Weekly Report for Week Ending
May 29, 2003
The LIGO Executive Committee
Agenda for Monday June 2, 2003 will be:
(Meeting time: 10:30
am Pacific Time)
Open meeting 10:30 - 11:30
Announcements
LSC Issues (Weiss)
Comments on Weekly Report
WBS 1 LIGO I Construction (Lindquist)
- Field Change Orders/Contingency Liens/Change Requests
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)
WBS 3 and 4 Advanced R&D and LIGO II
(Shoemaker)
CHANGE CONTROL BOARD/TECHNICAL REVIEW BOARD
SESSION AS NEEDED
Special Announcements:
Weekly
Report Highlights
LSC Issues (Saulson)
Minutes of LSC Executive Committee telecon 23 May 2003, 0800 PDT
(Attending: Bruce Allen, Barry Barish, Sam Finn, Albert Lazzarini, Irena
Petrac, Dave Reitze, Keith Riles, Gary Sanders, Peter Saulson, David Shoemaker,
Daniel Sigg, Ken Strain, Rai Weiss, Benno Willke, Stan Whitcomb)
1. Status of LSC author list
Irena Petrac announced that the full LIGO I author list will be compiled
in LaTeX format Tuesday of next week. Tom Frey and Albert Lazzarini are in
charge of that conversion.
Peter Saulson will give it a first look. Once that is done, it will be
posted on the Web. A message will be sent to LSC PI's, who will be instructed
both to check the list themselves, but also to inform their group to look
at it to check for errors or omissions. A message will be sent also to the
whole LSC
email list, asking them to make sure the PI sends them the pointer to the
list. In addition, all "old-timers" need to receive an email pointer to the
list. Irena Petrac will coordinate construction of the old-timers email
list.
Stan Whitcomb pointed out that the latest version of the lsc alias has
both errors and gaps. He will send "bounce" information to Irena, and his
info about gaps. Peter will look into ways of checking for missing names.
Sam Finn proposed that this might be a big enough job to involve a membership
secretary or committee. This is an idea that deserves serious consideration.
2. Plans for Hannover LSC meeting
Benno Willke presented the plans for the mechanics of the August Lsc meeting,
to be held in Hannover. Details have been worked out for meeting space, hotel
rooms, meals, GEO 600 tour, and the conference fee. All thought that the plan
sounded very good.
Benno said that the web site announcing the meeting would probably be ready
to post next week.
Barry Barish asked whether any plans for outreach or public meetings had
been included in the plans. David Shoemaker asked specifically about possibly
inviting funders. Benno promised to discuss these issues with his fellow hosts,
and to report back later.
3. Status of S1 paper
The Stochastic Background paper has now been released to the LSC for a final
reading. The one week comment period ends Monday 26 May. The Pulsar group's
paper is essentially ready -- it is being held until Tuesday 27 May to allow
the group to consider the latest timing issue, but however that is resolved
the paper should be ready to release. The Inspiral paper is also essentially
ready, but timing issues are getting consideration right now. The Burst Group
has intensively critiqued its latest draft,and is waiting to see how the corrections
look before deciding whether it is ready to release.
For Executive Committee approval, it will be necessary to carry out the
following steps. Firstly, the Exec Comm needs to receive a single statement
from a paper's Review Committee, stating that in its opinion the paper is
sound and ready to publish. The Spokesperson is to contact the Reviewers,
asking them to cast their review as they would if they were journal reviewers:
is the paper correct, interesting, novel, etc. The Spokesperson will also
collect from each Executive Committee member a written statement (which need
not be extensive), stating his/her opinion about the paper. A concatenated
collection of all of these materials will be sent to Exec Comm members in
advance of our next meeting. Whatever papers are ready to discuss for
approval will form the main agenda items of our next meeting. Given the difficulty
of scheduling ad hoc meetings, we will only plan on reviewing papers at regular
monthly meetings.
There was a general consensus that the S1 instrument paper draft was excellent,
and deserving of publication in a refereed archival journal. Stan and
David, the principal authors, noted that it would take some extra work to
get it into publishable shape, but agreed to take on the work. It isn't clear
whether to publish in RSI or NIM. The principal authors will have the primary
say in the choice of journal.
4. Two highlights of UL Chairs face-to-face meeting 1 May 2003
LSC Newsletter:
One important idea was the creation of an LSC newsletter. Its function would
be to ensure that LSC members are better informed about various LSC
activities. There needs to be better communication about both "technical"
work and about data analysis. A weekly or biweekly email would contain brief
statements about recent activities, and include pointers to more extensive
discussions.
To keep the workload manageable, the basic idea would be for individual
Working Group chairs or Search Group co-chairs to send the editor(s) the
summary and pointer, whenever they have something to report (e.g. meeting
minutes or other progress.) The editor(s) will collate submissions on a weekly
(or biweekly) basis, and send the summary email to the LSC membership.
Patrick Brady has volunteered to edit the portion of the newsletter concerning
analysis work. David Shoemaker expressed interest in helping with the technical
side, as did Sam Finn.
A few important issues were raised, that we will need to address. We need
to think about how to communicate important matters about data analysis freely
to all members of the LIGO-I collaboration, while keeping confidential that
which should be confidential. Use of password-protected links was discussed,
but even there careful editorial work is needed. We also probably need to
ensure that the newsletter and its links are archived; thus, pointers shouldn't
go to the wide assortment of websites now used for informal communication
within the LSC.
Gary Sanders offered to make adjustments to the LIGO Lab weekly to make
it dovetail with the LSC newsletter. Once the shape of the LSC newsletter
is a little clearer, we will take up that offer.
Additional LSC meeting(s):
The UL Chairs proposed the addition of two LSC meetings to the current annual
schedule of two, making four in all per year. The idea was that these additional
two would be "mini" LSC meetings, devoted primarily to discussion of data
analysis issues, and in particular to serve as forums for discussing new results.
Barry expressed a reservation that restricting the agenda would discourage
instrumentalists from attending, who would then be disenfranchised from the
process of discussing analysis results. Sam agreed that the restricted agenda
was not a good idea.
The Executive Committee settled on the idea of adding a third full LSC meeting
to the annual calendar. In principle, they should be roughly equally spaced
throughout the year, but the detailed calendar needs to be worked out. The
first additional meeting will be held in late October or early November at
LHO (assuming they agree to host it.)
5. Upcoming meetings
There was nothing controversial about the idea of sending representatives
to the Phystat 2003 meeting. The Executive Committee also endorsed participation
in the proposed Special Session on Gravity Wave Phenomenology at the Jan 2004
AAS meeting. David urged that the abstracts be written carefully, so that
there is no question of promising to present results that might not
be available in time.
6. MOU with the USC/ISI group
Albert Lazzarini said he had gotten comments on the revised draft of the
MOU with the USC Information Sciences Institute, and asked that any more comments
be sent to him promptly.
7. A brief report was given on the recent face-to-face meeting of the LSC
Computing Committee. Both Albert and Sam described it as extremely productive.
A particular highlight was the agreement to include the Tier 2 centers
in weekly telecons with the Lab, to allow for better coordination. For further
information on the outcome of the meeting, the minutes can be found at http://www.ligo.caltech.edu/~lazz/LSC_Computing/minutes20030514v2.pdf
The meeting adjourned at 0929 PDT.
LIGO I Construction/LIGO Laboratory
Administration (Lindquist)
LIGO Weekly Site Telecon (Lindquist)
There was a site teleconference held on Thursday, May 29, 2003. There
will be no site teleconferences on June 5 or June 12 due to PAC meeting and
Advanced LIGO Review respectively. The following items were discussed
on May 29:
Action 58 (Convenience Checks for Hanford, Livingston to follow)--the
system seems to be working at Hanford.
