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The LIGO Executive Committee Agenda for Monday May 5, 2003 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items: MAIDEN WIND FARM PROJECT (RAAB), NSF REVIEW OF ADVANCED LIGO (DAVID), SEI AND EPI PROJECTS (COYNE)
to: LSC Executive Committee
from: R. Weiss April 29, 2003
concerning: Notes from the LSC Executive Committee meeting April 25,
2003
LIGO I authorship guidelines
----------------------------
The list of LIGO I authors is being prepared and will be posted
once completed. ...
Policy for and status of the "upper limit" papers
-------------------------------------------------
It has been more difficult to pull together the papers than many of
us had imagined. Alan Wiseman has suggested that we do not impose unlikely
to be achieved deadlines since these tend to produce incomplete
drafts for which there has not been enough preparation. Instead he
now suggests the following steps:
Policy
------
1) Submission of only completed drafts
2) Place these drafts in the DCC for 1 week to allow comment by the
LSC
3) Provide time (weeks) to respond to the comments and suggestions
4) Give the iterated drafts to the reviewers for comments and recommendations
5) LsC Executive committee discussion based on the reviewers recommendations
The current status of the papers:
---------------------------------
Stochastic: Work on the assignment of random and systematic errors
to the
results. The paper is very close to completion.
Inspiral: Monte-Carlo simulations in process. Parts of the paper are
being
rewritten.
Burst: A first draft was completed and is currently with the reviewers
for
comment.
Periodic: The data for H2 is being rerun to account for the timing errors.
LSC organization of GRID computing
-----------------------------------
Patrick Brady reported on activities of the LSUG (LSC Software Users
Group) and
GRID computing. The group has begun to write software to be used on
the GRID for
ringdowns and periodic sources. LSUG is composed of people across the
collaboration
including the LIGO Laboratory and is specifically dealing with short
term scientific
computing issues to bring the GRID into current data analysis. Al Lazzarini
argues that we need also to look at longer term problems associated
with GRID as
is being done by the GRIPHYN collaboration in which the LSC plays a
role. The
issue is how to bring the two groups together naturally. The consensus
was that
as long as both groups contain membership across the LSC the coupling
will
occur and that there is not a serious problem.
DISCUSSION OF A SCIENCE RUN BETWEEN S2 AND S3
----------------------------------------------
The seismic retrofit in Livingston is now most likely to be installed
after
the beginning of the New Year 2004 so that the ability to operate both
day
and night in Livingston will not be possible until the spring of 2004.
The S3
run is intended to give both high sensitivity and high duty cycle and
will
not be carried out unless Livingston is able to operate during the
day. There
are shorter term goals that could be met with a science run in the
fall 2003
that would be consistent with commissioning. A discussion was started
about the
aims of such a run and what would be desirable. These include:
* a factor of 10 in reach (factor of 2+ in sensitivity)
* close to equal sensitivity in all three interferometers
* more stationary noise spectra and reduction in impulsive events
* more consistent and constant calibration with time
The criteria for such a science run will be further discussed at the
airport
meeting on May 1 and a decision needs to be made to allow planning
for the
commissioning steps.
LSC ROLE IN THE NSF REVIEW OF THE ADVANCED LIGO PROPOSAL
---------------------------------------------------------
David Shoemaker has contacted members of the LSC who could help in
the presentations to be made to the NSF review panel that will meet
in
Pasadena June 11-13.
Peter Saulson suggested that the review include a formal plan of how
the
LSC contributions to the Advanced LIGO detector hardware will be managed.
LIGO Data on the GRID
-----------------------
Al Lazzarinni raised the question of access to LIGO data on the GRID
by
computer scientists not interested in performing LIGO data analysis
but
interested in learning how to manipulate large data sets and remote
computations
on the GRID. He has written a template MOU between the LIGO Laboratory
and the
computer science groups providing rules for such data use and protection
of the
LIGO data.
Author Naming Conventions for the S1 and S2 papers
---------------------------------------------------
After a brief discussion it was decided to conserve space in the
journals by using only initials and last names of the LSC authors.
Next LSC Executive Committee meeting
-------------------------------------
Friday May 23, 2003 at 11AM Eastern time
LIGO Weekly Site Telecon (Lindquist)
There was no site teleconference on Thursday, May 1, 2003.
The list of current actions revised to reflect
the status of open actions assigned through April 17, 2003 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
| WE 05/01/03 | Packages | Faxes |
| In | 25 | 34 |
| Out | 24 | 21 |
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)
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Out of the office on 5.02
Weekly Advanced LIGO Project Controls meeting was not held this week.
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/
Advanced LIGO MRE Proposal (Highest Priority)
Cost Book Tool.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
The Construction project quarterly report for the end of February was scheduled to be submitted at the end of March. Irena has been working on this, but has been distrtacted by a number of other priority issues: LSC, contract activities for seismic isolation, core optics, etc. We have discussed priorities, and the quarterly report is still slipping.
I am scheduled to meet with Barry on Monday to discuss the NSF request for a cost increment for Operations in FY 2009 associated with operating an Advanced LIGO Detector--2009 is theoretically the first year of operations with Advanced LIGO. I have started a model for projecting FY 2009 operating costs, and I have requested additional input from Dennis, David, Fred, Mark, Albert, etc. However, the model is quite crude and there is little basis at this point for deviating significantly from straight escalation except for the fact that we will have installed an additional $100 to $200 million worth of equipment.
Paraphrasing a note from Tom Lucatorto: Very good news! The Office on Multidisciplinary Activities (OMA) and the Office of Informal Education (OIE) at NSF have agreed to support a LIGO video at the level which should enable us to end up with an excellent product. OLPA (Cliff Braverman) is formulating a plan for the project including a very brief description of the project along with a time line just to give the funding sources some idea of the general outlines. We conducted a conference call with Cliff, Tom, Jill Andrews and myself. The current plan calls for publication of a statement of work on the web in about two weeks and a total of 19 weeks for selecting a vendor.
I will need to be in close contact with the schedule for commissioning
and running the detectors to permit us to take advantage of opportunities
for filming interesting activities (e.g., equipment installed in the vacuum
systems, people working in the portable clean rooms, actual operation,
etc.)
The following change requests have been submitted for
consideration by the LIGO Change Control Board (possibly during the Executive
Committee Meeting scheduled for Monday, May 5, 200:
| CR-030008 | Furniture for the auditorium lobby, interaction area underneath the skylight atrium in the OSB, and on the second floor interaction area of the new laboratory/office building. | M. Coles | April 29, 2003 |
| CR-030009 | Cabinets, Case Work, Furnishings at Livingston | A. Sibley | April 29, 2003 |
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
The annual safety audit of LHO was completed during the past week. The main topic on the agenda was the status of the laser safety interlock system installation and operation at LHO (including some discussion/comparison to the LLO interlock system). The LHO system design and operation has evolved successfully to the point where LHO is now planning to make the beam shutter feature operational.
One aspect of LHO laser safety that requires more work has to do with developing procedures for tracking the removal and replacement of port covers. One thing that has been done is to apply labels and extra warning hardware to some ports and covers to identify those locations that have a higher risk of laser beam exposure than others (however, all ports are still considered "dangerous" and will always require appropriate safe guards).
Generally, LHO continues to display a very good safety program. There were some new action items generated. However, most of them are related to items that LHO was already working, but needed some guidance/input from the audit team.
Contact with Physical Plant was made to start the process of obtaining
cost estimates for a fire suppression system for the LIGO Server Room in
Bridge Annex.
