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The LIGO Executive Committee Agenda for Monday June 17, 2002 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items: S1 planning status report from Fred and Mark
no report
LIGO Operations--Administration
There was no site teleconference held on Thursday, June 13, 2002.
The list of current actions revised to reflect
the status of open actions assigned through June 06, 2001 may be found
at
ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>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
ACTIVITY
| 06/13/02 | Packages | Faxes |
| In | 40 | 44 |
| Out | 9 | 30 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
SUPPORT (Baldon, Torres, Lloyd, Tischler)
Progress Period from 06.07 to 06.13
Accomplishments:
The following additional change requests have been submitted:
| CR-010012
Revision B |
WBS 1.4.4.1 | Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites | P. Lindquist |
| CR-020007 | WBS 1.1.4 | Furnishing and Finishing of Livingston Building | G. Stapfer |
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by M. Landry)
--------------------------------------------------------------------
E8 concluded successfully on Monday night.
The 2k ifo remained in fully-recycled, common
mode lock for most of the run. The 4k however was not ready,
thus regular commissioning
efforts continued. Attendance during E8 was excellent, including
ten DMT authors, plus
sundry testers and operators, all of whom exercised 18 DMT monitors
and elogged
observations and suggestions. Keith Riles led an E8/DMT debriefing,
summarized at
http://blue.ligo-wa.caltech.edu/engrun/E8/info/minutes2_e8.txt.
A DMT summary page is
being devised for S1, to give a rapid overview of the current state
of ifo's.
State vectors for both ifo's are now available, comprising of 16 bit
words, each bit
assigned to a major component of an ifo. One bit is a "Go/No
Go" bit, set by the operator.
When all bits are set, the ifo is in "physics mode".
Three SURF students have arrived at LHO, including Heather Partner (tidal
actuation),
Aaron Virshup (DMT transient studies), and Brian Cameron (continuous
wave sources).
4K IFO Investigations
---------------------
LSC/ASC/DSC reboots were plentiful (on both 2k and 4k control systems),
in part to introduce
new code, and in part to rectify cpu crashes/seizures. Hardware
fixes included
coil bias module and coil driver circuits on the RM and ETMY, respectively.
MMT2 continues
to produce surprising alignment drifts. Test point dropouts noted
last week remain in
the small optics.
Optical lever pitch/yaw excitation points have been added to the large
optics (except MMT3)
in order to facilitate testing of the so-called 'super optical lever'
(SOL) and elliptic
low pass servo filters. Corey noted cleanroom curtains in contact
with optical lever piers
and loose mounting brackets for the optic lever laser were adding noise
to the op lev
error signals.
Nergis and Peter have been working along the chain of subsystems (psl,
pmc, iss, fss, mc),
making modifications to servo gains and eliminating oscillations along
the way. Details
are available in a series of Tuesday elogs, starting with
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=06/12/2002&anchor_to_scroll_to=2002:06:12:14:39:01-peterF.
Efforts to resume full locking continue.
2K IFO Investigations
---------------------
New ASC code is in use on the 2k control system. However WFS1
was not employed during E8 as
servo filters and gain issues had to be stabilized. The LSC FE
cpu was unstable prior
to E8 and may have been heating, as stability was achieved once the
racks were opened.
Daniel added a low frequency boost to the MC_L path of the common mode
board, significantly
reducing REFL_I and ameliorating the ifo transition into common mode.
Later in the week
he and Peter showed that DAC output noise is not our current limiting
source.
Optical lever servo fast channels have been added to the 2k. The
oplev servo will be
implemented on the ETMs, with the possibility of WFS feedback moving
to damp the ITMs.
The 59Hz harmonic forest in AS_Q has been shown to be produced by fans
in the ETM
controllers.
---------------
Facilities
---------------
The sheet rock is up in the office area and the contractor started on
taping the joints. The auditorium clouds are nearly finished, insulation
and sheet rock work is on going in that area. In the lab area mechanical
and electrical installations on going. Concrete work outside the building
is also on going.
----------------------
LASER SAFETY
----------------------
Last, week we commissioned
the new laser safety system here at LHO. The
system includes a new LHO site laser safety document (LIGO-M020131-01-W)
as
well as the hardware and access cards. This document describes how
we
currently are operating at the site as well as the minimal requirements
for
working at the site. Also a new Standard Operating Procedure for the
two
Interferometers is in effect (LIGO M020130-00-W). This document replaces
the 10W SOP. This document includes the full IFOs in their present
configuration, including the ISC/IOT tables, PSL tables, Transmission
Monitors and so on. If you are planning a visiting to the site or have
a
need to work unescorted in the laser hazard areas, please review these
documents. They are available from the DCC or I can e mail you an
attachment. The new system will take some getting used and is not without
some minor glitches that are being sorted out.
