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The LIGO Executive Committee Agenda for Monday October 29, 2001 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items:
Most of you are aware that Jordan Camp has elected to take a position with Goddard Space Flight CEnter in their gravitational research program. Although Jordan remains in our LIGO Scientific Collaboration and will continue to be associated with LIGO, most of his LIGO Lab responsibilities need to be re-assigned to others within the laboratory. These responsibilities, as well as a clarification of LIGO Laboratory personnel roles within the optics development area, are defined below.
1) Jordan Camp continues to lead the technical oversight committee for the Australian Gingin high-power test facility. This is really an LSC assignment but I mention it as one place where Jordan will continue to provide his expertise.
2) The Cognizant Scientist for the LIGO Laboratory optics activities is Bill Kells.
3) Sapphire Development:
In the interest of protecting proprietary information from our two contractors for sapphire materials development, we must take care to avoid inappropriate transfer of information between the two contractors. With this in mind, we have separate Technical Managers for each contractor. Thus:
a)
Technical oversight & management for sapphire development at SIOM is
provided by Ren-Yuan Zhu.
b)
Bill Kells will provide science direction, from the LIGO Laboratory, for
the sapphire development program at SIOM.
c)
Technical oversight & management of the sapphire development at Crystal
Systems will be done by GariLynn Billingsley.
d)
Peter Fritschel will provide science support, from the LIGO Laboratory,
for the sapphire development program at Crystal Systems.
e) Bulk absorption measurements, in the materials research phase, will continue to be done by Alex Alexandrovski, Martin Fejer et. al. at Stanford. We are very lucky that they are continuing to provide this very skilled and expert measurement and analysis capability. The LIGO Lab liaison for this work is Peter Fritschel.
4) Coating Development:
a)
Technical oversight & management for coating development at SMA-Lyon,
MLD and REO is provided by Helena Armandula.
b)
The Cognizant Scientist for the coating efforts is Greg Harry.
c)
Note the item on surface absorption in coatings below.
5) Polishing & Inhomogeneity compensation:
Technical
oversight & management by GariLynn Billingsley. This currently involves
contracts with Goodrich and CSIRO.
6) Metrologyand other optical characterization:
a)
Phase map measurement will continue to be GariLynn Billingsley's responsibility.
b)
The transmission/reflection scanning and birefringence testing will be
performed by Lee Cardenas and Bill Kells. (Note that this apparatus may
be extended to enable surface absorption measurement as well.)
c)
Surface absorption measurement, in the coatings research phase, will be
done by Alex Alexandrovski, Martin Fejer et. al. at Stanford. We are also
grateful for this collaborative effort. The LIGO Lab liaison for this work
is Bill Kells.
7) Contamination cavity/materials qualification: Lee Cardenas and Bill Kells.
8) Lasers: Peter KIng will be responsible for this effort and will serve as the manager of all of our laser R&D and production contracts.
One consequence of the above separation of responsibilities is that GariLynn Billingsley is the single Technical Manager for all interactions with Crystal Systems, CSIRO, Goodrich and Veeco. Likewise, Helena Armandula is the single Technical Manager for all interactions with SMA, MLD and REO. All LIGO personnel should work through these individuals when they need the services of these vendors. If you have any questions regarding these assignments, please contact myself or Dennis Coyne.
II. From Phil: Policy on Charges to the Cost Accounts of Others
General:
Charges sometimes go through the LIGO Procurement System where the individual making the commitment uses an account number for which he or she is not responsible. The intent of the following policy is to minimize mischarges as well as to ensure that the individual responsible for an account is informed regarding all charges against that account.
Policy:
It is LIGO Policy that when any procurement is made against an account number, the individual responsible for that account number must be notified of the commitment. Project Controls is responsible for notifying the account manager of all purchase commitments against his or her account. This is accomplished via a copy of the purchase request (PR) forwarded to the responsible manager.
Clearly this will be implemented when, and only
when, the account manager responsible for the account has not explicitly
requested or approved the procurement.
"The big news comes in this message from Nergis and Rana: "
No report.