Summary of Commissioning Activities at LIGO Hanford Observatory
(compiled by D. Sigg)
The automated power reduction system was put on the 4K ifo. This will
allow
us to increase the power incident to ifo after we have acquired lock
and after
the auto-alignment system has been engaged. This should avoid problems
due to angular misalignment induced by radiation pressure. Elog at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/25/2003&anchor_to_scroll_to=2003:04:25:16:59:37-rick
The 2k POY beam has been characterized. It is far off and our earlier
hope
that it may make it to the table with a larger vacuum viewport turned
out to be
wrong. It looks like a fix will require to adjust the second (small)
mirror of the
beam reduction telescope in order to hit all following steering mirrors.
Elog at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/25/2003&anchor_to_scroll_to=2003:04:25:18:55:37-daniel
The trigger photodetector has been installed and calibrated at the ISCT4
port.
This should show us the maximum power dumped at the AS port, when the
ifo
looses lock. This in turn will determine, if we can operate without
the EO shutter.
Elog at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/26/2003&anchor_to_scroll_to=2003:04:25:23:40:02-peterF
In preparation of higher power operations the transimpedance gain of
the QPD
sensors has been reduced. Elog at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/27/2003&anchor_to_scroll_to=2003:04:27:17:18:40-daniel
A status update of this work is elogged at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/28/2003&anchor_to_scroll_to=2003:04:28:23:22:12-peterF
Work to replace the lossy PMC is ongoing:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/30/2003&anchor_to_scroll_to=2003:04:30:19:47:22-malik
Acoustic noise studies continued on ISCT4. Elog at:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/30/2003&anchor_to_scroll_to=2003:05:01:11:44:32-akiteru
A new large tape library is installed by ldas this week. Ben Johnson
has joined us
to support and maintain the ldas infrastructure.
Commissioning: New FSS board was installed on Thursday and Friday (Rich Abbot, Joe Kovalik and Andri Gretarsson). Due to the fact that LLO picks off the reference cavity beam after the premodecleaner, whereas LHO picks their beams off before the premodecleaner, the board as delivered had to be modified to compensate for this. The new board has a unity gain frequency of about 300kHz and is quite prone to latch in an oscillatory state that sometimes requires breaking of the ref. cavity lock to quench. Since the new board was installed we have had trouble getting the common mode servo running properly and that is the current focus. A new scheme to do wavefront sensing feedback on the modecleaner by feeding back on the mirrors is being implemented. The pitch loop on MC2 has been closed and the other degrees of freedom will follow. (Joe and Valera)
The main interferometer WFS loops were closed last week with low bandwidth. (Gaby, Rana and others). Since then we have been trying to increase the bandwidth and track down suspicious behavior in WFS 3. (Gaby, Andri and others).
The new Frequency Servo board was installed. It has a 300 kHz unity
gain point which is higher than the 100 kHz unity gain point of the previous
board. It does, however, go into oscillation and saturation more easily
than the previous board. A new scheme to do wavefront sensing feedback
on the modecleaner by feeding back on the mirrors is being implemented.
The pitch loop on MC2 has been closed and the other degrees of freedom
will follow. Joe Kovalik
CDS: The following is my progress report for the week of May 1st. 2003,
1) Fixed the Mode Cleaner WFS Servo software bug, now all test points
work properly.
2) Developing Reset Scripts for CDS Target machines, to streamline
target reboot process.
Ash
LDAS admin.
1) Visited Caltech for LDAS workshop and P-card training.
2) Replaced failed disk in T3.
3) Ordered 22 batteries for T3s.
4) 6 days ago we apparently had some power outage that rebooted some
of
beowulf nodes. LDAS repaired itself and seems to be running fine now.
5) Learning DB2 performance tuning. Managed to reduce the run time
of a
typical query for a waveburst table by a factor of 100 by creating
the
right index.
6) Experimenting with databases at LLO and LHO talking directly to
each
other through VPN.
7) Received network switch and new beowulf and datacon.
LDAS data analysis.
1) Made a few minor improvements to waveburst: a) allow user to insert
an arbitrary comment/label per set of jobs; b) search_summvars table
now
contains detailed information about number of different kinds of events
in different channels.
2) Improving the TCL script to handle LDAS failures and retry a job
several times before giving up.
3) Together with Sergey Klimenko submitted a proposal to the burst
group
about using waveburst for S2 analysis.
--
Igor Yakushin
LDAS:
The LDAS VPN is up and in the process of being tested. Igor's database
tools are working well according to him. Everything so far is working as
expected. I still need to mirror the configuration to the backup VPNs,
but this will take some coordination with people at the other sites. At
some point I would like to try a recompiled kernel under vmware and see
if it improves the VPN performance.
GC:
Excel has made some requests to run an IIS server here so that they
can interface with the buildings control computer since they are taking
over maintenance of that system. I have expressed my strong objection to
IIS but if they need it, I can work some solutions for them. This box will
have to be heavily protected from the Internet for obvious reasons.
Added some new accounts along with the general everyday maintenance
of the servers.
Working on a quote from Sun for a 280R to replace our web server. Sun
was supposed to contact me a week ago and has not.
Hooking up more network connections in the new building.
Fixed a couple of email problems with the script that monitors the
cryo pumps and notifies various people by email or cell phone. Some people
were not getting the alerts. Allen's problem happened to be witht he cell
phone company.
Quickly approaching the time when I will be forced to restructure out
network and create actual DMZ and internal areas on our firewall. This
will be a major headache for all, but I think it will have to be done this
year.
Seismic Amelioration
Here is the weekly update for the seismic amelioration efforts:
Work on the modal analysis is virtually complete and I am working on
a
report for review by Dennis Coyne, Joe Giaime, and Brian Lantz. Upon
completion, I will post it on my home web page for all those interested.
Marcel
OTHER:
Harry Overmeier and his wife have a brand new baby girl. Her name is
Sarah (sp?).
Approximately 70 teachers and school system administrators used the
LLO auditorium Tuesday for a program to recognize new parish teachers that
have completed their probationary teaching period. The teachers had a brief
talk about LIGO and a tour of the LIGO facility as part of the overall
program for the day.
Construction work to place a traffic control gate at the entrance to
the LLO property from the access road has begun.
Jonathan Kern et. al. are getting quotes for common EPI components in preparation for orders and start of production, pending a recommendation from the review committee and a subsequent LIGO management decision on proceeding with one of the EPI approaches.
A request for a preliminary quote on a site installation
stainless reservoir has been made.
A sample of clear High Performance Fire Retardant
hydraulic
fluid from Chem-Sol has finished optical contamination
testing.
A request for quote on price and delivery of a 55
gal quantity has been made, as a possible alternate fluid.
The fluid biological growth test is showing nothing
after 21 weeks.
Rich Abbott
3. Motor speed control servo isolation amplifier has been tested and is undergoing final packaging for shipment to MIT. This should allow the motor speed control servo to be connected to the commercial motor controller without causing undue noise to be coupled back into the servo electronics.
The LSC timing performance overview is available from
the DCC at
http://www.ligo.caltech.edu/docs/T/T030080-00.pdf.
Its standard format is very similar to the one used for the S1 LSC timing
overview document (http://www.ligo.caltech.edu/docs/T/T030070-00.pdf).
During the Second Science Run (S2), we measured the
offset of the DAQ time stamp for the LSC channels relatively to the
GPS second tic at the three observatories. In this document (T030080-00.pdf)
we provide the time evolution of these offsets for the three LSC systems.
