Weekly Report for Week Ending
October 31, 2002
The LIGO Executive Committee
Agenda for Monday November 4, 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
- There are no open Change Requests
Executive Committee only 11:30 - noon Topics:
Special Items:
Special Announcements:
Weekly
Report Highlights
LSC Issues (Weiss)
No report.
LIGO I Construction/LIGO Laboratory
Administration (Lindquist)
LIGO Operations--Administration
LIGO Weekly Site Telecon (Lindquist)
There was a site teleconference held on Thursday,
October 31, 2002. The following issues were among those discussed:
Budgets and Costs--The Office of Sponsored Research has reported
that they have received an amendment to our Operations Cooperative Agreement
adding $16.5 million in funding for the first half of FY 2003. We have
provided them the information required to generate a "resume" allocating the
funds.
Livingston Staging Building--The contractor is still working punch
list items. He has been given until next Monday to complete the work.
Hanford Laboratory Building--Hanford personnel have moved in. The
contractor is working a few punch list items.
Hanford umbleweed Removal--the contractor for tumbleweed removal
is going out of business. The work will be transferred to Landscape
Horizons, the current erosion control contractor for the new building.
Traffic Control--Hanford had no additional data. Livingston
has a quote for $11K to widen the road and put an island in the middle. $14K
is estimated for the hardware.
The list of current actions revised to reflect the
status of open actions assigned through October 31, 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
- Researched several fax machines and finalized procurement of a Ricoh
machine. It was delivered last week and will add several nice features
for the staff's use, including 11x14 size, duplex, and eventually, fax-to-email.
- Helped organize and assemble all presentations for the NSF Review
last week.
- Due to the age of our large Mita 6090 copy machine, spent time with
the service maintenance representives in trying to get it fixed. After
several replaced parts, and the scarcity of the remaining part needed, began
researching the possibility of replacing it. It is 9 years old
and is no longer part-supported by Mita.
- Worked very hard in working through numerous piles of accummulated
backlog of documents. Brought the day-to-day documents current and began
attacking piles left by Stan Whitcomb, and several other scientists.
Additionally, sorted through a four-drawer file cabinet and tossed duplicates
or unnecessary papers, entered those that were important and passed along
about 100 publications for Gary's review. This effort represented documents
primarily from the 80's and early 90's. Just during the month of October
over 1,000 documents were entered into the system. The breakdown by
category follows:
Contract
|
252
|
Drawings
|
5
|
Engineering
|
5
|
Graphics
|
126
|
Letters
|
244
|
Managemnent
|
54
|
Publications
|
185
|
Technical
|
145
|
TOTAL
|
1,016
|
- Due to the increase in document prepared for filing, purchased three
additional open-stack file bookcases for the sub-basement. These arrived
today and will be anchored for earthquake safety by tomorrow. We will
then begin unloading older G and D files from the DCC and put them into the
sub-basement. This will hopefully free up filing space for approximately
the next six months.
- 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
- More historical documentation
was filed into the shelves. The amount of "historical" documentation
is a bit overwhelming and will require total reorganization of the DCC files
over the next month. Filing space has become almost nonexistent and
that will require us to move some documentation into the subbasement storage
over the next few weeks to accommodate the constant flow of new files coming
in.
- Electronic document activity
has perked up once again. Submissions for this period been very steady.
- Time was spent dealing with
new fax machine, which included organization, programming of numbers into
the machine, creating dialing lists, etc....
DCC Activity
| WE 10/31/02 |
Packages |
Faxes |
| In |
23 |
30 |
| Out |
8 |
25 |
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>
- Completed the extensions on several blankets to GP Manufacturing, City
of Pasadena, and Pacific Bell. Working on setting up a new blanket P.O.
for Jailand Ralls. Transferred funds on Metropolitan Electric.
Transferred funds on MIT to allow payment of September invoice.
- Received a list of credit card purchases and purchase orders to pull
for Property.
- Working on a change order to Support Services, setting up two new
blankets for LIGO Livingston.
- Working with Bill Tyler and JPL to resolve the discrepancy on the
JPL workorder with Raytheon. Set up a new requisition to add funds
for 6 mos.
From: Florence Kaufman <fkaufman@ligo.caltech.edu>
- Provided Sponsored Research with a schedule indicating how the $16.5
million that has thus far been awarded for FY2003 should be allocated.
- Prepared PTA Set Up Requests for two new account numbers - LIGO.MITTC
5.9 NSFLIGO.FY02OF for MIT Thermal Compensation R&D and LIGO.INOUT 5.14
NSFLIGO.FY02ON for the Advanced Input Output System.
- Submitted 5 Cost Transfers to relieve the over-spent of approximately
$7500 in Fiscal Period 2001 Award. After these Cost Transfers are recorded,
we will finally be able to close all Fiscal Period 2001 accounts.
- Provided Project Accounting with funding realignments required for
FY2002 OPS accounts and Construction accounts.
- Requested correction of incorrect equipment expenditure types for
a couple of PO's, corrections were required because of the new LIGO
equipment expenditure types which started on October 1.
- 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 Oregon: CO #09, adding FY' 03 funds for the on-site support
at LHO, is being processed by Purchasing.
- Univ. of Florida: CO #12, for a no-cost extension of the performance
period through Sept. 30, 2003, was released to Purchasing. All the construction/IO
tasks are completed. Residual funds are in the process of being de-obligated.
- MIT: CO #19, allocating the first half of funds budgeted for FY'03,
is pending MIT's input regarding the exact amount of FY'02 carry over.
- SEI Prototype: The Letter of Interest for the planned procurement
of LASTI prototypes is in preparation. The plan is to contact all firms on
the bidders list for the initial Advanced SEI Mechanical Structure design
and fabrication effort. In addition, HYTEC will also be included.
From: Ed Jasnow <jasnow@ligo.caltech.edu>
CONSTRUCTION:
- As a result of meetings last week at Livingston between Michael Ragusa,
president of Brunt Construction, and Ed Jasnow, final efforts are being made
to complete the LLO Staging Building. Brunt subcontractors are re-working
the doors, windows, concrete, and are examining the HVAC. Additionally,
the manufacturer of the wooden auditorium floor will assess the condition
of that floor on Thursday. Ed Jasnow and Gerry Stapfer will participate
in that review by phone.
- Yakama Industries, the company that has been removing and baling the
tumbleweeds at LHO, is going out of business. They have sold their baling
equipment to the company currently performing landscape maintenance at LHO,
Landscape Horizons. We intend to add the removal of tumbleweeds from
the entire site to the Landscape Horizons contract.
OPERATIONS:
- The site administrative assistants will be coming to Caltech on November
14 for a series of meetings on various Caltech administrative issues.
SUPPORT (Baldon, Torres, Lloyd,
Tischler)
>Irene Baldon
- Processed the paper work for seven (70) new/revised trips and there
are six (6) trips which are in various stages of completion before ticketing
can be done and paper work completed.
- Completed twelve (12) Expense Reports, one (1) Relocation and there
are six (6) 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 I can close their
trip(s). Travel Audit has gotten tighter with outstanding trips since
the new fiscal year (October 1st).
- Reconciled twenty (20) P-Card items which required numerous phone
calls to hotels, 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.
