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The LIGO Executive Committee Agenda for Monday June 9, 2003 will be:
CANCELLED DUE TO NSF REVIEW PREPARATION
no report
LIGO Weekly Site Telecon (Lindquist)
There was no site teleconference on Thursday, June 5, 2003 due to the
Program Advisory Committee meeting.
PROPERTY MANAGEMENT (Chargois)
From: Ed Chargois <chargois_e@ligo.caltech.edu>
No report this week.
DOCUMENT CONTROL CENTER (Turner, Mak)
>From: Linda Turner - turner@ligo.caltech.edu>
No report this week.
> From: Cleveland Mak <mak_c@ligo.caltech.edu>
Processed and distributed 7 DCN's
DCC Activity
WE 06/5/03 Packages/Faxes
In
20/36
Out
13/47
COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman, Salone)
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
Completed the internal modification to CSRS, change order 3 and an
internal modification for funds transfer to Star Service to re-do the Air
Condition system. Completed change order 6 to Excel Group. Working
on change order 16 to Research Electro Optics and change order #14 to Crystal
Systems.
Working with Ed Jasnow and Bill Tyler on the Raytheon work order.
Submitted the subcontract files on MIT, Northrop Grumman, and Butler
to the PWC auditors for review.
Placing and reconciling pcard orders.
From: Gina Salone <gsalone@ligo.caltech.edu>
No report this week.
From: Florence Kaufman <fkaufman@ligo.caltech.edu>
Completed monthly financial reports which have been posted on the network.
Financial reports can be found at: http://docuserv.ligo.caltech.edu/~fireport
SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)
From: irena@ligo.caltech.edu (Irena Petrac)
AdLIGO Optics Coating RFP: The RFP package is out on the street. Proposals
are due end of the month. Proposers Teleconference is planned.
Crystal Systems Inc.: CO No. 14, for the purchase of additional HEM
sapphire test flats, was released to Purchasing.
Research Electro-Optics: CO No. 16, for coating of additional LIGO
supplied test optics, was released to Purchasing.
From: Ed Jasnow <jasnow@ligo.caltech.edu>
CONSTRUCTION:
We continue to go down to the wire in spending out the remaining construction funds by June 30. Computer deliveries, completion of the LLO pre-fabricated storage building, and resolution of retention issues for Chervenell at LHO are the big drivers at this point.
OPERATIONS:
P-cards for new employees at the sites remains an issue since they must
be trained personally by the P-card team at Purchasing Services.
Arrangements are being made to have members of this team go to the sites
to train multiple numbers of new employees
SUPPORT (Baldon, Lloyd, Tischler)
>Irene Baldon
Processed the paper work for Thirty (30) new/revised trips. There
are approximately fifteen (15) trips in various stages of completion before
ticketing can be done and/or paper work completed. And an additional
seven (7) 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 four (4) Expense Reports and there are seventeen (17) 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 are six (6) reports more than 30 days old at this time.
Reconciled sixty-five (65) 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 June 2, 2003. Arranged three (3) new teleconferences and arranged
five (5) 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 26.
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
Advanced LIGO (Frey)
From: Thomas Frey <tfrey@ligo.caltech.edu>
Attended PAC meeting all day on Thursday the 5th.
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)
Finished updating the top level schedule prepared by Dennis in MS Project.
Continued preparing revised budget sheet data.
Corrected issue with total cost summary report and generated subsystem
cost summary reports as requested by David and Dennis.
Prepared a detailed cost sheet that shows only the costs included in
the request for Outreach as requested by Phil for Gary and Fred.
The following is a summary of status by sub system:
COC - Still need completed WBS dictionary and BOE. Garrilyn provided
a minor change to a WBS definition.
PSL - No action items pending.
AOS - Still need completed WBS dictionary and BOE. Sent templates
to David Ottaway.
IO - Still need completed WBS dictionary and BOE.
SUS - No action items pending.
Attended meeting and answered questions related to SUS interface with
LASTI.
