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The LIGO Executive Committee Agenda for Monday April 14, 2003 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items: POST
S2 COMISSIONING PLAN
no report
LIGO Weekly Site Telecon (Lindquist)
There was a very brief site teleconferences held on Thursday, April 10, 2003. The following issues were among those discussed:
Construction Contingency Status: Florence reported the current status. Including actual costs and commitments to dat (Florence indicates that the current open commitments are pretty firm) plus Albert's budget for computer hardware, there is only a couple of hundred thousand left to spend. Some of that has been pretty firmly allocated (e.g., storage building at Livingston). We will continue to monitor and report again next Monday.
Meanwhile, Livingston is preparing several Change Requests for stuff.
Dial In for Meeting Access: It was proposed that we return to
a fixed telephone number and participant code for the weekly site teleconference.
The list of current actions revised to reflect
the status of open actions assigned through April 10, 2003 may be found
at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
ACCOMPLISHMENTS
Reviewed the Laser Safety Program document with Bill for final changes and finalized several laser safety forms. These forms will be extracted from the document and prepared as stand-alone templates for web posting by the end of the week.
Converted several redesigned forms (process travelers [4], DCN, and technical paper cover sheet) into templates. These will be added to the template area on the LIGO web page.
Processed several ASP, Aspen, and Moriond presentations.
Continue to address the myriad of submittals with problems, ie. numbering, revisions, formatting, duplicates, etc.
ACTIVITY
| WE 04/10/03 | Packages | Faxes |
| In | 38 | 55 |
| Out | 16 | 36 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
No report this week.
From: Florence Kaufman <fkaufman@ligo.caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Weekly Advanced LIGO Project Controls meetings were not held this week. Next meeting scheduled for April 15 to discuss LDAS, DAQ, and Support Equipment.
For list of documents that are being used to develop Adv. LIGO Cost and Schedule, see http://www.ligo.caltech.edu/~tfrey/Cost_MTG_082002/
Advanced LIGO MRE Proposal (Highest Priority)
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
The Construction project quarterly report for the end of February was
scheduled to be submitted at the end of March. Irena has been working
on this, but has been distrtacted by a number of other priority issues:
LSC, contract activities for seismic isolation, core optics, etc.
We have discussed priorities, and the quarterly report is still slipping.
Dave Beckett and I have been gathering and editing materials for a
brochure discussing the current state of LIGO and the plans for Advanced
R&D. Drafts have been sent to Governement Publications folks.
The following Change Requests were discussed and approved
during the meeting of the LIGO Executive Committee on April 7, 2003:
| Request No. | Description | Requester | Date |
| CR-030002
Revision A |
Adjust FY 2003 Operations Budgets to reflect actual staffing levels | P. Lindquist | April 2, 2003 |
| CR-030003 | Implement an OC3 Wide Area Network Link fro Hanford via ESnet | A. Lazzarini/L Wallace | April 2, 2003 |
| CR-030005 | Furnish laboratories in the new Laboratopry Building at Hanford | R. Savage | April 2, 2003 |
Draft minutes have been prepared (LIGO-M030077-00-P) pending the receipt
of materials from Albert and Rick. Basically the task managers are
authorized to proceed.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
The LLO Incident Report and the Accident and Incident Investigation Report forms can now be accessed at the LIGO Internal Bulletin Board under Templates and Forms.
During the process of completing the update and
revision of the LIGO Laser Safety Plan, each of the two eye examination
clinics was contacted and asked to review the revised LIGO laser eye exam
protocol and to verify that they could conduct all of the eye exams required.
The Caltech Safety office was advised by the
Center for Occupation Health that they are no longer doing laser eye exams.
With this disappointing news, Barbara Cruz (of the Caltech Safety Office)
did volunteer that they had one other contract medical clinic that she
would contact to see if they could do the laser eye exams. Their response
was yes, they could, and would be interested in doing these eye exams for
LIGO.
Once again, we have two clinics that will do the laser eye exams in accordance with the requirements of the LIGO Laser Safety Plan and the ANSI Z136.5-2000. LIGO QA has contacted both clinics and reviewed with them the eye exam requirements to assure that there are no misunderstandings regarding what is expected by LIGO. The two clinics are: Pasadena Eye Medical Group and St George Medical Clinic (new for LIGO). Both are near to Caltech. Linda Turner has also prepared new eye exam request forms that will be "administrated" (mostly) by Ryan and Cindy.
The draft of the revised LIGO Laser Safety Plan will be distributed for approval early next week.
Meanwhile, the updated and revised LIGO Vacuum Compatibility, Cleaning Methods and Qualification Procedures (LIGO-E960022) specification is now posted on the LIGO Internal Bulletin Board for easy access by all of LIGO. Please take a look and use the forms included. The forms included in this specification will also be assigned LIGO form numbers and posted separately for convenience. The specification still needs the formal sign-off and release process completed. Please advise Helena Armandula, Linda Turner or Bill Tyler if there are corrections or changes still needed.
