Weekly Report for Week Ending April 3, 2003


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

The LIGO Executive Committee Agenda for Monday  December 23, 2002 will be:

(Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

1. Announcements
2. LSC Issues (Weiss)
3. Comments on Weekly Report
4. WBS 1 LIGO I Construction (Lindquist)

Field Change Orders/Contingency Liens/Change Requests
5. WBS 2 LIGO Lab Operations
Administration (Lindquist)
Sites (Raab, Coles, Shoemaker, Sanders)
Detector (Whitcomb, Coyne)
Campus Research Facilities (Weinstein (40 Meter), Libbrecht (TNI), Zucker(LASTI))
Data Analysis and Computing (Lazzarini)
6.WBS 3 and 4  Advanced R&D and LIGO II (Sanders)
 
7.CHANGE CONTROL BOARD/TECHNICAL REVIEW BOARD SESSION AS NEEDED Executive Committee only 11:30 - noon   Topics:

Special Items:  The Status of Operations Expenses vs Budgets for 1st Half of FY 2003


Special Announcements:


Weekly Report Highlights  


LSC Issues (Weiss)

No report.


Laboratory Administration (Lindquist)



LIGO Weekly Site Telecon (Lindquist)

There was a site teleconferences held on Thursday, April 3, 2003.  The following issues were among those discussed:

Change Request CR-030003:  This change request is for an OC3 WAN Link from Hanford via ESnet.  We will discuss this during the meeting of the Executive Committee on Monday, April 7, 2003.

Budget Issues: The construction liens list has been published on the web as a part of the report for the end of March.  We will review it during the meeting of the Executive Committee on Monday, April 7, 2003.  The report for the operations funds has also been prepared.  We are running at about 70 percent of budget.

Petty Cash Procedures: Would like to have the bank send the original bank statements and checks to Caltech/LIGO.  Caltech will send copies to the sites.  Ed Jasnow will be doing the reconcilliation. Hanford concurred.  If we change to corporate accounts, may have to start the coporate accounts with new money.  Will try to prepare a set of procedures for petty cash at remote sites.  Should be incorporated into procedure manuals for sites, as soon as those spring into existence.  Action 120.

Ed Jasnow has a previous action (action 118) to discuss with with the P-Card folks the need to update the documentation on the use of P-Cards.  LIGO is authorized to procure things using a P-Card that the rest of the Campus has not been allowed to do.  An list of exceptions needs to be provided for the LIGO rules.

Proposal from Chervenell:  Still hoping to have a quote shortly for the sun shades.  This is the only thing holding up the additional work on the Hanford Laboratory building.

Drainage at the Entrance to the Livingston OSB:  The concrete at the front of the building has an area where water accumulates.  Formulating a plan for a proposal.  Will have a proposal by next week.

Gate at Hanford:  The gate and camera are working in Hanford.  Opens from the control room.  Cost approximately $30,000.

Personnel:  An organization chart has been prepared.  Copies will be mailed to members of the site teleconference committee.

Property:  No excess now.  Have distributed some vehicles and a bucket loader to the city of Livingston.

The list of current actions revised to reflect the status of open actions assigned through December 12, 2002 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

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


DOCUMENT CONTROL CENTER (Turner, Mak)

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

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

ACCOMPLISHMENTS

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

ACTIVITY

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.

COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman)

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

Press here for ACCOUNTS PAYABLE HISTORY DATA .

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

From: Gina Salone <gsalone@ligo.caltech.edu>

Went to Superior Jig March 28 to deliver RFI (Request for Information) for fabrication of Advanced LIGO Suspensions.  Was provided a complete tour of their machine shop.  RFI's provided to three other vendors. Pricing due on or before April 18, 2003.  These will be picked up from the vendors to give the Technical and Engineering Support Group sufficient time to look them over.

Work-in-Process: Overloaded with purchase requests for Construction account materials.  Processing as quickly as possible.