The results show a significant and very encouraging
improvement in timing performance relatively to S1. Among the three, the
H1 timing was the most stable. H2 was proven to be less stable, showing
a few small jumps during the run. The L1 timing was more irregular,
as there were large number of jumps and cases of prolonged timing problems
(e.g. lightning or GPS antenna induced).
In the document, for each interferometer, we report
- the minute trend for the entire S2 duration
- the distribution (histogram) of the timing measurements
for each significant time segment
- a Gaussian fit and its parameters for the core of
each histogram
- a table summarizing the nominally valid offsets
(from the fit) for each distinct and significant time interval
Summary of results :
>> LIGO Livingston 4K LSC timing for the S2 run:
- Nominal offset : 5 ± 5 microseconds
(except from two short segments
with 14 ± 2 microseconds)
>> LIGO Hanford 4K LSC timing for the S2 run:
- Nominal offset : 2 ± 1 microseconds
>> LIGO Hanford 2K LSC timing for the S2 run:
- Nominal offset : 2 ± 1 microseconds
NOTES:
.. The quoted values are the measurements of the offset
of the DAQ time stamp relatively to the GPS second tic. The time stamp
of the data refers to the ADC input without any input filters.
.. The + sign in front of the offset means that the
DAQ time stamp second mark is after the GPS second tic.
.. Please note that the quoted errors are statistical
in nature and the systematic errors are not included.
.. Please remember that, in particular, we do not measure the arrival time of a GW wave, the DAC output or the time of the calibration excitations on the test masses. The first has to take into account the delay in the electronics at the AS port as well as the analog filtering, the second has to take into account the delay in the digital system sending data to the end station DSCs, and the third has to add the analog output filtering as well as the characteristics of the current drive and the pendulum transfer function.
- Continued installation of 40m systems. All controls
now installed and under
test. One problem has been that the suspension VME
software would die (or appear
to) after anywhere from 5 minutes to 5 days. We installed
a bus analyzer and
found that the new 2Gbit network card was hanging
up, continuously replying on
the bus with Target Device Not Ready - Retry. Unfortunately
for us, this is not
a bus error, therefore the processor PCI interface
chip will forever retry and
not return to the code. We found this was happening
on a read cycle after we did
16 writes to the card, but again, not always as it
can run for some time. We
contacted the vendor and after sending a few bus analyzer
traces to them, they
were able to recreate the problem in their lab and
are working on it. In the
meantime, by changing our code from writing to the
network card to instead
command the card to become the bus master and read
from the CPU memory, we are
able to get around the problem.
- I will be at LHO next week. I want to test the latest
LSC code, plus there are
some further change requests pending to the LSC code
and End station software.
The latter will also involve changes to the ASC software.
1. Put modifications on FSS card per instructions
from LHO. Obtained results that are not consistent with LHO results.
Cause under investigation.
2. Preliminary checkout of all ISS circuitry
is complete and satisfactory. The servo is being moved to the Lauritson
facility for further testing prior to Flavio's 12 May trip to LLO.
3. Mohana is testing boards as part of a large
board build including demodulator boards, DC drivers and more.
4. Built up another RF sniffer for final test. Will be shipping it to the sites for use in spot checking crate and rack RF isolation in the field.
Jay Heefner reporting
LOS Coil Whitening:
Boards have been received and are being stuffed. One should be ready for
bench test by 5/2.
Frequency Devices DAC: Noise testing of the prototype
continues. More should be known by next week.
EMI Retrofit:
- Preliminary test results and observations indicate
that both the Elma and Dawn VME crates provide significant shielding compared
to our present crates and the level of shielding for both is equivalent.
Mechanically, both crates need a few modifications. The suggested improvements
and observations have been sent to the respective manufacturers for comment.
We should hear back from them in trhe next week.
- The shielding of the Equipto rack was verified to
be as shown in the catalog. The interior fan used is extremely noisy electrically.
We also had some questions about lifting eyes and earthing connections
that have been sent to the manufacturer. They are looking for a better
fan and have said that they can provide lifting eyes and earthing points
in future units.
- The Knurr racks have yet to be delivered.
Sander Liu
Built 64 bypass jumper plugs for couple of 40M anti-aliasing
filter chassis.
Rewrite HEPI electronic design requirement draft
The laser shutdown twice this week due to a thermal
overload. The NPRO
went into standby. Opening up the needle valve
did not appear to remedy
the situation. Whilst the laser was down, I
re-arranged the plumbing to
adjust the pipe plug temperature probes. Now
at last I can reconcile the
temperature readings from them and two external thermometers.
When the
laser is in standby the amplifier heat load is 265
W, which is just about
half the cooling capacity of the chiller. This
is with short 7 ft. hoses.
There is a 1 degree temperature drop across the amplifier
when the laser is
operating.
Components on the PSL Lab optical
table have been re-aligned. Beam
profiles were measured at various points of interest.
Some problems were
encountered when the measured profile differed from
the calculated one.
The optical setup for testing of the new intensity
stabilization servo was
installed, ready for the full on power up test.
I started laying out the PCB for
a prototype 500 mA photodetector.
This will be a modular improvement over the current photodetector design.
Detailed drawings are complete for all errant beam baffles and the RM reflected beam cavity beam dump; vendors are expected to start fabricating the parts by 5/1. The skirt design for protecting the control wire ribbon cables on the errant-beam sides of HAM1 and HAM2 are in process.
The final detail drawings for the sheet stainless
steel baffles for MMT2 and MC2 are in the shop, table wire baffle drawings
are finished and will be sent to the fabricator 5-1
The sheet metal shop quotes approx 10 days for the
cutting and forming.
The aluminum attachment bracket feet and 304 stainless
beam traps are in the shop and scheduled to be finished 5-9.
The stainless parts will be baked using the same method
as used for the existing tube baffles.
This process makes the surface non-reflective at 1064nm, and should take 6 days to complete after receipt of the parts.
ITM03 went thorough several etching procedures. The
AR reflection is now 450 ppm. (see report below) I will stop the cleaning
at this time since I do not want to compromise the coating integrity.
Liyuan and Lee will scan the optic to test the uniformity
of the coated surface. They will also characterize the HR coating and possibly
measure scatter.
As requested by Doug, we expect to ship the optic to Hanford around May 12th.
OTF Lab. (W. Bridge)
Contamination Cavity # 1
The test sample kAPTON (Polyimid paint) still pumping DOWN.
We are taking ring down and beat frequency measurements everyday.
Please see Dr. Zhang graphs for absorption, ring down and thermal lensing.
Absorption Test Measurement prototype in PROGRESS
Scatterometer
Measurements of AR, HR reflectance, scattering and transmission of
different mirrors are completed.
The large mirror ITM S/N 2ITM03 after itching for the fifth time has
been measured.
The reflection of the AR coating is ~450 ppm. (previously was 110 ppm)
We are scanning the AR coated surface of the optic to test its uniformity.
We'll also characterize the HR coating and measure its scattering.
Mirror 2ITM01( R~600 PPM, T~ 3% Manuf.) AR coating reflectance measured ~ 1800 PPM.
We have received new mirrors, lens and mounts. We'll install it ASA time is permitted.
OTF Lab at Lauritsen ROOM 38
Cavity #3
The new test sample SR FR HF from Chem-Sol, Inc. an Undyed Fire
retardant Hydraulic Fluid still
under test. We are taking ring down and beat frequency measurements
everyday. The test will end this week.
Please see Dr. Zhang's latest graphs for absorption, ringdown and cavity
thermal lensing measurements.
