Weekly Report for Week Ending April 11, 2002


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

The LIGO Executive Committee Agenda for Monday  April 22, 2002 will be:

 (Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

A meeting of the LIGO Change Control Board has been scheduled.  Time permitting we will address the standard agenda items below:

Executive Committee only 11:30 - noon   Topics:
 

Special Items:


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



LIGO Weekly Site Telecon (Lindquist)

A site teleconference was held on Thursday, April 18, 2002.  The following items were discussed:

The list of current actions revised to reflect the status of open actions assigned through April 18, 2001 may be found at ACTION LIST.

PROPERTY MANAGEMENT (Chargois)

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


DOCUMENT CONTROL CENTER (Turner, Mak)

>From: Linda Turner - turner@ligo.caltech.edu>

Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .

ACCOMPLISHMENTS

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

ACTIVITY

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.


COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman)

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

Press here for ACCOUNTS PAYABLE HISTORY DATA .

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

From: Florence Kaufman <fkaufman@ligo.caltech.edu>

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

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

From: Ed Jasnow <jasnow@ligo.caltech.edu>

CONSTRUCTION:

OPERATIONS:

SUPPORT (Baldon, Torres, Lloyd, Tischler)

 
>Irene Baldon >Dorothy Lloyd >Rita Torres >From: Ryan Tischler <rtischle@ligo.caltech.edu>

Advanced LIGO (Frey)

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

Progress Period from 04.12 to 04.18

Accomplishments:

Schedule 04.19 to 04.25:

Reports (Lindquist)

I have distributed a DRAFT quarterly report for the Construction effort (end of February) for review and comment.



Change Control/Contingency (Lindquist)

The following change requests have been submitted:
 

CR-010012 
Revision B
WBS 1.4.4.1 Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites P. Lindquist
CR-020002 WBS 1.3 (OPS) CDS Remote Control Room D. Coyne
CR-020003 WBS 1.3 (OPS) Fine Actuators for the LIvingston Input Test Masses D. Coyne
CR-020004 WBS 1.2 Underrun ISC Budgets (Construction) S. Whitcomb
CR-020005 ALL WBS (OPs) Increased Benefits Rate P. Lindquist
CR-020006 WBS 1.3, 1.6 Technical and Engineering Support Increased Requirements for FY 2002 D. Coyne

A reminder that we will be doing a LIGO Change Control Board during the Executive Committee Meeting on Monday, April 22, 2002 at 10:30 am PDT in the SCR.

Press for the latest Contingency Needs Projection.


Human Resources (Akutagawa)

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


Quality/Safety (Tyler)

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

No report this week.
 


LIGO Hanford Observatory (LHO) Operations (Raab)


No report this week.


LIGO Livingston Observatory (LLO) Operations (Coles)


From: "Gerry Stapfer" <gerry@ligo-la.caltech.edu>

Control Room: (Rich Riesen)   MEDM on screen help files are 50% completed.  Mode Cleaned AutoLocking installed and operational.  Spiricon and Image acquisition software now installed and operational on a Control Room computer.  All PEM Microphones have been installed and are operational.
6 MEDM screens are now available for web viewing.  Larger, higher capacity on-board batteries have been installed on the Weather Stations at both ends.

CDS: (Russ) Installed new shielded cables on the Pentek boards in 1X9 and at both end station.  Completed testing of the newly modified SEI feed forward system at both end stations.

Optics and Installation: (Jonathan) Yesterday I met all day with Mike Yeatman, the installer of our Laser Safety Interlock System for an initial closeout!  Happily, the system is functioning properly, all perimeter doors are alarmed the workstation in the Control Room has now been setup with an Operator's  Console that now erupts with an audible alarm and a graphic popup of violations.  He's also replaced the defective camera on the observation deck.  Began coordinating with Stanford and MIT to receive the handoff of drawings for the EPI.  Obtained appropriate software to manipulate the source files.  Completed and installed new ITM cameras and scatterometers, along with a photometric camera in the vertex.


