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The LIGO Executive Committee Agenda for Monday July 3, 2000 will be:
CANCELLED DUE TO HOLIDAY
Special Items:
Minutes of the LSC Executive Committee meeting of June 16:
to: LSCexecutive committee
from: R. Weiss
concerning: Notes from June 16, 2000 committee meeting
1) We are planning a John A. Wheeler day at Hanford on August 14,
the Monday before the LSC meeting. This to be a celebration of
Wheeler who has multiple couplings to the Hanford site. During the
Second World War he was deeply involved in design and diagnosis of
the first production reactor at Hanford and, now, he is
responsible for many of the concepts in relativistic gravitation
which have motivated LIGO.
2) Meetings and events being planned
Workshop on r modes in neutron stars: L.Bildsten,
August 2 and 3 at Santa Barbara
Workshop on gravitational wave astrophysics: J. Centrella, in
late Oct - early November at Drexel Institute
GWDAW: December 14,15,16 in Louisiana at LIGO and LSU
Aspen to overlap the astrophysics and gravitation meetings in
February 2001.
3) Establish a writing committee for the second draft of the LSC
White Paper on Data Analysis. The committee to address the
analysis program and the long range needs for analysis.
People being asked to be on the committee:
Stuart Anderson
Al Lazzarini
Tom Nash
Keith Riles
Allen Weinstein
Alan Wiseman
One function of the committee is to take "testimony" from groups
who have asked for data analysis funds from the NSF.
4) Draft GEO/LIGO MOU on data analysis
Committee expressed caution in going forward with a bilateral
agreement with GEO without bringing the idea to GWIC. In particular,
to explore the type of bilateral (or hopefully multilateral)
agreements that would be useful to connect the data from LIGO,
GEO, VIRGO, TAMA and ACIGA as well as the neutrino, X-ray and
radio astronomy communities. A major concern was that an agreement
with GEO not prejudice an agreement with VIRGO.
The consensus of the meeting was not to present the GEO/LIGO
MOU to GWIC but rather to bring forward some talking points
(bullets) about the MOU which would become topics for discussion.
It was felt important to draw out the difficult
points in establishing agreements with the other gravitational wave
detection groups.
WBS 1.2 LIGO Operations--Administration
From: Ed Chargois <chargois_e@ligo.caltech.edu>
From: Cleveland Mak <mak_c@ligo.caltech.edu>
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA.
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
A meeting was held among Barry Barish, Donna Tomlinson, and Ed Jasnow, of the LIGO Project, with Sharon Borbon, of the Provost's office, for the purpose of discussing the processing of appointments of long-term visitors to the LIGO sites. The issue was the length of time required to secure the appointments, which were necessary to establish affiliation and, therefore, insurance coverage for the visitors. Sharon recommended that, if the visitors are receiving no reimbursement from Caltech, that they be categorized as "volunteers," with an official letter from Barry. This will establish affiliation and insurance coverage, but will not require the appointment processing by Caltech. It was also agreed that identification cards showing the term of the visit will be issued to long-term visitors.
Rita Torres
Progress Period from from 6.23 to 6.29
Accomplishments:
The following change requests have
been submitted:
| CR-990028 | WBS 1.1.3 | Beam Tube Enclosure Closeout | F. Asiri |
| CR-000005 | WBS 1.2.1 | Upgrade Pre-stabilized Laser | S. Whitcomb |
| CR-000006 | WBS 1.2.1 | Re-polish Core Optics Components | S. Whitcomb |
| CR-000007 | WBS 1.2.2 | Replacement of Optical Lever Lasers | S. Whitcomb |
| CR-000008 | WBS 1.1.4 | Cameras and Projection System at LIGO Livingston Observatory | F. Asiri |
| CR-000009 | WBS 1.1.4 | Cameras and Projection System at LIGO Hanford Observatory | F Asiri |
| CR-000010 | WBS 1.2.2 | Redesign Suspension Controllers | S. Whitcomb |
| CR-000011 | WBS 1.2.2 | VME Development System and Spares | S. Whitcomb |
| CR-000012 | WBS 1.2.2 | ASC/LSC Rework | S. Whitcomb |
Copies of these change requests have been distributed to memebers of the LIGO Change Control Board (See LIGO-M000176-00-P).
