensions
and its application to the suspensions of AdvLIGO is almost complete. For
example, using a 4x4 NDFeB magnet array interacting with a copper block a
damping constant of ~25N/(m/s) was achieved giving a Q~5 for the lowest
vertical mode (0.9Hz) of a GEO type triple suspension. It has been
demonstrated that similar Q's can be achieved for an AdvLIGO triple
suspensions and that eddy current damping would more than satisfy the
systems requirement for a "10 second or less" settling time for pendulum
motions. By extrapolation it has been shown that this technique could be
viable for damping of selected resonances of the proposed quad suspensions
(vertical modes). It is possible that eddy current damping will be used in
parallel with active damping within the final quad designs. Development work
to optimise the design of the damper unit with respect to size and mass has
also been carried out. A paper is almost finished being drafted and will be
submitted to the LSC for review within the next month or so. 
(MP/MB/NAR/CIT/CAC).
 
RIBBONS/FIBRES/BONDING ISSUES
A "preliminary design for discussion" has been created at Glasgow for the
AdvLIGO quad ear. More than one type of ear design will be required for
AdvLIGO and parallel designs will be developed to satisfy the range required
(e.g. quad/triple designs; options for silica/sapphire masses depending on
thermal noise; options to accommodate either ribbons or dumbbell fibres) -
(CAC/JH/GC/SR/MPL).
The impact of the bond area on thermal noise has been under investigation
for the last few months and work will continue on this with the results
being formally presented to the group as soon as the investigation is
completed and fully validated. In the meantime, via telecons and other
discussions the ear designers will be updated on an ongoing basis to enable
ear design to progress. (EE/JH/SR/GC).
 
HIGH Q SUSPENSIONS
Loading tests, violin and pendulum Q measurements and investigation of
wleding and bonding issues are ongoing. Preliminary tests of ribbon breaking
strength conducted at Glasgow were encouraging with up to 1.8GPa being
demonstrated. A very rigid pendulum support system under vacuum has been
used to measure violin Qs. Initial results were encouraging with a pendulum
Q of 1.3E8 measured and initial violin Qs of up to 1.4E8 with a 2.5kg mass
suspended on a 1.12mmx0.12mm ribbon. Investigations of the relationship
between the fiundamental material Q, the violin mode Qs and the pendulum Q
are currently being carried out. (GC/AH/JH/KS)
 
CO2 LASER PULLING/WELDING MACHINE FOR RIBBONS
A change from using oxy-hydrogen to melt the ribbons using light from a high
power laser will reduce the possible effects of water vapour and other
sources of contamination on the ribbon and will enable control of the ribbon
profile to a much higher level of precision. We have already demonstrated
the welding of ribbons using illumination from a 9W CO2 laser and work on
the development of a laser pulling/welding machine based on a 100W laser has
recently started. (GC/CAC/DC/RJ/JH + J. Bogenstahl)
  10 
February 06, 2004. 09:32 CST
Joseph Giaime 
Periodic Summary 
Seismic isolation 
Seismic summary, LSU and LLO, and a some of Stanford. 
LSU / LIGO Livingston SWG update, 6 Feb '04:

HEPI:

Preparations and R&D for the external hydraulic pre-isolation retrofit at LLO are essentially done, and installation is beginning. Jonathan Kern, after many months of hard work on the retrofit project, is leaving for a new opportunity, and Rich Abbott has ably taken over the engineering lead. Today (during our SWG call, in fact) the pipe fitting contractor and Rich are meeting at LLO getting ready to start the fairly extensive piping that will connect pump stations in our mechanical rooms with the actuators on the tanks. A supply of mostly-assembled actuators is ready, and last-minute glitches in the proportional-valve calibration stand are being worked out. Earlier this week, Ken Mason, Oddvar Spjeld and Joe Lacour spent time at the external housing vender doing a fit-check, which went well. Next week we will convene at LLO, work out the remaining details of the installation procedure, and have an installation readiness review on 11 Feb. At MIT LASTI, Rich Mittleman, Pradeep Sarin, Myron Macinnis, and others have mostly re-installed HEPI on the BSC (and await calibrated valves from LLO). Rich has been studying the effect of an external stiffening beam on the HAM system (we will not likely use it), and Pradeep has implemented the control and sys-id system using the VME-based DAQ/DSP system that we will use at LLO. At Caltech, Rolf has completed testing of the software and hardware design that will be installed in LLO later this month. 

