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The LIGO Executive Committee Agenda for Monday January 13, 2003 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items:
The LIGO Laboratory General Computing infrastructure and our support staff provide support for text document preparation using standard versions of Microsoft Word running on the Windows/Intel platforms. Documents archived in the DCC are stored in Adobe Acrobat format (.pdf files) and for text documents, the native Word files can also be stored with the Acrobat versions.
The LIGO Laboratory does not provide support for any forms of TeX or LaTeX. While these powerful typesetting programs are in wide use in science they have features that make standardization in our large organization difficult. While TeX files are simple text files, permitting easy exchange, common usage of these formats involves macros that have never been standardized. Office support staff are rarely trained in these unusual text programs. The files are simply not as universal as commodity Word files. Tex and LaTeX are free. However, costs to the LIGO Laboratory to provide true support of TeX and LaTeX far exceed the simple market costs of the various software packages. Any choice of macros, viewers, etc. that we would make in such an environment would fail to match all of our collaborators who have made individual choices.
For these reasons, document preparation in the LIGO Laboratory will be supported in simple text files and in Microsoft Word formats compatible with the recent versions only. We do not support Laboratory-wide document preparation under Solaris or Linux or Macintosh OS systems, nor do we support Star Office, FrameMaker, or other text editors, though these are in individual usage in the Laboratory to accommodate special needs. It is the responsibility of all LIGO Laboratory staff to provide and exchange files in this group setting that are fully compatible with the adopted standard. We cannot support conversion of TeX or LaTeX files provided to us by collaborators into the adopted standard as this would require maintenance of an infrastructure and detailed TeX expertise that is not economically sensible. This policy reflects the fact that Word is widely available off the shelf as a commodity and that sets the standard.
Most equation typesetting can be accomplished in Word. For more demanding equation editing, there are commodity addon packages such as MathType and the LIGO Laboratory is now supporting this capability.
GHS
From: Rainer Weiss <weiss@ligo.mit.edu>
to: LSC executive committee
from: R. Weiss January 5, 2003
Notes from the LSC Executive Committee meeting January 3, 2003
TAMA/LIGO working group
------------------------
The executive committee approved the candidates for the joint data
analysis
group which had formed at the GWDAW meeting.
Goddard Space Flight Center request to increase FTE to analyse LIGO
I data
--------------------------------------------------------------------------
Jordan Camp has asked for approval, prior to additional MOU negotiations,
to increase the effort at Goddard in the analysis of LIGO data in search
of
coincidences with Gamma Ray bursts. He is proposing to add John Cannizo
a
scientist at Goddard and the University of Maryland and Todd Strohmayer
a scientist and programmer at Goddard to the group. The scientific
value
of the investigations is recognized by the committee but several issues
were brought up which need to be dealt with. Some are not specific
to this proposal. I will call Jordan Camp.
1) The effort needs to be coordinated with others already on going in
the
LSC, in particular, the burst upper limit group needs to be coupled
to
this effort.
2) Need an understanding about the authorship of LIGO I papers. The
assumption is that new people at this stage of the LIGO I program
will not be general authors on the group papers but rather authors
on
special investigation papers. Also an understanding is needed
concerning the availability of new FTE for shift and other Collaboration
service functions.
3) Is the gamma and x-ray data shared across the Collaboration?
Moscow State University request for detector characterization data
-------------------------------------------------------------------
The request to access LIGO I data for the study of various instrument
features
without good coupling to the experimental teams at the sites was met
with some
concern. The proposed investigations should be coupled to the LSC committee
on detector
characterization. The major issue is possible misinterpretation through
insufficient
discussion with the scientists who actually know the idiosyncracies
of the
apparatus. I have been asked to discuss the proposal with Vladimir
and Kip.
Competition for time at the LSC meetings
----------------------------------------
Discussed the proposal by Ken Strain to include QND measurements
in the interferometer configuration session of the March LSC meeting.
Although
preparation of the first result papers for publication
and the increased activities in advanced LIGO planning have priority,
it was now
considered important even for advanced LIGO planning (primarily in
deciding on
fringe modulation techniques) to include these advanced techniques.
The amount of
time dedicated to the various activities at the March meeting will
need careful
planning which should begin in February and not wait until March.
Statement on shifts and other service functions
-----------------------------------------------
The draft letter on shifts and service functions will be sent
to the LSC Council with two changes. The first is to mention that LSC
groups
assign an individual to interact with the shift organizer. The second
change is in the numerical example where 12 hour shifts were assumed.
A more acceptable case are 8 hour shifts.
April 5-9, 2003 APS meeting speakers
-------------------------------------
Peter Saulson raised the issue of the need for LSC coordination of
a set of talks on
LIGO scientific results being planned by Sam Finn to be given at the
APS meeting.
A session on LIGO in general has been planned by Patrick Brady in consultation
with Gary Sanders and Barry Barish. The abstracts for the talks are
needed by January
10 so that coordination with Alan Wiseman, the upper limit group chairs,
and
Peter Saulson needs to take place in the coming week. The choice of
speakers
needs to consider that there will be other meetings in the coming year
and that the
talks should be distributed between the active participants in the
upper limit
groups.
Gary Sanders will provide a statement of acknowledgement (NSF, PPARC,etc)
to be used
by all speakers and in the papers to be submitted for publication.
Upper limit paper and report review committees
-----------------------------------------------
I have been requested to hold a telephone conference for the review
committees
to provide suggestions for process and to answer questions. Will try
to set
this up between Jan 20 - 22.
LSC Support for the advanced LIGO proposal
------------------------------------------
Gary Sanders suggested that the LIGO Laboratory organize the LSC wide
outreach
program. The plans for outreach activities are part of all NSF proposals
and
LSC institutions have been providing outreach on their own. The idea
would be to
coordinate and improve the quality of the program by hiring a person
especially
interested in and good at it. The program developed would then be used
by all
institutions in the LSC. The idea seemed attractive to the committee.