Press for the latest Contingency Needs Projection.
From: Kris Duncan <kris@ligo.caltech.edu>
FRED RAAB'S MAIL DESCRIPTION OF THE BRUSH FIRE AT HANFORD
Last night the LIGO Hanford Observatory survived an intense brush fire
without damage. The brush fire was started approximately 20 miles southwest
of LIGO by a fatal car/truck collision on Tuesday. As of Wednesday
afternoon it had jumped Highway 240 and was headed northwards, driven
by
high winds, toward the tank farms of the Hanford 200 area. At 6 pm,
with
the fire still about 10 miles west of LIGO and heading northerly I
went
home for dinner. Sometime after 7 pm I noticed the sky grow ominously
dark
over Richland and I began preparing to return to the observatory to
check
on conditions, suspecting the winds had shifted. Richard McCarthy
and I
learned through Hanford emergency personnel that the fire was racing
toward
LIGO. Richard called the lab to tell people working inside and a touring
Boy Scout group to evacuate the site. I drove in to ensure all personnel
were out and Richard followed shortly to actuate our groundwater pumps
and
valves to recharge our firewater tanks.
I found the site evacuated, except for Doug Cook, our laser safety officer,
who had just completed a walk-through of all the labs and assured me
that
all personnel and visitors were gone. Hanford fire had set up a command
post on the site, with a large number of fire engines, earth moving
equipment attempting to trench firebreaks around the 10 mile perimeter
of
LIGO, and aircraft dropping fire retardant on the most threatened
structures. By this time the winds had grown extremely strong with
a wild
fire out of control and bearing down on the observatory. For a time,
the Y
arm of LIGO served as a firebreak, but the winds eventually blew the
fire
over the arm and it raced further across the Hanford site. The fire
started
racing along the y arm past the mid and end stations. McCarthy and
I went
to the well (at the y end) to actuate the fire recharge system and
were
able to inspect those buildings at that time. The fire had burned out
all
the available fuel on the shrub-steppe surrounding these structures
without
damage to the structures. When we returned, the fire was challenging
the
corner station. I was able to inspect the site from the platform on
the
corner station roof and could see a line of fire advancing toward the
x
arm, but then a wall of smoke and high winds drove me off the roof.
The
combination of the extensive rock works we had installed surrounding
our
buildings and the firefighter's efforts prevailed as the fire burned
down
most of the grass and sage near the vertex, without placing significant
heat loads on the buildings themselves. By this time I could see fire
extending several miles to the east, about 15 miles to the west, about
10
miles south and ascending Rattlesnake Mountain. The corner station
was
about the safest haven around, so we remained there.
As the fire advanced along the Y arm burning away from the corner station,
the firefighters rapidly left our site. I later found out that this
was
when the fire jumped the Yakima River, headed for populated areas of
West
Richland and Benton City, which were under evacuation orders. We remained,
predominantly at the corner station, inspecting fire conditions with
binoculars as the fire burned along the x arm toward the end station.
The
fire failed to jump the x arm and by midnight, it had burned past the
x end
station. We were able to drive out on the x arm at this time and inspect
those buidlings, which looked OK. The winds were shifting and the fire
started to advance northerly again. I expected it to start burning
back
toward the corner station along the north side of the x arm, but I
knew our
roads would provide adequate fire breaks. We decided conditions looked
good
enough to leave the observatory by driving north to the Wye barricade
and
then to Richland along Stevens Way.
By morning the fire was mostly contained on the Hanford site, but was
burning near populated areas. The population of these areas was evacuated
to emergency shelters. According to radio reports, about 500-1000
firefighters were on the fire, which had by now burned about 150 square
miles of land. We instructed staff to remain at home while a few of
us
drove out to do an inspection under daylight conditions and to attend
to
checking systems. A power surge around midnight had taken down our
turbo
pumps (without any danger to the vacuum system) and we began a restart
procedure. We drove the full 10 mile perimeter of the buildings and
beam
tube and found no discernible damage. We met with Rex Jordan and other
officials of Hanford Fire and other DOE contractors who came out to
inspect
conditions at LIGO. The x end station was partially covered with fire
retardant compound, whose sticky surface had a layer of ash glued onto
it.
