Weekly Report for
Week Ending November 10, 2005
The LIGO Executive
Committee Agenda for Monday November
14, 2005 will be:
(Meeting time: 10:30 am Pacific Time)
1. Announcements
2. Comments
on Weekly Report
3. LSC
Issues (Saulson)
4. LIGO
Lab Operations
- Administration
(Lindquist)
- Sites
(Raab, Zucker,
Shoemaker)
- Commissioning
(Fritschel), Detector (Coyne)
- Campus
Research Facilities
- 40
Meter (Weinstein)
- TN,
( Libbrecht)
- LASTI (Shoemaker)
- Data
Analysis and Computing (Lazzarini)
5. R&D
and Advanced LIGO (Shoemaker)
6. CHANGE CONTROL BOARD/TECHNICAL REVIEW BOARD SESSION AS
NEEDED
Special Announcements:
The NSF conducted a review of the LIGO Project, November 9 – 11,
2005. Following are notes from the exit
debriefing:
- The
panel indicated that they were impressed with progress made over the last
two years.
- The
panel will report that the interferometers have been operated in
coincidence for extended periods of time and that we have met the
milestone of operating at the levels identified in the science
requirements document, although LIGO should continue to improve
sensitivity (balanced with running) especially at lower frequencies.
- The
panel will report that LIGO is ready for data archiving and processing,
although the panel also noted that the data volume will grow during S5 and
additional resources will be required.
- The
panel will report that the data analysis tools are working. The panel also suggested that LIGO
should become more active in astrophysics conferences to let that
community know that interesting physics is being done.
Advanced LIGO
- Test
mass down selection has been done.
- The
panel no longer considers the coatings to be a “show stopper, “ although additional research and development is
warranted.
LSC
- The
panel will report an active and effective program.
Two Year Extension
- The
budgeted amounts proposed seem reasonable and the panel will recommend
that the request for a two year extension be approved by the NSF. The panel also noted that there needs to
be a strong coupling between Advanced LIGO funding and Operations.
- The
panel noted good things about the CIT and MIT commitment to LIGO, and they
approved of the changes in organization involving the LSC.
Weekly
Report Highlights
No report.
LIGO Laboratory Administration (Lindquist)
STATUS OF LSC MOUs (Lloyd)
LSC MOUs and Research Plans and Progress Reports
- Nothing
of significance to report.
Non-LSC MOUs (Lloyd)
SITE TELECONFERENCE (Lindquist)
No site teleconference was scheduled for Thursday, November 10, 2005 due to
the NSF Review.
- The
list of assigned actions updated through November 3, 2005 (the last time
that it was updated) will be found Here.
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>
- Prepared
notebooks and contents for NSF Review.
General DCC operations
>From: Cleveland Mak mak_c@ligo.caltech.edu
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Week Ending
November 10, 2005
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In
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Out
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Packages
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35
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5
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Faxes
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22
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16
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- Working on updating list of copy/fax machines on
the maintenance agreement contract.
Also updating toner inventory for these machines.
- Working
on determining the number of 2006 personnel directories needed for the
entire project including MIT, LHO, & LLO.
- Update
on Scanning Project - Progress continues on Larry Jones' boxes of
files. To date, we have 11 of the
16 boxes scanned. We anticipate
completion of these set of boxes possibly by the end of next week.
COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman)
>
>From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
- The
MIT change order was returned with approvals. It has been distributed.
- Completed
change orders #165 and 166 to Triad and submitted to the vendor.
- In
the process of completing the change order to Galli
and Morelli.
- Working
on the change order to Support Services for approval.
>From: Florence Kaufman <fkaufman>
SUBCONTRACTS MANAGEMENT (Jasnow, Salone)
>From: Gina Salone <gsalone@ligo.caltech.edu>
- Nothing
significant to report.
>From: Ed Jasnow <jasnow@ligo.caltech.edu>
SUPPORT (Baldon, Hiroto, Lloyd)
>Irene Baldon
No report.
>
No report.
>Dorothy Lloyd
- Nothing
of significance to report.
- Jim
continued with data entry in the LIGO database and helping out in the DCC.
CHANGE CONTROL/CONTINGENCY MANAGEMENT (Lindquist)
HUMAN RESOURCES (Akutagawa)
>From: Cindy Akutagawa <cindy@ligo.caltech.edu>
- The next Staffing Committee meeting is scheduled
for Monday, November 28. All files
for the Staffing Committee are up-to-date and posted on the SC web page.