Action 103 (Posters for Weber Bar Display)--Ed Jasnow and I will
meet with Fred Raab while he is here for the Advanced LIGO Review.
Action 117 (Software to remove potentially sensitive data from excised
computers)--software has been acquired and is being used. Action is closed.
Action 119 (Flow Charts for Petty Cash Tracking)--no longer relevant
since the convenience checks are being implemented (Action 58), but it was
deemed a good idea to review how we are doing relative to the auditor's recommendations.
It was noted that we should check to see if a flag is required on the P-Card
reconciliation form to identify services that are not on contract that would
require Caltech to issue 1099 forms.
Status of construction funds--currently over-encumbered by $255K.
We will meet next week (after May costs are in) to review strategy.
Status of Operating Funds--We will spend over $2.5 million this
month. Since all construction spending will cease next month, there
will be a slight increment in monthly expenditures. Also, there is
a $3 million change request for EPI. Current projections, therefore,
are between $31 million and $34 million this year.
The list of current actions revised to reflect the
status of open actions assigned through May 29, 2003 may be found at ACTION
LIST.
PROPERTY
MANAGEMENT (Chargois)
From: Ed Chargois <chargois_e@ligo.caltech.edu>
- Nothing significant to report.
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
- Worked with George to compile a complete listing
of documents that are available electronically but are without the proper
electronic link on the website. This has been validated as accurate.
The next step will be to walk George through the complete submittal, processing
and posting cycle as he begins to diagnose the origin of the linking problem
and to assess the processes that may be causing instability.
- Experienced a few glitches on my computer that
caused Eudora to shut down anytime Netscape was accessed through an email.
It appears there's a problem with the keypad and mouse drivers. Larry
will be fixing it as he gets time.
- 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
- Worked on adding documents
to the DCC database from a large compiled list of documents containing
electronic files that apparently were not in the database as expected.
Unfortunately, a number of problems including many revision discrepancies,
were discovered in the process.
- A request was made for the
original cooperative agreement (and all the amendments) between the NSF
and CIT. Copies were made and distributed.
DCC Activity
| WE 05/29/03 |
Packages |
Faxes |
| In |
14 |
22 |
| Out |
8 |
38 |
Press here to access
the DOCUMENT CONTROL CENTER
WEB PAGE.
COST SCHEDULE
CONTROL SYSTEMS (Cunningham, Brambila, Kaufman, Salone)
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS
PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
- Completed change order #5 to Excel Engineering #1055977, change order
#5 to Excel Group ref # 1051885, change order #2 to CSRS ref. 1056645,
and change order #5 for the JPL Raytheon work order. Set up the blanket
order to Aztek. Working on change order #6 to Excel Engineering ref #1055977,
and change order #2 to Star Services ref. 1056319.
- Made internal modifications on tax code changes on various LIGO orders.
Coordinated transactions with Esther and Dorothy.
- Placed and reconciled pcard orders.
From: Gina Salone <gsalone@ligo.caltech.edu>
From: Florence Kaufman <fkaufman@ligo.caltech.edu>
- Continued close monitoring of Construction account. Currently
the Award is over committed by $225K. We need to determine what the
appropriate strategy should be in terms of which costs may need to be
transferred.
- Prepared an analysis of R&D accounts to try to analyze if budget
realignments that may need to be required.
- Requested correction of payments on 3 contracts where payments had
been applied to Over 25K before the first 25K had been fully expended.
These corrections have now been made.
- Phil Lindquist and I met with Suzanne Dodd of SIRTF Science center
to discuss the ways in which LIGO monitors financial performance against
budgets.
- Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
SUBCONTRACTS MANAGEMENT (Petrac,
Jasnow)
From: irena@ligo.caltech.edu (Irena Petrac)
- RFP for AdLIGO SEI Mechanical Structures: Proposals for Phase I have
been received and are in LIGO/LSC review.
- RFP for AdLIGO Coating: The RFP package is in LIGO review.
From: Ed Jasnow <jasnow@ligo.caltech.edu>
CONSTRUCTION:
- Work still continues on the modifications to the LHO Laboratory Building.
The glass for the double doors is on site, but the steel for the sun shades
is not.
- Concrete is being poured for the foundation for the LLO pre-fabricated
storage building.
- The concrete foundation for the LLO access gate is nearly complete,
and delivery of the parts for the gate itself to the site has been almost
accomplished.
OPERATIONS:
- LHO is successfully operating its petty cash system with the use
of P-card convenience checks. The petty cash account with the Bank of
America will now be closed.
- Direct deposit of travel and other reimbursements is now in effect.
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
- Processed the paper work for twelve (12) new/revised trips.
There are approximately twenty-two (22) trips in various stages of completion
before ticketing can be done and/or paper work completed. And an
additional one-half dozen (6) general inquiries. Until further notice
I will be doing travel for LHO travelers.
- The 2003 SURF Program will be held from June 16th thru August 22nd.
LIGO/Caltech will have twenty (22) students, LIGO/Hanford will have seven
(7), and LIGO/Livingston will have three (3), with four (4) going to Pisa,
Italy. I continue ticketing the thirty-two (32) coming to one of
the three (3) LIGO sites and Pisa will be handling the four (4) going there
as Passports and VISAs are confirmed.
- Completed six (6) Expense Reports and there are thirteen (13) 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.
There is only four (4) reports more than 30 days old at this time.
- Reconciled thirty-six (36) 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.
- I'm happy to report that the new EFT Program for Travel Reimbursement
Direct Deposit continues to be functioning well and although there have
been a couple of minor bugs Michelle and I are working on them. Prospects
are good for a successful implementation. If you have any questions
or problems with EFT please let me know so that we can address it promptly.
For those of you who have not as yet sent me your form for participation
please send it to me as soon as possible and I'll get you signed up
immediately. Thanks for your cooperation and help on this one.
- Worked on the preparation and distribution of the Travel/Vacation
Itinerary for May 27, 2003. Arranged two (2) new teleconferences
and revised one (1); and entered two (2) new reservations on the LIGO
Calendar.
- 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 May 19.
- 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>
- NSF Review -following up on details
- Mayfield High School tour -arrangements with C.Torrie, A.Weinstein,
V.Sannible
- Worked on a few LIGO/SURF orientation agenda items.
Advanced LIGO (Frey)
From: Thomas Frey <tfrey@ligo.caltech.edu>
Weekly Advanced LIGO Project Controls meeting was not held this week.
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)
- Started updating the top level schedule prepared by Dennis in MS
Project.
- Finished another round of schedule changes as directed by David Shoemaker
and Dennis Coyne. (ISC, AOS, and IO)
- Finished update of cost profiles base upon revised schedule data.
- Reviewed web sites prepared by Veronica for the AdL Proposal.
- Posted updated materials as required for the NSF review package.
- Continued preparing revised budget sheet data.
- The following is a summary of status by sub system:
- COC - Still need completed WBS dictionary and BOE. Input
task sequence for Coating Development as provided by Garilynn.
- PSL - No action items pending. Corresponded with Benno
Willke regarding LZH PSL scope and cost.
- AOS - Still need completed WBS dictionary and BOE.
- IO - Still need completed WBS dictionary and BOE.
- SUS - No action items pending.
- Revised the SUS baseline to be inline with progress to date.
- Updated the plan with progress as of 05.16.03 and posted
to site.
- Sent out update data requests for progress as of 06.13.03.
- 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. Received
a partial WBS dictionary from Peter F.
- 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 - No action required at this point in time.