SEI - Received revised (Version 3) data from Dennis and data input
of WBS and BOE is in progress. Completed WBS entries and will finish
BOE by Monday AM.
SC - Still need completed WBS dictionary and BOE. Issued WBS
and BOE templates to Peter F. to complete input.
LDAS - No action required at this point in time.
INSTALL - Dennis provided a revision and data input is in progress.
Completed WBS entries and will finish BOE by Monday AM.
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.
Continue to update the LASTI Schedule and incorporate any changes.
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.
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.
Preparing reports requested by Dennis and David, required adding some
reports and I made some changes to the cost database to accommodate other
requested reports.
Development of the Advanced LIGO Project Controls Guidebook continues.
Reports (Lindquist)
No report this week.
Change Control/Contingency (Lindquist)
A change board was held during the Executive Committee Meeting on Monday,
June 2. Minutes will be prepared and distributed.
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>
Nothing significant to report this week.
The 2K MC was locked and the pointing of the input train roughly restored.
No one had time to look at the 4K MC as of yet. To fix the pointing of
the 4K ITMX we are in the process to bring the coarse actuation system
for BSC 3 back to live. There are no other optics mounted on this table
so we should be able to rotate the table from the outside. The final word
on the asymmetry fix and the ITMX replacement will of course have to wait
until we have the arm cavities back.
In preparation for the vent, steering of the POY beam was dead reckoned;
see here.
More power at the AS port resulted in 10W over 10ms on the photodiode, killing it: don't look here.
H1 arm cavity lengths were measured, yielding Yarm: L= 3995.04437 m +,- 0.08mm, Xarm: L= 3995.08418m +,- 0.08 mm, Arm length difference = 39.81 mm, Yarm shorter. Details are here.
A new optics train layout on the AS port appeared to improve the noise in the 100Hz region; look here.
Potential beam clipping on the POX port was investigate, see the entry
here.
Dear Colleagues:
I will be leaving LIGO later today to begin my
new position at the NSF. Before I go, I want to let everyone know how much
I have enjoyed working with all of you, and express the special privilege
I have felt to be a part of the LIGO team. What we have accomplished together
has been spectacular. It has truly been a grand adventure to be part of
the effort that has transformed an arid stretch of tumble weeds and a snake
infested swamp into gravitational wave antennae with extra-galactic reach.
I'm confident that even more remarkable achievements are in store as LIGO
continues to progress.
I'd especially like to thank Barry Barish and
Gary Sanders; for hiring me in the first place more than eight years ago,
and for their kind and generous support as this opportunity at the NSF
has evolved. And finally, I'd like to express my thanks and appreciation
to the resident staff and LSC colleagues at LLO for all they have done:
their countless hours of hard work, the camaraderie, and the shared enthusiasm
that have made our efforts so worthwhile.
I'm extremely pleased that a candidate as able
as Mike Zucker will be taking over as the new LLO Observatory Head, and
look forward to hearing of your continued successes.
Mark
GHS NOTE: WE ALL WISH YOU WELL IN
YOUR NEW CHALLENGING ROLE. GOOD LUCK MARK!
D. Coyne note: This web page needs a number of revisions/updates. EPI and RFI change requests have been submitted to the CCB. A proposal for implementing an independent timing check system with atomic clocks has passed RTRB review and will be submitted to the CCB for evaluation as well. The low noise DAC effort is close to a point where the RTRB can review test results and a CCB request for funding a production order can be generated.
Awaiting a decision from LIGO management on which EPI system to pursue for deployment at LLO.
Ken Mason has sent all EPI actuator/spring assembly parts out for multiple bids for production.
HEPI Pump Station
Ken Mailand
see also the 40m Lab report
Dennis Coyne reporting for Jay Heefner et. al.
The output noise of a voltage reference was measured
before and afterfiltering
by a 2-pole filter at 1 Hz. The measured output noise was higher
than the expected value by about a factor of 2. This in turn was
well above the noise floor of the dynamic signal analyzer.