Detector/Technical Support (Whitcomb, Coyne)


 
Commissioning:
Hanford
Livingston
Science & Engineering Support
See also the daily electronic logs for the installation and commissioning activities:
Hanford Detector Log
Livingston Detector Log

LHO COMMISSIONING

2km Commissioning

Rolf Bork Stan  reporting:
David Shoemaker and Robert Scofield have taken transfer functions of a shaker on the HAM9 support beams as a possible means to damp the stack modes.  No definitive answer yet, but it doesn't look crazy.

4-k Commissioning

Luca Matone
On Thursday night, the 4k Yarm was locked, for the first time, with the Common Mode servo enabled. The UGF was set to 1kHz, with the ETMY/MC_L and MC_L/MC_AO crossovers a little below 100Hz. To achieve this, the MC crossover was lowered (19.2dB -> 6dB in slider unites) and the Output Matrix filters for ETMY were enabled. As a result, the error point (AS_I) was decreased by ~10x @ 200Hz (with respect to locking without the CM enabled). The PSD of the control signal for ETMY was also attenuated (~100x) between 1kHz and 100Hz: the control signal was sent upstream, to the MC_L and MC_AO paths, not only to ETMY.

Rolf Bork
Made some fixes for LHO 4k:

Stan reporting:
Nergis, Daniel, and Peter have continued to work on the common mode servo, pushing it as far as it can go on a single arm.  The next step is to see what it can do on the full interferometer.

LLO COMMISSIONING

Rai Weiss reporting:
Work on the interferometer
Noise:

Measurements of the residual angular noise in the optical lever servoes were carried out. The noise is about a factor 100 below our current limits at 100 Hz.

Measurements of the frequency noise of the laser continue.

The correlations between the various error signals are being measured to establish if the noise is leakage from an unregulated quadrature. The most significant correlations we have observed are between the two channels at the antisymmetric port. The relevance to the noise is being investigated.

Initial results of a study to establish the mirror "sweet" spots (the places where the mirror rotation does not couple into the cavity length) has been put into the log. The study may have uncovered a small systematic unbalance in the suspension and test mass we had not noticed before.

A continuing and important background task is to clean up the RFI and computer generated pulses that are flooding the system. A program to introduce shielded cables, to make the grounding and isolation more rational has been going forward for the past month. There has been a reduction in the pickup of line frequency harmonics but there is still much to do.

Operational improvements:

Some of the locking sequences are now part of computer driven auto locking scripts and at times the instrument will reacquire with little human intervention.

The tidal servo using the fine actuators at the end test masses has been installed and is functioning. The common and differential mode control signals of the interferometer now automatically stay within the coil controller bounds - a significant step in aiding uninterrupted operation.

Subsystem development:

Scatterometers have been installed to view the high reflectivity surfaces of all the cavity test masses. The signals developed will be divided by the output of the cavity power monitors to maintain a continuing record of changes in the mirror scattering.

More work has been done on the wavefront sensor optics - it is a long job and we will have a celebration when this wavefront sensor subsystem is finally working.

Jay Heefner
The cables to and from the penteks in rack 1X9 were replaced with shielded ribbons and the observed noise at the output of the LSC whitening boards was reduced by a factor of 2. The dominant noise in the signal is due to polling the pentek. The second largest noise source is the 2^22 Hz clock. Both of these noise sources should be reduced significantly when the differential driver/receivers and the new ISC timing fanout baords are installed.

SCIENCE & ENGINEERING SUPPORT

Seismic Retrofit

Dennis Coyne reporting
The conceptual design review was held last Friday morning, April 12th. Documentation for the Review is still available here, and has been submitted to the DCC on-line archives. The review committee’s report is pending, but all felt it was a good review.

Electronics layout drawings have been prepared for the EPI and AID approaches, aimed at the initial LASTI implementation with dSpace controllers, but with provision fro migration to VME based control.

A revised schedule has been posted. (Note: ignore the installation phase which is unrealistically short in this schedule; This phase requires more thought.) It still appears to be feasible to meet a Jan 2003 start of installation but with little or no schedule margin.

[Note: Progress reporting is light below, because the team’s weekly meeting was canceled due to the review.]
 

External Pre-Isolation
Hydraulic External Pre-Isolation (HEPI)
Jonathan Kern is scheduling a trip to Stanford and Caltech to discuss details of the hydraulic actuator assembly that he will take the lead on for the prototype fabrication for the LASTI integration tests. He will also visit Caltech to meet with Ken Mailand and get familiarity with the pump station.

