Weekly Report for Week Ending October 16, 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  October 20, 2003 will be:

 (Meeting time: 10:30 am Pacific Time)

STAFFING COMMITTEE MEETING


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Saulson)


no report


Laboratory Administration (Lindquist)


LIGO Weekly Site Telecon (Lindquist)

A site teleconference was held on Thursday, October 16, 2003.  The following were among the issues discussed:

Budgets  - We are still comfortable with our estimate of $6 million for the carry-forward. FY 2003 costs being expensed in October are close to $1 million so far, but some of these items were on the list of items to be covered in the carry-forward..

University of Oregon  - The University of Oregon has billed for more than is in their contact for R. Schofield.  There appears to be some confusion here.  This will be a priority item for Irena to straighten out when she returns.

Property - Ed Chargoiswill travel to Livingston to help with the sale of the excess property..
The list of current actions revised to reflect the status of open actions assigned through October 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>

ACCOMPLISHMENTS (This report reflects activity for the past month.)

Developed a phase II Statement of Work with George Stokes which includes three main areas that need consideration:  1) further system design, architecture, and maintenance enhancements; 2) automated processing of new electronically submitted documents; and 3) improved website search capabilities.  This will be submitted to Phil by the end of the week.

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

ACTIVITY


10/16/03 Packages Faxes
In 38 43
Out 9 37

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
(This report covers four working days, October 9-14).

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

ADVANCED LIGO (Cost Schedule Control Systems) T. Frey
From: Thomas Frey <tfrey@ligo.caltech.edu>

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/
 

 

Continued development of a proposal for implementing Primavera Project Planner Enterprise.

Advanced LIGO Request
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)

Have started a draft of a Final Report for Cooperative Agreement NSF PHY-9210038, the cooperative agreement that covered construction, installation and commissioning, and initial operations of the sites.  This cooperative agreement ended June 30, 2003.  I have been able to dredge up information from previously submitted documentation, specifically the annual reports, the Advanced LIGO Proposal, the Procurement Plan for the LDAS Hardware, etc.  Have requested Albert's group to provide some additional information.  The target is to have a draft on the web page in time for the NSF Review, November 17, 2003.


Change Control/Contingency (Lindquist)

The following change requests are open.
 
CR-030015 FY 2003 Livingston Observatory Detector Maintenance Expenses (Increment) R. Wooley July 14, 2003
CR-030016 Hanford Facilities 2.2--Divide the Large Equipment Access to Facilitate Movement of Large Items (currently assigned to FY 2004 liens list) J. Worden July 31, 2003

Additionally we have received a request to add budget to the Louisiana Facilities account to cover items moved there when the Construction Project was closed.  We will do this, but we are waiting for the final numbers for FY 2003 so that we can address all of the Louisiana accounts.


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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



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


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

2K IFO
The H2 IFO posted its greatest NS-NS inspiral range so far (444kpc).  All WFS d.o.f. have been
engaged, although this application degrades spob and arm powers.  Work on debugging the WFS
and adding the QPDs continues.  ASI problems were debugged.  Power was increased into the
IFO.

Bill Kells visited LHO and worked on 2k scatterometer measurements.  Initial findings include that
the predominant mechanism for scatter is from discrete point scatterers, likely coating imperfections
or contamination on the optic, and, the newly replaced ITMX shows far less scatter than the old
(replaced) test mass.  High-resolution beam spot images are given here.

4K IFO
As the 4k has been frozen, it has mostly been left to lock in full or acquire++ modes.  Fundamental
violin modes remain apparently high, perhaps three times thermal excitation.  New calibrations are
being performed (to ensure we've not introduced too much systematic error since S2 and the
violins are in fact simply thermally excited).
 


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


---------------------------------------------------------------------
 

Interferometer commissioning:
--------------------------------------------------------------------
Continued commissioning and stabilization work in preparation for S3. We
have made about a thousandfold improvement over the excess
noise reported this time last week but are still stumped by a
persistent broadband excess, holding us
about a decade off the previous best sensitivity. Tests have eliminated
numerous candidate mechanisms (see Rana's nice <A HREF="http://www.ligo-la.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/15/2003&anchor_to_scroll_to=2003:10:15:14:48:55-rana" TARGET="_top">summary</A>).
At present attention is focused on anomalous behavior of the signals
derived from the beamsplitter pickoff (POB) which control the minor
degrees of freedom (Michelson and recycling cavity lengths),
and on an observed but unexplained discrepancy in the gain of the
common-mode wavelength control additive offset (AO) path.
 

Some other highlights:
 

o in the process of commissioning the new atomic clock timing system we
noticed a failed GPS clock module at the Y end and replaced it
 

o the new ISS was tweaked up to improve reliability and fault recovery
 

o a failed mirror mount adjustment micrometer was replaced on the PSL/IO
final output periscope
 

o an F2P filter was added to MC2 to match those on the core optics and
tested
 

o the thermal controller on the PSL reference cavity was updated to an
improved revision like those at LHO
 

o the ETM tidal offload servo continued to suffer from bugs which caused
unlocking; these may have been fixed, or at least temporarily swept
under the rug.
 

o A nasty bug was found in the end station EPICS processors causing
timing hiccups every 64 seconds; it was eventually fixed by swapping in
a different type of processor.
 

o The control room remodeling is largely finished, with new projectors,
operator and scimon workstations, and fixed displays for data
figures of merit.
 
 

Safety/security (Riesen)
---------------------------------------------------------------------
Completed weekly IR scan on the PSL and the 4 IOT/ISC tables, Found no
errant beams.
 

