Weekly Report for Week Ending February 20, 2003


 Exec. Comm. Agenda
Highlights
LSC
Administration
Hanford Observatory
Livingston Observatory
MIT
Caltech
Detector
40 Meter
TNI
LASTI
Data Analysis
LIGO II/Adv. R&D
Past Weekly Reports

The LIGO Executive Committee Agenda for Monday  February 24, 2003 will be:

 (Meeting time: 10:30 am Pacific Time)

THIS MEETING WILL BE A STAFFING COMMITTEE MEETING
 


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


LIGO Weekly Site Telecon (Lindquist)

There was a site teleconferences held on Thursday, February 20, 2003.  The following issues were among those discussed:

Traffic Control Gates:  At Hanford the traffic control gate is working.  It is possible to talk to the control room from the gate.  The camera is not yet in place.  The password for entry is "I have doughnuts!"

At Livingston, presentations of alternatives are scheduled for Monday.

Livingston Storage Facility Inventory:  Plan to kick off big time on Monday

The list of current actions revised to reflect the status of open actions assigned through January 16, 2003 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

From: Ed Chargois <chargois_e@ligo.caltech.edu>


DOCUMENT CONTROL CENTER (Turner, Mak)

>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

> From: Cleveland Mak <mak_c@ligo.caltech.edu>

ACTIVITY

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.

COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman)

From: Esther Cunningham <esther@ligo.caltech.edu>

Press here for ACCOUNTS PAYABLE HISTORY DATA .

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>

From: Gina Salone <gsalone@ligo.caltech.edu> From: Florence Kaufman <fkaufman@ligo.caltech.edu> SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

From: irena@ligo.caltech.edu (Irena Petrac)

From: Ed Jasnow <jasnow@ligo.caltech.edu>
CONSTRUCTION: OPERATIONS: SUPPORT (Baldon, Lloyd, Tischler)

>Irene Baldon

>Dorothy Lloyd >From: Ryan Tischler <rtischle@ligo.caltech.edu>

Advanced LIGO (Frey)

From: Thomas Frey <tfrey@ligo.caltech.edu>

Progress Period from 02.14 to 02.20

Accomplishments:

Weekly Advanced LIGO Project Controls meetings were held 2/14 and 2/20.  Next meeting is not scheduled pending Gary's meetings with the NSF.

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)

Cost Book Tool. Development of the Advanced LIGO Project Controls Guidebook continues.

Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.



Reports (Lindquist)

Advanced LIGO Proposal.  Preparing budgets for submittal to NSF.



Change Control/Contingency (Lindquist)

Change Request CR-030002 to adjust the FY 2003 operating budgets to reflect actual staffing during the first quarter has been prepared.  Additional information is required.


Human Resources (Akutagawa)

From: Cindy Akutagawa <cindy@ligo.caltech.edu>


Quality/Safety (Tyler)

>From: Bill Tyler <tyler@ligo.caltech.edu>

No report this week.
 


LIGO Hanford Observatory (LHO) and Interferometer Operations (Raab)


Summary of S2 Science Run Activities at LIGO Hanford Observatory (compiled by M. Landry)
---------------------------------------------------------------------------------------
Both interferometers have had a cumulative science mode duty cycle since the start of S2 of 67%,
although this figure will be degraded by Friday due to sustained high and gusting winds on the Hanford
site.  Sensemon NS-NS averaged inspiral ranges were typically ~290kpc for H1, and ~190kpc for H2.
The monitor is a key indicator of ifo performance and provides a threshold for operator
intervention.

Lock duration records were broken in the first week on both ifo's: H1 (35h), and H2 (30h), with 21
hours of continuous overlap.  Opening run calibrations and in-run astrophysical injections have
been performed, impacting the duty cycle slightly.

Shift-taking has been relatively simple and quiet - we continue to sort out and update shift
procedures, and they are stabilizing.  Visitors have been taking science shifts, and LHO staff
have been backing up operators.

Perhaps the most serious impediment to stable running on H2 is occasional alignment instability.  See,
for instance, http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=02/17/2003&anchor_to_scroll_to=2003:02:17:07:56:57-daniel

Downtime related to DAQ problems have been minimal.


LIGO Livingston Observatory (LLO) and Interferometer Operations (Coles)


Interferometer: The interferometer is operating at just under 50% duty cycle. We are able to maintain lock in science mode for several hours during the day. This is a significant improvement relative to prior daytime operating experience. The Y end controller failed Wednesday night and was repaired and reinstalled during the night. Other than that event, operation is mostly routine.

LDAS admin:
1) Sent 24 tapes to Caltech.
2) Received 4 spare disk drives for beowulf cluster.
3) Running 107 channel RDS creation script keeping up to 4 hours behind
the real time.
4) Created AS_Q only RDS of injection data at both sites.
5) Created AS_Q only RDS of first few days of the run and rsynced it to
LLO. Still working out the details of AS_Q only RDS distribution.
LDAS data analysis:
1) Together with Sergey Klimenko running waveburst DSO at sites.
Preliminary results show that it is working well.
2) Fixed the bug with printf statement.
3) Fixed problems in computing power of swapped and mixed clusters.
4) Working on improving selection of clusters that go into the database.
--
Igor Yakushin

CDS: Automated script that can create the Daily Science Lock statistics files and also elog them. Checking on backups and working on the dvd backup option. Running a crude monitor (CrudMon) on AS_Q to monitor any glitches. Working on a list for post S2 work on CDS. (Chethan)