Project Plan for the 40-Meter Lab Upgrade continues.
- Revised the 40-Meter baseline to be inline with progress to date.
- Updated the plan with progress as of 05.16.03 and posted to
site.
- Sent out update data requests for progress as of 06.13.03.
Project Plan for the TNI Lab Project continues.
- Updated the plan with progress as of 05.16.03 and posted to
site.
- Sent out update data requests for progress as of 06.13.03.
Continue to update the LASTI Schedule and incorporate any changes.
- Started and continue input of changes and comments from Mike
Zucker.
Cost Book Tool.
- ROSTER DATABASE:
- BK is continuing work on action items.
- Input of supervisor, dept., and specialty codes on hold until
after review.
- Prepared an updated LSC Council mailing address report for Irena.
- Working with Irena to get authorship list done. We encountered
and issue that resulted in changes to the database structure to accommodate
the uniqueness of the authorship list.
- COST BOOK DATABASE:
- BK is continuing work on action items.
- Continued to 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, optics coatings, etc. We
have discussed priorities, and the quarterly report is still slipping.
DCAA Audit Report Response: Comments have been provided to Caltech
Administration, and Caltech Administration has prepared a response.
Change Control/Contingency (Lindquist)
The following change requests are pending or new.
Dennis Coyne submitted CR-030011 for the addition of an External Pre-Isolation
(EPI) stage to the seismic isolation systems on the LIGO Livingston Observatories.
This change is to improve the low frequency isolation of the currently installed
seismic isolation systems as a retrofit with little or no disturbance to
the alignment of the optics and without entry to the vacuum system.
I will put these change requests on the agenda for the next meeting of the
Executuve Committee.
| CR-030008 |
Furniture for the auditorium lobby, interaction area
underneath the skylight atrium in the OSB, and on the second floor
interaction area of the new laboratory/office building. (ON HOLD pending
additional cost data.) |
M. Coles |
April 29, 2003 |
| CR-030011 |
Seismic External Pre-Isolation at LIGO Livingston
Observatory |
D. Coyne |
May 16, 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>
- Pending completion of the LHO safety audit report, a draft
of the action items was distributed to the audit team and the LHO audit
"hosts" for comment/changes. (So far, no LHO comments).
- There are eight action items listed. The most significant AI
relates to the need to establish a "Work Permit" process for view port
covers/equipment which considers the safety "risk" (port location), and
includes a "close out" process to verify that the port is left in the required
"safe" condition, i.e., covers or equipment installed and this condition
recorded.
- The "Safety Audit Team", recommends that a view port cover "Work Permit"
process should be implemented throughout LIGO if not already in place.
- George Bowman (Caltech Engineering. and Constr. Mgmt.) has completed
a cost estimate for the LIGO server room fire suppression system. He has
submitted it to his management for review and approval. (Pending approval,
the "unapproved" cost number is available by request).
- Reminder, the updated revision (final sign off and release still pending)
of LIGO Vacuum Compatibility, Cleaning Methods and Qualification Procedures
LIGO-E960022 is available on-line.
- The Parts Cleaning Request form, LIGO-F030014 and the LIGO Vacuum
Bake Oven Procedure and Checklist form, LIGO-F030015 are also available
on-line as templates for easy access and use.
LIGO Hanford Observatory (LHO) and Interferometer Operations (Raab)
Most of the LHO crew has been involved in one way or another
with preparations for the vent scheduled to begin Monday morning and expected
to require keeping the gate valves to the beam tubes closed for several weeks
thereafter. Planned tasks include replacing ITMx in H2 and moving
the both ITMs in H1 by 28 mm to correct the Michelson asymmetry. The
DougC and BetsyB's detailed vent plan can be found at http://apex.ligo-wa.caltech.edu/~dcook/2K%20ITMx%20REPLACEMENT%20VENT%20PLAN.pdf.
Both interferometers were locking reasonably well (at times) so progress
was made on a number of commissioning-related activities.
Interferometer Commissioning
AkiteruT et al. continued acoustic noise investigations on the H1 AS port
table (details here: http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/22/2003&anchor_to_scroll_to=2003:05:22:12:44:04-akiteru).
PaulS and LucaM continued to make progress with the H1 wavefront sensing
system. They were able to get all ten degrees of freedom under control
for the first time (details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/23/2003&anchor_to_scroll_to=2003:05:24:01:48:52-paul).
Enabling the control of the differential ITM degree of freedom resulted
in about a factor of two reduction in the pk-pk excursion of the AS_I signal
For details see:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/25/2003&anchor_to_scroll_to=2003:05:25:13:08:43-peterF.
DickG continued his investigations of the cause of the AS port beam >ellipticity
and eliminated a couple of possible causes--details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/25/2003&anchor_to_scroll_to=2003:05:26:13:46:35-gustafso
and here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/27/2003&anchor_to_scroll_to=2003:05:27:18:43:53-gustafso.
NergisM, PeterF, and DanielS investigated PRM thermal effects by locking
H1 at higher laser input power levels--details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/26/2003&anchor_to_scroll_to=2003:05:26:16:31:27-peterF.
then measuring cool-down curves in PRM lock. They concluded
that the power buildups maximize at about 2.5 watts of laser power, well
below the specified 6 W level--details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/27/2003&anchor_to_scroll_to=2003:05:27:03:00:39-daniel.
With the increase in the laser power, there were also efforts to understand
the sideband recycling gain--details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/27/2003&anchor_to_scroll_to=2003:05:28:11:07:19-nergis
and other optical gains--details here:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=05/27/2003&anchor_to_scroll_to=2003:05:28:12:27:16-peterF.
Several mysteries remain unsolved.
NergisM and PeterF changed the optical configuration on the H1 AS port table.
They eliminated the EO shutter from the AS path and replaced the telescope
on the AS periscope with a single lens. Several optical path lengths
have changed so efforts are underway to re-measure demodulation phases, etc.
LIGO Livingston Observatory (LLO) and Interferometer Operations (Coles)
(Valera)
Interferometer commissioning: Work continues on the laser intensity
stabilization servo. It is not yet fully operational. The new temperature
stabilization control box with high gain was installed and tested. It caused
the MINCO controller to rail out and so the old setup was reinstalled for
now. The noise performance observed during S2 has been achieved again after
careful alignment by Mike Fyffe. See http://www.ligo-la.caltech.edu/ilog/pub/groups/detector/logs/2003/images/05/28/mfyffe-1054111849.pdf
There was concern that we might have backstepped in some way as a
consequence of the commissioning work undertaken in recent weeks, so this
is reassuring. Ground noise is VERY high during the day at present due to
the all of the construction activity on-site. The foundation work for the
storage building, the entry gate and traffic control island, the installation
of an improved ground, and excavation of a French drain by the front entrance
have all contributed to the awful seismic environment. This very noisy work
should conclude within a couple of weeks.
I continued working on the intensity noise of the light going into ifo.
Rupal and I checked the effect of beam centering on the ISS PD on the intesity
noise of the beam after the MC. I also looked at the effect of the ISS gain
on the full ifo noise.
(Rupal Amin)
- Scan and send requisition forms to both Bonnie and UF for equipping
high power laser lab.
- Start investigation with Sany regarding UF opto-mechanics that now
reside at SLU
- Search e-logs for gain settings of PDs monitoring MC
- Searching through e-logs for WFS and Gouy telescope info.
- Investigating a simple way of checking mode matching into the MC
- Helped(?) install the half-wave plate power control on PSL
- Sketching out the physics regarding fields inside the PRC
- Building model of ISCTs and IOTs in OSLO for scatter study
- Checked the ISS board with Valera
- Checked the ISS PDs after the MC (see e-log)
- Aided in "repair" of main laser.
