Weekly Report for Week Ending November 6, 2003


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

The LIGO Executive Committee Agenda for Monday  November 10, 2003 will be:

CANCELLED DUE TO LSC MEETING


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Saulson)


no report


Laboratory Administration (Lindquist)



 

LIGO Weekly Site Telecon (Lindquist)

There was no site teleconference held Thursday, November 6, 2003.
The list of current actions revised to reflect the status of open actions assigned through October 30, 2003 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

From: Ed Chargois <chargois_e@ligo.caltech.edu>


DOCUMENT CONTROL CENTER (Turner, Mak)

>From: Linda Turner - turner@ligo.caltech.edu>

ACCOMPLISHMENTS (This report reflects activity for the past month.)

> From: Cleveland Mak <mak_c@ligo.caltech.edu>

ACTIVITY


11/06/03 Packages Faxes
In 24 24
Out 13 32

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)
Status on LSC updates:

Still missing in action/reminds e-mailed again today:
ACIGA
CACR (have given up on this group)
CEGG (Prof. Drever promised)
Dominguez Hills (PI promised)

Goddard (sporadic)
LaTech
LSU (group very busy at LLO)
Michigan
Oregon (promised)
Southern University A&M (promised)
Wisconsin-Milwaukee
Washington State

Will fill in the LSC Excel update status sheet for weekly status by tomorrow..

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 Friday 10.31
 

 

Accomplishments:

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
Continue to update the 40-Meter Schedule and incorporate any changes. Continue to update the TNI Schedule and incorporate any changes. Continue to update the LASTI Schedule and incorporate any changes.
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)

A pointer for a draft Final Report for Cooperative Agreement NSF PHY-9210038, the cooperative agreement that covered construction, installation and commissioning, and initial operations of the sites, has been distributed for internal review.  The draft has also been placed on the web page for the NSF Review committee.


Change Control/Contingency (Lindquist)

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

CR-030017 proposes to upgrade the LIGO Laboratory Wide Area Network (WAN) at Livingston from 2xT1 (3.088 Mbps) to Gigbit Ethernet (1000  Mbps) at a cost of approximately $217K through 2006.  This change request was discussed and approved during the Executive Committee Meeting on Monday, October 27, 2003.  Minutes have distributed (LIGO-M030197-00-P). 


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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



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


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

The opening week of S3 saw some excellent stretches of locking on both interferometers, and a few mysteries, as well.  Duty cycles to date, longest lock stretches, and mean inspiral ranges are 73%, 20.5 hours and 2.4Mpc (H1), and 63%, 13 hours and 0.9Mpc (H2).  Note the longest lock stretches completely overlapped, for nearly 13h of dual science data.  As in previous runs, operators and scimons have been manning shifts around the clock, however, for this run there are no (well, few) training scimons.

The atomic and gps clocks show stability to better than 100ns.

Fake pulsar signals (five public and five hidden ones for blind analysis) are being injected near-continuously into both IFOs (later, on dedicated h1 and h2 machines).  PEM injections have also occured.

Up-to-the-minute figures of merit, uncalibrated noise, excitation waveforms and site overview screens are available as JPGs at the CDS site http://blue.ligo-wa.caltech.edu .  Data
dropouts have been observed on DMT figures of merit, some of which were traced to overloading of DMT machines, others due to disk and RMF problems (datapusher fix here).  We would like to see the LLO state vector and range plots, but technical difficulties have prevented this data transfer to date.

One of the persistent mysteries of the first week of the run has been, why is the 4k inspiral range unstable?  Range estimates are about a factor of five noisier on the 4k than the 2k, despite both machines having full (dc) WFS applied.  Along with the extra hash, the range wanders on hour timescales between 1.5-3.0Mpc.  Saturation of the SPOB photodiode was suspected to be occuring, however, reducing the light via ND filtering on the appropriate photodiode had no effect on the range noise.

Wednesday proved to be difficult locking, particularly on the 2k, which had some input pointing issues.  A 2k mystery is why the high frequency noise (normally the quietest in displacement of all three IFOs at hf ) has risen.

