Weekly Report for Week Ending May 22, 2003


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

The LIGO Executive Committee Agenda for Monday  May 26, 2003 will be:

 CANCELLED DUE TO MEMORIAL DAY


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)


LIGO Weekly Site Telecon (Lindquist)

There was no site teleconference on Thursday, May 29, 2003.
The list of current actions revised to reflect the status of open actions assigned through May 15, 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, Salone)

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>

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>

No report this week...very busy trying to finalize the Advanced LIGO schedule and budgets to send to NSF Review Committee.

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



Reports (Lindquist)

The Construction project quarterly report for the end of February was scheduled to be submitted at the end of March.  Irena has been working on this, but has been distrtacted by a number of other priority issues: LSC, contract activities for seismic isolation, optics coatings, etc.  We have discussed priorities, and the quarterly report is still slipping.

I have prepared and distributed another model for projecting FY 2009 operating costs and prepared a supporting document for Gary/Barry.

A response has been prepared and iterated for the DCAA audit questions.  A final response is being prepared by Caltech Administration.



Change Control/Contingency (Lindquist)

The following change requests are pending or new.  Dennis Coyne submitted CR-030011 for the addition of an External Pre-Isolation (EPI) stage to the seismic isolation systems on the LIGO Livingston Observatories. This change is to improve the low frequency isolation of the currently installed seismic isolation systems as a retrofit with little or no disturbance to the alignment of the optics and without entry to the vacuum system.  I will put these change requests on the agenda for the next meeting of the Executuve Committee.
 
CR-030008 Furniture for the auditorium lobby, interaction area underneath the skylight atrium in the OSB, and on the second floor interaction area of the new laboratory/office building. (ON HOLD pending additional cost data.) M. Coles April 29, 2003
CR-030011 Seismic External Pre-Isolation at LIGO Livingston Observatory D. Coyne May 16, 2003


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

>From: Bill Tyler <tyler@ligo.caltech.edu>
No report this week.  Bill did publish a list of action items from the safet review earlier this month.
 


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



Summary of Commissioning Activities at LIGO Hanford Observatory (compiled by M. Landry)

Brian O'Reilly was visiting from Livingston, working on S1 and S2 calibration studies, plus investigating tidal servo issues.  Bill Kells has been conducting a series of measurements having to do with understanding the performance of H1, in conjunction with improving the strain sensitivity. Details can be found in a series of elogs 5/19-21.  Robert Schofield reported on a series of acoustic mitigation experiments, starting here.

4K IFO

Full locks have been re-established on H1, after more than a week of difficulties.  Once again we do not have a smoking gun for why we could not lock, nor why locking is better now.  The x single arm locks had clearly degraded. but re-establishing these did not immediately yield full locks. Work continued on the 4k power increase.  WFS work resumed.

2K IFO, DAQ

Rolf Bork is visiting and testing LSC code on the 2k, endeavouring to rid it of crashes, and adding in new lock aquisition code from Matt Evans; see Rolf's elog.  This occupied the 2k for much of the week.  Earlier, comparisons of independent dc calibration schemes were made on H2, finding agreement at the few percent level between PZT fine actuator methods and sign-toggling/AC extrapolation methods.
 


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


no report


Detector/Technical Support (Coyne)


 
see also the Revision Technical Review Board (RTRB) status here

Seismic Upgrade Project

Dennis Coyne

The External Pre-Isolator (EPI) Review Committee's report has been released (M030101-00). It recommends proceeding as quickly as possible with implementation of HEPI at LLO. The recommendation was difficult to make because there are no strong technical discriminators between the HEPI and MEPI systems. LIGO management is reviewing the associated change request draft submitted to the CCB to allocate the funding required. There is a significant cost increase for HEPI as compared to MEPI. A decision is anticipated soon.

Jonathan Kern

·Maraging steel for the double-start springs was bid earlier this month and a PO issued this week.  Vendor is now unable to meet quoted delivery, and we intend to cancel the PO.  Resorting to the second lowest bidder has resulted in an unexpected surprise, and that is that they have the capability to forge material for us and this means we can expect accelerated delivery. They have ~50% of the alloy billets in stock.

HEPI Pump Station

Ken Mailand

·I have contacted the manufacturer of the LASTI 'Aquamil' fluid and have been referred to their lab that will do an analysis of the LASTI fluid in use now, after several months of use.