Summary of S2 Science Run Activities at LIGO Hanford Observatory (compiled
by M. Landry)
---------------------------------------------------------------------------------------
This last week of S2 has been mainly quiet, with stable IFO performance
and typical duty cycles
and inspiral ranges. As the run closes out, we are making final
diagnostic measurements.
Cheryl Vorvick investigated how hardware offsets were preventing the
WFS loops from being closed
and sometimes knocked the 4k out of lock. See the description
and the annotated plot at
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/08/2003&anchor_to_scroll_to=2003:04:08:16:06:40-Vorvick
The last 24 hours have seen little science-mode activity on all three
interferometers. The
mother of all injection runs took place last night; see Peter Shawhan's
elog at :
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=04/10/2003&anchor_to_scroll_to=2003:04:10:09:23:02-pshawhan
In addition to the typical battery of burst, stochastic and inspiral
waveforms, new ringdown
waveforms and simulated pulsar signals (monitored with Greg Mendell's
online LDAS DSO) were
injected into all three IFOs. Once astrophysical hardware injections
were completed, the third
and final S2 calibration run began at both sites, occupying the instruments
much of Thursday.
Duty cycles for the week were as follows: H1 (71%), and H2 (62%);
these numbers have been
limited somewhat by the recent studies noted above.
Interferometer Operation During S2: The LLO interferometer continues to operate routinely during the night, but poorly during the day due to seismic noise. The cumulative duty factor is around 37%. Injections Wednesday evening (conducted simultaneously at both sites) went very well, with all three interferometers locking throughout the period.
LDAS admin: Received tapes for the new tape robot, ordered and received
two UPS for the new tape robot, received two racks for the new beowulf
nodes. LDAS data analysis: still working on single pixel clusters and
coincidence with time-frequency window in waveburst. Took two owl scimon
shifts on Monday and Tuesday nights. (Igor)
LDAS: Received a quote on some dual processor Athlons to see if it was
even worthwhile to evaluate them for the next beowulf. However, it does
not look feasible.
Waiting for the run to end to put the VPN between sites in place. I
expect it will go smoothly. (Shannon)
CDS: Tested Matlab 'DataGet' program on solaris and got hongyu to fix a bug. Ported Matlab 'DataGet' program to Linux after porting D.J Bersteins "libtai" library with LIGO utc-to-gps and gps-to-utc functions. Compiled and tested on RH linux 8.0. Working on a Post S2 list of things to do. Preparing to change london to user access and make it a pure web server. Also adding a new machine "river" with individual user accounts. Chethan
Seismic Amelioration: I have been looking at schemes to lighten the offload springs for the EPI system. I have been able to reduce the weight by 7% without taking an appreciable hit on the factor of safety. (from 3.81 to 3.76) The ultimate hope is, of course, to drive the first frequency as high up as possible. I will start the mode shape analysis early next week. (Marcel)
GC: Put a call into Foundry to talk about getting quieter fans for the switches at the end stations. The support person I spoke to suggested just disconnecting the fans. He says there is a temperature sensor in the unit that will shut it doown if there is any danger of overheating. I am not sure how confident I am in this solution, but we will probably try it after the run is over. Working with Jonathan on some as yet unsolved Pcard problems. This is creating a hassle for him. After talking to Ciro at Caltech, it looks like in the long run more people will be affected by this. Another round of the usual - License purchases, security patches, etc. (Shannon)
Other: There will be an end-of-run party and send off celebration for
Rana on Wednesday afternoon at LLO with hot crawfish and other traditional
food. Everyone is invited. Andri Gretarsson is a father! His wife and his
new daughter Cassiopaeia are doing well.
For reference the documents and presentations from the last review are posted here: Last Review (4/2002)
Hepi pump controller low frequency noise investigation: see below
- As part of our continuing experimentation on how
to make our systems faster to
meet increased demands on some systems, we got a loaner
dual 1.26GHz Pentium III
VME processor board to test. This unit has a single
66MHz/64 bit PMC slot, so we
had it delivered to coincide with our receipt of the
new 2Gbit/sec reflected
memory network boards, which have a 66MHz/64 bit interface.
As an initial test,
we loaded it with the same Linux and suspension control
software we are using on
the PCs for the 40m lab. The timing numbers which
resulted were somewhat of a
surprise, at least to me. Running 4 optics on one
CPU resulted in 41usec.
Starting up the second CPU to run another 4 optics,
for a total of 8, resulted
in a processing time for all 8 of 47usec. For comparison,
the same timing
numbers for the dual 2.8GHz Xeon PC were 36usec and
41usec. This VME board also
does not exhibit the 200usec hickups every 64 sec
that was seen with the Xeon
PC. This code has not yet been modified to make use
of 64bit transfers or to use
the enhanced background I/O techniques employed in
the new LSC code, so we could
probably cut a little more. Our next test is to put
this unit right into the
front end VME crate and have it do all the I/O locally,
instead of over the
reflected memory network. Using the new I/O techniques
of the LSC and the
enhanced I/O features of the new reflected memory
card, it may be possible that
we could do all the I/O, control processing, and DAQ
for 8 optics within a
single crate. This would have an advantage over the
PC/VME solution in that it
does not rely on the reflected memory network for
control. The PC/VME version
has the advantage that if processing requirements
increase or other control
applications come about which want to use signals
from multiple I/O crates, one
simply inserts another PC into the network.