A letter endorsing the advanced LIGO proposal was discussed. The letter
is to be signed
by all LSC institution Principal Investigators and is addressed to
Bev Berger and Tom
Lucatorto. It will accompany the proposal submission. Several suggestions
to improve the letter were made. I hope to circulate the letter to
the PI's when the
the first draft of the proposal becomes available.
Next LSC Executive Committee meeting
-------------------------------------
Friday January 24, 2003 at 11AM EST
LIGO Weekly Site Telecon (Lindquist)
There were site teleconferences held on Thursday, January 2, 2003 and Thursday, January 9, 2003. The following issues were among those discussed:
Cost vs Budget Status--Based on current spending rates and factoring in extra bi-weekly payrolls period that occur twice each year, we forecast $32 million in expenditures for FY 2003. The $28 million flat funding profile plus the $4 million carry forward from FY 2002 will cover this, but does not provide the growth needed for full operations. Nor does it provide the bridge funds typically required at the end of the year while NSF funding gets through the approval cycle.
Civil Construction at Livingston--The interior walls in the Staging Building are approximately 70 percent complete.
Civil Construction at Hanford--Information needed for proposed modifications to the Laboratory Building have not yet been received..
Property--Ed is conducting an property inventory at Livingston.
Traffic control systems--The change request for Hanford has been approved and Hanford is proceeding, Livingston has some verbal quotes, but more work is required. Decisions are required concerning communications between the gate and the control room.
Advanced R&D--David Shoemaker is going to be in charge of the Advanced R&D Program. Project Controls will set him up as the task manager and reports will be distributed accordingly.
The list of current actions revised to reflect
the status of open actions assigned through January 2, 2003 may be found
at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
Weekly Status Report for 12/26/02 and 01/02/03
>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
Found about 20 articles on the internet about LIGO that hadn't yet been received by the DCC. Some of these are a year or two old, and there were even some technical documents and presentations that we didn't have. I'm in the process of assimilating these electronically into the DCC. It's a bit disconcerting to have viewed about 45 web pages and leave exponentially more pages unviewed given the articles found in this last search.
Reminder to LIGO staff: Please make sure that as a minimum, each document submitted has a LIGO number, author's name, and date. It's surprising how many documents are missing one of more of these essential pieces of information!
ACTIVITY
| WE 01/09/03 | Packages | Faxes |
| In | 17 | 29 |
| Out | 7 | 29 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
Weekly Status Report for 12/26/02 and 01/02/03
Weekly Status Report for 12/26/02 and 01/02/03
From: irena@ligo.caltech.edu (Irena Petrac)
Weekly Status Report for 12/26/02 and 01/02/03
The Change Control Board approved the use of $180,000 of construction funds for various activities at the Hanford site, including double glass doors and sun shades for the Laboratory Building, paving of parking lot, and traffic control systems. This should conclude construction at the Hanford observatory.
OPERATIONS:
Progress continues on the traffic control systems at both sites.
LLO has received a proposal for the widening of the access road to accommodate
the gates and readers, and is waiting for a quote on the gates.
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Accomplishments:
Weekly Advanced LIGO Project Controls meeting was held on Tuesday the 7th of January. The subject of the meeting was the status of the detailed cost estimate and a forecast of a request amount.
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)
We have completed the final draft of the annual report covering activities
from December 2001 through November 30, 2002. It will be sent to
the NSF tomorrow.
To support the proposal early next year for a LIGO upgrade, we have
prepared an update to the Annual Report for Operations that was submitted
to the NSF in September. This very first draft has been provided
to Gary for comment and assignment of additional action.
Change Request CR-030001 to provide funds for completion
of the Hanford Construction activities was approved during a meeting of
the LIGO Change Control Board held as part of the Executive Committee Meeting
on Monday, January 6, 2003. Meeting minutes have been distributed
(attachment to EMAIL): LIGO-M030001-00-P.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
An audit team consisting of G. Billingsley (LSO), C. Scislowicz, H. Issaian, A. Jefferson of Caltech Safety Office and W. Tyler, is conducting laser safety audits of various Caltech LIGO facilities where lasers are operated. Presently, only the 40M facility remains to be audited. As part of this audit activity, laser users are also being asked to submit a LIGO Laser Safety Inventory form (Appendix B, of LIGO-M960001) for all LIGO lasers at Caltech. Copies of the inventory data for class IIIb and IV lasers will also be provided to the Caltech Safety Office for updating LIGO's laser registrations.
A revised/update of the LIGO Laser Safety Program (LIGO-M960001) document was completed and distributed for comments/corrections. The primary revision was to incorporate ANSI Z136.5, "Safe Use of Lasers in Educational Institutions" for LIGO laser guidelines. The other revision was to update Appendix E baseline eye examination protocol and clarify the eye exam process. Once the program revision is approved and released, the updated forms (appendicies) will be available on-line.
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by M. Landry)
December 20, 2002 - January 9, 2003
---------------------------------------------------------------------------------------
Efforts are concentrated on WFS on the 4k and noise hunting on the
2k as respective S2
freezes approach. Visitors to the lab include A. Ivanov (CDS
reconfiguration),
R. Schofield (acoustic noise hunting on the 2k), and P. Brady (LDAS/LAL
S2 issues).
2K IFO (H2)
-----------
The 2k continues M2-like capricious behaviour of alternately locking
and not locking for long
stretches. Sometimes problems are understood (e.g. transients
in MMT1 due to bad
connections on an anti-aliasing chassis), at other points it is unclear
why good locking
resumes. Since last Saturday the 2k has been quickly and robustly
locking.