1) Continued the work on setting up a local cds network for testing and
debugging purpose
2) Working on the design requirement for the Watchdog Controller, to be used
in CDS control room
Ash

General Computing: Fixed a few bugs that were created by the Solaris Management Console. There are a lot of bugs that are introduced by this tool. However, Solaris is moving in the direction of using this for everything. Perhaps it is time to get serious about moving away from NIS+. Working on getting an audio conferencing device added to the auditorium. Hopefully this can be done before the LSC. Fixed a couple of mailing list entries. Reset some passwords. Made some firewall changes for Ash.
Audited the ldas-jobs server. There are a lot of ports left open on this machine that need to be shut down. Ordered a new projector for the new conference room across the street. If it works well, I will order two more. Instead of using LCD technology, it uses a TI technology called DLP. It will be interesting to see how well this works.
(Shannon)

Seismic Amelioration: I have continued to support the RFQ efforts by providing Larry Jones with Key information. This week we spent more time on the spring flexures and the problems that we encountered with the fabrication and installation. Discussion continued on the POD design and the rotary actuators. Additionally, my efforts have continued in properly configuring digital content for the seismic isolation for LIGO 1, HEPI, and advanced LIGO. (Marcel)

Modelling:  We continued modeling with E2E. Under coordination with CIT E2E group, we started to create a macro file to describe the LLO 4k interferometer. The structure of this file will be identical to LHO4k.mcr file. When the creation is completed, this file will be placed in the same directory as e2edb.mcr file in E2E home directory (/home/e2e/SimLIGO/SimLIGO/Boxes). Under collaboration with H. Yamamoto, Tiffany Findley (SLU student) simulated the motion of a model suspension that she set up on SLU campus and investigated in the past several weeks. The calculated transfer function of the pendular motion shows very good agreement with measurement (perfect agreement within the margine of the experimental eror). She will continue the analysis for yaw and pitch motion. (Sany)
 


Detector/Technical Support (Coyne)



 

DETECTOR SCIENCE & ENGINEERING

For the 3 week period of1/30 through 2/19

Seismic Upgrade Project

Hydraulic External Pre-Isolation (HEPI)
See the LASTI report

Ken Mailand

An optical contamination test of the LASTI fluid 'Aquamil' is finished, a new test of a sample of HSF-75-2 a [hydroforming water soluble fluid meeting our specifications] has begun.

The results of the Aquamil test look fine; no measurable absorption increase over time.

The biological growth test is showing nothing after 11 weeks. A third sample of clear fluid for possible use at LASTI, or at the sites should arrive this week; this is a hydraulic fluid meeting our specifications with the normal  red color additive not added. All the 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.

The second [new] screw pump and motor assembly and coupling is ready for shipping to LASTI. The motor, coupling, and motor fan, have been precision balanced. The new motor is a TEFC/TC this is a cast solid frame [more stable than the stamped steel of the motor now used] with a 'TC'  shaft which is shorter than the 'JM' long shaft in the motor now used [more concentric] TEFC was requested by Mike Zucker at LASTI

The tasks listed below thru 7 should be completed this week:

1) pump sta. User's manual
2) LASTI pump station dwg pkg
3) tech rpt: performance
4) tech rpt: fluids
5) design pkg for production
6) cost estimate for production
7) presentation incl. production strategy for the pump
Still working on an investigation of applications and practices of hydraulic systems in clean room environments (with Dan DeBra's leads). Difficult to find any relevant experience.

Jonathan Kern

The HEPI actuator as-built documentation was finished this week, and thecomplete drawing package with manufacturing details has been filed in the DCC.  The DCN releasing for record is pending.  All of the early revision drawings are also filed in the DCC.

Electro-Magnetic External Pre-Isolator (MEPI)
See the LASTI report

CDS Software

Rolf Bork reporting

- Lori continues to work on the digital input optics WFS software forthe 40m lab.  This system should also be compatable to be installed as an upgrade to LIGO interferometers after S2. Hope

to start tests next week.

- I've been working on trying to pick up the speed of the LSC system. We are presently near our limit in the installed system.  After S2, we will need to read in a minimum of 4 more ADC channels plus associated processing. At present, LSC processing takes 15-17usec, with I/O taking about 35usec. Requests for GDS signals, such as the calibration lines, etc, usually then pushes the system close to its max allocated time of 61usec.

One approach to the problem is to get a faster CPU. However, we presently have the fastest Pentiums available (1.26GHz) in VME format. There are a couple of dual CPU models available, and I'm checking prices. The LSC does not lend itself real well to parallel processing, as the intermediate calculations always have to come back together at the input and output matrices.

Started to concentrate on ways to pick up the I/O performance, as this is the bigger time consumer.  After trying different combinations of locking the VME bus for single transfers, DMA for ADC inputs in the background while processing continues, and parking the bus and waiting for the Pentek ADC to be ready with the next data set (not polling), I was able to reduce the overall LSC time. With the system reading in 24 channels, the overall time is still 6-8usec less than the presently installed system, which reads in only 14 Adc channels.  So, it looks promising that we'll be able to meet our increased requirements after S2.