- Volunteered for WFS.
(Ash)
- Helped Ray characterize the LOS coil driver board.
- Documenting & preparing a user friendly procedure for Lock Acquition.
- Documenting the changes needed for the Watchdog system.
(Chethan)
CDS: Fixed a the dvd backup script for bugs. Working on updating
the auto reboot logger. Added automatic logging for vacuum system changes.
Backed up /cvs directory on tape after moving the tape to the control room.
Tested lilnux dataviewer both Grace and XMGR version.
(Shannon Roddy)
GC: Finished up a security audit with Larry last week. There are
some loose ends that I need to tie up on several machines, but for the most
part the audit went OK. Looking into a backup system for GC. The system I
am looking at would allow me to give backup capability to pretty much any
machine on site. The software is also extremely multiplatform. It will backup
anything from Solaris, Windows, Linux, and even others like Novell, AIX,
Mac, etc. The cost seems very reasonable as compared to tape backups. Preparing
for a trip to the Usenix technical conference from June 8th to the 14th.
I will be attending tutorials on LDAP directories, Samba 2.2 and 3.0, and
advance DNS administration. Bonnie's machine crashed on Tuesday. She has
unfortunately lost all of her email since it was only stored on her machine.
All of her other files and data should be OK though. I initially thought
that she had a virus, but it turns out that her machine is clean from viruses
and that it was Windows just being Windows. After about two years of cruft
builds up, this can be expected to happen. I am rebuilding her machine and
reinstalling her software. This process usually takes at least 1-2 days
since she has lots of it. I had Marcell return his computer to ASA. This
machine has been back once already. When it came back I worked with it and
did a fresh install of the OS. The machine behaves fine for a while, but
once it warms up it locks up after about 3 minutes of use. I suspect it
is either a heat problem or a power supply issue. I tried running it on
a ombination of different hardware and none seemed to fix the problem. The
only thing I was unable to swap was the power supply due to lack of a spare
ATX supply with a high enough wattage. Worked with LSU a little this week.
Seems that one of the T1s is having some problems. Rick Simmons came out
here to inspect our end and it seems that it may be a Bell South issue.
Thinking about what my requirements will be for a computer to put in the
auditorium. I plan to order it in the next week or so. Getting ready to
reinstall the machine which serves as our dhcp server. This machine is also
my workstation. Had Bonnie follow up on a quote from Sun on a 280R to replace
my web server. She will have to order it since it is above my Pcard limit.
Once the web server is upgraded I will begin offering a web mail
(Igor Yakushin)
LDAS admin:
- Setting up test replication configuration between LHO and LLO.
LDAS data analysis:
- Fixing bugs in noise_rms computation for the new LAL/LALWrapper release.
Detector/Technical Support
(Coyne)
see also the Revision Technical Review Board (RTRB) status
here
Seismic Upgrade Project
see also the LASTI report
A decision on whether to proceed with HEPI or MEPI
is still pending. Jonathan Kern and Ken Mason are getting quotes on
production parts.
Ken Mailand
- I received a preliminary quote on time
and delivery of the site installation stainless reservoir
- I
have contacted the manufacturer of the LASTI 'Aquamil' fluid and have been
referred to their lab that will do an analysis of the fluid in use now.
- I have contacted IMO pump and discussed
the issues with pump noise, and described the type fluid we are using,
and the operating conditions of the pump.
- IMO has sent me a return authorization
for the pump, they will set up the pump in the lab and run it, then
take it apart to find what may be making the noise.
- A request for quote on price and delivery
of a 55 gal quantity of clear Chem-Sol has been made, as a possible
alternate fluid.
- The fluid biological growth test is
showing nothing after 25 weeks.
DMT
John Zweizig
This week I wrote a program to infer the As Photodiode
signal from the AS_Q and AS_I signals to make it possible to look for saturation
of the PD ADC during S2. I am now running this on the L1 data. Many data
segments have been flagged so far. The vast majority are cases where the
saturation occurred just at the end of a lock and are likely a side effect
of the lock loss (or visa versa). There are however, several cases where
the saturation occurred in the middle of the science mode segment. These
will be flagged for the benefit of the analysis groups.
CDS
see also 5/28
weekly CDS meeting minutes in the commissioning archives:
CDS Software
no report
CDS Hardware
Rich Abbott reporting
- A
filter has been designed for use in the ISS that will limit the high frequency
noise issue, but not compromise the bandwidth of the servo. As of now,
we feel that the final solution is in hand, and the results of our visit
to LLO are very encouraging.
- Measurements were performed on the
new 1mm diodes to be built into the RFPD. At 7 volts reverse bias,
the series capacitance is about 34 pf and the resistance is 8.5 ohms.
- 6 more L4C field interface modules
have been tested and are ready for shipment with all the paperwork
- 2 FSS cards have been stuffed and will
be ready to ship to LHO within a day or two.
- A high speed prototype HV driver was
shipped to MIT for evaluation by Rana. This unit may be useful
in the bandwidth extension of the FSS.
Jay Heefner reporting
EMI Retrofit
- The test report was issued to team
members for comments. All comments have been received and incorporated.
The report will now be issued to a wider audience for review.
- Vendors will be contacted with the
results of the tests and evaluation of their racks and crates. They
will be asked to respond with quotes for modifications to designs that
address issues found during testing.
PSL
PeterKing
I measured the relative intensity noise of an NPRO laser
out to 2 MHz to see if the ~500 kHz noise present on the site 10-W lasers
was present. No large signal was observed. Although there was
a large peak at 13 Hz that I did not see previously. Next go around
I will check the output of a 10-W laser.
Errant Beam Blocks
Mike Smith, Ken Mailand
All baffle parts and tooling are cleaned and baked,
and on the way to LHO and will arrive Thursday 5-29.
Optics Analysis
Erika D’Ambrosio
After last visit in Hanford by Bill who measured a power
gain very close to the one predicted by my simulations when the arms are
unlocked, we kept on preparing the draft on sideband imbalance and studying
some possible explanations for the thermal lensing effect. For example one
possibility is that the curvature of one of the mirrors does not coincide
with its nominal value. The numbers we have are due to measurements made
in Australia as far as I understood. The reflectivities are also due to different
measurements and there is a 10% disagreement. Also the last cool down curve
that has been measured by Daniel et al. is somehow strange.
Unfortunately
I can only use the starting and the ending value of the cool down curves
and the latter is used for scaling the former, so that basically there is
only one number available. The set of simulations I ran are characterized
by one parameter, that is the lensing effect. I had not even split that in
coating and bulk contribution and I had not split that in x and y arm.
However
the two measurements I had previously taken into account were at least consistent:
the two intercepts for the absorbed power are in the same ratio as the two
input powers. Scaling the maximum gain by the asymptotic power in the last
measurement gives a result that is not easy to understand unless more than
30mW are allowed to be absorbed into the mirrors. In this case we should
be exploring the other side of the curve. However this would not agree with
the model for thermal lensing which has been used for predicting maximum
gain at 6W of input power. That model implied 15mW of power are absorbed
in the bulk and 10mW in the coated surface of the mirrors when the system
is at its working point.
Optical Contamination Cavities
Lee Cardenas, Liyuan Zhang
OTF Lab. (W. Bridge)
Contamination Cavity # 1
The test sample kAPTON (Polyimid paint) contamination test was completed.
