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The LIGO Executive Committee Agenda for Monday November 17, 2003 will be:
CANCELLED DUE TO NSF REVIEW
no report
LIGO Weekly Site Telecon (Lindquist)
There was no site teleconference held Thursday, November 13, 2003 (LSC
Meeting in Hanford).
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
| 11/13/03 | Packages | Faxes |
| In | 29 | 28 |
| Out | 9 | 30 |
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>
From: irena@ligo.caltech.edu
(Irena Petrac)
LSC MOUs / Attachment Updates
and Prog. ReportsACIGA:
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
ADVANCED LIGO
(Cost Schedule Control Systems) T. Frey
From: Thomas Frey <tfrey@ligo.caltech.edu>
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.
AOS - Still need completed WBS dictionary and BOE.
IO - Still need completed WBS dictionary and BOE.
SUS - No action items pending. Started review of revised progress data / ETCs.
SEI - No action items pending. Prepared notes from meeting and sent them to Carol.
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.
Corresponded with Roster Database users regarding issue with Seiji's name on the LIGO roster.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
Nothing to report..
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 |
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Summary of S3 Activities at LIGO Hanford Observatory (compiled by M. Landry)
The LSC visited Hanford this week for the November meeting. Face-to-face
sessions
kicked off Saturday (stochastic) and Sunday (stochastic/inspiral/pulsars),
followed by
the standard battery of LSC talks during the week. Thanks
to Terry Gunter, Christine
Barker, Richard McCarthy, Linda Turner, Marie
Woods, Terry Santini and Co.,
Larry Wallace and others for the fine organization,
logistics and catering.
The first week of the science run saw considerable commissioning-like
activity (at least
by science run standards), with excursions into the LVEA and noise
budget studies
that had the 4K out of science mode for several hours at a time.
This week was
intended to be more typical of quiescent science mode running, with
reduced emphasis on
tweaking, however, small fixes were still underway.
A simulated stochastic background signal was added to the pulsar waveforms
and injected
into all three IFOs simultaneously. The correlated noise corresponds
to an Omega of
unity, and should contribute to the AS_Q noise budget at the level
of the LIGO-I SRD.
The signal was added for ~5 hours and then discontinued.
Hundreds of burst waveforms and some inspirals were also injected.
Earthquakes and incredibly high winds, gusting in excess of 60mph, unlocked
IFOs
midweek.
AS_I non-linearity and upconversion was investigated.
The 2k remained locked for ~19 hours today, its longest stretch of S3.
The variable range observed in the 4K Sensemon output is a product of
the non-stationarity
of the raw AS_Q noise. Periods of low range correspond
to high noise in band-limited
AS_Q channels. Ranges continue to vary between
1 and 3Mpc.
Noise budget measurements, such as PD shot noise levels, performed with
light bulb
calibrators, were performed on H1. DAQ coil outpt noise measurements
were made on
all 4K test masses, and are documented here.
---------------------------------------------------------------------
S3
--------------------------------------------------------------------
The L1 interferometer has mostly stabilized after a rocky S3 start.
We still have remnant issues with calibration and DMT monitors, most
resulting
from the frantic push to restore the interferometer to operation during
what
should have been the E10 engineering run. These should all be worked
out
by the end of the week.
Science uptime was limited in the first week of the run due to catch-up
commissioning
activity each night until Friday 11/7. Uptime has now begun to
slowly approach the
"theoretical maximum" given our daytime anthroseism, earthquakes, and
nightly trains. We really need HEPI; fortunately it's on track (see
below).
Scientific Community (Abbott, Frolov, O'Reilly)
---------------------------------------------------------------------
We hosted a tour for about 75 members of the Southeastern University
Research Association, the governing body for Jefferson Laboratory and
other national research facilities. We received many highly positive
reports from the visitors.
Safety/security (Rich Riesen)
---------------------------------------------------------------------
The intercom communications links from the main gate and the main OSB
entrance door to the control room are completed and operational.
#MZ NOTE TO VISITORS: This
improves access for cardless visitors.
Whenever possible, please
arrange for Rich to mail you a keycard
in advance if you will arrive
after hours or on the weekend. But if you
can't, just announce yourself
to the operator via the intercom at
the main gate to drive on
site, and then again at the
OSB main entrance to buzz
into the building after you park your car.
