Weekly Report for Week Ending
April 3, 2003
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
- CR-030002 Revision A, Budget Adjustments
to reflect actual staffing levels for first half of FY 2003
- CR-030003, Implement an OC3 WAN Link from
LHO via ESnet
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>
- Provided support to the Detector Group (G. Billingsley) with packing
and shipping of one (1) Fused Silica) 128mmx53mm and one (1) Axis 120mm x
80mm to Wave Precision (J.Tardif), Moorpark, CA. Account Number P204296.
- Provided support to the Detector Group (M. Smith) with packing and
shipping of a defective Glan Brewster Angle Polarizer to VINOD VATS (K. Lambrecht),
Chicago, IL. Account Nunber P205472.
- Provided support to the Data Analysis Group (S. Anderson) with packing
and shipping of a FastIron Evaluation Unit to Foundry Network (D.Allen), Alviso,
CA. Account Number P204261.
- Provided support to the Detector Group (M. Smith) with packing and
shipping of two Laser Mirrors to CVI Laser Corp. (T. Bradiger) Albuquerque,
NM . Account Number P205472.
- Provided support to the Detector Group (H. Armandula ) with the shipment
of two (2) Transit Case to LHO (D.Cook). Account Number P204324.
- Note: Four (4) Pickup Trucks and One (1) Forklift were donated to
the City of Livingston 3/27/03. [This was excess property donated with
government approval. --pel]
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
- Reminder
to LIGO staff: Please make sure that as a minimum, each document submitted
has a LIGO number, author's name, and date. It's surprising how
many documents are missing one of more of these essential pieces of information!.
> From: Cleveland Mak <mak_c@ligo.caltech.edu>
ACTIVITY
- Processed a handful of
LSC documents still trickling in. Electronic document activity was fairly
steady. Created file folders, sorted and filed documentation.
DCC Activity
| WE 04/03/03 |
Packages |
Faxes |
| In |
33 |
38 |
| Out |
16 |
30 |
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>
- Working on Change Order #8 to Sydney Meshkov, Change Order #21
to Excel Group, and Change Order #2 to Excel Group (T & M).
- Placed Pcard orders. Reconciled Pcard orders.
- Working on the Landscape Horizons maintance for the LHO facility.
The new maintance agreement covers the area landscaped by Heritage, and the
new landscaping by Landscape Horizons.
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>
- Completed and posted the monthly financial reports for March on
the network.
- Completed the report for the Visitor account for March and gave a
copy to Donna Tomlinson.
- Completed and posted charts comparing FTE's budgeted vs. actuals,
one by account charged, and the other by employee type.
- Met with Ed Jasnow to go over suggestions for recommended procedures
for petty cash accounts.
- Prepared schedule of budget staffing adjustments for the first six
months of the fiscal year.
- Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
SUBCONTRACTS MANAGEMENT (Petrac,
Jasnow)
From: irena@ligo.caltech.edu (Irena Petrac)
- Univ. of Florida: Proposal was received for continuing on-site
support at LLO through 2006. Contract modification is in the works. CO
14 adds funds for two new scientists through end of April 2006. The scientists
will be resident at LLO.
- RFP/SEI Mechanical Structure: Release of the solicitation is pending
definitization of design requirements.
- Quarterly Report/Coop. Agreement/LIGO Construction: The last Quarterly
Report (for period ending Feb., 02) has been delayed due to other priorities
(new procurements and LSC).
From: Ed Jasnow <jasnow@ligo.caltech.edu>
CONSTRUCTION:
- We are still waiting for the final proposal from Chervenell Construction
for the modifications to the LHO Laboratory Building. Additionally,
a propoal will also be sent for paving of the parking lot.
- A design is being prepared for a new drainage system for the front
of the LLO OSB. This will remove the problem of standing water.
- The final design for the LLO access gate is expected next week.
OPERATIONS:
- A new written procedure will be issued for the operation of petty
cash accounts at both sites.
SUPPORT (Baldon, Torres, Lloyd,
Tischler)
>Irene Baldon
- Processed the paper work for two (2) new/revised trips.
There are sixteen (16) trips in various stages of completion before ticketing
can be done and/or paper work completed. Also assisted a number of
P-Card holders with their travel plans/reservations or revisions. Until
further notice I will be doing travel for LHO travelers.
- Completed thirteen (13) Expense Reports and there are three (3) reports
yet to be done. I continue to contact travelers who have outstanding
Expense Reports (more than one (1) month old) to ask for their cooperation
in sending me their receipts so that they can be closed in a timely manner.