Causes of lockloss include seismic transients traced to our nitrogen dewar.


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



 

no report


DETECTOR SCIENCE & ENGINEERING

Seismic Upgrade Project

see also the LASTI report for HEPI experiment and control system development progress
(Jonathan Kern is on vacation; no report this week on production status)

Rich Abbott

1.  Continuing work on the seismic interface chassis.  Now that the science run has started, I am able to get a bit more time to work on the HEPI stuff.  I am considerably behind schedule at this time, I estimate that at best I am 3 weeks behind.

2.  Received the GE motor drives and forwarded them to Excel.  Excel is handling the packaging of the HEPI motor controllers at my direction.

3.  All materials are in for the valve calibration units.  Mike has put together one of the amplifiers, and we tested it.  It works fine.  Next step is to hook up a differential pressure sensor and complete the testing.

Ken Mailand

The drawings for the pump station manifold are at the shop, I'm continuing the details of the resistor internal parts and the 3 micron filter attachment plate. The motor mount plate and the manifold mounting brackets will be in the shop by Friday. I'm waiting for vendor dimensional prints on the VCO face valve and  flex connection joint to finalize the shop drawings for their of parts group .

I have selected a frame base foot and caster and electrical box, and will have the frame details in the shop next week. The motor / pump adaptor is in the shop for modifications we need, to mount the 3 axis accelerometer sensors and provide a drain for any fluid weeping by the pump shaft seal. I have contacted the granite base vendor and I'm waiting on information on pull out strength as well as available options on threaded insert style and materials. The 3 accumulator quotes are expected in by Friday and parts can be ordered; the factory indicated the lead time would be about 4 weeks. Detail parts to design are the docking assembly and the pump station valve plate and drip pan.

CDS

see also the CDS meeting minutes in the commissioning archives:

CDS Software

no report

CDS Hardware

nothing significant to report this week

PSL

PeterKing
The phase modulator was installed in the 10-W laser and the laser was
re-aligned.  During the alignment phase the laser power increased from

9.4 W to 10.5 W with a small deterioration to the beam profile.  The mirror

after the amplifier was then adjusted and the laser power increased to

11.1 W with an improved beam profile.  The astigmatism did not change from

prior to installation of the phase modulator.

Following on from problems experienced at LLO with the laser power monitor,

I had wondered if the drift problems were not in part due to the 8-bit ADC

in the laser power supply combined with the low output voltage of the

photodiode.  Although the photodiode output was similar to the LLO monitor,

I did not know the monitoring output at a point on the circuit inside the

laser.  This monitor voltage can be adjusted by a trim pot.  Probably the

best answer would be to simply replace the photodiodes altogether.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang
OTF Lab. (W. Bridge)
Contamination Cavity # 1 

This cavity is locked, power recovered as before.

We have introduced a new sample into this chamber, the solder for the OSEM assembly.

RGA, Ring down and beat frequency measurements in progress. 

Absorption Test Measurement prototype in progress 

The new 30 watts laser from Quantronix. is ON !

We have re-installed the laser on its new base bench.

Optics set up is in progress.

Scatterometer system in progress

The new base to house the larger Sapphire mirror has been finally completedand

installed. New base plate to hold the original Fused Silica ITM is under fabrication.

The new optical plate that holds the RTS head is completed and installation is in progress.

New optics preparation, replacement and installation is in progress.

A simple AR coating model has been done on the 2ITM04 mirror,please see the attachment sent by

Dr. Liyuan Zhang.to find some preliminary results.

OTF Lab at Lauritsen ROOM 38

Cavity #3 

This chamber is locked. We are taking ring down and beat 

frequency measurements every day as well as new RGA measurements .

Cavity #2 Test cavity in STANDBY.

Misc.. task, arrangement of the lab at Bridge to accommodate the new laser table.

We encounter a computer situation as the computer network(Sun station )does not want to support 

the old GPIB Interface box.This is and old and complicated configuration that Larry are helping uswith.

Most likely, we need to upgrade to windows as we did to the scatterometer system.