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

Advanced LIGO (Frey)

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

Weekly Advanced LIGO Project Controls meetings was held on Friday the 28th at 8:30am at SCR.

For list of documents that are being used to develop Adv. LIGO Cost and Schedule, see http://www.ligo.caltech.edu/~tfrey/Cost_MTG_082002/

Advanced LIGO MRE Proposal (Highest Priority)

Continue to update the TNI Schedule and incorporate any changes.

Continue to update the LASTI Schedule and incorporate any changes.

Project Plan for the 40-Meter Lab Upgrade continues.

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)

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, core optics, etc.  We have discussed priorities, and the quarterly report will slip.

With Dave Beckett, have been gathering and editing materials for a brochure discussing the current state of LIGO and the plans for Advanced R&D.  Four out of five articles substantially complete.



Change Control/Contingency (Lindquist)

The following Change Requests have been distributed for discussion during the next meeting of the LIGO Executive Committee (April 7, 2003):

CR-030002
Revision A
Adjust FY 2003 Operations Budgets to reflect actual staffing levels
P. Lindquist
April 2, 2003
CR-030003
Implement an OC3 Wide Area Network Link fro Hanford via ESnet
A. Lazzarini/L Wallace
April 2, 2003

The following Change Request was discussed and approved for $125K during the Exective Committee meeting held on March 24, 2003:

CR-030004
Provide funding for Storage Building at Livingston Site                    
A. Sibley                     March 24,    
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.


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


Summary of S2 Science Run Activities at LIGO Hanford Observatory (compiled by M. Landry)

We are extremely pleased to report that Otto Matherny has returned to work at LIGO Hanford.  Otto has started back at 20h per week, but characteristically exceeded that goal since Monday.  Welcome back Otto.

We also extend a welcome to Akiteru Takamori, who has joined the commissioning efforts at LHO for approximately four months.

Joe B and Nergis M studied the variation of the H1 calibration on short time scales, finding second-to-second fluctuations of +/-1% (mag) and +/-1.5deg (phase): Click Here

Both 2k and 4k arbitrary waveform generator (AWG) processors, which produce the waveforms for calibration lines, failed several times (in uncommon fashion) and had to be rebooted.

FB0's external raid disk failed, however no minute trend data were lost, thanks to FB3.

Duty cycles for the week: H1 (0.78), H2 (0.67).  Seismic events, both highly localized to the LVEA, and those due to remote earthquakes, continue to regularly unlock the interferometers.


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


S2 Update: The interferometer continues to operate at around the 40% level, a value roughly constant throughout the run. Most recently, that value has fallen to around 38%. Daytime operation has been negligible the last few days, with high seismic backgrounds. Today, the background was unusually high in the 0.3-1.0 Hz band. We have also had some hardware failures this past week. The end station controllers both burned out, likely due to attempting to operate in a demanding seismic environment. Ken Watts promptly repaired the controllers and restored them to operation. When the ground is quiet, the interferometer continues to run well. Last night we maintained lock for about 6 hours with an in-spiral range consistently above 1.1 Mpc.

Seismic Isolation System: I have continued to support Larry Jones with information regarding the inertial sensors and more recently information to support spring rate claims for the ETF and EPI efforts. Monday, the LIGO SolidWorks users group had the inaugural meeting and discussed Concerns about an enterprise solution for digital content configuaration control as well as storage. We have been trying to find ways to share electronic data for sometime, and are coming close to a solution. We also decided to upgrade our Software to SolidWorks 2003. (Marcel)
 
End-to-end Model: We continued modeling of suspension dynamics with e2e. We simulated the motion of a pendulum set up on campus using e2e and compared the result with mesurement. The transfer function measured for the yaw degree of freedom shows reasonable agreement with the simulation. The ratio between the peak value and the tail value at 3.3 Hz agrees with the simulation with +/-10%. (This pendulm has pend/yaw/pitch peak at 1.05/1.3/3.3 Hz). The experimental curve shows a peak near the natural frequency of the pendular motion, indicating coupling between pendular and yaw motion. (T. Findley and S. Yoshida)

General Computing: Investigating options for the switches at the end stations. These had to be shut down before S2 because of accoustic noise. I called and spoke to one of the engineers yesterday and he told me that Foundry is aware of the problem and they are working on it, however this will continue to cause major problems on my network until this can be solved.