Found no safety concerns on the weekly site tour.
 

Continuing work on the LLO Laser SOP.
 

Re-established Laser Safety System control computer access;
there are now 3 access levels on the LSS;
a) Read only. Allows minimum access in controlling the system (without
operator log-in).
b) Operator Control.  Allows Operators (after operator log-in) to control
the LSS for daily functions.
c) Administration. Has full function capabilities including program
modification.
 

The man door between the large equipment airlock and the LVEA is now
alarmable to the control room.
 

General Computing (Roddy)
---------------------------------------------------------------------
Spent some time making sure that we are fully recovered from last weeks
disk crash.
 

Received the server that was ordered for Jonathan as the PDM Works
server.Spent a couple hours setting it up.  The next morning the power
supply blew.  ASA is working on getting me a replacement.
 

Spent much of the night last night working on LDAP.  I finally got it
working with SSL so that the entire session is encrypted.  This is for
Solaris only so far, but I feel confident in deploying it at this point.
 I will repeat the process again and document all of the needed steps.
 

Expecting the new RAID disk server from ASA today or tomorrow.  As soon
as it gets here I will start working on it and burn it in.  Afterwards I
will begin moving GC files to it.
 

LLO Seismic retrofit (Kern)
---------------------------------------------------------------------
Our last large contract has been received by the vendor, and all of the
machine and fabrication work can now be termed 'in progress'.  Chips are
really falling on the floor.  The machine shop manufacturing complete
sets of parts for 12 actuators by November 14 is on schedule, meaning we
will be able to begin the welded assembly before December begins.  The
Parker valve test manifold is back in the shop for manufacture and
installation of sleeve bushings in the plug valve bores.  The new
configuration control software (PDMWorks) for the SEI effort is
installed and serving us well.  We're pleased with its functions and
learning to operate within it's constraints.  This is just what it is
intended to do.
 
 

CDS networks (Parameswariah)
---------------------------------------------------------------------
Finishing up on work needed to be done before E10/S3.
 

Completed a initial check of the automatic Daily Summary plot program -
ROBO-PLOTTER. This will complement the ROBO-SCIMON and run during S3.
 

Worked with Rolf last week to fix the End Station front end problems.
We found the CPU load hiccuped evry 62-66 seconds periodically.
Traced the problem to mv162 epics processor. Fixed the problem by putting
in a baja.  Cause of problem still needs to be understood.
 

Added all the requested channels to the master.config file. This has now
added 2400 channels to the frames. I still have to estimate the disk space
available for S3 with this change. Even though the thinking is that this
addition is equivalent to adding 2 16KHz channels, this is only true for
full-frames. For trends this is equivalent to adding 2400 channels.
 

Installed the Refl port half wave plate  with the help of Ash and Rupal.
 

Moved the autoburt snapshots for the previous 3 years to a backup disk on
control4.
 

Control room suns are now mostly in and I have been checking to make sure
they all have the same environments/paths. Updated the video database and
software for the new projectors and monitors.
 
 

Detector Commissioning, High Power Testing (Amin)
---------------------------------------------------------------------
WFS 2: The WFS 2 sensor at LLO has been dissuaded from its obstinate ways.
Following Rich Abbott's repairs to the detector head, the WFS team
found that the headaches of a dynamic I-phase resulted from four LEMO
backshells not being secured. Once Rich Abbott torqued the backshells,
the I-phases of all three segments with respect to the number two
segment were stationary and easily cancelled in the digital phase
settings. WFS 2 is now ready for running.
 

ISCT 1 Redesign: All equipment and optics have been prepared for Daniel
Sigg's arrival at LLO.  ISCT 1's new half-wave plate controller has been
installed and tested thanks to Chethan and Ash's assistance.
 

RM Camera Installation:  Prior to the vent, we noted some
operators and scientists wanted a camera looking at the recycling
mirror. Mike Fyffe and I installed the camera on BSC3's new viewport
only to find a dimensional problem. The camera housing being used
partially occludes the view of the RM. Unfortunately we do not have a
housing that sits 45 degrees offset to viewport axis.  Such a housing
would grant a camera full view of the RM.
 

High Power Laser Facility (HPLF): The HPLF's first high power laser is
expected to arrive this week. Our vendor has informed us that this lower
power laser may be kept until the arrival of the 100 W device. The SOP
governing the lab is one day from final delivery and review by both
UF-LIGO and LLO.
 
 

CDS software (Khan)
---------------------------------------------------------------------
 

Detector commissioning, modeling and data analysis (Franzen)
---------------------------------------------------------------------
1) Weili Ken and I tested the new MC2 f2p filter installed by Brian
O'Reilly.
 

2) The S2 RDS107 frame data necessary for my WaveMon veto analysis was
mounted to alvar. Veto triggers are now being produced.
 

3) Amber Lynn Bullington at Stanford discussed the AdLIGO MC class of
Melody with me.  She is planning to release a new, more realistic
version within short. This is good since the UF IOO group needs the
model very much.
 
 

LDAS (Zucker for Yakushin)
---------------------------------------------------------------------
Igor is busy installing the final pre-run version of LDAS and
updating the main frame builder FB2.



 

DETECTOR SCIENCE & ENGINEERING


Seismic Upgrade Project

see also the LASTI section for full scale prototype progress and the weekly CDS minutes

Dennis Coyne

Held a kick-off meeting with our two Quiet Hydraulics Consultants (Rich Duder and Stephen Osder) at Stanford Univ. Dan DeBra, Brian Lantz and Corwin Hardham prepared talks on the HEPI system with concentration on the quiet (laminar flow) aspects of the system. A follow up meeting is scheduled for next Wed at LASTI. The consultants will see the full scale prototype and we'll review plans for, and questions and issues associated with, the fluid distribution and pump station designs.