WBS 1.2 LIGO Operations--Administration
There was a teleconference on Thursday, October 25. Items discussed included:
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
ACCOMPLISHMENTS
ACTIVITY
| Packages | Faxes | |
| In | 24 | 34 |
| Out | 8 | 36 |
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)
SUPPORT
PLEASE NOTE: This report only covers four (4) working days.
Progress Period from 10.18 to 10.25
Accomplishments:
WBS 1.4.1.2 Project Controls (LIGO Construction)
The end-of-August Quarterly Progress Report has been sent to the NSF. We were expecting DCAA to initiate an audit of our revised proposal for LIGO Operations this week, but it was cancelled or, at least, postponed.
There are no change requests currently in the queue.
Press for the latest Contingency Needs Projection.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
From: Ed Jasnow <jasnow@ligo.caltech.edu>
Finalized travel arrangements for the Hanford Safety Audit (November 8th) team members.
Conducted computer fire suppression system discussions and walk through of room 215, Synchrotron with representatives of CalProtection. Turns out that this is also the company which provides the fire protection support services for Caltech. They will submit a bid by early next week. A second vender is planned for a visit next week. A major challenge (cost) to installing a suitable O2 depletion system in room 215 will be the cost/difficulty in making the room "air tight". An alternative would be to build a separate room within 215 surrounding the computers which could be easily sealed off if the fire suppression system were activated.
Arrangements have been made for getting cost estimates next week for
increasing the raised floor area in room 215.
General Items:
--------------
(F. Raab)
Commissioning activities (reported elsewhere) are the main activity
this week, with efforts continuing to involve operators more as hardware
set-up needs decrease. Attendance of operators at commissioning meetings
is now the default. We experienced a day of 50+ mph
winds this week that effectively shut down most commissioning activities.
Even the transmitted beam on the PSL reference cavities were visibly "hopping"
around in the camera views and gusting winds often threw the mode cleaners
out of lock. We may want to consider, for the future, steps to "harden"
the WA interferometers against such interruptions. I would not fancy explaining
to NSF why bad weather caused us to miss a nearby supernova.
The Livingston 4K interferometer was able to achieve and hold lock in a power recycled configuration during night time operation Wednesday evening. Multiple lock periods of around 10 minutes have been demonstrated. The high current LOS controllers at the end stations were used for this work. High current controllers for the ITM's have also been installed but were not utilized for these initial studies. We will now see how we can extend the capabilities of the interferometer to lock during the day by using these additional controllers. We are also modifying the controller boards for the BS and RM so that we will have the same control authority over them. We still have a lot to learn about the interferometer, especially some features of the side band power and asymmetry in the PRM that are not yet understood, but this achievement is an important milestone in the commissioning effort here. Congratulations to everyone for their contributions towards this achievement.
From another message from Mark:
From: Mark Coles <coles@ligo-la.caltech.edu>
Subject: Lock of the LLO 4K Interferometer
At approximately 9 pm Thursday evening, the LLO 4K interferometer began locking in a power recycled state for durations of several minutes of continuous locked operation! The locks were interspersed with brief unlocked periods and then the interferometer would quickly reacquire. Power buildups in the arms exceed 1000.
The interferometer is operating with the "zipped up" ETM controllers. (Zippy ITM controllers, also installed, have not yet been utilized. Wave front sensing for LOS control has also not yet been implemented.) Ground seismicity is around 20 counts at 20 Hz in the vertical direction at the Y end station (vs 200 during the day).
Congratulations to everyone for their help achieving
this important milestone.
Optics and Installation: Laser Safety Interlock hardware installation
is completed. The new surveillance cameras have been installed, and about
half are functioning as of today. Balance should be online by week's end.
They we begin programming the system logic. PSL table legs were removed,
and the original leveling screws have been replaced by HD machine wedges.
Completing modification of PSL safety enclosure to accommodate new acoustic
enclosure. Manufacturer of PSL acoustic enclosure promises engineering
drawings early next week. Made swept sine measurements of the new PSL periscope,
driven acoustically. See i-log. (Jonathan Kern)
GC: Spoke with Computer Associates about some software that may
make GC more reliable and ease some of the time requirements of Tom and
I.