The ring down and beat frequency measurements taken everyday was completed
and basically the test sample showed no contamination to the mirrors. Total
loss = 0.0 +/- 1.3 ppm/year, absorption loss = -0.2 +/- 0.2 ppm/year
We have now introduced into this cavity a new test sample a 10mm
Capacitance position sensor, which consists of a sma cable and a ceramic
connector at the end. The whole cabling was introduced and the chamber
is pumping down and cavity is locked and we are taking ring down and beat
frequency every day.
Absorption Test Measurement prototype in progress
The absorption measurements of a 5 inches diameter sapphire mirror
was completed. We got another 1.00" sapphire mirror which is
tested for absorption and it is in progress. Absorption results will
be released soon by Liyuan. Liyuan will be meeting with vendors to
acquire a high power laser for our absorption test bench.
Scatterometer system is in STANDBY for measurements. We
will be updating our optical train by replacing new mirrors and lens and making
a precise alignment to ensure measurement repetition more accurate without
having to adjust the alignment to catch the reflected beam each time we replace
a new mirror to be tested.
OTF Lab at Lauritsen ROOM 38
Cavity #3
As specified before, cavity with 50 ppm mirrors is hard to make it work.
After all the efforts to improve it, all we got was a power of only
~90 mw and its visibility ~70%.
We opened the chamber again and replaced it with a cavity with 70 ppm mirrors
and hung with one end at 1.8 degree higher that the other end and pumped
it down and made alignment, locked the cavity and we got 120 mw of power
with a 95% ! visibility. BUT the output still small in order for us to use
it. We found out by Helena that these 70 ppm. mirrors was not fully
cleaned as it should because the flat mirror has a small scratch almost on
center. We found two new sets of 70 ppm mirrors that Helena cleaned
for us and we have replaced with these ones. Now the cavity is locked
with these new cleaned mirrors and the power obtained is 147 mw. We
are improving this cavity as time goes by and cavity gets more stable.
Cavity #2 Test cavity STILL in STANDBY waiting on silver plated screws to
be replaced. Optical train upgrading is in progress.
40 Meter Interferometer (Weinstein)
May 30, 2003
Suspended mass mode cleaner (Ugolini, Miyakawa, Vass, Abbott):
- Dennis and company diagnosed and fixed a set of problems associated
with the new MCL electronics path, and the mode cleaner is now locking robustly.
- He measured the transfer functions from the MC servo board to the
coil driver. He discovered a filter on the Pentek Interface Board that apparently
was implemented at LLO; we don't know why it's there, but it didn't exist
in our old path; Dennis bypassed it. He found a gain 10 stage in the digital
PZ filter, which is not a good place for it (it amplifies any offsets); he
took it out. He found that the software filter that compensates for the hardware
dewhitening was not set correctly, and fixed it Finally, he found that the
RF local oscillator cable was 180degrees out of phase with what was needed
(don't know why!). He shortened it. After all that, the MC locked immediately
and robustly!
- We still have to optimize the gains, cross-over frequency, and other
parameters, to minimize the frequency noise. This can wait till Osamu returns.
Core digital suspension controllers (DSC), LSC, ASC, and other
Electronics (B. Abbott, Heefner, Bork, Taylor):
- All 6 installed optics are damping well. There is an issue with the
Universal Dewhite board which is the wrong Rev for the MC2 optic, however.
Dennis and Ben are fixing this.
- Ben and Art are populating the two end racks (ETM DSC's, oplevs,
QPD's, etc). They are progressing rapidly and hope to complete the wiring
by Monday.
- Rolf is working on the software required for the end DSC's. He reported
last week that the work required to prepare the end DSC software should only
take a few days. Rolf hopefully has the Pentiums, Penteks, RM cards and fiber
cables that are required.
- We will bring the GPS time signals from the vertex area to both ends
via long (40m) cables. We hope this will work; if the signals degrade too
much, Jay and Ben are thinking about building an optical driver for the signals.
- Jay reports that work on the rack and wiring diagrams for the ASC
and LSC has resumed and should be complete by the end of the week.
- From Jay: A new board for interfacing the beam line QPDs to an ICS110B
has been designed. After the wiring diagrams and cross connects ahve been
designed this board will be layed out and sent out for fab.
- Lisa continues to develop the EPICS controls (screens, state code,
and wiring and cabling) for the video switch, and Steve is ordering monitors
for the control room.
Mode Cleaner WFS system (Ourjoumtsev, Abbott, Eichenfield):
- Alexei has checked out all the IQ demod boards for the WFS system.
He is tuning the boards so that there's exactly 90degrees RF phase difference
between I&Q. He's preparing to determine the overall phase to maximize
the misalignment signal.
- Alexei and Ben will continue to debug and commission the photodetectors,
electronics, and actuators (PZT mirrors on the PSL table) for the WFS system.
- We will pursue feedback to these PZT steering mirrors and to the
MC suspended optics; so we are following the work done by Joe Kovalik and
Valery Frolov at LLO.
- Alexei continues to prepare the EPICS screens and databases that
control the WFS system.
- It would be really nice to be able to use dtt to produce a transfer
function for the MC ASC. However, dtt can't operate in real-time (for transfer
functions) unless the computer it runs on is synch'ed with the data (GPS
time) to within 1 second (accd to Daniel Sigg). This requires NTP to be running
on the machine, to get the network time from our gateway computer, which hopefully
can get the time from some accurate clock on the campus net. It's not clear
whether this will be possible; we have asked Larry & Lisa to help. We
may have to purchase a GPS-based NTP server for the lab.
- SURF Matt Eichenfield is learning Matlab/simulink to model the MC
WFS system properly.
Suspended optics:
- Bob will be baking the SRM optic this weekend. Early next week, Steve
will rehang it, and prepare it for installation. That's the last of the core
optics to be prepared.
PSL and ISS (O. Miyakawa, B. Abbott, R. Abbott, F. Nocera, D. Ugolini,
S. Vass, C. Mow-Lowry):
- Conor wants to measure the cavity pole of the pre-mode cleaner,
but it is too high to measure by conventional means. Nergis suggested that
we obtain a broadband AOM, and Conor will see if we can scare one up.
- Conor continues to develop a detailed layout of the PSL which reduces
the number of turning mirrors and picks of the FSS beam after the PMC. He
and SURF Matt Eichenfield are calculating all the mode matching lenses that
are required for the new layout.
Optical sensing (Smith, Ourjoumtsev, Goggin, Miyakawa):
- OPTICS PARTS LIST, Received parts: 1 Brewster's angle polarizer for
SPS anamorphic prism steering mirror from KLC; New mirror holders for PZT
steering mirror.
- Orders pending: 1 q-switch E/O shutter from Fast Pulse.
- FARADAY ISOLATOR: Parts are baked and ready for assembly.
- OPTICAL LEVER ASSY: Assembly on hold
- IFO STEERING MIRRORS: All parts are on hand, ready to be cleaned
and baked.
- MODE MATCHING TELESCOPE: Parts are baked and ready for assembly.
- SPS BREWSTER PRISM MIRROR: All parts, except for the Brewster prism
are baked and ready for assembly. The Brewster prism is on hand ready to
be cleaned and baked.
- Mike will work with visitor Koji Arai to assemble, align, and prepare
for installation, the Faraday isolator and mode matching telescope. They hope
to begin the work by the end of this week.
- Mike is working on designing an AdvLIGO R&D experiment with
a SURF student this summer to study photon-force induced movement of a locked
cavity mirror. The 40m mode cleaner cavity curved mirror will be pushed with
an external photon beam and the loop response will be measured (photon calibrator).
It may be possible to actively control the mirror position with the photon
beam within a narrow frequency band (photon actuator).
- Alexei installed one EOS on MCR. It is not yet powered, so a half-wave
plate is in place to permit the beam to get to the MCR LSC photodiode and
WFS's. Unfortunately, the EOS controller box is dying on him; he will work
with Sander to debug it.