Some intermittent problems are being experienced with
the 10-W laser at LLO. In particular the problem is noticed with
the frequency servo dropping out of lock -- for no apparent reason -- even
if the control from the modecleaner to the VCO is disconnected. The
symptoms are if you monitor the FAST actuator voltage every now and then
a level jump occurs. Looking at the trend data for the past 3 weeks, suggests
that the problem started between 2 to 3 weeks ago. On locking the
laser to the reference cavity, the laser would lose lock after about a
minute.
In checking out the laser, the laser frequency was
swept across the reference cavity resonance to display the discriminator
signal from the frequency servo. Ordinarily the discriminator signal
can be displayed on an oscilloscope without any problems and that any drift
in the relative position between the applied voltage ramp and the discriminator
occurs on a time scale of tens of seconds. What was observed was
a movement on the order of a second. The phase-correcting Pockels
cell in the laser was checked for correct alignment and did not appear
to be the problem. The capacitance of the FAST actuator was measured
and was consistent with the spare laser and an NPRO laser.
This morning (Wednesday) Ken Watts and Mike Fyffe
went out to check the power going to the rack because the fuse in the laser
power supply has blown a number of times in the past week or so.
One problem found is that the PSL rack is not grounded with respect to
the incoming mains power. When the rack was temporarily shorted to ground,
I found that the frequency servo could lock and everything appeared to
be normal. The rack was then allowed to drift to see if the problem
would return -- it did. Temporarily grounding the rack again appeared
to have cured the problem again but the test was interrupted.
Tests on the laser are on-going, as are comparison measurements and cross checks with the spare 10-W laser.
Errant beam baffles were installed in LHO HAM2 and
HAM8.
ITMY PO mirror was re-aligned by rotating the mirror 1.5 mrad ccw in the yaw direction, as viewed from the plan view of the IFO. This rotation of the PO mirror rotates the input to the ITMY PO telescope by 3.0 mrad, which was determined to be the correct PO beam alignment by measuring the rotation of the FMY mirror required to direct the ITMY PO beam out the center of the output viewport.
I had previously done some simulations when the recycling
cavity is only locked.Including
the arms the sideband power is basically the same and having a 3% loss
through the two internal test mass mirrors does not affect the gain much.
My personal interpretation is that the sidebands might
be so large in transverse distribution that they are basically lost after
crossing the two ITM mirrors and energy is not conserved. The effective
reflectivity of the ITM keeps on being ~97% instead of jumping to 1. The
gain of the carrier is high though as we expect since the impact of thermal
lensing is only a second order effect for it. Were the interferometer matched
the sideband gain should be roughly half the one of the carrier.
CR
SB+
SB-
61.42
7.57
7.14
CR TEM00
SB+ TEM00
SB- TEM00
61.17
2.83
2.76
With no arm: SB+
SB-
6.91
7.26
SB+ TEM00
SB- TEM00
3.03 3.13
OTF Lab. (W. Bridge)
Contamination Cavity # 1
New test sample a 10mm Capacitance position sensor (given By:
Rich Abbott)
which consist of a sma cable and a ceramic connector at the end. The
whole cabling it has been introduced
and tested. The chamber is pumping down and cavity is locked and we
are taking ring down and beat frequency every day.
Please see Dr. Zhang graphs for absorption, ring down and thermal lensing.
Absorption Test Measurement prototype in progress
Scatterometer system is in STANDBY for measurements.
We are taking more absorption measurements for the 6 inches in diameter
by ~ 3 inches thick Sapphire mirror.
We will be measuring the scattering of the this mirror. As a
result, We have made a base holder specifically for this mirror to accommodate
into the scatterometer system.
OTF Lab at Lauritsen ROOM 38
Cavity #3
This cavity has 70 ppm mirrors and hung with one end at 1.8 degree
higher that the other end.
Cavity is locked and we have 147 mw of power with a 95% ! visibility.
We are taking ring down and beat frequency every day.
Cavity #2 Test cavity STILL in STANDBY.
Optical train upgrading is in progress.
New cavity assembly is in progress for this chamber.
