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The LIGO Executive Committee Agenda for Monday January 15, 2001 will be:
CANCELLED DUE TO HOLIDAY
no report
WBS 1.2 LIGO Operations--Administration
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
| Packages | Faxes | |
| In | 39 | 29 |
| Out | 11 | 43 |
Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS
PAYABLE HISTORY DATA.
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
A determination of the amount required for major maintenance items at the observatories is underway. This item is not included in the current operations proposal, and will be presented to the NSF at the February review at Hanford.Support (Wood)
Three day report (January 8-10):
Progress Period from 01.05 to 01.11
Accomplishments:
WBS 1.4.1.2 Project Controls (LIGO Construction)
Annual Report: I have completed a first draft of what appears to be an adequate Annual Progress Report for the LIGO Construction effort as of the end of November 2000. I have provided a pointer for reviewers to access the document and comment as necessary.
The following Change Requests have
been submitted:
| CR-000018 | WBS 1.1.4 | Curbing for Service Roads at Livingston | G. Stapfer |
| CR-000019 | WBS 1.2 | Additional Lab Equipment | D. Coyne |
| CR-000020 | WBS 1.1.4 | Staging Building and Renovations to Existing Building--Livigston | F. Asiri |
Press for the latest Contingency Needs Projection.
From: Kris Duncan <kris@ligo.caltech.edu>
The financial reports on the web provide supporting detail.
http://docuserv.ligo.caltech.edu/~fireport
http://docuserv.ligo.caltech.edu/~finance
From: Ed Jasnow <jasnow@ligo.caltech.edu>
We issued a Notice to Proceed to the Brunt Construction Company on Monday, January 8. A kickoff meeting with Brunt was held on Tuesday, January 9, at Livingston, at which the construction schedule was finalized.
The presentation of the third and final A/E candidate for the Hanford Support Building is scheduled for Wednesday, January 24, at the contractor's facility in Glendora, California.
From: irena@ligo.caltech.edu (Irena Petrac)
General Items:
--------------
(F. Raab)
We are on schedule to begin installation of 4K hardware into chambers
on
Jan 16, provided tragedy stays away for a few more days. We have made
a
conscious effort to bring new people onto tasks, so visitors will find
the
"local expertise" on many installation tasks will not be the folks
they dealt
with on the 2K installation.
Seismic Systems
---------------------
H.Radkins, G. Moreno, C.Gray, M.Guenther
X-Mid: The original HYTEC design Z-Pivot assemblies were installed
to
provide earthquake security. The ljones design is in place on
only two of
the actuation stacks due to airbearing top and bottom positions and
two are
not sufficient for the job.
Fine Actuation: Both the mid stations Fine Actuator PZTs have
been taken
off line to allow dedicated power lines to be run. The dedicated
power is
in place for these units at all four VEAs; but, the mid stations have
not
been put back on the PZTs yet. The Fine Actuators PZTs at the
X-End are
online and running on the controllers.
CAS: The coarse actuation system for BSC2 has been activated and
ready for
elevation adjustment during COC installation. BSC1 still awaits
the data
base modification for the new rack. We will test the latest 'shimming'
to
fix our Yawing problem shortly.
ASC
-----
H.Radkins, J.Meyers, G.Moreno, B.Rivera
All QPDs for the 4K optical lever receivers have been upgraded to the
10x
version.
The 2K IFO recycling mirror optical lever transmitter LASER has been
exchanged for the new model. The new LASER model has required
a different
mounting scheme with a few different arrangements dependent on the
location. All 4K levers have been modified and are ready for
installation.
Data and power cabling and connectors are ready at X-End.
The new optical lever LASER power was measured to be 2.3 to 2.5 mwatts
ISC
----
H.Radkins, C.Gray, G.Moreno
All the initial alignment monuments for COC installation have been
placed.
2k 10-W laser
-------------
D. Cook and R. Savage
- Glen Truong from Lightwave Electronics was here last week to service
the 2k PSL. After adjusting the polarizers between the NPRO and
the
amplifier, optimizing the amplifier temperature, and increasing the
NPRO
and amplifier currents, the output power was about 10.5 watts with
more
than 96% in a circular TEMoo mode. The PSL output power was thus
increased significantly to about 8.9 watts.