- Notified LIGO personnel of the new/revised FY 2003 Domestic Per Diem
Rates, Meal and Incidental Expense Breakdown, Relocation Per Diem rates for
each family member and pointed out that there have been numerous changes in
the domestic rates, including several cities which LIGO travelers frequent
regularly. These rates took affect on October 1, 2002. You are
to use the FY 2002 rates for any trip taken and completed prior to October
1st. If your trip extends beyond October 1, 2002, please use both rates
for the appropriate dates involved. You can look/copy these new rates
at http://www.policyworks.gov/org/main/mt/homepage/mtt/perdiem/download03.html.
- Worked on the preparation and distribution of the Travel/Vacation
Itinerary for October 28, 2002. 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 and tracked and followed up
on invoice problems. For the total number of incoming invoices received for
this period see "Cost Schedule Control Systems" report by Esther Cunningham.
Reviewed and recorded payments processed by Esther for the weeks of October
14-25.
- Processed the usual requisitions and change orders on-line.
- Continue to monitor contract and blanket order encumbrance and notify
task managers when supplements are needed.
- Began updating PO Log Books.
- Jim continues with data entry in the LIGO database.
>Rita Torres
- Scanned documents from: Hobart & William Smith, Texas-Brownsville,
Loyola, and Salish Kootenai. Submitted these to the DCC for eventual
posting on the web.
- Updated the LSC database with info for the organizations from their
respective Attachments Z. While in the database, I corrected an address
submitted by Penn State.
- Formatted documents from Northwestern U., then posted on the small
web page for review.
- Made a few Pcard purchases, then chased paper work to reconcile some
others. Followed up on a delayed order.
- Changes this week to the LIGO roster were to MIT, mostly room number
changes because they recently moved offices..
>From: Ryan Tischler <rtischle@ligo.caltech.edu>
- Site Administration Meeting details, reviewing more photos of LIGO
group, addressing Press Folder/Brochure details with graphic designer.
Advanced LIGO (Frey)
From: Thomas Frey <tfrey@ligo.caltech.edu>
Working from home on Friday the 1st. I will
be checking email and voice mail.
Weekly Advanced LIGO Project Controls meeting was not held this week.
Advanced LIGO MRE Proposal (Highest Priority)
- Finished preparing comments and questions to discuss with Phil.
- Continuing the development of the Cost Estimate.
- The following is a summary of status by sub system:
- COC - Work on action items per second review continues.
Garilynn continues to execute action items.
- PSL - Management to secure commitment from LZH for
laser development. R&D review decided that a concurrent
bench effort at CIT will not fit into the budget. Next meeting
date has not been scheduled.
- AOS - Work on action items continues. Next meeting
date has not been scheduled.
- IO - Work on action items continues. Next meeting
date has not been scheduled.
- SUS - Working with Janeen doing updates and action items.
- SEI - Work on action items continues. Next meeting
date has not been scheduled.
- ISC - Mike continues to work on the WBS dictionary.
No comments as of 10.31.02 on the draft detailed schedule and no WBS
dictionary.
- LDAS - No data / feedback from Albert to date.
- INSTALL - Continue prepping cost data for import into
cost book. No comments as of 10.31.02.
- All other subsystems have yet to be scheduled for their
first review. These dates are pending per direction from Gary
Sanders and Dennis Coyne.
Cost Book Tool.
- ROSTER DATABASE:
- Resolved technical issue with one of the data input forms.
Barbara K. found a knowledge base article that relates directly to
our problem. Barbara also rebuilt the data file for us.
See http://support.microsoft.com/default.aspx?scid=kb;en-us;Q304548
for details.
- Related to the technical issue, I initiated a tech call
to Microsoft for the hot fix. This issue occurs when you have
Access 2000 on you machine and upgrade any application, besides Access,
to a 2002 version. In my case I installed MS Project 2002,
and that upgraded the visual basic that comes with all office
products. Access 2000 is not compatible with the version of VB
that comes with the latest MS applications. MS provided a
hot fix that is applied after upgrading Office 2000 to SR2.
If you are subject to this situation, you can download the fix at
http://www.ligo.caltech.edu/~tfrey/access_hotfix/5095_ENU_i386_zip.zip.
- I will run tests next week to confirm that the hot fix has corrected
the issue.
- Working with Larry and Barbara to set up a process by
which the roster database updates selected alias lists.
- COST BOOK DATABASE:
- Continue to verbally communicate the username and password
to users.
- Will be working with BK to correct similar technical issues
as roster database.
Continued assignment from
Gary to develop material for the Project Science Seminar.
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)
Nothing to report.
Change Control/Contingency (Lindquist)
No change requests are currently open.
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)
From: Michael Landry <landry_m@apex.ligo-wa.caltech.edu>
2K IFO (H2)
2k efforts continue to be centered on IOO: The MC remained highly unstable
with IOO WFS engaged, still no solution for this. The mode cleaner
servo board was modified to bring it inline with that of the 4k. The
2k MC2 has exhibited odd behaviour in which one sensor (LR) sees pitch and
pendulum modes, but not yaw. The optic does not appear to be mechanical
coupled to stops, etc.
Optical lever servo filters were set up, similar to those of the 4k.
4K IFO (H1)
Work continued on the 4k AS port; investigations of the beam properties on
and before the table, optic layout, and alignment of the EO shutter.
The resulting AS beamspot imaged on a CCD camera was highly elliptical.
While the culprit was initially thought to be the beam reducing telescope,
unfortunately this is not the case: the aspect ratio of the beam emanating
from HAM4 is roughly 1.5.
The ifo achieved arm, prm and state 3 locks, no full locking.
Frequency noise (Matone)
In the past few weeks, we've been measuring how frequency noise propagates
through the system, from the PSL to the IFO. Using one of the long arms,
we measured it out of the mode cleaner and we found that the simulated residual
rms frequency (when the IFO is locked) is comparable to the common mode linewidth
of ~1Hz.
Measurements of the residual rms frequency noise were then compared to the
simulation results and were found to be in agreement. A dtt template will
be set up to simulate the expected residual frequency noise and generating
a figure of merit on the noise level.
It was observed that the 60 Hz power line contributes significantly to the
rms and for this we plan to notch it out and hopefully make an impact on
the rms level.
On the 2k, the MC settings have been adjusted so as to have a bandwidth of
~20kHz with the crossover at 50 Hz. We are, however, experiencing problems
in engaging the WFS.
LIGO Livingston Observatory (LLO)
and Interferometer Operations (Coles)
Interferometer Commissioning: After some diagnostic work
on the coil controllers and balancing the output matrices at DC for the suspended
masses, the interferometer is once again exhibiting stable locking behavior.
We are now working on implementation of the common mode servo. (all)
All the WFS are now reinstalled, retuned and characterized. The only electronics
work left is the end-to-end test of the WFS2 RF. This was delayed because
the demod board is still faulty and needs another visit to the EE lab.
We are just beginning to recommission WFS1 using interferometer light and
will progress to the symmetric port as soon as the demod board is repaired.
Attention is also beginning to turn to the mode cleaner WFS which we are calling
WFS M2 and WFS M2 to distinguish them from the other WFS. The yaw picomoter
stearing light into WFS M2 was broken and a new one should arrive tomorrow.
(Andri)
Continue testing and tuning the WFS electronics with Andri. Have verified
that all electronics are functional but WFS2 demod board. Work on configuration
tool (graphical interface to burt). Can read/write from/to epics a list of
channels. More work needed to make the restoring safe for the optics. (Valera.)