As a reminder also. If you
are coming to the sites, and plan to work
around class IIIb and class IV lasers, you'll need to have completed
a
"baseline" eye exam prior to your visit LIGO-M960001-B-P "LIGO Laser
Safety
Program.
Detector: The new LSC code by Rolf was installed this week. It contains an added feature which makes it possible to switch in filters gently by phasing the output at a zero crossing of the control signal. We also installed the new two stage dewhitening filters We had hoped that these added features would improve the common mode performance, but there is little apparent difference relative to the previous noise spectrum.
It is now clear why opening and closing doors on relay rack 1x9 causes the 60 Hz and multiple to vary in the demodulated signals. It is indeed due to RF which has 60 Hz sidebands. The clock signal at 4.1943MHz has 60 Hz sidebands that are about -40db relative to the fundamental carrier. The RF at 16.777, 17.825 and 18.874 also has 60 Hz sidebands but -50db relative to the carrier. The RF lines with sidebands were discovered with a spectrum analyser using a 30 cm dipole antenna placed vertically in the back of the rack. A more efficient way to search for the RF with 60 Hz sidebands is with a radio. When this was done, and to our surprise, the 60Hz and multiples envelope on many small amplitude RF lines between 4 to 10 MHz were found to have much larger 60Hz amplitude modulation than the largest carriers. The space inside the relay rack is virtually singing with RF having 60 Hz sidebands. There is no point in chasing ground loops until we understand the source of this RF. (Rai Weiss)
CDS: Ordered material and began installation of power and illumination of office area in new building. Received quote and schedule for installation of telephone lines in the new building. Completed termination of the replacement fiber on the south arm. Completed termination of the new LDAS/GC and CDS fibers that run from mass storage to the communication room in the new building. Repaired level control system at the west end station cyropump. Installed additional power for LDAS in the mass storage room.
Seismic Mitigation: Machined Springs: The machined spring first article has been heat treated and is currently being plated at Simmons Plating (New Orleans). Per my last conversation with Simmons, the spring will be completed by Monday and will be hand delivered to Power Dynamics (Stennis Space Center) for the joining process. We should have the spring by Tuesday and be ready to test the spring Wednesday. Spring Testing Preliminary efforts have been made to coordinate the first article test with LSU's Civil Engineering Materials lab. Joe Giaime, Carol Jacobs (LSU Civil Engineering instructor), and I met to discuss the apparatus, the resolution of the Tensile Tester, and the setup. We now have reasonable expectations of what data the tester can produce and how we can get the data that we feel important. LIGO Spring Tester The spring tester that is to be permanently housed at LIGO should be ready for noon tomorrow (6/14/02). I have been asked to go there to test the MEPI springs just in case there are any software changes. The unit would then be shipped to LIGO on Monday. HEPI Actuator: - I have spent most of my time fine-tuning the actuator plate, actuator manifold and the associated pin valves. We do plan to further investigate the assembly to assure ourselves that there are no interferences and that the components fit together correctly at first installation. Spring Analysis - No major advances have been made on the spring analysis since Sunday (due to my involvement with the actuator) It is my intention to finish that analysis this Sunday and present those results by next week. (Marcel Hammond)
LDAS:
Installed GigE cards into metaserver, beowulf, datacon.
Together with Al Wilson configured the 48 nodes. One of them appears
to be damaged. ASA should ship the replacement tomorrow. One power 20A
power strip is not working. Asked Bill Tyler to replace it.
Ordering two more UPSes and one more rack.
Running the burn test on the nodes.
Additional power has been added to the mass storage room to support
the new nodes.
Shannon Roddy layed out the cabling for the new cluster in cable trays
so that it can be easily maintained.
no report
The final week of classes for the year made for a slow week at the TNI. Since our last report, Kyle has been working with Jay Heefner to design and build our new, low-noise servo electronics. The new filters have been designed and modeled, including their noise performance, and the circuit has been laid out. We expect to have the filter completed and tested by the end of the week.
no report
Simulation and Modeling (Bhawal)
SimLIGO - realistic LIGO simulation package
-----------------
In the weekly e2e meeting, Matt talked about details of the new SimLIGO
model.