Also, a reminder: when you
leave PLEASE remember to return your
keycard! Thanks.
Awaiting parts for OSB the side door (kitchen area). This task should
be
completed end of next week.
Nothing new to report for the weekly site safety tour.
Assisting GSA in removing equipment stored at the off site warehouse.
Detector commissioning and High Power Laser Facility (Rupal Amin)
---------------------------------------------------------------------
Commissioning I have started looking into glitches observed in AS_Q
as
well as why the interferometer lost lock following several extended
locks. Thus far I have few conclusions. However, last night's
lock
losses may point towards a large optic, the beam splitter or the
recycling mirror, progressively drifting.
I have also begun investigating the low frequency noise by first trying
to correlate AS_DC with other channels that obtain data from the core
optics.
WFS 2 and ASC work has halted due to S3.
HPLF: The final SOP has been received by LLO and is being evaluated
by
the site safety personnel. The high power laser's safety shutter will
arrive within a week +/- 2 days and installation of a connection to
the
site's laser interlock has been requested. An air compressor to isolate
the table from ambient seismic activity is also in the process of being
obtained. Currently, we have received shipment of the double walled
perimeter fence that will ring the high power table and are nearly
ready
to unpack equipment requisitioned during the summer. We have also
started the tedious process of placing property tags on the various
HPLF
equipment.
Beyond the trivialities of setting up the lab, UF-LIGO has been
assembling quotes to construct a larger aperture Faraday isolator.
The
20 mm clear aperture should reduce difficulties observed after vacuum
incursions and MC beam realignment. Five new Faradays will be built
and
ready for installation before any future vents.
LDAS (Yakushin)
---------------------------------------------------------------------
LDAS data analysis:
Attending LSC meeting at LHO. Made waveburst presentation.
Inspiral data analysis (YunYong Wang)
---------------------------------------------------------------------
I completed the veto studies with the S2 Inspiral high rate triggers
last week and posted some interesting results in my LIGO web
page:
httP://www.ligo-la.caltech.edu/~wangyy
in the title of
"Veto Studies with s2 Inspiral playground high rate triggers (2) ".
Now I'm preparing some software and try to use it to check the S3 data
quality during the Science running.
General Computing (Roddy)
---------------------------------------------------------------------
Working with Sean at LSU to coordinate the installation of the new
network connection. It appears that we will be able to use our
existing
firewall, but it will require the purchase of at least two gigabit
cards
for it. Also, we will have to put in a new router between LSU
and the
firewall. When this is over, I will have not only greater bandwidth,
but I will also have greater flexibility and the ability to perform
more
comprehensive network security audits.
Still in the process of archiving some old files that are stored on
the
file server. I am archiving these on the new file server and
also
burning them to DVD. Setting up a new backup process for alix (web
server) primarily to get daily backups of the ilog. This will
be
archived to the new file server nightly.
Changing the dhcp server to the PIX. I am hoping that this will
give me
a little more stability out of the dhcp server.
Set up a backup disk on Rich Riesen's workstation. Also set up
a
nightly scheduled backup for his machine to this disk.
Still compiling many of the applications on the new file server.
This
is a long tedious process...
Many of the intended changes to the GC network are on hold until after
S3.
LLO Seismic Retrofit and L1 Detector TLC (Abbott)
---------------------------------------------------------------------
1. Back to work on HEPI. Adding additional spare channels
to the SEI
interface box prior to releasing schematics.
2. Working with Excel to complete the pump motor controller boxes.
3. Packaged up the failed Lightwave power supply and am shipping
it
back to LWE for repair according to the RMA instructions.
LLO Seismic retrofit (Kern)
---------------------------------------------------------------------
The machine shop manufacturing the parts for the first 12 actuators
has
delivered almost all of their promised first batch, a few days ahead
of
schedule. Welding assembly of a first article is beginning this
week.
Proper generation of a final bill of materials is still in the works
but
we've completed 'by the book' documentation of all build to print
components. Striving with all our shops to obtain sufficient parts
to
assemble at least one complete HEPI at MIT in early December, for fit
check.
Began clearing a suitable area in the new building to stage arriving
HEPI
mechanicals, and unpacked and inventoried all of the received COTS
parts.