Cavity #2 Test cavity
The chamber is pumping with new cleaned mirrors ~ 70ppm each.
RGA measurements and optical train set-up is still in progress as we
continue to improve the set-up.
learning from previous experience set-up. NO CHANGE.
We have made some substantial progress at the TNI since our last report.
Stan Whitcomb came down to the lab and helped us do some diagnostics on
the instrument, mostly looking at coherences between NAC and SAC, between
the arm cavities and the mode cleaner, and between signals tapped at different
points in the mode-cleaner servo. We came to the conclusion that one prominent
noise source in the instrument was laser-frequency noise coming from electronic
noise in the mode-cleaner servo. After doing a quick, back-of-the-envelope
calculation, we decided that turning up the power would reduce this electronic-noise-limited
laser-frequency noise by a factor proportional to the increase in power.
Akira Villar, our new graduate student, built a new notch filter to take
care of a 22.897kHz body mode that had been cropping up in SAC's output
mirror, and he built a couple of voltage dividers to cut down on the electronic
gain in the arm-cavity servos. (Many thanks, yet again, to Flavio Nocera
for help with the notch filters!) We wanted to cut the electronic gain
in the arm-cavity servos down so we could increase the photodiode response
and, hopefully, reduce the total noise. (Again, back-of-the-envelope calculations
showed that this should help.)
The notch filter worked nicely, and we were able to go to full power
in the instrument for the first time in almost a year. This is mostly thanks
to the new, very robust servos we developed last year. Many months of hard
work improving the duty cycle and acquisition time of the instrument, with
no gains in sensitivity to encourage us, are finally beginning to pay off!
Bringing up the power did improve the laser-frequency noise, and that alone
improved the sensitivity in the arm cavities by about a factor of two around
1kHz.
Unfortunately, we were unable to increase the discriminant in the arm
cavities. The voltage dividers worked well in isolation, but depending
on where we placed them in the loop, they "ate" phase, dynamic range, or
even gain depending on which element they fed a signal into. We will have
to make changes to the arm-cavity servo filters on a lower level to get
room to increase the discriminant.
Bringing up the power in all three cavities had one, unexpected benefit.
The coherence between NAC's and SAC's error signals got cleaned up at high
frequencies, essentially becoming unity between 10kHz and 60kHz. This allowed
us to implement common-mode rejection and bring the total noise floor of
the instrument, the difference between the two arm-cavity signals, down
by a factor of ten over a wide range of frequencies. The differential-mode
noise is almost completely flat at 2e-18 m/rHz from 1kHz all the way to
60kHz. This is exactly what we should expect, based on the electronic noise
in NAC's photodiode. Increasing both NAC's and SAC's discriminants should
bring this noise level down.
LASTI (Allen, Coyne, Mason, MacInnis,
Mittleman, Ottaway, Rollins, Shoemaker, Zucker)
---------------------------------------------------------------------
MEPI Progress (Ottaway, Mittleman, Rankin, Zuo, Nayfeh, Allen)
----------------------------------------------------------------------
We installed and tested two damping systems on the HAM support
structure.
A tuned mass damper was placed on one of the HAM stiffening beams in
order to damp the 51Hz vertical motion. The results can be seen on
the LASTI ilog for April 28. The peak in the relevant modal transfer function
(Y-direction) was reduced by a factor of 5.
Two piezoelectric damping packs (originally marketed for
high-performance snow skis) were glued to the other HAM stiffening
beam. So far these do not seem to be very effective at reducing the
51Hz
peak.
We have also been working on the low frequency characterization of the
HAM plant and control system.
Dave O did a crash test on MEPI when the system was set to an
offsett of 0.2 mm and dropped. A peak velocity on the optics table
of 0.5 mm/s was observed. This was predominantly at the stack mode frequency
of 1.6 Hz.
-------------
LDAS Software
-------------
Work continues on supporting RDSs with multiple interferometers. With
the basic coding complete, testing is being done with LDAS raw frames
to ensure backwards compatibility and to validate new functionality.
The output directory for RDS creation can now be protected to prevent
multiple users from creating RDSs with the same pattern.
Progress has also been made in supporting the newer version of autoconf
and automake. For the 0.7.0 release of LDAS, these tools will be
upgraded as to ease compilation of the standalone wrapper under either
RedHat 7.3 or RedHat 9.0.
The base64 support in LIGO_LW is going through final testing and should
become part of CVS by the end of today. Several of the APIs were
modified to support this functionality.
Improvements to the metadataAPI insertion code resulted in an increase
of performance of 30%. These changes were all at the TCL level.
The controlMonitorAPI client is being modified to support system
validation testing. This will provide a means by which an LDAS
administrator can verify that their installation of LDAS can perform
the basic functions. The scripts for verification come directly from
the scripts LDAS uses in its own integrated system testing.
The dischcacheAPI now supports multiple matches scored by precedence
of ::MOUNT_PT entries and it supports matching of
multiple-interferometer frame files.
Philip Charlton:
Still working on creating S2 RDS. Have now done
about 45% of
LHO and 35% of LLO. New tape drives were installed
yesterday and this
should help speed the process.
LDAS coding:
added "sum" function to datacon
extended statistics code to work on complex data
fixed bug in "oelslr" function which
gave bad error message
for an invalid argument
checked in and validated code from Antony
Searle (ANU) for new
signal generators
made many changes to web documentation
(corrections and additions)
--------------------------
LDAS System Administration
--------------------------
Caltech
-------
(Dan Kozak)
* Continued to manage SAM-QFS resources to facilitate create of RDS frames.
* Worked with STK to get new drive wall and 4 new 9940B tape drives
installed--DONE! This involved a non-trivial amount of
HPSS wrangling.
* Configured new drives for use with SAM-QFS. They're in use now,
but
due to the 9940Bs writing higher density than the 9940As, more
work
will be required to fully integrate them.
* Upgraded all T3 RAID units at LHO to pSOS v. 1.18.02.
* Upgraded LHO's dataserver & gateway to SAN-4.2.
* Upgraded LHO's dataserver to full SAM-QFS (from standalone QFS),
version 4.0.26L.
* Upgraded LHO's gateway to latest version of standalone QFS (4.0.26L).
(Al Wilson)
* Getting ready for the arrival of the new Beowulf nodes.
* Clearing space, setting up racks, testing configuration for RH9.0.
(Stuart Anderson)
* Meeting with Caltech Engineers to obtain an additional electrical
panel and another 12 Tons of cooling for the large Beowulf cluster
to be installed at Caltech.
* Switched archiving of LHO and LLO trend frames from HPSS to SAM-QFS.
No new LIGO data should be written to HPSS.
* Received the 232 GigE port Beowulf network switch for LDAS-CIT.
* Received 6 new dual 3GHz/4GB P4 Xeon boxes for LDAS Beowulf and Datacon
server upgrades of LDAS-TEST, LDAS-DEV, and LDAS-CIT.
* Placed order with Bill Tyler for additional rack equipment for
Caltech and MIT.
* Finalized the T3 contract with Caltech purchasing and the Vendor in
order
to obtain contract service to replace the batteries in the 11
T3 units at
Caltech.
* Tracking the last large LDAS construction account procurements.
MIT
---
(Keith Bayer)
* Moved LDR to /export partition after filling up /usr1.
* Looked into ENOMEM error msg on pc raid unit.
* Tweaking LDR to prioritize certain segments of data to MIT.
* Received new datacon and beowulf P4's from ASA.