SimLIGO is the second generation LIGO simulation package. Han2k package
was
developed and used for the lock acquisition design, based on a scalar
field
calculation with minimal ISC content. SimLIGO is designed to be used
for the
noise simulation, as well as the lock stability study, of the as-built
LIGO.
In order to achieve that, it has the following features:
(1) realistic correlation of seismic motions and 6x6 stack transfer
function
(2) three dimensional mirrors, actuated by 4 OSEMs, with noisy
coil drivers,
enabling the simulation of the coupling
between length and alignment DOF.
(3) thermal noise (ad-hoc model based on Sam Finn's calculation):
pendulum, wire and internal
(4) digitized ISC and digital suspension controler
(5) realistic servo
(5-1) common mode servo implemented
(5-2) ADC-DAC running at 16k and 2k, with whitening-dewhitening
filer
(5-3) measured electronic noises
(6) shot noises
(7) ASC based on optical lever (on going) and WFS (waiting for
the LIGO design)
The simulation of the PSL/IOO is a simple model based on the
designed response.
In order to simulate PSL/IOO, the control bandwidth becomes
too wide, and the
simulation takes too long. The design decision was made to use
a simple model
for the major simulation, and a more sophisticated model of
IOO is used to study
specific problems of the mode cleaner. The building tool is
ready and can be
easily expanded. The issue is the simulation time.
Most of the major noise sources can be simulated now.
The running conditions, including the noise levels and IFO parameters,
can be easily tuned by editing a few input database files.
Right now, the speed of the simulation is around 600 times slower
(i.e., to
simulate 1 second of reality, it takes 600 seconds) for the
basic linear noise,
while it will be 6000 times slower to simulate with alignment
ODF activated.
Speed improvements (code improvements, compilers, faster machines,
etc) are now
under investigation.
Code development and maintenance
---------------------------------
(Hiro)
Keep working on the improvements of modeler for the new LIGO
simulation package.
One major issue in this week is the psd module, which is modified
to make sure it
works correctly when it is plugged in the digital circuit. The
accuracy of the
module is improved even when the spectrum is noisy. Combination
of macros (time
independent variable) and parameters (possibly time dependent
variable) is under
planning. This makes automation of the simulation involving
various stages easier
(e.g.,un-locked state -> locked state -> switch control to
low noise).
(Biplab) Fixed the problem of Recycling summation cavity that was giving
inaccurate
results when Matt changed the laser frequency as a part of the
common mode servo.
After that tested effects of laser frequency changes in 2-mir
Cavity, 3-mirror cavity
and Michelson recycling cavity.
(Matt and Biplab) While testing 3-mirror cavity, a problem was encountered
in
simulation runs of the primitive set-up of such a cavity. Several
changes have been
made in some functions of the field class and propagator to
fix this problem.
(Ed Maros) Started to work with Luca on tar ball build issues.
Alfi
-----
(Melody)
- Continuing on implementation of the 'Find' feature for alfi5.
(Bruce)
- alfi5 window resizing issue (visible area and the entire content
pane)
is worked out.
- Junction handling is being improved by taking into account
the
feedback.
LIGO Data Analysis System
Software Systems (Blackburn)
The reliability of LDAS to process jobs has greatly been improved over
the
course of the last week. We have removed all but one failure mode from
our
test suite which involves running a combination of 4 dataPipeline jobs
and
4 getMetaData jobs in a loop at a pace of about 7000 jobs per night.
This
remaining failure mode is due to a socket binding problem in the data
conditioning API and occurs in about 0.2% of the jobs and only in those
jobs that work with less than 2 seconds of data.
The memory leak in the dataConditionAPI remains at about 20KB per job.
Even
though a team of 3 people have been chasing it for a week. Looks like
we
will have to live with it in the Science Run. Our projections are that
it
will cause the managerAPI to restart the dataConditionAPI once near
the
end of the run resulting in an average of 5 jobs lost per restart.
We have begun testing the pre-release of LDAS on the systems at the
sites
(this excludes MIT which would prefer to stay with the old system for
now).
These systems have new Beowulf Clusters and we are still sorting out
the
configurations (which change daily as we find bad nodes). So far, during
the periods for which we have had stable hardware to test against LDAS
has run well. The overhead of starting MPI jobs on these larger clusters
is a bit disappointing, though not a show-stopper. We will make an
attempt
to find a way to improve this before the final release.
Testing of the generation of RDS frames using the previous (0.2.0) release
of LDAS during the E8 Run was very disappointing. This was because
of a
FILO issue in the 0.2.0 release of LDAS which was known and at the
top of
our list of changes for the 0.3.0 release (the TCL Channel Interface).