Went to Inspiral Upper Limits group face-to-face in Penn State. Work is
continuing on vibrational noise in the optical lever supports. We tried using
lead-shot filled bags to weight the pier bases and see if this had any effect
on the motion. Harry also tightened the floor bolts yesterday and Orlando
is seeing if anything changed. Gaby has more accelerometers which we are
going to get from LSU today (Thursday). (Brian)
CDS: LLOFb2 was hard down with boot problems. A sun tech support
guy was called in to fix. Found memory problems that forced the memory testing
at boot to look at a different location that was non-existent. Installed One
Sun Blade 2000 in the control room as control 5 with 3 flat panel monitors.
Solved problems with the projector interface when running with flat panel
monitors. Fonts on new solaris 9 are giving us problems and I am looking into
it. Also replaced control 0 in the control room with Sun Blade 1000 running
3 flat panel monitors. Tried the xinerama mode for the above machines. Of
the 3 graphics card, one is a m64 - PGX graphics card and the other two are
the powerful XVR-500's. In xinerama mode the XVR-500's take the least common
configuration of the three graphics card. LLOFb0's minute-trend disk was
98% full. This data should stay forever. So moved some of the old channels
that were not being acuired now to a safe place. With this change it is back
down at 92% full. I have ordered a A1000 disk array and will put in place
soon. Added the Optical Lever channels to the master.config file and reconfigured
the DAQ. (Chethan)
LDAS data analysis: Visiting UFL for collaborating on WaveDSO
with Sergei Klimenko. In the first approximation finished the whole data pipeline
from TCL LDAS job script to LAL. (Igor)
HEPI / LASTI: We are still dealing with assembly problems
with the HEPI actuator. We completed the second unit late last week and found
after all our pains that we have a single, small leak. The bellows were individually
tested in a fixture which permitted them to be pressurized to 90psi, and then
immersed in water. Crude but effective in the shop. This time we took extra
care to stagger the welds and use minimum heat. The unit looks beautiful but
we ended up with a single, small leak at the actuator plate and as before
it is leaking between the bellows and the weld assist band. All indications
point to marginal welding performed by HYSPAN. With the probability of a weak
weld that is thermally stressed by assembly we're proceeding down several
paths. Gerry Stapfer suggested a low temperature tin-silver eutectic solder
to repair the leaks. I've ordered the alloy and will attempt repair when it
arrives. I've also sent some suspect bellows to a vacuum brazing firm, in
the attempt to strengthen the weld joint with a braze alloy. They completed
a first article this afternoon and are sending it for inspection tomorrow.
The most promising solution is to replace the bellows with those of a different
manufacturer. I've located a firm known as Ameriflex, who have been very helpful.
We had a telecon with an engineer Monday afternoon and agreed upon an ring
attachment that was acceptable to Stanford. Corwin Hardham in turn modeled
it at Stanford and we (Marcel) checked it against our model and sent a drawing
to Ameriflex on Tuesday. Within an hour I received a quote, and gave them
the OK to proceed. I've heard from their production manager and they plan
to ship our replacement bellows on Nov 8, 10 days after receipt. This is
pretty unbelievable given our experience with the previous manufacturer. We
plan to wait until receiving the new bellows and have both products in hand
(brazed HYSPAN and new Ameriflex) before deciding which one to use. We are
completing all of the assembly work on the 2 next units, sans bellows. By
working over the weekend (and successfully leak testing) we should begin delivering
actuators to MIT about Nov 12. Katrina Carter, Joe Langdale and Gary Traylor
volunteered to help Marcel and me measure the constants on machines springs
destined for LASTI. They completed 2 today, which are now enroute. We've
yet to receive 4 additional springs which were promised Monday. ETD is now
tomorrow (Thursday) and with help we will measure and ship by week's end.
ETF / Advanced LIGO pod bases Still working on the simplified base and flexure
to support the GS-13 geophone on the ETF without benefit of a pod. Marcel
is detailing that and will supply to Joe Giaime for production in the LSU
Physics shop. (Hammond,Kern)
Detector/Technical Support
(Coyne)
DETECTOR SCIENCE
& ENGINEERING
Seismic Upgrade Project
Hydraulic External Pre-Isolation (HEPI)
(Jonathan
Kern)
We received the first vacuum brazed bellows from Solar Atmospheres yesterday. We checked to see if any
relaxation of the convolutions happened since the bellows
were heated vertically, but none occurred. We do see
a slight bowing along the axis, but it is no more than one of theothers that has not been heated. The
braze joint looks good all around. The areas
where the bellows and ring were in contact have a small fillet of braze alloy (Brazed 1). More typical
is the meniscus seen in the other views where a small
opening existed between the bellows and the ring. The engineer at Solar told us to expect this, and
is confident that the braze allow has penetrated the
gap around and fully wetted the area down to the weld. Before brazing the remaining bellows we're going
to hydro-test this one first. The amount of work hardening
that occurred in rolling the bellows is unknown, but
the brazing process has resulted in a fully annealed
structure.
We had a meeting Monday with an engineer
from Ameriflex, and Corwin. Corwin proposed several
weld designs, and the one we selected is seen on the
2 final images on the webpage. I've placed an order for 24 bellows, and Ameriflex has assured me they will ship no later that next
Friday, Nov. 8.
My plan is to assemble the remaining actuators
using Ameriflex bellows. We should be able to
deliver the first units to MIT ~Tues, Nov. 12. As a fallback, assuming the Hyspan bellows pass a hydro-test we can
use the vacuum brazed Hyspan bellows. A third option is using the lo-temp tin-silver eutectic solder, which has been ordered. I should receive it soon and
we will experiment with it as well.
http://www.ligo-la.caltech.edu/~jkern/Actuator_Bellows_VacBraze_Oct_31/
We are completing all of the assembly
work on the 2 next units, sans bellows. By working over the weekend (and successfully leak
testing) we should begin delivering actuators to MIT
about Nov 12.
Katrina Carter, Joe Langdale and Gary
Traylor volunteered to help Marcel and me measure the
constants on machines springs destined for LASTI. They
completed 2 today, which are now enroute. We've
yet to receive 4 additional springs which were promised
Monday. ETD is now tomorrow (Thursday)
and with help we will measure and ship by week's end.
(Rich Abbott)
EMI filters were designed and tested on the hydraulic pump stand motor control
unit. The filters are effective in removing the
switching noise from the pump servo interface. More
work needs to be done to filter the AC output to the pump motor for switching
noise. We are anticipating shipping the motor
speed control electronics this Friday to MIT.
(Ben Abbott)
The Dspace whitening interface and interface boards (for the seismic external
pre-isolator) were finished and were sent to PCB Express last week.
(Ken Mailand)
Assembly of the second resistor internal parts and packaging of a parts /
tools kit the week of 10-28.
New screw pump arrived 10-29.
Pump station shipped to LASTI MIT 10-25, est. 5 days to delivery. On going communication
with Ken Mason re.the re-assembly of the pump
station at MIT, arrangements made for facilities /
staging and tools.
Will make the final viscosity tests on the alternate
fluid mixture of alcohol and glycerin, as soon as a tantalum material ball
arrives for the viscosity tester. This material allows the instrument to
measure more accurately in our range.