Quality/Safety (Tyler)
>From: Bill Tyler tyler@ligo.caltech.edu
No report.
LIGO Hanford
Observatory (LHO) and Interferometer Operations (Raab)
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled by M. Landry)
At the outset of the S5 run, we decided to devote
afternoons and evenings to work on the 4k, and early morning hours to science-mode
running on a best effort basis on both machines. After dealing with AS_I
saturations in full power-up mode, the 4k was made to lock in excess of 10Mpc,
mid-week. Calibration data has been taken and some systematics
are being sorted. A partial suite of PEM
injections was made on both instruments. Periodically we have been beset
by high microseism, on the order of 1um/s.
A few salient links from the elog
this week include:
- see
the many H1 entries regarding the return to full locking, including summaries
such as this one
- last
week it was found that 4k RFAM glitches were on the distribution, so that
box was removed
- the
DARM unity gain has been set
to 200Hz
- 1Hz
lines and subharmonics are still
observed in the H1 control signal
- the
main modulation depth on the 2k IFO was reduced
by 3dB
Outreach (D. Ingram)
On our Event
Highlights page you will find news of Venga a Ver las Estrellas and
Corey Gray's recent talk at the Treaty 7
Education Conference. LHO's Local Educator
Network met on 10/27 to give outreach consultation and advice. LHO was
represented at the 11/5 MESA student conference in Sunnyside, WA and at the
Tri-Cities Visitor & Convention Bureau's annual meeting and trade show on
11/3.
LIGO Livingston
Observatory (LLO) and Interferometer Operations (Zucker)
There is still a fairly long IFO and CDS punch list but we're gaining on
it. Hardware configuration is frozen
solid and the last code update is done. Planning to hit the ground running and
join S5 Monday as scheduled.
The Louisiana
housing situation remains problematic. We have had occasional "hits"
with hotels by casting a very wide net, but it remains spotty and most will not
guarantee reservations. LLO has very limited housing, and will try to accommodate
specific requests in our trailer and rental room. Detector commissioning
support will continue to take priority over scimons
until there is nothing left broken.
Also, we cannot reserve "blocks" or tentative dates. Travelers
should supply exact arrival and departure info; we'll do our best to help, but
it is YOUR RESPONSIBILITY to insure you have a place to sleep.
Please email Bonnie and cc: Mike and Joe about housing or other logistics.
We have dropped the site speed limit to 10 mph to reduce momentum transfer
from trucks taking the curves on two wheels. Please observe this speed limit
and set a good example irrespective of your vehicle's
mass.
Science Education
Center construction has taken off with
a vengeance, now that our contractor has located a supply of dirt that isn't
earmarked for rebuilding New Orleans
levies. Fill and compaction should finish this week; boring and concrete forms
scheduled for next week (just in time for the run start).
L1 Interferometer (Frolov)
The laser arrived from the Caltech 40 meter lab on Monday. After the laser
swap the available power into the interferometer was increased to 7 W. The
interferometer optimization at the higher power is under way. The main
commissioning effort at the moment is to reduce the noise from the
back-scattering which is suspected to be one of the noise limiting sources.
Commissioning activities this week:
- the contribution of the TCS laser intensity noise to
the darm spectrum was measured. It was found
that the margin for this noise is at least a factor of ten. Other TCS work included installing the
new annulus mask and replacing the RF drive cable.
- the additional filtering of optical lever noise removed
the TCS chiller line at 259 Hz from the spectrum.
- investigation of the 45 Hz harmonics resolved in
replacing the MMT3 optical lever. The lines have not been observed in the darm noise after the replacement.
- the super polished REO mirrors were installed on dark
port optical path as part of the back-scattering noise mitigation. In
addition the beam dumping was revisited on all optical benches.
- the
beam splitter de-whitenning electronics was
modified to eliminate the transient during switching to low noise mode
- the
dust cover for the anti-symmetric port optical path was installed
- the RF preamplifier card was installed in one of the
anti-symmetric port photo-detector chains. The power line harmonic at the
180 Hz was significantly reduced by re-distributing the electronics gain.
- the glass window was removed from the ISS photo-detector
and tested for transmitted light distortion.
Computing and Network Security (Roddy)
Shannon is at CIT supporting the NSF review
CDS Code Support (Khan)
Porting the piezojena interface
software to VxWorks operating system environment.
We have a vxWorks mv162 in the PSL area that has a
serial port available, and I think it is easier to hookup the pzjena system to the vxWorks
system than bringing in a Linux PC system to the PSL.