- As an alternative to having a faster CPU in VME, we are testing the possibility of having a faster external PC, connected to the VME crate via a reflected memory network. Alex has been working on this, building small Linux kernels on a 2.6GHz PC we bought for this test.  Linux is used to boot and start the system, but the code then disables Linux on startup to avoid realtime contentions. Initial tests look promising as far as code speeds and data connections. We are still working on the time synchronization, as the PC seems to slip over 61usec cycle boundaries periodically.  If this pans out, the application most suited to this approach would be the LVEA large optic controls. For the three interferometers combined, we now use 10 VME crates. This could be reduced to 3 VME crates and a few relatively inexpensive PCs. This could result in a fair savings when we replace present VME systems with the RFI shielded VME crates.

- Alex and I have been working on the digital suspension controls using one VME processor connected with an external PC. We started testing today running 6 optics in this configuration. So far, so good. I talked with Alan, and it looks like we will be able to install this in the 40m lab when we are ready to go.

- Hongyu made some changes to the MatLab/DAQ interface software to allow choice of servers.

- Continued work on documentation. The LSC software document isessentially finished and should get turned into DCC in the next few days. Also, I'm updating the digital filter module document and should be finished with that early next week.

DMT

This week (2/6) was mostly taken up with the E9 run and attending the jointBurst and inspiral workshop on vetoing. I am now working on fixing some of the problems in the DMT that showed up during E9, e.g.

 a) Make the trigger insertion process less sensitive to network load and

    LDAS restarts (Peter Shawhan will rewrite the SeqInsert script)

 b) Lessen the reliance on network performance (status information and

    documentation should not depend on info from other sites).

 c) Making LockLoss and SenseMonitor data for all IFOs available at

    both sites.

 d) Make the frame comparison process work with 16 second version 6

    frames.

 e) Fix memory leaks (found and fixed one in DecimateBy2 class, only other

    known leak may be in PeakMon code).

 f) Review/improve monitor configurations.

CDS Hardware

Rich Abbott reporting
  1. Stuffed and tested a new pump servo box to enable remote debug of the one at Lasti.  I will be done with it on Friday, I lost some time due to moving into a new computer.
  1. Much good progress was made on the ISS.  Thanks to the help of Stan and Peter Fritschel, we now understand the low frequency noise limits of the performance as measured outside the loop.  We are limited by acoustic pickup on the photo-detector used for stabilization and slew rate.  We have communicated a new packaging idea to Ben, and he has already implemented it. Basically hemade a new mount for the DC Photodiode.  It is a very sturdy monolithic aluminum block the holds only the photodiode.  From there, it is connected to the PD circuitry by a short shielded cable.  This was done in an attempt to minimize acoustic sensitivity of the PD enclosure. We increased the slew rate for the limiting components.

  2. Flavio has achieved good results (will discuss his results with all at the weekly meeting) with the ISS.  He will need to cut a new board in the not to distant future.
    We continued the testing of the ISS in the 40 meter lab.  We now believe that the present limit of the servo performance is the out-of-loop photodiode (PDA-55).  Although the dark noise of this photodetector is lower than the presently observed stability limits, testing with a flashlight source revealed a noise floor with almost identical shape and level to that observed during evaluation of the ISS.  The long and short of it is that we might be doing better than we think already.  We are planning to use a different photodetector tomorrow to continue the search for the source of the excess low frequency noise.
    Put a similar DCPD to the inside-the-loop diode as an independent measurement.  Found that the residual low frequency noise is no different than that seen with the PDA-55.  Set up a jitter measurement at the same point I am doing intensity stabilization.  Noted excellent correlation with y and x jitter to the residual low frequency noise.  Next step is to focus the beam spot on the in/out of loop diodes to ensure that the whole beam is on the active element of the diodes.  If the jitter is still causing low frequency excess noise, then I will begin to suspect the homogeneity of the photodetectors or some other yet unknown source.
  1. Mohana has completed the photon calibrator prototype.  I went to the lab with her and reviewed the work.  She is going to take a bit more data and ship it out for testing per Peter Fritschel's suggestion.
  1. Finished testing and modifications on the MC servo card for LHO.  All documentation was updated and we now believe we have a clear picture of the design.
  1. Sent out some L4C boards to replace the ones built by PCBExpress.  The new ones don't require cutting out the profile, and trimming the pads like the old ones.
  1. A new Motor Speed Control servo was sent to Richard Mittleman at LASTI.  We requested that the old one be sent back for autopsy. Received word that the pump servo is now functioning in differential pressure mode.
  1. Built up a breakout cable for the dSpace ADC inputs to allow access to other channels
  1. Started the RFPD re-design by raking together the comments and requests for changes that have accumulated over the years.
  1. Researched antennas for the RFI measurements to be done at the sites.
  1. Mohana has completed a write-up of the MC servo as a starting point of the MC servo re-design in accordance with the new rules for re-designs.

Jay Heefner reporting

Low Noise LIGO DAC:

- The prototype from Frequency Devices is operational and will be shipped to us on Friday. We will begin functional tests and noise measurements next week.

- There does appear to be excess noise at 100Hz. Our spec called for <100nV/rtHz, but the module has as much as 130nV/rtHz at low frequencies. Frequency Devices is reasonably sure that this excess noise is coming from the DC-DC converter they have used. When they replaced it with a linear supply the noise dropped to 85nV/rtHz. At higher frequencies the noise is less than the 100nV/rtHz spec with either supply. It should be noted that these noise numbers are made with the channel idle. The noise tests to be conducted at CIT will be while the module is outputing a full scale sine wave. Frequency Devices could not conduct these tests due to operating system problems in their test set up.

LOS Coil DAQ: The prototype board has been received and is being stuffed. All parts for the prototype are now on hand. Testing of the board will begin 2/20.