Fred notes that the 2k needs a factor of ten in sensitivity by S2 in
order to be
scientifically relevant, as it is lagging the pair of 4k's. While
the noise floor may
not be well understood, work is underway to eliminate the grotesque
acoustic structure
observed mid-frequency by dumping beams properly and realigning ISC
chains. Much of the
structure seen at higher frequencies is coherent with the common mode.
December work on the
MC refl path improved frequency noise, for example, reducing a peak
at 320Hz by a factor of
five.
4K IFO (H1)
-----------
The 4k continues to lock robustly and with improved sensitivity, thanks
to a common mode
gain boost stage just in time for Christmas. The main contributor
of noise in the 100Hz
to 300Hz region is believed to be coming in on POB_I. Some lock
loss events due to the
AS_I servo reaching limits were fixed by doubling the servo's range.
A program of test mass diagonalization was effected.
A modified FSS card (like the one now operating on the 2k) was tested
on the 4k PSL and
a unity gain frequency of 600kHz and a gain at 100kHz of 25dB were
noted.
A collaboration of onsite measurements and offsite analysis yielded
an unexpectedly low
transmission through the mode cleaner, 0.640. Details:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=12/31/2002&anchor_to_scroll_to=2002:12:31:08:32:34-peterF
Another analysis by Fritschel and Co. details the shot noise performance
of the 4k.
Details may be found at http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=01/07/2003&anchor_to_scroll_to=2003:01:07:16:25:07-peterF
Interferometer: Valera worked on the reflected port optics - measuring the beam waist size and position. He also worked with Brian, Peter and Rana on the periscope lens installation. Joe Kovalik measured the calibrations of the various frequency control loops of the PSL and mode cleaner. (Joe Kovalik)
LDAS admin:
1) Changed all the passwords on LLO's LDAS;
2) Configured ldas-jobs in the first approximation;
3) Uploaded LHO's RDS.
4) Moving to the new building is 95% complete: what remains is to test
everything and to clean the mess. Thank you everybody who helped!
LDAS data analysis:
1) Finished debugging BLOB insertion to database from waveburst DSO;
2) Submitted first approximation of waveburst DSO to CVS;
3) Working on adding correlation calculation to waveburst DSO;
4) Working on vectorizing waveburst DSO;
--
Igor Yakushin
This week has been taken up with the LDAS move to the new building.
We
have all of the equipment moved over there and are bringing things
up
now.
I am also troubleshooting a problem with one of my edge switches. I
have 10-15% packet loss to the switch. This is the switch that LDAS
and
general computing will plug into in the new building.
--
Shannon Roddy
HEPI / LAST
Ken Mason called out attention to a problem on the hydraulic actuators,
which is allowing fluid to enter the volume between the bleed valves
and
their safety caps. I find that a machinist at the shop decided to
increase the depth of a threaded counter bore, which is the cause of
the
leakage. I failed to catch this when the received parts were inspected.
Similarly, the valve installed in the leaking bore was redesigned,
and I
installed and delivered an earlier, obsolete valve in the too-short
bore. This aggravated the problem. Recognizing the defects allows us
to proceed with bleeding and testing safely, and I'm having the correct
valves manufactured ASAP should Ken decide to install them.
Also working on summarizing for Dennis total costs incurred in
production of the 12 prototype actuators, as well as obtaining quotes
from our vendors for a complete LLO SEI installation. (Hammond, Kern)
ETF / Advanced LIGO pod bases
Nothing to report (Hammond, Kern)
Optics / Laser
Arrangements are complete and we have a new ophthalmologist to perform
the battery of tests required for our Laser Safety examination.
Received and installed the Laser safety Interlock card printer. It
prints too faintly, so we've ordered a quantity of 'dummy' cards to
experiment with. (Carter, Watts, Kern)
Outreach:
A review of the rough draft for the Livingston portion of the outreach
proposal was held Friday, Jan 3. Jerry Pine participated in the review
along with Karen Worth of EDC. Souhern University was represented by their
Vice Chancellor for Research, Mildred Smalley, along with Dean and Asst
Dean of the College of Education, an Ed faculty member, and Steve mcGuire
- chair of the Physics Dept. Kerry Davidson of the La Board of Regents
(the board that defines education policy for the state of Louisiana) also
attended. Gary Sanders, Mark Coles, Phil Lindquist, Jill Andrews, and Hall
Daily also participating in various parts of the daylong review. A second
iteration of the proposal with a narrow, more sharply defined focus will
be distributed in about 2 weeks. (Coles)
Marcel Hammond, Jonathan Kern
Ken Mason called out attention to a problem on the hydraulic actuators, which is allowing fluid to enter the volume between the bleed valves and their safety caps. I find that a machinist at the shop decided to increase the depth of a threaded counter bore, which is the cause of the leakage. I failed to catch this when the received parts were inspected. Similarly, the valve installed in the leaking bore was redesigned, and I installed and delivered an earlier, obsolete valve in the too-short bore. This aggravated the problem. Recognizing the defects allows us to proceed with bleeding and testing safely, and I'm having the correct valves manufactured ASAP should Ken decide to install them.
Note from Dennis Coyne: This
small “weeping” leak is internal to the actuator and does not present a
problem to the LASTI installation.
Also working on summarizing for Dennis total costs incurred in production of the 12 prototype actuators, as well as obtaining quotes from our vendors for a complete LLO SEI installation.
Note from Dennis Coyne: Costs
are being gathered in preparation for a design review and CCB request.
A decision regarding an electro-magnetic and/or hydraulic actuator implementation
will not occur until after sufficient LASTI test results have been obtained
and a lab review has been conducted.
Ken Mailand
An optical contamination test of the LASTI fluid (Aquamil) is nearly completed, the results so far look good (see the optical contamination cavity testing comments below).
Also a biological growth test is showing nothing after 5 weeks.