I think the worst damage we may have is if the fire retardant damages
the
underlying paint. Otto Matherny is trying to get a contractor out as
soon
as possible to wash this down. The ventilation systems prevented smoke
damage within the critical experimental areas although there is a slight
smoke smell and dust levels were exceeded in the clean areas during
the
fire. None of the critical optics were exposed. Vacuum system operation
has
been restored to normal.
The DOE contractors, especially Hanford Fire
and Hanford Patrol, were
exemplary in their efforts to keep us informed,
to let key people into the
affected areas while providing for public
safety, and most importantly to
bring tremendous resources to bear on protecting
our structures. As of
approximately 10:30 am PDT today, the state of
emergency surrounding the
LIGO area was lifted and roads into the area
were opened. Some personnel
are returning to resume installation/commissioning
work.
---------------
Some photos have been collected by Doug Cook, Richard McCarthy and Tom
Mahood and I have them posted at
http://www.ligo-wa.caltech.edu/wildfire/
We will post more photos as we collect them.
One of the noticeable oddities is the existence of small islands of
unburnt
shrub-steppe visible in the panoramas. Nightfire.jpg could have been
taken
in any direction last night.
GHS NOTE: We were very lucky. Fred
and his colleagues did a very admirable job of stewardship at the site.
The DOE earned our gratitude in this event. After the smoke clears, during
the next month, we will have a lessons-learned meeting to review this experience
and to capture insights for the next time.
OPTICS/COC INSTALLATION: Standoffs, guide rods and magnets were removed from our Beamsplitter, replaced, balanced and vacuum baked this week. BS returned to BSC-2 yesterday and we'll realign today. Used the time while the optic was in the oven to straighten the lab and shop areas. Small vacuum bake oven back online using an RGA Allen loaned us. Final COS bakeload completed; Kapton ground cables are now being baked. (Jonathan Kern)
PSL: We replaced the main output laser beam periscope with a fixed one, non-adjustable one. All the fixed mounts for the PSL are in place. There was no difficulty attaining alignment with these fixed mounts. We will replace the few adjustable mounts that are necessary next week with Optosigma ultra-stable mounts. (Joe Kovalik)
SMALL OPTICS: Three optics came out of the vacuum bake oven. We re-hung MC1 using the current suspension tower (i.e., the suspension tower that was on the HAM table before the door was opened). The new balancing angle is 0.18 mrad (the designed balancing angle of MC1 is 0 mrad, i.e., the new balancing angle is within the spec of +/-0.5 mrad). MC1 has been reinstalled on the HAM1 table. Before taking MC1 out of the HAM table, we checked the new alignment fixture using the PSL beam in HAM1 and HAM2. All fixtures work properly. (Sany Yoshida)
LLO seismic array: We are gathering price information for the vault components to finalize the design and array layout. It appears that there is some confusion at PASSCAL regarding the delivery of the seismometers as the original request from Louisiana Tech seems to have gotten misplaced. Noel Bartow of PASSCAL said that she is working to straighten out the mess, but this probably means that our seismometers will dribble in rather than all arrive July 1 as originally requested.
Community relations: Groups of 20-30 teachers from Livingston Parish public schools have been LLO for each of the three past Thursdays. This visit is part of in-service training for them. Many have expressed interest in coming for a return visit with their classes during the next academic year.
All activity reported in other categories
All activity reported in other categories
| Installation
& Commissioning:
Livingston |
Other Science/Engineering
Activities:
Issues/Concerns |
See also the Installation web page
We have moved IOT7 back to its location at HAM7 following flooring work. All light paths on the table have been aligned and the mode cleaner was locked.
ISCT7 and ISCT9 have also been moved to their nominal positions by HAM7 and HAM9. We are in the process of aligning the tables with 1.06 um beam out of the viewports, after which we will complete the field cabling on the tables.
