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The LIGO Executive Committee Agenda for Monday December 16, 2002 will be:
CANCELLED DUE TO GWDAW MEETING
no report
LIGO Operations--Administration
There was a site teleconference held on Thursday, December 12, 2002. The following issues were among those discussed:
This is probably the last meeting of the year 2002 unless something pressing comes up. The next meeting is tentatively scheduled for the first week in January.
Hanford Auditorium--Gary met with Tom Lucatorto (NSF) concerning public use of the Hanford Auditorium. Tom has to meet with the appropriate people at NSF.
Cost vs Budget Status--Last year LIGO spent $30.4 million on Operations and Advbanced R&D. The first two months of this year we are spending at a reate of $2.5 million. The FY2003 projection with months that increment up for three pay periods, etc., is $32 million.
We are currently down about 11 people relative to budget.
Civil Construction at Livingston--The construction contract with Brunt has been closed. Need to review the punch list for items where there is potential residual cost exposure and get those items on a contingency liens list. An example is the air handler. There is a design issue that will require mitigation.
Civil Construction at Hanford--Status of the punch list for Hanford Building: the doors represent the only significant punch list item.
Property--Ed is going to Livingston to conduct an property inventory sometime around January 6...depends somewhat on Livingston schedules.
Traffic control systems--Hanford has solicited additional quotes and is proceeding, Livingston has some verbal quotes, but nothing on paper.
Power Costs at Hanford--There will be an 8.3 percent increase in Hanford electric rates starting January 1, 2002. This was just approved by the Washington State Public Utilities Commission. Hanford needs to review how much of this, if any, has been budgeted.
The list of current actions revised to reflect
the status of open actions assigned through December 12, 2002 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
ACTIVITY
| For Week Ending
12/12/02 |
Packages | Faxes |
| In | 36 | 30 |
| Out | 11 | 19 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
The contract with Brunt Construction for the Livingston Staging Building has finally been closed. The auditorium floor has been accepted, and a smaller pulley has been installed on the HVAC to reduce noise. Ed Jasnow handed the retention check of $112,000 to Michael Ragusa, president of Brunt, to officially end the contract.
Although the installation of the smaller pulley reduced the HVAC noise somewhat, it is still quite loud in the high bay area. This is because the design has the blower right behind the return grille. Although the noise level is within acceptable limits, a study of a possible re-design will be performed.
Chervenell Construction will be given a change order on the Hanford Laboratory Building. This will be for extension of the sunshade and installation of a second set of glass doors in the front.
OPERATIONS:
We have received notice from the Benton County Public Utilitiy Disrict that electricity rates at Hanford will be increased by 8.3% beginning January 1, 2003. This increase was just approved by the State of Washington.
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Weekly Advanced LIGO Project Controls meeting was not held this week.
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 annual report is due to be submitted to the NSF at the end of December, covering activities from December 2001 through November 30, 2002. This Annual Report is required for the old (Construction Funds) Cooperative Agreement, and the focus is the end of Construction, Installation, and Commissioning, not Scientific Results. Instructions given during the Executive Committee Meeting Monday to make it short were a welcome simplification, ans a first draft is nearly ready.
Meanwhile, to support the proposal early next year for a LIGO upgrade,
we will be preparing an update to the Annual Report for Operations that
was submitted to the NSF in September.
There are currently no open change requests to be considered
by the LIGO Chnage Control Board, and there were no change requests addressed
during the Executive Committee Meeting on Monday, December 9, 2002.
We have requested Hanford to submit a change request to cover the costs
to complete the building construction effort there.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Coordinated a meeting with personnel from Caltech Safety and LIGO LSO to clarify LIGO baseline eye exam protocols. After some discussion, it was agreed that LIGO should consider revising the LIGO Laser Safety Program using, as a guideline, the recommendations of the ANSI for Safe Use of Lasers in Educational Institutions, ANSI Z136.5-2000. Therefore, Ocular Fundus examinations will not be administered unless requested by medical personnel when ocular function is found to be not normal during the baseline or terminal ocular examinations. Revision/markup of the LIGO Laser Safety Program document to incorporate the educational institution ANSI guidelines is in work.
A team comprised of Caltech and LIGO safety personnel have nearly completed
a laser inventory and safety inspection of LIGO campus facilities.
Only Wilson House and the 40M facility remain to be inspected at this
time. A report with recommendations and Action Items will be issued
shortly.
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by F. Raab)
-------------------------------------------------------------------------------------
(see ilog for details - if it's not in the ilog, it didn't happen...)
A lot of work was fixing old problems and continuing installation and
check-out of WFS for H1. The most significant result was the convergence
of Bill Kell's long and difficult effort to characterize optical losses
in the two interferometers.
2K IFO (H2)
-----------
The optical loss investigation occupied most
of the time on this interferometer. H2 has always been anomalous in its
optical behavior. It has never gotten the very high recycling boosts in
arm powers that we routinely achieve in L1 and H1. The problem with the
arm loss measurements is that all information affects a ~2% change in light
level reflected from arms and systematic effects can easily swamp this.
Bill feels he now has confidence and repeatibility in making these measurements.
His surprising conclusion is that the arm losses are well within spec,
but there is a 6% round trip loss for light in the x leg of the Michelson
in H2 (BS->FMX->ITMX and back). Effort to try to pin down the origin is
ongoing. The numbers explain fairly closely the limited boost from recycled
operation.