We are expecting delivery of 2 samples of other clear
fluids, for possible use at LASTI, or at the sites. These fluid formulas
are clear, water soluble, fire resistant, and non toxic, and meet our basic
fluid specifications on file in the DCC doc.#
E021116 -A-D.
I continue to work on the documentation and cataloging
of the Pump Station, and the production version design, and an assembly
strategy.
This week I have been summarizing the current configurations of the DMT monitors for use in determining what should be changed before S2. I have also been writing a DMT monitor that can will detect and tag injected signals.
Alex is at LHO this week, primarily to replace the
DAQ Framebuilder network with a new 2Gbit/sec
link. With the new network in place, the DAQ controller load dropped
from 98% capacity to ~54%, so we should be in good shape for a while.
Both Framebuilders
at LHO are now running with Frame Version 6. The LLO Framebuilders
will be upgraded tomorrow after the LDAS T3 systems are back on line.
Due to problems with the Variable Delay Timing (VDT)
modules, I've changed out the Digital Suspension and LSC code at LLO to
go back to polling the Pentek modules instead
of the VDT for data ready. To reduce the effects of polling on ADC
noise, the last Pentek in the end stations
and LOS controllers is polled instead of the first. In the case of
LOS controllers, the last Pentek does not
have any signals connected to its ADC inputs. For the LSC, a third Pentek
was added to avoid polling the first two, as these have critical signals.
We are also looking at moving the GPS Ramp signal to this new Pentek
to get rid of the cross talk noise. I'm hoping we can get a new IFO
spectrum this week to see what effects these changes have had before moving
the code to LHO.
New LOS controller code loaded at LLO also has the
new dewhite and run/acquire switching that
has previously shown to be successful in the end station controller software.
Lori is in the process of loading the new ASC code here at LLO. Testing should start tomorrow.
PSL Intensity Stabilization Servo (ISS): Worked with Flavio to get the ISS running. Thanks to his diligence, the system is now working with the new transfer function and the two actuator approach. The new system has much more dynamic range than the old single actuator system. We communicated the changes to Rai while he was at CIT and he is going to try and get it installed at LLO. He also obtained the current shunt from Peter King to examine the circuit for slew rate issues. We are characterizing the system and getting ready to make a better optical setup.
Note from Dennis Coyne: Like the PSL FSS modifications
at LHO, the planned ISS modifications at LLO are as yet unreviewed
by the Revision Technical Review Board (RTRB). The
intent is to explore the efficacy and robustness of this possible solution
as input to a review before adopting the solution on all interferometers.
This aggressive approach, which deviates from review policy, is also motivated
by the possibility of immediate performance improvement for S2.
CDS Shop Cleanup: Todd and I are directing a general cleanup effort (throw away session) in the Wilson House to allow for long range storage of stuff. Things are getting better over here in terms of organization...
Jay Heefner reporting
Pentek Noise and Glitch
Testing: Testing of the pentek
modules for input referred noise, output referred noise and output glitches
is 95% complete and a draft report has been written. Next week a few final
tests will be conducted, then the report
will be issued as a technical document.
LOS Coil DAQ Readout: Preliminary circuit design
and simulation have begun.
EMI Upgrade: Equipto is providing us with a preliminary quote for EMI racks. It should be available next week.
Jay is meeting with Tracewell
next week to discuss their EMI-rated VME crates.
Advanced LIGO DAC: Frequency Devices is planning
on shipping the prototype to us for test in the next two weeks.
The high current photodetector
is now functional. The thermal shutdown
mentioned in previous reports
was due to a short in the series output
resistor, either because
of some stray solder or FR-4 shavings. The
magnitude response of the photodetector
requires some tweaking of the
compensation capacitor used
in the transimpedance stage but is flat
to 10 MHz,
exhibits about 3 dB of gain
peaking at 20 MHz before falling off.
The output noise measurement is a little affected
by the varying output
noise of the SR560 amplifier
used to boost the output. Early numbers for
the dark noise of the photodetector
are 3 nV/Sqrt[Hz] at 10 Hz and
1 nV/Sqrt[Hz]
above 100 Hz. At 10 Hz, the photodetector
is 3 times the
design specification.
I hope to start high power testing of the
photodetector later this week.
Lee Cardenas
MOPA S/N 119 sent to be repaired on 8/16/02
Lightwave Electronics contacted and found
out that the Pockell Cell (EOM) sent to
be
aligned along with the optical train of the 10 watt laser is not going
to be possible.
Dan Feehan from Lightwave
explains that the power drift of the laser was due to the
thermal cavity length and the changed of the
beam waist location due to the
Pockell Cell (EOM). The mode match was off
by ~ 1.00 inch from the input
aperture of the power amplifier. Without the EOM in place, They
claim power
obtained is 12.0 watts. and stable.
We'll have to install the EOM in place and
make the mode match ourselves. I have explained to Dan that the
most power
dissipated across the EOM when i
aligned in place was no more than 5-20 milliwatt.
He said that he is going to send back the laser without the EOM in
place, Otherwise,
He won't be able to warrant the Laser.
I run Melody for the "cold" configuration corresponding to Livingston and I got results that for the sidebands are different from the ones I got running the FFT-code, even using a huge number of modes in Melody (all TEM_mn with m+n<=20).
OTF Lab at Lauritsen
ROOM 38
Cavity #3 Reference Cavity.ready!
Taking measurements every day.
Cavity #2 Test cavity
The chamber is pumping with new cleaned mirrors ~ 70ppm each.We
are taking RGA measurements.
New chamber ready for modification (soldered base and base insulator) -- waiting on the machine shop.
Found a good glass blower shop to make a few contamination cavities.
Designing the new cavities is in progress. (pockets
for sample to be next to mirror)
Looking into suspending the cavity with springs,
the same configuration as the PSL reference cavity.
OTF Lab. (W. Bridge)
Contamination Cavity # 1
Cavity with test sample aquamill still
in progress and taking measurements every day.