- Reconciled eleven (11) P-Card items which required numerous phone
calls to hotels, car rentals, etc., in order to track down which traveler
incurred which charge; and the pulling of each traveler's file to assure
that charges are correct for each fee incurred. Assisted a few travelers
with their questions in regard to their P-Card and/or reconciliation.
- I continued to collect a few EFT stragglers and hope that more will
come. It is anticipated that this pilot program will now start up by
May 1, 2003. Your cooperation in promptly returning the form to me (Irene
Baldon, M.C. 18-34), filled out, with a VOIDED check or deposit slip attached,
is greatly appreciated.
- Worked on the preparation and distribution of the Travel/Vacation
Itinerary for March 31, 2003. Arranged three (3) new teleconferences;
arranged cancelation for two (2) meetings for this week; and entered four
(4) new reservations on the LIGO Calendar. Performed normal recording
and filing associated with Travel and Reimbursement.
- I continue to do MIT's travel to the sites for installation activities
and also to assist them wherever possible.
>Dorothy Lloyd
- Processed the usual invoices for payment. Tracked and followed
up on invoice problems. Reviewed and recorded payments processed by Esther
the week of March 24.
- Processed the usual requisitions, change orders and payment requests.
- Continue to monitor contract and blanket order encumbrance and notify
task managers when supplements are needed.
- Jim continues with data entry in the LIGO database and helping out
in the DCC.
>From: Ryan Tischler <rtischle@ligo.caltech.edu>
- Set-up laser eye exams for new LIGOites this week. Worked
with B.Tyler/CIT Safety to set-up laser safety training. Organizing
photos from various CDs to turn over to D.Beckett. Scanned some documents
for submission to DCC. Draft newsletter articles for March/April. Gathered
originals for sites re: press kit inserts.
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 work on revisions / corrections to the Adv. LIGO
cost profiles and will generate budget sheets for review by Phil.
- The following is a summary of status by sub system:
- COC - Still need completed WBS dictionary and BOE.
- PSL - No action items pending.
- AOS - Still need completed WBS dictionary and BOE.
- IO - Still need completed WBS dictionary and BOE.
- SUS - No action items pending.
- Updated the plan with progress as of 03.28.03 and posted
to site.
- Sent out update data requests for progress as
of 04.18.03.
- SEI - Received revised (Version 3) data from Dennis and
data input of WBS and BOE is in progress.
- ISC - Still need completed WBS dictionary and BOE.
- LDAS - No action required at this point in time.
- INSTALL - Dennis provided a revision and data input is
in progress.
- DAQ - No action required at this point in time.
- PM - No action required at this point in time.
- FAC - No action required at this point in time.
- SUP - Need estimate for support equipment. Action
item to be executed by Dennis.
Continue to update the TNI Schedule and incorporate any changes.
- No update issued. Revised baseline pending action
by Eric Black.
Continue to update the LASTI Schedule and incorporate any changes.
- No update issued due to lack of data. No direction
provided to date regarding a revised plan.
Project Plan for the 40-Meter Lab Upgrade continues.
- Updated the plan with progress as of 03.28.03 and posted to
site.
- Sent out update data requests for progress as of 04.18.03.
Cost Book Tool.
- ROSTER DATABASE:
- Working with Larry and Barbara to set up a process by
which the roster database updates selected alias lists.
- BK is continuing work on action items.
- Continued input of supervisor, dept., and specialty codes.
- Providing assistance to Irena on a as needed basis.
- COST BOOK DATABASE:
- BK is continuing work on action items.
- Started work on preparing format for hard copy version
to be submitted for NSF reviews.
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>
- Various personnel/payroll /HR related work.
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)
- Prepared the design and implementation documentation for the Digital
Suspension Watchdog System.
- Attended the Scimon duties for the thursday and sunday shift.
- Made progress in developing diagnostic routines to help operators in
the control room
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:
- Waiting new high speed reflective memory boards. Call last Thursday
said they were shipping, but just received call today that they have not
shipped yet. They will ship today.
- Waiting rack mount 3.0 GHz P4 processor (should arrive today).
- Finishing cleanup work on timing diagnostics and data acquisition/GDS.
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.
- Helena cleaned the two ETMs. They are ETM02 and 03. Their radius
of curvature are very close, 59.92m and 59.75m respectively. The magnet/dumbell
standoffs are also assembled. She went over the bonding procedure with Steve.
- Bob is cleaning and baking the last earthquake stop screws that are
needed for the MOS suspensions
- Bob has fully assembled the two MOS and two SOS suspensions. Janeen
reviewed the suspensions and they look ready to go but for these screws.