Also working on an EPICS serial port device driver
interface for NewFocus pico
motor controller. With this device driver we can
specify only a database to interface with the pico
motors.
Site Safety and Security (Riesen)
- The
traffic sign w/flasher has been installed at the site guard gate.
- Ordered
Janeen Romie's
prescription laser eye ware.
- Gave
Lisa Szechter (out reach) the site safety indoctrination.
- Completed
an in depth inventory of all clean room garb and cleaning material. Ordered items in short supply.
- The
site security gates have been rescheduled to remain closed starting Monday
11-14-05 for the S-5 run. The
building's exterior doors will remain on the current schedule of 6am thru
6pm.
- The
site security gates (main and side) have been realigned and adjusted. This should end the intermittent partial
opening & closing problem.
- The
new LSS software has been delivered.
Installation is TBD.
- I
found no laser/site safety concerns this reporting period.
AdL SUS/SE Mechanical Engineering (Spjeld)
Quad SUS Installation Fixtures
- completed assembly drawings for transport table and
lift table - meeting with Calum and Ken Mailand on 8/11†to discuss†Ken's
alternative design to airbearing, genie
interface, etc.
- currently
looking over drawings from Ken on his new design for X-Y positioning table
- attempting to upload models and drawings onto the vault again after
instructions from Calum
LDAS/Condor and data analysis (Yakushin):
I was on vacation from Nov 1 to Nov 7, so not much to report
Storage/Condor/LDAS admin:
Nodes 87-94, that are on the same power strip (and circuit), went down
yesterday night. Resetting the breaker on the power strip fixed the problem.
Most likely it is time to replace the power strip.
Data analysis:
Working on S5 waveburst online
scripts.
LDAS admin (Giardina)
- replaced
disks in nodes 111, 113, 139, 166 and 209
- LDAS
was shutdown for 4 or 5 hours on Wednesday due to transformer upgrade
- troubleshooting errors
with my cmonClient install, tclglobus is
the culprit. can
still connect via password auth.
Initial LIGO Detector Science & Engineering (Coyne)
CDS
see also the CDS weekly meeting minutes in the commissioning archives
CDS Software
Rolf Bork
Recieved a HEPI code change request from LLO. This change involves
adding two more filter modules per chamber, which connect the STS-X/Y signals
to RX/RY filters. This code change involves epics, all Hepi
front ends, and renumbering of HEPI excitation channels (ran out of numbers as
number of Hepi filter modules/chamber now > 100).
The changes are complete and scheduled for installation at LLO Tuesday, 11/8.
CDS Hardware
Ben Abbott
Fast Shutter: Completed reliability tests. I have sent out all of the fast
shutters to the sites with associated paperwork. ISS PDs: Four of
the five ISS PDs had been sent out to the sites last
week. The remaining one had a cracked photodiode, so I swapped it out for
a good one that Todd found. The remaining ISS PD has been tested and shipped to
Hanford.
DMT
No report.
40 Meter Interferometer (Weinstein)
IFO commissioning
- Mike
Zucker called on Friday and said that LLO needed
our Lightwave 10 watt MOPA laser, as their laser
was dying. On Saturday morning, Osamu and Steve disconnected the laser and
packed it up in an old crate we had lying around (the Lightwave
box was nowhere to be found). Bob drove the box to Fedex,
but they wouldn't take it, so Mike lined up UPS drivers to drive it all
the way to LLO. It arrived on Monday morning and was immediately pressed
into service. L1 was back to 10.5 Mpc by the end
of Monday.
- Rick
Savage offered to send us the old H2 MOPA laser as a replacement. Hopefully
they will be able to swap out the noisy NPRO for a newer-style 500 mW model. He
and Doug are checking it out and plan to ship it down to us by Thursday of
next week, so we should have it the following Mon or Tues. Thanks, Rick!
- It
will take some time to integrate the new laser into our PSL. In our old laser, the phase-correcting Pockels cell was internal to the MOPA box. We will now
install one external to the MOPA box, as they do at the sites. We will
also take this opportunity to install a new pickoff mirror which will send
more light to the ISS photodiodes.
We are debating whether to install the table-top FSS; probably we
will (at long last). We will NOT
move the FSS pickoff (it will remain after the PMC but before the Mach-Zehnder). Steve
will clean out the cooling water lines.