EMI Upgrade:

- Quotes for VME crates have been received. We have ordered two shielded VME crates from each of two vendors, Elma and Dawn. The evaluation units will be available in 6-8 weeks and will be tested for shielding effectiveness and operational usefulness at LLO. Test plans and criteria are being developed, but will include shielding effectiveness, cooling, and ease of use in the LIGO environment.

- Quotes for EMI racks have been received. A decision on how to proceed should be made some time next week, after Mike comes back.

Universal Dewhite Boards: A revision C of the board has been designed. This board incorporates all the changes to date, including offset trim resistors on the final stage. Boards will be procurred for production of additional spares and the 40 meter.

Sander Liu

Started on a draft for the EPI electronics design requirements document.

Richard Mittleman requested another set of  micro-seismic signal processor for their third STS-2. Currently we do not have enough spare parts to build another one. But I still have the first working proto type sitting in my office. I will check with him to see if he will accept them after we thoroughly retest them.

PSL

PeterKing

The PSL quadrant photodetector was dusted off and examined.  It waslast used around the time of the PSL installation at LLO.  A visual inspection of the board did not reveal any obvious problems other than a blown bypass capacitor.  Further checking resulted in finding a problem with the board's power planes.

The optically contacted pre-modecleaner that was dropped last summer was rebuilt.  It now appears to be okay.

I re-worked the PCB layout of the composite amplifier, the change being a change in foot print.  The standard foot print, although correct, is a bit small to solder onto.  I also looked into the packaging of the high power photodetector.  I think I can cram everything into a box whose external dimensions are 2" x 2" x 2".  With 0.25" walls to allow for mounting holes, things might be a bit tight.  I have yet to CAD everything up.

I provided Flavio with the transfer function data of the AC current adjustactuator of the lasers measured.  Along with spectra of the free-running intensity noise.

Still have not solved the problem of excess noise at 10 Hz in the high power photodetector.  For the past few days I have been struggling to cram all the components on a 1-3/8 in. x 1-3/8 in. board, as some of the traces have to meander around to accommodate the heatsinking of the voltage regulators and 5-W feedback resistor.

A low-noise amplifier board was laid out, milled and stuffed.  Themeasured input-referred noise was below 1 nV/Sqrt[Hz] for frequencies above 10 Hz.  At 10 Hz, the best measurement was 0.6 nV/Sqrt[Hz] whilst the worst

was 1.5 nV/Sqrt[Hz].  The variation is probably due to air currents around the test setup, as the amplifier board was only covered by a piece of paper (the schematic).

The shot noise for 15 mA of photocurrent was measured with the high power photodetector.  Problems with the measurement arose because of the large drain on the MagLite batteries.  The low-frequency measurements require repeating.

Lee Cardenas

The 10 watt laser installed inside the PSL enclosure still waiting to be checked.

Several small tasks (new OTF cavity design, laser bases, new chamber etc...) are underway. We have new laser bases nicely made.

Optics Analysis

Erika D’Ambrosio

I have been working on thermal lensing for Ligo I using FFT-code simulations. If the normalization of NSPOB is as described in the thesis by Matt Evans,there is a factor of two difference between measurement and prediction, whenthe arms are not locked. According to the simulations in the cold configurationthe recycling  cavity is unstable and the amplitude of the TEM00 of thesidebands is different  at the dark port of the order of ~20%, while thisasymmetry goes away when there is a power load on the two ITMs, so that the recycling mirror surface is matched to the resonating beam.

Bill and I are reviewing all the work we have done on the sidebands in the last year in order to make an article out of that. We decided not to prepare a letter but a long article.

The sidebands asymmetry has a straight impact on the detection scheme, since the output at 2 f_mod is

ASQ = [ (sb+) + (sb-) ]/2 . Im[delta CR]      delta CR = CR(arm1)-CR(arm2)

ASI = [ (sb+) - (sb-) ]/2 . Re[delta CR]

with a phase of Pi/2 between ASQ and ASI.

The carrier is reflected from the arms

with a different phase    =>    Im[delta CR]

and a different amplitude =>    Re[delta CR] .

The former is related with fluctuations of the length of the two Fabry-Perot. If the losses are not the same in the two arms the contrast is not ideal and there is a contribution Re[delta CR] at the dark port. Unfortunately this couples with the difference of the amplitude of the two sidebands. The product above is meant as a scalar one.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab at Lauritsen ROOM 38

Contamination Cavity #3  We have introduced a new test sample from Leander Lubricants CHEM DRAW’ # HSF-75-2,  Batch 12302001.  (a synthetic, hydraulic fluid.) with different additives. It is pumping as right now.
As far we can tell from the Beat frequency measurements, this fluid has not contaminated the mirrors.

Contamination Cavity #2 Test cavity
The chamber is pumping with new cleaned mirrors ~ 70ppm each. We are taking RGA measurements. It looks like the cavity has small leak (leak check test next) We are gathering all the necessary optics for the new optical train set up.

Contamination Cavity # 1
We have changed the cavity with a new cleaned 70 ppm mirrors.
 We have made a new complete alignment.  This time we can see clearly the round Gaussian TEM00 mode beam.  Picture taken because this beam is hard to get it.   Visibility is ~ 90%. The cavity is now locked.

We are taking ring down and beat frequency measurements everyday. This cavity is ready for the next test sample.
 