Jonathan Kern

Ken Mailand

CDS

see also 10/15 weekly CDS meeting minutes in the commissioning archives

DMT Software

John Zweizig

This week I have been working to identify channels for use as epoch vetosfor the burst analysis. I have also been preparing to install DMT software for the E10 run.

CDS Software

Rolf Bork reporting

- Working on getting the remote control room (RCR) machine at Caltech up to date. We 

downloaded the EPICS 'gateway' software from Argonne and got it running on both 

the LHO and 40m lab gateway machines. With this software, EPICS programs, such 

as MEDM, run on your local machine and makes connections to the gateways to 

send/receive EPICS data. In the past, it was required to log into a gateway and 

bring MEDM screens back on an X window. Besides running much faster in this data 

only mode, the gateway software provides added security (set to default of read 

only) and reduces loading on EPICS front end processors (never makes more than 

one connection to a front end regardless of number of clients). We will continue 

testing today, and, if it seems stable, we will add a gateway to LLO.

We are also in the process of updating the other tools on the RCR today.

- Spent last week at LLO trying to find problems with end station controller 

(ran late and had periodic errors). Turned out to be a strange problem with some 

up our EPICS cpus holding up the VME bus (up to 15usec) at a fairly periodic 

rate of every 64-66 sec. We replaced these Motorola processor boards with MIPS 

processor boards and the problem was fixed. (See LLO elog for more details).

- Working on getting the LSC operational at the 40m lab. Since layout is 

different than sites, code changes will take about a week.

CDS Hardware

Hardware installed for the new LLO Caesium beam clock based timing system

Szabi Marka

 During the weekend we installed the hardware components of the new atomic clock based timing system at LLO. The mass storage room (MSR) houses the CsIII clock and the Master Clock Assembly of the optical fiber based distribution system. Time is transferred via single-mode fibers to the LVEA and the Mid/End stations, where it is compared to the GPS time. Every component of the MSR assembly is installed, tested and running.

 The Time Code Translators (TCT), timing comparators and related cabling are installed in the LVEA and  the two end stations. These installations are tested and running fine.

 The basic communication to the 162s(EPICS) is not tested as it would require more installations and software changes, as there are slight differences between LLO and LHO. It is not clear whether the changes can be safely finished before E10. The lack of communication will prohibit us from recording the timing difference second trends during S3.

The LVEA setup indicates a stable ~0.5 us difference between the Cs time and the PEM GPS time.

 The X end stations shows a stable ~2+20 us difference between the Cs time and the GPS time. It is consistent with the delay we expect due to the fiber delays (~5ns/m).

 The Y end station measurement unfortunately indicates wild and periodic variations

http://www.ligo-la.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/15/2003&anchor_to_scroll_to=2003:10:15:12:47:54-smarka

of the time lag between LIGO’s GPS 1PPS and the CsIII clock’s 1PPS. I observed the same behavior using the EX hardware and the CsIII clock at EY. Therefore it was very likely that the either the GPS receiver or the fan-out board was misbehaving. Replacing the GPS board fixed the problem. Now the Y end stations shows a stable ~1.2+20 us difference between the Cs time and the GPS time. It is consistent with the delay we expect due to the fiber delays.

 For now I set the fiber delay for the end stations to the generic 20.00us, to be consistent with the LHO setup. We plan to measure the precise fiber delays after S3, as the distribution system is capable of subtracting it with 5 ns accuracy.

 I would like to thank Mike Fyffe, Rupal and Andri for their help during the installation and testing.

Rich Abbott reporting

EMI Upgrade

Jay Heefner reporting

- Completed tests of first article VME crates from Dawn. We found several deficiencies in the gasketing that should be easy for Dawn to correct. Once they have addressed the issues the next batch of 5 crates will be shipped to LLO.

- Tested a VME crate from AP Labs. The crate did not perform very well. We have informed the manufacturer.

- Tested another EMI rack from Knurr. This rack is produced in Europe and the performance was comparable to our Equipto racks. A quote for price and delivery has been requested.

PSL

PeterKing

After approximately 12 months of being exposed to the open surrounds of

the PSL Lab, the pair of optically contacted flats was inspected.  The

contact was still good.  After inspection, the bond was deliberately broken

and the flats were contacted together again.

Thermal Compensation

Mike Smith

Working with Dave Ottaway on the design of the CO2 laser imaging optics for thermal compensation of the HR side of the 4K ITM mirrors.

Errant Beam Blocks

Ken Mailand

I will review with Bob Taylor the complete list of cleaned baffles, mounts, and hardware, sort, and prepare for shipping to LLO and LHO.

Optical Contamination Cavities

Lee Cardenas, Liyuan Zhang

OTF Lab. (W. Bridge)

Contamination Cavity # 1 

This cavity is going into a new optical alignment because the people who worked in the lab to

install the water cooling bumped into the mode match lens.We are recovering this cavity.

Absorption Test Measurement prototypein standby

We have received the new 30 watts laser and took it down to OTF Lab.

We have wired the Laser and the power supply already and attached the water cooling.

I am now working on the SOP for this laser so we can turn it ON.

New bench for the new laser is under fabrication.

Scatterometer system: A new and complete scan for the HR and AR surface Reflectance and transmission for the 2ITM04-C (Inner test mass mirror) is in progress.Complete plot and results will be released by Dr. Zhang.