- An initial port of EPICS to Linux was done this
week. We also received the
Linux drivers for the new reflected memory boards,
and this all seems to work.
The idea is to use a Linux PC in the 40m lab to run
the EPICS interface to all
of our realtime systems, instead of a VME Pentium
processor or Sun. We did some
checking with members of the EPICS collaboration,
and, while they have done some
porting of EPICS modules to Linux, the part that traditionally
runs on the VME
front end units has only had a limited port to small
PC104 processor boards. We
are thinking that it might be fairly useful to continue
this port to support PCI
I/O modules (the EPICS collaboration would have an
interest in this). This could
make for a fairly inexpensive system for the small
test systems that spring up
from time to time, such as optics test stands, etc.
Instead of an expensive VME
system, one could add a few I/O cards to an inexpensive
PC. I could even imagine
taking it a bit further. Given that our DSP software
is now fairly modular, the
realtime DSP tasks could almost be defined from an
XML file (with graphic editor
if one wanted to get a little fancier), which describes
the various I/O, digital
filter banks, I/O matrices, and DAQ/GDS connections
for a control system. Add in
Daniel's FOTON software to develop the digital filter
coeffs, and one is close
to being able to easily develop a new control system
without writing code, per
se. Maybe put this into a dual CPU box using PCI I/O,
with one CPU running the
realtime DSP and the other EPICS (or one can even
add PCI card based Intel
processors) and one might have a useful control system
in an expensive package.
Add a 2U high Linux box with 4x100GByte disk system
and a reflected memory
card, and you add a reasonable DAQ system, with its
storage and NDS capabilies,
and access to dataviewer and GDS tools.
1.All
printed circuit boards have been sent off for manufacture. We are
on schedule for a trial of the new ISS servo at LLO during the week of
the 21st of April.
2.My
agenda for the LLO trip during the week of the 21st of April is:
RFI measurements using the new tools, ISS characterization with the new
servo and modifications to the LLO FSS to add the newest revisions per
LHO findings.
3.Progress
was made in analyzing low frequency noise in the HEPI pump motor speed
control. Source of 0.5 Hz oscillation tracked to ground bouce in
the interface to the pump motor controller. An isolation amplifier
and associated components have been chosen to break the ground connection
between the speed control servo and the motor controller.
4.Discussed, at length, the re-design of the RFPD. I am ready to begin the final design.
Ben Abbott
The new stands for the ISS PD are in the machine shop being fabricated. They should be done early next week. I have sent in the PCB for the ISS PD transimpedance heads, and the satellite boxes. The heads should be here by Friday, and the boxes' PCB should be back by Tuesday. The whole thing should be ready to go to Livingston for testing, the week of the 21st.
Jay Heefner reporting
1.LOS
Coil Whitening: Schematics are complete and being reviewed. Board layout
will start 4/10 and should be complete by 4/11.
2.EMI
Retrofit: The Elma crates have been received. Dawn crates were shipped
on 4/7 and should arrive next week. Both sets of racks are due at LLO late
next week.
3.WFS Feedback to Mode Cleaner Mirrors: A proposal on how to set up a quick test of the feasibility feeding back to the MC mirrors from the WFS was circulated and discussed. The test will be done at LLO the week of 4/18 and will require the installation of a temporary VME crate in rack 1X4.
Sandr Liu
1.Repaired EO Shutter Controller S/N 204 from 40M. From the damages seen, I believe the cause was deliberate rather than normal wear and tear for the following reasons:
a.The threshold adjust potentiometer was railed and locked in that position to disable any photodetector signal from operating the unit.
b.Couple tracings on the PCB have been cut and lifted in places not obvious from normal visual inspection. One of them disabled a large portion of the output circuitry.
2.Shipped the spare micro-seismic signal processor to LASTI.
3.Received
the custom build shielded housing model for the Euro card cage from vendor.
Form and fit seems OK
and will be used for future HEPI/MEPI design.
I have been trying to figure out the appropriate size
of chiller for
upgrading the Lightwave 10-W laser with. Part
of my confusion is trying to
match the data we have available with the measurements
that refrigeration
mechanics are familiar with and would like to have.
As some of the
measurements they would like to have are not easily
do-able without some
extra hardware and time with the laser.
The optically contacted pre-modecleaners for Hanford
were shipped out from
Livingston. The mounting hardware was also shipped
out.
A PCB for a discrete component amplifier board was
re-laid out after a
slight modification to one of the component footprints
(TO-92).
I have stitched (manually) the tidal data from the
first four weeks of the
S2 run. Nothing out of the ordinary, although
some rather large
displacements were experienced (+/- 150 microns at
X-end).