Looking into some Mathematica issues. Tom is going to call Wolfram and change the license, but there are still some font issues.
Added security pathes to several machines at LLO. There has to be a better way of managing patches now that we have so many machines.

Talked to a friend today that works for Cox cable to revisit some possibilities of getting increased bandwidth to the observatory.
Started reading the documentation on updating the software on the PIX since it has been having a few problems lately. I have had to reboot the PIX twice in the last three months because it stopped passing any packets to the internet.

Ordered several Matlab licenses for some additional toolboxes, etc.

Ordered a laptop for Chethan. Dell canceled the original order.

LDAS: Checked into the dual processor AMD systems with Angstrom Microsystems. They also offer two dual processor units in 1U of rackspace. However, due to time constraints and other reasons that are architecture dependent, Stuart says that this will not be a realistic option. (Shannon)

LDAS admin: The new tape robot is mostly installed, still waiting for tapes.

LDAS data analysis: Working on single pixel clusters and coincidence with time-frequency window in waveburst. (Igor)

CDS: (Ash)

ROBO-SCIMON's TWIN is successfully doing his automatic e-logging of Figure-of-Merit displays at the end of each shift. Dave is thinking of setting up this at Hanford. ROBO-SCIMON's TWIN will be getting his brains soon and will do intelligent logging of noise spectrum when the ifo is locked. Setup an automatic script to download latest applications for sun workstations. Working on porting the Matlab Dataget code to Windows environment. DVD_Robot backup is working well and used for backups. Planning on re-configuring london and river after S2. S2 has gone well in terms of software and CDS issues. No major problems reported. Systems have been up for above 97% of the time.  (Chethan Parameswariah)


Detector/Technical Support (Coyne)


DETECTOR SCIENCE & ENGINEERING

Seismic Upgrade Project

See LASTI report

Preparing for review on 18 April.

CDS Software

(Rolf Bork)

1) LSC code updated to include addition photodiode correction filter banks and outputs; undergoing testing with 40m system.
2) New digital suspension software for 40m lab should be ready in the next few days. Still to do:

3) Started testing digital IO WFS system. This should be ready to install at 40m lab early next week.

4) New Linux dataviewer was built to run on Linux 8, but seems most people who want to use it still run Linux 7. We are rebuilding a PC here to run Linux 7 and then get dataviewer to work on this older version.

CDS Hardware

(Rich Abbott)

1.  The ISS CAD files will be ready before the end of this week and will be at the board house for rapid manufacture.  We are planning to get everything together so we can do performance checks at LLO during the week of April 21.

2.  Ordered two HP network analyzers for the site as well as various RFI related antennas.

3.  Preparing for trip to work on seismic pre-isolator next week

(Jay Heefner)

LOS Coil DAQ Whitening: The schematics are complete and have been sent out for comment. Once comments have been received the board layou will be started.

PSL

(PeterKing)

The dark noise of the latest revision of my high power photodetector was measured.  Although the measurement was limited by the output noise of the SR785 dynamic signal analyzer, a rough inspection indicates that at 10 Hz, the dark noise is 1 nV/Sqrt[Hz].  Which is about a factor of 2-3 better than previous prototypes.  The dark noise spectrum has a peak at 23 MHz which was not present in the other prototypes and a few other small peaks beyond 100 MHz.  I am not sure why this is but some extra capacitance in the previous prototypes may have masked this out.