- Immediately after the service call we experienced two problems
unrelated to the laser head. The fuse in the power supply blew
twice.
We replaced the fuse holder with one that makes better contact with
the
fuse. The old holder showed signs of thermal damage from poor
contact.
With the new holder, the fuse has not blown. We should consider
retrofitting the supplies for the other lasers.
The other problem is that when the chiller is located in the chiller
closet at the end of the 100 ft. hoses it is unable to maintain the
laser at the optimum temperature. We have temporarily installed
the
spare chiller near the laser head. Using short hoses, it easily
maintains the laser at the optimum temperature. We are investigating
solutions to what appears to be a "low flow" problem.
4k psl
------
M. Guenther and T. Mahood
-4k PSL buildup continues. We are expecting the electronics for
the
frequency stabilization servo to arrive by early next week.
OPTICS INSTALLATION: Y-arm beamtube was opened last Thursday, and we found the beam immediately. It was close enough to the optic that it drifted onto ETM-y from time to time. When it did, we found the return at ITM-y minutes later. You can find some images in last January 4's LLO i-log. Joe Kovalik, Joe Giaime and I temporarily installed and aligned the LSC photodiode, as well as a video camera on ISCT-4. Mark Coles, Joe Kovalik and I are doing the same thing on ISCT-1. (Jonathan Kern)
CDS: Installed all LSC inputs to large optics. Reworked LSC cross-connect. Installed ASC input to MMT3. Installed EO shutter controls at ISCT1 & ISCT4. (Rus Wooley)
PEM audit: I've received some correspondence from Julien Sylvestre
during the week which I am hoping to apply to my Matlab program over the
next few weeks. Warren Johnson also showed me a matlab utility program
written by Mark Barton which may be of some use in my project. It will
probably take a couple of weeks for me to
understand the examples I have been given but I am hoping to have something
by February. Also over the next couple of weeks I intend to do a complete
audit of the
accelerometers. At this time I believe that all accelerometers are
functioning, however I have noticed that some of the cabling from the sensors
to the Endevco
amplifier in the 1X5 crate in the LVEA is flaky and may need to be
replaced. (Doug Lormand).
Facilities: The machine shop is completely moved from the staging
building, and partially operable in the pump house now. A kickoff meeting
was held with the construction contractor and subcontractors for the staging
building renovation. Work is now underway!
| Installation
& Commissioning:
Livingston |
Other Science/Engineering
Activities:
Issues/Concerns |
See also the Installation web page
We resumed the commissioning activities on the 2 km interferometer. The initial effort is on understanding the offset in the Michelson common mode length servo which had been observed by Peter and Matt in early December. We reproduced the observed offset using the power-recycled Michelson (no arm cavities). The first test was to see if the suggestion that the beam on the reflection port photodiode (used to lock this degree of freedom) was overfilling the diode, allowing it to act like the central element of a bulls-eye detector. We used a lens to focus the beam more tightly, but observed only a ~1% increase in the DC light level and essentially no change in the offset. We tried an attenuator on the reflected port beam to eliminate the possibility of some sort of spatial dependent saturation--again no change.
We next tried locking the PRM with the pickoff photodiode. This has less light and a noisier signal but locked the PRM adequately to observe that it too showed an offset, which behaved qualitatively (and even to some extent quantitatively) like the reflected port signal. In doing these measurements we noted that the offset was somewhat sensitive to misalignment of the PRM. It is possible that this might be indicative of a miscentering in one arm of the Michelson which distorts the mode internal to the PRM (due to non symmetric losses in that arm) and gives an offset. This notion is bolstered by a couple of observations of different optical gains in the two arms (one operating half-PRMs on the two arms and seeing different power buildup, and the other locking at the discriminants of the two arm cavities and seeing different P-P voltages). So we are off into alignment space.
SOS Coil driver boards are being fab'd and should be back for stuffing by 1/17. SOS Anti-Image/Dewhitening boards are due back by 1/12. A preliminary schematic for the Coil driver whitening board has been sent out for comment. Once comments have been received, a final schematic will be generated and circulated to a wider audience.