Design requirements review was held.(presentation) Requirements for reflectivity and BRDF of the errant beam baffles were developed based on allowed scattered light phase noise into the IFO. The proposed design was approved contingent upon increasing the stiffness of the baffles, and doing a further scattering analysis of scattered light from COC mirror surfaces being re-scattered by the proposed baffles. Ken is working on redesigned baffles with increased stiffness; a baffle-mounted cavity beam dump for the RM reflected beam is being designed; the RM reflected beam dump will be placed on the MMT2 baffle, because a ray height analysis shows that location allows the maximum tilt angle of the RM. Mike is extending the scattering analysis to include COC mirror surfaces.
The current plan is to make all the baffles except the 3 beam dump baffles at MMT2from stainless steel. A test is under way to air bake the stainless to produce an absorptive coating @ 1064. The MMT2 beam dump baffles are 1/4" aluminum and will have an absorptive coating from an outside vendor. There may be additional baffles required to protect the tabled wires and connectors running from the osems.
The earthquake stop SOS is ready to be moved over to the OTF. Mark will move it soon.
A draft report on the contamination test results for potential hydraulic fluids is available here; to be revised soon with recent results, mineral oil results and minor edits.
OTF Lab. (W. Bridge)
Contamination Cavity # 1
We have concluded taking measurements of the Chem-Sol Hydraulic fluid
(pink dyed fluid) and there is no contamination reported.
NEW test sample INSTALLED KAPTON(Polyimid) paint. It is
pumping down.
We are taking ring down and beat frequency measurements everyday.
Absorption Test Measurement prototype in STANDBY.
Scatterometer
The function of the scatterometer has been fully recovered as mentioned
before.
A preliminary result of our measurement of the AR reflection for the
large mirror
ITM S/N 4ITM08 has been released. The reflection of the AR coating
averages ~1330 ppm.
We measured its transmission T= 2.95% (The mirror data
reports to be 3%)
OTF Lab at Lauritsen ROOM 38
Cavity #3
The test sample SR FR HF from Chem-Sol, Inc. ( Undyed Fire retardant
Hydraulic Fluid)
still pumping down. We are taking ring down and beat frequency
measurements everyday.
Please see Dr. Zhang's latest graphs for absorption, ringdown and cavity
thermal lensing measurements.
Cavity #2 Test cavity
This chamber still pumping down with new cleaned mirrors ~ 70ppm
each.
RGA measurements and new optical train set-up is in progress as right
now.
The new contamination chamber has been baked (40m South Annex).
Preparation for insulation covers, heat tapes and tem.sensors is under
way.
The new Viewport windows are being placed in hold since it is
expensive($1330 ea. plus)
Instead, I will modify the position of the cavity in an angle in order
to prevent feedbacks.
no report
LASTI (Abbott, Allen, Ballmer, Coyne, Harry, Hardham, Lantz, Mason,
MacInnis, Mittleman, Ottaway, Rankin, Rollins, Zucker)
---------------------------------------------------------------------
PSL (Jamie)
--------------
Jamie continues to improve his AdLIGO intensity stabilization
prototype. With Rich Abbott's help, he implemented the latest
rev's to the Lightwave power supply and current shunt actuator;
these greatly improved the stability and reproducibility of
his results. He also has installed an air current shield around
the PMC and the sensing and out-of-loop monitoring photodiodes.
EPI Design (Ken)
-----------------------------------------------------------------------
A modal analysis of the HAM crossbeams and stiffeners was done to
duplicate the existing structure and to see the effects of additional
stiffening. A similar modal analysis was created
for the BSC piers. The top of the BSC piers currently sway at approximately
25 hz. Structual modifications are being modeled to eliminate this problem.
EPI Electronics (Rich A, Jon, Rich M., Mike)
----------------------------------------------------------------------
Went through the substantial amount of redlines and rev's to the drawings
now comprising the HEPI and MEPI systems. Jon will propagate
these back into the design CAD files and organize them under a
project drawing tree to better position ourselves for flat out
production when it all hits the fan.
EPI VME Controls Port (Stefan)
----------------------------------------------------------------------
Stefan has collected enough guidance from
Jay Heefner, Rich Abbott, Dave Barker and Alex Ivanov to build a block
diagram and scarf VME modules and CPU's. He has started to assemble
a new VME crate directly above the existing MEPI dSpace control system
and is setting up its software infrastructure while we wait for the
remaining hardware modules.
HEPI Characterization (Brian, Corwin, Bill, Dennis, Rich A)
-----------------------------------------------------------------------
Brian Lantz and Corwin Hardham are visiting from Stanford, making
improvements to the loop and better characterizing resonances of the
HEPI system. Documentation for the upcoming review has been started.
Rich Abbott and Brian traced the previously reported spurious
pressure fluctuations to electrical pickup; it is now unclear
whether the measured physical effects themselves were
real or an artifact. Steps to cure the problem have
been taken and the lessons rolled into design considerations for
the next generation pump controller.