Pump Station:

Electro-Magnetic External Pre-Isolator (MEPI)
Nothing significant to report

Internal Stack Damping
All six degrees of freedom were closed (SISO) on the HAM-like demonstrator in the Lauritsen high bay.

CDS Software

Rolf Bork reporting

CDS Hardware

Jay Heefner

PSL

Peter King
More measurements were taken of the NPRO laser whilst it was locked to the reference cavity using the power actuator.  Within the loop bandwidth, the intensity noise is reduced by approximately 10 dB when the laser is locked.  Otherwise there do not appear to be any detrimental effects.

Rich Abbott, Flavio Nocera
Schematic development is complete on the ISS.  Board layout began today (17 April).  The board layout process should take less than a week.

Optical Modeling

Erika D'Ambrosio
SB Imbalance:
the problem with the CACR allocation permission is fixed and I was able to do many simulations with a view to finally wrap up the SB Imbalance analysis for the steady case, that is, the perturbations we considered do not depend on time.

Mirror maps:
the details of the runs performed by Prof. Ganezer have been discussed and it seems that indeed the sensitivity of Ligo II to microroughness is higher just
because of the Finesse.

Bill Kells
New interesting item is that Erika and I are actively in dialog with Ken Ganezer (CSDH) on the results they presented at the LSC meeting on performance of a Dual recycling ifo vs mirror surface scatter quality. We are uncovering a lot of interpretation and "translation" disparities which significantly alter the apparent implication of their original results. A full analysis is underway.

Optics Testing

Lee Cardenas
Contamination cavity #2,  Still locked.  Mr. Zhang and I, are continuing taking data of ring down and beat frequency everyday. The ring down is 33us and the beat frequency 74 Mhz. same as previous measurements.

Contamination cavity# 1  It is locked. But, we still have the same situation as before.  ring down is still 48us. (the one previously reported by J.Camp is 36us) and the transmission power is only 6mw with an input power of 110mw.  Bill kells still advise us for us to find out the reason why is a longer decay.  We are going to change the two modematch lenses for a shorter focal length and re-align it.  The other alternative will be to switch this cavity for the third one that it is sitting in the side and compare.  But, Our priority is to test the mineral oil ASAP.

I have the mineral oil and the test bars already baked by Bob Taylor(40m South Annex).
I have given (4) test bars to Dr. R. De Salvo for the samples of Kapton paint.
We will be installing the test bars with the mineral oil as soon as we get our digital oscilloscopes that we gave to Paul Russel (electronics) to have them calibrated.

Core Optics Support

Mike Smith
The input Faraday isolator polarizer, which generates the REFL beam, will induce astigmatism onto the REFL beam. This effect only happens to the reflected beam; the transmitted beam is unchanged. The amount is fairly small with the glan-laser polarizer that is currently being used in LIGO; however, if a glan-Brewster polarizer were to be used, the astigmatism would be significant, as shown below:
glan-laser polarizer (normal entrance and exit faces)-- diameter H=0.94, diameter V=1.00
glan-Brewster polarizer (Brewster's angle entrance and exit faces)-- diameter H=1.32, diameter V=1.00

LSC/ASC/DSC

Rich Abbott, Mohana Mageswaran


Jay Heefner
State code, operator screens and databases for the input crate of the LHO 4K DSC are nearly complete and operational in the test stand.

Rolf Bork
Lori tested new timing modules.  Next week, we will run further tests and begin software to integrate their use in LSC.  Lori is also finishing/testing new ASC code for use on LHO2k.

Alex and Khan continued work on integration of new digital filters into DSC.  Hongyu is working on the EPICS interfaces.  Alex also further optimized the new digital filter code for better speed performance.

Microseismic and Tidal Correction

Jay Heefener
LLO Tidal System
The tidal hardware and software for the LLO Tidal System has been installed and tested at LLO. The hardware was tested by using ezcaservo slaved to the LSC output to ETMX and controlling with the tidal offset slider. Early tests were successful and the CARM signal was kept near zero over a several hour period. In the process it was found that the anti-image monitor did not have sufficient gain to be effective, so the gain was increased to +19 on the boards at both the X and Y ends.