Trying to track down a Nimda infection at LLO. A couple files are getting
copied to shared directories on a windows machine that are infected.
LDAS: Gathered all of the information for the QFS licenses and
sending the information on. I have prepared a document on installing BigBrother
in the ldasadm home directory. I have it installed in this manner on ldas-la.
I am using ldas-sw as the machine to create the documentation from. This
machine has not had a local install of bigbrother so it is easier to use
for the documentation. Shannon Roddy
|
Commissioning:
|
|
Mode cleaner leveling continued. The situation
for the bounce modes in the 2 km interferometer has proven substantially
more complex than for the two 4 km interferometers. Each of those
interferometers showed peaks clearly associated with the bounce modes of
the individual MC optics, though in a couple of cases the MC bounce mode
was coupled to the bounce mode of another optic and clear splitting was
observed. Here the bounce modes of the optics on HAM7 seem to all
be coupled. The MC_F signal in the 16 Hz region shows at least seven
peaks (one for each optic on HAM 7 plus MC2) and they don't seem to be
associated with single optics but rather with multiple optics, typically
three or more.Attempts to realign the MC to bring down one peak typically
cause one or two of the others to increase. In the end we have minimized
the one which is farthest in frequency from the others and attempted to
notch the remaining ones. The rms contribution from the 16 Hz peak
is now comparable to that of the 12 Hz stack mode, so we are calling a
temporary halt to the levelling and starting to bring the 2 km interferometer
back.
Betsy and Ski remeasured the noise in the coil drivers for the 2 km LOS controllers, to see the effects of the changes that were made two weeks ago. Details are in the elog, but the main result is that in our normal operating configuration (bias and dampings on), the noise at 100 Hz has dropped by more than a factor of 100.
The process of hook-up and checkout for the electronics
continues as we get ready for locking the full interferometer. A
photodiode has been installed, aligned and cabled for the SPOB signal,
as well as the normal BS pickoff rf signals. The various whitening
gains and filters have been set. QPD signals are now present on both
arms and being read by the software to produce the arm cavity transmitted
light signals. Rf phase setting is in progress. We are revisiting
some of these items after replacing a faulty EOM; the originally installed
EOM had an open connection internally and produced very little modulation.
(as it turns out, all of the locking done to date was done using the little
bit of capacitive coupling that comes from the pockells cell housing!)
The power recycling cavity has been locked and the
power levels look normal. A video camera has been aligned to look
at the recycling cavity beam.
Optical levers have been modified to get pitch and
yaw readouts going the correct direction
Careful measurements of the fss electronics are being made to identify where the phase shifts that limit the gain are coming from.
week's work is that the Livingston
interferometer is now power-recycled
with typical lock stretches
of 2 to 3 minutes and the longest of 9 minutes.
With good alignment we typically
see power buildups of 1000, but have seen
some buildups in excess
of 1400. The power fluctuations are typically 50
to 80%.
To get to this point a lot of
time was spent measuring the lock acquisition
parameters and debugging our
often inconsistent results. The big break on
that came when we found a saturation
problem in the LSC whitening filters
(by design they are supposed
to have high frequency gain, which we did not
account for correctly). Other
things we had to carefully set up were the
ISC table alignments, and, of
course, alignment of the full interferometer.
Some mysteries persist in the
optical behavior of the RF sidebands; a lot
of effort was put into measuring
the RF sideband components of the light
using scanning Fabry-Perots
at the reflection and antisymmetric ports,
with confounding results.
--------------------------------------------------------------------------
The wavefront sensor at the
antisymmetric port is now working - a
significant accomplishment
as it shows the way to bringing the other
wavefront sensors into operation.
There is a strong hunch that the
wavefront sensors (with some
increase in servo bandwidth) will be needed
to allow operation of the full
interferometer during the day.
Attempts are being made to lock
the power recycled Michelson and a single
cavity during the day time.