CDS

see also 5/21 weekly CDS meeting minutes in the commissioning archives:

CDS Software

Rolf Bork reporting

At LHO this week to troubleshoot problems with new LSC code loaded a

couple of weeks ago. I ended up backing out one rev of the LSC code and

gradually incorporated the new changes for high power ops. The code has

run fine since Monday evening. Spent Tuesday trying to track a suspected

problem (LSC was rebooted by ops Monday evening because LSC ETM outputs

were railing). This turned out to be coincident with a 3 times larger

CARM gain being entered by an operator, causing CARM to oscillate

between its limits. Also, the GDS time monitor for LSC and ADCU-MX kept

moving around. After checking trends, found that this started April 30

(new LSC not installed until May 5). Further investigation found data

glitches on many channels of the 2K DAQ. This was finally tracked down

to a problem with the 2k suspension ADCU (bad fiber or reflected memory

board transmitter, exact fault TBD). We took that unit out of the DAQ

loop, and now signals appear good again.

To improve LSC EPICS performance, the MV162 was replaced with a MIPS

processor VME board.  We have not experienced EPICS crashing since this

change.

This afternoon, I updated the last part of the LSC changes which was to

put in Evans' latest lock acquisition software. The 2K LSC has been

rebooted and appears to be functioning properly, but we still need to

perform new calibrations and try to lock with it.

The mid station controller software was also updated. The changes are

minor: 1) Check incoming control signals from LSC/ASC to verify that

they are valid floating point numbers, such that suspensions do not end

up at a rail, as seen last week, and 2) fix the white/dewhite switches

such that they respond to a BURT restore.

CDS Hardware

Rich Abbott reporting

1.  Installation work is complete for the ISS at LLO.  All the controls function the way we wanted, but there is a large high frequency noise contribution (~500kHz) to both the MC servo and the ISS (the ISS now taps off after the MC).  It looks similar to noise we saw months ago and believed was due to the NPRO.  Measurements are ongoing trying to track the source of the noise as it is swamping the ISS and limiting the bandwidth.  The noise appears unrelated to the ISS.  It is the limiting factor for the MC servo gain setting right now as it is causing observable slew rate limiting.

2.  A frequency servo board is being prepared for shipment to LHO so that Paul S. can do the modifications to it.  This course was chosen to be sure we give the bandwidth extension changes a fair chance here at LLO.  As similar difficulties were encountered at LASTI, we will measure the transfer function of the modified board and make it available to LASTI.

Jay Heefner reporting

Freq. Devices DAC Development:

·Measurements of the output noise voltage tend to confirm FDI's number of ~140nV/rtHz. This is still above the 100nV/rtHz spec, but FDI claims that the spec can be met if the DC-DC converter on-board is replaced with an external linear supply. We are investigating this claim.

Pentek DAC Glitch: Pentek has sent us the file needed to program the onboard FPGA with the fix for the DAC glitches. We will verify that it works at CIT and then propagate it to the sites.

ICS110B Glitch: ICS has discovered a potential problem with the design of their latest revision modules and feels that it may be the source of our problems. They would like us to send them a module to be upgraded. LHO will pick a module to send to them.

LOS Coil Whitening: The first module is fully functional and tested. Three more are being tested. Eleven modules are being stuffed.

EMI Retrofit: A draft report has been issued for comments to the group involved with the rack and crate testing. Once their comments have been incorporated the report will be circulated to a wider audience for review.

LHO 2km POY Beam Re-alignment

Mike Smith, Ken Mailand

Awaiting a decision from Doug C. regarding the placement of the ISC laser autocollimator, either outside one of the viewports of BSC4, or inside the BSC4 chamber.

Tooling for alignment of the ITMY PO Telescope at LHO has been completed and is being vacuum baked with the other baffle parts. This is one methodthat could be used to align the ITMY beam out the window.

Errant Beam Blocks/Dumps

Mike Smith, Ken Mailand

All parts for installation at LHO on 6/2 are in process of cleaning and baking. Parts expected to ship to LHO by 5/28.

All the Stainless Steel Baffles for the June LHO vent, have been baked at West Coast Porcelain in Corona, CA.

All parts stainless and aluminum have been numbered, cleaned, and will be in vacuum bake tomorrow 5-22.

The parts packaged and sent to LHO 5-27 two day, for arrival Thursday, 5-29

The stainless parts were baked using the same method as used for the existing tube baffles, in the continuous furnace set at a temp of 849C, two passes ~12 min. each. This process produces an absorptive surface at 1064nm, on 304 stainless materials. A test on a stainless witness sample is being made by Peter King on both the mirror polished side and the standard finish opposite side.

PSL

PeterKing

A number of changes were made to the PSL EPICS records database for the

new intensity stabilization servo.  I also made the changes to the

cross-connect for some new signals and control sliders.

The beam propagation for the spare 10-W laser at LLO was measured.  A pair

of cylindrical lenses was ordered to correct for the astigmatism, these

were scheduled to arrive yesterday.  A temperature scan of the laser was

started.  The operating temperature was reduced by 0.3 degrees C, without

any detriment to the output power.