40 Meter Interferometer (Weinstein)



April 19, 2002 INCIDENT REPORT:
Location: 40m South Annex baking oven room.
Time: ~6:45pm Thursday, April 11
Report: baking oven heating tape shorted out and caused overheating insulation that resulted smoking. Steve vented the room, disconnected heaters, removed smoking insulation and took it outside. No damage was done. By this time security and fire department showed up and confirmed that it was safe to reenter room and smoke alarm was reset.
Response: Extra insulation was added to bake ovens. Post emergency response list on entrance door to South Annex baking oven room. Will obtain and install oxygen sensors.


Thermal Noise Interferometer (Libbrecht)


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

This week we identified one prominent source of noise in the TNI: a 15.75kHz oscillation on ground caused by one of our closed-circuit video monitors. This signal couples into the second sr560 in our servo filter, and the height of the resulting peak in our data is proportional to the gain in this amplifier. More importantly, harmonics of 15.75kHz also appear in our data, leading us to suspect that our prominent and regular peak at 31.5kHz is not, as we had first suspected, a mechanical resonance.

We also identified a similar peak in the photothermal experiment, caused by one of the R.F. signal generators in that experiment.


LASTI (Zucker)


No report this week.


Data Analysis and Computing (Lazzarini)



Data Analysis and Computing (Lazzarini)

Simulation and Modeling (Bhawal)
E2E Physics meeting



In Thursday's Physics meeting, we discussed the short and long term plans of some of the e2e activities. Details may be found available at http:/www.ligo.caltech.edu/~e2e.  Discussion on the rest of the topics will continue at next Wednesday's meeting.

Mechanical simulation



(Virginio)
- Final debugging stage for better 3D model for the LIGO I suspensions.    This model now includes the bounce and the right coupling with the roll mode of the mirror.  The  wires flexural stiffness has also been added.    This model has been done using a quite general maple program, which is able to provide the dynamics of the system if the analytical expression of the Lagrangian is given. Implementation into e2e is underway in parallel.

- Still working with Giancarlo Cella on the first release of MSE2, which   will provide the thermal noise calculation of the simulated mechanical systems.

LIGO I simulation system



(Matt) Began testing of COC and LSC sub-systems in SimLIGO.

Code development and maintenance



(Hiro) fixing some bugs.

(Biplab) Testing recent guoy-phase and mismatch related changes.

(Ed Maros)
- Finished first draft of Makefile.am changes for JAlfi
- Minor port support for Linux.

Alfi



(Bruce)
Last week's report:
  - Out sick half the week.
  - Working on a new and better implementation of connections and junctions in Alfi5.

(Melody)
- Fixed some PRs which included enhancing the settings value editor for alfi5.  Continuing on fixing some refresh problems with the popup menus.

LIGO Data Analysis System

Software Systems (Blackburn)
The majority of the week has been spent identifying and fixing bugs in the pre-release versions of LDAS. On Monday we pushed a pre-release version onto LDAS-TEST so that the members of the LSC that are developing search codes would be able to test their codes against this new version of LDAS. This pre-release version was found to have a very high failure rate and once a new version of LAL and LAL-wrapper needed to be pushed, we took that opportunity to upgrade LDAS to a new pre-release version as well. This version was having about an 11% false failure rate in our nightly testing. The primary cause of these failures were a set of bugs in the managerAPI, diskCacheAPI, and mpiAPI.  These were fixed on Wednesday and the test results for Wednesday night indicated that we have now reduced the false failure rate from about 11% down to about 0.25%.  This is a tremendous accomplishment and places us back in the ballpark of the failure rate that we experienced in the pre-release version of LDAS used in the E7 run last December.

We have begun the process of pushing the pre-release versions of LDAS to the Laboratory LDAS systems. At this time the pre-release version of LDAS is successfully running at LHO and MIT (in addition to already being on DEV and TEST). We will be working to get this pre-release versio of LDAS up at LLO today. Also, we have placed this pre-release version onto the new CIT system (which currently lacks a beowulf cluser).