This is stage 3 of the acquisition process and
must go smoothly if there is
to be any hope of locking the full
interferometer during the day.
The higher current coil controllers have
now been installed in the ITM
as well as the ETM. Work is underway to
ready these controllers for
the recycling mirror and the beam splitter.
Spectra are being taken to understand fully the 200
Hz mode of the new
periscope on the laser table.
- We have completed the testing of the pentek ADCs
here at CIT and have found
that a few have bad channels. These bad channels were
previously suspected to be
bad at LHO and were sent to CIT for confirmation.
The modules that have good
channels are very consistent. The input referred noise
is ~15uV/rtHz with a
small hump around 4KHz. This is consistent with the
measurements we made on the
original units in 1997.
- We are in the process of developing a circuit that
will allow us to use a
delayed 16384 sample clock for the DAC output. This
will allow us to set the
total delay through the system to a minimum without
turning up the sample clock
to rates where output noise is a problem.
- The code to test input and output noise on the penteks
while they are in place
at the sites is ready. We can use it to test each
channel of each pentek in-situ
without disassembling the system.
- I am in the process of collecting the proposed revisions
for the SOS Coil
Driver module. Once the list is collected I will distribute
it for approval and
rev the boards. Anyone with changes should email them
to Jay.
Drafted test & RF compensation procedure for LSC
RF photodetectors.
Preparing for next week's visit by Nathan Hindman
to begin his Jedi
Training, so that he can do this testing at Hanford
I am back on validating Melody: perturbing the geometry
of the two ITM mirrors
one sideband is an order of magnitude larger than
the other while the results
obtained by the FFT-code for the same distortions
give an imbalance of 10%. If
the common and differential lengths are changed by
offsets introduced by hand,
both the dark and bright port drop in power and no
consistency with the output
of the FFT-code is achieved. I have been changing
the positions of the mirrors
and the beamsplitter without finding a better convergence
toward the FFT-code
results. In the meantime I am developping a simple
model that explains how the
imbalance between the sidebands is generated, when
the Schnupp asymmetry and a
geometrical asymmetry that makes the two branches different are both included.
EO Shutter Controller
got the coating wrong on the pre-modecleaner mirrors.
The substrates were
sent out on Monday.
40m Lab PSL: The 21.5 MHz photodetector was replaced
with a modified Thorlabs
PDA-55 photodetector. The laser frequency was
swept through the reference
cavity resonance and the frequency servo mixer monitor
signal looked clean.
Apart from the low RF output from the 21.5 MHz reference
card, the other
signals appeared okay. The RF output was about
a third of what it should
be. The distorted discriminator signal reported
last week was due to the
RFPD not working properly. Heater jackets for the reference cavity vacuum chamber have been ordered.
Sander Liu
In the process of finalizing the acceptance test procedure
for the FSS servo board
Rick Karwoski
I have set the levels, re-tested and burned in both Frequency Reference
boards for the LASTI installation. Both units were shipped overnite yesterday,
complete with the new board Travelers. Test results are included
in the traveler package. I have completed test procedures for both Freq
Ref boards, the PMC servo and the VCO. The Freq Ref ATPs have been
submitted to DCC. DCNs for all PSL boards have been completed and submitted
to DCC.
ISS Electronics: A second prototype unit has been completed and is undergoing testing.
Picking up where Jordan left-off last at the sub-basement
in bridge.
reviving the scatterometer.
I checked and turned on the NPRO S/N 190 , made a
fast alignment check.
I have turned on the vacuum pump and allow the chamber
to be cleaned. (pressure gauge and rga needed)
Lab needs put things in order, cleaning, fixing cable
rack, tool box needed, attach and secure many of the power strips.
All of these are ongoing.
One periscope was received at LHO. The second one is being shipped to LHO on10/25. The next unit for LATI is in fabrication.
Continued to add the dtt code to the new gds archive
and compile it under
linux; this week the lidax (LIGO data access) tool
was moved.
