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The LIGO Executive Committee Agenda for Monday November 19, 2001 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items:
Late yesterday, I received word that our retired LIGO Safety Officer,
Mike Zydowicz, died suddenly at home.
Even in retirement, Mike continued with an active interest in the
progress of the LIGO Project.
His most recent contribution to LIGO, was as a member of last week's
Hanford Safety Audit team and he was looking forward to participating in
planning for the next safety audit.
GHS note: Last week I traveled to Hanford for an annual safety audit,
accompanied by Bill Tyler, Caz Szcilowicz (head of Caltech Safety) and
Mike Zydowicz. We spent a productive day at Hanford with Otto, Fred, Doug
Cook, and in telecon with Jonathan Kern. Mike contributed his many years
of experience to thinking about our safety issues. He had decades of flight
systems and propulsion experience, largely at JPL. He earned a NASA Exceptional
Service medal for his contribution to resolving important technical issues
in a Mars mission that was successful. He helped us put into place many
of our safety policies and practices. He enjoyed interrupting his retirement
to help on LIGO appraisals. We spent a fine evening last week talking about
his very recent RV tour around the western states and many space program
war stories. He enjoyed helping us and he cared for LIGO. He will be missed.
no report
LIGO Operations--Administration
| Action No. | Description | Responsibility | Assigned Date | Due Date |
| 58 | Establish Corporate Checking Accounts for Sites | E. Jasnow | September 2, 1999 | --- |
| 87 | Press Controller for a Chart of Accounts (supporting documentation for Operations Review) | E. Jasnow | January 18, 2001 | August 2, 2001 |
| 99 | Get Weber Bars for display at sites. | E. Jasnow | August 2, 2001 | |
| 100 | Develop a first draft staffing plan for FY 2002 based on budget model | P. Lindquist | August 30, 2001 | October 4, 2001 |
| 102 | Prepare policy draft concerning procurements and issues of safety, shipping, reliability, maintainability, etc. | W. Tyler | September 27, 2001 | |
| 103 | Close LLO Construction Petty Cash Account and reduce petty cash amount from $20K to $10K. | TBD | November 15, 2001 | |
| 104 | Circulate Information on 24/7 operations and schedule meeting for discussion. | TBD | November 15, 2001 |
The list of previous actions assigned through
November 1, 2001 may be found at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
ACCOMPLISHMENTS
ACTIVITY
| Packages | Faxes | |
| In | 38 | 30 |
| Out | 14 | 46 |
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>
Attended meeting by Project Accounting department describing the life cycle of a Grant, Award or Cooperative Agreement.
Attended meeting with Property Accounting regarding issues related to tracking of LIGO property.
At Alan Weinstein's request, tracked down some charges to Campus Research accounts, issued Cost Transfer Request for charges posted in error.
The reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
From: irena@ligo.caltech.edu (Irena Petrac)
SUPPORT
Irene Baldon
Progress Period from 11.09 to 11.15
Accomplishments:
Reports (Lindquist)
Nothing to report.
I have scheduled a meeting of the
LIGO Change Control Board (CCB) for Tuesday, November 20, 2001 at 9:00
am PST in the Engineering Conference Room (ECR). The following
Change Requests will be discussed (Because some personnel will not be available,
it may not be possible to act on all of these. However, at a minimum
I would like to address completed and closed accounts.):
The following change
requests have been distributed to the Change Board:
| CR-010011
Revision D |
Construction | Adjust LIGO Construction Budgets to Reflect Actual Costs for Completed Tasks as well as REU Expenses, Accounting Adjustments, and 7-LIGO (old work order) costs. | P. Lindquist |
| CR-010012
Revision B |
WBS 1.4.4.1 | Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites (Larry Wallace will argue for spending these funds on network connections) | P. Lindquist |
| CR-010013
Revision A |
WBS 1.4.3.3 | Realign budgets for LIGO Data Analysis and Computing. This is a zero-sum change request. | P. Lindquist |
| CR-010014 | WBS 1.1.4 | Additional budget to complete Livingston Staging Building. | G. Stapfer/
P. Lindquist |
Press for the latest Contingency
Needs Projection.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
CDS: Added an "l1ifoconfigure" medm screen that has save and
restore buttons for saving the configurations of the interferometer in
Michelson, PRM, Xarm and Yarm. Changed the scripts to make it working.
ezcawrite and ezcaread channel access commands need new Solaris 8 OS. Currently
the scripts for restore are running on "control2" control room machine
which has Solaris 8, through rsh.