Misc. tasks.. placing orders to modify the scatterometer system to accommodate the new sapphire mirrors for the advance Ligo.
no report
MEPI (Myron, Ken, Rich, Dave, Bill)
We ran a sensor correction measurement cycle over the weekend and got
a
full set of data on all three directions (X,Y,Z). This was done by
locking up 7 modal loops, varying the sensor correction coefficient
and
recording the ground and witness seismometers. The transfer functions
were then calculated and the effects of varying the sensor correction
could then be evaluated. Some of the data from this run can be seen
on
the ilog for Tuesday June 3. Their resolution (in terms of sensor
correction coefficient) is limited due to the low loop gain at low
frequencies. Plots of the loop gain are also in the June 3rd ilog entry.
We reworked the control laws to get more low frequency gain and reran
the measurement; some of these data have been entered into the ilog,
on
June 5.
HEPI (Myron, Ken, Rich, Dave, Bill)
After installing the new pump and motor we remeasured the hydraulic
pressure spectrum. This spectrum along with a spectrum for the old
pump
can be found on the June 3rd ilog.
LLO EPI Installation (Ken Mason)
Bid packages have been delivered to 5 suppliers for all fabrication
and machined parts (excluding actuator) for the EPI systems to be installed
at Livingston. Three bidders have already completed quotes.
ISC TELESCOPE IMPROVEMENT (Ken Mason)
An ISC telescope has been designed with a very high stiffness, the
first mode being at 415 Hz. Also included are provisions for acoustic isolation.
Fabrication drawings are now being created for building a prototype.
Thermal Compensation Advanced LIGO (Dave)
Spent time preparing for NSF Review.
Thermal Compensation Initial LIGO (Dave, Dan Mason)
Dan Mason is coming up to speed on the CO2 laser that will be used as
the actuator.
LASTI Optics
Waseem Bakr (UROP student) has started a trade study to determine whether
it is feasible to increase the g factor of the LASTI cavities given the
expected excellent seismic isolation that LASTI will have.
SIMULATIONS AND MODELING (BHAWAL)
_______________
E2E MODELLING:
_______________
e2e weekly Physics meeting
---------------------------
Luca, Matt, Malik, Virginio, Hiro, Biplab discussed the new optical
model
code and WFS issues in hardware and e2e-model.
e2e in Japan
-------------
Dr. Hayakawa of the Institute of Cosmic Ray Research, working with
Prof.Kuroda and Prof.Ohashi, raised a question regarding the use of
e2e and
presentation of the work using e2e. Barry and Gary endorsed that e2e
is a
freeware copyrighted by LIGO/Caltech and that people/groups with a
proper
MOU/attachment exchanged with LIGO can present and publish their works
so long as they quote e2e/LIGO/Caltech properly.
New Optical Model
------------------
(Matt & Hiro) Matt revisited the new optical model code, adding
and updating
comments and writing a new test program. This has new implementation
of the
modal model for the next generation of the optics/field simulation
in e2e.
This object oriented implementation makes it easier to model
complicated
objects (mirror with wedge and thickness). Hiro received the
package and
started playing with it.
FFT modeling
------------
Hiro started (again) to prepare the mirror phasemap for the FFT
simulation to study the as-built LIGO performance using the measured
phasemap. This work will be used later for the calculation of
the mode
decomposition matrix to be used in e2e so that mirror aberration
effect
can be included in the time domain simulation.
WFS signals in presence of mode mismatch
-----------------------------------------
(Biplab) Started calculation of dynamical misalignments in presence
of
mode-mismatch using as-built parameters in order to see how the
signals
may change in a not-so-hot IFO.
Code development and maintenance
---------------------------------
(Ed Maros) Work was completed on the CVS repository for the e2e.
The
JAlfi directory has been removed and a new directory called
alfi
now appears at the same level as e2e. This allows the simulator
and the alfi editor to have different release cycles.
(Melody) Figuring out the reasons for the differences in the results
generated by the different versions of gcc in different platforms
(Linux and Sun) using different optimization levels.
Alfi
-----
(Bruce)
- Fixed copy/paste problem regarding adding of some ports (PR
404).