* Working on upgrading power for cluster nodes in ldas lab.
Livingston
----------
(Igor Yakushin)
* Visited Caltech for LDAS workshop and P-card training.
* Replaced failed disk in T3.
* Ordered 22 batteries for T3s.
* 6 days ago we apparently had some power outage that rebooted some
of
beowulf nodes. LDAS repaired itself and seems to be running
fine now.
* Learning DB2 performance tuning. Managed to reduce the run time of
a
typical query for a waveburst table by a factor of 100 by creating
the
right index.
* Experimenting with databases at LLO and LHO talking directly to each
other through VPN.
* Received network switch and new beowulf and datacon.
(Shannon Roddy)
* Much of this week has been spent getting the VPN up between the sites
for LDAS. The VPN is up between MIT, LHO and CIT.
LLO will be up
tonight.
* Also been working with the electricians on some network wiring issues
in
the new building, some of it involving the LDAS room and GC
connections.
* The LDAS VPN is up and in the process of being tested. Igor's
database
tools are working well according to him. Everything so
far is working
as expected. I still need to mirror the configuration
to the backup
VPNs, but this will take some coordination with people at the
other
sites. At some point I would like to try a recompiled
kernel under
vmware and see if it improves the VPN performance.
Hanford
-------
(Greg Mendell)
* Ben Johnson has started as an Assistant Engineer, assisting with LDAS at LHO.
* Supported the installation of the StorageTek L700e Tape Library System
at LHO. The installation was completed by StorageTek on
04/23/03.
* Assisted with the assembly of 3 racks to support the upcoming
installation of the new beowulf cluster at LHO.
* Finished setting up LDAS VPN boxes at LHO for Shannon Roddy to
configure. (There was a problem with the GC network connection
to the
boxes, and the spare box needed temporary IP addresses so that
both
boxes could be plugged into the network at the same time.)
* Working with Ben Johnson to rebuild and test the repaired beowulf
nodes returned from ASA.
* Arranged to have Sun replace the batteries in all of our T3s which
have reached their 2 year lifetime. Sun has ordered the batteries,
but they are on back order.
* Worked with Dan Kozak and Ben Johnson to upgrade the QFS licenses,
SAN, and the T3 raid controller firmware on the LDAS system
at LHO.
One QFS license is still needed, and the system is still down
pending
work on the AC.
* Continuing to prepare for the installation of the new beowulf cluster
at LHO.
* Assisting Igor with the transfer of ndas data from CIT to LLO.
(Ben Johnson)
* Assisted in the assembly of three computer racks for the upcoming
beowulf cluster.
* Assisted in the hardware installation of the new StorageTek L700e
tape library. Installation completed on 4/23/2003.
* Worked to diagnose continuing problems with an ASA Computers beowulf
node. Set up self as LHO contact person for this problem.
* Assisting Dave Barker with installation of weather station
monitoring/operator alarms in the LDAS computer room.
* Working with Dave Barker on the temperature monitoring software for
the LDAS computer room.
* Assisting Greg Mendell with bringing up and shutting down the LDAS
system at LHO. This is due to the expected work on the cooling
system
this week.
* Responded to disk full error on LHO metaserver.
* Performing burn-in tests on three beowulf nodes. Wrote new script
to
perform md5sums on burntest output files.
-----------------
General Computing
-----------------
MIT:
(Keith)
-Investigating IPsec for our wireless network
-Testing MIT network speeds to another location on campus
-Investigating RedHat up2date utility for laptop users
Livingston:
(Shannon)
-Excel has made some requests to run an IIS server here so that they
can
interface with the buildings control computer since they are taking
over
maintenance of that system. I have expressed my strong objection
to IIS
but if they need it, I can work some solutions for them. This
box will
have to be heavily protected from the Internet for obvious reasons.
-Added some new accounts along with the general everyday maintenance
of
the servers.
-Working on a quote from Sun for a 280R to replace our web server.
Sun
was supposed to contact me a week ago and has not.
-Hooking up more network connections in the new building.
-Fixed a couple of email problems with the script that monitors the
cryo
pumps and notifies various people by e-mail or cell phone. Some
people
were not getting the alerts. Allen's problem happened to be with
the
cell phone company.
-Quickly approaching the time when I will be forced to restructure
out
network and create actual DMZ and internal areas on our firewall.
This
will be a major headache for all, but I think it will have to be done
this year.
Hanford:
(Christine)
- Narrowing in on what equipment is needed for the GigE network
upgrade. The quotes from the vendors included quite a lot of
extra
equipment and it has taken quite a bit of time and research to figure
out exactly what is needed and what is not.
- Had to reboot our router a few times because of "out of memory"
errors. Can't wait for the new router to arrive. Also,
had to change
the access list for the TRINET computer.
- The usual user support for on-site and off-site users.
CIT:
(Mike)
-Worked on the PC located in the conference room, setting it up with
the
VRVS software. There was a problem with the audio not working with
VRVS
software. I ended up down loading updated drivers from the manufactures
website. This corrected the problem.
-Updated ghost images on Irene Baldon & the PC in the conference
room.
-Loaded a new laptop for Phil Willems & Bill Kells. This included
GC
software and additional engineering packages. Plus I transferred over
Bill
Kells old data over for him.
-Setup a VRVS meeting in the SCR for a LIGO seminar. I had multiple
problems with this setup and now know that I must give myself more
time for
setting up future meetings.
-Reloading an engineering workstation for Calum & Janeen.
-Loading a laptop for Erica D'Ambrosio; I have a few more applications
that I have to load and get a ghost image of this laptop for a quick
recovery.
- M79, The ghost server is having some Operating System problems and
have ran
out of disk space. This did corrupt some data. I am in the process
of
reloading this server. After I have completed working on this server
I will
be updating all our windows workstations.
-Updated ghost images on the following servers: Amaldi, Antares, Pherkab,
Pc72.
(Lisa)
-Finished the www.ligo build. It is ready for Larry to look over.
- More user e-mail support. Most of the discomfort of moving
over to becrux
seems to have passed now.
- Did monthly backups. This required a rewrite of the monthly
backup scripts
(again) to accommodate the unpredicted growth of a few home accounts.
Here I
ask
that the few people who regularly fill up their home account with things
that
are more appropriately placed on a local disk space, please be more
conscientious.
(Veronica)
-LIGO website: posted various updates. Looking into a DCC database
to
see if a missing document indicates a problem.
Most time was spent working on a website for the upcoming Advanced
LIGO
NSF review.
Continue capturing the footage of the LIGO miniDV video archive into
files
for non-degradable archiving.
- LSC website: posted a few updates, the usual upkeep.
- CaJAGWR website: posted updates, working on a smil combo of the last
talk.
(Larry)
-Worked a number of procurement issues. The paperwork and checking
on items is a
never ending task. A number of the past orders has started arriving,
including
the equipment for LDAS.
-Worked a number of DCC issues. Most related to document transfers
and file
fixes.
-Spent a deal of time working on a s/w licensing issue. Most of the
items have
been cleared up and the rest of the concerns are being dealt with by
Dennis and
others.
-Spent time working on some VRVS issues.
-Re-tested one of the servers for security holes. Still have a few
more items to
change before it gets put out.
-Worked with Lisa on getting a number of accounts cleaned up.
-Assisted in a number of equipment moves and installations. Working
on more
modifications to the server room.
-The regular user assistance. Just as a note we are spending 1-2 hours
a day
going over the e-mail logs checking for false positives and related
items.