MEPI (Rich, Gregg, Rich A, Bill, Dennis)
----------------------------------------------------------------------
We are finishing up another round of system ID after last week's plant
modifications. These consisted of changing the spacers between the
actuator housing and the piers from shims to plate, and adding
additional clamps at this interface. The modification have reduced
the
rocking in the actuator housing that was observed in most of the modes
above 50Hz. There is still some residual pier rocking which, in at
least
one mode, is actual movement of the pier (i.e. it could be connected
to
the ground more firmly). There is still one troublesome mode at 51.3Hz,
which consists of a flexing in the stiffening beams and rocking of
the
gullwings. Ken now has an FEA model which almost matches the
observations, the predicted frequency being 52.4Hz. The model claims
that this is the second lowest frequency mode; we have not observed
the
predicted lowest frequency mode and are currently investigating this.
In
any case, with an accurate model it should be much easier to predict
the effects of the various stiffening or damping measures under
consideration.
Simulation and Modeling (Bhawal)
E2E Physics meeting
--------------------
We (Matt,Virginio,Malik,Hiro,Biplab) discussed the linear noise model,
the 4k Schnupp asymmetry problem, mode-matching and setting of reflection-angles
for various optics in SimLIGO.
4k Schnupp asymmetry problem
------------------------------
(Matt) I conferred with Daniel Sigg on a possible solution to the 4k
Schnupp asymmetry problem. I proposed a control system
that utilizes
the non-resonant sidebands to produce a signal for the common
mode servo
and the pick-off for PRC and MICH. This eliminates the
need for REFL_I
in detection mode, thereby circumventing both the concerns about
critical
or indeterminant sideband coupling with improved mode-matching,
and the
emerging REFL_Q problem. This proposal has not undergone detailed
testing
(e.g., model work), but Daniel agrees that it looks promising.
LLO LVEA seismic analysis
---------------------------
(Hiro) Sany Yoshida summarized his analysis of the LLO LVEA seismic
motions
and wrote a note, which will be submitted as a DCC note.
This analysis, motion and coherence as a function of frequency
and
separation, provides a very useful input for the e2e modeling
of the
LLO. Also included is the correlation between the seismic motion
and MC
output beam pointing. Due to the placement of MC mirrors, MC
ASC and LSC
cannot control the output beam direction. This will be analyzed
by e2e.
Seismic model
---------------
Hiro received the matlab code from Matt to create the coherence
matrix
for the seismic simulation.
Hiro started using LLO data with the help from Sany Yoshida and
Doug
Lormand to create the e2e module to simulate the LLO seismic
motion.
Linear Noise Model in Matlab
------------------------------
(Matt) I built linear noise model (for use in Matlab) with modular
structure similar to that of E2E. This model allows for subsystem
reuse
(e.g., for suspension systems) and multiple versions (e.g., for
different
IFOs and changing electronics). I plan to use this model in conjunction
with SimLIGO in an attempt to develop a more detailed understanding
of
the noise spectra seen at the sites.
Mode matching in recycling cavity
----------------------------------
(Biplab) Investigated if changing the input beam waist position could
reduce the total mismatch effect in a not-yet-hot-enough recycling
cavity
and reduce the generation of Sideband higher order modes. The
effect
turned out to be very small due to almost "opposite" nature of
mismatch
at two mirrors involved (ITM and RM) in a range of plus-minus
10% of
Rayleigh range for the waist-position [Change in this range has
negligible
effect on Carrier build-up].
Radiation pressure module
---------------------------
(Hiro) More test was done and was committed to CVS. This will be included
in the next release. Those who can access e2e CVS can just cvs
update to
get this function.
Code development and maintenance
---------------------------------
(Melody)
- Tested the optimizations using SimLIGO. Currently cleaning
up the code
and getting ready to hand it over to Hiro.
- Working on a new if-then-else construct for the modeler.
(Ed Maros) Started working on some installation issues that are present
with RH 8.0 distributions.
Alfi
-----
(Bruce)
- Continued cleaning up and redesign Ports and Junctions to be
based on
the same superclass, the same one that Bundler will also
then be
subclassed from.
New Linux Box - "Ren"
----------------------
(Virginio) The e2e 1.7.11 version has been compiled in the linux box
ren
using the e2e account. Tested modeler with the latest SimLIGO
version and
it worked. The e2e home folder is accessible from the e2e group.
The binaries are located into the ~/e2e/bin folder (the e2e folder
is a
symbolic link to the latest version).
LIGO Data Analysis System
Software Systems (Blackburn)
We are currently testing the code base in CVS for a new interim release
of LDAS
in the 0.6.xx series which will resolve the problems identified in
the Science
Run associated with the frameAPI and mpiAPI. These fixes will improve
the LSC's
ability to conduct scientific investigations with LDAS prior to the
next full
release of LDAS (0.7.0) scheduled for late May. This new interim version
will
be placed on LDAS-TEST after the test suite is completed on LDAS-DEV
for a full
weekend of testing. We will push the new version to the sites after
the Science
Run completes early next week so as to not interfere with the ongoing
activities
associated with the run.