Rick Karwoski
Bench-Test Status: All frequency
stabilization boards are now fully bench-tested. (i.e. the Photo detector
module, Frequency Reference, 80 MHz VCO, Servo)
PSL Integration Test Status: Lauritsen lab is fully operational and serving as an integration platform for the Frequency Stabilization modules. Here's where we stand:
- Frequency Reference --
Tested satisfactory
- Servo -- in test
We will continue the test/burn-in process until these modules are needed at Hanford
Full up ASC now operational, including X end station; still some minor problems with reading test points, but hope to track that down and have it fixed today. LSC operational with some initial testing using GDS to excite ITMX/ITMY thru LSC system; continued testing today to verify end mass drive after we install dewhite filter boards.
I tried to measure the intensity noise filtering afforded by the new PMC but ran into some problem with the broadband photodiode that I have not sorted out yet. This measurement will take a break for a few days to allow for testing of the newly stuffed frequency servo card and components.
Work is still proceeding on the high power photodiode, hopefully a prototype circuit will be milled out by week's end. I'm still having some problems with the PSpice model but pretty soon we should be in a position to measure the transfer function of interest.
Progress on rework of the poorly coated heads: Progressive Technology shipped 20 grit blasted and polished heads to us. Orbit Industries supplied us with 2 heads that they'd acid etched to remove the coating. We will ship the rejected heads to Orbit tomorrow. Working on PAM bracket/screw gauling problem.
Mark Barton
This week I did thermal
tests of the new OSEM sample provided by Peter Fritschel. The test OSEM
was a fully complete LOS one, including the coil, the ZrN coating, the
circuit boards, the filter, the PAM screw and magnet, and the pigtail.
It was held at the standard nominal position in a bracket of the same material
and shape as on the LOS structure. The two main heat inputs are the
coil (max 200 mA through 13.3 ohms = 528 mW) and the LED (1.72 V at 50
mA = 86 mW). However the LED is on a small circuit board not well connected
to the body of the OSEM so one could easily imagine it cooking itself.
So I did measurements of the temperature both at the coil and at the casing
of the LED. With 200 mA of coil current the temperature at the coil was
47.1 C (or 22.3 above ambient), and the temperature at the LED was 40.3
(or 15.5 above ambient). This is comparable to results by Miyoki and Kawamura
for OSEMs of the old design. Adding 50 mA of LED current increased this
only 1 C at the coil but about 6 C at the LED. Thus the thermal conductivity
to ground is somewhat worse from the circuit board but not enormously so,
and the dominant source of temperature increase at both points is still
the coil current.
No report.
No report.
* Peter Fritschel wants to start studying the suspension for LIGO II.
Virginio Sannibale is going to build a suspended quadrple pendulum
based on the design document by the GEO group. This will be done in
a several weeks. Hiro will finish the interface between e2e and MSE
so that the mechanics stimulation can be fully and easily integrated
with MSE.
* Rick Savage's SURF student, Brad Zamft, is back this week at LHO
to continue his study of the PSL noise using e2e. His study covers
the noise caused by the table motion, which induces the dithering
of the beam, which could affect the demodulated signal off of the
reference cavity. Biplab and Hiro assisted him in discussiong physics
and explaining tools of e2e.
* The understanding of the seismic noise is close to the end. It looks
like the simulation is doing right, and the numerical tools to analyze
the time series and the way to use them has problems. In order to
avoid this kind of complexity in analyzing the time series, a module
has been designed as a e2e primitive which generates a PSD of a given
signal automatically applying whitening and unwhitening to generate
a correct spectrum.
* Biplab is working to understand systematically the effect of the
angular fructuation to the lock acquisition.
* Biplab and Hiro sent a note to LSC members and to the upper limit
study group leaders. This memo explains the current status of e2e,
focusing on the noise generation, and calls for the collaboration
to implement necessary modifications so that it can be used for
the data analysis.
>> Simulation code : T.DAngelis, M.Evans, H.Yamamoto
Tavio worked with Matt and Hiro toward the implementation of threads.