Electro-Magnetic External Pre-Isolator (MEPI)
See LASTI report
CDS Software
(Rolf Bork)
- Alex and I spent most of the last week trying to get
a new Epics Data Collection Unit (EDCU) running. The new version is needed to increase the channel capability to ~10000, run some channels at 16Hz, and make
it independently bootable. The
new EDCU was built to run on either a Sun (using latest
EPICS R3.14) or a MIPS, connected to the Framebuilder network instead of
sharing the DAQ controller VME crate. Code ran fine here, but at LHO, we ended up overloading the Framebuilder network, causing DMA errors on
the DAQ controller. New
(2Gbit/sec) network cards are on order for LHO, but won't be in until late November/early December. When
the new net goes in, we will try these again. In the meantime, we are trying a variation with multiple
MIPS boards still in the DAQSC crate, but they would
be independently bootable, without affecting the DAQSC
controller.
- Hongyu is continuing work on 'grace' version of dataviewer.
- Lori is working on new GDS EXC/TP monitor sequencer
which will combine/sort selected GDS signals into a
single list (requested by LHO).
- Starting to further pursue the "channel hopping" noted
in code running with the ICS110B modules. I have a call into the factory and am also rechecking
the software for possible faults.
Other possibility is timing jitter from timing boards which
feed Pentek and ICS11B ADC modules.
CDS Hardware
(Rich Abbott)
Progress was made on the ISS testing at
the 40m lab. A test was performed of a single
loop control with sufficient gain to achieve the specified noise suppression
using a single loop topology. The new loop achieved
~80kHz bandwidth and 45 degrees of phase margin, with
a preliminary measurement of suppression, out of the loop, at 10 kHz of about
16 dB. Lower frequency measurements are being
performed, and will be posted when available. The
single loop approach seems robust as tested before the MC, but could not
function if sensed after the MC due to large AM fluctuations associated with
ground noise. Flavio Nocera is making new cables that will work with the
electronic pressure sensor readout box.
(Mohana
Mageswaran)
I have sent two tested CM Mode Servo boards
to Rana with the DCN change and documentation. I am testing the Variable
Delay timing boards. I am also helping Rich with testing
his Pump Servo and ordering the correct filter for the driver.
(Jay
Heefner)
FPGA Timing Module
- A draft of the requirements has been released for comment.
- The FPGA prototype board is functional and has been
tested. It works and can replicate the functions of the existing variable
delay timing module.
Adv LIGO Suspension Prototype
(which has potential applicability for initial LIGO):
- Anti-image baords have been received and are being stuffed. They will
be tested next week
(Mike Zucker)
Completed draft requirements spec for
the LOS Coil DAQ readout filter & distributed for
preliminary review.
With Jay and Sander Liu (also visiting
this week) went through rack locations and cable run
options for LASTI SUS and SEI installations.
RFI Mitigation
(Mike Zucker)
Detector electronics (Zucker):
With Jay Heefner (visiting MIT this week)
and Rich Abbott (by phone) reviewed plans for our upcoming
EMC upgrade review, distributed invitations to outside
reviewers (from NRAO Greenbank and Los Alamos), and
tuned up technical design features of the plan. Comments
and questions are welcome on the current drafts of
our core documents, now posted at E020966-00.pdf
and E020350-08.pdf
The design review will be held 22 November starting at
09:30 Pacific.
PSL
(PeterKing)
The slow loop code was compiled for a
Motorola processor, so that it could be run on the LASTI
PSL. An EPICS database required for the code
to run was copied over to the m1psl target area.
A coarse PSpice model for an Hamamatsu
photodiode was written and the part created in Capture. Of the 14 parameters required, only 5 have been figured out. Some of the remaining
parameters are probably not important for circuit modeling.
Optical Contamination Cavities
(Lee Cardenas, Liyuan Zhang)
OTF Lab. (Bridge)
Contamination Cavity # 1
Cavity has the new test sample--65 % Glycerin and 35% Ethyl. We
encountered an alignment situation with the new mirrors. So we have replaced the cavity with the old cleaned mirrors. Now the cavity
is aligned and LOCKED. We are getting 83% beam
visibility so far. We RGA scan the cavity and
one can see clearly the Ethyl is outgasing as the Ethyl partial pressure
peak is larger than before.
We took ringdown and beat frequency measurements
for absorption, ringdown and cavity thermal lensing
measurements.
New OTF Lab at Lauritsen ROOM 38
Cavity #3 Reference Cavity still pumping
down. Optical train ready. Continue taking RGA
measurements. Beam visibility is low ~ 65%, we
may have to open the cavity to change the mirrors.
Cavity #2 Test cavity
This cavity still pumping, optical alignment
and installation in progress. Continue taking RGA measurements.
Ray Tracing for Errant Beams
(Mike Smith)
Working with Dennis Rose to analyze all potential stray
laser beams in the 2K and 4K IFOs that might damage the COC suspension wires
and/or electronic cables.
Earthquake Stops & OSEMs
(Janeen Romie)
Received comments on Earthquake Stop Design
Requirements document and will incorporate this week. I'll submit this to
the DCC & the Revision Technical Review Board (RTRB) after that. Coordinating
with Gregg Harry and Dave Ottaway at MIT about getting a spare SOS, from
Dave Reitze, and a spare SOS optic (not sure where it will come from yet).
Doug Cook has been designing and buying materials for prototypes.
Right this minute, the new osems are somewhere on campus.
I'll inspect them upon delivery and send them to the coil winders after that.
(These OSEMs are for Gin Gin, 40m, and spares for the observatories).
Dry Entry
(Larry Jones)
The outlet port of the canister was enlarged from 1/4" NPT to 1" NPT and
flow checks were conducted with full face mask/mask mounted blower and with
half face mask/belt mounted blower, blowing through an empty canister. The
full face system had more than sufficient flow, and the half face system
was barely sufficient. Silica gel was added to the canister and the full
face system was again tested, this time with insufficient flow indicated.
Samples of four variations of size of molecular sieve and activated alumina
beads were ordered in an attempt to find a system setup that will provide
sufficient flow rate for safety; these desiccants should work nearly as well
as silica gel, and are more readily available in the larger bead sizes desired
for lower pressure drop.
40 Meter Interferometer (Weinstein)
Suspended mass mode cleaner (Ugolini,
Miyakawa, Vass, Abbott, Benna, Bonfield, Berdnikov):
- Osamu is studying the effect of seismic and acoustic noise (at MC2)
on the MC lock stability. He estimated the contribution of seismic and acoustic
noise to the MC frequency noise, and it quantitively explains the noise
spectrum below 30 Hz (but he's still working on refining this). Seismic noise
at the 40m is 10 times noisier than typical seismic motin of 10^(-7)/f^(-2).
- Osamu finds that lock is lost after an impulsive event (deep-knee
bends near MC2, shouting, etc) with low frequencies, below a few Hz. Lock
is lost when the MC frequency loop error signal runs out of dynamic range.
The MC length loop does have enough dynamic range, but not enough gain.
The proposed cure is to increase the length path gain at low frequencies,
which is difficult because of a 7 Hz oscillation in that path at high gain,
which Osamu does not yet understand. He will continue to investigate the
MCL path.
- The MC beamtube appears to act like a microphone, amplifying acoustic
noise at the MC2 table. The MC2 table itself may also be behaving this way,
with a resonance at ~ 50 Hz.
- Steve put a box of sand around the MC beamtube to damp acoustic
noise from propagating into MC2; Osamu finds that it does indeed reduce
vibrations at the MC2 table by 5-20 dB between 10-500 Hz.