- Completed new port reposition interface for internal and external
movement of ports on nodes (PR 380).
- Working on Copy/Paste problems with Macro and settings not
being
copied into the new nodes properly (PRs 394 and 413).
-------------------------------------------------------------------------------
LIGO DATA ANALYSIS SYSTEM
SOFTWARE SYSTEMS (BLACKBURN)
----------------------------
The 0.7.0 Release of LDAS went out this week. It was installed onto
the
Caltech systems on Wedesday and being installed at LLO, LHO, and MIT
as
of today (Thursday). This release includes an enhanced "createRDS"
command
to support merging LLO and LHO channels into a single RDS frame. It
also
fixes the issues seen during the science run. Most of the effort over
the
past week has gone into testing and packaging up this release. It requires
a new LDCG and that LAL and LALwrapper be compiled with GCC 3.2.3 under
Redhat Linux 7.3. However, the wrapperAPI's binarys will run successfully
under Redhat 9.
We grabbed the S2 locked segments from LHO and LLO and inserted them
into the database at CIT. A Burst script is now running on CIT,
"walking" along the S2 RDS frames. It is running three burst
jobs
analyzing H1:LSC-AS_Q. There was a small problem with one of
the
ligotools (lwtprint) which the script uses. The attributes in
the XML
entities are in a different order which confused the ligotool.
Philip
fixed it temporarily for me so that The Burst script works again. Results
of these pipelines are going into the TEST database on LDAS-CIT.
Modified waveburst table in database, and added new table "sngl_block"
to support the BlockNormal search code being developed at Penn State.
Modified guild to work with the new table.
Traced the problem with using NDAS frames in stochastic searches to
an
issue in the generation of the NDAS frames. The DMT tool used to create
these frames was occasionally dropping out data. It was reported that
about one NDAS frame per day per IFO had this problem. These problematic
NDAS frames are being regenerated by the DMT group.
In order to trace the problem with the NDAS frames, the frame file utility
programs such as frverify and frdump6 had to be enhanced to isolate
the
problem and make sure it wasn't a bug in LDAS. These now provide much
more
diagnostic information than previous version.
Work continued on the porting of LDAS to the new GCC 3.3 compiler. The
Sun port continues to be a problem. We have developed simple test programs
that clearly show the problem on the sun but the same test programs
run
without fault under Redhat Linux 9. We have found GCC patches that
we
will be testing out this week. Unfortunately, every rebuild of the
GCC
compiler on our current Solaris test platform takes 7 hours. We hope
to
have faster boxes next week to increase the turnaround time as we look
for a solution to the issues of this compiler under Solaris.
HARDWARE SYSTEMS (ANDERSON)
---------------------------
Caltech
-------
(Dan Kozak)
* Got bad 9940 drive (wouldn't mount tapes) replaced.
* Provided some assistance to LHO vis a vis their bad T3 (t3-4).
* Staged NDAS data to support Szabolcs Marka's effort to find the bad
frames.
* Began re-archiving data (specifically NDAS frames) to 9940B drives.
9940A drives are now switched off. Am trying to figure
out why the first
few tapes were written with small block sizes (16k). Subsequent
tapes
are being written with the correct blocksize (256k).
* Leaned on StorageTek to clean up the mess in Powell-Booth left over
from
the silo upgrade. Finally successful (today). Am
also leaning on STK
to get correct power supplies for our two new 9940B drives.
(Al Wilson)
* Setting up systemimager for cloning of nodes at CIT, LHO, LLO.
* Setting up nodes 41-56 on the LDAS-CIT system.
* Preparing the old nodes 1-16 from LDAS-CIT for use in LDAS-DEV.
(Stuart Anderson)
* Worked with Albert and Al to install the first full rack (40 units)
of the new LDAS-CIT Beowulf nodes. Two units developed problems
during the weekend burn test. The failures where combined into
one node and sent back to ASA (power supply and memory). The
remaining
39 nodes have passed the memory stress test.
* Installed new 224-port copper GigE switch which has been successfully
used by Al to start cloning the new Beowulf nodes for LDAS-CIT.