A bug was discovered in the LDAS account extension code used to quickly
provide a three month extension to accounts about to expire. This bug
was
isolated and fixed in the managerAPI after tracing through the secure
web
page cgi, the controlMonitorAPI server and finally the managerAPI.
The migration to the latest version of SWIG (Simple Wrapper Interface
Generator)
used by LDAS to interface C++ code with TCL code continues this week.
This new
SWIG has changed significantly and much of the interface code must
be reworked.
It is necessary for us to migrate to this new SWIG in order to migrate
to the
new TCL/TK release (which fix several issues we have with TCL). Currently,
we
have succeeded in carrying a dataPipeline through to the eventMonitorAPI
with
the new SWIG. This upgrade will be added to CVS after the interim release.
The XML C++ Parsing I/O library (Xerces) upgrade has almost been completed
this
week. This required significant modification to the lightWeightAPI
and a minor
change to the eventMonitorAPI to complete the upgrade. Testing with
the new
Xerces library has completed on a standalone LDAS system and will be
added to
the CVS after the interim release.
A new username/password validation interface is being added the the
managerAPI's
emergency socket to be able to log user actions and enforce disclosure
of the
user modifying the system.
A three hour meeting was held this week to review the state of problem
reports
in the LDAS problem tracking system (GNATS). There were 209 current
problems
filed in the system at the start of the meeting. Many actions items
were
assigned in the meeting and the list has been reduced by close to 40
problem
reports since the meeting with many more likely to be resolved in the
near term.
A new menu in the controlMonitorAPI will allow super users to test LDAS
systems
from a GUI interface. This new menu is based on the system level tests
current
carried out in our preparation for a release and requires organization
of the
test scripts and the Make distribution rules in the LDAS build process
with the
controlMonitorAPI's client software. A meeting between the tester,
builder and
the code developers to sort out the integration details was held this
week. The
new menu will be part of the 0.7.0 release of LDAS in late May.
A new (smarter) script is being developed by Philip Charlton to produce
the
RDS frames on the LDAS-CIT system. This new script resolves many of
the failure
modes in the scripts developed in the past for generating RDS frames.
It is
expected to go on-line by Friday of this week, allowing the generation
and
hence the transfer of RDS data to the Tier II centers to begin in full.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Got ldas-archive running again. There seem to have been two
failures.
One was a stuck 9940 tape of the form we'd seen before (if the
leader
block isn't seated right originally, the tape won't load correctly).
The other was a hang of the T3 housing the data for /site (testsite).
As best I can tell, this caused the entire FC network to hang
in such a
way that when ldas-archive was rebooted it couldn't see any
FC
devices. Once the T3 was power cycled, it came up and
began RAID
reconstruction. The fact that this completed successfully
(2 hours
later) leads me to believe that there wasn't a real hardware
failure.
Once the T3 was back up (online for both FC and Ethernet), a
cfgadm -c
configure c4 allowed ldas-archive to see all of the FC devices
and to
start archiving data to tape again.
* Manually checked 100+ 9940 tapes to make sure that their leader blocks
are seated correctly. This involves ejecting them from
the silo,
examining each one and then reloading them. I'm going
to continue this
at intervals until I've checked all the rest of the prelabeled
tapes,
as they didn't receive much inspection when they arrived.
* Locked some S2 data on disk for Julien Sylvestre to improve
performance. This involved manually staging the data and
then running
release -n on the files so that their disk space would not be
released.
* Got back to setting up a SAM-QFS multiwriter test.
(Al Wilson)
* With the arrival of the new Beowulf nodes. I have been testing the
new
release of systemimager 3.1. in the preliminary test it looks
like it
has been improved and will work great.
* Also I am testing kickstart and install procedures for the new release
of RH9.0. The testing has just started and will continue
over the next
couple of weeks.
* Two new racks are assembled in 215. They are awaiting the single rack
unit Beowulf nodes.
(Stuart Anderson)
* Successfully finished the 72hour memory test and copper Gigabit Ethernet
performance tests on the 3 beowulf candidate test nodes.
* Submitted the purchase request for the large Beowulf clusters
(420 dual-processor nodes).
* Submitted the purchase request for the large Beowulf Gigabit Ethernet
switches.
* Continuing to refine the configuration and pricing for the remaining
LDAS
servers and disk storage, including a backup frame builder disk
cache.
MIT
---
(Keith Bayer)
* Working up power requirements for NW17-017.
* LDR reinstallation received certificates (personal/host/service).
* Patched linux pc's.
Livingston
----------
(Igor Yakushin)
* Received tapes for the new tape robot, ordered and received two UPS
for the new tape robot, received two racks for the new beowulf
nodes.
(Shannon Roddy)
* Received a quote on some dual processor Athlons to see if it was even
worthwhile to evaluate them for the next beowulf. However,
it does not
look feasible.
* Waiting for the run to end to put the VPN between sites in place.
I
expect it will go smoothly.
Hanford
-------
(Greg Mendell)
* The primary sys admin focus continues to be keeping tapecontrol,
createrds, and LDAS running at LHO. Two createrds scripts
are currently
running to catch up and the S2 rds frames should be completed
within a
few hours after the end of S2. The last shipment of tapes
with S2 raw
data will go out to Caltech on Monday, April 14.