PSL and ISS (O. Miyakawa, B. Abbott, R. Abbott, F. Nocera, D. Ugolini,
S. Vass, C. Mow-Lowry):
- The beam on the FSS RFPD is jittering, causing the signal to fluctuate.
Conor has been investigating. Conor made several changes to the PSL table
around and downstream of the AOM. There were two major concerns: (1) The
beam jitter of the double passed AOM beam and (2) Fluctuating power levels.
Conor increased the RF drive to the AOM through the VCO from 3.50 Volts to
5.00 V, realigned the AOM, and aligned the beam as close as possible to the
PZT side of the AOM crystal. These three actions resulted in an increase
in single pass efficiency through the AOM from 40% to 75%. After realignment
and iterative adjustment to the retro-reflector angle and the AOM angle,
a maximum double pass power of 19.3 mW was obtained, form a 31.5 mW incident
beam. This is a double pass efficiency of around 60%. The beam jitter appears
to be gone, but this requires further investigation. The single- and double-pass
power fluctuations are still present, but appear to be significantly reduced.
It may be necessary to translate the AOM along the propagation axis to ensure
it is at the beam waist. After all these changes, the FSS will have to be
re-optimized.
- Ben is working on a final design, layout, and packaging for the ISS
DC PD. He hopes to have it to the board house by Friday.
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):
- Ben and Bob are rewiring the DSC system. They have finished the crate
and module rearrangement, and the cross connect re-wiring, on 1Y4 and 1Y5,
and will go on to the back panel and front panel wiring starting today.
- Jay has modified the system drawings for the IO WFS rack to combine
two VME half-crates into one split-backplane crate. This crate collects signals
from the IO WFSs through Pentek ADCs and thence to a linux box via RM for
ASC filtering, sends signals to the IO PZT steering mirrors through a Pentek
DAC, collects fast signals from the PSL through an ISC110B and thence to
DAQS via RM, collects the MC length control signal from the MC servo through
Pentek ADC and thence to the DSC system via RM. The other half of the crate
is an EPICS IOC for signals from the PSL and MC.
- From Rolf: LSC code updated to include addition photodiode correction
filter banks and outputs; undergoing testing with 40m system.
- From Rolf: New digital suspension software for 40m lab should be ready
in the next few days. Still to do:
- Waiting new high speed reflective memory boards. Call last Thursday said
they were shipping, but just received call today that they have not shipped
yet. They will ship today.
- Waiting rack mount 3.0 GHz P4 processor (should arrive today).
- Finishing cleanup work on timing diagnostics and data acquisition/GDS.
- From Rolf: Started testing digital IO WFS system. This should be
ready to install at 40m lab early next week.
- Jay reports that the system drawings for our LSC / ASC system are
around 90% complete.
Optical sensing (Smith, Ourjoumtsev, Goggin, Miyakawa):
- OPTICS PARTS LIST, Orders pending: Input mode-matching telescope off-axis
parabolic mirrors are expected first week in April from SORL; repair of
two damaged tilt platforms expected first week in April from Piezo Jena;
1 q-switch E/O shutter from Fast Pulse; 1 Brewster's angle polarizer for
SPS anamorphic prism steering mirror from KLC; Brewster's angle polarizer
mounts for the Faraday isolator are in process; spherical mirrors for MMT
are expected from CVI in a few weeks; Guoy phase lenses for IMCR are expected
from CVI in by 4/7; replacement power connector for the 4 W 940n from Applied
Optics is expected by 4/7.
- FARADAY ISOLATOR: Working drawings for the Brewster's angle polarizer
mounts for the Faraday isolator were completed, and parts are being manufactured.
- OPTICAL LEVER ASSY: Reworked parts were received and are awaiting
checking and assembly.
- IFO STEERING MIRRORS: Parts are awaiting checking.
- MODE MATCHING TELESCOPE: Replacement power connector for the missing
power cable for the 4 W 940nm alignment autocollimator laser was ordered.
Awaiting telescope mirrors.
- INTEGRATED LAYOUT DRAWING: The ILD was revised to incorporate the
new Brewster's angle Faraday isolator, the SOS anamorphis prism mirror,
and the revised SPS beam path.
- Mike has ordered some replacement Guoy telescope lenses for the IO
WFS, that are still missing.
- Alexei has made one electro-optic shutter (EOS) work. He resolved
some questions about how to wire up the Q-switch, and where to ground it.