* Started installing new Sun 280R server to replace ldas-sw.
* Identified incorrect disk drive size in recent Sun order and initiated
remedial action with Sun.
* Received notification from Shipping and Receiving that 14 pallets
of
computers from ASA have arrived at Caltech.
* Decomissioned a rack full of old 4GB drives that would not die but
where taking up too much space in Millikan.
* Transferred one dual- and one quad-processor Intel machine to General
Computing at Caltech to make room for newer LDAS servers.
MIT
---
(Keith Bayer)
* Configured Gigabit card in pcraid2 (using reiserfs).
* Moved S1 data to make room for S2 rds triple coincidence data.
* Running burn-test with RH7.3 of new 3GHz datacon/beowulf boxes.
* Electrical work on ldas lab scheduled to begin June 5/6.
Livingston
----------
(Igor Yakushin)
* Set up a test replication configuration from LHO's LHO_TEST database
and LLO:'s H_TEST_R. At first it worked fine but later H_TEST_R
completely lost replicated data. My guess, is that some kind
of overflow
happened (not enough primary logs, insufficient buffer pool
or something
like that). I increased the number and size of primary logs,
turned on
logging both for capture and apply programs and restarted replication.
* Experimenting with multipage_alloc configuration parameter of a
database. According to the documentation, turning it on should
speed up
the insertion rate.
* Got all the remaining hardware from SUN.
* Upgraded kernel on both IDE RAID boxes.
* Restored /frame21 after multiple disk failure.
* Since it turned out that currently LDAS cannot work with NDAS frames,
I generated AS_Q only RDS frames both at LHO and LLO to exchange
them
between sites.
* Wrote a perl script to set up creator_db differently for different
sites.
* Backed up the databases at MIT before LDAS upgrade.
Hanford
-------
(Greg Mendell)
* Assisting Ben Johnson with installations of the new LDAS beowulf
cluster, new L700 tape library system, new switches, and recabling
the
room to work with the new switches.
* Assisting Ben Johnson with T3 problems: t3-4 has a firmware/hardware
problem. Ben has been working with Sun to fix the problem.
* Assisting Igor Yakushin with creating and writing to tape H1H2 AS_Q
only S2 RDS frames to be sent from LHO to LLO. The reverse
will be done
for L1 AS_Q.
(Ben Johnson)
* Continuing work with Sun about t3-4. I have updated the firmware
level on u1d4 of t3-4 to revision 1204. Problems still persist...
* Configured StorEdge 3510 FC RAID with 11 disks as one RAID 5, with
one hot spare disk.
* LDAS room temperature monitor is sending data into the CDS network
for testing. It has not been fully put into the EPICS, i.e.
the
operators won't know if the room gets too hot yet.
* New beowulf and datacon boxes have passed memtest86.
DATA ANALYSIS ACTIVITIES (LAZZARINI)
------------------------------------
Greg Mendell:
1) Assisted the PULG group on the final draft of its S1 paper.
2) 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.
3) Continuing to prepare my SURF student project, which is to study
various methods of parameter estimation for continuous wave sources.
4) Found memory leaks in LALIndependentTestDetResponse.c, the
independent test of the beam pattern response functions that Malik
Rakhmanov and I are working on. The problem does not seem to
invalidate
the simple test the code currently does, but these need to be fixed
before we can expand the tests.
Philip Charlton:
The only thing I have to report this week is that I looked into Isaac
Salzman's observation that running LDAS pipelines with NDAS frames
produced slightly different results from the same pipelines using
RDS or raw data. The differences were very small (order 10^-6).
I found that the raw NDAS and RDS/raw data were identical, however the
downsampled data had a few tiny differences (order 10^-7 to 10^-6).
Downsampling of data is done on frame-sized chunks. Although the
algorithm is designed so that (as much as possible) downsampling a
long
data set in chunks should give the same result as downsampling the
entire
data set in one operation, there are necessarily some differences,
due to the slightly different ways that data must be processed when
downsampling in chunks vs a continuous data stream.