Optics Analysis

Erika D’Ambrosio

I made more FFT runs focusing on the sideband resonance curve, using the optical

configuration corresponding to H1.

The results are public in the first entry of my web page and the numerical data

I got are very close to the experimental observations lately made by Bill Kells.

I am also going on with the paper on the sideband balance, Bill and I have begun

to write, more systematically.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)
Contamination Cavity # 1
The test sample kAPTON (Polyimid paint) contamination test will be completed by the end of this week.
ring down and beat frequency measurements taken everyday.
Please see Dr. Zhang graphs for absorption, ring down and thermal lensing.

Absorption Test Measurement prototype in progress
We have measured the absorption of a 5 inches diameter sapphire mirror.
We got the absorption signal but not stable because the laser power is not large enough.
Absorption results will be released soon by Dr. Zhang.
We are looking into acquiring a laser of a minimum of 5 watts power.

Scatterometer
We have completed measurements for the  2ITM01(1200 ppm < R <2200 ppm generally, T~ 3% Manuf.) mirror.
after that we have rotated the mirror at 90 degree angle and measured it reflectance and scattering
of a surface area of 80 mm x 80 mm. of the AR coating.
 Please see Dr. Zhang's graphs.

We have revived the new transmission and reflectance measurements optical bench and
We went through measuring transmission in ppm, of all the 1.0" mirror available in the lab.
We found only two sets( flat and curved) of 70 ppm mirrors that we need.
 All the rest are 50 ppm mirrors.
Helena have already cleaned these two sets of mirrors and we will use them on the other
cavity that it is waiting to replace the mirrors and hung it.

OTF Lab at Lauritsen ROOM 38

Cavity #3
The new cavity introduced with fresh clean 50 ppm mirrors.  Did not work!
After all the efforts to improve it, all we got was power of only ~90 mw and its visibility ~70%.

We opened the chamber again and replaced it with a cavity with 70 ppm mirrors and hung with one end at 1.8
degree higher that the other end and pumped it down and made alignment, locked the cavity and we got
120 mw of power with a 95% ! visibility.  BUT the output still small in order for us to use it.
We took the mirrors out and have them cleaned.  We introduced the cavity again and pumped the chamber,
and as right now, alignment completed and locking is in progress.

Cavity #2 Test cavity is in STANDBY waiting on silver plated screws to be replaced.
Optical train upgrading is in progress as time goes by and we learn from the other two chambers set up.


40 Meter Interferometer (Weinstein)



 


Thermal Noise Interferometer (Libbrecht)


Since our last report, we have focused on improving our noise curve at

high frequencies, above 1 kHz. By looking at the coherence between the

two arm cavities and by measuring the individual contributions from

various noise sources, we have determined that our noise floor is

dominated above 1 kHz by laser frequency noise and electronic noise.

 

We can reduce laser-frequency noise by increasing the high-frequency

gain of the mode-cleaner servo, and to do that we are designing a fast

Pockels-cell path to implement frequency stabilization up to 500 kHz.

(Our current bandwidth using the laser's pzt actuator is only 90 kHz.)

For this high-frequency loop to work, we have to have positive phase

margin up to at least 500 kHz, and higher would be better. Right now we

are in the process of finding and eliminating components that eat

phase above 100 kHz. So far, arrested culprits include an SR560 used as

a summing junction and a mini-circuits low-pass filter at the output of

the mixer, both of which contributed substantially to the loss of phase

at high frequencies. Some phase loss remains, however, and we must

identify and eliminate its cause before we can implement the

Pockels-cell path.

 

We can reduce the net contribution of electronic noise by turning the

power (or the discriminant) up and the electronic gain down, if we can

preserve the input-referred noise in the servo filter. Right now our

servo filters are at their minimum gains, and any external attenuation

would either raise the input-referred noise or lower the dynamic range.

We are working with CDS on both a new arm-cavity servo filter design

and new mode-cleaner electronics.

 

Separately, we have installed a broadband Pockels cell in the beam path

and begun to measure its response up to 100 kHz. Preliminary

measurements indicate a response of 0.02 Rad/V, very close to the

factory spec of 0.015 Rad/V.
 
 


LASTI (Zucker)


LASTI (Allen, Coyne, Mason, MacInnis,
Mittleman, Ottaway, Rollins, Shoemaker, Zucker)
---------------------------------------------------------------------
 

EPI Progress (Ottaway, Mittleman, Rankin, Zuo, Nayfeh, Allen)
----------------------------------------------------------------------
HEPI
We investigated the coupling between the platform motion and the
Streckhiesen ground monitor, and estimated the ground stiffness. Some
results can be seen on the LASTI ilog for May 20 and 21.
 