- Two notable acoustic noise sources are the dry scroll pumps and
the HEPA filter on the PSL enclosure. These generate +20 dB noise peaks
at the MC2 table, at 830 and 500 Hz, respectively. These don't seem to
affect the lock, and Osamu does not think these are a problem.
- Dennis is working on implementing a resonant gain stage in the
MC length path, at the bounce frequency of 16.3 Hz. So far, it just causes
the MC to lose lock; Dennis continues to tune the parameters. (The work
is hampered by the fact that we still don't have fast MC signals in DTT/DAQ;
but we will, soon).
- An earthquake (4.8M) a couple of days ago knocked all the suspensions
out of whack, and the watchdogs that limit the actuation appear to have
worked correctly.
Intensity stabilization (B. Abbott, R. Abbott, F. Nocera,
D. Ugolini):
- Ben continues to work with Flavio and Rich on the testing of the
Intensity Stabilization Servo (ISS) at the 40m.
- Ben continues to stuff the ISS DC photodiode PCB board.
Electronics (B. Abbott, Taylor):
- Ben has consulted with Richard M about how to get fast signals from
ISS and MC into DAQ. He has a second DAQ interface board, and there should
be sufficient empty channels in our DAQ Lemo Intfc Board to accomodate them.
- Ben has begun stuffing the end racks (mostly DSC stuff for the ETMs)
in order to get an idea of what we have, and what we need. Bob will start
working on the cross-connects for these racks.
- Steve and Bob have made implemented protective trays and cable
strain relief for the 3 installed satellite amplifiers.
- Ben is testing 7 more satellite amplifiers for the core optics DSCs.
- Completion of the vertex core optics DSC system (rack 1Y4) awaits
Penteks, Pentiums, and software. We aim to have a working system in 2 weeks.
- Ben continues to design the interface between the Glasgow suspension
electronics and CIT electronics. The Dspace whitening interface and interface
boards were finished and were sent to PCB Express last week.
Optical sensing (Smith):
- OPTICS PARTS LIST, Orders pending: 29 each, 1in mirror mounts
are pending from Newport; input mode-matching telescope off-axis parabolic
mirrors are pending from SORL; IFLEX1000 IR laser for optical lever is pending
from Point Source Ltd; ; polarizers and half-wave plates for Faraday isolator
from KLC; Faraday rotator from EOT; 3 PZT tilt platforms and 2 servo control
drive electronics and strain gauge read-out electronics from Piezosystems
Jena; 1.5 in and 2 in fixed vacuum mirror mounts and an adapter spacer
from ASCO; Faraday Isolator mechanical parts from CA Machine Co.
- FARADAY ISOLATOR: Awaiting parts.
- IFO MODE-MATCHING TELESCOPE: Detail working drawings for telescope
housing are complete; however, the remote focus mechanism will be re-designed
for a more cost-effective approach. Aiming for a complete system in 1 month.
- LIGO: Working with Dennis Rose to analyze all potential stray laser
beams in the 2K and 4K IFOs that might damage the COC suspension wires and/or
electronic cables.
Optics (Billingsley, Armandula), suspensions (Romie),
OSEMs (Bob):
- Our BS, ITMx, and ITMy, are suspended and sitting on the South
Annex clean room flow bench.
- Steve, Dennis and Osamu will swap out dirty OSEMs for new clean ones
in these 3 suspended optics, next week.
- Janeen is making drawing changes for 40m TM suspension optimizations.
Will continue and then gets the parts reworked.
- Bob continues to build and clean OSEMs.
Facilities and vacuum envelope (Ugolini, Vass, Jones):
- The ion pumps continue to belch out on occasion; CC1 pressure is
observed to jump up for a few minutes every once in a while. It's not a serious
problem.
- Dennis will try to get RGA information into the DAQ system.
- Dennis has fixed the hair-trigger software interlocks on the vacuum
system, eliminating spurious trips.
- Dennis installed a long ethernet cable to read out the STACIS SV
controller; now all controllers are being read out and logged.
- One STACIS seismic isolator (SENW-x) is failing; this is the third
such failure since the system was installed. Also, one of the controllers
(now at the east end) is reading faults from all three feet, even though
the isolators are fine and the EPICS readings are normal. Dennis will pursue
this.
South Annex Bake Ovens (Taylor, Cardenas):
- Bob is putting his new oven F through its paces.
- Bob is repairing temperature controllers to ensure a full complement
for all 5 bake ovens.
Thermal Noise Interferometer (Libbrecht)
Since our last report, we have opened the vacuum chamber
and removed two collimating lenses from the output paths, the in-vacuo broadband
Pockels cell, and a number of extra mirrors from the output paths just before
the RF photodetectors. All of this is an attempt, based on a similar experience
in TAMA, to reduce scattered light noise in the TNI.
After removing these optics, we then realigned each of the cavities to improve
the shot noise limit and to generally clean things up. We now have the best
visibilities yet seen in the TNI in all three cavities, 75% for the mode cleaner,
69% for the South Arm Cavity, and 78% for the North Arm Cavity.
Early this week we closed the vacuum chamber and started pumping out. Closing
the chamber perturbed the alignment some, but the visibilities quoted above
were easy to recover with minor adjustments to the mode cleaner's input periscope
and the pitch of the mode cleaner's back mirror. The error signals and reflected
powers are not as symmetric as we expected, and not a symmetric as they were
with the chamber open. We are now in the process of tracking down the reasons
for these differences.
LASTI (Adhikari,
Coyne, Hammond, Kern, Mason, MacInnis, McKenzie, Mittleman, Ottaway, Rollins,
Shoemaker, Zucker)
PSL (Adhikariu, McKenzie, Rollins, Ottaway)
Found the PMC control was flaky, and traced it to a blown demodulator. Replacement
with a spare appeared to affect operation of the new FSS; investigation is
in progress.
EPI design and installation (Mason, MacInnis)
The plumbing continues for the HEPI pre-isolators. Tubing has been run from
the pump room to the large manifold below the BSC chamber.
Myron has lifted one side of the BSC crossbeams for fit checking a housing
assembly. If everything looks good we will bring it down and attach the springs.
Mike Hennessey from Stanford will be visiting next week to help with the installation
of the HEPI assemblies on the remaining piers.
Additional FEA stiffness modeling was done on the MEPI housing assembly
to help Rich and Dennis with the overall model.
MEPI Characterization and Test (Ottaway, Coyne, Mittleman)
We upgraded one the dSpace memory from 256K to 1M, this should enable us
to take long swept sine data segments. Upgrading the other memory would
allow us to run more complicated or higher sampling rate simulink programs.
We also retrofitted a 1 micro-farad capacitor onto all of the current driver
boards (following Rich Abbotts instructions) which should now make the current
monitors operate correctly.
The control effort hasn't accomplished as much as we would have like last
week due to the NSF and thermal lensing reviews.
HEPI Fabrication (Kern, Hammond)
We're still dealing with assembly problems if the HEPI actuator. We
completed the second unit late last week and found after all our pains that
we have a single, small leak. The bellows were individually tested in a fixture
which permitted them to be pressurized to 90psi, and then immersed in water.
Crude but effective in the shop. This time we took extra care to stagger
the welds and use minimum heat. The unit looks beautiful but we ended
up with a single, small leak at the actuator plate and as before it is leaking
between the bellows and the weld assist band. All indications point to marginal
welding performed by HYSPAN. With the probability of a weak weld that is thermally
stressed by assembly we're proceeding down several paths.