(GHS note: Hurrah for Bill and
his insight and persistence ! )
In other work, on-board 5V regulators have been retrofitted on all boards
in both interferometers where the 5V supply is divided for setting gains.
Previously drifts in the 5V supply had been generating indeterminate gain
states, which should now be a thing of the past. A number of changes were
made to the MC servo board to mitigate saturation and slew-rate issues.
The dewhitening filters for PRC-related optics were reworked, resulting
in more quiet operation of this loop.
4K IFO (H1)
-----------
The optical loss investigation shows that
this interferometer is within spec and the recycling boost estimated from
the measured optical values agrees quite closely with experience.
ISCT1 was worked extensively to relieve potential clipping problems (better
beam reduction and a careful realignment) and prepare for higher power
operation. A script was generated that allowed automatically measuring
the unity-gain frequency of the DARM loop at regular intervals to better
understand how this drifts. Some drift is expected due to varying sideband
power in the recycling cavity, but an additional 15% drift was unaccounted
for in the overall (factor of 2-ish) drift overnight. Might be that drift
of the sideband spatial overlap with carrier is implicated. Hardware for
WFS 3 and 4 was installed and checked/tuned with AM laser.
Detector Commissioning: I have been learning how to use E2E/SimLIGO for WFS modeling. With the help from Hiro and Matt I was able to run the recent version of E2E/LIGO at LLO. The code is setup to run for LHO now. I am in the process of making changes for LLO. I have also set up the beam scanner to make beam parameter measurements on the reflected port, but have not been able to make measurements yet. This is a part of the WFS investigation. (Valera Frolov)
LDAS administration:
1) made and distributed for review and comments floor plan for the
new
LDAS room;
2) restoring LHO's RDS;
3) together with Erik working on proposal to replicate and distribute
AS_Q only RDS in real time;
4) sent 2 M1 tapes to Caltech;
5) ordered Solaris 9 media.
LDAS data analysis
1) debugging waveburst DSO
(Igor)
CDS: Updating the very essential and much needed Red Book. Received the DVD Robot and the two disk arrays this week. These will be installed some time soon. Working with Rolf on getting the ASC processor code installation sorted out. Working with DTT to identify bugs and fixes. Disk backup for the DTT directory inplace. Installed new versions Tcl, Tk and expect. Cleaned out the master.config file and removed all bad channels identified by Orlando. Identified causes for three missing data segments in S1 data emailed by Peter Shawhan and Bruce Allen, to reboots of Frame builder and DAQ. Three more missing data segments - a mystery. (Chethan)
HEPI / LASTI The last two (of 10) welded actuators has shipped to MIT this morning. We also completed the mounts for the L4Cs and sent the set, along with mounting hardware yesterday. Marcel has completed submitting the as-built drawings for the actuator, as well and many incidental fixtures to the DCC. (Hammond, Kern)
ETF / Advanced LIGO pod bases: Harry and Harry disassembled the GS-13s and we shipped the cans off to a machine shop in Lafayette in order to have the 'bomb proof' coating machined off. This is after a wasted week's work trying to use paint removers and bead blasting. (Traylor, Overmeyer, Hammond, Kern)
GC: We are in the process of upgrading our Matlab and Mathematica licenses
to the current versions. We have ordered a ledger-size InkJet printer so
we can print B-size color drawings. We are getting close to moving into
our new building, and Shannon has been working on the logistics of moving
servers, clients, and associated hardware. (Evans)
Jonathan Kern,
Marcel Hammond
The last two
(of 10) welded actuators has shipped to MIT this morning.
We also completed
the mounts for the L4Cs and sent the set, along with
mounting hardware
yesterday. Marcel has completed submitting the
as-built drawings
for the actuator, as well as many incidental fixtures
to the DCC.
This week
I have tagged version 2.4.0 of the DMT and installed this code
on all the
DMT nodes at both observatories. This version uses
FramCPP-5.20.0
which reads and writes format 6 frames. The early
introduction
of this code will allow us to discover and fix any problems
before E9/S2.
It now appears to be running sufficiently stably that it can
be used in the M2run at LHO this Saturday (Dec. 14).
- The latest
version of dataviewer, using xmgrace, seems to be running fine at
Hanford now.
Hongyu is working on adding a trigger capability for trend
playbacks.
- Alex has
fully ported the EPICS IOC code to a Sun Workstation.This
is being
tested by
running the digital suspension EPICS code at the 40m lab on a Sun
instead of
the usual VME based Pentium.This
new port to Sun may then also
allow DMT
programs to directly output all or some of their data directly as
EPICS records
(Barker is checking with a few DMT authors to try this).
Advantages
of this are display of DMT data directly on control screens and data
acquisition
via the EDCU.
- Code for
40m lab digital suspensions is ready to go. Last bug (hopefully) was
that excitation
signals did not work, but that was resolved Monday.Once
the
new Pentek
modules are installed (probably tomorrow), we should be ready to go.
- Have been
working with Rana on various filter switching schemes to get the
Run/Acquire
to switch without kicking the IFO out of lock.I
had to make some
changes to
the standard digital filter code for the most recent change.This
code was downloaded
to LLO today for Rana to try.
- Lori has begun work on making the changes requested for the ASC software.
1.Shipped
the pump servo, cables and documentation to Mike Zucker
2.Flavio
is closing the loop on the ISS with the laser power adjustment actuators
supplied with the laser power supply to increase the dynamic range.