Some of the dtt crashed people experienced can probably
be attributed
to insufficient memory. Ordered and installed an additional
512kB of
memory on most of the control room machines. In the
process noticed that
some of the machines out in the LVEA have 64MB of
RAM only!
Ordered some second hand (i.e., cheap) ATM equipment
to move the
control room machines to 100bT (they are current at
10bT). Some
preliminary tests with the new frame size indicates
rates well above 1MB/s
for NDS access. Also ordered two additonal 10bT expansion
modules for
the LVEA, since we are running out of ports there.
preparing for the Burst analysis group 'PEM Deep Mine' study.
This week we closed the vacuum chamber and pumped down. The pressure
is
now in the mid 1e-6 torr range, and we have begun measuring transfer
functions in preparation for attempting lock.
LASTI (Bayer, Fritschel, Harry, MacInnis, Mason, Miller, Mittleman,
Ottaway, Phinney, Rollins, Shoemaker, Zucker)
=======================================================================
INFRASTRUCTURE:
The modifications to the cartridge clean room has been completed. The
modifications made were to make the leg height adjustable and provide
openings in the top to allow the stack masses to be lifted with a crane
and dropped into place.
A meeting was held with Harry Overmeier and Gary Traylor from Livingston
in preparation for their trip to MIT to assist in the assembly of the
BSC stack on 11/5 thru 11/9.
HYDRAULIC ACTUATORS:
A schedule for the hydraulic isolators has been completed by Ken Mason
and Brian Lantz and handed out to members of the seismic isolation
team.
A finite element analysis of the springs designed for the hydraulic
isolators revealed stress concentations on the ID of the spring. Design
refinements are being done to reduce this excess stress.
The prototype pump stand is nearing completion in the shop. Josh machined
the flow resistors and plumbing adapters and finished the motor
electrical panel.
CDS/DAQ/GDS:
Our GDS RAID disk woes will be temporarily resolved by swapping in a
spare unused "old style" unit from LHO (thanks Dave!). The
manufacturer's firmware revision which disabled Sun support on all
the
newer units is still being worked.
NOISE BUDGET:
Gregg H. went through the noise model and checked it against all the
factor-of-two errors that have been found in bench recently.
Everything was
fine, except there was an extraneous two on thermoelastic damping that
was
removed. So the internal mode thermal noise estimate for sapphire
mirrors on
the graphs shown at our LSC review were a factor of root 2 too high.
PSL:
This week the commisioning of the PSL has been delayed while we wait
for
delivery of electronics and the enclosure. The electronics have arrived
so
commisioning of the PSL will become a major focus for next week.
Preparations continue for the installation of the SOS optics in HAM
13 in
the near future.
Simulation and Modeling (Bhawal)
E2E for LIGO-I meeting
----------------------
Luca gave a talk on his recent progress in characterization and modeling
of LSC. There was discussion on Stan's questions (from last week's
e2e
Physics meeting) and how and who to follow those up. Details are available
from http://www.ligo.caltech.edu/~e2e
Modal Model
-----------
(Hiro) In process of summarizing the analytic calculation of fields
in a FP cavity when
curvature mismatch and tilt exist, up to 4th order, and adding
them to
the e2e ModalModel document (T990081). This note explicitly discusses
how a few
of the null tests that are used actually work, and can may used
for the validation of the e2e code.
(Biplab) Did a null test for the effect of waist size mismatch of the
input
light with that of the eigenmode of a cavity. A back-of-the-envelope
calculation shows that the effect should be same as sending a beam
of matched waist-size
but of different wavelength so that the Rayleigh range remains
to be same
(Note that the round trip phase should be appropriately adjusted
to get the resonance condition to be the same for both cases). E2E passed
this test nicely.
Doing other mismatch studies.
Mechanical Simulation
----------------------
(Andrea) Written a document (T010126) which outlines a proposal to
integrate
existing mechanics simulation models in e2e. This has been prepared
to provide
a starting point for the discussion in a future meeting on this
topic. This
document will soon (in a week) be submitted to DCC and circulated.
(Virginio) Rewriting the code for the LIGO2 suspension simulation because
of the
necessity to have a better code maintenance ( No more C/C++ mixed
code).