Data Analysis Activities (Lazzarini)
Weinstein:
- Continuing to work on burst paper, figures, etc.
- Prepared list of burst HW injections.
- Looking at the HW injections.
Mendell:
1) Continuing to generated 2048 s calibrated SFTs for H1 for S2 data
between Feb 22 2003 and the present.
2) Finished the first version of a command line tool called getFstat
that streamlines running knownpulsardemod DSO jobs that output the
F
statistic (requires an ldas password and ligotools to run). The
script
will allow nonexperts to run my DSO.
3) Working to analyze the 6-8 hours of pulsar hardware injections done
last night (Apr 09 2003). Posted preliminary results to the pulgroup
email list.
Reilly(Caltech)
I spent the end of last week doing shifts at Livingston.
This week I worked with Joe and(Albert on some Stochastic
data analysis issues. Eventually I convinced myself of the correct
way to create the plot of the average coherence for the
full S1 production data set. Finished the H1 H2 plot yesterday.
The H1 L1 and H2 L1 finely resolved coherence have now
been calculated. Expect plots later today or tomorrow.
At the griphynligo telecon yesterday it was decided that
future changes in the stochastic DSO are not significant
enough to prevent moving forward with work
to use grid technology for stochastic analysis.
Yakushin:
LDAS data analysis: still working on single pixel clusters and
coincidence with time-frequency window in waveburst.
Shawhan
* Studied the effect of the epoch veto in the inspiral upper limit analysis;
found that we
were making a mistake in implementing it.
* Took scimon shifts at Hanford.
* Did a bunch of hardware signal injection studies.
Lazzarini:
Have almost completed the study of the effect of systematic calibration
errors (variations in *alpha*) on the estimated value of Omega_GW for the
stochastic background analysis. This will allow us to complete the error
analysis section of the paper.
General Computing (Wallace)
MIT:
(Keith)
-Getting extra 30Amp circuit brought into gc computer room
-Spec'd out/ordered laptop for Ken Mason
-Ordered spare computer equipment parts
-Investigated printer troubles on pc
-Attended phone conference for 'neoteris' firewall product w/ LHO
Livingston:
(Shannon)
-Put a call into Foundry to talk about getting quieter fans for the
switches at the end stations. The support person I spoke to suggested
just disconnecting the fans. He says there is a temperature sensor
in
the unit that will shut it down if there is any danger of overheating.
I am not sure how confident I am in this solution, but we will probably
try it after the run is over.
-Working with Jonathan on some as yet unsolved Pcard problems.
This is
creating a hassle for him. After talking to Ciro at Caltech,
it looks
like in the long run more people will be affected by this.
-Another round of the usual - License purchases, security patches,
etc.
Hanford:
(Christine)
- Attended a web conference and demo for a remote access firewall
product.
- Solicited quotes from Cisco, 3Com and Foundry for the GigE network
upgrade. Met with the Foundry rep. at our site for a walk through
of
the network.
- Helped with a new laptop software install. Ordered another
Matlab
license for Linux.
- Dealt with some purchasing problems. Misc. user support.
CIT:
(Mike)
-Loaded a new Dell PC for the optics lab; this included loading all
General
Computing software, security and setting up user accounts.
-Swapped out Paul's old computer with a new Dell computer and loaded
all
updated GC software, plus I transferred his old data over and configured
his printers.
-Started loading Ben's new computer, this is a new Dell running XP
and
loading all GC software plus some additional software packages that
I have
to load.
-Started loading a new computer for a student who is going to be
assigned to be working at Wilson House. This computer is also running
XP.
-Setup a computer for a Dr. Cantley a visitor from Glasgow. This computer
needed to run some engineering packages such as Solid Works and Ansys.
After I started loading it turned out that the Operating System was
corrupted, therefore I had my work cut out to get this workstation
running
correctly.
-Setup a meeting for LIGO seminar that included more testing to clear
up
the output of the audio. This last meeting went pretty well, in regards
to the
audio/video.
-Worked some more on the new replacement server for PICTOR; I am still
getting this ready to swap out. It looks like I will be swapping this
server real soon.
(Veronica)
- LIGO web: installed a webpage for the APS April meeting.
Most time was spent working on the draft for the Advanced LIGO website.
Posted updates to Internal Bulletin Board.
Working on a DCC issue of adding a new document category to the search
engine.
Posting updates to various webpages. Processed a video for one of the
Aspen presentations.
- LSC website: posting the March meeting talks as they arrive. Posted
updates to the website.
- CaJAGWR website: updates to the website.
(Lisa)
- Spent most of my time working on the replacement server for
www.ligo.caltech.edu. There is an issue with how user url's will
be handled
that needs to be resolved. There is also a question with the
mount points for
document access.
- Looked into a problem for CDS regarding regular hangs they are seeing
on a
system.
- Did root partition dumps.
- Patched the mail servers against the latest sendmail exploit.