3.Mohana
has been supporting the seismic pre-isolator by trouble shooting her rack
mounted seismic interface box.She
has shipped it to MIT for HEPI installation
Mohana Mageswaran
I have tested
and shipped two Photo Diode DC Drivers to Hanford yesterday, and I will
be shipping two more chassis to Livingston next week. I sent a Seismic
Interface chassis to MIT this week, and I worked on the DCN and will be
sending it to the DCC.
I have sent out the 4 pulse daughter board to the PCB express and I will be working on its DCN.
Jay Heefner
Pentek ADCs
and DACs
- Lori and
I have started to test and document all the noise characteristics and peculiarities
of the pentek ADCs and DACs. This includes input and output noise using
pentek polling, timing module polling and interrupts. We are also looking
at the glitches that occur on the DAC channel 5 and 6 outputs. All of the
results will be summarized in a technical note and distributed for comment,
etc. Hopefully we can get the note out in the next two weeks.
Protel
- CDS is evaluating
Protel DXP. So far it looks as if we can migrate from out current Protel
98 version with relatively little pain. This new version has many desirable
features including an integrated simulator, support for FPGA designs, ECO
generation and version tracking, and multi-channel design capabilities.
Sander Liu
Working on the micro-seismic pre-isolation requirement document.
I drew up
the schematic for a low-noise amplifier to be used for VCO
phase noise
measurements.As a check I breadboarded
a discrete amplifier.
The noise
performance was awful but that would be rectified by use of a
better transistor, I believe.The board layout has been started.
At LLO, we
installed a phase camera which is a special configuration of
the sideband
camera without a second laser, and obtained some meaningful
images of
the phase and amplitude of the laser beam which the wavefront
sensors actually
detect. This week Go and Dave will use Ryan's galvos to
take the last
data for publication. Go is planning to use the sideband
camera's optics and electronics for a squeezing experiment.
Phase Camera
at LLO (Dave O, Andri, Gabby, Nergis, Go, Valerov)
After installing
the phase camera two weeks ago at LLO, last week we were
able to obtain
data that made some sense. The conclusions were:
1. In a nominally
aligned state a significant amount of asymetric RF is
observed in
the pattern seen in POY_I and POY_Q. This can appear as a
significantly
center offsett, disk of RF.
2. By using
the phase camera as a monitor and realigning the BS POY_Q
pattern can
be turned to a bullseye pattern. By aligning POY_I the RF
pattern can
be turned to a bullseye pattern. Both bullseye patterns are
centered on
the carrier.
As
this appears to be a useful alignment tool, a sideband camera will be
made
for each of the sites.
I have been
working on a couple of papers by embedding the comments I have been
receiving
in the last few days. In the meantime I discussed with Garilynn on the
joint presentation
for the Aspen Conference and I made some simulations for the
configuration
corresponding to the interferometer in Louisiana using the values
found on Garilynn's
web page for the radii of curvature of the mirrors, but with
no curvature
on the beamsplitter. The FFT-code and Melody give different results
for the sidebands
when 66 modes are used in Melody while there is no difference
for the carrier.
Such difference is larger than I expected and I will spend some
time to investigate
better what the problem is comparing these new results with
the ones I
got for the validation of Melody and which are included in the paper
Ray Beausoleil has submitted last week with a few requested minor modifications.
OTF Lab.
(W. Bridge)
Contamination
Cavity # 1
Cavity with
test sample aquamill is in progress and taking measurements every day.
for absorption,
ringdown and cavity thermal lensing measurements.
Scatterometer
Scatterometer
recovering is taking place slowly.
New OTF
Lab at Lauritsen ROOM 38
Cavity #3
Reference Cavity it is pumping down.
with new cleaned
mirrors ~70ppm each(Flat & Curve).
Taking measurements
every day.
Cavity #2
Test cavity
In this cavity,
we took the dirty mirrors out and installed a new cleaned mirrors ~ 70ppm
each.
The chamber
is pumping and we are taking RGA measurements.
New chamber
modification is in progress ( solder a new base and make base insulator)
We had safety
inspection review on all the OTF labs and need to comply with some safety
issues.
Doug Cook
from LHO is here this week to support earthquake stop testing. We have
a number of prototypes to test. The SOS is assembled and in the OTF. The
vacuum chamber is pumping. Paul Russell is making cables for the feedthrus.
Doug has brought along with him a hand-held electrometer. However, it is
not meant for in-vacuum use. He's talking to the vendor now to find out
if leads can me made for it or if another unit needs to be used.
no report
no report
SIMULATION AND MODELING (Biplab Bhawal)
E2E @ LLO
---------
(Hiro) Implemented the latest e2e stuff at LLO, and explained the
basics of e2e to Valera Frolov
SimLIGO
-------
(Matt) Added the lock-acquisition code to SimLIGO. Also included
pre-arranged measurement scripts for measuring the WFS sensing
matrix and the lock-acquisition gain ratios.
Common mode servo & recycling summation cavity
----------------------------------------------
(Hiro) Worked on the formulation and implementation of an accurate
summation cavity for scalar field for the implementation of
the
common mode servo.
Misalignment calculations
-------------------------
(Biplab, Hiro) Worked on the proper formulation and implementation
of reflection matrix with tilt.