Jonathan installed the optical isolator on the pump controller and we
remeasured the hydraulic power spectra. Some results can be seen on the
Lasti ilog for May 20.
 

Myron has reshimmed pier #1, #2 and #4 (#3 had been done previously). He
has also been working on replacing the motor and pump. In doing this he
has found that the existing motor-pump combination are not as well
aligned as they should be, as specified by the manufacturer, and that
(as a result?) there has been a considerable amount of wear to the inner
seal.
 

MEPI
After the controller had been retuned last week we attempted to find the
optimum sensor correction coefficients. We did this by locking all 7
loops and measuring the transfer function from the ground to a witness
(either geophone on the optical table or streckheisen on the support
structure) as a function of the sensor correction coefficients. We are
currently analyzing the results.
 
 

LASTI PSL & other experiments (Ottaway, Rollins, Zucker)
------------------------------------------------------------
This week three of our UROP(Equivalent to Surf) students have started.
David Lopez will work with Gregg on looking through the S2 data to get
the test mass internal mode Qs and frequency. It is hoped that these
will provide a thermometer to measure the temperature of the optics and
give us a guage on the amount of absorption present.
David Kaplan will work with Dave and is developing a vacuum compatible
photo-diode for LASTI utilising the ultra quiet photo-diode circuitry
that Jamie has developed recently.
Dan Mason will work with Dave and is evaluating the CO2 laser that will
be used for adaptive thermal compensation for LIGO1
 

Work this week has mainly focussed on the adaptive thermal compensation
system and finishing off the paper on the sideband camera experiment.
 
 
 

ISC Periscope Design (Ken Mason)
------------------------------------------------------------
The ISC periscope is being redesigned to be stiffer and less sensitivity
to acoustical noise. Professor Samir is providing assistance in
designing an acoustical damper which will wrap around
the periscope.
 


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)
E2E weekly Physics meeting
----------------------------
Matt, Hiro, Biplab discussed about ASC control and sensing matrix and some
needed modifications in SimLIGO PSL set-up after it was realized from e2e's
validation that some sideband terms contribute significatly in misalignment
signals (see below). The speed and compilation issues for code in the new
Linux boxes were also discussed.
 

Correct WFS signals
---------------------
(Biplab & Hiro) The validation effort for e2e's alignment signals finally
 produced something useful for the commissioners of the WFS system.
 We found the reason for the discrepancy between measurements and
 predication of WFS 3 and 4. The reason was that the theoretical calculation
 used hitherto (using Daniel-Nergis' Mathematica model) for non-resonant
 sideband (NRSB) demodulated signals at reflected ports took into
 consideration only those beating terms coming from plus-minus NRSB and
 carrier. The e2e run took into account other beating terms like those
 between Resonant sidebands (RRSB)  and "RRSB plus-minus NRSB" as well
 which turned out to be not negligible mainly due to the degeneracy of
 the recycling cavity.
 Biplab produced a new alignment matrix for the common modes to reflected
 port with demodulation by NRSB that will be compared by the WFS team.
 

SimLIGO
-----------
(Matt) This week I worked on the problem of ASC control in SimLIGO and at
 the sites.  The trouble is that the ASC sensing matrix is not diagonal
 and not easily diagonalized (due to noise and gain variation).  I have
 developed an algorithm for producing a robust control matrix.  The
 resulting control matrix gives stable control in SimLIGO and will
 (hopefully) be tested at LHO next week.
 

TAMA outreach
--------------
Dr. Hayakawa of ICRR started using e2e, under the guidance of
Prof.Ohashi. This is based on the MOU attachment regarding the
collaboration of simulation effort. They are going to purchase a
workstation for the simulation.  Hiro is helping to finalize their
specification. (Dr.Hayakawa is very impressed how Alfi is maintained
and updated.)
 

Code development and maintenance
---------------------------------
(Hiro) modeler code:
 The latest configuration has a erroneous setting to create a Makefile
 with inlining OFF, which makes things run much slower.
 For now, problematic Makefiles are modified manually to generate fast
 binary, but will be fixed soon so that inlining will be on by default.
 On the linux box, a few different sets of codes generate different
 results, although they supposed to generate same results. The cause of
 this problem is being traced.
 

(Melody)
        -  Preparing for the next build by modifying the build instructions
           to exclude obsolete programs and related software.
        -  Performed more benchmarks in the Linux
 

(Melody & Hiro) Speed optimization:
 Various optimization is being tested. Using -msse2 improves ~15%, -O(N)
 gives almost same results with N>=2.
 

(Hiro) CVS:
 The current CVS has many obsolete legacy contents and confusing
 documentation. The reorganization is discussed to remove those obsolete
 ones. Also, it was decided that Alfi will move out of the e2e CVS, but
 will be in a separate CVS.
 