* Transmission measurements made for 1.00" mirrors (Helena's mirrors).
* Absorption Test Measurement prototype is in progress.  Testing small  sapphire substrate.
* In preparation to measure the  reflection for the   ETM mirrors (Helena's Request).
Most likely we'll be using the Scatterometer System.

OTF Lab. (W. Bridge)
Contamination Cavity # 1
We have changed new cleaned 50 ppm mirrors for the 70 ppm.
We still have this situation of the noise level . We have made a new complete re-alignment hoping to get rid-off the noise but nothing.  Instead we got better locking and more output power. So we got help from Dr. Peter king and after checking our servo and other equipments, we concluded that we are picking this noise from the building besides the 60Hhz noise level. So Peter suggested to get  an isolator transformer to run our equipment from. We have encountered  with another situation with the cavity mirrors.  We can not make the laser beam go through the center of the mirror as we align the beam.  We  found out that mirrors likes the beam to go through 1:00  O'clock position.  We had this situation before  (Jordan Camp could not get signal) with these 50 ppm mirrors.  We decided to install a new pair of mirrors freshly cleaned by Helena.

Absorption Test Measurement:

Prototype is in progress. Testing small sapphire substrate. We have attempted to measure the absorption of a sapphire and fused silica mirrors but we could not get any signal.  We encounter with the He-Ne beam signal of being unstable. It is very sensitive to the room air environment.  We decided to make an enclosure for theabsorption prototype set up.  Also, we need more  ND:YAG laser power.  We have use all theNPRO power ~700 mW but no signal.  We did take absorption measurement for a neutral density filter which it has high absorption therefore we were able to get the signal and measure it at different laser power settings.  Right now we are looking for a sapphire mirror( from Garilynn?) with a high absorption index so we will be able to take measurements.  Otherwise, we are going to need a higher laser output power. (at least a 3-10 watts of power ND:YAG laser)


40 Meter Interferometer (Weinstein)




Thermal Noise Interferometer (Libbrecht)


no report


LASTI (Zucker)


no report


Data Analysis and Computing (Lazzarini)


------------------------------------------------------------
LDAS Software (Kent Blackburn)
------------------------------------------------------------
 
 

LDAS has been closely monitored since the beginning of the Science Run. On
Friday of last week, we added pager email addresses to the LHO and LLO LDAS
systems so that critical messages in the system would contact Kent Blackburn
or Ed Maros day or night. During the first three days of the Science Run, the
two systems generated a critical message about once every four hours. These
were primarily due to the frameAPI core dumping, but there was one core dump
of the dataConditionAPI, one socket connection failure in the managerAPI and
one time out in the eventMonitorAPI. These typically occurred late at night
or very early in the day, leaving Kent and Ed exhausted by the end of the 3
day weekend. For some unknown reason the systems have since greatly stabilized
on their own, the last frameAPI coredump at LHO occurring 5 days ago and the
last frameAPI coredump at LLO occurring 4 days ago.
 

The other known issue with the release was the random failures at startup of
parallel wrapperAPI jobs on the Beowulf Cluster due to a bug (or bugs) in the
mpiAPI. These have been occuring at a rate of about 0.2% of jobs, close to the
expected from pre-release testing at Caltech. NOTE: Overall, the version of
LDAS running now is about 100 times more reliable than the version run in
E9. However, it is also about 100 times less reliable than the one used in
Science Run 1.
 

The createRDS command has not been able to keep up with the significantly
larger RDS frame at LHO. At LLO, LDAS is able to handle the smaller RDS frames,
needing about half of real time to generate. At LHO, LDAS is almost able to
keep up, but with the occasional frameAPI core dumps early in the run, added
delays have put the RDS generation about 40 hours behind.
 

This week, we have focused on fixing the issues that could not be addressed
in the last LDAS release prior to the start of the second science run.  This
is primarily the frameAPI core dumps and the mpiAPI start up bug, but it also
includes fixes to problems restarting APIs and some clean up of control and
monitoring functions in the controlMonitorAPI.
 

We have not been able to find a cause for the frameAPI core dumps on Solaris.
However, a similar frameAPI core dumping problem on Linux was traced to TCL
source code and a patch has been made. We are currently testing this patch on
Solaris to see if it removes the problem on that platform as well. If so this
would be allow for a significant improvement in reliability of the frameAPI
during the remainder of the run if we can get it in place soon. We have a
lead on the issues in the mpiAPI and have seen that the failure rate for this
bug is much higher on the UWM LDAS system with its much larger Beowulf cluster.
We are testing a possible improvement and working closely with UWM to assure
that the fix is universal.
 

In addition to the activities mentioned above, we have been working very hard
to migrate LDAS to the newest GCC compiler release. This is in part motivated
by the scary list of bugs that were fixed in this release that could impact
LDAS, and also motivated by a prospect that this new compiler will significantly
improve the performance of LDAS. It has already been seen that LDAS components
running under Linux run twice as fast with this new compiler. We are now making
the port to Solaris to see if similar performance boosts will materialize on
that platform. If so, we should be able to solve the problem of keeping up
with the data during the generation of RDS frames at Hanford.
 

Other background activities include:
 

 - instrumenting the eventMonitorAPI with additional debugging and logging
   code to trace a memory leak issue
 - instrumenting LDAS to use the /proc file system to determine process
   state information
 - improved API shutdown management
 - removed unnecessary LAM schema files from mpiAPI
 - patched TCL and FLEX
 - removed almost all warning messages from LDAS compile
 - corrected much of the "how to build LDAS" documentation
 - fixed problem in dataConditionAPI for
   a) response filters with zero values in gain
   b) fixed broken links for dataConditionAPI documentation
 - updated crawlink script to more successfully check for bad
   links on the LDAS web sites.
 - began testing LDAS against waveburst DSO on nightly bases
 - began tracking test suite in preparation for new release
 - modified ldasjob package in LIGOtools to support submission
   of jobs from machines on the LDAS network.
 