Alfi
----
(Bruce)
- Alfi5 is now distributed as a separate package by one tarbal.
This makes it possible to distribute Alfi5 more
timely.
- Worked on implementation of dynamic redefinition of E2E_Path
by user (PR 359). In the process, I fixed
some event processing
inconsistencies which may have later caused problems
and would
be (were!) difficult to track down.
(Melody)
- Continued optimization work on the modeler.
LIGO DATA ANALYSIS SYSTEM
LDAS SOFTWARE SYSTEMS (Kent Blackburn)
Port to new GCC 3.2.1 Compiler (Kent Blackburn)
We continued our efforts to port LDAS to use the new GCC 3.2.1 compiler
this week. At present the Red Hat Linux 7.3 port is looking very good,
having successfully tested many DMT, dataPipeline and database functions.
In fact, there is about a 10 to 20% speed improvement without fully
optimizing the code.
The port to the Solaris operating system has been much more problematic.
We are able to compile the code now. However, the compiler itself will
coredump if full optimization is turned on for Solaris. In addition,
we
have combined the long awaited upgrade to Solaris 9 with this port
of
LDAS to the new GCC 3.2.1 compiler. There is a bad interaction with
the
Solaris 9 distributed SSH and LDAS which we are close to solving. But
we
have had only very limited success so far with running the full LDAS
system based on this new compiler with Solaris 9. We are, however,
fully
committed to the port and expect to stabilize significantly by tomorrow.
One of the most exciting aspects of the new port to the GCC 3.2.1 is
that
we have noticed a significant improvement in our memory leak problems
that
we have been working on for years. It looks like 95% plus of the memory
leak in the dataConditionAPI has been removed by this migration and
that
the frameAPI is leaking one fifth as much as with the old GCC 2.95.3
compiler.
We do not have any data on the reliability of threads yet. However,
that
was a major theme in the advertising for this new GCC compiler.
We are still struggling with some issues with compiling LAL and LALwrapper
using this new compiler. We have also come across some issues with
using
this compiler with the newest LAM MPI library which we are still sorting
out. I estimate that we have put in close to two man months on this
port
with a few more man weeks of effort needed before it all settles down.
DataConditionAPI (Philip Charlton)
* convolution function using the same conventions as Matlab.
Useful for (among other things) multiplication of polynomials.
* obtaining the coefficients of a polynomial from its (complex)
roots. Will be used to convert a transfer function in ZPG representation
to IIR filter coefficients.
* functions for "cloning" a real UDT to its complex equivalent.
* Ed found that the test code for windowing was using a tremendous amount
of memory and being very slow. This was because of much
allocating/deallocating memory to check exception behaviour
on too-large
input. I've modified the code to make it less thrashy.
* Met with Alan Weinstein for about an hour. He wants to use a
frequency-domain transfer function to convert a burst waveform
from strain
to voltage for injection. The basic method is to Fourier transform
the
burst waveform and multiply it by the (suitably padded) transfer
problem.
For an arbitrary time-series and transform function, issues
with the
general problem are:
- often the transfer functions are given as a function of log(frequency)
rather than linearly
- frequency spacing must be the same for the transfer function
and
Fourier transform of the time-series. Transfer function
may need to be
interpolated (our current interpolation is of a
different sort
than that required for general interpolation).
- Transfer function may need to be extrapolated into regions
where it is
not given (probably setting to zero is fine)
Some of this can be done already in the datacon for specific cases,
although I think the general problem may not be doable. Would be more
convenient to wrap this up in action "molecule".
Database (Peter Shawhan)
Created new database tables submitted by Igor Yakushin to store output
from
the new WaveBurst search code, plus tables to store generic information
about
simulations.
Worked with John Z. to iron out some problems with the ingestion of
DMT
info into the database at Hanford. They are due to the software
starting up
slowly, which seems to be caused by a long delay in connecting to the
LDAS
web server at Caltech.
Corrected problems with documentation for setting up the IBM database
on a
single box LDAS system.
LDAS HARDWARE SYSTEMS (Stuart Anderson)
CALTECH (Dan Kozak)
* Continuing to synchronize files on HPSS/SAM-QFS/IDE-RAID. This
has led
to investigating a problem getting files from HPSS using hsi
on ldas-archive.
* Qlogic HBA problem has been escalated, but still no results.
* Request for SAM-QFS 4.0 evaluation copy sent off to Sun.
* Called STK vis a vis upgrading 9940A to 9940B. Haven't heard
back.
* Working on Solaris 9 sendmail.cf configuration.
(Al Wilson)
* New release of BB out. Compiling for Solaris and Linux.
* Finished the last of the Linux desktops machines on the 6th floor
Millikan.
* Setting up 2TB IDE-RAID box datacache9.
* Did some housekeeping in 215 Synchrotron. Installed the dust mat.
(Stuart Anderson)
* Upgraded LDAS-DEV Sun servers to Solaris 9.
* Helped Ed Maros rebuild the /ldcg software tools with the new
gcc-3.2.1 compiler for both Solaris and Linux.
* Switched all 6th floor Millikan Linux machines to use the new
gcc-3.2.1 built /ldcg for standard software tools.
* Upgraded desktop machine to RedHat 8.0 for early testing. LDAS will
almost certainly not upgrade to 8.0 but will eventually upgrade
to
8.x or 9.
MIT (Keith Bayer)
* Continuing to spec hardware for pentium cluster machine.