For this reason, I believe the observed differences are due to the fact
that the NDAS frame files are downsampled in 1-second chunks while
the
the RDS and raw frames are downsampled in 16-second chunks.
Peter Shawhan:
1) Worked on S1 inspiral paper
2) Organized face-to-face meeting of the inspiral group, to be held
at Caltech on June 20-22. Primary goal is to get analysis of
the
S2 data going.
Kaice Reilly:
I prepared the stochastic scripts to produced the necessary intermediate
data products. I didn't run them yet becuase of disk space logistics.
Worked
with Stuart and the group to setup a work area at Caltech for the stochastic
group and to move the stochastic cvs to Caltech (ldas-sw). Most
of my other
time has been dedicated to preparing for PAC 14. Computer problems
and getting locked out of the building have made this interesting.
Teviet Creighton:
Prepared a talk on the S1 pulsar analysis for the PAC.
-------------------------------------------------------------------------------
GENERAL COMPUTING (WALLACE)
MIT:
(Keith)
-Rebuilt Ultra 1 workstation guinevere with new harddrive
-Investigating tryplesync software package to sync with
calcium calendar service
-General support for summer students
Livingston:
(Shannon)
-Added three hard drives to the GC File server. Spent most of
Tuesday
working with Sun tech support on an issue with the Solaris Management
Center. This software has been causing problems on both NIS+
tables and
Logical Volume Management. Installed the recommended patch cluster
to
the file server on Monday. Sun had me roll back one of the patches
as a
result of the call support call. The issues are still unresolved.
-Pricing various options for a new backup system. I am considering
a
RAID similar to what LDAS has for backups. This would be periodically
backed up to tape. We have significantly outgrown our tape library
for
backups. I am also considering different software options that
would
allow me to use the RAID instead of the library for daily/weekly backups.
-Set up a new computer for Allen. His old computer will be wiped
and
given to one of the summer students.
-Working with ASA on a computer that has been having problems.
This is
the second time the computer has been back for service.
-Still working with Bonnie to restore most of her software. It
had been
upgraded from Windows 98 to Windows 2000 a while back and it just
finally died. She lost some e-mail when it did die, however most
of her
files are intact.
-Setting up computers for the SURF students and teachers today and
tomorrow.
-Worked on a couple configuration issues on some of the Sun servers.
Turning of various services and ssh configurations, etc.
-Planning on how to upgrade the web server/ilog files, since the order
has gone through for the hardware. I am beginning to think that
perhaps
the ilog server should be a separate server. Also, the database
functions on the web server should be moved to a separate machine.
The
web server upgrade will probably take several days to a week to do
everything I believe should be done.
Hanford:
(Christine)
- Writing the PR to buy the GigE network equipment.
- Started setting up the new Cisco router.
- Various user support.
CIT:
(Lisa)
- An incredibly large pile of spam blocks
- Did monthly's and root dumps of all servers
- Did a couple of small scripts for users
- Went to a Sun seminar on core dump analysis
- Worked on an ntp sync problem for the 40meter
(Mike)
-Worked on loading two PC's for up coming surf students.
-Worked on loading a laptop for the loaner pool.
-The Scanner up on the 3rd floor went out. After troubleshooting it
I ended
up replacing this with a backup scanner we had in storage.
-Finished up loading Pro/Engineer for Calum. This installation took
many
hours due to loading this software on win 2000.
-Ran end of the month ghost backups on all NTSRV's.
-Called in a laptop to Dell tech support.
-Backed up Lori Robison's computer by getting a ghost image of her
workstation. Then I set this computer up for a visitor that is going
to
work from this computer.
-Loading a laptop with an OS for testing for a Dell technician to test
with
after he replaces parts.
-Larry and I setup SCR for the PAC meeting that included setting up
additional network connections and rearranging furniture to allow adequate
seating.
-Worked on Ken Mailand's computer due to some OS problems and installed
zone alarm.
(Veronica)
- LIGO website: worked with George Stokes on troubleshooting of the
DCC
databases. Helped him understand the d/b architecture and the workflow.