(Ed Maros) Started process of removing old code.
 

Alfi
-----
(Bruce)
 - Added error viewer which was essential to Alfi use via Web Start (PR 400).
 - Completed work on port movement options (PR 392).
 - Working on matching this interface in the node External view (PR 380).
 

LIGO Data Analysis System
 

Software Systems (Blackburn)
The issue in the wrapperAPI which was preventing the same binary versions from
being run on both Redhat 7.3 and Redhat 9 has now been solved. This required a
"hack" of the code and relies on the operating systems properly cleaning up on
exit. A problem report was filed on this "hack" so that once we migrate away
from Redhat 7.3 altogether, we don't forget to undo the work around in favor of
proper exit code. This now paves the way for installing the final LDAS Beowulf
cluster with Redhat 9 instead of having to install several operating system
versions between now and the next science run on 400 nodes.
 

The memory leak in the metaDataAPI has been traced to swig names registered as
commands associated with delete_$class such as dbEasy and dbEasyStmt classes.
These leaks have been fixed and tested on the both standalone boxes and the
LDAS development system.
 

The mpiAPI can now distribute the wrapperAPI master process out onto the
Beowulf cluster. Previous versions of the code only allowed running the
master process on Node0 which occasionally caused a bottleneck in both the
CPU usage and available memory for the wrapperAPI master. Three new resource
variables in the mpiAPI's resource file allow/disallow and tune this new
functionality.
 

The bug which prevented the concateframe command from writing out frames
has now been fixed. A new bug was discovered with using the new RDS frames
which contained multiple IFO data in a single combined frame. This bug was
also quickly fixed. There is still an issue with using NDAS frames in LDAS
jobs. Part of the problem was traced to the frameAPI not handling an error
associated with bad NDAS frames and part of the problem is associated with
an as yet poorly understood corruption of some NDAS frames. An enhancement
to the FrVerify utility is being made to better isolate the form of the
corruption in the frame files.
 

The new createRDS command allows LLO and LHO channels to be integrated
into single output frames (not supported in previous releases of LDAS). It
will also have a new user option (-usertype) which will allow users to
uniquely distinguish "designer" RDS frames from the LSC standard RDS frames.
 

The S2 run RDS generation was completed last weekend. Early this week
the binning of the RDS frames into subdirectories containing 100,000 seconds
each was also completed. These frames are now available in the CIT archive
for LDAS jobs and replication to the Tier II centers.
 

One of the remaining memory leaks in the dataConditionAPI has been traced
to the the actions used in the slope dataPipelines. This should help to
pinpoint the location in the source code responsible for this small leak.
Work also began this week on an open problem report for mixed complex and
real vector algebra in the dataConditionAPI. The way the code is currently
written makes it difficult to fix this bug without major alterations, so
it probably won't be ready for the code freeze next week. A problem was
discovered with reading truncated ILWD files in the dataConditionAPI this
week. This was traced back to the ILWD library and is now fixed.
 

The migration of LDAS software to Redhat 9 using the newest GCC compiler,
version 3.3, continued this week. This is not the platform target for the
next LDAS release (0.7.0), but it is complex enough that we need to get it
started and understood as soon as possible. It has already uncovered that
much of the latest frameCPP code is not following the ANSI/ISO standard
close enough to work with the new GCC 3.3. It took several days to under-
stand the source of the problem, but it is now understood and fixed. The
fix is backwards compatible with the older GCC 3.2.x compilers, but they
didn't complain about the non-standard use of templates so the developer
needed to be up on the standard enough to not violate it but wasn't. It
is expected that this issue will occur in other modules of LDAS as we
continue to port the code to this newer compiler and OS.
 

Effort began this week to migrate our standard test suite into webpages which
will allow better tracking of new tests and test results in the future.
 

Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
 

* Got permanent standalone QFS licenses for 4 more machines.  We now
  have two permanent standalone QFS licenses that we haven't activated
  (for framebuilders at the sites when they go to Sol9/SAM 4, presumably).
 

* Continued to monitor SAM-QFS behavior (staging and releasing) and run
  archiving by hand occasionally.
 

* Began research/preparations for re-archiving of all data to higher
  density drives.
 

* Helped with install of new Beowulf nodes in Synchrotron.
 
 

(Al Wilson)
 

* Tested the nodes (new machines). Will now build a master image for
  cloning. Also will compile a master list for RH9 rpm's from this
  configuration.
 

* Posted on ldas-sw the driver and procedures for setting up the network
  for RH7.3 installation for the new one rack unit servers. These
  machines come with e1000 NIC's and will not work with a base RH load.
 

* The new kernels are here. Updated the kernels on Linux boxes in the Dev
  system. The new kernel in 2.4.20-13.7 it is located at our RH mirror
  under updates.
 