The new base to house the larger Sapphire mirrors is completed and it will be installed next week.

There is some modification that it needs to be done on the old base.

OTF Lab at Lauritsen ROOM 38

Cavity #3: We have recovered the old results and the chamber is pumping now and we are taking ring down and beat 

frequency measurements every day as well as new RGA measurements .

We will introduce a new test simple of solder joints.Kester SN63Pb37 solder vacuum cleaned with RGA results.

Cavity #2 Test cavity in STANDBY.


40 Meter Interferometer (Weinstein)




Thermal Noise Interferometer (Libbrecht)


Since our last report we have made considerable progress in enhancing the modulation depth, and hence the discriminant, in the TNI arm cavities. By phase locking two separate function generators, we are able to deliver all of the power from one unit straight to the Pockels cell, with the other output going to the local oscillator. Not only does this boost the modulation depth, it also allows us to do away with the NIM phase shifter and limiter we had been using.
 

While we are able to boost the modulation depth, and while we see an analogous increase in the discriminant, we still do not observe any dramatic reduction in the noise floor. With the much-higher discriminant, the electronic noise at the output of the mixer appears to no longer be large enough to account for our noise floor. This noise is, as before, flat from a few hundred Hz up to 100 kHz, and its level is about 1e-18 m/rHz. Neither a theoretical prediction for the shot noise nor an experimental measurement of it appears to be high enough to account for this noise floor.
 

On the photothermal experiment, we have measured the loss in the cavity and compared it with the mirror absorption as measured by the photothermal response. Assuming the bulk value for Sapphire's thermal expansion coefficient, the two values for the absorption agree within experimental errors. Put another way, if we use the cavity-loss measurement to obtain the absorption, we can then measure the substrate thermal expansion coefficient and obtain a number consistent with the tabulated value.
 


LASTI (Ottaway)


no report


Data Analysis and Computing (Lazzarini)


---------------------------------------------------------
LIGO Data Analysis and Computing (Anderson for Lazzarini)
---------------------------------------------------------
------------------------------
LDAS Software Team (Blackburn)
------------------------------
 

The 0.8.0 release of LDAS is in great shape and expected to go out tomorrow
without a hitch. Over 100 problem reports have been closed out in the past
few weeks and of those identified as critical and/or important for the S3
run, only one will remain in a non-closed state for this release. This will
allow for running the new release of LDAS during the E10 run this weekend.
 

Changes to the frameCPP dictionary class to removed the Standard Template
Library's String class and replace it with a more stable thread safe version
of our own design has resulted in no core dumps in the frameAPI even when
optimized with inlining options since last Friday. An exception specification
bug caused an unrelated core dump but has been fixed.
 

The sites have new database tables configured specifically for E10. These
were setup under the old Solaris database server and that is the dataabase
environment that LDAS will use during E10. The plan is to create a new S3
set of database tables under the new Linux servers for S3 once the Solaris
databases can be migrated between the two platforms post-E10.
 

We have repeated our suite of regression tests on the LDAS pre-release three
times this week and will repeat one final time on the final tagged release
this Friday.
 

One of the newest regression tests confirming data integraty out of the
frameAPI was run since last Friday night without any instances of data
corruption out of the nearly 100,000 repeats of the test.
 

We updated the known pulsar search scripts and short Fourier Transform
search scripts per recommendations from the LSC developers. We are waiting
for updated instructions for the inspiral and power to allow us to begin
testing against the latest LAL and LALwrapper releases.
 

The documentation changes this week will continue until close of business
today. After that, the official LDAS version will be tagged in CVS and
the release built over night.
 

-----------------
E2E team (Bhawal)
-----------------
 

QND lecture
----------------
Kentaro Somiya of Univ. of Tokyo was visiting the 40m group. He gave an
informal lecture of QND to a few people around. This was a nice introduction
to understand what is necessary to implement this physics in e2e simulation.
 

SimLIGO study
-----------------
 Xiao Xu, sophomore, has started working with us, who has worked as a
 SURF student this summer.
 He runs SimLIGO under different conditions and studies the effects. His
 first tasks are
 (1) sensitivity degradation by the existence of radiation pressure -
     when locked, no degradation
 (2) stability and performance degradation when the input beam tilts
 (3) stability and performance degradation when the cavity axes have
     offset with respect to beam axes
 

WFS
------
(Biplab) Effects of differential heating in arms on WFS signals were studied
  and some of the effects like sign-flip and changes in magnitude that had
  been recorded in experiments were observed in simulation. To explain the
  effects that could not be seen in e2e simulation, we decided to use FFT
model.
  The experiments at LHO are related to heating from an initial cold state to
  a medium-hot state whereas, due to the limited number of modes in e2e,
  the e2e results become quantitatively more accurate as the interferometer
  approaches the final hot state.
 

Code development and maintenance
----------------------------------
AdLib code:
(Melody and Hiro) worked to make the new FUNC module using C++ compiler
 work properly. The new FUNC module code is compiled, if necessary, after
boxes
 are loaded, and dynamically linked and used when needed. For a FUNC with a
 complex code, the speed gain is over 10. This method of using dynamic linking
 of C++ codes could change the concept of modules dramatically and could make
 the e2e system very flexible.
 

 Several issues were found in a hard way. One is the setting of stack
 pointers. When a function in a shared library is called, the stack pointer is
 not properly set in a certain situation and the argument passing failed. A
 work around was found : at the top of the function body, insert an
unnecessary
 instruction to force the compiler to set the stack pointer and place actual
 body of the code.
 