40 Meter Interferometer (Weinstein)



 



Thermal Noise Interferometer (Libbrecht)


Last week we reported a measurement of coating thermal noise. This week
we have broken down several different noise source contributions and
shown that they do not account for the noise floor. (See the plot.below).

Also, we have performed two additional tests on the data to rule
out unknown noise sources before or after the cavities. First, we
varied the laser power and looked at the total noise in the instrument
at two separate modulation depths. The total voltage noise scaled
linearly with the power, ruling out shot noise or electronic noise in
the photodetector and subsequent measurement electronics. This, and the
fact that the Pound-Drever-Hall discriminant is proportional to the
laser power, indicates that the equivalent length noise is independent
of laser power.

Second, we varied the modulation voltage applied to the arm-cavities'
Pockel cell. Again, we found that the equivalent length noise was
independent of the modulation depth, as expected for fluctuations in
the arm cavities' lengths as opposed to, say, phase noise introduced by
the Pockels cell. (Thanks to David Shoemaker for pointing out this
possibility.)

These two tests, along with the measurement of the servo noise shown in
the figure, indicate that the noise originates inside the cavities, and
not before or after them in the servo or measurement loop. This,
combined with the fact that the noise floor between 500 Hz and 20 kHz
is incoherent between the two cavities, provides strong evidence that
our noise floor is dominated by thermal noise and not some other,
spurious noise source.
 


LASTI (Ottaway)


no report


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Yamamoto)
 

>> Commissioning support
Matt worked at LLO on ASC system (QPDs, WFS3 and WFS4), and scripting tools
(ezgain, ezlockin).
Biplab is on S3 shift at LHO.
 

>> Linear noise Model
Matt has been working on a linear noise model to analyze the sensitivity.
He has sent out first version of LinLIGO, a linear model of the initial LIGO detectors
to limited parties.
 

>> Mechanics modeling
There was a biweekly teleconference of the mechanical simulation on Wednesday.
Cella, Virginio, Mark Barton and Hiro attended. Virginio showed a measured
transfer function of a simple blade which will be used to validate the MSE blade model.
A few test programs of MSE have been discussed which showed apparent bugs to be fixed.
Cella and Virginio will address the problem this week working together over phone.
Mark has built a LIGO I like simple suspension model which can be used to validate the
MSE model.
 

>> FFT
Hiro has replaced the Fast Fourier Transform code in the FFT model by FFTW v3.0.1 and
the speed was further improved by 40%. Now the speed is entirely dominated by the
speed of the actual FFT calculations for the field propagation.  The speed of FFT program
on linux box is almost 10 times faster than the same job on the SUN box using the original code.
 

Hiro tried to use multiple threads to further speed up the calculation, but, for some reason,
no speed gain was achieved. Multi threads can be used, but the gain of using multiple threads
is somehow waisted somewhere.
 

The comparison between the FFT and the e2e calculations for the same LIGO I configuration
showed some sign difference. Biplab is looking into this problem.
 

Aside from this sign issue, the code can calculate 3 pick offs, POB, POX and POY.
 

>> Modeler code
Melody and Hiro have been working on the implementation of the C++ based FUNC,
taking the comment of Matt into account.
 

The interface design is underway which allows to implement easily a simple case like
out0 = PI*in0;
as well as to implement a code which takes full advantage of using the C++ compiler.
 

The infrastructure testbed has been implemented to demonstrate the basic design.
The compilation is needed only for those which are modified since the last build of
the shared library.
 

>> SimLIGO run
Xiao is running SimLIGO to test the effect of the arm offset (wrt to the beam axis).
He is installing the latest version of JAVA on his linux box to use alfi.
 

Hiro is studying the mysterious excess noise at around 100 Hz predicted by SimLIGO
by building a simple box, TestSeis, which contains only the seismic motion and the
LOS box. Several people had hard time to use these modules, so more comments will
be added to boxes to clarify the usage.
 