Gerry Stapfer suggested a low temperature tin-silver eutectic solder to
repair the leaks. I've ordered the alloy and will attempt repair when
it arrives. I've also sent some suspect bellows to a vacuum brazing firm,
in the attempt to strengthen the weld joint with a braze alloy. They
completed a first article this afternoon and are sending it for inspection
tomorrow. The most promising solution is to replace the bellows with
those of a different manufacturer. I've located a firm known as Ameriflex,
who have been very helpful. We had a telecon with an engineer Monday
afternoon and agreed upon an ring attachment that was acceptable to Stanford.
Corwin Hardham in turn modeled it at Stanford and we (Marcel) checked it
against our model and sent a drawing to Ameriflex on Tuesday. Within
an hour I received a quote, and gave them the OK to proceed. I've heard
from their production manager and they plan to ship our replacement bellows
on Nov 8, 10 days after receipt.
This is pretty unbelievable given our experience with the previous manufacturer.
We plan to wait until receiving the new bellows and have both products in
hand (brazed HYSPAN and new Ameriflex) before deciding which one to use.
We are completing all of the assembly work on the 2 next units, sans bellows.
By working over the weekend (and successfully leak testing) we should begin
delivering actuators to MIT about Nov 12.
Katrina Carter, Joe Langdale and Gary Traylor volunteered to help Marcel
and me measure the constants on machines springs destined for LASTI. They
completed 2 today, which are now enroute. We've yet to receive 4 additional
springs which were promised Monday. ETD is now tomorrow (Thursday) and
with help we will measure and ship by week's end.
Data Analysis and Computing (Lazzarini)
Simulation and Modeling (Bhawal)
Weekly meeting
Luca explained the frequency noise characterization of the LHO 4k IFO. He
wants to start using e2e to understand the effect of the seismic noise to
the frequency noise induced by the mode cleaner.
Hiro and Virginio are talking to simulate the LLO 4k IFO with the measured
seismic noise by the train and logging, in order to set the requirement
on the improvement of the seismic isolation in order to LLO IFO insensitive
(locking-lock breaking, and the noise level) to these noises.
Mirror motion - simulation vs data
Virginio is working to compare the simulated table top and suspended mirror
motion with the data. He is using a HAM table which has several suspenbded
mirror on top of it. This is a approach similar to the one by S.Yoshida and
his stundent at SLU.
SimLIGO development (M.Evans)
Released SimLIGO_021020 which includes functional wavefront sensors (WFS),
and associated control loops, for all degrees of freedom of the COC (except
the BS, which is not controlled by WFS in the LIGO design). WFS control
has been observed in SimLIGO to stabilize the IFO power and reduce the AS
port noise relative to optical lever control.
Version 021020 also includes an improved intensity noise model (more accurate
in the 0-10 Hz region), and variable amplitude line harmonics in the coil
driver output. Both of these noise source are important for many bilinear
noise couplings.
Of interest in the SimLIGO noise curve is the contribution of DAC timing
jitter noise (which results from having the DACs clocked at 1 MHz rather than
16 kHz). I believe the plan is to reclock the DACs, but until this
change is made, I expect this noise source to dominate other actuation noise
sources.
New field model development (M.Evans)
Work on the E2E field model continues. Most recently I have compiled,
and tested, albeit very superficially, the highest level operator component
(AmpOp) and one of the low level optical building blocks (Interface).
Simulation code development
Melody is working on the input part of the modeler (C++ program) to read
the revised file format and to implement optimizations using caching.
Hiro is working on debugging based on the findings by Matt and Bill Kells,
both of which are related to frequency modulation of the input field.
alfi5 development
Bruce completed the implementation of the copy and paste. A few bugs were
fixed and a minor interface change were done based on the feedback.
Melody Araya continued working on the automated tester for alfi5.
LIGO Data Analysis System
Software Systems (Blackburn)
A schedule was distributed for the next LDAS release this week. It outlines
a code freeze late this week with the release late next week. This release
of LDAS will be used to carry out the LIGO/GriPhyN Applications demonstration
at the Super Computing 2002 Conference in the middle of this month. It also
incorporates the first release of LDAS based on the new version 6 frame specification.
The bulk of software development this week has been focused on getting all
of LDAS to work coherently with the new frameCPP I/O library and to support
the new metadata associated with the greatly enhanced FrProc structure in
that specification. This has also involved developing frame handlers for LDAS
that are based on the frame specification's table of contents.
Several issues with the new dataStandalone and putStandAlone user commands
which will be at the core of the LDAS contribution to the LIGO/GriPhyN Applications
demo were discovered this week. They are being addressed and we hope to have
all the bugs worked out in a couple of days; This would put the finishing
touches on the new functionality for the next LDAS release.
The current performance of LDAS with the new frameCPP is about 50% of the
maximum achieved in earlier pre-release code based on the old frameCPP. It
is known that this is all contained within the frameAPI and mostlikely the
new "table-of-contents" handlers which are very inefficient in memory management.
There is not sufficient time in the schedule to rework these handlers so the
performance will be somewhat less than desired in this release of LDAS.
Two minor changes were made in the wrapperAPI so that in its stand-alone
configuration (remoteAPI) it would more easily integrate with the Grid tools
being used for the Super Computing 2002 demo.
Hardware Systems (Anderson)
Caltech
(Dan Kozak)
- Mostly just HPSS (migration off of Redwoods) this week. We're
down to 65 Redwood tapes with data still on them as of this writing.
When these are completed, there will be a little bit of mop up work vis a
vis trying to read tapes that had problems when we first tried to copy data
off of them.
(Al Wilson)
- Moved pctest1 to 215 sync and reconfigured it to replace the old beowulf
machine in LDAS-CIT. It has GigE connects as well as a two CPUs.
- Rebuilt M27 with redhat 7.3. During the rebuild process, it was discovered
the cfdef rules for "workstation" machines is in need of a overhaul.
So I am currently correcting this.
- Called cybernetics for the coverage info for are tape robot. Waiting
for the response.
- GST came and picked up the bad parts and computer. Waiting for their
response on when we will have it back.
(Stuart Anderson)
- Continuing discussions with Sun regarding SAM-QFS licensing fees after
receiving favorable comments from the NSF review panel last week.
- Re-started mirroring of all trend frames and 1% of full frames from
LLO which had been disabled since S1. Re-start at LHO will wait until after
the LDAS move to the new building next week.
- Help support getting more of the LDAS stand-a-lone servers up and
running as productive test/development for each of the LDAS programmers.
- Integrated all of the S1 frame data into the LDAS-DEV system--currently
all 3 LDAS systems at Caltech can see the full S1 frame data from the IDE
RAID system.
- Mirrored 3 hours of GEO S1 reduced data to all LIGO Lab LDAS systems.
MIT
(Keith Bayer)
- Investigated command line interface to 3ware raid cards.
- Moved improved GEO data onto server (Stuart replicated to all sites).
Livingston
(Shannon Roddy)
- I have a starting point for the pf firewall script on the LDAS VPN.
Now it is a matter of automating the configuration I have. I hope
to have an "alpha" script by Monday.
- Installed the VPN in the rack where it will stay.