* A systematic study was done to understand the thread-related
overheads, delay between sending signal and awakening, and between
unlock and lock. These are necessary to design the dynamic queue.
The overhead observed is ~50 microseconds, which is much larger than
we expected, and Tavio is now trying to contact a SUN enginner to
obtain a definitive answer if what we observe is a real limitation
or if there is some workaround.
* Tavio is finishing the testbed program and tools for managing
the modules following the discussion with Matt and Hiro.
After these preparatory work is done, he will try logics to
group modules to find the optimal one to use the thread most
efficiently.
>> ALFI : E.Maros, B.Sears
* Copy&Paste of modules and a new interface for setting parameters
are the
imporvements going on.
* A new version of alfi, 4.0.24, has been release and has been installed
at CIT and LHO. This is a maitenance release, and all major reported
bugs has been fixed. Next release will have several new fetures added.
Software Systems (Blackburn)
This week has focused primarily on making the necessary changes to the
LDAS software needed in support of the MPI Mock Data Challenge. This
is in conjunction with our planned release of LDAS this Friday. A lot
of missing functionality has been added this week and a tremendous
effort to test and validate the new code has brought within a day of
formally tagging the ldas source code in the repository and installing
the new version on all LDAS system. The LDAS webpages were also cleaned
up and enhanced during this week to now present a much fuller set of
documentation and links to the complete set of LDAS APIs.The group also worked on getting all the prerequisite software installed
and configured onto the LDAS development server for the LSC's LAL and
LALwrapper packages. This are needed as part of the MDC and will now be
maintained on the LDAS file systems.Three quarters of the team from UWM participating in the MPI MDC have
already arrived at Caltech. Several meetings have been held to determine
the overall integrated status of code development and readines from both
camps. It looks like all the prerequisite source code will be available
in time for the official start of the MDC this Monday, but a significant
amount of work is needed to better structure the organization of the
actual tests and the supporting scripts. This will mostlikely not be
any problem since scripting the tests is significantly less time consuming
than getting the code to be tested functional and integrated.The dataConditionAPI received a significant amount of attention off and
apart from the LDAS release and MDC effort. A new UDT based version of
the mixer classes were implemented which has cleared the way for the
necessary changes to other classes. Another significant change to the
dataConditionAPI was the introduction of a FFTW plan cache manager which
removes old plans thereby reducing the amount of memory needed to run
the API. This significantly improved memory management issues in the
API and we are now for the first time able to run all the FFT tests
through the API without restarting it.
Hardware Systems (Anderson)
The procedures for the first major LDAS hardware purchase (> $1M) have
been initiated.The ldas-test system has had all of its Solaris filesytems (UFS) modified
to use the native Solaris logging options to improve small file performance
and largely mitigate the need for length and dangerous filesystem
recoveries (fsck) after unexpected system shutdowns.A 2 Gigabit/24 Fast Ethernet port switch has been purchased to upgrade the
ldas-test system.All 10Mbit/s Ethernet ports have been upgraded to 100Mbit/s on the 6th floor
of Millikan.----- Forwarded message from Greg Mendell -----
LDAS Activity at LHO:
1) Code has been written to produce test tables for the ldas meta data
database. The code will be used
for the upcoming database mock data challenge.2) A utility called FrSplit has been written that will split frame files
with multiple frames into
frame files with one frame each. This will be useful for splitting up
frame files retrieved from
the Caltech archive with getFrames. Some more work is needed to make the
output compatible with
the DTT.----- End of forwarded message from Greg Mendell -----
Lazzarini: We are working with Jasnow to develop a request for approval to issue the fiurst procurment of LDAS major hardware.
Philip Charlton:Data Analysis Activities
Livingston:
Working a number of network and security issues.
Working on resolving problems with one of the LDAS computers.
Larry will be contacting Bellsouth to try and get pricing information
that was
promised for the first of the year.
Hanford:
See Hanford report.
CIT:
(Barbara)
- Began changes to CostBook for contingency override and for equipment
indirect cost calculations. Expanded the indirect cost calculations
for
subcontracts.
