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The LIGO Executive Committee Agenda for Monday November 10, 2003 will be:
CANCELLED DUE TO LSC MEETING
no report
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.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
ACCOMPLISHMENTS (This
report reflects activity for the past month.)
ACTIVITY
| 11/06/03 | Packages | Faxes |
| In | 24 | 24 |
| Out | 13 | 32 |
Press here to access the DOCUMENT
CONTROL CENTER WEB PAGE.
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA.
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
From: irena@ligo.caltech.edu
(Irena Petrac)
Status on LSC updates:
ACIGAWill fill in the LSC Excel update status sheet for weekly status by tomorrow..
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
From: Ed Jasnow <jasnow@ligo.caltech.edu>
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
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.
Progress Reporter - http://www.projwebsite.com/GroupServerP3e/en/ Login using Username: admin and Password: admin.
Static HTML Example - http://ligo.caltech.edu/~tfrey/SUS_WebProj/ (AdL Suspensions Only) NOTE: This is after importing and before any data corrections.
Static HTML Example - http://ligo.caltech.edu/~tfrey/DAQ_WebProj/ (AdL DAQ Only) NOTE: This is after making adjustments to the WBS so that it displays as expected.
Finalized travel arrangements for attendance at meetings at Livingston as requested by Carol Wilkinson.
AOS - Still need completed WBS dictionary and BOE.
IO - Still need completed WBS dictionary and BOE.
SUS - No action items pending. Worked with Janeen and Calum preparing revised progress data / ETCs. Janeen provided the ETCs and I will review with Carol.
SEI - No action items pending. Posted updated SEI schedule with progress through 09.26.02.
LDAS - No action required at this point in time.
INSTALL - No action items pending.
DAQ - No action required at this point in time.
PM - No action required at this point in time.
FAC - No action required at this point in time.
SUP - No action required at this point in time.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
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.
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).
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
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.
no report
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.
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.
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.
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.
no report
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.
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.
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
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
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
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 Pdf. More
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)
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