Meanwhile, Brian Lantz has been remotely supporting both the sys-id/controls effort and the fabrication/installation planning, wearing out his telephone and matlab fingers. We look forward to a visit by Brian to give a hydraulics mini-course to our staff. 

If anyone wants more details, please sign up for the SEI notebook. 

Advanced LIGO SEI:

At Stanford, Wensheng Hua and Joe van Niekerk have been debugging the ETF tech demo platform. Since our last SWG update, they have found and replaced faulty actuators that caused rubbing, which was discovered by analyzing non-linearity in the response, and have recovered from the radio-transmitting power supply that LLO sent them. 

Hua used this platform to refine his design of a polyphase FIR filter that allows better phase and amplitude matching for feedforward (AKA, sensor correction) based on ground noise measurements, a design that will likely be used in the HEPI system at LLO. Work on the platform continues, now focusing on its Advanced LIGO use. 

Larry Jones and our mechanical contractor, ASI in Pasadena, have been working hard on designing the LASTI SEI systems. Larry and the UHV testing folks at Caltech have been laboring on the difficult task of specifying the materials and fabrication methods for the UHV actuator, as well as the even more difficult task of convincing our supplier to make them our way. 

Joe


Pre-stabilized Laser

From: Peter King <pking@ligo.caltech.edu>


    I have partially clarified some line items in the LZH laser budget that
related to hardware quantities.  The changes have not yet been incorporated
into my cost estimate.  Other smaller matters I hope to clear up during the
working group telecon..

Input Optics

No report.

Core Optics

From: "Erika D'Ambrosio" <ambrosio@ligo.caltech.edu>

I started FFT simulations of LIGO II with very curved mirrors.
The first problem I encountered is related with the maximum angle
that the paraxial approximation can represent for a given grid.
In analogy with the diffraction angle due to the waist size and propagation:

theta_diffr=lambda/(pi*w_0)

there is a maximum angle that can be reproduced, due to the fact that
we are not able to model a light beam whose transverse size is smaller
than the pixel size and therefore there is a maximum angle that can be
generated by propagating the light represented by a map with finite resolution.

That corresponds to the angle

theta_max=lambda/(pi*delta_x)       (*)

formed by light diffracted after a squared aperture of size delta_x=delta_y.

For this reason, I asked Hiro to compile a version of the FFT-code
on the cluster of personal computers he manages, as decreasing the size
of the pixels means larger running times for each simulation. This is only
necessary for simulating LIGO II with R.O.C.=2076m, since w_0=1.15cm compared
to w_0=3.51cm in LIGO I. No problem has been found in running simulations
for R.O.C.=54km since w_0=5.88cm.

I talked with Hiro about all this and he agrees with my interpretation,
although there is something more I have to understand on the anti-aliasing
filtering techniques. I fear that is subtracting more power than it should
and I want to test different sizes for the window.

(*) In the thesis by Dr. Brett Bochner the maximum angle
    is a result of the size of the grid too:

    theta_max=lambda/(2*delta_x)

    and it is related to the limit of the Fourier representation
    of the propagation.

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

AdvLIGO Coatings

CSIRO
On a second trial run, CSIRO had a problem achieving the required uniformity due to the malfunction of a uniformity mask during deposition.
I'll be visiting their facilities next week.
************************************************************
Fused silica studies
Silicate bonded a second ear on a fused silica substrate and shipped it to Steve Penn.

Auxiliary Optics

No report

Interferometer Sensing and Controls

No report

Data Acquisition, Diagnostics, Network & Supervisory Control

No report

Other Laboratory R&D

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

Hareem
sent paper on Maraging springs quality factor for internal review. the draft is available at
http://www.ligo.caltech.edu/~htariq/ric/maraging_hysteresisLRP.pdf
please send any comment to Hareem.

Riccardo
prepared an animated presentation on Advances  in Passive Seismic Attenuation Systems
you can find it in
http://www.ligo.caltech.edu/~desalvo/presentationLIGO-G040029-feb-04
it appears both in mac and PConly version which should allow you to watch the movies on both platforms.
If you have trouble, please watch the movies (also in the folder) independently.  They will amuse you.
Some work on glassy metals.

Maddalena
out for exams, visiting INSA Lyon to coordinate Maraging measurements.

Barbara
out for exams, visiting LMA Lyon to discuss manufacture of mexican hat mirrors.

No Mesa profile interferometer meeting, the mechanical design of the interferometer should be ready this week,   Pricing shortly later.


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