Putting a filter on my Caltech account has helped a great deal on eliminating
the spam that was getting through to my account on the LIGO mail server.
_______________
E2E MODELLING:
_______________
SimLIGO results
-----------------
(Matt)
This week I wrote a draft technical note concerning the implications
of
thermal lensing and the 4k asymmetry for lock acquisition and
lock
robustness. The note, T030089, also proposed a solution
to the problems
presented. I tested the proposed solution, use of the non-resonant
sidebands to generate an LSC signal for CARM, in SimLIGO.
The test showed
that this control scheme is robust, at least in simulation.
LLO seismic modeling
----------------------
Qualitative and quantitative seismic modeling of LLO is still
going,
being carried out by Hiro, Sany and Tiffany. A LIGO document
will be
released in a few weeks.
Dynamical misalignment
------------------------
(Biplab) A few more points regarding differences between e2e and Daniel's
results have been sorted out but one major concern for us is
the absence of
a zero signal notch in transfer function (from say differential
ETM to
dark port) at half the FSR.
Dual recycling Michelson cavity- summation model formulation
------------------------------------------------------------
(Hiro) Based on the discussion with Hiro, Osamu could find an analytic
formula necessary to complete the summation cavity module of
a dual
recycling Michelson cavity. With this expression, the internal
field of
a cavity can be expressed using a finite number of terms - number
being
depending on the accuracy required. This formulation will be
used in an
e2e primitive which can speed up the simulation speed by a factor
of 100.
Also important in this calculation is that all physics quantities
are
treated using a linear approximation. This allows the simulation
of
frequency noise and the common mode servo.
This formulation will be used in all the summation cavities in
the
future version of e2e. The explicit formula for the dual recycling
summation cavity was the last missing one. The details will be
documented in a LIGO document.
Code development and maintenance
---------------------------------
e2e distribution:
Hiro, Bruce and Ed worked to setup a new e2e distribution kit.
So far,
e2e tarball contained both the simulation software and GUI software
(alfi). From the next release on, a tarball contains only the
simulation software, and the README file included explains how
to get
the latest alfi. This is done because of two reasons. One is
that alfi5
is updated more frequently, and Bruce has setup to download the
latest
one automatically using JAVA Web Start. Second is, it comes out
to be
too complicated that one installer script is used to install
both
g++-based softwares and JAVA-based software.
(Biplab) A bug in recycling summation module is fixed. This bug
(in recycling_sum.cc) was giving a wrong sign to the "distance
to waist"
value [for the modal basis] of the dark port output light.
So, in SimLIGO, the WFS signals obtained so far after the
dark port light passes thru telescopes were not correct.
Signals calculated (e.g. by me for comparing with Daniel's results)
just
at the dark port were correct though because this basis parameter
does
not affect the amplitude of lights coming out of dark port.
When the dark-port light was propagated by telescope, wrong guoy
phase
was added to the beam and as a consequence a wrong signal was
calculated
on interference.
After the bug-fixing, Matt could make the WFS work again with
new signals.
(Hiro) Working on updating the simulation code to speed up by improving
the expression parser and to set the user have more control on
the output
data.
(Ed Maros)
1. Enhanced the building process for the e2e code.
2. Eliminated the building of JAlfi, Alfi, or Adlib.
Alfi
-----
(Bruce)
- Cleaning old code which
depended on casting to Port and
Junction objects
instead of using the new GenericPort
superclass for
these.
- Fixed several bugs created
by forementioned code cleanup.
(Melody)
- Worked on fixing
some problems with the cut/copy/paste feature.
-------------
Data Analysis
-------------
Teviet Creighton:
I have been doing a detailed study of precision issues in my LAL
time-domain filtering routines. The PUL group reported ``nonlinear''
results from these routines, which turned out to be digital precision
noise due to the large dynamic range of the pre-filtered data (thus
multiplying the pre-filtered data by a constant yielded slightly
different output than multiplying the post-filtered data by the same
constant). I am now performing tests to see whether this can
be
reduced at all by applying a double-precision filter to
single-precision data.
Igor Yakushin:
1) Made a few minor improvements to waveburst: a) allow user to insert
an arbitrary comment/label per set of jobs; b) search_summvars table
now
contains detailed information about number of different kinds of events
in different channels.
2) Improving the TCL script to handle LDAS failures and retry a job
several times before giving up.
3) Together with Sergey Klimenko submitted a proposal to the burst
group
about using waveburst for S2 analysis.
From: sheila rowan <srowan@fastloki.Stanford.EDU>
Pierre's RA and Student (GoksenYaralioglu and Ira Wygant) now have (preliminary) measurements of 3 coatings, each on a silica substrate.
One SiO2/Ta2O5 coating from MLD (part no 8107)
One Al2O3/Ta2O5 coating from MLD (part no 5701)
and
one Al2O3/Ta2O5 coating from Waveprecision
(part no. 8223).
They made two measurements on each coating to test reproducibility.
In essence they measure the difference in (acoustic) reflectivity between water and the coating and water and the substrate and thus extract information about the properties of the coating.
They then model their experimental results using a combination of values for the coating thickness (which in principle we know well), density, Poisson's ratio and Young's modulus.
The fit to their data is excellent for the Al2O3/Ta2O5 coating from Waveprecision (part no. 8223) for a coating Poisson's ratio of 0.2 and a Young's modulus of 2.8e11/2.82e11. This agrees pretty well with our estimates of the properties using known bulk values.
They also get a pretty good fit for the SiO2/Ta2O5 coating from MLD (part no 8107) using Poisson's ratio of 0.2 and Youngs mod. of 9.3e10 or 1.03e11.
Interestingly the data for the Al2O3/Ta2O5 coating from MLD (part no
5701) is very different than the Waveprecision
sample and requires a modelled Young's mod. of
4.38e10 or 2.89e10.
We're not sure what is different about this sample - whether this is
a genuine vendor specific difference or an artifact of the measurement.
We have a second sample with the same coating so they will measure
that as a double check. We will also check the sensitivity of the model
to the thickness of the coating etc.
---------------------
From: Eric Black <black_e@ligo.caltech.edu>
We have made some substantial progress at
the TNI since our last report. Stan Whitcomb came down to the lab and helped
me do some diagnostics on the instrument, mostly looking at coherences
between NAC and SAC, between the arm cavities and the mode cleaner, and
between signals tapped at different points in the mode-cleaner servo. We
came to the conclusion that one prominent noise source in the instrument
was laser-frequency noise coming from electronic noise in the mode-cleaner
servo. I did a quick, back-of-the-envelope calculation and decided that
turning up the power would reduce this electronic-noise-limited laser-frequency
noise by a factor proportional to the increase in power. Akira Villar,
our new graduate student, built a new notch filter to take care of a 22.897kHz
body mode that had been cropping up in SAC's
output mirror, and he built a couple of voltage dividers to cut down on
the electronic gain in the arm-cavity servos. (Many thanks, yet again,
to FlavioNocera
for help with the notch filters!) We wanted to cut the electronic gain
in the arm-cavity servos down so we could increase the photodiode response
and, hopefully, reduce the total noise. (Again, back-of-the-envelope calculations
showed that this should help.)
The notch filter worked nicely, and we were able to go to full power in the instrument for the first time in almost a year. This is mostly thanks to the new, very robust servos we developed last year. Many months of hard work improving the duty cycle and acquisition time of the instrument, with no gains in sensitivity to encourage us, are finally beginning to pay off! Bringing up the power did improve the laser-frequency noise, and that alone improved the sensitivity in the arm cavities by about a factor of two around 1kHz.