A
couple of jobs have been run to test the generation of RDS frames on
the
pre-release of LDAS which did not suffer from the FILO problem but
did
indicate that we are not able to keep up with the data. It is taking
about
5 to 10 percent longer to generate RDS frames the the original frame's
length. One factor in this is that the amount of data int the RDS frames
continues to grow. We were originally told that 121 channels would
be in
the RDS frames and we found that the testing was done with 152 channels.
This more than accounts for the 5 to 10 percent fall off.
The web site for applying for new user accounts and passwords for using
LDAS is nearly complete. We need to test it extensively before going
live
with the system on Monday.
Several new graphing packages are now working in the controlMonitorAPI.
It
is now possible to graphically track the node utilization over a user
specified time range. This proved very useful for tracking down a bug
in
the mpiAPI which was reporting resources not available when we could
clearly
track that there were plenty of nodes unused in the system.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Assisted James Patton with integration of Sun T3s into HPSS
configuration (configured T3s and fibre channel switches and
pulled
fibre between hosts, switches and tape drives).
* Assisted LLO with installation of SAM-QFS 3.5.0-57.
* Installed SAM-QFS 3.5.0-57 on Caltech machines (the gateway, dataserver
and metaserver machines in ldas-dev, ldas-test, ldas-cit).
* Began testing multiple interswitch links on the ldas-archive machine.
(Al Wilson)
* Setting up new Beowulf nodes at LLO and LHO.
(Stuart Anderson)
* Remote support for Beowulf and GigE upgrade at LLO and LHO.
* Obtained initial standard discount pricing information to complete
the Storage Area Network (SAN) at LHO and LLO.
* Re-enabled the OC-12 connection from LIGO to the high performance
network
at CACR and setup static route to allow 20+MB/s transfers from
Caltech
to UWM.
MIT
---
(Keith Bayer)
* Had sun replace T3 disk.
* Swapped Foundry switches.
* Installed new version of QFS on E450 / SF880.
* Fixed /dso-test mount points on cluster nodes and beowulf.
* Getting quotes for PC Raid NAS.
* Redistributed ldas power load onto 4 separate circuits.
* Received extra rack shelving from Caltech.
Livingston
----------
(Igor Yakushin)
* Installed GigE cards into metaserver, beowulf, datacon.
* Together with Al Wilson configured the 48 nodes. One of them appears
to be damaged. ASA should ship the replacement tomorrow. One
power 20A
power strip is not working. Asked Bill Tyler to replace it.
Ordering two
more UPSes and one more rack.
* Running the burn test on the nodes.
* Figuring out how much more power we need to run LDAS safely at LLO:
we
already twice overloaded the circuits here.
Data Analysis Activities (Lazzarini)
Shawhan (from the week of 6 June) Discussed hierarchical search algorithms
with Anand Sengupta, who arrived
this week for a three-month visit.
Wrote a handbook about hardware signal injection, and worked on plans
for
a campaign of injecting a series of many simulated signals shortly
before
the S1 run.
Mendell: For The Weekly Report: June 6, 2002; Data Analysis Update:
Continued work on the knownpulsardemod DSO. Updated the calls
to the
barycentering and amplitude demodulation LAL functions and identified
several more issues with the LALDemod code that I am sorting out with
the AEI group.
General Computing (Wallace)
MIT:
(Keith)
-Working on NIS+ setup
-Setup forwarding web server (ligo -> emvogil-3)
-More Solaris system upgrades with MU7
-Wireless troubleshooting
-Ordered AIT3 tape drive
Livingston:
No report received
Hanford:
(Christine)
- Continued cleaning personal files and software off old PCs.
- Setup one of the old PCs as a "new" PC for a staff member who's old
PC
was older than the old PCs.
- Working on a very baffling e-mail problem on a Windows 2000 PC.
- Purchased more 8 mm tapes, cat5 cables and wireless cards.
- Set up new modem accounts for SURF students. Helped the SURF
students
with various e-mail and account setup.
- Various other user support including printer repairs, help setting
up
a new laptop, and troubleshooting a log-out problem on Windows 2000.
(Larry)
- Worked on VRVS setup with Christine and Mike. The setup is pretty
clean.
However, the resolution needs to improve and the setup for VNC also
needs
to be worked on.
- Review computer security audit materials with Christine. This is
in
preparation for a internal security audit of equipment at the Observatory
that will take place this year.