- Made numerous updates to the LDAS web site to support the data challenge
next week.
- Fixed problems with the DCC database compact/repair process and backup
of
the LDAS equipment database.
- Helped Chargois generate spreadsheets from the equipment databases.
- Made numerous LIGO web site changes -- MOU's, LSC Roster, fellowships,
etc.
(Lisa)
-Working on getting the new modem pool up. All initial testing
is complete for
the analog modems. I am ready to start creating new users.
I've put in a
request to have an ISDN line installed but do not yet have a time frame
on that
work.
(Suresh)
-Worked with Larry on setting up a 2810 for Millikan.
-Setup a couple of new user accounts.
-Setup a couple of new computers for use by LDAS.
-Worked on cleaning up some old user accounts and moving accounts to
larger
disks.
-Assisted in the memory upgrades on the color printers.
(Sam)
Nothing to report for this week.
(Larry)
-Ordered networking equipment for LDAS test being run. Placing a new
order for
computer projectors. Checked on a number of orders that are in place
and will
have to redo a memory order.
-Ordered a couple more PC's and laptops. The PC's have arrived and
one of the
laptops has arrived and has been delivered.
-Working with Lisa on the modem pool.
-Worked with Suresh and Stuart on a network switch box installation.
-Updated the Mathematica license on the server so we are now good for
another
year. Found it easier to get information from Wolfram this go around.
-Still working out the logistics for the SDRC license renewal.
-Worked with the Livingston people on a couple of security issues.
-Just as a side note, everyone should try and change their password
if they have
not done so over the past year. Also, there are are a number of people
with a
large number of files in their directories that have not been accessed
for over
3 years, if you are keeping the files for just-in-case, they are on
backup tape.
You can also get them burned on to a CD, I am encouraging people to
delete
files/directories they have not used in some time.
--
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Proceeding with assembly and tuning of TAMA attenuation towers, all
parts are in house, except accelerometers, several minor problems but
no
major one.
Still in the details assembly and tuning phase, not yet in the global
system check phase; accumulating some delay.
Mounted IP and both Filter 0 and the standard filter. The MGAS
of the
standard filter is weak and is being remanufactured: the long lead
time
is the baking for hardening, the IP flexes, also marginally (but
acceptably) weak are being remanufactured at the same time.
(The IP zero frequency payload is 105 Kg instead of 110 Kg, could be
corrected with marginally stronger parassitic springs in the position
tuning motors, the standard filter blade lifts 1 Kg less than necessary,
could correct by machining holes in the control mass but decided to
do
it right and accept the ten day delay).
Fine tuning the IP counterweights in the new shaker.
Found play in the hexawire ball joints, re-machining ball housings.
Assembly tooling of Mini-MGAS for the mirror suspension being remade
in
house.
Accelerometer material delivered, manufacturing.
Electronics will be late, NIM crates OK, VME crates will be delivered
end of January/beginning February, the digital cards being finished,
the
analogue cards are ready but will receive NIM chassis to mount in after
January 20th. Cables will be OK but may have problems in Japan
with
Vacuum feed throughs.
Coils OK, on their way to Pasadena. Actuators working fine.
Prototype tests, working on diagonalization, measuring IP resonant
frequency versus temperature and working point drift (at 20 mHz 2 mm
drifts with our floor and the temperature variations, MINOS opens the
doors during the day and the temperature changes and come back slowly
the night). Built a small thermal and wind shield hut for the
TAMA
prototype also.
Probable delivery time Febrauary 10th.
Peter King
3.1 LIGO II PSL
Revised versions of the
PSL costings and schedule are being
worked
on. I hope to try and sort out some more details when Benno Willke
arrives
for the NSF R&D Review.
3.2 LASTI PSL
The LASTI PSL optical table
was scheduled for delivery to MIT on
01/15. Myron McInnes rang me about scheduling the delivery and
it was
decided that he would organize riggers, if possible.
3.3 40m Lab PSL
The reference cavities,
vacuum chambers and vibration isolation
stack pieces have arrived.
For additional information about this report, contact sanders@ligo.caltech.edu