The photodetector was then taken out for a test drive.  With an output consistent with a photocurrent of 175 mA.  It was left running at this level for about 30 minutes.  No detrimental effects were observed to the photodetector, although the 5W feedback resistor did get a trifle warm every other component seemed okay (ie, was okay to put your finger on).  The dark noise was measured again and was found to be the same.

A low-noise amplifier is in the beginning stages of fabrication.  The difference between this one and the previous one is a number of component values are different.

Earthquake Stop Redesign

(Janeen Romie, Mark Barton)

The earthquake stop stuff is still on hold pending replacement of damaged magnets. (It turns out that the old test optic does not have the complement of scribe lines to allow the magnets to be properly positioned with the new fixture, so they're being added.) In the meantime I've been working on references and a section on electronics for the LIGO I suspensions paper.

Helena has glued the guide rod and wire standoff on the optic. On Monday, Mike in CES scribed lines on the barrel of the optic, 90 deg apart, so we could orient the magnets and wire standoff. I'll glue the magnets this evening or tomorrow morning.

Errant Beam Blocks

(Mike Smith, Ken Mailand)

Polished aluminum sample plates were electro-plated with Ni and produced an excellent mirror surface with negligible visible scattering of a red laser beam; this will be our preferred substrate for the MMT1 baffle/beam dump. Super-8 mirror-polished stainless steel sheet is also an excellent mirror surface with negligible visible scattering of a red laser beam; this will be our preferred substrate for all of the other errant beam baffles. A sheet of super-8 mirror-polished stainless steel was purchased and is at a laser cutter facility awaiting instructions for cutting. Bids are still being received for an absorptive coating on the baffle substrate.

Ken is working on the detailed drawings of the baffles. Mike is in the process of establishing the reflectivity and BRDF requirements of the errant beam baffles, and writing a requirements document. The MMT3 baffle and the baffle near the RM may cause phase noise due to the light scattered from the symmetric port beam back into the IFO; an estimate of the scattered light phase noise is being calculated.

*** Note by D. Coyne: Mike Smith will present the design requirements and concept at Monday’s commissioning telecon as part of a Revision Technical Review Board (RTRB) review.

Optical Contamination Cavities

(Lee Cardenas, Liyuan Zhang)

OTF Lab. (W. Bridge):
Contamination Cavity # 1
The test sample. CHEM-SOL Hydraulic fluid still pumping until the end of this week.  We are taking ring down and beat frequency measurements everyday and so far we can tell that there is no contamination.  Please see Dr. Zhang for graphs for absorption, ring down and thermal lensing.

Absorption Test Measurement prototype: on hold..

Scatterometer:
The function of the scatterometer has been fully recovered as mentioned before.  A preliminary result of our measurement of the AR reflection for the large mirror ITM S/N 4ITM08 has been released. The reflection of the AR coating averages ~1330 ppm.  We have also finished taking measurements for the reflectance of the HR coating.  New and more precise alignment is in progress as we are changing the optical mounts
and new mirrors are being replaced.

OTF Lab at Lauritsen ROOM 38:

Cavity #3
The new test sample SR FR HF from Chem-Sol, Inc. is an Undyed Fire retardant Hydraulic Fluid. We are taking ring down and beat frequency measurements everyday.  Please see Dr. Zhang's for latest graphs for absorption, ringdown and cavity thermal lensing measurements.

Cavity #2 Test cavity
The chamber is pumping with new cleaned mirrors ~ 70ppm each. RGA measurements and optical train set-up is in standby.  The new contamination chamber has been baked (40m South Annex).

New View port windows with a 5 degree wedge  quote from a vendor has been received.  Each will cost $1330. plus one time charge for tooling $600.  We need a minimum of six for three chambers.


40 Meter Interferometer (Weinstein)


Dennis and Osamu are both on shift at LHO all this week.