We have completed about 40% of our required test suite used in qualifying an LDAS release. At this time on one major problem remains that needs attention for this release. The system does not allow Process Frames produced by earlier jobs to be reused in dataPipeline later dataPipeline commands. This is being looked into today. We also have significant documentation preparations still to make to the system before the release. There are several minor issues which will not hold up this release.

One minor change to the wrapperAPI forces it to buffer the messages between the wrapperAPI and the mpiAPI to not occur more frequently than once every 2 seconds - system tunable with the resource file. This was needed because a lot of poorly organized search codes are requesting to send messages at rates higher than unix allows without major unix reconfigurations.

A new problem tracking catagory was added to the LDAS GNATs system for GUILD this week.

The actual release date of LDAS will be closely coupled to the tests of the search codes by LSC authors. We will wait for an a-o-k before finalizing the release in the event that we resolve our internal issues before the search codes are adequately tested against this new release.

Hardware Systems (Anderson)
Caltech



(Dan Kozak)

* Continued HPSS migration from Redwoods/3590s to 9940s.
* More HPSS user directory reconfiguration and account maintenance.
* Worked on resetting everything after one big HPSS failure.
* Helped Igor at LLO with Qlogic HBA firmware, T3 pSOS and FC switch firmware upgrades.
* Helped Keith at MIT with Qlogic HBA firmware upgrade.
* Still working to get StorageTek to make good on replacing the Ultra 10.
* LIGO SAN testbed:

After much assistance from LSC/Sun to identify the problem (a SAM vs. Sun FC driver problem) SAM-QFS has finally mounted and unmounted a tape!!

(Al Wilson)

* Released BB for LHO.
* Setup BB for LLO.
* Learning AIDE as a free alternative to tripwire for intrusion detection.
* Upgraded LHO, LLO, MIT, DEV, and TEST to the latest ldas-linux patch set including openssh.

(Stuart Anderson)

* Pushed new LDAS pre-release versions to LHO, LLO, and MIT. This involved finishing the upgrade of all LDAS computers to openssh-3.1p1 for security reasons.
* Investigating the use of VPNs to solve the inter-LDAS Database communication problem.
* Moved the LDAS archive server from the CACR network to the new LIGO Gigabit Ethernet network at Caltech.

MIT



(Keith Bayer)
* Upgraded HBA firmware.
* Loaded several LLO super reduced set data.
* Loaded LLOcoin data out to lancelot for developers.
* Installed Ethernet card in lancelot and inspected cabling requirements to attach it to SF880.
* Started investigation into roll-our-own cheap pc/raid array.

Livingston



(Igor Yakushin)
* Upgraded firmware on T3s and switches.
* Upgraded fiber channel firmware on gateway and metaserver.
* Working on setting up replication between DB2 databases at LLO and Caltech.

(Shannon Roddy)
* Worked on the GC firewall configuration to allow db2 traffic in and out of LLO to Igor's machines.  There are still some issues, but as far as I can tell the problem is on the db2 machines and not the firewall.  I will follow up on this with Igor.

Hanford



(Greg Mendell)
* Finished worked with Igor and Julien to get an E7 reduced data set onto tape and sent to MIT.  The tapes were sent on Mon Apr 15.
* Tapes with LHO E7 data returned from UWM on Tue Apr 16.
* Sun replaced the DC converters in the SunFire 880 ldas dataserver on Fri Apr 12. (Originally Sun had come on Tue Apr 9 to do this, but found they did not have enough part to complete the job.)
* Assisted with the pre-release of the new version LDAS at LHO.

Data Analysis Activities (Lazzarini)
Mendell:
For The Weekly Report: Apr. 18, 2002; Data Analysis Update:

1) Updated the knownpulsardemod DSO to handle the new version of the LALUnitPair data structure. Ran tests in stand-alone mode, check the code into cvs, and ran test on the LDAS-TEST system, verifying the this code runs correctly with the new prereleased versions of lal, lalwrapper, ldas.

2) David Chin reports that he has verified that his new clean locked segments posted Apr 6 are valid. I will regenerate SFTs on the E7 data at the sites once the new release of lal, lalwrapper, and ldas is pushed to the sites.