- Working with Albert, Christine and others on the updrade to the WAN.
CIT:
(Lisa)
- Caltech had a power surge that brought down some of the machines.
Mike and I
did a walk through to make sure everything came back up again.
All of the
servers in the server room are on UPS units and were unaffected.
- Installed a new hard disk in propus. Sun is no longer honoring
the 5 year
warranties on hard disks.
- Installed an external hard disk and tape drive for use as backup
in the
40meter martian network. I still need to put backup scripts in
place for that.
- Installed and began evaluating a demo of sarcheck. It is commercial
software
that takes the output of sar, analyzes it and makes performance recommendations
on a system.
- Spent time on the luna rebuild. The final installation will take
place
when Rolf OK's it.
(Veronica)
- LIGO website: posted several updates to Postodoctoral/Fellowships,
MOUs,
Employment, Internal Bulletin Board. Reworked several pdfs of the Elba
Conference talks: to reduce file size and to shorten the download time,
I
retyped text-only pages in the scanned files; in some cases, it reduces
the file size in half. Dealt with a DCC search engine unable to locate
an
existing file. Working on the Travel Policy webpage and on LIGO Press
Kit
online version. Started working on a webpage for the upcoming LSC August
meeting.
- GNATS database: need to edit the GDS part of it; need the input from
Szabi and others about what needs to be done. Getting familiar with
the
how-to in the meantime.
- LDAS websites: there are several updates waiting to be made. I started
to edit images offline; will post them shortly.
- CaJAGWR website: added another member information.
(Mike)
-Loaded a Laptop with OS and General Computing software.
-Tried working the PHERKAB server but having problems bringing the
new
server up due to a caching of old server that looks like is being cache
at
the router.
As far as database and webserver goes this seems to be running like
it should.
We will run some more tests on Friday to see if we can clear up the
caching
problem.
- A PC computer was having problems with Anti Virus Software; I had
to
reinstall Anti Virus software and FrameMaker 5.5 that seem to have
got
corrupted possibly from an old virus.
-Problems with the 5000 printer, it seems like the Duplexer has went
out. I tried cleaning the rollers and other components but had no luck.
I ended up calling HPC to have them come out and check this out, and
it
turns out that the duplexer is out and needs to be replaced; we have
this
on order.
-Cleaned up and ran Norton Utilities on the Bridge 3rd floor computer
that is
used for scanning and writing CD's.
-Worked on getting the required information from ANSYS people to upgrade
server and workstations.
-Received the new licensing from Ansys and have upgraded the Flex LM
server.
-Upgraded multiple users with the new Ansys 6.1 software; everything
seems
to be working okay.
-Installed Ansys on my win98 computer that is in my office and
notice that Ansys is no longer supporting their software on win98 Operating
Systems. This software has not been tested on win98 and should only
be run
at a minimum of NT4.0 with service pack 5 installed.
A brief reminder at the end of this year Microsoft is no longer supporting
NT4.0. We could be looking into some problems with software drivers
in
regards to upgrading our current engineering packages in the near future,
due to the lack of support from Microsoft. This well eventually flow
down
to software manufacturers that well force us to upgrade all win98 Operating
systems to Win 2000 pro. From here on out I will try not to reload
computers with Win98 only with Win 2000, but I might run into some
hardware
compatibility problems. This might include some of our current computers
to
get upgraded with more memory and possible motherboards/cpu's etc.
(Larry)
-Resolved a few procurement issues. Working on a number of supply procurements.
Mostly cables and memory cards. Reconciling a number of orders placed
on P-card.
Updating the licenses for Exceed and the maintenance contract on the
router.
-Added more domains to the blocked tables and removed a couple that
we need. We
do have a way to block an entire domain and let specific users through
and that
has helped in some cases.
-Reviewing documentation and present h/w setups. If there are not too
many
problems this next week, the group will have a test network setup to
check out
some of the upgrade equipment being installed.
-After the power glitch Caltech had this week, it looks like the new
edge
switches are too sensitive and will need to be put on a UPS.
-Still checking on security equipment for the remote control rooms.
-Worked a few printing issues and reviewing the warranty dates. It
appears that
all but a couple of the printers are now no longer covered. The extended
warranty period has expired on most of them.
-ToUcam is no longer being manufactured and we are looking for a WEBcam
of the
same resolution, performance and price. So far no luck. The suggested
replacement webcams that have been tested did not perform well.
(Bruce Sears)
ILOG maintenance:
(1.0 day)
- New user administration and tracking of problems
accessing
the various
log installations for maintenance.