Suspended optics: We are preparing to suspend our two ETMs in the next couple of weeks, and shortly thereafter, our two recycling mirrors, completing the suspended optics for the 40m.
PSL and ISS (O. Miyakawa, B. Abbott, R. Abbott, F. Nocera, D. Ugolini, S. Vass, C. Mow-Lowry):
Suspended mass mode cleaner (Ugolini, Miyakawa, Vass, Abbott):
The Digital Suspension Controllers are being rebuilt this week, and Osamu and Dennis are at LHO, so there's been no work on the MC.

Core digital suspension controllers (DSC), MC WFS, and other Electronics (B. Abbott, Heefner, Bork, Taylor): Optical sensing (Smith, Ourjoumtsev, Goggin, Miyakawa): Facilities and vacuum envelope (Ugolini, Vass, Jones): South Annex Bake Ovens (Taylor, Cardenas):


Thermal Noise Interferometer (Libbrecht)
We did a noise breakdown of the two cavities, including:

  1. Electronic Noise - Measured
  2. Mode-cleaner Seismic Noise - Measured
  3. Shot Noise - Not measured; photodetector noise dominates due to low laser power. That is the relevant noise source at these power levels, so it was measured instead.
  4. Laser Frequency Noise - Estimated, but checks on mode-cleaner error signal reveal potential problems (see below)
  5. Laser Intensity Noise - Still to be measured
  6. Pendulum thermal noise estimate - done, based on
a. Loss angle in wires ~3e-4 from Gillespie and Raab, Phys. Lett. A (190) 213-220 (1994).
b. Pendulum Dilution Factor <1e-2, from Saulson, Fundamentals of Interferometric Gravitational Wave Detectors, p. 122(World Scientific, 1994).
The results are shown in the following plots:

TNI NAC Sensitivity

TNI SAC Sensitivity

Photothermal Expansion

We also investigated some mode-cleaner pathologies:
  1. UGF measured, found to be 90kHz at present gain settings, but transfer function deviates from prediction as frequency approaches 100kHz from a substantial loss of phase.
  2. Lightwave 126 PZT resonance expected around 130kHz (Peter King, private communication), which could account for loss of phase.
  3. Need higher-frequency network analyzer to measure transfer functions above 100kHz. Obtained Agilent 4395A and started setting up. Measurements to follow.
  4. Free-running laser frequency noise checked by mode cleaner's error signal with all boosts off. Some increase in noise since last measurement (Fall 02), but not significant.
  5. Mode cleaner's error signal with all boosts on does not agree with predictions.
We did an arm-cavity calibration check: Measured electronic transfer functions in both NAC and SAC.

On another front, the photothermal experiment has interesting results, showing excess thermal expansion towards the upper end of the LIGO sensitivity band due to the mirror coating.

We measured the photothermal response for two specially prepared mirrors. One is a sapphire flat with a 180nm gold coating (to increase optical absorption). The other is a 30-layer high-R sapphire-backed mirror, also with a thin gold coating. At 4 kHz, where the thermal diffusion length scale is a few microns, the sample with the HR coating has 50% more expansion than expected by the standard photothermal model.

In the attached picture, the orange dots are consistent with the theory of the photothermal effect. The divergence of the blue dots are more consistent with a f-1/4 spectrum at high frequencies. We are working on a model to explain this, possibly including thermal expansion and 'bimetallic' expansion stress. (see Braginsky and Vyatchanin's new paper, arxiv.org/cond-mat/0302617)


LASTI (Adhikari, Coyne, Hammond, Kern, Mason, MacInnis, McKenzie, Mittleman, Ottaway, Rollins, Shoemaker, Zucker)

MEPI: Myron, Ken and Bill completed the modification to the alignment shims under the remaining MEPI piers, and Bill re-measured their mechanical transfer functions.  As Rich had predicted from the exploration done last week on the first pier, the most troublesome resonances are all greatly improved. This should allow a significant improvement in the MEPI bandwidth and noise suppression (stay tuned).