Some very minor bugs need to be fixed.
Implementing just one leg of the HAM stack to evaluate the feasibility
of using
MSE to simulate the entire stack. The aim of this simulation
is to have a tool
able to estimate the effects of short-circuiting one of the attenuation
stages.
The expected benefit is a reduction of the rms displacement noise.
This
modification can improve the stability of the Livingston mode
cleaner. The
seismic attenuation should not be endangered because in this
case the HAM stacks have ample performance margin.
Beam object still under debugging.
Next week I'll have some freshman students playing with an inverted
pendulum
prototype I designed (60cm long) for the freshman lab course.
see http://m8.ligo.caltech.edu/Phy003 for more details.
PSD Estimator
-------------
(Andrea) still working on the modifications to the E2E spectral estimation
routines to implement automagic whitening and de-whitening.
Code maintenance and improvement
--------------------------------
Biplab tested the parallelized runs with ordinary runs and found
differences.
Hiro fixed a bug in the simulation engine when threads are used
for
parallelization. After that results matched with each other.
(Hiro) Fairly extensive modification of the simulation engine is completed
and all changes will be committed to cvs very soon. This will
be the base
of the next release of e2e.
CVS
----
(Ed Maros) Created CVS account for Andrea Vicere.
Alfi
----
(Bruce) Continuing work on Alfi 5 port and connection widgets.
(Melody)
- Worked on event processings for the member nodes (displaying internal
and
external view, popup menus, etc)
- Worked on the alfi5 schedule and submitted it to Hiro.
LIGO Data Analysis System
Software Systems (Blackburn)
The long awaited new release of LDAS will happen later today.
A final freeze for source code and scripts took place earlier
and only two more documentation changes will be made before
the LDAS CVS repository is tagged for release 0.0.21. New in
this release are the following:
a) the ability to generate a quality channel base on an SQL
query's result using DMT metadata.
b) the ability to send N-tuples of simple data sets in the
form of flat tables (N - sequences) to the search codes.
c) the ability to extract spectra from the database for use
in search codes.
d) the ability to enable debugging modes in the wrapperAPI
without recompiling through a resource file.
e) a DB2-ready metaDataAPI from the /ldas rsync site.
f) a much much more stable multi-parallel job handling
environment through significant changes to the mpiAPI.
g) a release of LDAS which is "nearly" compatible with the
new libtool standard adopted for lal and lalwrapper code
development. (one issue reported for the framecpp and
a
patch is needed to the libtool distribution).
h) first draft of documentation for building a full complement
of ldas on a single computer (not distributed across hardware).
i) supports for new one-sided power spectral density standards
in the dataConditionAPI.
j) support for returning data products from the dataCondtionAPI
to the users in the form of processed frames.
k) better handling of frame file directory caches.
This is a significant amount of new functionality and we have
worked very hard to test it all and get the bugs out. Of course
there are still some bugs and the problem tracking captures these
however, we do feel that this is a release we can be proud of
even if it was significantly delayed in its delivery. This new
version should be available at all sites tomorrow.
A.L. NOTE: Kent and the LDAS team should be very proud of their accomplishment.
The full benefit of the investment in the infrastructure is starting to
manifest itself by the way in which substantially new functionality can
now be added as the need is identified and requirement is defined.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
(Al Wilson)
(Stuart Anderson)
The order for the next set of 8 LDAS servers was placed with Sun with
the
exceptional help of Gina Salone.
A semi-permanent floor space allocation was obtained in the CACR machine
room for 3 racks of LDAS equipment. The first installation was to move
1 rack of disk storage from the ldas-test system across campus to operate
as the cache for the LIGO archive system.
Started testing RedHat 7.2 and a recent kernel patch to RedHat 7.1 to
determine the next upgrade path for LDAS Linux machines.
Added additional software mirroring functionality (rsync) via a secure
web interface.