HEPI remains on schedule to begin installation at LLO in January.
Marcel and I have turned our attention to completing a draft piping
drawing,
for internal review and presentation to the Consultancy Board. Completed
an
RFQ (sans drawings) for the mechanical and piping installation at LLO.
Dennis and Ed have weighed in and their comments incorporated. Oddvar
has
completed a schematic of the valve test manifold's auxiliary tanks,
valves
and hoses and we are working with the shop that manufactured the manifolds
to assemble the various pieces into a deliverable system
HEPI Valve Test Station (K. Carter)
---------------------------------------------------------------------
The LabVIEW code is fully functional for calibrating the test stand
and
the valve. Colin is currently working on adding a section that
will
test the operation of the valve and enable the user to check for errors
in the measurements.
Three issues are being dealt with for the physical aspect of the test
stand. Colin Campbell provided the following update:
1. Problem: The o-ring grooves on the three plates that
mount the
absolute pressure sensor and the inlet and return pipes are half as
wide
as they need to be. Solution: Corwin fixed this by milling out
the
center "island" defined by the groove. The depth of the groove
was also
increased from 0.048 to 0.050-0.052 to match the Parker design table
for
face seals.
2. Problem: The holes for the differential sensors were
too small for
an o-ring seal. Solution: We had good success boring out the
holes for
the differential pressure sensors and using o-rings. We bored
them out
to 0.232 (following the Parker design table for radial seals) and used
a
2-006 o-ring. They have not yet leaked at pressures up to 80PSI.
3. Problem: The OD of the flow resistor cylinder that drops
into the
lower half of the manifold is too large. Solution: The OD is
1.495,
while it should be 1.475. The machinist at Stanford was able
to turn it
down, being very careful to keep it concentric with the small alignment
cylinder above it that keeps it centered in the hole in the manifold
base.
no report
no report
no report
Simulation and Modeling (Bhawal)
NOTE: Hiro is visiting Virgo this week to discuss modeling
information exchanges and collaboration.
Linear Noise Model
--------------------------------
(Matt) Continued work on LinLIGO. Current version supports point-to-point
linear transfer functions, which can be used for plotting measured
and theoretical noise sources, but does not have a functioning
integrated
noise model. Next major upgrade will read control log (ConLog)
data
files to reconstruct the detector as it was at a specified time
(i.e.,
when I noise curve was measured). Also working to reduce
memory usage
and increase performance.
FFT's Matlab interface
-------------------------------------
(Biplab) Continued use and validation of the Matlab code (that calculates
length and angular sensing control signals) and the new version
of the FFT
code. Some of the sign differences (at field amplitude level)
between e2e
and FFT still remain to be mystery.
Code development and maintenance
-------------------------------------------------------
(Melody) C++ FUNC:
Work is underway to provide more functionality for the C++ based
FUNC.
Working on the interface design for user defined functions such
as
f(x) in the FUNC body as well as retrieving values from the macro
database.
LIGO Data Analysis System
Software Systems (Blackburn)
The controlMonitorAPI has a new interface for allowing database
queries to be plotted in a histogram. This will allow a selected
table and column with numerical values to be visually analyzed.
This will facilitate both testing and interaction with LDAS.
The STLPort testing continues. A hardware failure over the
weekend interfered with our memory tests. We had to start this
up again on Monday. The test needs one week of running to reach
a conclusion concerning memory leaks that may or may not exist
in this library.
The frameAPI has been modified at both the TCL and C++ level
to enforce a one-to-one handling of frame data for a single
job being processed in a single thread. Previous code had
the behavior of using one thread per frame query which in
some cases could result in a first in last out race condition.
The build rules for LDAS based on the STLPort library have been
added to lowest order. Support for debugging doesn't exist yet.
The build rules don't allow for the use of GCC's STL library
when STLPort is installed in /ldcg. This may not be needed at
this time given the problems with GCC's STL library.
Several minor bugs in the LDAS APIs (eventMonitorAPI, frameAPI,
managerAPI and genericAPI) have been fixed this week.
The db2utils code that manages the web page summaries for the
database have all now been updated to support all the restored
databases after the migration from solaris database servers
to linux database servers.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Refined monitoring of unarchived files at sites.