* Put ldas Solaris machines on ScholarPak to facilitate upgrade to 9.
LIVINGSTON (Igor Yakushin)
* Made and distributed for review and comments floor plan for the new
LDAS
room;
* Restoring LHO's RDS;
* Together with Erik working on proposal to replicate and distribute
AS_Q only RDS in real time;
* Sent 2 M1 tapes to Caltech;
* Ordered Solaris 9 media.
HANFORD (Greg Mendell)
* I've ordered a replacement disk for the ldas-jobs box and linuxbox1,
plus a couple of spare 20 GB IDE hard drives (on the todo list
for long
time). Also ordered IDE cables to try to fix node32, the
one remaining
beowulf node that is not working.
* Worked out a backup plan to write S2 data to tape using AIT-2 tapes;
worked with LDAS on general issues of raw and RDS data management
during S2.
* Performed the usual service tasks of assisting users of LDAS and
keeping data available at LHO.
DATA ANALYSIS ACTIVITIES (Kent Blackburn)
CALTECH (Alan Weinstein)
- Wrote report on burst group efficiency simulations, with Laura.
- Working with Philip Charlton on making use of time-dependent
calibration info in datacond.
- Collecting code and documentation for burst group CVS archive.
- Marvelled at high quality of all the LSC upper limits telecons.
(Peter Shawhan)
* Spent the weekend in Baton Rouge working with other members of the
Inspiral
Group to finalize the upper limit analysis for binary neutron
stars in the
S1 data. Also helped prepare and give the presentation
to the LSC.
* Working on addressing Stan's and Daniel's concerns about using auxiliary
interferometer channels as vetoes.
HANFORD (Greg Mendell)
1) The main activity of the last week was to run driver scripts that
ran
the knownpulsardemod DSO (off and on) between Dec 4 2002 and Dec 6
2002,
regenerating SFTs for PULG at LHO and LLO using LDAS 0.5.0. Everything
went very well, with almost no errors except due to missing data.
LDAS
ran great! At LHO 1431 jobs were run; 20 jobs failed. All
the failure
were due to missing data on the disks. No failures were due to
LDAS!
The SFT jobs input 2048 s of data. The mean time to run the jobs
was 86
seconds, or 23.8x real time. This is 33% improvement in performance
from LDAS 0.4.0!. At LHO 691 jobs were run; 20 jobs also failed.
Of the
failures, 14 were due to missing data on the disks, and 6 were due
to
network problems. The latter jobs were rerun and they suceeded
on the
second try. The SFT jobs input 2048 s of data. The mean time
to run the
jobs was 107 seconds (which includes the time to transfer a small frame
file from LHO to LLO per job), or 19.1x real time. This is still a
15%
improvement in performance from LDAS 0.4.0!
2) Otherwise I am working PULG group as part of their effort to place
upper limits on known pulsars. I have updated some preliminary
results
I previously gave to this group, using the knownpulsardemod DSO under
LDAS 0.5.0 with the regenerated SFTs desribed above.
LIVINGSTON (Igor Yakushin)
* Debugged waveburst search code DSO.
GENERAL COMPUTING (Larry Wallace)
MIT:
(Keith)
-unmirrored NIS+ server due to failed hdd
-investigated port problem on NW22 switch affecting several Sun boxes
-moving old users onto secondary disk partitions
-investigating sw monitor idea for dhs
-received / installed backup hdd for laptop
Livingston:
(Tom)
- We are in the process of upgrading our Matlab and Mathematica
licenses to the current versions.
- Ordered a ledger-size InkJet printer so we can print
B-size color drawings.
- We are getting close to moving into our new building, and Shannon
has been working on the logistics of moving servers, clients,
and
associated hardware.
(Larry)
- Shannon and Larry have started looking into other methods for getting
more bandwidth to the Observatory. Presently, there don't appear
to be
any low cost solutions.
- Caltech has made several requests from different ISP's to locate someone
that has a virus which is spamming forged mail. There appears
to have been
some success in that the amount of forged mail has diminished.
Hanford:
(Christine)
- Installed the replaced exabyte tape drive. Restarted the daily
backups to tape.
- Purchased and downloaded the latest Eudora e-mail software.
Made the
software available at our standard PC apps site and wrote installation
instructions.
- Set up two new PCs with our standard software and moved user files
from old PCs to the new ones.
- Evaluating network monitoring software to replace our old Network
Analyzer software.
- Most of this week spent as my alter ego doing CDS vacuum control
software enhancements.
CIT:
(Mike)
- Going over security logs due to unknown users trying to log into
servers.
So far everything seems to be okay. The firewall software we
loaded seems
to be working pretty darn well; we are still getting a lot of
attempts with
unknown users trying to login, but for the most part this type
of activity
has really cut down.
- Finished up loading 2000 server that is hosting the Project Science
website.
- Added the amaldi99 webpage back on to this server. This still needs
some
fine-tuning with .asp files.
- Loaded another 1U-Server running 2000 server to transfer the real
media
server to host all real media, which is currently running on
NTSRV 4.0 and
is having problems.
I still have a lot of work ahead of me to finish up this server.
- DCC, I had to work on access database to trouble shoot a few issues
we were
having. I had to compact and repair database plus run the Time
Target
scripts manually.