- Alexei continues to prepare the EPICS screens and databases that
control the electro-optic shutters. Dennis has booted up the the EPICS cpu
(c1aux) in 1X1 which will control these devices. He and Bob will get the
remaining cables in place.
- AC power is being run to the small racks that hold EOS electronics,
from rack 1X1.
- Steve ordered picomotors and one controller for our shutter flags
(one goes in front of every test mass, to block or attenuate the beam if
desired). Bob has vac-prepped the shutter flag parts.
Facilities and vacuum envelope (Ugolini, Vass, Jones):
- Steve got the cranes inspected. The vertex crane did not work (again!).
The crane repair guy fixed it today.
- Steve has arranged for power to be installed for a portable A/C unit
for the control room.
South Annex Bake Ovens (Taylor):
- Cleaned and baked the parts for the Mode Matching Telescope.
- Cleaned, baked and shipped the Baffle parts for LHO.
- Cleaned and baked the Faraday Isolator parts.
- Cleaned and baked the Brewster Mirror ASSY.
- cleaned and baked the special fix in vacuum 1.5 Mirror Mount.
- Helped Art with wiring the So. End 1Y9.
- Cleaned calcite Prisms for Faraday Isolator.
- Finished Hybrid OSEMs for Janeen.
- Will finish cleaning and start bake job on silver mirrors tomorrow.
- will start bake job on ETM optic tomorrow.
Thermal Noise Interferometer (Libbrecht)
Previously we reported that we were looking for sources of phase loss above
100 kHz in the mode-cleaner servo, in preparation for improving our frequency
stabilization at high frequencies. This week we identified the remaining
sources of phase loss as a pole in the RF photodiode's response at 700 kHz,
and an apparent 60 ns delay in the mixer. We are now able to model
the response of the Pockels cell path accurately in both magnitude and phase
up to 30 MHz, well above our expected unity-gain-frequency. We have
now begun design on an amplifier, based on our current model of the system,
that will implement the fast-frequency-correcting Pockels cell path up to
a few hundred kiloHertz.
LASTI (Zucker)
LASTI (Adhikari, Allen, Coyne, Mason, MacInnis, Mittleman, Nayfeh, Ottaway,
Rankin, Rollins, Shoemaker, Zucker, Zuo)
HEPI
We have been working on the hydraulic pumping system. With the optical
isolator from Rich Abbott installed in the pressure sensor signal path we
have looked at the pressure spectra. Except for some high frequency signals,
which are independent of the pump, the pressure noise meets the required
noise specifications.
We are currently replacing both the pump and the motor with the new models
supplied by Ken Mailand. Myron is developing a precision alignment procedure
to reduce wear and vibration in the coupling (see the LASTI ilog for results).
MEPI
We are still working on the sensor correction coefficients.
We have developed a matlab model of the sensor correction using measured
and modeled transfer functions to set the sensor correction coefficients
and filter functions.
We are also using a measured time series from all of the sensors as a second
approach.
PSL
Jamie continued characterization of his advanced intensity stabilizer and
is writing up his results to date.
Rana further updated and characterized the frequency stabilizer electronics.
Data Analysis and Computing
(Lazzarini)
Simulation and Modeling (Bhawal)
E2E weekly Physics meeting
Luca described the lock acquisition problem recently faced in H1 and issues
related to increased input power. Luca and Matt also discussed about Wavefront
Sensor issues and how SimLIGO could be effectively used to look into the
problems. Generation of noise curves from SimLIGO was also discussed. Attendees:
Luca, Matt, Virginio, Hiro, Biplab.
New Optical Model
(Matt) This week I returned to the new optical model code. My intent
is to do some final documentation and testing, then hand it over to
Hiro for work with the summation cavities and eventual incorporation
into E2E.
Code development and maintenance
(Hiro)
Modeler support:
Several example programs using e2e are posted in the e2e home page.
(1) pendulum with locking servo
(2) Simple FP (ETM moving longitudinally)
(3) FP simulation using multi mode (ETM moving and rotating)
Modeler code:
Hiro and Melody worked together to investigate various compiler issues,
including
- optimization (-O4 and above do not exist, -O3 is not necessarily
faster than -O2, these are documented and are consistent with our experiment
using e2e, CPU specific options using SSE on Xeon was tested to speed up
10-20%),
- compiler dependence (gcc 3.2.2 and gcc3.3 generates binaries which
generate different results) and
- machine dependence (SUN gcc2.95.3 and linux 3.2.2/3.3 do not match).
Investigation is still going on to resolve mysterious issues to make
sure correct simulation results are generated.
CVS and tarball distribution:
A meeting was held (Hiro, Ed, Bruce and Melody) to follow up the last week's
meeting about the reorganization of CVS so that a leaner and cleaner tarball
would be distributed. All obsolete components, including C++ based alfi (alfi4
and older), are "deleted" from CVS (still one can get codes if needed), and
the tarball contains only the minimum needed.
(Melody)
- Preparing build instructions with discussed changes for the upcoming
build.
- Installed gcc 3.3 in the Linux box with Virginio's assistance.
- Trying to figure out the differences in the results generated by the
different versions of gcc in different platforms (Linux and Sun).
(Ed Maros) Removed Alfi from CVS.
Alfi
(Bruce)
- Completing work on port repositioning in external view (PR 380, 391)
- Working on E2E_PATH issues (PR 395)
LIGO Data Analysis System
Software Systems (Blackburn)
We are now in a code freeze in preparation for the 0.7.0 release of LDAS.
I would estimate this release to be between one and two weeks away. As of
today, we have begun rerunning all system level tests. Only bug fixes that
have been approved will be allowed into CVS for this release.
It was discovered this week that the DB2 version 8.1 that we have been
evaluating for the next LDAS release (0.8.0) only supports a 90 day evaluation
license, even though it was licensed under the Academic Scholastic Program
at IBM. This was just reported to LDAS team leaders yesterday so working
the problem to find the constraints has just begun. In the worst case
we could buy the licenses for roughly a thousand dollars per DB2 server.
The issue with using certain NDAS frames in LDAS continued this week. The
confusion levels have only gone up since last week. We still do not know
what in the NDAS frames the LDAS Frame I/O library is unhappy about. It appears
that some NDAS frames point to illegal locations on the file system for
locating particular data sets. But this issue is not seen in the framelib
I/O libary from VIRGO. We have modified our FrVerify to report more details
of the issue and are now modifying the FrDump code to report additional details
to locate the problem. Note that some NDAS frames do not cause any issues
in LDAS while others do.
The memory leaks in the metaDataAPI have now been fixed. However, the dataConditionAPI
still has a one to two kilobyte leak per job. There has been some isolation
of the memory leak to certain types of jobs, but no progress in identifying
the place in the code that causes the leaks. Use of memory leak detection
tools such as valgrind and insure++ on standalone codes based on the same
code base have not pinpointed the problems either.
New code from Penn State for Kalman filtering was checked into CVS this
week. Eric Rotthof (the author) has made many fixes and brought the code
up to date for the new GCC compiler.
We have begun testing LDAS against the newest GCC compiler (3.3). This
compiler will be the foundation for the 0.8.0 release of LDAS but not for
the 0.7.0 release which uses 3.2.3. LDAS has been shown to work with only
one issue under Redhat 9 with this compiler. The issue is with the new DB2
8.1 developers library and our interface in the metaDataAPI to that version
of the library. Looks like we will need to modify out dbEasy library (ODBC
interface library) to work properly with DB2 8.1. We are now beginning to
evaluation this compiler under solaris.