* Got HPSS migration working again after dataserver upgrade.
* Worked with Ben to try to figure out cause of problems when
importing/exporting/labeling tapes at LHO. Checked that
the robot's
FC configuration is the same at both sites (we're not having
the same
level of difficulty at LLO).
* Labeled more tapes at both sites.
* Transferred S3 full frames from observatories to CIT successfully.
Discovered that it is still possible to end up with a mix of
copy 1 and
copy 2 on the same tape, despite the "reserved" option.
While this
is (and was) easily fixed, it's something else I need to check
for.
I suspect that it happens when the system is being worked on
for other
(tape) problems because it's happened so seldom.
* Worked on the 'shiptape' script for the sites to automate the transfer
of SAM-QFS archive tapes to CIT.
* Worked on samfsdump scheme to get us hourly, daily, weekly, monthly
backups and to prune old backups automatically.
(Hari Pulapaka)
* Published S3 L1 and L2 data at CIT.
* Tried out the new VDT for RH 9.0. That didn't build mysql properly.
But the VDT server and client packages were built without problems.
I
did some minimal testing and they seem to work fine without
problems.
But I did not test condor yet on RH 9.0. But I did install condor
on a
RH 9.0 earlier, and that worked.
* Setup GRIS at ldas-grid.ligo.caltech.edu for the SC03 demo.
* Updated the LDR Installation at CIT to include the new LDRTranfer,
LDRSchedule and LDRMetadata files.
* Also, I was looking into pyGlobus and investigating writing a small
FTP utility for directories.
(Al Wilson)
* Check IDE Raid drive for possible bad drives. Also setup a BB server
to see
about added this to BB to automatically check for drive failure.
* Repaired Dataserver on ldas-dev. Found bad memory in the Slot B CPU
board.
* Setup wireless on Kaice laptop.
* Another Xserver problem with a desktop machine. Used the latest from
Xfree
to cure the problem.
(Stuart Anderson)
* Added the DMT SenseMonitor minute trend frames to the LDAS diskcacheAPI
so they can be used to calibrate on-line analysis jobs.
* Updated ligotools on ldas-jobs at LLO to allow inspiral jobs to
run on S3 data.
MIT
---
(Keith Bayer)
* Putting cluster nodes 45-88 online.
* Moving data off of first pcraid in order to upgrade motherboard.
Hanford
-------
(Greg Mendell)
* Archiving full-frame data, and generating level 1, 2, and 3 RDS
frames for S3 continues without significant problems at LHO.
(Some tape
drive and tape problems have been overcome by redundancy of
the system.
An fb3 framebuilder crash did result in a small loss of data;
Ben
Johnson's script that copies data from the framebuilder to ldas
now
automatically fills in these gaps by getting missing data from
the fb0
framebuilder. Thus, no data is lost as long as one framebuilder
is
running.)
* Finished creating L2 RDS of the data for injections done between E10
and S3 for the stochastic group. These are in the directories
H-RDS_R_L1-7511 and H-RDS_R_L1-7512 under
/frame40/S3H1H2StochasticL2RDS, visible from fortress at LHO.
Sukanta
Bose plans to transfer this data to WSU for analysis.
(Ben Johnson)
* Newest version of disk2disk copy script is running successfully at
LHO. It has filled several gaps so far, and verified (FrCheck)
every
file since Nov. 6 2003. The only gaps in LHO data so far are
on Nov.1
when the daq system crashed due to a problem upstream of the
framebuilders.
* Sent L0 data to Caltech Nov. 11
* Ran badblocks on tekoa and defiance, Nov. 12. 3ware card on defiance
reported that it repaired a sector.
* L700: Two tapes, HL0173 on Nov.10, and HL230 on Nov.11 were stuck
in
"Cartridge In" in the robot. SAMFS thought they were in
their slots.
Tape drives manually cleaned on the 10th. The library was put
into "Fast
Load Disabled" mode on the 11th. These two actions should lessen
the
number of "MEDIA ERROR"s and stuck tapes.
* Set up DMT archiving set and rsync cron job, Nov. 11. We are now
archiving all DMT trends except "spectrumArchiver" data at LHO.