Hanford
(Greg Mendell)
- The main activity this week is the preparations to move LDAS at LHO
from the staging building to the new building. S1 data will not be available
at LHO during this move. Only a limited amount of data (the last 12-13 hrs)
will be available in the LHO control room during the move, since the move
involves the T3 disks used by the framebuilders. The move will start
the morning of Sat Nov 2, when I beginning shutting down the LDASsystem and
disconnected cables. Once the move is completed and cables are reconnected
S1 data will be available again, and the framebuilders will have their usual
disk cache's restored. Hopefully this will be by early next week.
Data Analysis Activities (Lazzarini)
(Shawhan)
- Spent a week at IUCAA in Pune, India working with Sanjeev Dhurandhar
and Anand Sengupta on the Extended Hierarchical Search algorithm for binary
inspirals.
(Weinstein)
- Did a quick study of burst network detection efficiency, including
GEO.
- Continuing to work on implementing time-dependent calibration info
(when available) into burst pipeline.
- Writing some sections of the burst S1 paper.
(Yakushin)
- Visiting UFL for collaborating on WaveDSO with Sergei Klimenko.
- In the first approximation finished the whole data pipeline from TCL
LDAS job script to LAL.
(Mendell)
- More work was done with the PULG group to debug LALDemod as part of
our preparing a report on our progress with the S1 data. See the PULG web
page, http://www.lsc-group.phys.uwm.edu/pulgroup/, and the S1 investigations
link (which is password protected).
- Coding to use the calibration data in the knownpulsardemod DSO is
underway, and hopefully will be finished by the end of today.
General Computing (Wallace)
MIT:
(Keith)
- Spec-ing out equipment for wireless in NW22
- Spec-ing out upgrade for NW17 wireless architecture
- Continued testing on packet loss / bw from LIGO subnet
- Troubleshot backup problem on file server
- Purchasing another laptop plus several harddrives
Livingston:
(Shannon)
- Worked some issues with VRVS Monday and Tuesday. I am not sure
what was blocking IP discovery, but I spent Monday afternoon working with
LSU to find out why it was not working. LSU was having the same problem,
so I know that it was not a problem on my local network. By Tuesday
mid-morning, it was working again.
- Spoke with Ric Simmons at LSU to get a status update on possible upgrades
to our connection to LSU. Several months ago Larry Wallace and I had
a meeting with Ric Simmons and Charlie McMahon to discuss our options.
Unfortunately the ideas that they came up with at that time do not look like
they will pan out.
- Read more documentation on RAV anti virus and anti-SPAM for our mail
server. This looks like it is a good product and should be evaluated.
Especially since the volume of SPAM seems to be increasing.
Hanford:
(Christine)
- Did some more network testing. The internal network is providing
8 to 9 Mb/s between all computers. The network to Caltech, as well as
MIT, is providing 5 to 6 Mb/s out but only .4 to 1 Mb/s in. No further
word from PNNL on their DOE router problem.
- The main tape backup unit suffered a dead power supply on Wed.
The tape library is still under warranty, so it will be replaced. I
removed it from the server and packaged it for shipping. Turn around
time from the manufacturer is 10 business days. Meanwhile, I am backing
up the user accounts to disk.
- Purchased some computer supplies for the new building. Set up
a GC PC in the Control Room for the Operators. Repaired the digital
camera card reader on another PC. Helped users with various problems.
Caltech:
(Mike)
- Finished reloading the engineering workstation for Dennis Coyne, with
various engineering software plus general computing software.
- I just about have the simba workstation reloaded this is one of the
lab computers that I had to salvage due to a power failure that burnt out
some of the hardware.
- Cleaned a computer in Synchrotron that was infected with a virus.
I am still working on this computer this is looking like a possible reload.
- Setup a print server in Synchrotron and connected computers to this
workstation for printing services.
- Lisa and I swapped over all computers in Synchrotron from Caltech's
subnet over to the ligo 115 subnet. Plus I ran a few cable drops to
connect computers to the LIGO switch.
- Loaded a new laptop for Szabolcs that included all GC software plus
a variety of engineering packages.
- Loading both with General Computing software and hardware upgrades
on a PC workstation and a laptop.
- Doing daily NT administration checking security logs, system failures
such as hardware/software problems. Everything seems to be running okay. I
still have four servers to upgrade to 2000 server. (Time Permitting)
- Setup a meeting for LIGO seminar in the science conference room.
(Veronica)
- LSC website: worked on the progress report database; updated the database
for the new reporting period.
- LIGO website: reworked the webpage for 2002 SURF projects; posting
the abstracts of this Summer's work on the web. Preparing a webpage for the
2003 projects announcement. Posted a new webpage with the 2002 NSF Review
presentations. Working on cgi scripts for the GC incident report form.
Started working on the webpages for the Aspen 2003 Winter conference.
- CaJAGWR website: edited a video of Milos Milosavljevic's talk; cut
out a segment in the middle of the video file; posted the file at the
website. Requested a virtual name host cajagwr.caltech.edu at the ITS,
a url that's shorter and easier to remember.
- Project Science website: posting updates as they arrive.
(Lisa)
- More work on the STARTTLS pop/imap services on becrux. I have
a version that works with an older version of openssl, but not with the latest
version. This can be put aside for now but will need to be revisited.
- Worked with Mike to move the computers in the synchatron over to the
115 subnet.
- Burned 8Gb of data from a users home account off to cd so that I could
free up that disk space on the server.
- Did monthly backups.
(Larry)
- Resolved a number of PC issues. Driver updates appears to have resolved
the problem.
- Worked on the network performance issues at all locations. Still no
update on the Hanford problem other than what Christine has reported. LSC
has informed us that the cable company will not be able to make the connection
we were looking for. However, they are putting a little more pressure on Bellsouth
to get their pricing a little more competitive. They are still working
on the recent performance problem. Nothing to add to the MIT issue
that others have not already reported.
- The amount of SPAM mail has been increasing across the board. A good
part of it is coming from e-mail accounts at the local institutions, which
can't be blocked by the LIGO mail servers for various reasons. The local filters
being used is blocking a large amount but we are still looking for more tools
to improve the filtering. Also, looking into a number of tools for virus-scan
on the mail server.
- Worked a couple of purchase issues. Still have not received quotes
from SUN. Getting new quotes from Foundry and waiting for the ship dates
of equipment purchased for Livingston. Ordered a battery replacement for
one of the UPS units that is now having problems as well as ordering another
UPS unit to accommodate the additional load in the server room.
- Reworked some of the network cabling and power in the server room.
Also, still working on rebuilds of some of the servers.
- Started working on the rewrite of the security plan.
- Worked a few more issues for the DCC. Looking into a DVD burner for
their archiving in place of the CD burner.
LIGO II/Advanced R&D (Sanders)
Core Optics
(From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>)
No report this week.
Advanced LIGO Coatings
(From: Helena Armandula <ahelena@ligo.caltech.edu>)
After receiving an invitation from Ramin Lalezari, formerly the Vice-President
of REO, to visit his new company, Advanced Thin Films, I was there last Tuesday.
The State of Colorado has created the Colorado Advanced Photonics Technology
(CAPT) Center on the Higher Education Advanced Technology (HEAT) Center Campus
at Lowry. Ramin's lab is in the CAPT Center. Actually this facility
was designed and built by REO during their expansion days, and they never
got to use it. The university took over the facility and equipped with state-of-the-art
characterization equipment left behind by many companies from the failed telecommunication
business. Ramin's company acquired a large IBS coating chamber with
simple rotation that he has already characterized and is producing coatings.