Planning on upgrading the CDS machines to Solaris 8 operating system.
Also in the process of identifying the memory upgrade needed for the cds
machines. I will be ordering them as soon as I finalize the part numbers
for the models we have.Found a problem with Lan Emulation Configuration
Server (LECS) on our ASX 1000 ATM Backbone switch. Three of the control
room machines which were rebooted didnt come back. Temporarily they have
been brought back with 10 base T ethernet. We tried to restart the LECS
server after loading the lecs.cfg file. But the computers still gave an
error "LECS failed to respond". ATM switch needs to be shutdown and restarted.
(Cheithan)
Detector: Optics and Installation: Received a set of drawings
from the manufacturer of our PSL acoustic enclosure about a week ago. Found
a disconnect occurred between the salesman and engineering staff and the
access doors Stan wanted along the electronic rack side were too large
to be opened completely. I finally got into the engineering loop and spoke
with the detailer. Turns out that the weight/ft^2 is about 10 pounds and
hinged windows are a problem because of the thin steel skin. He suggested
that we
use what they call 'plugs', being removable panels ~ 3 ft^2 held into
position by snap latches. They will have substantial "D" handles on each
side and can be removed in the few seconds that it takes to pop 4 latches.
nFurthermore, they can provide better isolation because the clearances
are closer than necessary for a hinged door. Joe, Rai and I agreed that
this was acceptable and I returned the marked up drawings last Friday.
Spoke with their installation foreman Mark Johnson and he briefed me on
the installation scheme. The panels will be shipped in palletized form
within plywood crates. They will have shop dust on them, and I plan to
offload the panels in the large airlock where we can uncrate and clean
them before moving into the LVEA. Looks like we'll receive the material
Dec 10 > 15. Programming of the Laser Safety Interlock system is in progress,
and the installer hopes to complete the programming Spent some time identifying
and locating logging and industrial noise sites from aerial surveys. See
LLO
i-log 11/13/01. (Jonathan Kern)
LDAS: Spent a little bit of time showing Igor around the computing
equipment for LDAS. Received the SF in yesterday. Unpacked it and placed
it in the Mass Storage Room this morning, but I will have to find a permanent
place to put it. It is starting to get crowded in there.
GC: Installed Pcard software on Allen Sibley's machine. Received in
the rackmount Penguins to replace the ones given to the laser safety interlock
and the building control machine. I will start experimenting with IMAP/SSL
and SSL web pages for our email service here. If it works well, I may ask
for some volunteers to test it for a couple of weeks, and if people like
it we can switch over. (Shannon)
We have been preparing for the support of the E6 run this weekend. We replaced failed power supplies in one of the raid disks on decatur.We have been looking at the possibility of upgrading two of our older PCs which are dedicated instrument controllers. (Tom Evans)
|
Commissioning:
|
|
We have received 2 of the repolished mode cleaner pieces from Wave Precision.
These are the additions and comments that I have received
for the new module:
1. The 1811 DC readback should be included.
2. An amplifier should be added to the RF input. The
signal levels can be quite low. 20dB of gain should be sufficient.
3. We will use DC block to eliminate potential ground
loops. These will be added to the RF cables where they are needed.
4. We will try to measure the shielding effectiveness
of the RF can to be used.
We found that the source of the 40-50Hz noise on the
QPDs at LHO was
the optical lever laser that was being powered from
the rack +5 supply.
We powered the laser from a separate power supply
and the noise
disappeared. We need to change the laser power supply
to separate power
for all optical levers. LHO has moved some to DC-DC
converters and this
appears to be effective.
The third periscope is being vibration tested before being shipped to LASTI. Drawing documentation packages for the LLO prototype and the production model periscopes have been released.