We'll want to do a temperature scan to maximize the power. We'll then do a beam scan, mode match
into the PMC, and measure the beam power everywhere.
- Osamu
is working on the seismic noise paper with David Blair, and has begun
writing the 40m lock acquisition and optical spring paper.
- Monica
and Dan began to take some single arm transfer functions as a first step
towards a calibrated noise spectrum, but their work was interrupted when
the laser was shipped out.
- Rob
is making major structural changes to the length sensing code in the front
end cpu. He's getting
input from Osamu on the changes he'd like to see. He's adding new features
such as ramping of gains and other signals. He's including lots of
comments and will prepare full documentation.
IFO modeling
- Monica continues to
develop and debug her AdLIGO e2e simulation with
the dual recycling cavity, with lots of help from Hiro.
Looking to get results by end of week, do some validation checks,
and then plan to look at the optical spring.
DC detection development
- Ben
has been designing the in-vac DC PD electronics.
A prototype board run will be sent out tomorrow. He's also looking for
appropriate DC PDs, working on the mechanical
support for the PDs, and the satellite amplifier
that will be needed just outside the vacuum chamber.
- Mike
Smith continues to acquire parts for the output mode matching telescope
and output mode cleaner. An alignment target was designed and a purchase
order let to ASCO.
- Steve
and Liyuan tested the new HR supermirror
from Newport.
The transmission was 600 ppm, at 0 and 5degrees
incidence. now we have two low-transmittance
mirrors for our output mode cleaner.
Electronics, controls
- Our
framebuilder RAID disk array filled up over the
weekend (due to a large number of extra channels that were added to full
and trend frames). Alex reconfigured to store only 40 hours of full frames
instead of 48, and restarted it.
- Meanwhile,
our RAID disk array is dying, so we got a spare from John Zweizig, and also put in an order for a new array,
with 3 times the capacity.
- Dan
is building a Rai Weiss low-noise preamp box to
have around the lab.
- Dan
continues to work on suspension diagonalization.
Much of this work can proceed without the laser. But the laser is needed for
diagonalization of the mode cleaner suspended
optics.
- Steve
is measuring the mechanical resonances of the PMC using his phonograph
needle apparatus. Will have some results by next week.
Lab Infrastructure
- Steve transferred the
loads of the ITMY and ETMY stacks from STACIS to jackscrews. Go-no go
gauge was used. Sensor voltages changed less than 100mV. Now all
STACIS isolators are bypassed and seismic stacks are sitting directly on
the floor.
Thermal Noise Interferometer (Black)
In the past few weeks, we have been trying to
find out the reason our arm cavities have such poor visibility. The best visibility we have been able to get
in the past was 70 percent, and that was keeping our ultimate, shot-noise
limited sensitivity at about 2 x 10-19 m/rtHz. This noise floor was good enough for us to
measure coating thermal noise below 10kHz, but it was
more than an order of magnitude above where it should have been.
Careful measurements by Matt and Akira
revealed that one of the lenses in the mode-matching optics, between the mode
cleaner and the beamsplitter had its focal length
mislabeled. This produced a final waist that was about three inches away from
where it should have been, close enough for the beam to couple into the arm
cavities at 70 percent visibility, but not close enough to do any better.
Matt and Akira have corrected the mode
matching and verified it using a beam scanner.
Many thanks to Steve Vass for loaning us the 40-meter's beam scanner!
LASTI (Ottaway)
No report.
Data Analysis and Computing (Lazzarini)
Data Analysis Activities (Anderson)
(Chatterji)
I made a number of improvements to the "X" Pipeline coherent burst
search code. It now gracefully handles
more than three detectors, it includes a Bayesian
formulation of the problem proposed by M.
Tinto, and it thresholds on significance and write triggers. The pipeline was then applied to both white
noise data as well as S4 data (with H2 masquerading as V1) to produce a rich
set of triggers for further study. A
preliminary study of the results confirms that the algorithm is working as
expected.
I did some research on submitting jobs via globus
and can now successfully run analysis jobs on the Pleiades cluster at Penn State. I have also successfully used the Condor
schedulers on the LIGO Laboratory clusters to manage the submission of globus jobs to the Pleiades cluster. I am looking into a simple interface that can
be used to launch X Pipeline and Q Pipeline analysis jobs at all LSC and LIGO
Laboratory computing clusters.
I am working on getting an on-line version of the Q Pipeline running under
the Onasys system for S5.