 A few code structure changes were necessary to use shared libraries on
 the fly. A new generic support was added so that modules can request the
 modeler to call certain functions just before the time loop starts. Together
 with initialize_before_run() function calls, the use of macros, settings in
 par files, data_in modules can change in the near future for more clean
 environments.
 

(Melody) Finished code reorganization for the framework to do the on-the-fly
 compiling & dynamic linking.  Tested the code base using multiple and boxes
 primitives.  Continuing with code modifications to extend FUNC_X to VxV
 primitives and enabling backward compatibility to previously created box
files.
 
 

Propagator module:
(Hiro) Yoshida and Tiffany found that a propagator primitive could change the
 amplitude of fields which should not happen. This was caused by an
 interpolation algorithm used in the module when the time step was not exactly
 the one way travel time of the field through cavity. The interpolation has
 been changed to apply to the amplitude and the phase, instead of the real and
 imaginary part. This reduced the unwanted effect by 1000. The effect is
 O(10^-14) and is very small, but the existence of this needs to be kept in
 mind when we are dealing with a wide dynamic range problems. Fortunately, for
 LIGO I, this fix did not affect the sensitivity curve.
 

Alfi
--------
(Bruce) Completed edit window initialization fix (PR 431).
 
 
 
 

-----------------------------------
Data Analysis Activities (Anderson)
-----------------------------------
 

(Shawhan)
* Went through the latest draft of the S1 burst paper.
 

* Worked with Kaice Reilly and Gaby Gonzalez to catalog time intervals
during the S2 run when calibration information is not available, which turns
out to be the first and last partial minute of most locked segments.
These intervals will be flagged and incorporated into the
<a href="http://tenaya.physics.lsa.umich.edu/~keithr/S2DQ/S2seglists.html">
Segment Data Quality Repository</a>.  Also, the current algorithm in LAL
actually looks for calibration info one minute later than it "should", and
the consensus is to revise this algorithm.
 

* Fixed conlog to construct its index correctly even when Epics controllers
have badly wrong system clocks.
 

* Verified that the frame files now being written at the sites contain the
correct detector geometry information, the appropriate excitation channels,
and the slow channels which keep track of Epics timing discrepancies.
 

* Working on a new control-room tool called 'beacon' which continuously
compares the current control settings against an established configuration,
e.g. "science mode".  This is to help avoid variances in the control
settings from one locked segment to the next, which happened some during S2.
Hopefully, this tool should be ready for use beginning tomorrow afternoon.
 
 
 

(Creighton)
* Tracking down bugs in LAL 3.0.
 
 

(Weinstein)
* Prepared final (?) draft of S1 burst paper
 

* Working on hardware burst injection waveforms for S3.
 
 
 
 
 

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

Caltech
-------
(Dan Kozak)
 

* Migration from 9940A to 9940B format tapes finished (several hundred tapes).
 

* Continued to copy E7 data from HPSS (until HPSS went down on Wednesday).
 

* Worked with Sun to try to fix problem with part of /archive disappearing.
  Following Sun's directions, reset 3510's FC ports to "point to point only"
  and upgraded FC swith firmware.  So far, we've had no reoccurences.
 

* Received tapes from LHO and LLO with MDC data on them and incorporated
  these into /archive.  Some LHO data appears not to have made it to tape.
  Am pursuing the cause of/fix for this problem.
 

* Submitted problem reports to Sun about archiving continuing after a disk
  disappears from a SAM-QFS filesystem and some data not making it to tape
  (when moving data from LHO to CIT).
 

* Finished copying RDS from IDE-RAID into SAM-QFS at LLO.
 
 

(Al Wilson)
 

* Continue installing RH9 on desktop machines
 

* Fine tuning of BB on ldas-archive/dataserver
 

* Added sendmail fixes to cfdef
 

* Replaced motherboard in node210/cit  Unit is running burntest now.
 

* Used Ben's fix to reset the port 11 on blade 12 on the switch in cit.
 
 

(Stuart Anderson)
 

* Coordinate system upgrade tasks associated with LDAS S3 release
  scheduled for Fri (Oct 17).
 

* Worked with Larry Wallace to order replacement motherboards for
  all of the IDE-RAID systems we have to increase system stability.
 

* Tracked down the last LDAS server order (3 8-way Sun V880's) for S3,
  and found that they are scheduled to ship Thurs Oct 16.
 
 
 

MIT
---
(Keith Bayer)
 

* Installed FC-AL card in 280R.
 

* Installed metaserver 1U unit into rack and am configuring it now.
 

* Moving data off of pcraid#3 in prep to swap motherboard.
 
 
 

Hanford
-------
(Ben Johnson)
 

* The disk2disk full frame copy script appears to be working robustly at
  both Observatories. I am presently working on the error handler/monitor
  script, to further ease administration.
 

* Cut short the MDC run to 11:00 PDT Oct 16, in order to patch the FC
  switch, reconfigure the 3510 RAID array, and turn on striping for
  /samraw and /samrds.
 

* diskcacheAPI stopped seeing new data on Friday Oct. 10, I had to
  rebuild the frame cache in order to get LDAS to see new raw frames.
 

* I updated the sendmail configuration on the ldas-jobs box, Oct. 15.
 

* The new linux metaserver has been re-partitioned so that hda and hdb
  now have identical partition tables.
 