MIT
---
(Keith Bayer)
ordered cables/converters from NTI
patched Solaris machines
installed Greg's backup script (w/o fssnap) into cron
Livingston
----------
(Shannon Roddy)
Gathered all of the information for the QFS licenses and sending
the information on. I have prepared a document on installing
BigBrother
in the ldasadm home directory. I have it installed in this manner
on
ldas-la. I am using ldas-sw as the machine to create the documentation
from. This machine has not had a local install of bigbrother
so it is
easier to use for the documentation.
Hanford
-------
(Greg Mendell)
1) Worked with Stuart Anderson, Dan Kozak, Shannon Roddy, Dave Barker,
and Sun to obtain QFS licenses and install QFS. Currently working
on
configuring QFS on the LDAS dataserver and CDS fb3 hosts.
2) Completed changes to backup script to turn off xntpd while running
fssnap on Solaris hosts. Sent script to ldas_admin_all.
3) Logged a memory problem on metaserver with Sun. Sun will replace
the
suspect CPU if the problem occurs again.
4) A leak in the valve that brings water to the Liebert AC unit's
humidifier was shutoff by someone, and fixed by Otto. This cause the
Liebert unit to shut down its humidifier when the bulb associated with
the humidifier became too hot. The LCD display does not show
this (it
still showed the humidifier was running), even though the humidity
dropped from 43% to 21%. However, a reset button underneath the water
pan must be pushed to restart the humidifier when this happens. The
unit
is now working and the humidity is now back up to normal and within
Sun's specifications for data centers.
General Computing (Wallace)
MIT:
(Keith)
-MIT PPP dial in service now operational.
-Ordered laptop for new postdoc.
-Investigating wireless options for use in building next door.
Livingston:
(Shannon)
-Spoke with Computer Associates about some software that may make GC
more reliable and ease some of the time requirements of Tom and I.
Trying to track down a Nimda infection at LLO. A couple files
are
getting copied to shared directories on a windows machine that are
infected.
Hanford:
(Christine)
- Investigating a problem with slow disk access when running Framemaker,
compilers, and Matlab. Appears to be related to having the application
software and files on separate computers and then accessing each of
those computers from a third computer.
- Setup a new travel laptop.
- Investigating using encrypted passwords with Samba.
CIT:
(Mike)
-Daily administration on the NTSRV's, keeping up with system logs and
keeping up with security; created an additional website for Veronica
on the
Amaldi server.
-Hard Drive failure on the Steve Vass PC, replaced his hard drive then
reload PC
with all General Computing software.
-Jay's laptop is broadcasting what looks like the Red Worm virus that
was
affecting the Caltech community. LIGO was not affected by this virus,
which
means that our users are keeping their virus software updated.
I downloaded red-worm utility to clean this from user laptop and installed
service pack 2 and critical updates.
Users on the LIGO project must install the critical updates then install
service pack 2; this well prevent being affected by the red-worm virus
or
any other security problems.
-Installed Solid Works for multiple users that included,
Ken Mailand, Janeen Romie 'having a problem with her SUNPC card running
solid
works', we are still looking into this problem.
Dennis Coyne's and Calum Torrie also have the s/w installed.
-Problems with office 2000 causing Mike Smith's computer to freeze
up on him, I
uninstalled office and system works that was running on his computer
also
then reinstalled office and things seem to be okay for now.
-Instructed a user on how to run exceed to launch XMGR for him to plot.
-This week I had a lot of onsite and phone support to take care of.
This is a good thing, users are letting me know right away when they
are
having software and hardware problems with their PC's before matters
get worse.
(Lisa)
-Rebuilt canopus (internal ftp server) with solaris 8. Helped
users set up
their ssh connections to canopus after the rebuild.
-Resolved an ssh1 problem with sargas.
-Chased down a laptop that had code red worm running. Mike did the
disinfection.
-Built an ultra30 as the frame broadcaster for the 40meter martian
network.
-Troubleshooting license issues with solid works on sunpci. Once
I got past
the licensing problem, we discovered a video incompatibility.
I'm currently
trying to find a fix for that.
-Looking into wireless security issues.
-Updated more pcard users for travel.