LIGO Data Analysis System
 

Software Systems (Blackburn)
LDAS continues to run very well at the sites during the science
run. This is particularly true of the createRDS commands that are
generating the Reduced Data Sets that are being moved back to
Caltech and on to the Tier II centers. A few dataPipeline jobs
have been submitted at LLO and LHO for waveburst and knownpulsar
search codes. But the full onsite searches have not begun. It
looks like that may be delayed until next week. Also a new release
of LALwrapper will be needed before some of the planned onsite
searches can begin. With the LSC meeting next week, it looks
like this will be more likely to begin late next week at this
point.
 

A small patch to the mpiAPI was placed at the sites this week
which corrected a problem with wrapperAPI-master processes being
assigned to nodes on the cluster when they should not have been.
This didn't cause any issues in nominal jobs, but would have
caused debugging and tracing confusion without the patch in a
job that was behaving poorly.
 

The LDAS software is currently based on the TCL 8.3.5 release. The
current release is 8.4.4. Until recently, we have experienced SWIG
wrapper issues with post 8.3.5 TCL. This week we made significant
progress towards wrapping up C++ code with SWIG for the newest TCL
release 8.4.4. This new release has fixes for several problems we
have routinely seen in LDAS.
 

A few minor changes were made to the build-ldas script to allow
more flexibility in the selection of compiler options.
 

The FrDump6 utility that is used to look at the contents of frame
files was "polished" up a bit this week.
 

Changes were made to the mpiAPI and the wrapperAPI to decrease the
amount of diagnostic information logged at runtime.
 

The official release of STLPort (version 4.6) came out this week.
We began testing it within LDAS on Monday. There may be a memory
leak exposed by this version of STLPort. We will follow the memory
usage over the next week to determine if there is a problem or not.
We have also backed out our home growned STL::String class in LDAS
in favor of the true STL::String class provided by STLPort. The
STLPort version is just as stable in a threaded environment as the
one we had to develop just in time for the science run AND is
definitely far more stable than the GCC version of this class. The
STLPort library comes with the option to use different memory
allocators. We are experimenting with these to see if any are
superior in performance on Solaris and/or Linux.
 

We have begun a pilot effort to provide graphical presentations
of the results in the database using the controlMonitorAPI. This
will help with system testing of LDAS and may also have a role in
the monitoring of science results during the science run in the
control room.
 

Hardware Systems (Wilson)
LHO
Ben Johnson
1) Replaced T3 disk u1d9@t3-8. Disk reconstructed without mishap.
2) Storagetek came and replaced the 3rd 9940B tape drive in the L700. He
initially installed and powered on the drive, without unlocking the drive
head. Drive would not initialize properly until the head was unlocked.
3) Replaced motherboard on defiance/datagateway Linux IDE RAID box. The box
booted successfully and sees all of the original devices.
4) Developing and testing new features in the disk2disk copy script. The
script should now automatically attempt to recover missing files from the
backup framebuilder when it sees data gaps or if no new data has been
written for a long time. I have also added the capability to run FrCheck on
each file and report any errors.
 

Greg Mendell
1) Started archiving full-frame S3 data, and generating level 1, 2, and
3 RDS frames.  RDS frames are being archived onto tape as well.  Each week
tapes with full-frame data are being sent to CIT, and tapes with level 1 RDS
data are being exchanged between LHO and LLO.  The level 3 RDS data is being
pulled over the internet to CIT, for distribution to tier II sites.
2) There have been some problems with tapes and tape drives at LHO.  The
system is redundant and this has not caused any significant problems with
archiving or RDS generation.  We are working to fix the problems.
3) Archived preS3 stochastic injection data.  Currently creating a L2 RDS of
this data for the stochastic group.
 

LLO
Igor Yakushin
1) Restored all the old databases at all the sites.
2) Restored DB2 installation at MIT after the disk crash.
3) Configuring sites for regular database backups.
4) Archiving raw S3 data, creating L1,L2,L3 RDS is going fine.
 