HEPI: Brian Lantz isolated a noise problem due to some electrical interference with the pump controller; this prevented the sensor correction from working properly by swamping the required coherence between ground motion and pier motion with common-mode pressure noise. Good suppression performance has now been recovered and the controller is being re-optimised to improve it still further. Also, additional geophones have been added to the internal BSC payload to map its response in more degrees of freedom.


Data Analysis and Computing (Lazzarini)


Simulation and Modeling (Bhawal)
E2E Physics meeting: Malik talked about the FP dynamics at FSR and at SB resonance. Rick Savage presented some more experimental details. Reproduction of these results in e2e and other models was discussed (also see below).

France Trip:
Biplab attended Moriond workshop on Gravitational waves and Experimental Gravity and gave a talk on E2E.  He also demonstrated E2E's capabilities and runs in laptop to interested participants in the workshop. Biplab also visited the Virgo groups at Observatoire Cote d'Azur, Nice and Laboratoire Accelerater Lineare at Orsay and gave talks and e2e-demonstration there.  Several Virgo scientists showed interest in using it.

FP dynamics: Malik and Rick measured FP dynamics at modulation frequency around FSR.  Hiro and Biplab used e2e and twiddle to reproduce the measurements to validate the model. One caveat is that the summation cavity showed a limitation to simulate this high frequency region.

Radiation pressure modeling: (Hiro) The radiation pressure module is tested more and will be committed to the standard code library soon.

Seismic motion: Matt finished the matlab code to generate e2e code to simulate the coherent seismic motion. Hiro received the code and starts using it to generate the actual code with the input provided by S.Yoshida.

Noise Paper: Matt wrote a LIGO note summarizing the sensitivity curve produced by the SimLIGO model. T030063, "Noise Hunting in SimLIGO"

Code development and maintenance: (Melody)
Alfi: (Bruce)


LIGO Data Analysis System


Software Systems (Lazzarini for Blackburn): Work this week has been  focused on finding the cause of mpiAPI lockups in 0.6.0+ versions of LDAS and tested various work-arounds. As a current measure in order to support a release for the post S1 analysis, we have settled on a strategy which avoids the use of lam inspection utilities which seemed to be interfereing with lamd communication. The was also work to support  Greg Mendell to develop a 'self-expanding' user command that uses a simple syntax to replace complex user commands with repetetive structure.  A user command 'sftPipeline' is currently being tested which makes use of this expansion mechanism. This will help improve user friendliness for the CW effort he is leading. The software team also worked with Kaice Reilly to identify shortcomings in  the option parsing and handling of the datacond API. We determined that support for simultaneous writing of products to disk and sending to the wrapperAPI was not satisfactory.

There was discussion about improved data  caching strategies which could be used to speed up the control and monitor API with Mary Lei.

The ligolwAPI is being ported to the xercesc-2.2.0 xml library.

In the area  of SW testing,  stand-alone documentation was updated  to include a list of required RedHat updates.  This activity was to close an open problem report.  A new feature for cmonClient was developed to allow the user to send sample jobs to LDAS.  I provided some scripts to her which are based on my test scripts. There is ongoing work on documentation that will describe how to reinitialize the test database after it is cleaned out. From Monday through Wednesday the ldas-dev system was exercised with a mpiAPI from version 0.5.0to verify the assumption that a later bug has been responsible for the lately observed instabilities.  This is related to the ongoing mpiAPI work mentioned earlier.

The metadataAPI  has been improved to eliminate the slave interp and saving of data in jobid array as prescursor to providing enhanced threading capability for this API.

The CIT systems is in use producing reduced data froms S2 raw frames.  We also followed up a suspected problem with downsampled reduced data.  Erik Katsavounidis reported some differences in results when looking at triggers produced by auxiliary channels in DMT on reduced vs. raw data.  After scrutiny, it is believed that the differences are probably not an LDAS bug but are caused by the fact that on the raw data no downsampling was done before going to the DMT, while on RDS frames the data had been downsampled first.