Measurements of absorption, ringdown
and cavity thermal lensing measurements.
We'll continue taking measurements for two more weeks.
Note from Dennis Coyne: By eye it appears that
the change in absorption is < ~0.2 ppm/year;
A chi-square fit will be performed.
Waiting for more samples from Ken Mailand. Ken will let us know.
Scatterometer
Scatterometer recovering is in progress now.
From: Richard Mittleman <richard@ligo.mit.edu>
HEPI/MEPI Weekly Report from MIT
The first round of system ID on the hydraulic actuator system
which is
installed on the BSC has been completed. If anyone wants to look
at this
data they should send me email at richard@ligo.mit.edu. The pumping
system
has been running for 5 days now without any problems being noticed.
We are
now putting the system in bleed mode to remove any air which might
have
accumulated in the actuator in the last week, where it will remain
over
the weekend.
The HAM with the magnetic actuators has been recharacterized
with the
repaired electronics and efforts are currently under way to control
it.
no report
LASTI (Coyne, Forbes, Hammond, Kern, Mason, MacInnis, McKenzie,
Mittleman, Ottaway, Rankin, Rollins, Shoemaker, Zucker)
---------------------------------------------------------------------
LASTI PSL (Ottaway, Rollins)
---------------------------------------------------------------------
Still on travel
Sideband Camera (Goda et al)
-----------------------------------------------------------------------
Blair finished the first draft of her undergraduate
thesis on the enhancements of scanning methods of a sideband camera,
and
Nergis and I are reading through it and will give her comments
and suggestions this week.
Before the Christmas, Dave and I took the final set of data in order
to
understand the sideband camera better so that we will be able to install
a
sideband camera at each cite without serious problem.
EPI characterization (Mittleman, Rankin)
-----------------------------------------------------------------------
No report
HEPI Design, installation, test
-------------------------------------------------------
The installation has been completed with all sensors functioning. Brian
Lantz
was able to
measure transfer functions on all four piers before he left for Stanford.
Tested the noise at each hydraulic actuator in an attempt to determine
the
amount of air
remaining in the hydraulic actuators. Pier 2 horizontal was found to
have
substantially more
noise than the others. This weekend we are going to flip the horizontal
actuator
up and bleed
all actuators for 48 hours.
Triple Suspension Prototype Test
-------------------------------------------------------
The design of the solid stack stand-in
which will be used on HAM 21 at LASTI has been completed and
has
been ordered. All parts are scheduled to arrive on 1/17. They
will require a
clean and bake
before they are installed into the HAM.
Data Analysis and Computing (Lazzarini)
Simulation and Modeling (Bhawal)
Summation cavity code
------------------------
(Hiro) FP and PRM summation cavity code improvement
and validation still
going on.
Osamu and Hiro discussed further about
the fast calculation of the
field in dual recycling cavity.
Adlib code
--------------
(Hiro) ModalModel codes are updated. It now supports
the curvature mismatch
reflection matrix and implements some caching
for speed improvement. One
immediate use is to remove the explicit limit
of the modes used in e2e.
(Biplab) Modified files so that the code is able
to run with any spatial
modal order (there had been an upper
limit at m+n<5 until now).
Took first steps for comparison of the
e2e results with Melody which is
also a MOdal Model based simulation.
Documentation
----------------
(Biplab) The "primitive" document is updated for
the recent changes related
to the introduction of the global simulation
option "KeepGuoyOffset".
Alfi
-----
(Bruce)
- [4.0 days] Worked on streamlining the local
and remote
distribution of Alfi.
(Melody)
- Continued working with the automated tester for
alfi5.
- Worked with Bruce in improving the alfi5 distribution
process.
REPORT DATED JAN 02, 2003:
--------------------------
Weekly Physics Meeting
-----------------------
Matt, Hiro, Biplab discussed SimLIGO and WFS issues.
e2e outside support
---------------------
(Hiro) Michaela Malec (Institut fuer Atom- und Molekuelphysik
/ GEO) has
started using e2e, and posted a series of questions
in the ligo-e2e-physics
mail. Questions and ambiguities are answered and
the answers and sample
codes are available in http://www.ligo.caltech.edu/~hiro/cavhiro.tar.Z.
Adlib physics
-----------------
(Hiro, Biplab)
- Clarified the rotation operation
- Found the condition to preset a mode
mismatched cavity close to
resonance.
Summation cavity
------------------
(Hiro)
- Summation cavity code (FP, PRM) updated
- validating now
- Osamu Miyakawa has started formulating
for the dual recycling cavity
based on the formulation
by Hiro and Malik
- Started writing LIGO Document T030001-00-E
"Fast simulation of fields
in compound optics systems",
which summarizes the summation cavity
formulation.
Adlib Code
------------
(Biplab) The "keepGuoyOffset" option associated
with each propagator
(for both primitive and summation modules) is now
made a global option
and can be set in a "field_gen" module. This option
is utilized (e.g.)
to study the thermal lensing problem and to keep
track of the mirror
displacements as the IFO gets hotter. With new changes,
if this option
is set to "false", the IFO can build-up its power
even in presence of
mismatches. Several files were modified.
Alfi
-----
(Bruce)
- [2.0 days] General minor bug work
and documentation updates.
(Melody)
- Continued working on the automated
tester for alfi5.
- Finished updating the Alfi5 manual
available from the e2e homepage
LIGO Data Analysis System
Software Systems (Blackburn)
The month long struggle to resolve the core dumps in the lightWeightAPI
were
solved this week when Kent postulated that the objectSpace C++ socket
library
had been compiled with too high an optimization. This also fixed the
more
recent core dumping problems seen in the frameAPI. Since the C++ socket
library
was recompiled on Monday with lower optimization levels, no API has
dropped
a core file during normal operations (only during shutdowns). This
has been
a source of tremendous concern so close to the software freeze for
the E9 and
S2 runs. All are greatly relieved at having solved the puzzle. It does
mean
that we will not be building the version of LDAS for the runs with
high compiler
optimizations (a limitation from the transition to the new GCC 3.2.1)
so there
is expected to be slight performance hit until a new compiler arrives.