------------------------------------------------------------
LDAS System Administration (Stuart Anderson)
------------------------------------------------------------
 

Caltech
-------
(Dan Kozak)
 

* Exchanged more email with Qlogic trying to get the old 1Gb host config
  to work with the new switch.
 

* Have now labeled and put into the silo all but 3 boxes (90 tapes) of
  the 420 tape order.
 

* Put into the silo all but 9 boxes (270 tapes) of our prelabeled 1200
  tape order.
 

* Helped with move/hook up of AIT2 tape robot to Powell-Booth (ldas-archive).
 

* Confirmed that all S1 data is in SAM-QFS/HPSS before it's deletion from
  IDE-RAID.
 

* Worked on SAM-QFS issues related to ingestion of S2 data, mostly housekeeping
  related to only having 200 tape slots with our evaluation license.
 
 

(Al Wilson)
 

* Completed reliability checks for the IDE Raid units. All units check out
  ok. No disk failures.
 

* Finished building MOE, a Linux computer for a desktop workstation.
 

* Increased the warning and red alert levels on BB for the CPU usage
 

* Starting to work on a history graphing plug-in for BB
 

* Reverse engineering a way to monitor drive failures for the 3ware cards
 
 

(Stuart Anderson)
 

* Started archiving S2 data to SAM-QFS only--no more HPSS.
 

* Rewrote tape archive script to use both AIT-2 drives in parallel and
  to run directly on the main SAM-QFS server to avoid disk-to-disk copying.
 

* Placed an order for 3 years of SAM-QFS software maintenance.
 

* Removed all E9 and S1 data from the disk cache at Caltech to make
  room for S2 reduced data set. E9 and S1 data remain in both the
  HPSS and SAM-QFS tape archive.
 
 
 

MIT
---
(Keith Bayer)
 

* Continuing to tape off S1 ASQ data in prep for S2 data.
 

* Still having troubles with pc raid device scsi timeouts.
 
 
 

Livingston
----------
(Igor Yakushin)
 

* Sent 24 tapes to Caltech.
 

* Received 4 spare disk drives for beowulf cluster.
 

* Running 107 channel RDS creation script keeping up to 4 hours behind
  the real time.
 

* Created AS_Q only RDS of injection data at both sites.
 

* Created AS_Q only RDS of first few days of the run and rsynced it to
  LLO. Still working out the details of AS_Q only RDS distribution.
 
 
 

Hanford
-------
(Greg Mendell)
 

* The tapecontrol scripts have been running smoothly since Feb 10 to
  record on tape all the raw full frame data at LHO and LLO.  Three
  shipments of tapes have been sent from LHO to Caltech.
 

* The creatrds loop script has been running at LHO, generating the
  "level 1" rds frames.  The LHO rds frames are 42 behind real time and
  losing ground slowly.  However, this is not a panic situation yet, and
  we have plans to catch up before we fall to far behind.  (And all rds
  frames for all S2 times will be regenerated from raw data at Caltech
  regardless.)
 

* Ran the burntest on node23 and node25 with recently replaced hard
  drives; node25 passed by node23 crashed again during the test.  The
  manufacturer will be contact about the failed node.
 

* Working with Robert Schofield to save some of the PEM injection data
  on disk at the sites.  (All pre-S1 injection data was archived onto
  tape, and the tapes have been sent to Caltech.)
 
 
 

------------------------------------------------------------
LDAS Data Analysis (Stuart Anderson
------------------------------------------------------------
 
 

(Igor Yakushin)
 

* Together with Sergey Klimenko running waveburst DSO at sites.
  Preliminary results show that it is working well.
 

* Fixed the bug with printf statement.
 

* Fixed problems in computing power of swapped and mixed clusters.
 

* Working on improving selection of clusters that go into the database.
 
 

(Peter Shawhan)
 

* Spent several nights doing hardware signal injections into the three
  interferometers, mostly just before the S2 run began.
 

* Updated the dfm utility (in the LIGOtools 'dataflow' package) to make the
  'getFrames' utility work again.  This was necessary because LDAS no longer
  makes frame-cache information available via http.
 
 
 

Data analysis activities at MIT (Erik Katsavounidis):
 

Laura Cadonati:
 

Set up a web page that loads the Burst triggers (AJW's online ETG
production) and produces daily/weekly summary plots, updated every hour
or so - see:
http://lancelot.mit.edu/~cadonati/S2/BurstProd/S2-burstETGplots.html
 

Looked at the pre-run and first intra-run hardware burst injections:
http://lancelot.mit.edu/~cadonati/S2/Inject/S2injections.html
 

Now setting up for an online playground Burst analysis. Also on the
playground, investigation of the nature of the triggers produced by the
ETGs (Event Trigger Generator).
 

Erik Katsavounidis:
 

Re-did S1 playground and production pipeline analysis for TFCLUSTER
and SLOPE triggers. Working on understanding discrepancies with
numbers reported in the S1 Burst report and streamlining same analysis
on S2 data.
 