- Looking over Pictor, this server to be upgraded to 2000 server. This
is
currently running on NTSRV 4.0 but is according to the logs
this server is
reporting a lot of OS errors that requires a lot of work. This
server is
still moving right along considering the state it is in.
- Loaded two laptops for the loaner pool that included reloading the
OS and
all General Computing software.
- Finished up loading two Dell computers for Sander Liu and Mohana.
This
included loading OS, General Computing software and transferring
users data
to new computer. I have swapped out Sander Liu, but I still
have more work
to do on Mohana's new computer and should have her swapped out
later on
today. I have brought back these users old systems to my office
for
upgrades and reloads.
(Lisa)
- Installed sendmail 8.12.6 on acrux.
- Generated a new root certificate for the certificate authority on
becrux to
resolve a problem from when I first set it up. Re-issued
server certs for
becrux and acrux. Tested the new certs with apache and
starttls.
- Resolved the remaining problems with starttls pop/imap on becrux.
Am now
working on documenting the client setups to use these services.
- Put in a work around on both acrux and becrux that enables eudora
to properly
use smtp starttls.
- Disabled the autolock service and upgraded the ram on lionking. This
box is
still having performance issues that are probably partially
related to the
network.
- Installed a new power supply in the wireless AP in the 40meter.
Currently
trying to get the part RMA'd.
- Worked with Irena on how to maintain the lsc and ligo1 mailing lists.
(Veronica)
- LIGO website:
LIGO has a number of analog videotapes, some of which (or all)
may be
posted online. These tapes (preferably all of them) need to
be digitised
for posting, as well as for archiving. Prepared a summary and
cost
estimate for Project Office on setting up an in-house system
for
digitising vs hiring an outside contractor. Working with Caltech
Digital
Media Center on this order.
Added a new section to the 'News and Highlights' webpage that
points to
PAC, LSC Transparencies and to NSF Reviews pages.
Posted updates to various parts of LIGO website (Aspen 2003
Winter
Conference, Fellowships, LIGO Conferences). Updated the Publications
database.
- Attended a seminar on adding multimedia to PowerPoint presentations.
Learning SMIL.
- GNATS dabatase: administration and user support.
(Larry)
- Working on the purchase of the new GigE router. Finally, was able
to get in
contact with our CISCO rep. and received some preliminary quotes.
The 7513
unit appears to be the best bang for the buck. There are some
cheaper models
but they don't perform at wire speed. We should be placing the
order next
week once we get the logistics worked out with Campus. Also,
working with
Christine in getting the same unit for the Hanford Observatory.
- Worked a number of SUN issues. One of the SUN880 units shutdown for
some
unknown reason. I've replaced the UPS to that unit since the
UPS it was
connected to appears to have some problems. Presently, building
a new
SUNblade with a few new options. So far the unit looks to be
pretty stable.
- Spent time monitoring the main network connection to Campus. There
appears to
be a conflict in the communication between the CISCO and the
Foundry edge
switch. At half duplex we get good performance but a lot of
collision errors
at full duplex we get poor performance but no more collision
errors. I'm
presently working with the Foundry rep. to try and figure a
fix.
- Spent time working a number of DCC issues. Between the new items
required of
them and other document related issues it has been resolved
that there will
be a new server built to handle temporary secure web access
to documents
that are in transition. The logistics of this are still being
worked on.
- Working on a number of documents. The LIGO Computer Usage policy
is now out
and we will soon be sending out a notice for everyone to read
it.
http://www.ligo.caltech.edu/docs/M/M020105-00/
- Worked a number of virus, spam and hack issues. We will have to put
out more
instructions to the users on how to deal with this. We have
had people forward
infected e-mail to a large group, informing them that it was
infected, when it
should only be sent to the local system administrator.
- Worked on a couple of mailing list problems. Still have a few more
groups to
work out.
From Benno Willke:
LSC LASERS WORKING GROUP
Minutes of telecon Dec 5 th 2002
LZH
- still problem with higher order modes in ring resonator (can not get
M 2 <2 for 95W beam
- they think the thermal lens in the quarz rotator causes a problem
(stability range of
oscillator showed dependence on position of quarz rotator) an plan
to move rotator to a
position with less intensity
Stanford
- second edge pump slab broke ( Spectralon caught fire and when diodes
were turned of
after a couple of seconds the slab was broken)
- due to this second accident all Spectralon parts will be replaced
in the future by Al pieces
- damage on slab (crack close to the end) can be repaired in local
crystal shop by cutting it
4mm shorter (one zig-zig less)
- inspection showed that the original slab was a quater of a zig-zag
to short which might
explain the changing slope when increasing the pump power that was
measured earlier
(aperture effect due to the not completed last zig-zag)
- end-pumped slabs were coated by MLD and are currently at a local
vendor for final
dicing
- as soon as final slabs for end-pumping are back (15.12.02 expected
delivery) the end-pumped
experiments can start (LaserLine pump diodes are ready and run ok at
the 125W
level)
Florida
- waiting to get FK51 AR coated
- continuing experiments with index matching fluid
Adelaide
- new slabs arrived, have extremely high material and machining quality
- laser head is assembled, lasing experiments will start in a few days
- LZH fibres arrived, new waveguide to match the 800um fibres are on
order
- 10W laser does not need to go to TAMA before middle of next year
(so that this laser can
be used as front end for injection locking if NPRO as a front end does
not give a big
enough locking range)
high power stage decision
- suggested times to do the measurements fit with the schedule of all
groups
LZH: Feb. 24 - Feb. 28
Adelaide: Mar. 3 - Mar. 7
Stanford: Mar. 10 - Mar 14
next conference call: January 9 th (one week later than usual due to
new
years break)
-----------------------------
ETF / Advanced LIGO pod bases
Traylor, Overmeyer, Hammond, Kern
Gary and Harry disassembled the GS-13s and we shipped the cans off
to a
machine shop in Lafayette in order to have the 'bomb proof' coating
machined off. This is after a wasted week's work trying to use
paint
removers and bead blasting.