The EPICS controls are not yet ready, so he's patching around that with an
old 24-volt power supply and a function generator. He tested the EOS controller
box, and works ok for a while; after about 10 minutes, it no longer send
the correct gate signal to the pulser. But until then, he can adjust the
HV and observes the output power to vary from near-zero to near-max. He is
optimizing the HV and alignment. After resolving all the remaining problems,
he will install the shutter in the MCR beamline, then turn to the EOS's needed
for the SP and AP beamlines. A 2nd Q-switch is in hand, a third on back-order.
Two more controllers are in the shop.
- Ben ordered some SHV connectors to connect the HV to the Q-switches;
they should arrive by the end of the week.
Facilities and vacuum envelope (Ugolini, Vass, Jones):
- The maglev TP1 was at the manufacturer for repairs, but they found
no problem. They've shipped it back, we should get it by the end of the week.
- Steve has set up the camera to view ITMy, in addition to cameras already
in place for MC1, MC2, MC3, ITMx, and BS.
- The CC gauge near TP3 is not working; the controller has a bad board.
It's been sent out for repair.
- Steve completed the laser inventory forms required by the safety officers.
- Our second new dry scroll pump is making squeeking noises, just as
the first one did before it failed.
South Annex Bake Ovens (Taylor, Cardenas):
- Bob is baking the remaining EQ stop screws for our suspensions.
- Bob finished a bake job for Lee.
- Bob has finished cleaning and baking a new set of cleanroom tools
for use in the South Annex.
Thermal Noise Interferometer (Libbrecht)
We did a noise breakdown of the two cavities, including:
- Electronic Noise - Measured
- Mode-cleaner Seismic Noise - Measured
- 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.
- Laser Frequency Noise - Estimated, but checks on mode-cleaner error
signal reveal potential problems (see below)
- Laser Intensity Noise - Still to be measured
- 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:
We also investigated some mode-cleaner pathologies:
- 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.
- Lightwave 126 PZT resonance expected around 130kHz (Peter King, private
communication), which could account for loss of phase.
- Need higher-frequency network analyzer to measure transfer functions
above 100kHz. Obtained Agilent 4395A and started setting up. Measurements
to follow.
- 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.
- 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.
- Rough agreement with predictions. Need to fine-tune pole and zero frequencies
for better calibration.
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)
- Worked on some more ways of simplifying the equations for the modeler's
functions analyzer. Also incorporated the changes to the code base
and doing some benchmarks with SimLIGO.
- Working on a new if-then-else construct for the modeler.
Alfi: (Bruce)
- Design and implementation of bundle features. Currently cleaning
up ConnectionProxy to be used as a base class for BundleConnectionProxy.
May turn into an abstract class to be used as a base for all types of connections.
- Testing of new JGo package which has now been installed.
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)
- Worked a bit on the temperature graph component for Big Brother.
- Got a copy of RH9.0 (final release beta) So have started to explore
revamping the Install procedures for ldas machines.
- Download a new copy of System Imager. With the new Beowulf nodes coming,
this will need to work flawless.
- Also setting up email account for syslog email to be sent to. This
should help with administrating the large clusters.
(Stuart Anderson)
- Worked with several vendors to obtain configurations and quotes for
the remaining LDAS construction equipment. The largest sub-system is the
cluster nodes for which the bid closed on April 2 and a winner has been identified.
The remaining two sub-systems are networking, and servers/storage.
Livingston:
(Igor Yakushin)
- The new taperobot is mostly installed, still waiting for tapes.
(Shannon Roddy)
- 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.
Hanford:
(Greg Mendell)
- The primary sys admin focus of the last week has been to keep tapecontrol,
createrds, and LDAS running at LHO. The tapecontrol script continues
to archive the raw data without problems. The createrds script is also
running without problems, but still falling behind by about 3 hrs per day.
By running a parallel copy of the script it will be able to catch up before
the S2 run ends. The LDAS mpiAPI hung twice during the past week. This
was believed to be due to a known bug and the problem was fixed by restarting
the mpiAPI. Otherwise LDAS has been running without problems for the
past week.
Data Analysis Activities (Lazzarini)
(Mendell)
- Currently generated 2048 s calibrated SFTs for H1 for S2 data between
Feb 22 2003 and the present.
- Distributed to the PULG group the latest getsftdata script, which is
a command line tool for accessing the SFT data via LDAS (requires an ldas
password and ligotools to run). The Michigan group used this to analyze
S1 SFTs and plans to use it to start looking at S2 SFTs.
- Submitted to LDAS an enhancement request to reduce the syntax needed
when requesting SFT data to make running jobs on long stretches of SFT data
manageable within LDAS.
- Working on a command like tool called getFstat that streamlines running
knownpulsardemod DSO jobs that output the F statistic (requires an ldas password
and ligotools to run). The purpose here is to make it easier for nonexperts
to run my DSO and easier for me to configure batches of jobs.