Rana is testing/tuning the LSC photodetectors and has gotten at least one fully tuned for use on ISCT7.
###SEW
adds
The
shorted coil on the RM will need to be fixed eventually, but should not
prevent us from making significant progress bringing the LSC system up
and beginning tests of its performance. We will defer any action
to fix this problem until a later date, possibly in conjunction with 4
km installation.
Mike Zucker, Rana Adhikari,
Richard McCarthy
Diagnosed and patched a
high-frequency oscillation in the MC servo demod board. This may
have caused the wandering DC offset problem which sporadically impaired
mode cleaner operation.
Began measuring cable delays and wiring up the new (beautifully engineered!) RF reference distribution system for the three 2k modulation frequencies.
Dale Ouimette, Mohana Mageswaram,
Flavio Nocera
We shipped to Hanford the
following LSC boards this week:
Elliptical baffle staged and assembly in process.
APS/PO Telescope: Four telescopes were pre-aligned and focussed and are awaiting installation.
APS/PO Telescope Optical Train: Optical train parts are awaiting assembly.
HAM2/HAM3 Beam dumps: The HAM2/HAM3 beam dump assemblies are in process.
Orders for beam dumps and monitoring equipment for the 40m Lab PSL and LASTI laser have been ordered.
Rich Abbott
Prototype of new pockels
cell driver for the frequency servo is being constructed with the goal
of extending the useful bandwidth of the PA-85 output driver.
Beginning the ordering of new items for the 40 meter and MIT PSLs. All of the documentation is being reviewed with the goal of matching to "as builts" from the sites. New release wiring diagrams and point to point wiring lists are being prepared.
Beginning to plan the photodiode and servo for the intensity servo using the current shunt actuator that was retrofitted during my last visit to LHO. This was chosen as the next item to finish as reports from LHO by Peter F. indicate that the ISS is the next most desired item.
The ISC layer showing all ISC supplied equipment supplied to LLO has been completed and sent to Caltech to add to the integration drawing. Work has started on the LHO supplied equipment.
Computing A new version of MSC Nastran finite element analysis 4.5.1 has been recieved and installed on several pc's.
I also modified the name server to handle nodes that are connected to more than one network. Before this modification a client process would only be able to contact a given process through the network from which it registered. This change will allow monitors or servers running on the DMT machines to be contacted from either the CDS consoles or the GC network machines.
Finally I worked with LDAS to verify that the Hanford LDAS system was receiving triggers properly from the DMT.
Global Diagnostic System Signal Processor - Printed Citcuit Board design is in progress.
While working on the test cavity assemblies for the TNI, we also started
installing a new version of our photothermal experiment, with which
we
intend to measure one of the thermal noise sources predicted by Braginsky,
et al. (Phys. Lett. A 264, 1-10 (1999)). We laid out a new optical
setup,
mode matched to the test cavity, and aligned one of the two beams we
will
be using to make the measurement. We now have a nice TEM00 mode
resonating
in the cavity, and should be able to lock the system and get a preliminary
signal in the next few days.
Our test cavity is L-shaped, with a beamsplitter at the fold, and we
observed an interesting effect while aligning it. When misaligned,
the
cavity resonates in a "necklace-shaped" mode, much like a Herriott
delay
line. The effect is not really surprising, once you think about
it, but
the spot pattern is quite pretty!
No report received
Biplab visited LHO last week. He continued the work initiated at LHO.
He worked with Rick and his SURF student, Brad on PSL noises.
For those noise study of PSL, he introduced 'beam-wiggler' module.
Kept working together with Brad on the shot noise in the error signal
of the reference cavity when the mode is not matched.
He introduced E2E to Rana Adhikari and David Ottaway. Rana wants to
use it for Michelson runs.
He sorted out differences among all latest versions of PSL and
finally settled on a new version 0600.0_std_config which is not
much different from 08.0_std_config
Adlib
Hiro wrote the code to parse a text expressing equations.
The code development is almost over and modeler code
will be modified so that users can use expressions in the
settings and can embed formulas in the box file using
a new primitive.