Worked with the ANU group ( Antony Searle and Eric Rothoff) to inform them of release schedule for LDAS and request their updates as soon as tested & documented.


Hardware Systems (Anderson)

Caltech:

(Al Wilson) (Stuart Anderson) Livingston:

(Igor Yakushin) (Shannon Roddy) Hanford:

(Greg Mendell)

Data Analysis Activities (Lazzarini)


(Mendell)
(Yakushin)  LDAS data analysis: working on single pixel clusters and coincidence with time-frequency window in waveburst.

(Shawhan)
(Charlton) Working on FCT paper.
(Weinstein)
(Creighton)  This last week I finished an article on Advanced LIGO sources and astrophysics for the GWDAW2002 proceedings.  I have started preparing the LIGO seminar talk on pulsar upper limits from S1.  I also helped sort out some confusion with simulated heterodyned pulsar signals with the UWM group.


General Computing (Wallace)

MIT:  (Keith) Nothing to Report

Livingston:
(Shannon)
Hanford:

(Christine)
(Larry)
CIT:

(Lisa)
(Veronica)
(Mike)
(Larry)

LIGO II/Advanced R&D (Shoemaker)


Seismic Isolation

From: Dennis Coyne <coyne@ligo.caltech.edu>
 
Performed a frequency analysis of the quad suspension structure to help establish a design concept and a mass for SEI payload mass property requirements. The analysis is documented in LIGO-T030044-02. This document is temporarily available here:
http://www.ligo.caltech.edu/~coyne/AL/SUS/T030044-02.pdf until it is filed in the LIGO document archives.

Revised layouts for the non-folded interferometer have been established (optics tables in chambers HAM1, HAM3, HAM4, BSC1, BSC2 and BSC3; not yet the ETM chambers). These layouts have been used to get payload mass properties and are being used to establish the balance weight distributions and the SEI payload mass property limits for the SEI structure RFP. These layouts and final payload mass property estimates/limits will be documented soon in a system, configuration controlled interface document.

Suspension

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

Caltech Suspensions Summary:
Mike Perreur-Lloyd and Calum Torrie designed a rotational adjustment for the upper blades on a triple suspension while Mike was here on his last visit. The rotational adjuster is based on a design created by Alastair Grant for the MIT quadruple pendulum.

Dennis Coyne has performed detailed frequency analysis of the quad pendulum structure and has created a preliminary report of this. Ask Janeen or Dennis for a copy, if you're interested.

Recycling mirror blade drawings are ready for the RFQ process. The design of the RM upper mass is complete but for review of stiffness and deflection.

The mode cleaner drawing packages were delivered to three local machine shops for quote information to support the AdLIGO proposal.

 AdLIGO Suspensions:
Caroline Cantley from the Glasgow group will be visiting us here at Caltech next week, April 7-16. We'll be working on the triple structure stiffening and FEA along with the quad structure concepts. We look forward to her visit.

Still interfacing with Dennis, Larry, Norna and Florida people on optical layout issues.

The Solidworks User Group met on Monday and we are all working to different vrsions and types of licenses. We've recommended 2003 Research. We'll meet again in a short time.

The three notebooks of mode cleaner drawings were dropped off with vendors for quotes. We should receive information in 3 weeks time.

Gin Gin:
Ed Chargois has gotten a packing crate ready for us to ship the ITM suspension to John Jacob. We're just waiting for the reworked controller to check out the damping then we'll box the whole thing up and send it. I've completed the top assy drawing for the ETM suspension and only have the magnet fixture drawing to finish and submit.

Earthquake Stops:
Helena has glued the guide rod and wire standoff on the optic. On Monday, Mike in CES scribed lines on the barrel of the optic, 90 deg apart, so we could orient the magnets and wire standoff. I'll glue the magnets this evening or tomorrow morning.