(Sutton)
I re-submitted the LIGO-TAMA bursts paper to PRD after revising in light of
comments from the reviewer and the burst review committee. It has since been accepted for
publication. I've derived the
uncertainty principle(s) for the LIGO cheese (space of GWBs),
and I'm editing the cheese paper. I've
also been testing and editing Maria Principe's Network Simulator files. We'd like to get the simulator package
functional and demonstrate it at GWDAW.
(Shawhan)
- Completed
a major reorganization of LIGOtools software
packages.
- Assembled
a technical document describing the S4 LIGO-only untriggered
burst search, with contributions from several other people.
- Worked
on organizing reviewing of burst analyses in preparation for the LSC
Meeting and GWDAW.
- Attended
a workshop, "Probing the distant universe with gravitational
waves", at East
Tennessee State
University.
- Diagnosed
hardware signal injection problems observed during the first several days
of the S5 run (with Vuk Mandic).
(Yakushin)
- Working
on S5 waveburst online scripts.
(Mendell)
- S5
SFT generation from uncalibrated DARM_ERR is
running under onasys at LHO. This will switch to calibrated SFTs generated from h(t), as
that becomes available.
- Review
of the StackSlide code continues, and some
results for the LSC meeting next week will be generated, though the LSC
clusters are heavily loaded right now.
Simulation and Modeling (Bhawal)
Simulation of 40m Advanced interferometer
(Monica) Debugging of the e2e 40m package with the dual_sum
module is done. Validation of this new package with Twiddle results will be performed
soon. In the meanwhile, the simulated 40m IFO has been locked at the operating
point: no offset appears for the IFO central part while DARM and CARM have some
offset. The optical spring effect will be verified under this condition.
Modeler
(Melody) Worked on properly handling an interrupt signal
(CTRL-C) when the shared object (libe2e.so) is being created.
Alfi
(Bruce)
- Completed
new more user friendly parser error handling (related to PR 476).
- Implementing
new data object to track changes in bundler I/O names in inherited
bundlers (PR 511).
(Melody) Testing the newest release of JGo
(5.14) on the Mac. Working on PR 296 - easier access
to settings.
LDAS Software Systems (Blackburn)
LDAS:
- Started
work to enhance the performance of the diskcacheAPI
(pr2753). After doing a code read, one area has been identified as a
potential candidate.
- Currently
a test program is being developed to measure the performance of the diskcacheAPI so modifications to the code base may be
verified to achieve performance goals.
- Upgraded
the MIT compute facility to the latest version of LDAS (1.8.0) and
installed a newer version of DB2 as well. MIT is now up and running.
- Put
in new package cmonGlobusChannel to support tclglobus channels associated with PR 2951.
- Put
in fixes for PR 2281 - start ddd/gdb from server
side. Fixed PR2950 - cmonClient fails to authenicate when running as user ldas.
- Removed
code to check ::DEBUG_DEFUNCT_JOB_REAPER resource
var but always log when cleaning defunctjob as a blue ball in the frameAPI.
- Testing:
Monitoring LDAS-Dev disk usage while run loops script tests suite to try
and understand the source of disk space leaks.
TCLGLOBUS:
- Completed
and tested blocking XIO read/write implementation of Tcl
channel. Will work with Mary to
test this XIO channel within LDAS.
- Completed
15 out of 77 Globus FTP control functions and
the functions are to be used to write GridFTP
client/server program from scratch.
GRIPHYN/IVDGL/OSG:
Prepared a presentation to the NSF review committee the
Grid computing activities of LIGO and the LSC focusing on the current
involvement with the Open Science Grid.
Began upgrading the LIGO/Caltech OSG Integration Testbed Cluster from its current configuation
of Fedora Core 3 and OSG 0.2.1 to Fedora Core 4 and the recently announced OSG
0.3.0. There is an option of installing this OSG release with or without
Web Services. We will be installing and testing the version without Web
Services. So far 5 nodes of the 8 have been upgraded to FC4.
Super Computing 2005 began this week. LIGO is submitting jobs to the OSG
production sites that support our VO, but we are finding that we fall into the
queue and are not seeing a lot of jobs actually running. This has been reported
by other VOs to the various OSG lists managing the
SC05 demos. The LIGO jobs are only test jobs on playground data since issues
with Pegasis and the transfer of data remained
unresolved at the start of the SC05 and make running the much larger DAGs on science data very difficult give the network
bandwidth and disk space issues at OSG sites available to LIGO.