- Rebooted all the servers.
(Larry)
-Worked a couple of security issues. Most dealing with patches and
getting the
e-mail header information needed to block some of the spam.
-Worked a number of DCC issues. Most were files having permission problems.
Worked on some of the DCC cleanup that Linda asked for.
-Put in the WAN connection PR for Hanford. The change request was approved
and
the PR was put on motion soon after. Gina now has the paperwork and
has made
initial contact with the IPS provider for the WAN connection.
-Helped a number of people out with PC problems. So far most of the
problems
have been rogue processes. Killing the process and restarting it has
fixed the
problem in most cases. Also, went through to see where we need to upgrade
some
of the older PC's with units being turned over to GC from LDAS in the
July time
frame.
-Started working a ansys setup issue but I've been side-tracked and
will not get
back to it until next week.
-Worked a number of procurements. Resolved a couple of maintenance
issues and
have a few more to go. Placed a number of orders for computers and
related
items.
-Installed another UPS and have the router connected to it. The unit
has been
tested several times to make sure it can handle the load from the router
and so
far it has passed the tests.
-Worked a couple of web issues but nothing major. The move to the new
web server
has started. Users will soon be asked to start moving their home web
pages to a
new location, that announcement should be made next week, as soon as
a few
logistical items are worked out.
The RFP (Request for Proposal) package for designing, prototyping and production of the stiff, active SEI structures for HAM & BSC chambers was sent to 7 prospective proposers on 5 April.
Contracting will be broken into three phases: Phase 1, 3 contractors, recommending value engineering modifications to the Technology Demonstrator design (assuming that would go into production); Phase 2, (downselect to) 2 contractors, designing and building a prototype of a HAM SEI structure and of a BSC SEI structure, to be delivered to LASTI for testing (one structure per contractor); Phase 3, either 1 or 2 contractors, producing two or three sets of HAM and BSC SEI structures for installation at the observatories. Phase 2 is an Option to the contract, with a fixed-price bid up front. Phase 3 is an Option to the contract, with a ROM (rough order of magnitude) estimate up front, changed into a fixed-price bid at the end of Phase 2. Our objective is to maintain competition to the production phase, which will be an expensive fabrication effort.
A Proposers' Conference will be held
at
Gin Gin
The final drawing for the ETM suspension went to the machine shop last
week. The machine shop is planning to deliver the machined parts by April
18th and the fixture parts by April 25th. I'm planning that Bob Taylor
will clean and bake the ETM and ITM parts the week of April 21-25. We will
assemble the suspensions from April 28-May 9. The week of May 12-16 will
be for shipping the suspensions to Gin Gin.
We are planning for Doug Cook and Mark Barton to reassemble and install
the suspensions the week of May 19-23, if Gin Gin
is ready. I'm awaiting John Jacob's validation of this.
Earthquake Stops
The earthquake stop SOS is ready to be moved over to the OTF. Mark
will move it soon.
From: ctorrie <ctorrie@ligo.caltech.edu>
RM
MPL and I have designed a rotational stage for the upper blades. This
will be directly transferrable to the quadruple
pendulum design. We plan to review it at Janeen's
LASTI meeting next week.
QUAD
Mike Lloyd has created an assembly of a possible upper mass. Caroline
and I will start to look at the deflection and stiffness of this assembly
as well as considering it wrt the preliminary
quad structure.
ANALYSIS
Caroline, Janeen and I have been modelling
the MC structure in ANSYS and I-DEAS. We are trying to tie up these results
with those measure experimentally before
we move forward with stiffer structures for the triples and start to look
at the quad design created by Dennis Coyne.
LAB
Caroline and I are in the process of the re-assembly of one of the
MC suspensions, after taking it apart earlier this week.
A full report, including work done with Caroline will be composed for next week.
From: Jay Heefner
<jay@ligo.caltech.edu>
Gin Gin Controllers
======================
- The fisrt controller and satellite
amp have been tested with the dummy mass and are ready to be shipped. The
second units will be ready by 4/10. The third unit will be complete by
4/17.
Fused Silica
Q
--------------
After two attempts to suspend the spare LIGO I
optic ITM11, the best Q we have
measured for this mass is 1.0e8, for a mode at
11.202 kHz. This value is well
above any previous measurements for a LIGO optic,
and not very far below the
best values for fused silica measured by Ageyev
and
have such high Q is puzzling, since previously
such values required hard
annealing or flame polishing or maybe both.
This optic was mechanically
polished (by CSIRO) and has not been annealed.
We intend to continue our measurements and see
if we have reached the limiting Q
for this optic or not.
#DHS Note: Quite an interesting
result!
Arrived and going through internship period- being trained on melting
and
splatting by Eric and Hareem
Hareem
trying to get splatter to work
Eric
melted various new alloys and standard MoRuB
assesing x-ray diffraction crystal % technique,
found pitfall which can be
solved (surface must be smooth), verfied
machines credibility with Si
standard and checked background noise on puddy
etc..
For additional information about this report, contact sanders@ligo.caltech.edu