* Nodes 29->32 were having network connectivity troubles since late
October. This has been fixed by moving their cables to another
card on
the Foundry Switch (they are not in the node list yet). I'll
contact
Foundry Networks after S3.
Data Analysis Activities (Lazzarini)
Landry:
Mike Landry and I have completed the first version of the stackslide
code that does both stacking and sliding of SFTs. We have run
this code
on the injected pulsars in the E10 data. Our main effort now
is to
debug on simple test data and the S2/E10/S3 pulsar injections.
(Note
that there was some corruption of the E10 injections, due to a floating
point overflow. Still, we could find the injections we expected
to
see. However, probably we will now focus on the S3 injections.)
We
presented results on the E10 injections at the PULG F2F/NOV LSC
meeting. See DCC talks G030562-00.pdf and G030575-00.pdf.
Lazzarini:
Working to develop a new formulation for the stochastic background
search
analysis when all 3 interferometers are operating in coincidence. There
is an
improvement in the optimal filtering apprach that one can use to account
for
local H1-H2 correlations. This is important for S2, and (hopefully)
less important
for S3 and beyond ...
for an early draft of the idea see:
http://www.ligo.caltech.edu/docs/T/T030256-00.pdf
Shawhan:
* Spent last weekend at the Gravitational Wave Phenomenology Workshop
at Penn State.
* Spent the rest of the week at the LIGO Scientific Colaboration Meeting.
* Did further veto studies for the S2 inspiral analysis. The
L1 MICH_CTRL channel,
with a very high threshold (30 sigma), looks promising.
* Did signal injections on a few nights.
* Made some improvements to the conlog software.
Weinstein:
- Worked with Szabi and Julien on E10/S3 hardware burst injections,
and presented some results at LSC meeting; see
http://www.ligo.caltech.edu/~ajw/bursts/injectS3/G030599-00.ppt
- resubmitted Amaldi writup on S1 burst analysis,
which has now been accepted. See
http://www.ligo.caltech.edu/~ajw/bursts/weinstein_amaldi03.pdf
Yakushin:
Attending LSC meeting at LHO. Made waveburst presentation.
General Computing (Wallace)
MIT:
(Keith)
- Walking around and patching windows computers
- Attended MIT email session - MIT will no longer allow
unauthenticated email on it's servers
- Building new NAT wireless router
- Trying to move Marie over to newer desktop
- Trying to build/setup replacement computers for old lab PCs
Livingston:
(Shannon)
- Working with Sean at LSU to coordinate the installation of the new
network
connection. It appears that we will be able to use our existing
firewall, but
it will require the purchase of at least two gigabit cards for it.
Also, we
will have to put in a new router between LSU and the firewall.
When this is
over, I will have not only greater bandwidth, but I will also have
greater
flexibility and the ability to perform more comprehensive network security
audits.
- Still in the process of archiving some old files that are stored
on the file
server. I am archiving these on the new file server and also
burning them to
DVD.
- Setting up a new backup process for alix (web server) primarily to
get daily
backups of the ilog. This will be archived to the new file server
nightly.
- Changing the dhcp server to the PIX. I am hoping that this
will give me a
little more stability out of the dhcp server.
- Set up a backup disk on Rich Riesen's workstation. Also set
up a nightly
scheduled backup for his machine to this disk.
- Still compiling many of the applications on the new file server.
This is a
long tedious process...
- Many of the intended changes to the GC network are on hold until
after S3.
Hanford:
(Christine)
- The whole week has been spent on the LSC meeting. Thanks to
Larry for
getting the VRVS and VNC working and for fixing our printer and setting
up phone conferencing.
- Spent a few minutes emailing Lisa B. about what I need to have ready
for her visit on the 19th to upgrade our mail server.
CIT:
(Mike)
- Finished loading and swapping out a PC for Fumiko Kawazoe. I loaded
this
PC with GC software/engineering packages and transferred over her data
from
the old PC.
- Finished loading a visitor workstation. I used it to swap out an
older
computer that was up on 3rd floor of Bridge.
- Finishing loading a replacement PC for Cleveland Mak.
- Loaded additional software on Cindy Akutagawa laptop.
- Burned the end of month ghost backups for the NTSRV's to DVD.