MSE
G.Cella has committed his delivered software, including example codes
and documents,
in our CVS repository. Ed is working to modify so that MSE is fully
integrated with e2e from the code management point of view.
The problems found with the managerAPI and genericAPI last week have
been
fixed and much of the week was spent retesting the LDAS system with
these
new patches. A run of the DMT trigger ingestion into the LDAS system
early
this week was fully successful at entering all 7120 triggers into the
LDAS
tables. ILWD socket test, database table insertion tests and frame
to ILWD
translation tests are currently underway. Preliminary results are looking
great. The new tester has worked closely with the TCL staff during
these
tests as he prepares to take over these activities. We will meet later
this week to determine the readiness of the LDAS software for a new
release.
All indications are that the system is in the most reliable state ever.
There are still a few known problems, including a small memory leak
in the
frameAPI (most likely the TCL layer) which amounts to a few hundred
bytes
per gigabyte of data processed. And this is cleanly handled by the
LDAS
system managerAPI by having the frameAPI cleanly shutdown and restart
during
an idle period after a threshold memory leak has been detected.
GUILD has been getting a lot of attention this week with new functionality
being added to this user interface to support requests for frame data.
The
GUI will also display a list of channels in the frame and allow frame
data
from consecutive frames to be concatenated into a result set (frame/ilwd/xml).
The work on the wrapperAPI has moved away from the MPI code development
to
modifications to the LAL library build process to support shared objects.
The
wrapperAPI itself had a bug discovered late last week in which data
sent from
the master to the slaves usually fails. This will need to be fixed
before a
test of the wrapperAPI with the LAL code from UWM can be made. The
build of
the MPI library and the wrapperAPI will also need to be repeated with
several
configuration modifications before the test to support shared objects.
A meeting was held here at CIT to outline the user command that will
drive
the dataConditionAPI during its MDC. Two proposals were on the table.
One
with an OOP look and feel interface and the other with a scripting
language
look and feel. It was determined that the scripting language look and
feel
was adequate and easier on users and easier to implement. The code
to handle
pushing chains of commands down into the C++ layer and into threads
is near
to completion but much testing is still needed.
Also this week, the FFTW development team finally responded to our weeks
of
notices concerning huge memory usage within this package. The FFTW
teams
now agrees with us that there is a problem and has made a commitment
to have
this fixed in the next release. But there is no commitment as to when
that
release will take place.
We have a lot of work on the dataConditionAPI, mpiAPI, wrapperAPI, and
the
controlMonitorAPI still ahead of us. The debugging of the new release
of
LDAS has interfered with new development on these APIs but this is
expected
to shift in favor of new code development after the release.
Lazzarini: I met with Eric Katsavanitas several times to go over LDAS
with him as he starts
to ponder his MIT involvement.
Livingston:
We are in the process of surveying our software and hardware to
determine what is in need of upgrade.
Hanford:
Working on the network expansion and s/w upgrades.
CIT:
Samantha (still on crutches) sshed into every sun and linux box and
ran the sun
script that detectspatches.
Worked with screen savers.
Called and chatted with Gateway personal multiple times, in a vain
attempt to
get the gateway box sitting on my desk fixed. They finally concluded
that the
hard drive is bad, just as Larry said it was weeks ago.
Worked on a CD Rom that was not working quite right, I believe the
problem is fixed, but will not know until the user gets back to me.
Learned all sorts of new and cool stuff all unix related.
Burned a number of CD's.
Futzed with my desktop computer, vainly attempting to make it back
into
an even semi-stable system, but alas it is not to be. Lookinginto
different
options to keep it stable in the future.
Aquired mad crutching skills. I can now walk to work. It
takes over
fifteen minutes, but I do eventually make it:+)
Barbara reworked the CostBook database and web forms for a different
Activity
Sheet identifier.
Continued efforts on web forms for next LSC reporting period.
Purchased
2 remaining license upgrades for WebBase. Installed Office 2000
on my NT
box. The existing LSC reports database will not open in Access
2000; I'm
trying to figure out why.
Continued updating LSC web pages. Added more reports and attachments.