LDAS System Administration (Anderson)
Caltech
(Dan Kozak)
- Started
S5 at LHO (got archiving/LDR running).
- Had
STK replace tape drive 57 at CIT (was failing, but not being marked down).
- Repacked
more (L0.2) tapes at LHO.
- Did
more work on the "eject tapes at the sites" script.
- Ejected
A4/S5 tapes at LHO and had them shipped.
- Imported
them and started to verify them at CIT (ongoing).
- Fine
tuned archiving at LHO (spent a _lot_ of time on this one, but I think
it's working well now).
- Verified
that /archive/home was going to tape at LHO/LLO/CIT.
- Updated
the lag plot for S5 (still a few tweaks I want to do to make it easier to
modify/maintain).
- Helped
with LLO shutdown (mostly wrote up stop/start routines).
- Did
samfsck on CIT export-dev and recovered lots of
disk space.
(Phil Ehrens)
- Modified
the security model on the apache/svn
installation on dziban to allow admins to edit pages on the wiki
on that server using
only a password while maintaining full certificate auth
protocol for svn.
- Tested
apache/svn and Tcl-Globus
with all certs located in /etc/grid-security and
with the trusted ca bundle linked into /etc/grid-security. Tcl-Globus will need modification to support this
model, which remedies a security issue raised by the current implementation.
- Began
rewriting gpstime.tcl module of LDAS genericAPI to be make it more
robust through new leapsecond transitions.
- Issued
various service certs and added users to the
grid resource files.
- Disposed
of 9 PC and Sun computers that were past useful life or broken.
- Set
up conference room for NFS review.
(Erik Espinoza)
- Configured
Areca RAID Controller w/ FC4.
- Investigating
NFS Issues w/ latest testing kernel.
- Examined
pricing for Opteron 175 Configuration.
- Tested
3ware 9500 RAID rebuilding via web interface.
- Tested
3ware 9550 RAID, crashed upon removal of the disk.
- Spoke
with Appro about RAID + IPMI possibility.
- Investigated
IPMI issues with support@supermicro.com.
- Tested
new USB sticks for booting compatibility.
(Stuart Anderson)
- Testing
cluster evaluation units.
- Helped
with MIT LDAS/OS upgrade.
- Monitoring
dataflow S5 status.
- NSF
review.
MIT
(Keith Bayer)
- finished FC4 and Solaris 10 upgrade.
- LDAS
is now running.
- LDR
is now running.
- Trouble
with condor is being looked into.
- 280R
hardware trouble dealt with motherboard and graphics card replaced.
(Junwei Cao)
- LDR
configuration for S5 data transfer to MIT.
- Setup
S5 data transfer monitoring at MIT (e.g. emails, websites, cron jobs, ...)
Livingston
(Igor Yakushin)
- Nodes
87-94, that are on the same power strip (and circuit), went down yesterday
night. Resetting the breaker on the power strip fixed the problem. Most likely it is time to replace the
power strip.
(Dwayne Giardina)
- Replaced
disks in nodes 111, 113, 139, 166 and 209.
- LDAS
was shutdown for 4 or 5 hours on Wednesday due to transformer upgrade.
- Troubleshooting
errors with my cmonClient install, tclglobus is the culprit, can still connect
via password auth.
Hanford
(Greg Mendell)
- S5
RDS generation has been running flawlessly since the start of the run,
modulo a few minor changes in the Level 1 RDS channel lists. The current list (with downsample factors in the second row) is posted here:
http://ldas.ligo-wa.caltech.edu/ldas_outgoing/createrds/dsorun/contrib/createrds/S5_L1/adcdecimate_H-RDS_R_L1-S5.txt
- S4
Level 4 RDS frames were generated at CIT during the past week. These are now available for use.
(Ben Johnson)
- L0
and /frames publishing now up and running at LLO. The SEGNUM channel is
still not in the LLO frames (as of 11:20 PST Nov 10). LLO is waiting for Dave Barker to return
from CIT to reconcile the LLO/LHO channels.
- The
createRDS configuration parameters were tweaked
at LHO to leave the A4 data out of segment calculations. This has reduced
the segment calculation part of creatRDS from
5-7 minues to 5-7 seconds. Also reducing the load on gateway
significantly (though createRDS was niced +19), and reducing RDS creation latency by ~5
minutes.
- Continuing
to work with LHO cluster users with Condor/onasys/node
misconfigutation issues.
- Several gaps in fb1 data have appeared this week,
due to fb1 reboots. Fortunately, the gaps were filled in from fb0 data.