A preliminary design for a 7.5 m to 54 m zoom objective lens, to be added to the optical lever sensor package, is in process. With this objective lens, the optical lever beam displacement will be converted to purely angular motion of the test mirror; the maximum deflection sensitivity of the new optical lever sensor will be < 0.2 microradians. The design requires the position detector assembly optical lever box to be approximately 29 inches long, instead of the present 16.25. It may be possible to place the new box in the same location as the BSC2 box at LLO.
The beam propagation of NPRO #259 was measured and
its output
circularized in preparation for modematching into
the pre-modecleaner in
the PSL Lab.
I completed testing of the new layout PMC servo (Rev D). It has been shipped to LHO with Traveler paperwork included. Additional DCNs for all PMC boards have been generated and submitted. Except for any design changes down the line, the PMC documentation is up to date.
Worked to get the third ISS electronics module slated for LLO ready for fab. The board is currently being stuffed and bench testing should begin today. The enclosure is built.
An older version of the mother board was sent out for fabrication by mistake. Fred has corrected his mistake and new replacements are on order.
Since our last report, we have been working on improving lock
acquisition in the TNI. With our old servos, full lock took at
least
two hours to acquire, and that needs to be substantially reduced before
significant progress can be made in noise reduction.
Our initial lock had a unity-gain frequency of about 350Hz, which leads
to a mean time between locks of some tens of minutes. It is reasonably
straightforward to increase the gain uniformly at all frequencies,
bringing the unity-gain frequency up to 1.3kHz. This improves
lock
acquisition somewhat, but the mean time between locks is still several
minutes. This is an improvement, but since the system catches
in the
TEM00 mode less than one-third of the time, we would like to do better.
With our current filters, the highest stable unity-gain frequency we
can
obtain without exciting mechanical modes appears to be 1.9kHz.
We can
increase this frequency somewhat at the expense of attenuation at
27.5kHz, our lowest mechanical resonant frequency. The system
then
catches promptly, but the mechanical mode quickly rings up to an
amplitude that produces nonlinear oscillations in the error signal,
making effective noise or unity-gain frequency measurements impossible.
Our highest priority now is to change the rolloff in our filters,
preserving the attenuation at 27.5kHz but improving phase margin below
10kHz. We are currently putting together electronics to do that.
The photothermal experiment is also coming along well. The cavity
locks and we find a thermal displacement of our aluminum mirror of
about
10^-11 m/sqrtHz, which is roughly that expected from theory.
However,
the model gives a signal proportional to 1/f, while the data is roughly
proportional to 1/f^2, and the phase differs by 70 degrees between
the two. We are proceeding to investigate these discrepancies.
LASTI (Bayer, Fritschel, Goda, Harry, Laliberty, MacInnis, Mason,
Miller, Mittleman, Ottaway, Phinney, Rollins, Shoemaker, Zucker)
=======================================================================
BSC SEI INSTALLATION:
The last phase of SEI installation was to add 500 lbs of counterweights
to simulate the (absent) internal payload. These were shipped
from LHO
and arrived yesterday, but with damage to the crate; several weights
broke out and breached their wrapping, compromising cleanliness.
Fortunately some similar weights earmarked for HAM13 were on hand.
The
dirty ones will be reprocessed and used in the HAM later. We
expect to
finish and seal up the BSC today (Thursday). We are going to
delay
leakchecking until work on HAM13 is completed as well.
HAM13 SOS INSTALLATION: The SOS balancing is underway in the optics
lab. While we now have all the vacuum parts except the viewports
(currently delayed at the coater; originally expected 11/1), we did
come up short on some of the installation aids such as platforms, belly
bars and internal handles. They are being shipped but the sum
of these
details probably will slip the SOS installation to the week after
Thanksgiving (no real schedule impact, we had just wanted to be done
before the holidays).
HYDRAULIC ACTUATORS: Ken ordered the three Streckheisen seismometers
(>$40k worth). He is still having difficulties simultaneously
satisfying stress concentration, mounting, and manufacturability
constraints. We hope some brainstorming with Brian Lantz and
Dan DeBra
from Stanford will help; they are visiting us today and tomorrow.