Hardware Systems (Anderson)
Caltech
(Dan Kozak)
- Assisted with T3 failures/reconstruction at both LHO and LLO.
- Continued SAM-QFS hand holding (recovering from stuck tape situation,
running archiving by hand, etc.).
- Assisted in unpacking and installation of new Sun gear (Jupiter switch,
2 3510s).
- Working on setting up to re-archive all SAM-QFS data on 9940B drives.
(Al Wilson)
- Install DB2 on test system for Solaris.
- Have System images for CIT beowulf and datacon ready for install.
- Over the weekend took care of some BB daemon starting problems.
(Stuart Anderson)
- Received the last LDAS construction account order from Sun Microsystems
and started unpacking and installing: 10 FC disk units, 1 2Gb/s FC switch,
and 4 dual-1.2GHz rack mount servers.
- Received notification from ASA that 98% of the chassis needed for
the large LDAS Beowulf cluster order have been received by them and that
108 out of the remaining 310 units have been assembled. This confirms
that ASA is still on schedule for a June 6th ship date.
- Placed order with Larry Wallace to get additional fiber patch cords
for the new LC GigE standard and new FC disk storage.
- Continuing to help support the electrical work for the Synchrotron
computer room upgrade. The floor mount for the additional cooling unit
has been installed and bolted to the floor.
Livingston
(Igor Yakushin)
- Setting up test replication configuration between LHO and LLO.
Hanford
(Greg Mendell)
- The multiple disk failure that I reported last week on t3-14 was
fixed by Ben Johnson without loss or corruption of data. Only one
disk had failed, but the replacement of this faulty disk failed to reconstruct,
causing other disks to go into fault state. Reseting the volume and T3
and running the disk recon command by hand fixed the problem. Ben
Johnson had written a detailed report on the fix in LDAS Gnats Problem
Report 2002.
- Assisted Ben Johnson with the installation of a new UPS, transformer,
GigE switch and FC switch in the LDAS room. In general, we are working
towards recabling the room and installing the new beowulf clusster which
should ship to LHO on June 6.
(Ben Johnson)
- Rearranged racks in the LDAS room so that we can start building our
new cluster without taking down the old beowulf. APC 5000VA UPS, and 30A
step-down transformer have been placed in a new rack.
- Physically installed new GigE and FC switches. No software configuration
of either has been done.
- Room now has a cable ready to become part of the CDS network. This
will initially be used for a temperature monitor that will place data into
the EPICS system.
- Replaced u1ctr controller card in t3-4. This did not fix the odd notices
it has been reporting. Continuing to work on a solution.
Data Analysis Activities (Lazzarini)
K. Reilly:
Most of my time now is being spent learning how the stochastic DSO works.
This is my first introduction to LAL an LALWrapper so it is taking some
time. I have also re-started going through the GW phyics notes and
looking up the references explaining the theory behind the stochastic data
analysis. I have begun preparing for next week's talk.
Mendell:
- Continuing to work on a proposal with Mike Landry for the PULG group
to start writing a stackslide DSO to run under LDAS, in preparation for
the PULG face-to-face meeting June 16-17.
- Continuing to prepare my SURF student project, which is to study various
methods of parameter estimation for continuous wave sources.
- Opened LDAS Gnats PR 1997 and worked with LDAS to resolve a bug that
causes the start_freq to be set incorrectly when requesting frequency series
data (in my case SFTs) with an initial gap in the data for the times
requested.
Yakushin:
- Fixing bugs in noise_rms computation for the new LAL/LALWrapper release.
Weinstein:
- Continuing to edit the Burst S1 paper.
- Working a bit on hardware injection analysis, with Laura.
Creighton:
Finished writing and testing LAL routines for double-precision time-domain
filtering of single-precision data. These routines reduce truncation
errors, and also (surprisingly) execute 20% to 30% faster than the existing
single-precision time-domain filtering routines.
Lazzarini:
Completed a new analysis for the stochastic group. This is motivated by
the inspiral group's "chi2" analysis on the consistency of a signal's
spectral content with the expect model signal. It is the f-domain analog
of the time-shift chi2 analysis I conducted for large amplitude
injections. The analysis uses the run-averaged cross-correlation statistic
spectrum and related optimal filter spectrum. Results are in nice concordance
with the optimal filtering results -- the so-called "point estimates". However,
for the H-1H2 pair this provides a way of quantizing the degree to which
the observed negative correlation is inconsistent with astrophysical process
(let alone the sign of the effect!).
General Computing (Wallace)
Livingston:
(Shannon)
- Finished up a security audit with Larry last week. There are
some loose ends that I need to tie up on several machines, but for the
most part the audit went OK.
- Looking into a backup system for GC. The system I am looking
at would allow me to give backup capability to pretty much any machine
on site. The software is also extremely multiplatform. It will
backup anything from Solaris, Windows, Linux, and even others like Novell,
AIX, Mac, etc. The cost seems very reasonable as compared to tape
backups.
- Preparing for a trip to the Usenix technical conference from June
8th to the 14th. I will be attending tutorials on LDAP directories,
Samba 2.2 and 3.0, and advance DNS administration.
- Bonnie's machine crashed on Tuesday. She has unfortunately lost
all of her e-mail since it was only stored on her machine. All of
her other files and data should be OK though. I initially thought
that she had a virus, but it turns out that her machine is clean from viruses
and that it was Windows just being Windows. After about two years
of usage, things build up and this can be expected to happen. I
am rebuilding her machine and reinstalling her software. This process
usually takes at least 1-2 days since she has lots of it.
- I had Marcell return his computer to ASA. This machine has been
back once already. When it came back I worked with it and did a fresh
install of the OS. The machine behaves fine for a while, but once
it warms up it locks up after about 3 minutes of use. I suspect it
is either a heat problem or a power supply issue. I tried running
it on a combination of different hardware and none seemed to fix the problem.
The only thing I was unable to swap was the power supply due to lack
of a spare ATX supply with a high enough wattage.
- Worked with LSU a little this week. Seems that one of the T1s
is having some problems. Rick Simmons came out here to inspect our
end and it seems that it may be a Bell South issue.
- Reviewing what requirements will be for a computer to put in the
auditorium. I plan to order it in the next week or so.
- Getting ready to reinstall the machine which serves as our dhcp server.
This machine is also my workstation.
- Had Bonnie follow up on a quote from Sun on a 280R to replace my web
server. She will have to order it since it is above my Pcard limit.
Once the web server is upgraded I will begin offering a web mail
server like the one at Caltech.
Hanford:
(Christine)
- Attended a phone conference with all people involved with the network
upgrade. Sounds like our upgrade to OC3 should happen about mid June.
- Setup another SURF student accounts on the network.
- Started writing up the PR for the GigE network equipment.
- User support.
CIT:
(Mike)
- Setup a surf student's workstation and loaded additional software
for this user.
- Worked on loading some software for Calum that failed I have to do
some research on this product.
- Finished up loading two PC's for in-coming surf students. I still
have to ghost these machines then setup move them on up to a cubicle.
- Went through security logs checking for intrusions and OS/hardware
errors. Intrusions were unsuccessful. OS errors were minimal. There are
some hardware errors on Pictor that need to be taking care of.
- Had to replace a hard disk, due to bad blocks being reported in event
viewer. I restored this server from a ghost image and it is now back up
and running.
- Found some issues on trying to build a system using a Ghost image
when trying to build a image of Larry's portable on to another unit. Will
work on that issue later.
(Lisa)
- Miscellaneous user support
- Vacation
(Veronica)
- Advanced LIGO CD and website for the NSF Review Panel were again
the top priority in the last days of last week. CD preparation required
rewriting several scripts and importing support files to make it 'self-contained.'