 
 

(Alan Weinstein)
 

- Running tfclusters, slope and power ETG's online
  during S2 on h1,h2,l1.
  Maintaining a summary web page at
  http://lancelot.mit.edu/~ajw/S2/dsorun/contrib/burst/web/burstS2.html
  in addition to  the online search status pages:
  http://ldas-jobs.ligo-wa.caltech.edu/dsorun/cgi-bin/index.cgi?action=index
  http://ldas-jobs.ligo-la.caltech.edu/dsorun/cgi-bin/index.cgi?action=index
- Feeding back to LDAS and ETG authors on problems during online running,
  and fixing some bugs in my scripts.
- Assisted Laura in running daily and weekly summary plots, in:
  http://lancelot.mit.edu/~cadonati/S2/BurstProd/S2-burstETGplots.html
- Gave an updated list of hardware burst injections to Szabi and Peter
- Ran LDAS jobs on hardware burst injections from 2/13 and 2/17,
  and assisted Laura in preparing and interpreting summary plots:
  http://lancelot.mit.edu/~cadonati/S2/Inject/S2injections-1302.html
  http://lancelot.mit.edu/~cadonati/S2/Inject/S2injections-1702.html
- Working with Shourov and Joe Giaime in evaluating the
  filtering done on the data before passing to the ETG.
 
 
 
 

(Kaice Reilly)
 

I have been working on the stochastic playground analysis this week
(and last).  The playground analysis has been completed and results
are looking reasonable (no more 10^9s). Joe Romano
and I have been spending hours each day on the phone getting this
worked out. I am working on a matlab code to create a time-frequency
plot of the FFTs of the CC spectra from this analysis.
 

Did a preliminary analysis of the stochastic hardware injections
from Wednesday night. The analysis will have to be redone when
better pre-S2 calibration files are available.
 

Also I am going through the reading of the Phys 237a course (week 1)
on gravitational waves.
 

More quotidian tasks, related to configuring my new box (I lost all my
email at one point),  required some attention this week. In this
category
I took care of some travel arrangements for Livingston and subscribed
to multiple new LIGO related mailing lists.
 

I have been working on a matlab script to make time frequency maps of the
cross correlation statistic (between the three IFOs) . This work
is being done for the Stochastic group.  Learning much about matlab.
 
 
 

------------------------------------------------------------
E2E (Biplab Bhawal)
------------------------------------------------------------
 

Mode mismatch
---------------
(Biplab) completed FFT runs for a number of intermediate states between
 Hot and Cold states of LHO4k. Finally these would be compared with
 Melody and SimLIGO locked state results with limited number of modes.
 

Code development
------------------
(Melody) Continued on the optimization of the modeler's FUNC_xxx modules.
 

Alfi
-----
(Bruce)
        - Worked on implementation of automatically managed data path
          junctions.
(Melody)
        - Started creating the web based manual for alfi5.
 
 
 

------------------------------------------------------------
General Computing (Larry Wallace)
------------------------------------------------------------
 

MIT:
(Keith)
-Fixed backup scripts using rsync/ssh
-Updated wireless hubs with new MAC addresses
-Installed 2nd NW22 wireless hub in printer room
-Troubleshot cisco mini-pci wireless hardware with Orinoco hubs
 (it appears that 128bit security will not work successfully)
-Installed sun Fortran compiler (CSR's) on straw
-Re-ordered extra matlab toolbox licenses for PCs
-Added new urop students to gc computers
-Troubleshooting virtual control room software
-Following up on purchasing trouble with Office XP software
-Adjusted Calendar software on emvogil-2
 
 

Livingston:
(Shannon)
-Fixed a few bugs that were created by the Solaris Management Console.
 There are a lot of bugs that are introduced by this tool.  However,
Solaris is moving in the direction of using this for everything.
 Perhaps it is time to get serious about moving away from NIS+.
-Working on getting an audio conferencing device added to the auditorium.
 Hopefully this can be done before the LSC.
-Fixed a couple of mailing list entries.  Reset some passwords.  Made
some firewall changes for Ash.
-Audited the ldas-jobs server.  There are a lot of ports left open on
this machine that need to be shut down.
-Ordered a new projector for the new conference room across the street.
If it works well, I will order two more.  Instead of using LCD
technology, it uses a TI technology called DLP.  It will be interesting
to see how well this works.
 

(Larry)
-It should be noted that since the run has started the two T1 lines have been
saturated pretty much most of the time. Check the following url for the
information LSU is keeping on the network traffic to and from the Observatory.
 

http://kahuna.net.lsu.edu/mrtg/ligo.html
 

Hanford:
(Christine)
- Dealt with a broken monitor that is still under warranty.  Called the
manufacturer for an RMA and shipped the monitor back to the
manufacturer.
- Fixed some problems with ssh1 on various computers.
- Purchased a new laptop for one of the operators.
- Worked with a Dell technician to troubleshoot display problems on a
laptop.
- Continued upgrading to Solaris 9.
 

CIT:
(Bruce Sears)
-(BS) Ilog maintenance.                         (0.5 day)
- Adding tons of scimon users.  Uhhggg.  I will need to put
some time into batching this job in the future.
 