Set up new institutions. Updated the Council page using latest
Z attachments.
Worked with Larry changing the setup on the Primavera NT server in
attempts
to improve the performance of the unit.
Lisa performed a demo network installation of StarOffice 5.2 on graffias.
The
installation procedure went well but it still needs a round of client
testing
before it is deployed on sirius.
Replicated the samba problem that Jay was experiencing using Protel98
on Luna
(but not on sirius). This indicated that it was a problem in
either samba or
the network connection to luna. I installed version 1.9.17p3
of samba on luna.
Initial testing looks like this might firm up the connection, but we
won't be
sure until after Jay has a chance to run the connection during a
high load of traffic.
Installed ssh2 on luna. Now that this is working we need to make
sure that
F-secure is running on all the PCs and that everyone is trained on
how to use it
with Exceed.
Installed the 6/23/00 jumbo patch cluster on luna.
Began working with Rolf on how the VME crates boot from luna/kater.
Got a tutorial on monthly backups from Suresh. Sam and I are
jointly running
the monthly backups for June.
Got a tutorial on managing user accounts.
Worked with Sam on running patchdiag to determine the patch level of
all the
Solaris boxes.
Began looking into the problems Todd Etzel (Wilson house) is having
on Cheetah.
These include:
- file locking errors in his email (fixed)
- NIS+ password problems
- SSH daemon has fatal errors when it starts. This looks like
a shared library
problem. Cheetah is running OS 5.5.1. A recent set of patches
will probably
fix this, but Todd would prefer to have cheetah swapped out for a PC
instead.
He needs StarOffice.
(Suresh)Installed GPIB-SCSI-A driver in system named tiger after loading
solaris
2.5.1 in RSE Lab in Lauritsen. This would enable to display output
from spectrum
analyser by using Labview.
Put system named bala (Ultra 1) in 131.215.120 network and made a client
of
LIGO domain in Synchrotron Lab for use by SAS (Ricardo's) group.
Demonstrated how monthly backups of LIGO servers are done to Samantha
and
Lisa.
(Larry) Resolved a number of PC issues. There are a number of utilities
such as
crash guard that cause more problems than they prevent. The best things
is to
run the utilities once a week or at bootup but don't have them running
in the
background, this takes away resources the computer can use for other
programs.
Worked a number of procurement issues including the SUN order. It looks
like the
order is now with SUN and we are trying to get a partial part of the
order
expedited.
Working on some of the logistics and costs to get the Observatories
network
connections upgraded. Both Larry and Albert have been making contacts
to try and
get more information on what needs to be done.
Evaluating a problem tracking s/w pkg. that LDAS is using to see if
it would
work with the GC group.
From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>
I am requesting a quote for Suprasil 311 SV glass in the shapes of rods and "microscope slides" from Heraeus Amersil. These are for Phil Willems and Gregg Harry (Syracuse.)
Veeco has still not responded with a quote for upgrading the IR Metrology interferometer.
The first 15 cm diameter sapphire blank shipped to CSIRO, they are to measure the homogeneity of two pieces.
From: Helena Armandula <ahelena@ligo.caltech.edu>
Attended CleanTech 2000, an International Cleaning Technology Conference
and Exposition.
The most positive outcome from the Conference, was to be able to identify
and contact some vendors that could supply equipment needed for LIGO II.
As an example: an ergonomic arm to perform mirror lifting and positioning
in fixtures during substrate/mirror characterization, cleaning, and assembly.
And a customized cleaning and drying system for mirrors.
LIGO II coatings:
A preliminary talk (for costing purposes) with
Ramin from REO, reinforces the fact that REO took a "real commercial"
business path during the last year.
Each ion beam sputtering chamber, they have around
10 by now, produces $100,000.00 a day.
Research and development of coatings implies
tying a coating chamber for extended periods of time.
LIGO II optics would require coating development
to achieve uniformity on the larger substrates and to achieve lower absorption.
To accommodate the larger substrates the chamber
would require mayor re-tooling.
A ball park figure for these tasks is between
$1.5 M and $2 M. (Does not include the coating of the LIGO II mirrors).