3) Currently updating job scripts to run with the new prerelease of ldas to further test the system.  I will especially be testing the ability of  the new release of ldas to read in frequency series data from the proc structure of an SFT frame file.

General Computing (Wallace)
MIT:
(Keith)
-Installed new printer in NW22, created print queue, tested on various o/s's
-Troubleshot old laser printer 'tiny'
-Started investigation into tape robot

Livingston:
(Shannon)
-Reinstalled a windows 2000 domain at LLO.  This was set up a while back, but there was no redundancy designed into the domain.  As Microsoft software does, the domain server crashed the last time.  It also would not restore from the backups.  This time I have taken 4 spare machines that people have had replaced recently and set them up as servers with the domain data replicated between all four servers.  I have joined the windows 2000 professional machines into the domain so that I can manage software updates, hardware inventories, etc.  Also this allows people to have "roaming profiles" on the windows machines, if they want to utilize them.
-Received a couple of laptops in.  I am currently installing software on one.
-Spent several hours on the phone with Cisco tech support to try and work on some configuration issues with the PIX firewall.  I believe that long term, we will have to change the network topology and addressing schemes here at LLO to make full use of the PIX.  I have been discussing this with Larry.
-Installed a "CD Server" on the LLO network.  This allows me to copy images of CDs and leave them in a dedicated machine so that they are accessible by ftp, NFS, Windows Networking, www, etc.  This means that no one should lose any more CDs from now on.  They will still have to get the serial number for software, but they will not need a copy of the media.
-Installed a 4' high wall mount 19" rack in the new building.  This is to accommodate the patch panels etc. for the networking in the new building.
-Set up Norton Anti Virus so that it is centrally administered by me.  Everyone's virus updates etc are controlled from a central server now.  There is also a central quarantine and a central log.  Norton now notifies me if there is a virus found on any machine that I have set up in this manner.
-Ordered some spare batteries and chargers for the Dell laptops we have here.
-Installed a 160 GB hard drive in Marcel's computer.

(Tom)
-The network usage for Livingston can be found at : http://kahuna.net.lsu.edu/mrtg/ligo.html

Hanford:
(Larry)
-Working on the WAN issue. So far we have received some quotes from NoaNet and Albert is working out the issue of connecting to the Internet2 system.  Technically things are looking positive. There are a number of items that we still need to work out but so far it looks like NoaNet will be able to accommodate us on most of them.

CIT:
(Mike)
-Rebuilt two PC's and reloaded OS and General Computing Software for visitors that started on 4-15 and 4-18.
-Moved equipment around by replacing monitors and computers, for two visitors that started this week.  Reloaded OS and GC software on three Laptops.
-Went through Linda T.'s Laptop and corrected multiple software errors and added upgrade patches plus service pack 2. Everything seems to be running fine for now.
-I have been continuing to work on updating our list for the PHP webserver database; I just about have this done as far as the PC's go.
-Larry and I ran new cable drops to new control room in the sub basement conference room at bridge annex and one office.
-Had to reload a computer due to a virus that corrupted the OS. I restored this from a Ghost image.
-I had a lot of onsite user support this week that included networking, printing, e-mail, software and virus problems that I had to work out with users.

(Veronica)
- LIGO website: made yet another version of the new LIGO Science Links webpage. Added several links that were left out. Posted various updates to the LIGO website.  The LSC website has been transferred to a web server of its own; I went through the scripts to make sure everything runs smoothly, the link structure is preserved, and that nothing is left out.  Posted more LSC March meeting talks.  Working on the LIGO Policies and Procedures website.  Meeting with Ryan about the new LIGO Press Kit website; started working on the website layout.
- CaJAGWR: posted Tinto's talk as video and pdfs. Updated the seminars page.

(Lisa)
- Fixed the php installation on vega.  Restored the inventory system to that.  Mike has been actively loading it with accurate data.  This still needs some work regarding how mac addresses are handled.
- spent the majority of the week working on the mailserver vacation problem -- this has involved quite a lot of troubleshooting regarding dependencies in the development environment that don't show up in any of the documentation.  The problem with the vacation messaging has shown up on another of other platforms, but the general UNIX community is stumped about how to fix it.