-Added a couple of new FAQs to the GC web pages.
-Was really grateful that Larry came back from SANS.
(Bruce S.)
Gnats maintenance:
(2.0 days)
- Ongoing attempt to set up gnats for the detector hardware group.
(Larry)
-Spent time working with Veronica trying to get her up to speed on
things.
There is quite a learning curve and it will be some time before she
learns
all of the logistical procedures one has to go through on the WEB servers.
-Worked a number of procurement issues. Mainly updating service contracts.
-Returned from the SANS conference. A lot of things are happening in
the
computer security world. There are number of things we will have to
start
investigating in more detail. Two of them being; the new laws related
to
computer usage and security, and home usage. We are working on some
steps
for users to apply when using their home computer and that will be
on-line
the first of next week.
-Worked on a couple of servers and network hardware.
-Worked a couple of virus issues. Just a reminder that everyone using
MS should keep their virus-scan s/w up to date.
(Lazzarini)
- I convened a meeting among General Computing, LDAS, and CDS this
week to discuss the network topology we wish to implement across the laboratory
sites (with the exception of MIT). The discussion focussed on how to create
secure firewall protection at several levels without impeding people's
work. We have a rough draft in mind That separates out www services from
user directory services from LDAS, from CDS, and from GDS in a way that
will allow users who need to access these LIGO subnets to do so while
providing the benefits of programmable protection via a firewall.
From: Helena Armandula <ahelena@ligo.caltech.edu>
Q measurements
Two more thin substrates have been measured at Syracuse.
There is a new coating schedule that will be discussed with Mackowski.
After his review, it will be implemented.
AdvLIGO PSL
Peter King
I received information from Shally Seraf about the current state of
the 10-W laser (SN #104) and contacted Lightwave about an upgrade.
I have
not heard from them as yet.
AdvLIGO SUS
Calum Torrie
I spoke with about 10 machine shops in the Los Angeles area and a few
in northern California about the possibility of doing work for us. I am
waiting to receive brochures and a list of there capabilities.
The design for the mode cleaner suspension is very close to the design
for the signal recycling design in GEO 600. I have been having a lot of
contact with both Both Mike Plissi and Harald Luck in GEO group and have
obtained several engineering drawings and sketches of these suspensions.
This is not a complete set that could be sent to a vendor immediately,
there are several reasons for this including the fact that the signal recycling
suspension has not yet been installed in GEO. My priority is to work on
these in order to obtain a complete set, in English, for our prototype.
Started discussions with Eoin Ellife in Glasgow to model the curvature
of the blades we will use in the first prototype.
Mark Barton
This week I got the wire-bending parts of my model mostly debugged,
in the sense of producing plausible results that pass assorted
consistency checks. Unfortunately the fix for one bug that I found
cause
the recalculation time to go up significantly (about an hour for
producing the matrix elastic constants). However that shouldn't be
a
showstopper because the wire-bending terms make little difference to
the
normal mode shapes and frequencies, so they can be left out of most
runs
and only included to check the thermal noise. And there are several
points where more optimization could probably be done if necessary.
I
also reverse-engineered the Bench program to extract the parameters
it
uses and the thermal noise estimates it produces and am in the process
of
doing detailed comparisons.
Q measurements
Helena Armandula
Two more thin substrates have been measured at Syracuse.
There is a new coating schedule that will be discussed with Mackowski.
After his review, it will be implemented.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Charlotte
Study of metal diving boards samples.
Charlotte, Riccardo
Update on creep, please see report
LIGO-T-10123-00-R.
Gathering informations on glassy metals.
Riccardo
we submitted to NIM the actuator paper (after long delay), can find
under
LIGO-P010026-00-D.
Going Nov 4 to 14 to Italy to start Ultra Sound Milling Machine
construction at Faimond
Akiteru @ Hongo
Now we have a tower completed and get started with the Michelson
measurement in a few days.
Alessandro @ Pisa
Participating to the Fermi 100th anniversary celebration.
Happy birthday Enrico
For additional information about this report, contact sanders@ligo.caltech.edu