MIT
Keith Bayer
Completed work on pcraid series 2 motherboard replacement doing cabling and
setup for two more racks of cluster nodes (45-87) rebuilt metaserver after
failed drive LDR setup work
 

CIT
Hari Pulapaka
1. Published S3 L3 rds data from the sites.
2. Migrated the LDR installation to ldas-cit from ldas-cit-g
3. Developed a new script for publishing the data with some improvements on
performance.
4. Wrote a new storage module for ldas.mit.edu, setup LDR at MIT and now S3
data is flowing to mit using LDR.
5. Installed some parts of globus again on desktop, as there were problems
created during hte upgrade.
 

Dan Kozak
Imported tapes with S2 L1/3 RDS at observatories.
Set up S3 directory structures and archive sets at observatories.
Electronically labeled tapes at both sites.
Transferred pre-S3 full frames from observatories to CIT successfully.
Recovered bad file in archive from old tape.
Helped sites with tape problems.
Set up web monitoring of files remaining to be archived at sites.
Worked to figure out slow frameAPI performance...
 

Data Analysis Activities (Lazzarini)
Lazzarini:
Wrote a note on optimally combining the two Hanford interferometer data streams
with the Livingston stream when it is known that the H1, H2 machines have
intstrumental cross-correlations.
See http://docuserv.ligo.caltech.edu/docs/public/T/T030250-01.pdf
 

Mendell:
Mike Landry and I are working hard on the stackslide code.  We have done
a preliminary analysis of the pulsar injections in the E10 data for the
first 5 pulsars, stacking the data only, but not sliding.  The results
look good, so far.  That is, we see the injected pulsars that we
expected to see.  However we need to do a more in-depth study to make
sure we are getting the proper SNR. We are working to get results with
sliding by the PULG F2F this Sunday, Nov 09.
 

Yakushin:
1) Ran simulation to estimate waveburst sensetivity to BH-BH merger
depending on strain, direction and black hole mass..
2) Preparing waveburst presentation for the LSC meeting.
 

Sutton;
- Looking at the E10 hardware injections.
 

General Computing (Wallace)
MIT:
(Keith)
-Replaced emvogil-3 hardware - bad board or cpu
 (after trying just about everything else I could think of)
-Investigating cisco wireless hub to solve problems with
 mini-pci wireless card access failures (IBM & Mac laptops)
 

Livingston:
(Shannon)
-Still working with the new file server.  I have been trying to tweak the
performance issues for a Solaris NFS client and a Linux server.  I have
started by changing the rsize and wsize on the Solaris client.  I will
start tweaking settings on the Linux server tonight.  I will mail out
the performance numbers when I get them all compiled.  I have also set
up RAID 10 vs. RAID 5 on the file server.  Because of the instability
that I experienced in the first two weeks, this gives me a little extra
peace of mind due to the added redundancy.
-Shuffling some files off of our existing file server to the new file
server to free up some space.  Most of these are archived files that are
not being currently used.  I have also burned some of them to DVD for
archival purposes.
-Still working on recompiling all of the gnu and GPL applications on the
new file server.  This is a time consuming process since each one has to
be compiled individually and at last count there were over 100
applications compiled in the existing directories.  I am also employing
the gnu stow software to aid in future updates for software.
-Placed an order for a replacement machine for our web server.  The web
server currently is an Ultra 10 which is aging and is also short on disk
space.
-Received a quote from Sun for some additional software in their Sun ONE
line.  This includes a web mail server and a calendar server, among
other things.
The usual round of patches, ordering parts/computers for people, support
etc.
 

Hanford:
(Christine)
 

- Installed a new wireless access point that does both b and g
standards, which is  11 Mbs and 54 Mbs at 2.4 GHz.  This will be
available in the auditorium during the LSC meeting.  I plan to upgrade
all the wireless access points to at least the b&g, possibly the a
standard, which is 54 Mbs at 5 GHz.
- Most of the week has been spent getting ready for the LSC meeting.
- The usual user support.
 