(Larry)
-Back to working procurement issues. Foundry still owes information on a purchase from last year. Trying to get a double charge from ITS taken off. Placed, multiple computer and equipment orders for different groups. Working on a order of new units for the 40M.
-Tried to spend some time working on the vacation problem but have not been able to get much done with it other than running tests for Lisa.
-Restored a number of directories for different people. The backup system Lisa has in place saved quite a bit of time.
-Worked a number of cable issues. Switch cables and cables for the new control room.
-Windows XP has been a topic of discussion and found so far that it does not work well in our invironment. There are network, wireless, driver and application issues. Presently, the sysadmin group still recommends using Win2K if one needs to run under Microsoft.
-The group is working on changing the wireless setup. Working on setting up a standard configuration so the user will have minimal changes to make when going from one site to another.
-Working a couple of security related issues. Mostly viruses and some other minor incidents. After talking with ITS and their problems, we've been going pretty good on keeping the number incidents down.
-Working on documentation for a number of items. The GC policy has a few changes to be made but so far it is looking pretty good.


LIGO II/Advanced R&D (Sanders)


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

Homogeneity Compensation - Goodrich has delivered the 25 cm sapphire blank with compensating polish.
I've measured the homogeneity of the piece.  The good news is that they have compensated the inhomogeneity of the piece. See the image at http://www.ligo.caltech.edu/~coreopt/GoodrichComp.JPG  This represents the central 150 mm diameter of the piece.  The measurement is through side 2 (see below) reflecting off side 1 and back through the bulk.  I have not subtracted side 1, yet, this is the situation where the homogeneity appears best.

See the Goodrich data at: http://docuserv.ligo.caltech.edu/docs/internal/C/C020137-02.pdf  (yes the first page is blank..oops.) I believe they have subtracted surface 1 in this view.  The blob at 8 o'clock may correspond to what I measure at 12 or 6 o'clock.

The bad news is that the piece appears badly scratched, either that or it has something on the surface that doesn't clean with acetone and methanol.  The surface specifications were waived in this instance because the piece has several bubbles breaking through the surface, Goodrich can't possibly control the bubbles.  However it is interesting to note that most of the "inhomogeneity" now comes from the scratches and circular machining marks.

The other bad news is that they appear to have confused which side they should be working on.  What was a nice 4nm surface on side 1(former) is now the compensatED surface (the new side2) This is proven by the characteristic defects at the bottom of  both upper images at http://www.ligo.caltech.edu/~coreopt/SurfacesPostComp.JPG
This image shows the clockwise change of the surfaces
Surface 1 before Goodrich (upper left)
Surface 1 after Goodrich (now surface 2 the "compensated" surface)(upper right)
Surface 2 before Goodrich (lower right)
Surface 2 after Goodrich (now surface1)

It's interesting that (speaking currently now) the compensating polish compensates for an error polished into Side one (did they try compensation on this surface at one time?), yet the specification calls for the side one data to be subtracted from the inhomogeneity. The exact text of the specification is:
 

"Figuring of surface 2 is intended for compensation of bulk inhomogeneity of the index of refraction of the mirror blank. There is no explicit requirement for the surface alone, only in combination with the bulk material. The optical path difference of the surface/bulk is measured in transmission through surface 2, passing through the material, reflected from surface 1, passing again through the material and again in transmission through surface 2. All requirements under this heading refer to this double pass measurement.

The real contribution of surface errors on surface 1 are removed from this measurement using an independent phase map of surface 1."


I will be in touch with Goodrich regarding these results.



From: Helena Armandula <ahelena@ligo.caltech.edu>

Silicate bonding  - Heavy Glass
Bonded four 1/2" dia. pieces of heavy glass (#24935 from Viox) to fused silica substrates, using a silicate solution.  The parts were not flat to the 1/10 wave specified, so, about a couple of hours after bonding some separation appeared.  Two of the bonded parts were taken apart 4 hours after bonding. I will attempt to correct the flatness on these pieces and re-bond them.  The remaining bonded substrates will be cured for some time before being tested for strength.



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

Suspensions


Mark Barton

Added the corrected thermal noise code to my triple pendulum model, bringing it up to date with the quad model.


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