Joshua is continuing experiments on the prototype pump/accumulator
skid
to understand its dynamics.
CDS/DAQ/GDS: Our GDS system is running smoothly and stably with
the
replacement RAID disk provided by Dave Barker at LHO. Keith mounted
it
on Lancelot with no problems.
PSL:
Continued work on characterizing the frequency stabilization servo
actuators and electronics. Calculated the final modematching
into the
SOS test cavity going into HAM13; now implementing the solution
on the table.
Simulation and Modeling (Bhawal)
> Mechanics modeling
Next Tuesday, Nov. 20th at 9:00AM PST, a telephone conference is scheduled to discuss the modeling of mechanics in e2e for the adv.LIGO. Information is available at e2e home page http://www.ligo.caltech.edu/~e2e.
Giancarlo Cella is visiting CIT from 11th till 20th. The main focuses
are
(1) transfer knowledge of MSE (mechanical simulation engine)
to Virginio so that Virginio can maintain and develop without heavily relying
on Cella
(2) resolve known issues (bug fixes and completion of important objects,
BLADE, BEAM, etc)
(3) complete LIGO I HAM stack and adv.LIGO 4 pend. models.
Cella gave a talk at the weekly e2e meeting about his MSE, and the improvements in the new version. Virginio summarized the modeling he is working with Giancarlo.
> LIGO I locking simulation with mode mismatch
Biplab, Hiro, Matt: We were having problem in locking when a
mismatched beam was sent as input to Han2k model. Some success
has been achieved in this problem by choosing proper offsets
in mirror position thus helping the locking system by keeping it
closer to the locked state.
We discussed about the proper interpretation of locked state
in presence of mismatched beam.
> LSC modeling (Luca)
The Matlab model describing the LSC electronics (from the Whitening
to the
Anti-Imaging board) has been copied into e2e. The TF of only the LSC
electronics as produced from e2e and Matlab are identical. There is,
however, disagreement in the way the LSC digital filters are digitized
in e2e that produces an unacceptable disagreement above 1kHz. This
problem
needs to be addressed.
Hiro has prepared an e2e model of one LIGO arm, with local damping
to the masses and a simple LSC controller. I am presently getting familiar
with it before I include the LSC model of the controllers.
> alfi4 and box parser
A few crucial issues related to alfi4 and box file
parsing were found, and Ed fixed.
One of the bug prevented Bill Butler from running
his configuration with better seismic model.
> alfi5
Bruce and Melody are working on the new alfi based
on JAVA.
LIGO Data Analysis System
Software Systems (Blackburn)
The 0.0.22 release went out over the weekend. It was needed no later
than
Sunday for the Supercomputing Conference demo of Griphyn/LDAS. There
was a
small startup issue at Hanford which has been seen in the past but
not to
the extent seen over the weekend. There were also several problems
found
with the system during testing and after the release which we had no
choose
but to forge ahead with given the time schedule demands placed by the
demo.
These have now been fixed in the development snapshot of LDAS. One
of these
bugs was impacting the ability to prepare for the Periodic MDC. The
problem
was with data requests which didn't overlap a frame boundary. The frames
at
Hanford are now 16 seconds long and so it is very likely to have a
request
which falls in the middle of a frame. The temporary workaround is to
request
data which starts at modulus 16 of a GPS second.
(AL NOTE: We have been informed that the numerous LIGO-GriPhyN demonstrations
in Denver at SC01 went
well and was very well received! My thanks to everyone who made it
possible, not only at Caltech, but also at USC and UWM)
We also assisted Penn State with setting up their database for release
of
LDAS. A script was developed for the PEM Deep Mining project and the
Inspiral
group which will query the segment tables in the database to determine
if new
data has been generated before issuing a job to LDAS to analyze the
data.
We also discuss in several meeting with the LSC the issue of how to
best
provide response functions to the community and to LDAS search codes.
This
could involve using the database, but another complementary option
may be
to have a webserver with a cgi script which can serve up appropriate
sets
of response functions to user requests.