 
 
 
 

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

MIT:
(Keith)
-Fixed desktop PC that wouldn't post with 3rd set of ram
  (bad initial ram and bad replacement ram)
-Installed / replaced hdd in Dell laptop
-Investigating old penguin computing node that won't turn on
-Removing / shifting old users on gc filesystem to free up disk space
-Ordered software
-Obtained MIT site-license for Adobe 6.0
-Walking around to windows computers to force users to patch their nodes
 

Livingston:
(Shannon)
-Spent some time making sure that we are fully recovered from last weeks
disk crash.
-Received the server that was ordered for Jonathan as the PDM Works
server.Spent a couple hours setting it up.  The next morning the power
supply blew.  ASA is working on getting me a replacement.
-Spent much of the night last night working on LDAP.  I finally got it
working with SSL so that the entire session is encrypted.  This is for
Solaris only so far, but I feel confident in deploying it at this
point.  I will repeat the process again and document all of the needed
steps.
-Expecting the new RAID disk server from ASA today or tomorrow.  As soon
as it gets here I will start working on it and burn it in.  Afterwards I
will begin moving GC files to it.
 

Hanford:
(Christine)
- A lot of user account activity this week.  I added some users to
additional groups, had to create several new user accounts, reset the
password on a few accounts and added several users to the lho-all e-mail
alias.
- Started investigating wireless access points and nat routers for the
LSC meeting network setup.
- Helped get a new long-term visitor setup with a computer and place to
sit.
- We are still being probed by hackers.  I have blocked ping to all
computers on the site, so the hackers started sending messages
requesting the address mask, another ICMP protocol message type.  I have
blocked that at the firewall and now the hackers are sending HTTP
messages.  I am still working on a way to block the hacker HTTP traffic
without blocking legitimate HTTP traffic.
- Spent some time in training for my upcoming S3 operator shifts.
- Spent time working on upgrades to my laser power and refl transmission
software for both here and at LLO.
 

CIT:
(Veronica)
- LIGO website: Set up and monitored VRVS for the last seminar; posted the
presentation at the seminars webpage. Reworked a webpage for the 'Next
Seminar' announcement at the LIGO homepage.
Worked with Kip in providing him with a high-resolution image of a Hanford
aerial shot. Kip decided to use a negative to generate a printer-quality
image.
Repointed the links fro the old PAC url to the new one. Posting updates to
the Undergraduate Projects'03 page, internal bulletin board and fellowships
pages. Updated the roster database.
Met with other GC members to discuss a proposed makeover of the DCC
architecture. We agreed that the new system needs some further fine-tuning
but is an overall improvement. Continue working with George Stokes on the
DCC issue.
Per a request from Larry, looking into web cameras with higher resolution
for VRVS. The last seminar was a successful test of a combined VRVS/VNC
setup and can be used for future seminars/meetings.
- LSC webiste: Posting daily updates to the website for the November
meeting, as well as updates to other parts of the LSC website.
- CaJAGWR website: Updated the seminars schedule webpage. Compressed the
video of the last talk and transferred it to the streaming media server.
It is now posted along with the visuals. Provided user support.
 

(Mike)
-Reloaded a laptop that came back from travel that seemed to be having
problems with the operating system. It seems to be okay for now.
-loaded Linda Turner's old laptop that has been assigned to the loaner
pool. Mohanna is going to be using this laptop which she has requested that
I load additional engineering software.
-Loaded and configured a NT 2000 Server for PDM/WORKS (this is for Calum
Torrie) testing purposes.
-Loaded some additional software on Calum Torrie's workstation.
-Worked on a Hardware issue on our ghost server. This was a hard drive
failure that has lost multiple ghost images; I have tried to restore them
with multiple tools that I have, but had no success. I have a lot of
ghosting to catch up on to get these images back on the server through out
the weeks ahead.
-Problems with my office workstation. This seems like a hardware failure.
The cpu fan went out and now I my computer continues to crash. I will have
called Dell and they are claiming that it is a software problem. They have
asked me to reload this computer from scratch and if it happens again then
call them back.
- Reload Millikan's conference room PC that is a dual boot computer. The
windows OS ended up getting corrupted. I am reloading the windows side once
again.
-I worked on VRVS setting up and testing multiple configurations that
included testing the share option in VRVS and also running VNC
concurrently. Then I tried to run VRVS on one computer then on an
additional computer I ran VNC transmitting the guest speakers talk. The
problem we are having with the video conferencing is you can not read the
guest speakers talk from the VRVS camera. This is why we are trying many
different configurations to transmit a quality presentation. Larry and I
will be trying a few more configurations using some additional peripherals.
-This week I had a lot of onsite user support that included software &
printing issues.
 

(Lisa)
- Worked with Stuart to try and get a mail configuration for their servers that
would properly masquerade e-mail from their cronjobs (using submit.cf).
- Updated apache and openssl on castor.  That server had php compiled with
openssl, but the new version of php was not compiling properly.  I am waiting
for a more stable release of php to come out.
- Demo'd a bayesian spam filter called dspam.  I could not get it properly
working on becrux.  It would need to be compiled on acrux.  I'm going to look at
other packages before returning to this one.
- Began testing a package called CanIt for spam/virus filtering.  Right now I'm
not too happy with their support.  They don't provide binaries for solaris 8, so
I have to compile all their code myself.
- Dealt with a mailserver outage.
- Addressed a problem with a user who dumped 10Gb of data into a home account
thereby filling up the disk and preventing others from working.  Folks, if you
need a big chunk of disk space, please talk to someone in GC.  We can
accommodate your needs if you let us know what they are.
 