(Mike)
-Reloaded a laptop for the loaner pool that included OS and GC software.
-Received a replacement laptop for Helena and am just about finished
loading GC software and a few additional packages that she requested.
-Michael Lloyd - I setup a workstation for him; this consisted of moving a
sun workstation to another office and replacing it with a pc workstation.
Plus I had to update all security/os patches on pc, in order for solid
works to run correctly.
-Stefano Tirelli - I setup his workstation for him that setting up users
preferences and loading some additional software.
-A few users up on the 3rd floor W/B were having problems with their
Ethernet connections after troubleshooting I ended up activating different
ports and switching them over; everything seems to be okay for now.
-Activated a few more Ethernet ports for some users with
laptops/workstations in their cubicles.
-Onsite/phone support,
This included networking, software, and printing issues; plus ran some
service pack/security updates on some user workstations.
 

(Veronica)
- LIGO website: made and posted a page with AAAS'03 presentations.
Working with the DMC on converting LIGO VHS tapes to DV. Tested the
quality of the DV on our camcorder; requested that the DMC redo the
original batch for better quality to compensate for tape degrading.
Posting Aspen conference transparencies as they arrive.
Posted various updates.
- LSC website: updating the March meeting page as the information becomes
available. Posted a few updates to other LSC-related pages.
- CaJAGWR website: working on smil combos for past seminars. Compressed
one of the past talks, awaiting JPL clearance required for publishing.
Provided admin support and updated the website.
 

(Larry)
-Spent a deal of time working on maintenance contracts. Most of the issues with
Foundry and SUN have been cleared up and should be wrapped up next week.
Campus has also sent in their yearly request for money to cover the Campus
maintenance contracts.
Procurements took some extra time since I had a number of items to reconcile
this past week.
-Worked on the network replacement boxes. Still testing them out. We had one
that was DOA and had to swapout a number of parts between two of the edge
switches to get the replacement one working.
Mike will replace the 3rd floor edgeswitch early in the morning and the core
switch swap out is on hold for now.
-Cleaned up a number of accounts and working on a few different lists of people
that will be contacted for various reasons. One list is for those that need to
signoff on the GC policy and the other is for accounts that need to be cleaned
out.
-Resolved a number of PC issues. Most dealing with spam and viruses.
- File restoration was also in the rise this week.
- Over 100 sites has been added to the block list this last week.
 
(Lisa)
- Mostly worked on the replacement server for www.ligo.  It is ready for
testing.
- Helped Larry with some quotes for software and replacement parts.
- Cleaned up the DHCP leases.
- Higher number than usual of file restores from tape backup.


LIGO II/Advanced R&D (Sanders)


Jay Heefner
Advanced LIGO Suspension: The electronics for the adv LIGO suspension prototype in the synchrotron building are installed and operational. The transimpedance of the GEO receiver module needed to be adjusted from 120K to 60K ohms

40 Meter LSC: Initial designs of the LSC have begun.
 

From: "Mark Barton" <mbarton@ligo.caltech.edu>

This week I continued the integration and testing of the LASTI MC
prototype electronics but encountered a moderately serious problem: many
of the coils are shorted to the coil former and thus to the structure
when mounted. i worked with Calum on a plan to send some back for rework
and to make others usable in the short term with an arrangement of
insulating spacers.

I also released v3.0 of my triple and quad suspension models in
Mathematica, along with a user manual, T020205-00.
 

From: Phil Willems <willems@ligo.caltech.edu>

Sapphire Q Tests
----------------

Satisfied that we can safely and precisely suspend the 40kg monster sapphires,
we disassembled the structure, refinished it, polished and greased a steel wire,
cleaned the good sapphire, and resuspended it.  We have data for several modes
but the best value so far is 2.0e8 for an antisymmetric radial mode.  This value
is reproducible in the sense that, for fun, we globbed some extra lard on and
saw the Q drop to 5e7, but cleaning the sapphire in situ restored the Q to the
initial value within 10%.

[GHS note: This is an amazing high Q!  Very impressive result on a 40 kg sapphire piece!]
 

This Q might improve with finer or better suspension wire, and we are preparing
tests.  We also will analyze the data for all modes and see if surface polish
losses are consistent with the observed variation.
 
 

From: ctorrie <ctorrie@ligo.caltech.edu>

ADVANCED LIGO SUSPENSIONS

VISIT
Mike Lloyd is visiting from the University of Glasgow until mid-March he is sitting opposite Janeen in west Bridge and can be reached on 6263952071.

MODE CLEANER

Janeen and I prepared 4 sets of drawings and assemblies for a complete controls prototype suspension. These are now with Gina ready to be set out to various vendors.

Mark, Janeen, Helena and I have been looking at possible upgrades to the coil design. These came about due to several of the coils having a short to ground. Several of these coils are already back in Glasgow for re-works and will be re-wired and re-assembled on their return.

RECYCLING MIRROR
Janeen, Mike and I met with Norna and Mike Plissi in Glasgow to discuss aspects of the RM design. Once a design has been chosen Mike will start a 3-D representation of the masses later this week.
 

From: Janeen Romie <romie_j@ligo.caltech.edu>

AdLIGO Suspensions
Ken Mason's HAM spacers should be out of the oven tomorrrow. I have a large optics carrying case ready to ship them back to MIT.
Three mode cleaner suspension drawing packages were given to Gina and Ruth for RFQ. They expect quotes in 3-4 weeks. This costing will back up our proposal estimates.

Calum, Mark, Helena and I have been working on optimizing the hybrid osem design. Calum and I have been working on updating the documentation.

Gin Gin
Helena has assembled the dirty ITM suspension structure. She and I will glue on the magnets and guide rods. Bob Taylor reports that the osems should be ready Thursday of next week. Jay reports that the electronics should also be done next week.
 
 


For additional information about this report, contact sanders@ligo.caltech.edu