UWM has carried out a mini-MDC of the inspiral search code using the
LDAS
system at UWM. The challenge successfully discovered the set of single
blind
inspirals injected into a simulated data set of frames.
After the release of LDAS, we tested the new release of LAM, the message
passing interface (MPI) library used by LDAS and the LSC. We found
this
release fixed a bug that was causing some of our search requests to
die
and it has the added advantage of being backwards compatable so we
didn't
need to recompile against it (an advantage of using shared objects
in LDAS
and LAL). We subsequently pushed this release to all the LIGO Lab ldas
systems and informed the LSC MPI group of the results.
The efficiency of several of our release test scripts was reviewed and
were possible improved.
We also added the LDAS home page (web) files and cgi scripts to the
LDAS
cvs repository. Previously this was managed by Barbara, but with her
departure we are taking a more active role in managing these files.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
Worked on HPSS data migration to 9940 tapes (ongoing). Dug HPSS
out of
the hole it was in vis a via no available 3590 tapes and the
corresponding disk caches having filled. For the first time in
months,
there are no tape warnings in the classes of service that use 3590
tapes.
Began work on scripts to semi-automate the process of migration off
of
3590 and Redwood tapes.
Restarted HPSS many times.
Worked on purchase of LIGO 9940 tape drives (ongoing).
(Al Wilson)
installed kernel 2.4.9-12 on the linux machines at cit,dev,test. A couple
of them still need to be reboot on the new kernel. Set up the rpmsync
packages for RH7.2 Still refineing the cfdef program.
(Ed Maros)
Did major cleanup of /ldcg directory for Intel Linux and Solaris.
(Stuart Anderson)
Installed additional KVM ports in ldas-dev and ldas-test systems.
Installed UPS units to support the new SF880 servers at Caltech.
Handed off the request to buy and install 50um multi-mode fiber at
Caltech
to support LDAS GigE and Fiber Channel networks.
Rebuilt filesystems at LHO to continue diagnosing the QFS filesystem
problems.
Installed Solaris 8 Maintenance Update 6 on E450 to evaluate suitability
for LDAS servers.
MIT
---
(Keith Bayer)
requested and received license key for QFS software
began looking into Shannon's BBrother setup
received fax of P.O. for sun hardware
Livingston
----------
(Shannon Roddy)
getting price quotes for Igor's computer. Spent a little bit of
time showing Igor around the computing equipment for LDAS. Received
the
SF in yesterday. Unpacked it and placed it in the Mass Storage
Room
this morning, but I will have to find a permanent place to put it.
It
is starting to get crowded in there.
Hanford
-------
(Greg Mendell)
1) The QFS "File system full - ENOSPC" error occurred again on
fb3
(last occurred Nov 2). One of the stripe groups may have been full.
A
case # for this problem had previously been opened with Sun.
Followed
up on this with Sun, and emailed them a description of the QFS problems
we've had and corresponding kernel messages. Stuart has configured
and
built new QFS file systems to make disk space usage easier to diagnose.
Testing continues.
2) Worked on creating test scripts for the Known Pulsar Demod Mock Data
Challenge.
3) Prepared the tapecontrol script configuration files for E6 and ran
tests. We are ready to go at LHO and LLO.
The main log files for this script during the run are at:
http://www.ldas.ligo-wa.caltech.edu/ldas_outgoing/tapecontrol/logs/log.html
for LHO,
http://www.ldas.ligo-la.caltech.edu/ldas_outgoing/tapecontrol/logs/log.html
for LLO.
4) Worked with LDAS to debug job failures during request for frames
by
time at LHO.
General Computing (Wallace)
MIT:
(Keith)
-Wireless troubleshooting
Computer/networking setup in NW22 (bldg next door)
Ordered more wireless accessories
-Ligotools upgraded (that package is sweet)
-Restored user archive data from tape
-Spec'd out and ordered replacement video pc
-Troubleshooting backup script for new file server
-Larry extracted and e-mailed data files to Richard M.. The difficulty
was
finding a 5&1/2 floppy drive that worked.
Livingston:
(Tom)
-We have been preparing for the support of the E6 run this weekend.