* Put online (network connect) Primarydb2(10.16.10.1) and
  testdb2(10.16.10.2) That would mean that they are located behind the
  gateway server on dev. They have a standard load of RH7.3 and are
  configured as ldas class servers.
 

* Did some minor work on assy the new racks as physical therapy.
 
 

(Stuart Anderson)
 

* Continuing to support the facilities upgrade in the main LDAS computer
  room at Caltech.
 

* Successfully tested 8 of the new Beowulf nodes with a 60hr memory test.
 

* Received the last 2 STK9940B drives ordered for the central archive system.
 

* Received 2 additional 5000VA UPS units for the LDAS-CIT system.
 

* Upgraded the 5 ldasbox development machines to the latest RH7.3 kernel
  in an attempt to obtain increased stability--to early to tell yet.
 

* Investigated options for powering the new 10+TB SAM-QFS disk cache for
  the central data archive in Powell-Booth.
 
 
 

MIT
---
(Keith Bayer)
 

* Helping Scott Koranda with LDR setup on ldas.
 

* Put last pcraid into rack.
 

* Put datacon/beowulf into rack.
 

* Running memory burntest on datacon/beowulf.
 
 
 

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

* u1d1 disk failed in t3-9. After replacing it, it could not get
  reconstructed: it turned out that there is also a problem with u1d5.
  t3-9 corresponds to /frame21 that contains S2 RDS data. I am currently
  backing up /frame21 to the new IDE RAID unit. SUN is shipping another
  disk to replace u1d5 which should arrive tomorrow.
 

* 70 new beowulf nodes arrived.
 

* Discussing with Allen, Rusyl and Shannon AC replacement and new power
  requirements for LDAS room.
 

* Got some of the ordered cables and UPSes from CDW.
 
 

(Shannon Roddy)
 

* Ordered some more PC interface cables for the KVM.  Igor needs these to
  hook up the new PC RAID.
 
 
 

Hanford
-------
(Greg Mendell)
 

* Multiple disk failures on t3-14 at LHO have made /frame20 on the LHO T3
  disk farm unavailable. S2 RDS data is kept on this file system. I
  rebuilt the LDAS diskcache at LHO without /frame20, so that LDAS can
  continue running without this file system.  However, /frame20 and S2 RDS
  data for the GPS interval [729273600 731529536) will be unavailable
  until we recover from the T3 problem and restore the data.
 
 

(Ben Johnson)
 

* Had difficulties restarting LHO LDAS Monday evening May 19, the
  Foundry FastIronIII switch froze, requiring it to be power cycled. Also,
  4 beowulf nodes encountered errors running "fsck" on themselves,
  requiring "fsck" ro be run manually.
 

* Had difficulties restarting LHO LDAS Tuesday morning May 20, an LDAS
  resource file had been changed, changing the startup port for
  diskcacheAPI. This unexpectedly caused the API to fail. Changing the
  resource file back to the original configuration allowed for a
  successful restart that afternoon.
 

* In beowulf node 32, replaced power supply and fan, newly supplied
  from ASA Computers. The node is presently being burntested.
 

* Working on two more T3 problems: replacement of a failed disk in t3-14
  and replacement of a controller card in t3-4
 

* The network driver for the new beowulf and datacon has been installed
  on both machines successfully. They are presently being burntested.
 

The final shipment of hardware for the large Caltech cluster is on track for delivery around the time of the
PAC -- on schedule with the information provided several weeks ago.
 

Data Analysis Activities (Lazzarini)
Shawhan:
* Checking the S1 inspiral upper limit analysis.
* Some more work on S2 data quality.
 

Yakushin;
1) After introducing noise rms estimate and new table columns into the
waveburst DSO, several new bugs appeared. Working to fix them.
 

Weinstein:
Weinstein:
- continuing to work on burst paper
- reading detector and stochastic papers
 

Creighton:
I have begun to implement an improved time-domain filtering routine in
LAL that maintains double-precision internally even when operating on
single-precision data, similar to the implementation in the
datacondAPI.
 

Reilly-K.:
I started moving the stochastic DSO functionality into
LAL routines, but then stopped because this may
not be the direction the group goes. I then started working
on moving functionality, which is now in the datacondAPI
to the LALApplySearch routine under LAL wrapper.
Whether we decide to use LAL apps or mpi processing
in the DSO, it will be necessary to have this functionality in
the apply search routine.
 