Unfortunately, we were unable to increase the discriminant in the arm cavities. The voltage dividers worked well in isolation, but depending on where we placed them in the loop, they "ate" phase, dynamic range, or even gain depending on which element they fed a signal into. We will have to make changes to the arm-cavity servo filters on a lower level to get room to increase the discriminant.
Bringing up the power in all three cavities had one, unexpected benefit. The coherence between NAC's and SAC's error signals got cleaned up at high frequencies, essentially becoming unity between 10kHz and 60kHz. This allowed us to implement common-mode rejection and bring the total noise floor of the instrument, the difference between the two arm-cavity signals, down by a factor of ten over a wide range of frequencies. The differential-mode noise is almost completely flat at 2e-18 m/rHz from 1kHz all the way to 60kHz. This is exactly what we should expect, based on the electronic noise in NAC's photodiode. Increasing bothNAC's and SAC'sdiscriminants should bring this noise level down.
---------------------
Suspensions Report from GEO600
Caroline A. Cantley
1st May 03
A. SUSPENSIONS
A.1.
Discussions are underway between LIGO/GEO600 Glasgow on how to incorporate
RAL in the AdLIGO project. Funding of the
(GEO600
A.2. Monolithic Suspensions in GEO600
Violin modes continue to be investigated. Many closely spaced violin
modes have been resolved (13 identified so far in frequency range 620Hz
to 670Hz) with Q's ranging from 6E5 to 3E6. Recall Teflon has been
applied at selected locations on the fibres
to damp the violin mode peaks and the measured Q's are as per design intent.
(GEO600 team)
A.2. Suspension Wires & Blade Clamp Design / Blades
/ Blade Dampers
The parts for two new designs of blade wire clamps (Caltech/Glasgow
and RAL designs) are currently being manufactured. The testing of these
concepts should be completed in the next month and conclusions can then
be drawn to decide upon the optimum design for future suspensions. The
rig for blade wire clamp testing (in
Cost estimates are being drawn up to determine whether funds are available
to manufacture a blade test facility in
ANSYS modelling of prototype quad suspension
blades is continuing with the model being updated to include the changing
stress distribution with increasing load.
Blade damper drawings based on the GEO600 design have been created
and are currently being refined.
(M. Plissi, M.P. Lloyd,
R. Jones, C. Torrie (Caltech),
A.3. Analogue Electronics for LASTI
Construction continues and a second complete set is ready to be tested
and shipped. We now have confirmation from Mark Barton that the first set
of electronics for the MC were satisfactory with only a minor adjustment
required to the original electronics (gain setting resistors changed to
40K). This change is now being implemented.
(D.I. Robertson, H. Ward).
A.4. Recycling Mirror Suspension Design
The Rotational Adjuster for the Recycling Mirror was redesigned to
introduce improvements and is now ready for manufacture.
(N.A. Robertson (Stanford), C. Torrie/J. Romie
(Caltech), M. Perreur-Lloyd,M.Plissi,
A.
A.5. Mode Cleaner Structure FE Analysis
The boundary conditions used for FE analysis
of support structures was investigated during C. Cantley's
visit to Caltech. Initial models were previously run with rigid boundary
conditions thus giving higher than realistic structural frequencies. To
prove this swept sine tests on an MC structure were carried out (further
to the initial tests previously conducted by M. Barton) to further investigate
the effect of the base clamping method on the lowest modal frequency. The
stiffness of the boundary conditions in the FE model were
then varied to provide coincidence of the lowest modal frequencies of the
FE model and the structure. Further investigations of the effect of the
method of attachment and stiffness of the mounting bench will be carried
out. Ultimately the proposed attachment method to the SEI table will be
considered. C. Cantley will also investigate
suitable equipment for a potential multi-channel modal test facility at
Caltech.
(C. A. Cantley, C. Torrie/J.Romie
(Caltech)).
A.6. Quadruple Suspension Design
Work has started to investigate a quad model with common design of
blades and upper two masses and all wire lengths for suspension of baseline
sapphire test mass (31.4 cm diam by 13 cm
thick) or fallback silica test mass ( 34 cm diam
by 20 cm thick), both 40 kg. The assumption is made that penultimate mass
is also 40 kg and same aspect ratio as test mass.
A basic upper mass for the ETM quad has been drawn up in Solidworks
and is now being edited to match the latest specification provided by the Matlab
model. Over the next month we hope to develop an accurate layout of the
quad suspension by design iteration between the Solidworks
models and Matlab models.
(N.A. Robertson (Stanford), C. Torrie/J. Romie
(Caltech), M. Perreur-Lloyd,
A.7. Hybrid OSEMS
Aluminium coil formers are currently being
manufactured. Drawings for Peek formers have been passed to the
(R. Jones, C. Torrie/J. Romie
(Caltech), C. Cantley, N. A. Robertson (Stanford))
A.8. Ribbon Pendulum Q Measurements
Experiments to test the effect of seismic noise and the validity of
the initially measured pendulum Q of 8.8e8 are underway. Air was
allowed into the vacuum system during ringdown
until the oscillation amplitude decreased to a fifth. Vacuum was then made
again and a second run has started. The Q dropped down from its original
value to 1e8. Charging of the mass could be the reason for the drop since
an electrostatic signal at the pendulum frequency has been detected. Investigation
into the electrostatic effect is ongoing. The orthogonal modes of the pendulum
are also being investigated..
(A. Heptonstall, G. Cagnoli,
K. Strain, J. Hough)
A.9. GEO Mass Catcher Design
The GEO600 mass catcher replica has arrived
from
(S. Go?er,
R. Jones, M.Perreur-Lloyd, C. Torrie/J. Romie
(Caltech), C. Cantley, N. A. Robertson (Stanford))
B.
MATERIALS
See separate report from Sheila Rowan.
-------------------
From: JaneenRomie
<romie_j@ligo.caltech.edu>
Caltech Suspensions Summary - March & April 2003
Natural Mode Analysis and Testing
Caroline Cantley joined us in mid-April
for a very productive visit. We focused on comparison of FEA models (between Algor,
ANSYS and I-DEAS) and experimental results. Caroline's industrial vibrational
damping experience is greatly appreciated. Caroline, Calum
and I performed several experiments on the bare mode cleaner structure.
These suggest that the first mode is around 50 Hz. Both the ANSYS and I-DEAS
model currently estimate the first mode to be ~75Hz. In order to try and
improve this we investigated adding "springs" between the suspension and
rest of the world. Initial results suggest that we should be able to come
up with a reality factor that will allow us to better predict actual mode.
Dennis Coyne has performed detailed frequency analysis of the quad pendulum
structure and has created a preliminary report of this. Ask Janeen
or Dennis for a copy, if you're interested.Caroline
has proposed a series of experiments and analyses to support the quad research
and risk reduction.
Cantley (Glasgow) and Torrie, Romie,
Barton, Coyne, (Caltech)
Recycling Mirror Design
Recycling mirror blade drawings are ready for the RFQ process. A 3D
layout of the RM upper mass is complete but for review of stiffness and
deflection.
Plissi, Lloyd (Glasgow) and Torrie
(Caltech)
Rotational Blade Adjustment
Mike Perreur-Lloyd and CalumTorrie
designed a rotational adjustment for the upper blades on a triple or quadruple
suspension while Mike was here on his last visit. The rotational adjuster
is based on a design created by Alastair
Grant for the MIT quadruple pendulum.