After the AdvLIGO cost/schdedule documentation was finalized late
Friday afternoon, a batch of 26 CDs was burned and shipped to the NSF in
a narrow time slot before the holiday weekend. A copy was sent to David
Shoemaker, and a tar archive of the CD was posted per his request. I updated
the website to mirror the CD and made other changes required before its
publishing, and keep maintaining it.
- LIGO website: catching up on what was pushed aside in the past days
as I was working on Advanced LIGO. Working with George Stokes on
troubleshooting the DCC databases; support for George in accessing/testing
the database per his requests. User support for the Advanced Suspensions
group (a webpage, vnc).
- Project Science: Support for the upcoming October workshop. Sent out
announcements and filed responses of prospective attendees.
- LSC website: catching up on postings accumulated during Advanced LIGO
crunch.
- CaJAGWR website: upkeep and user support.
(Larry)
- Performed a few more tests for the GC audit at Livingston. Overall
things went well. Shannon and I did not get everything tested out, a number
of distractions took up some of the time we needed but we did get a pretty
good view of things. I am working on a report of what we found and
hope to have it out next week. Just as a note from the audit at Livingston
and going over some of the PC's here at Caltech, the PC Windows users
should be running the defragmentation and virusscan on a regular basis.
There are a number of people that do and they seem to have fewer problems
than those that do not.
- Spent time working on a number of PC's. Everything from printdriver
problems to rogue processes. We are trying to get a list of the unneeded
processes that can be killed in Windows. Also, discovered that some of
the patches can cause windows to perform slower but Microsoft is working
on a fix.
- Attended the Hanford LIGOWAN meeting with Christine. Things are looking
good. There will be a short network outage at the Hanford site this
evening (May 29th) as PNL will be setting up their new router. If all goes
well we should have our OC3 connection in by mid June. Christine is presently
working on the setup of the new router the Observatory is to install for
the switchover.
- Worked a number of user accounts and issues. Added a couple of new
people to the system.
- A group of us worked a couple of VRVS issues with Callum. VRVS now
no longer supports the audio part of the USB cameras. So now you need a
separate microphone on the computer. The built-in mic on the laptops appears
to still work. I used the VRVS system while on travel and did not have
a problem.
- The e-mail monitoring and adding locations to the filter table is
and will be a daily task.
Advanced LIGO Development (Shoemaker)
Advanced LIGO and supporting R&D
Seismic Isolation
No report
Suspension
From: Janeen Romie
<romie_j@ligo.caltech.edu>
AdLIGO
Suspensions
Six hybrid osems
are with Bob Taylor being assembled. He hopes to get them completed this
afternoon with Helena's help.
Helena and Calum will assemble them aand Mark will set up the electronics for the mode
cleaner.
Preparing for the NSF review.
<!--[if !supportLineBreakNewLine]--><!--[endif]-->
From: ctorrie <ctorrie@ligo.caltech.edu>
1) QUAD Layout for the ETM
a) Eddy Current Damper (ECD)
- A lightweight 4x4 array design has now been drawn up, this weighs
approx. 180g compared to the original weight of 460g.
- A couple of test arrays will be made along with several different
2x2 arrays. the plan is to show that the lightweight
arrays gives comparable damping as the original design.
b) Upper Mass
- Mike Lloyd and I are continuing with the layout of the upper mass.
Several aspects have now been added including the wire fixtures and pitch
adjustment.
2) Cantilever Blades
- Mike Lloyd, mike Plissi and I are working
on updating the drawings for the MC and RM blades to include the design
information. It is hope we can start getting prototype RM blades made very
soon. We have also started writing up some of the experiments and analysis
we have been doing on different aspects of the blades.
- An initial concept exists that will allow us to easier test the deflection
of the new RM blades and hopefully several proposed prototype quadruple
style blades. Hopefully production on this will start early next week.
3) MATLAB model
Norna and I have been working on creating
a help file, a schematic explaining the parameters and including revision
control oin the quad input file. It is hoped
that a new set of files with the 2001 MIT quad parameters can be sent to
MIT later this week.
4) MC Suspension (OSEMS)
6 Anodised Aluminium osems have arrived
safely from the U. of Glasgow.
These have been tested, assembled with LED's, PD's and pigtails. On Thursday
morning Helena and I will install these in the suspension and then start
damping tests with Mark Barton. Twenty new lightweight, one piece,
coil clamps have also arrived from the U.
of Glasgow.
Pre-stabilized Laser
From: Peter King <pking@ligo.caltech.edu>
I am in the midst of preparing material for the up-coming
NSF Review.
Input Optics
No report.
Core Optics
From: Helena Armandula
<ahelena@ligo.caltech.edu>
Sodium Silicate Bonding, SF4 / Silica
Bonds:
- Performed a few baking tests on 4 bonded SF4 / Silica bonds.
- Baked 4 parts at 80 degrees C for 1 hr on two
different baking loads (2 and 2).
- Turned oven off, allowed to cool for about an hour and removed from
oven when the parts were still warm. Observed a fair amount of stress on
the parts, by eye and thorough a polariscope; the SF4 on one of the bonded substrates cracked
without the parts separating.
- Unlike silica / sapphire bonds, where the
stress remained when the parts cooled, the
stress on the SF4/Silica bonds disappeared when the substrates cooled.
- The tested parts came from 2 different
bonding batches, 2 of them were aged longer than the other 2. Silicate
solutions were also from 2 different lots, one being older (time of purchase)
than the other. Except for the cracked part, all the others looked similar
under a dark field microscope.
- Have not tested for strength yet.
Auxiliary Optics
From: Michael Smith <smith@ligo.caltech.edu>
Working on designing an R&D experiment for a SURF student this summer
to study photon-force induced movement of a locked cavity mirror. The 40m
mode cleaner cavity curved mirror will be pushed with an external photon
beam and the loop response will be measured. It may be possible to actively
control the mirror position with the photon beam within a narrow frequency
band.
Interferometer Sensing and Controls
No report
Data Acquisition, Diagnostics, Network & Supervisory Control
No report
Other Laboratory R&D
TNI (Sander Liu):
Working on the preliminary circuit board design for the TNI boost amplifier.
Shipped ten 850 Hz filter modules to LHO.
From: Youichi Aso<aso@granite.phys.s.u-tokyo.ac.jp>
Eric
Melted a series of new candidates, one looks like another step forward
towards a glass. Am having problems with explosion while melting due
to thermal stresses and
seeminly brittle casts,
beleive this is due to high
Si concentration, will lower this and see what happens.
Greg
- Cast thicker rods of the new alloys.
- X-rayed new rods; not as glassy as before
- Tried developing technique to make x-ray spectrum clearer. Trying to reduce noise from Iron fluoresence.
Allyson
I am currently comparing the UCLA
vicker hardness
results to the Caltech ones. The UCLA ones seem to be more
consistant. I am planning to finish the indentations
using the UCLA machine next week.
Enrico
- I continued working on the simulation made with bench.
- I analyzed the effect of changing the length of the last two suspension.
- I modified the program to obtain the as output also the signal to
noise ratio for the coalescing binaries including a cut off frequency
(due to the template limitations over the inner stable orbit frequency)
and the cosmological red shift correction.
- Now I'm trying to obtain the same outputs by two interferometer working
togeter.
Youichi
- Modified the program to calculate MGAS blade shapes to improve the
speed.
- Now checking the validity of the results.
Also writing documentation.
- Waiting for clamp pins for test.
For additional information about this report, contact sanders@ligo.caltech.edu