(Larry)
-This has been a busy week with procurement issues. Mainly, trying to get
invoices so I can get my P-card account reconciled.
-Assisted Mike on a number of PC related issues. The problems covered h/w, s/w
and user implementation.
-Worked with the DCC on a number if issues including trouble shooting the
upgrade of the s/w they are using.
-Working with Christine, Shannon and Ed C. with some of the logistical issues
for the different meetings that are coming up.
-Worked with Mike and Veronica on the VRVS and VNC setup. We still have a number
of items to investigate but so far things are looking better.
-We have moved over to the campus GigE backbone. I have been able to spend a
little time monitoring the new installation. So far no major problems. Still
have a number of performance checks to run.
-Touched on a number of projects which include: Updating the remote control
room, Calcium Calendar tool and options, new servers for the 40M, new sandbox
units for Hiro's group.
-Resolved a couple of hiccups with the servers.
-General assistance for the user community.
 

(Bruce Sears)
* Systems Work:                                    (0.5 days)
     - Evaluated eNote for general LIGO use.
     - More admin work on the JAWG Ilog.


Advanced LIGO Development (Shoemaker)



 

Advanced LIGO and supporting R&D

Suspension

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


Planning for and participating in the Advanced LIGO Suspensions Alignment Workshop. Received two quotes for the RM blades. We will review them at the weekly meeting Tuesday.

 

From: "Mark Barton" <maaku@attglobal.net>

This week I did some new impulse-response tests on the LASTI MC
prototype. In these tests all 14 OSEMS were installed and being monitored
by the dSpace (as opposed to just the 6 on the top mass of the previous
tests). I participated in the AdvLIGO SUS Workshop at Caltech and rewrote
several pages of Helena's assembly instructions to take into account
issues that people had. I also did a Mathematica model of a LIGO-I style
two-wire pendulum to provide results for comparison with a test case that
Virginio is using to debug MSE.


Pre-stabilized Laser

From: Peter King <pking@ligo.caltech.edu>


 

    With ShallySaraf, of Stanford, a short low-finesse triangular cavity was
fabricated.  Right now the assembly is curing; hopefully the cavity will be
ready for testing on Friday or Monday.  Assembling such a short cavity
presented some problems with the fittings used..

Core Optics

From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>


The 30 watt laser is in and is being checked out.  The new baseplate and beam delivery plate are scheduled to be installed on or around Oct. 22.  A table frame for mounting the laser is due to be installed on or around Oct 27th.  All utilities are in place.  Lee Cardenas is working on a laser safety procedure for the lab.

Helena will be requesting a quote from the group at Lyon to measure the absorption of one or two additional sapphire pieces.  The primary piece is the one ordered by Glasgow.  We may also have the lower quality "pink" 40Kg piece measured.  It is likely to have high absorption, and does have many inclusions.  This may cause a problem with the measurement.  The advantage to having it measured is that we stand a chance of getting more information on the structure of the absorption, so if the cost is low enough we will attempt this as well.

FROM THE CORE OPTICS WORKING GROUP TELECON:

Status reports for the CO Working Groups, Thursday, October 16, 2003

Helena: Coating Development Status

Meeting with JM Mackowski took place at Caltech on October 6. Details in last week’s report.

Garilynn: Sapphire Status

Nothing significant to report…

.

Bill Kells: Scatter measurements in LIGO I

Hi Res beam spot images.

Have made a detailed study of the video beam spot images on 2k optics under full

lock illumination: TMs (from HR side); FMx (from HR side); BS (from split side); and

RM (from AR side, HAM 9 video VP). All of these were from BSC ports except for the

ETMs which were viewed from the [short] spool positions (this to get as

normal as possible face view to eliminate depth of focus problems). This allowed detailed

magnified views with minimum optical zoom. In all cases a 75mm f1.4 video camera lens

was used with the addition of an auxillary 2x magnifying lens (and in some cases for the

frame grabber analysis two 2x lenses). The normal Watekccd video camera was used

(also the Sony handy cams were tried, with "super night vision" but had inferior S/N).

Typical images (with single 2x mag) are attatched. A survey (just eyeballing the images)

reveals:

1. The characteristic "globular cluster" of point defects dominates the images as a whole.

However it is visually clear that the interstitials between points is quite dark. It is this

background level (presumably from inherent surface/coating "microroughness") that

motivated these studies. We analyze the images to extract this (see below) by utilizing the

Spiricon frame grabber.

2. MOST of the optics have additional flaw patterns: particularly bright point defects;

gouges; near verticle streak patterns (cleaning?). These are exemplified in that attached

images.

3. For optics where the beam is 45 deg. incident, the point pattern distinctively

"scintillates" with a bright/dark frequency of 1-2 Hz. The ratio of bright/dark can be

dramatic: ~10x. The cluster pattern does not uniformly pulsate, so that the integrated

scatter is very closely constant. For instance it has been accurately established that scatter

(from all these optics) into the integrating scatterometer detector is precisely correlated in

time with NPTRX/Y). The scintillation is clearly associated with the residual optics

motions. By driving the RM (LSC ext.) this can be greatly accentuated. A third plot

(attached) shows a spectrum response (the GDS_TEST_22 channel is the scatterometer

output while aimed at FMx from BSC7 illuminator port) to the RM being driven

longitudinally at 0.6 Hz (260 units). The reference traces are for no excitation. An

upconversion series is clearly evident. The fact that this series is absent in the NPTRX

trace is probable indication of the scintillation "grating" noise. Whether this might be an

actual noise source in detection is not clear.