Plissi, Lloyd, Grant (
Mode Cleaner
Efforts to ready 2 mode cleaner suspensions for damping tests are under
way at Caltech and Glasgow. See details in
Jones, Lloyd (
Mode Cleaner Costs
The mode cleaner drawing packages were delivered to three local machine
shops for quote information to support the AdLIGO
proposal. The pricing information has been returned. Calum
and I will tabulate this in preparation for the NSF Review in June.
Romie,Torrie (Caltech)
Quad Design
Norna has created as set of possible parameters
for a proposed silica or sapphire quadruple pendulum suspension for LASTI.
These are currently under review. Mike Lloyd created a 3D layout of an
upper mass assembly to aid with this work.
Robertson (Stanford) Cantley,
Lloyd (
Blade Testing
Drawings for a blade testing facility are nearing completion; these
should be available for workshop soon. This will allow us to more easily
characterize the larger cantilever blades used in the quadruple and RM
suspension. It is as yet un-clear where best this work will be done.
Plissi, Lloyd, Elliffe
(Glasgow) and Torrie (Caltech)
Visits
Mike Perreur-Lloyd will be joining us
at Caltech again from mid-June through mid-July. We look forward to his
visit. Caroline and many members of the GEO suspension group will be at
Caltech to support the NSF review in June. CalumTorrie
plans to visit
Russell Jones from
------------------------
From: RiccardoDeSalvo
<desalvo@ligo.caltech.edu>
MoRuBisa great
material, but we finally concluded that in its present formulation it is
unsuitable to produce mirror suspensions.
It can be produced up to 50 micron thickness (with some trouble) which
would seem more than sufficient to produce the 10 micron (or less) thick
flex joints. The catch is that when we load the 10 micron thick part
close to the required 4 GPa
it elongates 1.6%, and the thick part (the 50 micron one) still elongated
more than 0.3%.
This elongation has to go progressively to zero in the brazed region,
and in this process the stress is transferred through the
braze. This behaviour is called
shear-lag.
We have only two possibly suitable brazes,
one with surface failure shear of 20 MPa
and the other with 50MPa. The first one is softer
(Yields more) and works better, but still nowhere close to requirements.
No other solution was identified.
The problem rapidly fades away if thicker samples could be manufactured.
Two ways are being followed, one is to
fiddle with theMoRuB recipe to try to glassyfy
in mm thick injection molded forms. The other is to use existing
recipes of iron-based glasses that are proven to glassify
at least to 3 mm thicknesses.
These iron-based alloys are less strong (3.8 GPa
instead of 5 GPa for MoRuB)
so they will require thinner and wider joints (say 8 microns instead of
10) to outperform fused silica but allow the production of monolithic hooks
with no braze at all.
We will explore the two possibilities for a few more months.
------------------------------------
From: Larry Jones <ljones@ligo.caltech.edu>
Seismic Isolation (Lantz, Sanders, Petrac, Giaime, Jones & Coyne)
The SEI Structure Proposers' Conference was held at Stanford on 25 April. Eleven representatives from five companies attended. Test hardware was viewed and discussed, including the SEI Tech Demo structure, which has been undergoing tests. Presentations were given on contract strategy, science background of the Tech Demo design, and design requirements, with special emphasis on mass limits, balancing and FEA modeling. The contractors expressed their concern for being able to provide reasonable firm, fixed-price proposals for the Phase II task of design of the structures for HAM and BSC chambers and fabricating a prototype of each for testing. This is due to the unknown amount of iterations that will be required for passing the complex FEA and mass limits requirements. As a result, we are meeting to revise our contracting mode for Phase II.
--------------------
From: Helena Armandula <ahelena@ligo.caltech.edu>
Advanced Coating Development
All coating vendors contacted expressed their interest to participate
in the LIGO Advanced Coating Development Program.
All of them called with some questions or comments except MLD; they
just called Irena and said they would like to participate.
Some of the concerns most of them have is about the doping tests since
it requires multiple large targets which are very expensive. Some mentioned
alternatives such as to do doping in stages as well as other methods to
modify the mechanical properties of the coatings like ion beam assisted
deposition.
Drafting of a formal RFP is in process.
-----------------------
Pre-Isolator work -- please see
http://www.ligo.caltech.edu/~coyne/IL/EPI/review2/EPI_review2.htm
for documentation for the recent review.
From: ctorrie <ctorrie@ligo.caltech.edu>
Quadruple Pendulum
Norna and I have been working with Mike Lloyd
and Mike Plissi in
Workshop
The Physics and Central workshops at Caltech long with the workshop
in
Structure Analysis
Some progress has been made with the analysis of the structures for
the triples and the Quads. Caroline and Janeen
have been taking the lead on this and I have been helping where I can.
RM an MC Suspension
At the same time as working on the Quad model Norna
and I are assessing key aspects in the triple model that are directly related
to the modelling of a quad suspension.
From: Helena Armandula
<ahelena@ligo.caltech.edu>
Advanced Coating Development
All coating vendors contacted expressed their
interest to participate in the LIGO Advanced Coating Development Program.
All of them called me with some questions or comments except MLD; they
just called Irena and said they would like to participate.
Some of the concerns most of them have is about the doping tests since
it requires multiple large targets which are very expensive. Some mentioned
alternatives such as to do doping in stages as well as other methods to
modify the mechanical properties of the coatings like ion beam assisted
deposition.
Irena and I will work in the RFQ hoping to have it ready by Monday
to send it for approval.
From: JaneenRomie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
On Friday, I participated in a fruitful telecon
with Calum and the GEO suspensioneers
about Rutherford Appleton Laboratory coming onboard in June. Caroline will
be holdling another meeting on Tuesday.
In the meantime, I'm updating the Development Plan to include the PPARC
proposal tasks and considering an addendum to the Design Requirements Document
that will serve as a quad design specification.
40m
I've created travelers for the spare SOS mechanical parts that need
cleaning and baking. Bob Taylor is busy until next week so early next week
I'll bring over the parts and travelers and the Gin Gin
suspension parts and travelers for clean and bake.
From: RiccardoDeSalvo
<desalvo@ligo.caltech.edu>
Alessandro
Process development for controlled etching of MoRuB
and other glassy metals using both salty water and organic solutions of
acetic and percloric acid.
This is an explosive mixture if improperly prepared, not anybody can
prepare it.
But it polishes very well, manufactured a 15 micron membrane with a
very sharp edge with 10 minutes of current. Promptly cut a finger
without even noticing.
Masking the part with nail polish, as done so far, is good in salty
water but not for the organic solution. For now using mechanical
masking, but it gives rugged edges. To do good masking we will need kaptonphotoresist,
which will be OK, but is cumbersome to use
(requires a dark room and a deep freezer for storage. We will do
if and when necessary.
Gregg
Melting along the three iron based recipes published by Lu, Liu and
Porter at
This has 3.8 GPa
quoted strength, but was processed up to 3 mm thicknesses.
Learning to use the large arc melter
to make the larger samples needed for the thicker samples.
Eric
Fiddling with the MoRuB recipe to try
to glassify it in larger thicknesses.
Different additive combinations (that worked already in other alloys) are
tried. The tests are a mixture between educated guess and magic.
May use DTA instead of X-ray to characterise,
because of the background from the additives.
Aso
Detailed design of mechanics of interferometric suspension point suspension
system.
Designed new clamp pin for the wires, put into production at G&M
together with a testing tool.
Riccardo, Ed
The old prototype of TAMA tower leaving for
For additional information about this report, contact sanders@ligo.caltech.edu