Also, the possibility exist, that when the time
comes for the LIGO II coatings to materialize, REO could be on a different
business tempo.
We discussed different possibilities, I think
that a meeting is required to develop a plan to ensure we can procure coated
optics in time, within specs. and budget.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Welcome Susha and Paolo
Started lab removal, big mess but will get better.
Due to removal slowdown and 4th of July festivities next week no group
meeting and no weekly report.
Virginio will run group meeting of July 12th and write status report.
Hareem, Paolo, Riccardo
Started oil bearing, shortly followed by recycling pump breakdown,
despite specs the pump lining was not oil compatible, an oil bath
ensued. Tested second set of oil pump, this one was not compatible
with
the bubbles in the recovery oil. Finally tested pumps from C&H
surplus
store; these pumps seem to work, The oil bearing and IP testing
facility should be finally up and running by the 4th of July.
Hareem, Akiteru
Measured thermal drift of GASF and MGASF at 230 mHz. This time
it is a
stable 1 mm/degree. Proven that the Akiteru-Tatsuo measurement
was
transient dominated.
Start designing a simple bi-metal spring compensator to passively null
the filter vertical load point thermal sensitivity.
Hareem
Changed load disk in GASF, obtained 170 mHz, going to extend Quality
factor and thermal stability measurements in this frequency range.
Hareem, Virginio
Writing GASF paper.
Brett
Component acquisition for stepper motor controllers, e.t.a. this week.
Finished and tested hand wired driver boards, will make PCB version
in
background priority with Flavio’s assistance.
James
Learning Transfer function measurement techniques.
Populated an LVDT board, built some coils.
Erik.
Reported on suspension fiber TNI feasibility and on related discussions
with Vladimir.
Susha
Started working/learning MSE
Studying static profile of blades in MGASF plus dynamic range behaviour
around w.p..
Chenyang
Starting up Marconi AC electrostatic actuator demonstrator.
Akiteru, Kenji
Confirmed 50 dB performance of 1.5 mm MGASF; The 70 dB were faked by
a
miscalibration in connecting two different frequency ranges.
Result now
qualitatively agrees with expectation that less stressed blades produce
worse attenuation plateau.
Akiteru
TAMA suspension design.
Alessandro
Advancing in accelerometer circuit construction.
Accelerometer item one construction delayed by lack of special end
mills.
Present accelerometer item one e.t.a. is Monday or Tuesday.
Soy
LVDT driver work.
Tooling up a stand for acoustic emission measurements in stressed
blades.
Virginio, Riccardo
Continuing heavy duty supervision work.
Virginio
Re-diagonalization of Ip controls for new load and new LVDT
positionings. Wrapping up for removal of IP.
Remaining some accelerometer testing with Akiteru before removal.
Virginio, Akiteru
IP long term drift measurement. Found no correlation with temperature.
Only floor tilting (within 5 micro rad/day) observed occasional sudden
shifts of tens of nano-rads.
Tilting compatible to known building stability.
Gilberto
LVDT calibrations for creep measurement. 4 made, found some glitch,
probably in measurement technique.
Lisa
Running thermal stability measurement. Found problems in including
LVDTs
in the DAQ, may be simpler to change existing card.
Szabi
Remotely assisting in solving DAQ problems.
Paolo
Starting compilation of transfer function, sensitivities and seismic
activities.
Data acquisition status report (from Virginio).
Three PC computers in the lab.
C1 reserved for creep with K. DAQ
C2 running IP controls and thermal measurements with DSP and NI DAQ
C3 general purpose use
Receiving a work station from Suresh.
Need to run thermal stability stand, TAMA SAS stand and acoustic
emission stand.
Filter transfer functions generally run on spectrum analyser.
Need at least another PC and two DAQ cards.
Waiting for the return of the second broken DSP card (shipped today).
We will need another one for the lab plus need to order all the TAMA
ones.
Waiting for a second DSP crate, late on e.t.a..
For those who enquired, the report order is given by the sitting
position of the people coming to the meeting, starting clockwise from
my
chair.
For additional information about this report, contact sanders@ligo.caltech.edu