CIT:
(Mike)
-Worked on Calum Torries computer. He is having problems with all
applications and I cannot get the new video card to work with solid
works. This computer seems to be having a memory/motherboard problem.
-Worked on the printers up on the 3rd floor of W/B; mostly paper jams.
-Worked on VRVS. I setup a meeting with Veronica running the share
option within VRVS. This approached seemed to have worked as far as
being able to read the speakers presentation.
-I worked on loading a visitors workstation that is currently running
win98. I am loading a workstation that is a lot faster and will have
2000 pro loaded.
-I worked on Cindy's new laptop. The internal wireless card seems to have
taken a dump. I called Dells tech support on this and after a few hours
of running diagnostics with them they have decided to send me out
another wireless card.
I have received the wireless card and swapped it out.
-Worked on all NTSRVs getting all end of month ghost backups.
-Worked on Antares troubleshooting DCC database. I used the access tool
that was designed to troubleshoot the database/drive mappings. This tool
works.
-Setup two laptops and got them ready to ship out to Hanford.
(Angelo gave me a hand with this)
-Worked on writing up Angelo some installation notes for General
Computing Workstations.
-I worked on finishing up loading Janeen's new laptop with GC software
and multiple engineering packages.
-Searched for a compatible video card for solid works that will work
for Calum Torrie & Ken Mailands computers. This is an additional video
card to implement a dual monitor system per workstation. I spent a lot
of time with this, due to a good percentage of the video cards according
to solid works HCL are APG cards. This slot is already taken by the
original video card. This forces me to look for a pci card that works
with solid works. I found a dual head AGP video card that is compatible
with solid works. This should take care of the problem. I will be seeing
about ordering this card through Larry Wallace.
 

(Veronica)
 

- A good portion of the week was spent producing a video of beamspot
scatter for Bill Kells. Combined trimmed clips into a single movie. I
captured it in different formats to see which one gives the best playback
on his laptop. Bill needed to download the upgrades of his media players.
Working on making a compressed version that will play back on his slower
machine without compromising too much quality.
Captured and compressed a video of last LIGO seminar by Karl Gebhardt. The
video was posted online for streaming within 2 hrs of the talk. Set up and
monitored VRVS for the talk. Downloaded the latest VRVS/VNC package on
Karl's laptop. This required a trip to Carnegie observatory where he was
stationed. As Mike reported, the broadcast went well, we received a 'thank
you' from Pisa.
Helping Karen Willacy of JPL with setting up a document database for LISA,
similar to our DCC. Meeting with her to explain the 3-tier application
architecture and practical implementation.
Updated the personnel roster. Updated the LIGO website.
- LSC website: Posting updates to the LSC meeting website.
 

(Bruce)
* (BS) Systems Work:
       - Continuing work on Ilog upgrade to implement entry
         editing features.
 

(Lisa)
- Started monthly backups and verified the dailys.
- Continued evaluating a new anti-spam package.
- Cleaned up random tasks that accumulated while I was out of town.
 

(Larry)
-Spent time going over a number of procurement related issues. Paperwork for the
Pcard system has really been taking up some time. Along that same line, I
discovered that those who have real old versions of the P-card s/w will need a
couple of files changed. On Oct. 25th, the P-card server was changed and the
older s/w needs to be updated by hand. Most of the LIGO people will be OK but
there are a few of us that this does affect.
-Assisted the E2E group on a number of computer setups and moves. One of the
computers appears to have a h/w problem but that will not be resolved for a few
more weeks.
-Worked with Christine and others on a couple of logistical issues for the LSC.
-Assisted a number of users with different PC related issues.
-The regular setting up of accounts and helping end users work out their
configuration issues.
-Continued working on the server system in the 40M. The OS is loaded with the
patches but now there are a number of configuration issues as well as the
in-house s/w loads that still need to be addressed.
 


Advanced LIGO and supporting R&D (Shoemaker)


Seismic Isolation

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

Actuator Testing and Redesign:

The wound bobbin for the small actuator was cleaned and vacuum baked at 204C for 120 hr; an RGA scan was made, which did not meet LIGO requirements. When the oven was loaded and heated for the next run, one of the three heater circuits (the door heater) was found to have a blown fuse. This could have had an effect on the adequacy of bake for the bobbin. We're now considering what should be the conditions for a vacuum re-bake. The 204C temperature of the first bake did not cause any problems due to differential thermal expansion (Cerabond cracking or wire "pinching").