Provided support files and information. Working with him on possible
immediate and long-term solutions.
Worked with Larry on DVD burning issues. Contacting Caltech Digital
Media
Ctr for help in converting a set of files to a format suitable for
our
software, in response to Phil's request for a backup copy of a DVD.
Posted several updates to various parts of the LIGO website.
- CaJAGWR website: user support. Updated the website in several places.
Vote count for the Executive Committee elections.
- Project Science: user support.
- LSC website: posted a stray talk from the last LSC meeting.
(Larry)
-Went through a number of purchases. Most were minor items for various
people
and LDAS. Started going through where things are at financially this
year on the
GC budget.
Discussing the pros & cons people have had with the IDE raid systems.
We need
more disc space and just checking on the best way to get it now that
we have a
few more options.
-Worked with a number of users going over their setups, adding and
modifying
their accounts. We've spent a great deal of time going over logistical
issues to
get a computer up and going for all of the summer visitors and SURF
students.
With the surplus units coming in from LDAS we should have enough equipment
for
everyone.
-In between all of the distractions for user needs and going over different
issues for the PAC and NSF meetings, I have been able to start working
on the
Livingston GC audit report. So far it appears that most of the problem
items
were already identified and being worked on.
-Worked on the server room. It looks like the air-conditioning will
not handle
any more equipment, I plan on talking to the PMA group to see what
some of our
options may be.
From: ctorrie <ctorrie@ligo.caltech.edu>
Mode Cleaner
Several attempts have been made to damp all
of the degrees of freedom in the new mode cleaner suspension. Shake down
of the electronics by Jay Heefner revealed
that everything was working. I am currently working on testing the different
degrees of freedom one at a time.
The current situation is that I believe the pitch, vertical and transverse
modes can be excited and damped within 10 seconds. More work is required.
2 of the OSEMs which were accepted that
did not meet the specifications, in E030084-00-D
are back with Bob Taylor. More OSEMS are expected to arrive
from
Eddy Current Damping
I have created drawings of the various light weight arrays that we plan
to test on a single pendulum. This will allow us determine if this new
design could be incorporated on an upper mass like the one proposed fro
the ETM.
Blades
Mike Plissi and I have been gathering
information and previous experimental work done here at Caltech on cantilever
blades. We hope to have several technical notes finished by later this
week and posted on the DCC.
Visit
10 girls and 3 members of staff from
From: JaneenRomie
<romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Preparing for the NSF Review.
Local control hybrid osems are installed
on a MC triple suspension in the Synchrotron. As Mark is on vacation, Jay
and Calum are working on tweeking
thedSPACE system
to damp the suspension.
CES is manufacturing some tablecloth brackets that will allow for more
vertical adjustment of the upper mass, and therefore, the test mass. They
are also working on a prototype of a low-mass eddy current magnet holder.
Calum and I worked on comparing the cost
estimates for the triple suspensions.
In the weekly suspension meeting, we discussed the suspension schedule.
We will continue that talk next week.
From: Helena Armandula
<ahelena@ligo.caltech.edu>
Advanced LIGO Coatings
The RFP for the coating development work was FEDEXed to the vendors today, Wednesday!
Greg
- X-rayed samples. Still Noisy.
- Talked to Bill about ways to filter out Fe fluoresence
from x-ray
spectra. 25-40 micron Cr filter should help.
- Designed new mold to be made which better fits ideal Q-factor
measurement dimensions.
Enrico
I finished the code for calculating inspiral NS range with the system
of
the 2 IFOs together but I'm trying to
solve a bug I found for heavy masses.
I did some test with different last stage lengths.
I started looking at Kenji's work on thermal noise and Youichi's
work on blades.
Youichi
Compared the results of my MGAS design program with the Virginio's
paper. The results almost agree with the paper, but I found a
small
discrepancy. Trying to figure out the reason.
Tested wire clamp pins. Found that they hold only a little load. Will
test pins with bigger bulge.
For additional information about this report, contact sanders@ligo.caltech.edu