(Yakushin) LDAS data analysis: working on single pixel clusters and
coincidence with time-frequency window in waveburst.
(Shawhan)
- Finished studying the "safety" of the REFL_I veto used for H1 in the
S1 inspiral upper limit. As expected, the glitchMon-based veto condition
that we finally settled on is extremely safe.
- Gave a talk about the S1 inspiral analysis at Penn State.
- Discussed statistical issues, especially those involved in claiming
a detection with some confidence, with Sam Finn.
- Reviewed drafts of various people's presentations to be given at the
APS Meeting.
(Charlton) Working on FCT paper.
- Had status meeting with Massimo Tinto and Rick Jenet.
- Have written up section describing numerical differences between correlation
calculated via matched filtering vs. FCT.
(Weinstein)
- Writing sections of the Burst search paper.
- Running on hardware injections.
- Took scimon shifts remotely from Caltech. Following up with Rolf,
Lisa Bogue, Peter Shawhan, and MIT to get all the right software installed
there.
(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)
- Investigating options for the switches at the end stations. These
had to be shut down before S2 because of acoustic 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 patches 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.
Hanford:
(Christine)
- Helping with re-build problems on an old laptop.
- Working with Dell to fix a video problem on a new laptop.
- Sent a request for quote for the GigE network upgrade equipment.
- Purchased two more laptops and some site license software upgrades.
- Reinstalled the Caltech VPN client on the guest PCs.
- Ordered a large key keyboard for Otto.
- Installed latest version of Sun compilers on the license server.
- Misc. user support.
(Larry)
- It appears that things are a go for the WAN OC3 connection to the Observatory.
Albert has worked things out with the DOE and PNNL. Equipment is on
order for the installation and the contract details are being worked out
by Fred Raab.
CIT:
(Lisa)
- Monthly backups.
- Worked on a mail problem where a self-propogating e-mail worm got into
a loop with the RAV software.
- Took care of a number of file restoration requests.
- Worked on an ssh problem with Glasgow. Problems could be resolved
by using a server with a newer version of ssh.
(Veronica)
- LIGO website: posting various updates. Posting belated Aspen meeting
talks as they keep arriving. Last week Larry and I worked on locating and
ultimately correcting a problem with the DCC database. It was caused by two
non-standard entries in one of its fields. It has been corrected and now
runs properly. We suggested that the entry format be followed closely.
- Taped a video of the Apr 1 LIGO seminar. Processed and posted it for
streaming.
- LSC website: posting the March meeting transparencies as they arrive.
Posted updates to the website. Working on the LSC meeting talks database
on a query of sessions for closed talks.
- Advanced LIGO: working with David Shoemaker on the contents of the
website.
(Mike)
- Finished up loading Barry's new office PC and have it swapped out.
- Helped Ed J. put together a staff Flow Chart.
- Brought over some old equipment over, from Wilson House, to surplus
that included computers & monitors.
- Reloaded a PC from the back house that is hooked to the milling machine.
This had a lot of data that needed to be transferred over to a replacement
computer which is a 750Mhz compared to a 233Mhz.
- Finished up loading a replacement PC for Phoenix and copied users data
over to new PC & swapped out her computer.
- Finished up loading Don W.'s replacement PC and copied over his data
& now have it swapped out.
- Loaded a new replacement 2U server for PICTOR. I still have a lot of
work ahead of me for this is the Primavera server & Flex LM license server
for ansys software. This is currently running on NTSRV4.0, which I
am upgrading to 2000 server.
(Larry)
- Went through a number of procurements. We've a number of new computers
on order and have received a few new ones. Two units have been returned for
replacement since they were DOA. Still trying to resolve a maintenance contract
with SUN. Putting in for a new contract with Foundry.
- Spent a deal of time working on various DCC items. Getting the linking
program issue resolved was the big one.
- Worked on a couple of file restorations. Working on one from old tapes
that are in the process of being catalogued. This one will take sometime
to finish.
- Worked with Lisa on a couple of RAV issues. We are now blocking quite
a bit of spam and obscene e-mail. It should be noted, users with ITS accounts
and having their e-mail forwarded to their LIGO account will receive more
spam since we don't block any of the Caltech domains.
- Worked on a couple of PC repairs. We've been having some problems with
memory boards.
- Setup a number of new user accounts.
- Checking out portable air-conditioners to be used as a backup.
- Powered up the new Cisco router and will be changing its power setup
today. We should be able to start the s/w installation next week.
- Cleared up some minor security issues.
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