40m:
Today, Bob Taylor is going to clean and bake the last earthquake stop screws that are needed. I reviewed the suspensions and they look ready to go but for these screws.

 From: ctorrie ctorrie@ligo.caltech.edu

Recycling Mirror:

The cantilever blades have been designed for the Recycling Mirror suspension and are ready to go out for requests for quotes.
The majority of the work on the RM suspension will be put on hold so we can concentrate on the prototype quadruple suspension assembly.

Mode Cleaner:
Aluminium heads with an anodized layer for the hybrid coils, to replace the stainless steel heads are under production in Glasgow. The first step will be to get 3 or 4 made and cycled through the machining and anodizing steps before a batch of ~32 are made. The 32 will be used on the RM, MC and a vacuum test for the anodized layer. At the same time Glasgow are looking at PEEK 1000 as an alternative material for the head.

Helena and I have been working on various upgrades to the Mode Cleaner suspension including increased adjustment for the hybrid coil assembly, back up isolation for the coil head using KAPTON, Macor and Teflon, stops for the lower blades and an alignment mechanism for the dummy aluminium intermediate mass.

Quad Suspensions:
When Norna Robertson returns we hop to move forward with the design of a quadruple pendulum suspension, with stages of 22-22-40-40 kg.  Mike PL and I have started to look at the assembly of the upper mass.

SOLIDWORKS:
See report by Janeen Romie.

Visit:
Caroline Cantley from the U. of Glasgow will visit Caltech next week, from the 7th to the 16th of April,  to work on and discuss various aspects of the prototype suspensions currently being built and designed here at MIT

Pre-stabilized Laser

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

A memorandum about the recent PSL technology downselect was circulated by Benno Willke for preliminary comments. 

Input Optics

No report.

Core Optics

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

Having completed our series of Q measurements on the two large sapphires, one has been shipped to Lyon for optical testing, while the other is staying in our lab to allow for mode identification, which we plan to do using a Chladni experiment.

Meanwhile, we have made a first attempt at measuring the Q's of a spare LIGO I input test mass, ITM11.  This mass is polished, but is not coated and has no wedge.  Most of 26 modes we measured have Q's in the uninteresting 10-30 million range; however, the lowest-frequency mode we found (actually, a doublet with 10mHz splitting) has a Q of 53 million.  While this result is not so spectacular compared to other results in fused silica lately, this is pretty high for a LIGO optic, one that has been mechanically polished, but not annealed or flame polished.

Auxiliary Optics

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

The polished, absorbing baffles that are being developed for the errant beams are a prototype baffle for Advanced LIGO.

Interferometer Sensing and Controls

No report

Data Acquisition, Diagnostics, Network & Supervisory Control

No report

Other Laboratory R&D

From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>

Last week LSC

(Riccardo, Eric, Allyson, Valerie)
Presentations at Career day at Mayfield H.S.
http://www.ligo.caltech.edu/~desalvo/EricATMayfield.ppt
http://www.ligo.caltech.edu/~desalvo/AllysonATMayfield.ppt

(Allyson)
Made SEM photos of indentations of missing concentrations. Measuring.

(Eric)
Big step forward in modified MoRuB recipe. Achieved the required crystalline structure in crystalline state. X-ray measurements to complement Brians work, calibration and analysis of the apparatus.  Melted balls for Hareem tests on splatter.

(Hareem)
Retuning splatter. The coil gets continuously polluted by the people using aluminium and other low melting alloys. Installed new clean coil. Almost retuned. We may need to protect the coils with Kapton coatings in Pisa to preserve the coils and not having to clean and retune them all the time.

(Alessandro)
Providing informations to G&M to build the TAMA towers for University of Napoli.  Proceeding with Ultrasound milling machine testing and improvements.  Sent Stefano's AgSn brazed MoRuB sample to Roma.

(Riccardo)
Disassembling prototype of TAMA tower for shipping to Pisa.


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