The frameAPI has dominated the effort of much of the group this week.
It now
has compress capabilities which are being tested and turning up lots
of bugs.
It also has a tendency to stall on some jobs until the 3600 second
time out
has been reach - A similar issue was last seen with the E7 version
of LDAS and
fixed for the S1 run. It is not expected to be from the same bug but
the source
is not understood and still being studied. At present, we loose a few
jobs out
of every 1000 from this issue.
Several issues with the metadata written to FRPROC structures have been
identified in problem reports and fixed. These issues were minor but
needed
to be cleaned up before the science run. Most were related to the large
conceptual change in the FRPROC structure in the last Frame Spec Update.
We are also seeing a few out of a 1000 jobs fail in the wrapperAPI due
to an
error on the first call into the MPI library. This could be due to
changes in
the mpiAPI or due to the recent upgrade of our LAM MPI source code
to the
latest version. We are backing out the LAM library first to see if
it is in
our mpiAPI code or in the Notre Dame LAM code. This will require more
study
and will not be better understood until we've had a couple of days
of testing
with the old LAM in place.
A gradual code freeze on the CVS repository is now in place. All developers
not on the 6th floor are temporarily limited to read only access and
those
developers on the 6th floor which have completed developing required
functionality for the next release are frozen out. It is expected that
a full
CVS code freeze will take place on Monday. Only bug fixes that have
been fully
tested and code reviewed will be allowed in after that and they must
go through
the CVS librarian.
A bug in the eventMonitorAPI which caused it to group several DSO multidim
objects into a single data product has been fixed. Now if a unique
output
product is requested by the user, they will get one per multidim object
instead
of being lumped together based on the socket tranmission objects.
The documentation for using the controlMonitorAPI client with its new
BLT
widget set is on the development web pages. The new GUI is much faster
and
has a nice look and feel to its plots.
Several minor modifications to the database tables have been requested
by the
upper limits groups in preparation for the S2 run. These changes are
now in
place on the LDAS-DEV system and will be added to test scripts. They
will be
generated at the sites in time for the pre-release pushes.
For the dataConditionAPI this week, completed datacon action for producing
a linear filter from a specification of zeroes, poles and gain. Documentation
for the new function called zpg2linfilt() has been added to the LDAS
User
Command web pages. Also completed code for polynomial expansion from
roots
and polynomial multiplication, added C++ functions for promoting real
data
objects to their complex equivalent while preserving all other attributes,
e.g., TimeSeries<float> to TimeSeries<complex<float> >. Several
open problem
reports on the dataConditionAPI and its documentation were also close
this
week. Commenced working on PR1818 "Need action for applying time-dependent
calibration" requested by Alan Weinstein.
A performance test of the new compression routines in the frameCPP library
were carried out using LDAS. There are several compression routines
which
were compared with GZIP's compression/performance. Preliminary results
are
interesting in that they suggest that the frameCPP compression can
actually
bet GZIP under most circumstances! This implies that it might be better
to
compress the data arrays in the frame files as opposed to compressing
the
full frame files (from a disk storage point of view).
A benchmark of the FFTW fast Fourier Transform C library using the new
GCC
compiler this week suggests that even though we are not able to gain
LDAS
performance with the new C++ compiler, the C compiler has speeded up
the
FFT by about 15%. The FFT boost will effect the dataConditionAPI and
the
DSO search codes running on the Beowulf Clusters.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Made HPSS and SAM-QFS data consistent with each other, working on
making
IDE-RAIDs consistent as well.
* Working with Sun to fix memory in ldas-archive.
* Got "fixed" Qlogic cards and instructions for installation.
Will
install as soon as ldas-archive is back up.
* Installed SAM-QFS 4.0 on ldas-archive, began to test.
* Got quotes for 1050 9940 tapes, am putting together order.
* Did some work on HPSS to try to revive hsi/ftp, but it ended up needed
hardware work.
* Did some HPSS project/account creation.
(Al Wilson)
* Installed BB on the test system. I am having a lot of false positives
with the new code. I will have to iron out some of the bugs
before I
release it on to the DEV system
* Working with GC to get updated NIS+ passwords.
* Also working with Dan Kozak on the command line interface for the IDE Raids.
(Stuart Anderson)
* Archived the M1 and M2 frame data.
* Upgraded LDAS-TEST and LDAS-CIT admin servers to Solaris 9.
* Upgraded web services on LDAS-TEST to use apache-2.x.
* Identified and debugged reduced NFS client read performance on Solaris
9
(set nfs:nfs3_nra=4).
* Built additional /ldcg tools for Solaris9 (perl, python, ...)
* Dealt with unexpected loss of air cooling to Millikan computer room
with
automatic electric outage to prevent equipment overheating.
MIT
---
(Keith Bayer)
* Successfully moved pc raid onto UPS.
* Dealing with space issues on gateway /export partition.
* Finished specing out Rambus cluster node.
Livingston
----------
(Igor Yakushin)
* Changed all the passwords on LLO's LDAS.
* Configured ldas-jobs in the first approximation in the absence of
more
specifications.
* Uploaded LHO's RDS.
* Moving to the new building is 95% complete: what remains is to test
everything and to clean the mess. Thank you everybody who helped!
(Shannon Roddy)
* This week has been taken up with the LDAS move to the new building.
We
have all of the equipment moved over there and are bringing
things up now.
* I am also troubleshooting a problem with one of my edge switches.