4. More detailed studies of 2kBS(face view) ant ETMy (short spool view) were

conducted by Spiricon frame grabber. These two optics showed the the least additional

flaws (point 2 above) A full analysis of this will be forthcoming. The object was to

determine what fraction the "globular cluster" point scattering contributes to the total

scatter (loss). The strategy was to grab two images, one sharply in focus, and a second

with the image strongly defocused (via the 75mm lens focus ring). Then the level of

interstitial minima (focused image) could be compared with the mean level of the

"smoothed" defocused image (which presumably has the same Net scatter). This scheme

works but is technically limited. The focused image still has some significant point

spread function (thus limiting the depth of interstitial minima). The defocused images

suffer from coherent light "speckle" patterning (never become completely smooth).

However it is clear from extensive image disection that the scatter from the globular

cluster substantially dominates the scatter, at least by a factor ~3 over any diffuse

background. This must be taken as only a lower limit.

See image at:

http://apex.ligo-wa.caltech.edu/ilog/pub/groups/detector/logs/2003/images/10/13/BillK-

1066074717.pdf

Elog entry link:

http://apex.ligowa.

caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/13/2003&anchor_to_

scroll_to=2003:10:13:12:51:57-BillK

the previous image was of ITMx HR (GBnote: newly installed) face shot at 45 deg from

the video camera port of BSC7. This next image is the same view (BSC8) of ITMy. Note

in both that defocus, side to side is evident due to the depth of field.

See image at

http://apex.ligo-wa.caltech.edu/ilog/pub/groups/detector/logs/2003/images/10/13/BillK-

1066074954.pdf

E- log entry link:

http://apex.ligowa.

caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/13/2003&anchor_to_

scroll_to=2003:10:13:12:55:54-BillK

Ju Li/David Blair: High Optical Power Test Facility Project Summary (Perth)

Thermal lensing simulations:

Even with the compensation plate, thermal lensing correction for Gingin Test 3 remains a

challenge. The compensation plate restores the original power recycling cavity modes but

cannot change the ‘hot’ arm cavity modes. So we can expect a serious mode mismatch

between the laser modes and the hot arm cavity modes. Due to this mode mismatch the

carrier power circulating in the FP arms will be divided by 2.

Solution investigated:

- Heating ring to change the radius of curvature of the ETM, not practical for

Gingin (required too much radiative power).

- Dynamic mode matching, seems to be a promising solution but difficult to

engineer.

- Change the ‘cold’ mirror radius curvature to include the possible thermal

expansion. I don’t recommend this solution.

The Mach-Zender interferometer using to test the compensation plate is having a major

hardware upgrade (new optics).

Gingin High Power Facility update

The last few items are installed in the laser hut, which will make it ready to be cleaned

down next week. Then the installation of the laser will start. This will be a 500mW laser

initially, to be replaced by the 10W laser. The pre- mode cleaner will be installed

consequently, from which point the mode matching for the 80 m cavity will be set up. A

10 MHz phase modulator is installed to provide the RF sidebands for locking the laser to

the cavity.

Group meetings for integrating the local control and the global control are instigated.

More attention is needed for a smooth operation of the local control of the isolator

system. Initially the LIGO SOS will be used for damping the test mass motion. In the

case when the residual test mass motion is to large, DC to ~20Hz feedback to the LIGO

SOS will be applied.

Baking of the central tank will take place early next week. This will take up the next 5 to

6 weeks. In the mean time, the cleaning and baking of the isolator part will be started. A

large portable clean room assembly tent is under construction which is used to cover the

open tank when the isolators are installed. John Jacobs is in contact (or will be soon) to

ask for LIGO technicians to come over to help installing the LIGO SOS.
 

 

Materials report from Glasgow with input from Stanford – Sheila Rowan
 

At Glasgow we have been investigating the amount of shear energy stored
in each of the modes of the samples used to calculate coating losses;
shear plays no part in the coating thermoelastic damping so we need this
information to calculate the thermoelastic damping correctly. We
are now in the process of gathering this data for the 3" x 1" and
3"x 0.1" silica discs.

Gregg and David Crooks have been comparing their respective codes used
to calculate 'Intrinsic' thermal noise and thermoelastic coating noise.
After initial discrepancies the two codes now essentially agree, with
one or two points of difference only remaining.

EoinElliffe has been running some FE models to check the effect of
including the finite size of the test mass on expected coating thermal
noise and we are comparing results from this with the calculated thermal
noise for a half infinite test mass.

RE: recent discussions with JMM on plans for future plans for coating
runs - the following is extracted from Greggs summary of discussions:

> > 2 - We tentatively agreed that he will provide two small
> > coater runs of monolayer coatings, one each of silica and
> > tantala.  We agreed on a canonical thickness of 2 microns.
> > He (the vendor) felt any thicker would seriously distort the  > properties of
> > the layer.  We will check to see if this thickness will work
> > for Q, absorption etc measurments.
 

Sheila checked with Ira Wygant - the Stanford student making
measurements of coating young's modulus - whether this would be a
suitable thickness, currently his setup is optimised at 5 micron
thickness and sensitivity drops signficantly for a 2 micron coating.

From: Eric Black <black_e@ligo.caltech.edu>
 

Here is a description of our photothermal experiment. We have finished a paper on it, including how we extract both the thermal expansion coefficient and thermal conductivity of a coating. Link to a copy at my website is

http://www.ligo.caltech.edu/~blacke/0310194.pdf

Auxiliary Optics

From: Michael Smith <smith@ligo.caltech.edu>

SUSPENSION
Attending the SUS conference. Set up an autocollimator demo for aligning the Triple suspension prototype. Preparing slides and a presentation to describe the initial alignment of the LIGO1 IFO using the COS autocollimator.
 

PHOTON DRIVE R&D
Awaiting replacement of the 500 mW laser.

 

Other Laboratory R&D


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