-We replaced failed power supplies in one of the raid disks on decatur.
-We have been looking at the possibility of upgrading two of our older
PCs which are dedicated instrument controllers.
(Shannon)
-Installed Pcard software on Allen Sibley's machine.
-Received the rackmount Penguins to replace the ones given to the laser
safety
interlock and the building control machine.
-I will start experimenting with IMAP/SSL and SSL web pages for our
e-mail
service here. If it works out correctly we will try distributing it
out for
all of the locations.
Hanford:
(Christine)
- Setup two new guest computers, 2GHz Dell PCs. This included
installing the standard application software packages as well as a
few
specialized software packages. Setup the network configuration
and
installed printers. Created user areas for guests to get their
e-mail
and provide work storage space.
- Installed more freeware software on the application server. Fortress,
the LSC "sandbox" computer, is still running Solaris 7 because until
recently drivers for the peripherals and network cards were not
available for Solaris 8. These drivers are now available, but
the
computer is so heavily used and relied on for Engineering run data
that
there has not been a good time to take the computer down for the day.
This has caused some problems in that every other Sun on site is now
running Solaris 8 and all the freeware software is for Solaris 8.
Now
some of the freeware software won't run on fortress. The plan
is to
find some time early next year, after the E7 run, to upgrade fortress.
- Purchased more memory for all the GC Sun Ultra10s. Purchased
a flat
screen monitor and computer cart for the video conferencing system.
Purchased fast ethernet card for the GC 3810 in the staging building
so
fortress can have fast ethernet access to the LDAS T3 disks for
Engineering run data.
CIT:
(Mike)
-Ken M.'s is PC acting up when running AutoCAD 2000i looks like I have
to reload
AutoCAD.
I have made necessary arrangements with Ken to correct this problem.
-Loaded 2 PC's with full General Computing software, and ran a diagnostics
on all hardware.
-Laptop ran a ghost image after reloading all G/C software and transferred
to backup server.
-Ran created ghost images for two PC's that are transfers to backup
server.
-Project Science website keeps losing its TCP/IP connections. I have
been
trouble shooting this web server to try to prevent this from happening
again. We have stopped all other web services besides projectscience.org,
to run
this website by its self.
-40M printing problem on Martian network.
Called HPC to do a complete service that included changing fuser and
rollers and cleaning up the printer.
I had a networking issue to take care of that included connecting a
'lab
computer' to this printer on the Martian subnet 113. I ended up using
Jet
Direct software to get this computer to print.
(Lisa)
- Compiled, tested and installed a mac address access list on the orinoco
wireless access points.
- Built an ultra1 as a secure samba server for Riccardo to transfer
his data in
the synchatron.
- Cleaned up some mail aliases
- Did research to find undocumented keywords for the .mailrc file.
I began a
FAQ to collect this information where everyone can find it.
- Wrote some other FAQs. The General Computing FAQs have quite
a lot of useful
information at this point. You can view them at:
http://docuserv.ligo.caltech.edu/docuserv/computing/faq/faq.html
(Larry)
-Once again worked a number of purchases. No real problems just a lot
of little
items needed for different people. I have canceled a number of s/w
maintenance
contracts, Island and Applix. These packages very rarely get used and
the
licenses are good for some time, as people move over to other packages
we will
remove these old packages. We will keep the s/w around a year for historical
needs.
-Did some more P-card s/w installation work. Tested the written procedure
and
will be making some minor changes to it. Sent out the new library to
the
Observatories.
-Worked with Ed C. on getting rid of old equipment.
-Went over a number of NIS+ procedures with different people. The setup
of the
credential tables has caused some minor issues.
-Working a number of security related issues. Mostly documentation
and policy
statement work.
-Working on getting more information for high-speed WAN connection
at Hanford.
Still nothing new for the high-speed Livingston WAN connection but
we will keep
looking.
From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>
Homogeneity of one a-axis sapphire piece has been completed, for one
polarization. The rms homogeneity of the a-axis
piece is 13 nm compared to 30-50nm for the m-axis pieces we have measured.