-----------------------------
From: "Mark Barton" <mbarton@ligo.caltech.edu>
This week was mostly preparations for Doug Cook's
visit and the
experiment for the testing of earthquake stops. I also did a calculation
for Phil on the expected response of the advanced LIGO mode-cleaner
to
pitch and yaw actuation on the intermediate mass.
From: Jay Heefner <jay@ligo.caltech.edu>
Adv LIGO Suspensions
============================================
- Electronics modules for the CIT and LASTI prototypes are fabricated
and some have been tested. We are making progress, but initial LIGO work
has made oit slower than expected. We hope to complete the installation
and wiring by 12/20.
--
From: Michael Smith <smith@ligo.caltech.edu>
40 METER IFO
OPTICS PARTS LIST
Received parts:
3 PZT tilt platforms and 1 servo control drive electronics and strain
gauge read-out electronics from Piezosystems Jena.
Orders pending:
3 each, 1in mirror mounts are pending from Newport; input mode-matching
telescope off-axis parabolic mirrors are pending from SORL; Faraday rotator
from EOT; . The half-wave plates from KLC, for the Faraday isolator, are
being re-worked to vacuum-compatibility standards.
Only one set of servo controlled drive electronics to drive the x and
y axes of the two PZT vacuum IFO steering mirrors was inadvertently ordered.
A second set will be ordered.
Part numbers were scribed and the in-vacuum mirrors and beam splitters are being cleaned and baked.
FARADAY ISOLATOR
Faraday Isolator mechanical parts and polarizing prisms for Faraday
isolator have been cleaned and baked, and are awaiting assembly.
IFO MODE-MATCHING TELESCOPE
Telescope mechanical parts are in process of being fabricated.
OPTICAL LEVER
Working drawings for magnified focus lens are almost complete.
LIGO
ERRANT LASER BEAMS
An analysis of the ASAP results and a final report are still pending.
From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>
I have visited ASML, formerly part of Tinsley. They are capable of doing the "Mexican Hat" shaping. They don't have much experience with sapphire, but believe there will be minimal problems. Their figure metrology is comparable to the metrology at Caltech. They also have the capability of measuring "micro-roughness." They are interested in looking into homogeneity compensating polish as well, their specialty is aspheric optics for use in microlithography.
I plan to visit Kodak (Rochester in January... cool!) with Kathy Creath to assess their capability for polishing "Mexican Hat" surfaces as well.
Worth noting here for completeness: JMM at Lyon has said that he could do the "Mexican Hat" surface today using corrective coating.
Gin Gin optics are back from polishing and are awaiting coating.
Chandra Khattak reports to Jim Hough (copied to GB) on edge polishing
of the large sapphire piece for Glasgow:
"An interesting observation was that there are two poorly polished
sections along the entire length of the cylinder. These sections
are on opposite sides, approximately 0.88" wide and about 49 degrees off
the c-axis. It appears to be a crystallographic phenomenon
which currently I do not understand. I wanted you to be aware of
this observation and have also informed GariLynn. As I mentioned
to John this area is not a "weakness" but like a "hard spot" in polishing.
I do not see any difference except that in this area the transmission is
not as good."
Note that this is the first occurrence of this phenomenon we have seen.
We have at least 16 sapphire optics where the OD has polished beautifully.
From: Peter King <pking@ligo.caltech.edu>
2.2 AdvLIGO PSL
I have been going through the costings for the PSL,
with an eye on the
laser costings and the cost of the intensity stabilization task.
A request
was put into Coherent Laser for an update of their previous quotation
for
laser pump diodes, in order to gain an idea of how the price changes
over time. This would be factored into the "basis of estimate"
for the
laser costing.
From: Phil Willems <willems@ligo.caltech.edu>
Sapphire Q:
-----------
We tried a two-wire 'hammock' suspension for the sapphire to see if
we could
measure high Q's using it. We could not. If we could, it
would have simplified
the installation of the 40kg sapphires from what is needed for a single
wire
loop. So, we are now preparing a single wire loop suspension.
(w/ Dan Busby)
Thermorefractive noise:
-----------------------
We have identified electrocaloric dissipation as the loss mechanism
related to
thermorefractive noise by the fluctuation-dissipation theorem.
Simply put, the
free energy of a dielectric has a term proportional to the permittivity
and to
the square of the applied electric field. Because the permittivity
depends on
temperature, changes in the applied field cause temperature changes
in the
dielectric, and thus heat flow and dissipation. Calculations
of the
thermorefractive noise based upon this loss mechanism are in agreement
with
those of Braginsky et al. (w/ Sergey Vyatchanin and Misha Gorodetsky)
From: ctorrie <ctorrie@ligo.caltech.edu>
Advanced LIGO Suspensions
Mode Cleaner
Janeen and I have spent some time going over the various aspects of
the suspensions with Doug Cook, who is visiting from Hanford.