Mendell:
1) I have checked into LAL cvs under the lal/packages/tools/test
directory the initial code Malik Rakhmanov and I are writing to
independently check the beam pattern response functions in LAL. It is
called LALIndependentTestDetResponse.c. and is located in the same
location as the already existing LAL test code for the LAL DetResponse
functions, Dave Chin's LALTestDetResponse0.c. The basic code, based on
that written by Brian Cameron, compares the output from LAL for F_+ and
F_x with the expressions for these given in Jaranowski, Krolak, and
Schutz gr-qc/9804014.  The latter treats the detector as lying in a
plane tangent to a spherical Earth. Our tests to date find the
difference between the LAL routines and JKS are less than 6.0e-4. Malik
and I will expand the unit test run during "make check" when building
LAL to include some of our independent tests and to add comprehensive
independent tests for all detectors, quadrants of the sky, years, and
seasons that can be run from the command line. We will document this in
LAL.
 

2) Proposed to the PULG group that Mike Landry and I start writing a
stackslide DSO to run under LDAS.  A more complete proposal will be
given at the PULG face-to-face meeting in June.
 

Lazzarini:
Worked to formulate a X^2 analysis for the stochastic background analysis
analogous to the "X^2 cut^ used by the inspiral group. Looks promising.
Working with Romano to validate the approach. Basically, once we get an
upper limit, it would allow us to say the degree of to which the , e.g., time series behavior
is consistent with that upper limit . The analysis can be done by either time shifting the data
or asking whether the power distribution of the correlation kernel is consistent
with the underlying astrophysical process we are seeking to detect. It allows
us to use the broadband information of the interferometer in a manner not possible
with narrowband measurements.
 

Blackburn: Reviewing instrumentation paper.
 

General Computing (Wallace)
MIT:
(Keith)
-Supporting influx of urop students
-Hardware/network drops/software/accounts etc.
 

Livingston:
(Shannon)
-Worked on Marcel's computer to try and figure out why it was locking up.
Spent several hours swapping out various parts on a fresh install of
windows and it is still locking up after about 3 minutes.  It is not a
heat issue, so I am still not sure why it is locking up.  This machine
has already been back to the vendor and they can not find anything wrong
with it either.
-Set up a laptop for Bonnie so that she could do a presentation this past
Monday.  This will become a loaner laptop when she is done with it.
-Working with Larry all this week on a security audit.  I expect to be
busy with this through the end of the week.
-Ordered some more hard drives for the file server.  These will be
configured as a software RAID.
-Taking care of various pieces of paperwork and reservations for the
conference I am attending on June 8-14th.
 

Hanford:
(Christine)
- The first SURF student arrived.  I helped her get an account and get
setup on our computers.
- The new Cisco router has arrived.  I will be installing it next week.
- Had to cycle power on the old Cisco router due to memory errors.
- Delivered some documents and PC hard drives to the NSF.
- Lots of user support.
 

CIT:
(Mike)
Laptops:
-Finished up reloading Linda Turners laptop and configuring her user
environment.
-Started reloading a laptop for the loaner pool that was returned
from Hanford.
-Finished up loading a workstation for Greg McIvor who is a visitor up on
the third floor room 360 W/B. Who was using a older computer that I had
schedule for an upgrade.
-Started loading two additional workstations to replace a few older
computers. These replacements have much more processing power and will be
used for visitors/surf students that will be coming out to the project soon.
-Updated security patches on all NTSRV's and went through and search the
security logs looking for any intrusions. (All looks good)
-Transferred all NTSRV's ghost images to DVD; this will be an ongoing
process from here on out. After updating ghost images at the end of each
month I will also have a monthly backup copied to DVD. This will save disk
space on the server plus insures redundancy just in case of hard disk failure.
-This week I had a lot of onsite user/phone support that included printing,
software and OS issues. I also installed additional software for many users.
-Setup a meeting for the LIGO SEMINAR.
 

(Lisa)
- Built a solaris 9 jumpstart server.  I haven't tested it yet but I expect it
will take another day of tweaking to get the finish scripts right.
- Rebuilt bellatrix with solaris 9
- Rebuilt ascella with solaris 9
- Worked on a mathematica font problem for Hiro and Virginio
 

(Veronica)
- This week again time was spent almost exclusively on the preparation of
the Advanced LIGO website, finalising and testing. The website is now
posted at the LIGO homepage. I also prepared a CD version of the
website for the upcoming review and I am about to start burning the CDs.
- Project Science: prepared an email list of participants of previous
workshops and those who expressed interest. Sent out an announcement and
provided user support.
- LIGO website: Provided user support for ADvanced LIGO Suspension group
(webpage assistance and VRVS/VNC help). Monitored the VRVS of the last
LIGO seminar. Did usual upkeep.
- CaJAGWR website: user support; posted several updates.
 

(Larry)
-Spent a great deal of time reconciling my Pcard for the last month. Most of
the orders have arrived and the items have been distributed.
-Worked on a number of PC's and reworked a couple of network connections
in Bridge.
-Working on a computer audit with Shannon. So far things are going pretty good.
We should have a report out next week on what we have found.
-Misc. user support at the Observatory.
 