Advanced LIGO and Supporting R&D (Shoemaker)
Advanced LIGO Systems, Management
No report this week, except that the NSF review went very well indeed. Thanks to all who helped, at the moment and
over the year(s), to make it happen.
Seismic Isolation
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Assembly
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Status
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Top Assembly Components
20007970-A
Stage 0 Assembly
2000795-A
Stage 1 Assembly
20007825-A
Stage 2 Assembly
20007825-A
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Purchase order placed with Arland Tool for all large parts. All material has been recieved. Project currently in Engineering for CNC
programming. Amendment made to purchase order to change mounting holes on
optics table from 2 x 2 to 1 x 1 hole pattern.
Purchase order placed with Limerick Machine for the end milled plates and
remaining Top Assy, Stage 0,1,
and 2 Componants.
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Stage 0-1 Spring Assembly
20007878-A
Stage 1-2 Spring Assembly
20007890
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Fabrication drawings are
complete. Drawings must now be checked.
RFQ for blades and rod flexures complete. Quotes due 11/22.
RFQ for remaining spring assembly parts complete. Quote due 11/22.
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GS-13 Pod Assembly
20007810-A
L-4C Pod Assembly
20007820-A
STS-2 Pod assembly
20007941-A
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Geophones, seismometers and lockers are in house.
Purchase order placed with Norcal for vacuum
housings.
RFQ complete for machined components. Quotes due 11/16
Design of harnesses completed. RFQ required for internal pod harnesses.
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Stage 0-1 Kinematic Lock
20007941-1-A
Stage 1-2 Kinematic Lock
20007941-2-A
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Tooling design complete.
Purchase order placed with Limerick Machine for kinematic
Lock Assemblies.
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Stage 0-1 Actuator Assy.'s
20007966-A
20007967-A
Stage 1-2
Actuator Assy.'s
20007968-A
20007969-A
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Tooling design complete.
Purchase order placed with Limerick Machine for actuator mounts and tooling.
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Stage 0-1 Standoff Pin
Stage 0-2 Alignment
Tower and Washer
Stage 2 Keel Plate Alignment
Tower
Blade Pre-Load Tooling
Blade Calibration Fixture Modifications
LASTI Test Stand and Spreader Bar
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Solidworks part files exist for
the standoff pin and alignment towers. They will require a dimensioned
drawing and checking prior to soliciting bids.
The blade pre-load tooling and calibration fixture tooling will require
redesign following the redesign of the blade springs by ASI.
Purchase order for test stand issued to Southern Enterprises. Joe Hanson will
be visiting Southern Enterprises on 11/11 to pre-assemble and inspect the
test stand. Delivery to MIT by 11/18.
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From: Joe Giaime
Agenda for the weekly SEI
telecom
Friday, Nov 11, 2pm Eastern,
1pm Central, 11am Pacific time
Announcements
- Dump
truck deliveries and soil compaction underway at LLO for the new Science Education Center.
High-disturbance HEPI tests underway.
- Science
run 5 begins Monday at LLO.
Comments on the NSF review
(Dennis, Carol, David, Brian?)
- NSF review close-out
report seemed very positive. They anticipate we may
need more compute cycles for data analysis. They declared
that LIGO is at design sensitivity. They recommended that initial
LIGO improvements can be considered and balanced against Adv LIGO
work. In particular, they pointed out that the sub-100 Hz noise might be
improved. No specific recommendations on the seismic subsystem.
Special presentation by Shyang
- see slides in previous log entry.
(Or get the slides from the DCC after they are transfered:
LIGO-G050588-00-L)
- In
the initial HEPI incarnation, there is still a lot of vibration at the 1.2
and 2.1 Hz BSC stack modes. Shyang has put
resonant gain features in the geophone path and resonant notches in the displacement
sensor path for the x and y modal servos for the BSC tanks, thereby
reducing test mass motion by a factor of about 4, which is quite
impressive.
pressing issues in the labs?
-MIT
-Stanford (computer)
- Rich
has been playing with the FIR model simulink
program.
- We
failed to discuss Rich's log
entry, so we should so so next Friday.
- The
ETF dSpace host computer is broken. Data
recovery underway. dSpace
'experiment' files OK.
Suspension
From: Janeen Romie romie_j@ligo.caltech.edu
Nothing significant to report.