Janeen, Doug and I have switched out the initial catcher and have installed
the earthquake stops for the aluminium intermediate and test mass.
SolidWorks
ADVANCED LIGO Bill of Materials for an Assembly drawing.
The Excel BOM works for the following conditions: -
· All parts must be saved
as DCC#_Name. e.g. D020445_BladeClamp
· The same BOM can be used
to supply individual Bill of Materials and an overall Bill of Materials
and an automatic Drawing Tree. (It is necessary to change the properties
of the BOM for each different case!)
· Bolts and Washers will
be referenced from the Customised Toolbox library, see below.
· Alternate and Referenced
parts must be pre-defined using File/properties/custom.
CUSTOMISED TOOLBOX LIBRARY
The following parts have been created, allowing easier sharing of assemblies
between external collaborators.
SST_Socketheadcapscrew.SLDPRT
Ag-SST_Socketheadcapscrew.SLDPRT
NAS 620 FLAT WASHERS.SLDPRT
SST_HexNut.SLDPRT
SST_setscrew.SLDPRT
Interlocking_Test_Weights.SLDPRT
These are available at the following location: -
http://www.ligo.caltech.edu/~ctorrie/documents+downloads/documents.html
Visit to Glasgow
I am visiting IGR at the University of Glasgow from the 13th until
the 23rd of December, I leave tomorrow. I will be back in my office at
Caltech on the 3rd of January. I will be available on email contact at
my usual address.
From: Janeen Romie <romie_j@ligo.caltech.edu>
LIGO 1
Doug Cook from LHO is here this week to support earthquake stop testing.
We have a number of prototypes to test. The SOS is assembled and in the
OTF. The vacuum chamber is pumping. Paul Russell is making cables for the
feedthrus. Doug has brought along with him an hand-held electrometer. However,
it is not meant for in-vacuum use. He's talking to the vendor now to find
out if leads can me made for it or if another unit needs to be used.
GinGin
Working on the magnet standoff assembly. With the repreive in schedule,
the ITM drawings do not need to get to the machine shop until Jan 2nd,
however, I'll try to get them to CES by the end of this week to allow for
holiday vacations.
AdLIGO Suspensions
Calum reviewed the mode cleaner triple suspensions with Doug, who is
providing input for the installation fixtures for these suspensions. He
is working with Calum and I this week assembling the earthquake stop components.
Doug is getting pushers from the Hanford site for us to test pushing the mode cleaner suspensions around the optical table. It is our assumption at this point that a number of LIGO 1 HAM installation fixtures will be usable for the LASTI. We will be designing some interface fixtures.
We're still waiting for the two sets of digital electronics from our electronics group. With Paul Russell out, Jay is getting someone else to make cables and electronics boxes for the mode cleaners. GEO has already delivered one set of analog electronics. Caroline Cantley reported that they've had a delay in their electronics deliveries as one of their vendors has gone into foreclosure. She'll forward our proposed delivery of mid-January for the second set of mode cleaner analog electronics to David Robertson. He'll report back on the chances of meeting this after he talks with his vendors and technicians.
On a Purchasing note, Gina Salone has been quite helpful these last
few months negotiating with vendors. She has requested (and received) competitive
pricing and lead times. She's also been quite helpful interfacing with
tardy vendors to expedite quotes and, especially, deliveries. She has provided
valuable advice on all aspects of the purchasing process.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Akiteru
Finished all immediately necessary measurements and concentrating in
writing his thesis.
Alessandro
First test run of the numeric control Ultra-Sound milling machine to
make flex joints and mirror support points.
Works nicely, a first report is available at
http://www.ligo.caltech.edu/~desalvo/Ale.REPORT.DOC
Brian
Finished his SURF report (for long time delayed by Riccardo), available
at
http://www.ligo.caltech.edu/~desalvo/B_Emmerson_SURF_report.doc
It is a good report, we will probably extract a paper from the core
of the report, adding a few more details.
Stoyan
Baked (700, 835, 1000oC) MoRuB samples off center in the oven to avoid
secondary transients, provided the samples to Jan for measurement.
Ansys, comparative resonance analysis of glassy metal and fused silica
wires.
Studying the effective bending length of the MoRuB flex joints.
Writing final report.
Hareem
Working hard on exams.
Allyson
Working on improvements of Vickers measurement systematics.
Xavier
Finishing measurement of heath radiative losses of thermometer shoes
in the cryostat to complete the thermal conductance measurement.
Preparing to load the second thermal capacitance measurement and broken
calorimeter wires, need replacement.
Writing final report.
Charles, Stoyan
Working on automated vacuum controls for the sputtering machine.
Charles
Stress-Strain machine, learning the controls with pulsed motor excitation
to reduce the strain speed below 1 micron/sec, now at 2 microns/sec. Optimizing
the control loop.
First tests on samples:
Test one: standard stress strain loop, the braze broke (was a bad looking
one made by simple dipping) and the Youngs module was all wrong. Look for
the wrong calibration factor.
Test two: test on a 3 mm wide sample with a 1 mm crack, cycled at increasing
stress levels and observed progressive advance of the crack with rotation
of the two jaws. Nice to look at.
Preparing for expedition at Malibu for Ni sputtering and AuSn evaporation.
For additional information about this report, contact sanders@ligo.caltech.edu