I have 10-15% packet loss to the switch. This is the switch
that
LDAS and general computing will plug into in the new building.
Hanford
-------
(Greg Mendell)
* The raw M2 frame data was sent to Caltech and successfully archived
in HPSS. GPS times available are 723952784 to 723974432 (as
previously
reported this data is also available on on disk in /frame10/M2/Data[0-6]
from fortress, sand, and stone, at LHO.
* A limited amount of LLO v5 RDS frames from S1 for GPS times 714994352
to 715069216 have been made available on fortress, by request
for dtt
studies, in this directory: /ldasdisks/LLOrds/Tape14.
* Worked on AIT-2 tape requirements for S2.
Data Analysis Activities (Lazzarini)
Yakushin:
1) Finished debugging BLOB insertion to database from waveburst DSO;
2) Submitted first approximation of waveburst DSO to CVS;
3) Working on adding correlation calculation to waveburst DSO;
4) Working on vectorizing waveburst DSO;
Weinstein:
- Working on modeling of burst sources in the galaxy; see
http://www.ligo.caltech.edu/~ajw/bursts/GalaxyModel.pdf
- Working on making use of time-dependent calibration info
in burst simulations in datacond; in consultation with Philip,
requested added functionality to datacond.
- Reviewing the tools for running burst DSO's online during S2.
Shawhan:
I have continued to study the use of auxiliary-channel vetoes in the
inspiral upper limit analysis, in particular to evaluate their "safety"
(i.e. confidence that a gravitational wave could not veto itself).
I found that the coupling between AS_Q (the gravitational-wave channel)
and AS_I is much larger than expected, though the degree of coupling
varies significantly over time. This has led us to discard AS_I
as a
veto channel. I have done a fairly thorough study of AS_Q couplings
to REFL_Q and REFL_I, including a survey of various times thoughout
the
S1 run, which constrains the degree of coupling to these channels.
I am proposing to the group to use REFL_I as a veto for H1, with a
high
SNR threshold and a very conservative SNR-ratio requirement, which
still is able to eliminate the occasional H1 glitches which show up
so
clearly in REFL_I.
General Computing (Wallace)
MIT:
(Keith)
-Installed / configured IBM and Dell laptops
-Testing wireless connectivity in XP to Lucent AP-1000 hubs
-Investigating new cite licenses for matlab / mathematica
Livingston:
(Shannon)
-This week has been taken up with the LDAS move to the new building.
We
have all of the equipment moved over there and are bringing things
up
now.
-I am also troubleshooting a problem with one of my edge switches.
I
have 10-15% packet loss to the switch. This is the switch that
LDAS and
general computing will plug into in the new building.
Hanford:
(Christine)
- Started upgrading GC sun computers to Solaris 9 OS.
- Created a new user group for LSC people working on an LDAS/DMT web
page so that they could write files to the apache directories on the
ldas-jobs workstation set up by Greg Mendell.
- Blocked some IP addresses at the router that were trying to hack
into
a Linux/Windows XP laptop owned by a UofO long term visitor.
- Reordered a laptop and desktop from Dell, the original orders placed
over a month ago had gotten lost at Dell.
- Helped a user track down an e-mail problem that ended up being a
corrupt e-mail file on the server. Removed the corrupted file
and the
user's e-mail worked again.
(Larry)
-Contacted John M. and Cullen T. to see where things were with the
WAN
installation and getting the existing connection back to an acceptable
performance level.
John is working on setting up a meeting to go over the new WAN installation.
No reply as of yet on the network performance issue.
CIT:
(Lisa)
- Implemented certificate based relaying on becrux. This is currently
in beta
testing.
- Opened a case with sun regarding upgrade of the Solstice Backup software.
Sun
is currently saying that our support contract does not entitle us to
the
upgrade.
- Replaced a failing hard disk on luna.
- Made changes to the daily/weekly backups to fix some glitches and
add rigel to
the backup scheme.
- Helped a user with some csh questions.
- Fixed some user problems resulting from the home account move to
rigel.
(Mike)
-Loaded a new laptop for Dennis Coyne.
-Swapped out a laptop and hardware for John Zweizig.
-Reloaded two laptops for loaner pool.
-Updated firewall software on all NT servers.
-Added additional security features to all servers.
-M91 was having problems with the real player media server; I ended
up
having to reinstall the software which is now back up and running.
-Reloaded a pc for Hareem Tariq that was infected with a virus plus
had to backup a huge amount of data that was stored on this PC. I am
just
about finished with this reload.
-Had a computer at Wilson House that was infected with a virus, which
required a
reload; plus I found a hardware problem that I corrected.
-Performed a lot of user support this week regarding viruses, software
& network
issues.
(Veronica)
-LIGO website: scheduled a training session at the Digital Media Center
for a trial run of digitizing/compressing a short VHS tape. In addition
to
training, this will provide an example of what would be involved in
processing of existing VHS tapes should we decide to do it in-house.
Obtained a rough cost estimate from DMC for the job.
-Completed, tested, and posted the video/slideshow combo of last LIGO
seminar. That required troubleshooting of the RealMedia server, which
we
did with Mike.
-Updated various webpages throughout the website.
- LSC website: posted a few updates.
- GNATS database: troubleshooting a category that does not pipe incoming
problem reports into a corresponding directory. The directory will
need to
be reconfigured. Provided user support.
- CaJAGWR: posted the updates to the website. Provided administrative
support.
- Started working on the Advanced LIGO proposal.
(Larry)
-Made a number of changes in the computer server room. Mostly rearrangement
of
computers and cables. Moved the users home accounts to another server
and
increased the disk space for the home accounts. Most of the problems
from the
move were stale NFS issues. So far things appear to be running well.
The setting up of new accounts procedure has changed. The new home-account
server is running Solaris9 which is not compatible with the tools we
use for
setting up accounts. Two additional steps now have to take place.