From: Ken Mailand kmailand@ligo.caltech.edu
I have finished a preliminary SUS installation plate style fixture layout
for Calum,
this is an alternate to the air bearing and can be used either with the chamber
lazy susan setup, or the genie lift. We talked with Oddvar
re. the air bearing design, and the plate style
fixture, at that time he thought plate style had all the required
movements. The plate fixture matches the
air bearing assembly in the way it attaches to the rest of the assembly.
I’m working on a vertex BSC layout for Mike Smith that will show stay
clear areas inside for the beam path.
From: Jay Heefner
<jay@ligo.caltech.edu>
AdL SUS and SEI controls
- The
Anti-Image and Anti-Alias boards needed for the quad controls have been
stuffed and are being assembled into chassis for test. They should be
ready by next week.
- The
Myrinet nic cards,
switch and fibers needed for LASTI have been ordered and are due by 12/1.
- Racks
and power supplies for LASTI are being shipped from LLO.
- Jay
and Alex will be at MIT next week to discuss equipment locations,
installation plans and to assess what additional upgrades to the LASTI
infrastructure may be needed.
- Wiring
diagrams for the LASTI quad controls are complete.
- Wiring
diagrams for the ISI controls are 80% complete.
- Initial
discussions with Riccardo regarding the SAS
controls requirements have begun. A rough cut block diagram of the
required software has been generated and will be iterated over the next
few weeks.
Core Optics
No report this week.
Pre-Stabilized Laser
From: Peter King pking@ligo.caltech.edu
I had the chance to work with and see the high power laser at LZH for the
first time. Despite some last minute preparatory work by Maik and Lutz to get more laser power, the laser only
delivered around 100-110 W. The mode content was analysed
using the diagnostic breadboard that includes a pre-modecleaner.
Some problems with the output beam were due to a large corona that was present
on the beam. Although not viewable with the CCD camera-based beam
analysis hardware, comparision with the pre-modecleaner visibility revealed that a large portion of the
output power in the beam was in the corona. This was later traced to some
damage on one of the resonator mirrors and is also due to a possibly damaged
rod. The cleanliness implications are obvious. Some problems were
present with the injection-locked slave laser's PZT which meant that the NPRO
seed laser was locked to the slave laser, rather than the nominal operating
condition. The slow thermal drift
experienced by the laser was compensated for by feedback to the slow actuator.
The free-running noise of the high power laser was recorded, along with
transfer functions of the diode current for the various diode boxes to the
output power. In addition the transfer function
of the diode current to a single high power.
Auxiliary Optics
From: Michael Smith <smith@ligo.caltech.edu>
I designed stay clear models of the ITMx and ITMy SUS, a BS SUS, PO mirror BS SUS, and PO
mirror ITMx SUS in Solid Works. I have inserted STEP files
of these CAD objects into the ZEMAX layout of the ADLIGO vertex. ZEMAX cannot
trace rays with more than several of these CAD objects inserted. I am working
with ZEMAX support to determine the cause of the problem.
Other Laboratory R&D
From: Riccardo
DeSalvo <desalvo@ligo.caltech.edu>
Juri
I worked on the model of anisotropic dielectric coating. Improved
the Matlab code for the eigenmodes
of optical cavities with general shape mirror. I’m working on
several issues related on some papers I will write in the next months about
thermal noise and optical coating.
Chiara
I repeated the measurement of the transfer function of the system from 0.5Hz
to100Hz with more points in each range of frequency to have a better definition
of the function. I
also exted the range of mesurement
up to 150Hz.
Yumei
Just read and learn something about ANSYS.
Valerio
I finally managed, with the help of V. Sannibale,
to obtain a completely working model of the HAM-SAS inverted pendulum leg with SimMechanics. The model includes almost all the components
of the real IP: the leg, the flex joint, the counterweight bell and the
counterweight. One important improvement is that the Simulink
GUI is used only to build the model and all the linearization is now done with
a Matlab script. In this way we can easily obtain
families of characteristic functions, like transfer function or load curves,
varying the parameters of our model. In particular we have studied the system
for different values of the Load and of the mass of counterweight and we have
obtained results in complete agreement with the expected behavior. We have also
built a working model for the complete HAM-SAS horizontal attenuation stage:
this system is composed by the Optical Table, 4 IP legs, the sensors and the
actuators. We are beginning to study this model in a closed loop configuration
adding the expected noises coming from the sensors and actuators electronics.
At the same time we are still in contact with Mathworks
to understand the origin of our initial simulation problems.
For additional information about this report, contact S. Whitcomb or P. Lindquist