Advanced LIGO Development (Shoemaker)



 

Advanced LIGO and supporting R&D

General activity in reviewing and updating schedules, and coordination between subsystems.

Seismic Isolation

No report

Suspension

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


Advanced LIGO suspensions
1) QUAD Layout for the ETM

a) Eddy Current Damper (ECD)
It has been decided that if possible the copper should be attached to the suspended mass. In order to accommodate several copper arrays a new lightweight copper array has been designed. This is based on numbers supplied by Mark Barton. Work has still to be done on this design. Several methods for isolating each assembly are being considered.
Tests comparing different arrays will be carried out on a single pendulum at Caltech.

b) OSEM assembly
A lightweight OSEM assembly has been created. This will be approximately 3-4 times lighter than the previous assembly. The new assembly also includes isolation of each osem head from the rest of the suspension and a reduced number of parts.

c) Table cloth - OSEMS and ECD
Norna Robertson and I have created a rough layout of an upper mass that includes 6 OSEM assemblies and 7 eddy current damper assemblies. Further work is required.

2) RM Suspension

a) Cantilever blades
Drawings of the recycling mirror suspension have been created. These, revision 3 drawings, include a section that details numbers behind the design of the blade, manufacturing notes and dual dimensions.

3) Suspension Web-page for the weekly meetings
http://www.ligo.caltech.edu/SUS.html

4) MC Suspension

a) OSEMS
AnodisedAluminiumosems are due to arrive from the U. of Glasgow this weekend. It is hoped that the assembly can be completed and that these will be installed into the MC suspension sometime next week.

From: JaneenRomie <romie_j@ligo.caltech.edu>
 

AdLIGO Suspensions
Working on updating suspension-related documentation.
I have circulated an agenda for our visit to Glasgow the second week of August, along with the LSC meeting.  I've circulated the key items from Thomas's updated SUS Baseline Plan for discussion at the June 3rd weekly meeting. Calum, Mark and I worked on a revised eddy current damper design (see Calum's report.)

40m
Bob Taylor has all but one component for a spare SOS suspension. The AWOL bracket is being re-fabricated by CES and will go into the bake load when done.

Gin Gin
The mechanical components for the ITM and ETM suspensions are with Bob Taylor for cleaning and baking.


Pre-stabilized Laser

No report.

Input Optics

No report.

Core Optics

No report

Auxiliary Optics

No report

Interferometer Sensing and Controls

No report

Data Acquisition, Diagnostics, Network & Supervisory Control

No report

Other Laboratory R&D

From: "Erika D'Ambrosio" <ambrosio@ligo.caltech.edu>


I launched Mathematica with higher that standard precision, in order to check
if the giggles in the phase front of the top beam were due to numerical
errors and in fact they disappeared.

The profile thus evaluated has been inserted in the proposal for a prototype of
flat top beams, submitted lately by Phil Willems and me to the attention of
Gary Sanders and Barry Barish.

From: Youichi Aso<aso@granite.phys.s.u-tokyo.ac.jp>

Virginio and Riccardo
 

  Collected some leftover LVDT and coil actuator electronics, and sent to
  Alessandro for implementation on TAMA-SAS towers in construction for NAO.
 

Riccardo and Ed Chargois
 

  Shipped three Minus-K low frequency optical table feet to Akiteru in
  Hanford for testing in acoustic noise mitigation effort.
 

Riccardo off to Italy to start production of TAMA-SAS towers.
 

Greg
 

  - Melted another set of the 3 new alloys
  - Learned how to operate casting box
  - Cast strip of each alloy
 

Eric
 

  SEM'd indentation for Allyson.  Worked on MoRuB overview paper.  Work on
  alloy development- have cast with ~15% glass, will hone in on that
  composition to try to raise glass %
 

Allyson
 

  Last week Eric and I SEM-ed all the indentations i took at UCLA and now I
  am measuring them and waiting to get kaleidagraph on this computer so I
  can calculate the Vicker Hardness.
 

Enrico
 

  I did studies in LF advanced LIGO ITF sensitivity making an internal note
  for the COC meeting.
  I studied the gain obtained by varying the Q of the mirror, the phi of the
  coating and the beam spot size. Essentially I found a saturation at the
  values that are now reasonably acheiveable.
 

Youichi
 

  Wrote a program to solve boundary value problems of non-linear ODE's with Mathematica.
  The program is useful to calculate the profiles of MGAS blades.
  Designed and ordered MGAS blades, test apparatus, jigs.

Since Riccardo is out now, this weekly was edited by Youichi Aso.
 
 

 

 


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