The small actuator's frame and (epoxied) magnets were cleaned and placed into vacuum bake at 80C for 48 hours. These conditions were chosen as the default bake for LIGO magnets. The post-bake RGA scan did not meet LIGO requirements. We've since found that the magnets are Sumarium-Cobalt, good for at least 150C. A vacuum re-bake at 150C for 120 hours was started on 10/31.


Suspension

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



Working with various suspension team members on a top-down progress report for the preliminary design phase. Preparing for the NSF review.


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

Recycling Mirror suspension
A have completed the parts, drawings and assemblies associated with the test mass assembly for the RM suspension. The only addition required is a recess for magnets for global control (I am not sure what size of magnet is required? diameter?)
MPL, Alastair Grant and I are continuing to consider designs for the pitch adjustment ant the addition and removal of mass.

MATLAB model
Norna and I met on two occasions this week to discuss several action items related to the QUAD, RM and MC parameter files. At present the modelers plan to meet weekly at the end of the SUS meeting.

Coils
A summary of the coils required for the controls prototype at LASTI was discussed at the weekly SUS meeting. As a result Glasgow will go ahead and order the hardware required to make the 3 main parts associated with each head.

Eddy Current Damper
Mark Barton and I worked in the laboratory testing several eddy current damper designs on a suspended 6kg mass. Full report to follow, as experiment had to be re-done due to unexpected coupling of modes. This problem has now been fixed and a new set of data recorded. Mark and I met with Norna, Caroline and Mike Plissi to discuss the final stage of a joint paper on this and related subjects.

ETM (BTF)
Ian Wilmut and I held introductory discussions on several concepts he had devised for the proposed RAL Blade Test Facility. Aspects of this discussion will be brought up at next weeks SUS meeting. A plan of action of how to proceed with respect offering input to this work and who should be involved was discussed with US and UK members of the SUS team this morning.

Visits
Russell Jones will visit Caltech from the 11th to the 25th of October. Janeen and I have written a plan of work for his visit.
CalumTorrie

Fasteners: Galling and Dust
Larry and I met with Mike Gerfen this week to talk more about our plans for an experiment to look into galling and dust in fasteners. We composed a small document with our plans and an estimate of the time it would take to do the work. Mike is going to get back to us next week with his ideas and hopefully an idea of the cost, so we will keep you informed. I guess if it is suitable, and cost effective, we could get Mike and co to do it with support from Larry and me?

SolidWorks
Go Engineer have been persuaded to offer us 2 hours of software support to write a small macro that will make the additions that MPL and I have recommended for SolidWorks easier to use, especially in association with PDM Works and Push Button PdfMore info to follow. All of the SolidWorks accessories are available on the DCC and are referenced in T030143-02. (More up to date versions of these referenced documents are also on the DCC: - D030382, D030383, D030384)



Core Optics

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


Research on Teflon AF

Teflon AF Type 1601 - 18% solution was applied to the silica fibers on the GEO suspensions to damp certain violin modes . We'll probably need to do the same on Advanced LIGO.

The extractable fluoride levels on this product should be less than 1 ppm; higher levels will etch the fused silica fibers overtime.

After lots of contacts made at DuPont, we'll be buying some of this material to be tested at JPL for the presence of trace HF.
The way they'll approach this would be as follows:

1.      Extract the material into a hot, buffered water solution.
2.      Perform trace fluoride analysis using Ion Chromatography.

The lab has an Ion Chromatograph that it is used frequently. It is extremely sensitive and quantitative. A 1 ppm (or less) level of extractable HF should be readily detected and measured.

We'll RGA test a sample to confirm that the overall outgassing level from all AMUs is within limits, as directed by Dennis.

Test on the LIGO optical contamination cavity may follow, however, this product is very expensive about $1,580 for 100ml.

Research is ongoing.
 



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