- This week I had a lot of user support that included software &
printing
issues.
(Veronica)
- LIGO: Continued working on video editing for Bills Kells. I searched
for
ways to achieve the best playback quality for a reasonable file size
suitable for Bill's laptop to handle. I made several versions of a
clip
combining edited and trimmed original footage with various degrees
of
compression. Burned CDs and DVDs for Bill to use and distribute.
Posted updates to the webpages throughout the website.
Addressed an issue related to maintenance of the roster database.
Met with Karen Willacy of JPL to discuss a setup of a document database
for LISA. Explained the architecture of the DCC and issues of its
maintenance and upgrade.
- LSC website: Installed webpages for the presentations for the meeting
in
progress. Posting the talks as they arrive daily.
Supported the VRVS/VNC for the LSC meeting. Larry and I tested the
setup
prior to the meeting, and we monitored it here at Caltech during the
plenary session Tuesday afternoon.
Made a massive web posting of MOUs.
- CaJAGWR website: Posted updates and provided user support.
(Lisa)
- Worked on a disk problem in the 40m. Their main working disk
had 2 block
errors. I created a new partition and moved their data over to
it.
This is a
temporary measure until the e450's can be put into production.
- Enabled clamav, an open source virus scanner, on becrux.
- Worked on 2 machines that were having problems and verified that
they are
having hardware problems that warrant surplusing.
- Began building a test box for the hanford mail server replacement.
I am also
working with Christine so that we are both ready to go when I get up
there.
- Spent more time working with the new spam filtering software.
So far I like
it very much.
- Installed latex on canopus.
(Larry)
- Spent the week in Hanford supporting the LSC and am now on my way
to
Livingston for the NSF Review. I will give a detailed report
next week
AdLIGO
Suspensions
Preparing
for NSF Review.
Calum and I welcome the arrival of Russell
Jones from
This morning we had a telecon with Betsy, Helena and Doug at LHO and with Calum, Russell and I down here at CIT about the catcher and Russell's product design specification for it. Betsy and Doug provided some very good input to the design. Helena took away a number of issues to bring to her ribbons/fibers/optical bonding monthly meetings, such as 1)what type of protective cover will be used on the optics during assembly, transport and installation, 2)shall the protective cover be in place during the welding operation and 3) issues related to the fixturing of the ears w.r.t. the optic's wedge and tilt.
Calum, Russell and I have been working on tying up the experimental results of the natural mode testing of the mode cleaner with the ANSYS brick fea modeling and the IDEAS beam and shell fea modeling. We feel that we are coming close to some good agreement. Also, we are working on calculating or estimating the representative factor for the clamps that hold the structure to the optical table. We talked with Larry Jones yesterday and hope to continue our discussion tomorrow. Caroline Cantley started this work when she visited in June and we hope to make more progress.
Dan and I have finished our attempts to measure the Q's of the Suprasil
311SV
test mass on load from Garilynn Billingsley.
It has been extraordinarily
difficult to excite the modes of this mass, and in three month we have
collected
less than half the data we could collect in one month on the previous Suprasil
312 mass. Why? No idea.
Nevertheless, we see no obvious difference between the quality factors
of
Suprasil 311SV and Suprasil
312, even the the highest Q's we measured
were 53
million and 120 million, respectively. This is because the data
trend to higher
Q at lower frequency, and we have a dearth of data at low frequency
for the
smaller 311SV mass, where the larger 312 mass had its best Q.
When the Q's vs.
frequency of the two masses are plotted together, the distributions
are pretty
much the same, with the same limiting upper envelope. This data
may be viewed
in LIGO document T-030264-00.
Adaptive Optic Compensation:
----------------------------
I have developed a 3D thermal model in FEMLAB to evaluate the effects
of
inhomogeneous and assymetric heating
in test masses and their effect on LIGO. I
have checked it against Dave Ottaway's
2D model (taken from Ryan Lawrence) and
they compare favorably when they model the same heating. So far
the model only
includes heat diffusion but for fused silica this is a good first approximation.
Using this model it appears that the CO2 heating ring planned for installation
into initial LIGO can be offset by several millimeters from the test
mass center
without the thermal correction degrading significantly.
For additional information about this report, contact sanders@ligo.caltech.edu