There are still 3 detailed measurements to perform, 2 for the other piece
(for each polarization) and one for the other polarization on the current
piece.
Bill Kells and I have been probing the question of "surface vs. bulk" as the cause of the inhomogeneity we see. I have rotated a piece through 16 degrees in an attempt to see if the homogeneity features move with features on either surface. Bill is scrutinizing the data.
From: Helena Armandula <ahelena@ligo.caltech.edu>
Advanced LIGO Coatings
Trip to SMA/VIRGO - Lyon
The meeting in Lyon with J.M. Mackowski was very positive.
His latest research on coating absorption anticipates
that reaching our 0.05 ppm absorption goal may be tangible.
He identified factors contributing to absorption losses and developed
methods to minimize them.
Factors found that contribute to absorption are:
1) from the substrate: residues from polishing and cleaning processes,
sub-surface defects, diffusion
2) from the environment: dust particles and chemical contamination
3) from the coater: chamber walls, ion sources, target material impurities.
His latest absorption measurements at 1064nm show:
Mean absorption on a 18mm dia. fused silica substrate : 0.20ppm
Sampling: 450 micrometers
Resolution: 100 micrometers
Sigma= 0.14 ppm, max.=1.87ppm
Sensitivity: 0.05 ppm
This result is repeatable.
Visit to VIRGO / Perugia
This visit was very valuable because one of our discussion with Michele
Punturo and Helios Vocca was the handling of coated masses.
Mackowski set up very strict handling requirements for the VIRGO coated
optics during assembly. These folks complied by developing very sophisticated
procedures.
These same handling requirements are about to be imposed on Advanced
LIGO coated masses and this is an issue that we have not addressed at that
level.
Jean-Marie's concerns are very valid ones.
He designed and had manufactured very expensive baking vessels to prevent
coating contamination during annealing, as an example, as well as covers
to protect the surface of the coated optics during assembly.
He does not advocate cleaning the optics after they have been coated.
He performed surface analysis on parts kept for months covered in HIS
clean-room finding no traces of contamination.
How should we proceed?
Silicate Bonding
Discussed silicate bonding processes, they have very similar experiences
to ours having seen many of the effects that we observed.
Thermal noise studies - "Q" measurements
Shipped to Lyon as planned, 4 thin substrates. Four thick substrates
were shipped from Glasgow.
Two of each substrate type are being coated with 2 layers - 1/4 wave
each of SiO2 and Ta2O5 .
The others with 30 layers-1/4 wave of the same materials.
Shipped 5 substrates to Glasgow and 5 to Stanford to have "Q" measurements
taken before coating.
Have 4 thin substrates to be shipped to MIT or Syracuse for the same
purpose.
Received 9 coated substrates from MLD. They have been sent to Roger
Route at Stanford to be characterized for absorption.
AdLIGO Suspensions
Calum Torrie
Janeen and I went over the proposed plans for pre-prototype work with
Norna Robertson at Stanford and Eoin Elliffe and Mike Plissi in Glasgow.
As a result I added to the existing AUTOCAD drawings that were in workshop
with Ricardo Paniagua.
The various off the shelf parts we require have arrived.
Designed the upper mass, including all of its extra parts, for the
prototype Mode Cleaner suspension in AUTOCAD. The position of the centre
of mass and the exact mass is now known. This latter is crucial for the
blade design.
Continued discussions with Glasgow of tests on existing blades. Eoin
Elliffe is producing good results so far. Hope to verify with experimental
data from GEO 600 soon.
Janeen Romie
We have some C-250 maraging steel on order, due for delivery in early
January in time for Norna's visit.
Working with Calum and SEI folks on blade design.
Mark Barton
This week I did a final tidy-up of my suspension model and released
it: <
http://www.ligo.caltech.edu/~mbarton/SUSmodels/asus4v2/index.html>.
It
has all the features I planned for it except that I withdrew the export
to Matlab feature because I struck a bug/misfeature in the Export[]
command. It's obvious how a workaround can be done, but I wanted to
release something useful in advance of the suspension modelling meeting
next week.
For additional information about this report, contact sanders@ligo.caltech.edu