At this time they are manufacturing a planetary rotator that should
be finished by the end of the year. One of his active partners is an
ex REO coating engineer. He has other two silent partners with extensive experience,
more than 30 years, in the coating field. They rent clean room space
from the university as well as access to the available equipment at the center.
They have a variety of good ovens and microscopes including an Atomic
Force Microscope; an ellipsometer, an interferometer, spectrophotometers,
they are in the process of building a ring down cavity. Besides they have
numerous clean benches, general DI water and point of use DI water units under
clean benches. They have excellent potential to provide good coatings;
they are mainly interested in R and D work, and of course, they are looking
for business. http://www.captcenter.org/about/Default.htm
MLD
Received two SiO2/Al2O3 coated substrates, one thin and one thick. The parts
have been shipped to Glasgow and MIT. The coating has not been annealed.
"Q" measurements will be taken before and after annealing.
SMA
We have planned a meeting, tentatively for Nov. 7th, with Jean-Marie Mackowski
at Stanford. Jean-Marie will be in the States attending a conference.
During the meeting we'll be discussing possibilities for future coating
development work.
Adv LIGO Core Optics:
(Erika D’Ambrosio)
No report this week.
Advanced LIGO Suspensions
(From: Janeen Romie <romie_j@ligo.caltech.edu>)
- Working on mode cleaner design tasks, specifically, small updates
to the earthquake stop brackets and osem brackets. MC height adapters should
be delivered 10/31.
- Working with Larry Jones on the LASTI cabling PO. Also working with
Larry and the suspension group on determining the maximum quad pendulum suspension
length. This information is needed for the seismic prototype RFP, due near
the end of November.
- Magnets for the suspension prototypes have been lost somewhere outside
of England. The vendor MagDev have filled out a form to have Royal Mail track
it. We have enough for the MC and RM prototypes, however.
Mode Cleaner:
(From: ctorrie <ctorrie@ligo.caltech.edu> )
- Janeen, Helena and I have been working on the assembly of the 2 prototype
suspensions. Several of the updated aspects like the pitch adjustment
and winch system have already been tested on the bench and seem to operate
as required.
- We have been taking a lot of photographs this week and these can be
seen at http://www.ligo.caltech.edu/~ctorrie/ligotriple.html,
and by clicking on the recent diary dates.
- Helena and I have been testing the assembly of the upper mass and
the coil and have started to build up .jpg pictures and photographs of th
e procedure.We have been taking a lot of photographs this week and these
can be seen at http://www.ligo.caltech.edu/~ctorrie/ligotriple.html,
and by clicking on the recent diary dates. The photographer and I sent a couple
of hours with Bob Taylor documenting aspects of the LIGO 1 OSEM, that will
be used for global control for the LASTI prototypes.
- Drawings for an eddy current damper prototype are now in workshop.
- In the Synchrotron laboratory we now have several new cabinets that
will aid with the transfer of dirty suspension parts for cleaning and re-assembly
in the 40m annex.
Electronics:
(Jay Heefner)
No report.
40m Suspensions:
(From: Janeen Romie <romie_j@ligo.caltech.edu>)
- I've started making changes to the drawings. Will continue and then
gets the parts reworked.
Prestabilized Laser (PSL):
(From: Peter King <pking@ligo.caltech.edu>)
- Checked that the two EEPROMs that the University of Hannover requested
functioned properly by booting up a Motorola IOC.
- I received word that the hardware shipped a couple of weeks ago made
it to Benno Willke's office intact.
Software:
(From: "Mark Barton" <mbarton@ligo.caltech.edu> )
This week I worked on reconfiguring Mal Gray's interferometric position
sensor to use a corner reflector as a sensing target instead of a simple mirror.
The sensor is a Michelson interferometer in which one arm is internal to
the sensor and the other extends to a mirror on the object whose position
is to be sensed. The end mirror of the internal arm is servoed to keep the
arm lengths matched, and the feedback signal is a measure of position. The
defect of the original design that we're trying to address is excessive sensitivity
to angular motion of the target. We get around this by folding the external
arm using a corner cube on the target and a static end mirror on the outside
of the sensor housing. I've set up the new configuration and with the help
of Phil Willems I got it aligned well enough to produce interference fringes
using an external laser, but not yet with the internal LED source (which has
a much poorer coherence length of only about 30 microns).
Low Frequency Seismic Isolation:
(From: Hareem Tariq <htariq@ligo.caltech.edu>)
(Charles)
Received the load frame back from the material science but the power supply
broken and voltage regulator not in working conditioner. New setup prepared
with two LVDTs and drivers this time and a new gauge (~100 lb). Can modify
gain now through a separate amplifier (amplification up to 2000 if LVDTs
put in series configuration). Ready to calibrate the LVDTs.
LabView: Working on modifying the LabView programme to incorporate
the LVDTs. It is now ready to be tested.
Braze: Made the AuSn braze. Looking for an evaporator, consulting Axel regarding
it.
(Stoyan)
ANSYS: Voodoo mystery solved in 3-D as well and now can bend and flex
naturally the flex joint. ANSYS limited number of nodes causing trouble again.
Had problems with incorporating 2-D autocad design in ANSYS, solved it by
importing simpler models.
Furnace: Received the gate valve. Ready to put it in.
X-ray: X-rayed B17 (multiple samples) which would be used for annealing
tests.
Splat Quencher: Working on converting the mechanical valves to electric ones.
Placed an order for more sample holders and coils.
(Alison)
Hardness: Measured more samples for hardness including B16.5. Getting
lower values than previously measured by Maddalena.
(Xavier)
TTO: Conductivity analysis continues. Verified that QD values are
indeed are inconsistent, completely relying on our own data analysis. Now
can control almost all parameters independently of QD software. Ready to
test a multiple MoRuB sample.
ANSYS: Almost done with the monoflex model and would soon have results.
Valerie (Xavier):
TTO: Finished almost all radiation loss data and will now have our
own measurement for the radiation losses.
(Xavier/ Stoyan/ Charles)
Splatted a night and produced B16, B16.5, B20, B21 and B22. Discovered B22
was contaminated.
(Akiteru and Riccardo in Hongo)
Received repaired vacuum extension rings and mounted on the towers, the vacuum
was better but unfortunately there was a residual leak in one of the two
extensions that was sent back for repair. Met with other people in
TAMA to discuss the design improvements for the production run of TAMA-SAS.
(Alessandro and Riccardo in Pisa)
Looked with the SEM at the failed braze joint, it is not clear yet if it
separated between MoRuB and NiP or between NiP and AuSn. We will need
chemical analysis of the surface with scattering x-ray analisys, but need
liquid Nitrogen to do that. Will do it next week. The braze still
may be sufficiently good as is for most measurements, especially if we manage
to improve it by better cleaning and more agressive etching, but it looks
more likely that we will have to resort to spattering deposition to get a
more intimate bonding of the layers for mirror suspensions and ultimate low
noise operation. Met with G&M and others to discuss details of
the TAMA-SAS production run for Florence and Naples, and later for TAMA.
(Akiteru)
I can happily announce that the vacuum envelope for the 3m is fixed this
time. We achieved the best vacuum level of 10-3 Torr and
it remains below 2 Torr after left for a day. Certainly there is still some
leak but within an acceptable level.
For additional information about this report, contact sanders@ligo.caltech.edu