-The purchasing arena has been a busy one. More items for a number
of people.
The big items are the new routers for CIT and Hanford. The CIT router
order is
in place and the Hanford one will be after a few more logistical issues
are
worked out.
A couple of laptops have been ordered. It should be noted that most
people
should expect to use their laptop/workstation for two-three years before
being
eligible for an upgrade. We are getting most of laptops with a three
year
warranty.
-The General Computing Usage policy has been sent out. So far about
45 people
have responded. That with some of the feed back and questions, has
been a
pleasant surprise. We are now working on updating some of the documentation
and
getting web pages setup with more detailed information/instructions
related to
the policy.
-Worked a number of issues getting different users back up and running.
-We now have a site license for Math Type, which
is a equation editor for
Microsoft Word. We have already started distributing
it and will be passing it
along to MIT, Hanford and Livingston.
-The regular of setting up users, blocking bad e-mail locations and
documentation all being done on a daily basis.
-Working on the distribution of the new licensing we have for Matlab.
From: ctorrie <ctorrie@ligo.caltech.edu>
Advanced LIGO Suspensions
Visit
I was visiting the U. of Glasgow from the 13th of December until the
24th of December. I will write a full report on this visit for next week.
Mode Cleaner
Mark Barton has been measuring the pendulum frequencies of the mode
cleaner suspension. In order to compare this to theory it is necessary
to edit the parameter set in the model to be consistent with the actual
suspension.
Therefore I have been calculating the mass and moment of inertias of
the various stages of the assembly using SolidWorks.
Helena and I are working on completing the assembly of the second suspension and hope to have this done by the end of the week.
Workshop have been working on several duplicate parts that are needed for one suspension to go to LASTI.
Cantilever Blades
Eoin Elliffe, Mike Plissi and I met to discuss the modelling and manufacture
of cantilever blades using an ANSYS model written by Eoin. The plan is
to get several prototype blades made using numbers predicted by Eoin's
model.
From: Larry Jones <ljones@ligo.caltech.edu>
Advanced SEI
David Shoemaker raised the question of whether the fallback optic (fused
silica) for the AdvLIGO FM would be a worse interference problem (with
the BSC support tube) than the planned sapphire. It turns out that the
planned optic for the FM is fused silica, with no change for fallback.
This optic is 35 cm dia. X 11.8 cm thick, compared with the 32 cm dia.
X 13 cm thick that was drawn for the interference check. This is
not a major difference; the interference problem remains about the same.
From: Helena Armandula <ahelena@ligo.caltech.edu>
Silicate bonding - SF4 glass
Bonded 8 SF4 substrates to silica substrates. These were 1/2"dia. pieces.
Used a 1:6 sodium silicate solution. The bonds were cured for 36 days
before they were tested.
The bonds did not show signs of stress when viewed under the polariscope.
The first bond was loaded with 16 kg and failed after ~20 minutes.
A second bond loaded with 4.5 kg also failed after a few hours. We are
looking into the problem.
Made 4 more bonds with newly bought sodium silicate solution.
Advanced LIGO Coatings
J.M. Mackowski will coat a 3"dia. x 1"thick substrate with doped tantalum
to compare results with the thin substrate already coated with the same
material. He expects to have the part finished by the end of the month.
From: Bill Kells <kells@ligo.caltech.edu>
Have been preparing to investigate the H1 and/or H2
TL next week at LHO. Besides cooking up specific things
to measure, have devoted much time to reviewing old
simulations (FFT) on this. Working with Erika (now back
stateside) and P. Fritschel (to understand agreement
with his new estimates of AS port detection "efficiency".
Have also been analyzing how the full locking servos
cope with the offset in the l+ servo (due to the TL).
Have been analyzing this with Biplab who has been doing
related things with the e2e. So he is now doing some
pertinant e2e simulations for me.
From: Peter King <pking@ligo.caltech.edu>
2.2 AdvLIGO PSL
===============
I am chasing up the hardware prices for a photodiode
test setup. These
are to be included in the "basis of estimate" costing. In going
through
the costings, I have identified 5 items that, perhaps, ought to be
removed.
These items do not have a large dollar amount associated with them,
so the
impact is minimal, especially when the costs for the photodiode test
setup
are put in.
From: Janeen Romie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Inputing my proposal changes.
Mark and I started pendulum frequency testing last week. An accelerometer
was used first. Now, Mark is using an eddy current sensor with a shaker.
He is working with Calum on checking the parameter set. This week,
the second MC will be moved to another table for structure frequency testing.
We're awaiting cables from Paul Russell for local damping testing, and
hope those will come any day. Mark and I already moved the dSPACE system
over to the Synchrotron. Helena and I glued magnets and dumbbells onto
the two metal masses this week. They are ready to be swapped in tomorrow
morning. Helena has been writing up a preliminary assembly document
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Happy new year to everybody
Charles, Riccardo
More misery on brazing. Now we can wet well MoRuB and Vitralloy, but
having problems with braze surface oxyde.
Alessandro
While writing the paper, made an additional check on the horizontal
accelerometers. Found a stupid limitation in the old accelerometers damping
performance. The wiring was underestimated and was limiting the Q. New
wiring boosted the Q from ten or a few tens to well over 1000 (at <0.5
Hz!) and still rising (presently limited by vacuum in his test setup).
The result is an even improved horizontal accelerometer performance,
now limited by the electronics even with the cheaper aluminium body (the
CuBe is for the moment redundant).
Received the Ultra Sound Milling Machine, Installing in Pisa.
Mike
Finished up cryogenic measurements on sapphire fibers thermal conductivity.
No surface roughness effect found and no effect to be expected unless the
fibers roughness is reduced to less than 4 Angstrom level.
Hareem, Charles
Splatting samples.
For additional information about this report, contact sanders@ligo.caltech.edu