Lazzarini:
Lazzarini, McCarthy, Patton, Raab, and Wallace met with PNNL and NoaNet
representatives on 7 June in order to discuss upgrade options and
paths for the LIGO WAN at LHO. The meeting identified the technical, programmatic,
and fiscal issues that need to be surmounted before the upgrade can happen.
A number of action items were identified and assigned. The plan is to implement
a 2-stage (near-term, long-term) upgrade that can hopefully be put
in place by mid-summer (unfortunately not in time for S1).
LSC LASERS WORKING GROUP (Benno Willke)
Minutes of telecon June 6 th 2002:
participants: morning call: Jesper, Damien, Maik, Michèle, Volker,
Rupal, Benno
, evening call: Peter F., Peter K. Garry, Shally, Ralf, Maik, Benno
1) updates
Adelaide:
- problem with Teflon coatings at TIR interface, when pumped with high
power bubbles
seem to show up on the Teflon coating and the spatial waveform of the
output beam
looks terrible
- SiO2 coating on that interface won’t work, because the TIR angle
is different and the
hence the angle of the end faces are wrong, changing these angles and
coating the TIR
surfaces with SiO2 would cause a big delay and is expensive,
- this problem was not encountered in the earlier work on the system
pumped with 100W,
now the pump power is 600W and the temperature of the slab is expected
to be higher
- next steps will be to make test and optimize the Teflon coating under
thermal load
- in the afternoon conference call Peter King mentioned, that he knows
a company that
makes very good Teflon coating and will contact Jesper or Damien on
this topic
LZH
- laser rods are back at LZH and will be coated within the next 3 weeks
(these crystals had
initially a wedge which caused parasitic lasers to start beside of
the main laser path)
- in the mean time amplifier experiments were started with a rod longitudinal
pumped with
150W through both end faces, 60W were achieved by amplifying a 10W
laser in 4 path
through this rod,
- during spatial profile optimization of the amplifier the crystal
cracked at the position of
the O-ring sealing, with only 10W 1064nm seed laser and no pumplight
present
- in spite of the claim of the O-ring vendors the O-rings were found
to absorb a lot in the
infrared, the plan is to replace them by Teflon O-rings which were
measured to have a
small absorption
- Rupal Amin is visiting from the University of Florida to work on
the thermal lens
compensation of the Faraday Rotators supplied by Efim
Stanford
- Peter King and a colleague visited Stanford to optimize the LIGOI
type laser, result:
output power increased from 7W to 10.5W by realigning the amplifier
stage and
increasing the NPRO power
- after the amplification of this laser by the external Lightwave amplifier
a power of 21.5W
(not optimized yet) could be injected into the first stage edge-pumped
Stanford slab, the
output power was 30W for 150W pump power, M 2 = 1.2 (M 2 measurement
might be
inaccurate due to beamscan problems)
- end-pumped slabs will be send out for coating and are expected back
in about 4-5week,
by that time the first prototype laser head with microchannel cooler
will be available
From: Helena Armandula <ahelena@ligo.caltech.edu>
Advanced LIGO Coatings
After evaluating 1"dia. coated substrates annealed at different temperatures,
we asked MLD to anneal the "Q" substrates coated with Ta2O5 /SiO2 at 450
degrees C for 24 hours. Also, to include in the same annealing cycle, 1"
dia. substrates coated with Nb2O5 / SiO2.
Another set of 1"dia. parts coated with Nb2O5 / SiO2 will be annealed
at 500 degrees C for 24 hours to evaluate for absorption and decide on
the best temperature to anneal the "Q" coated substrates.
Advanced Suspensions - Silicate bonding
Researching measurement options to characterize silicate bonds to determine if creep is present after the bonded substrates have been submitted to a load.
We are procuring some Schott FS-4 glass to evaluate polishing behavior
and to run silicate bonding experiments.
From: ctorrie <ctorrie@ligo.caltech.edu>
SUSPENSIONS
Mode Cleaner
Drawings and assemblies ongoing.
MIT Quad
I had a telecon with Norna to discuss the recent work on the Quad by Rich at MIT. We hope to gather a full set of impulse responses, transfer functions and frequency tables to compare the experimental and theoretical results on the quad in its current status.
Other
Worked with Phil in the OTF for a morning helping to install new table
legs.
I have written a basic project plan for the 2 SURF students, John Vietch
and Dan Mason start with Janeen and I next week.
From: Janeen Romie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Working with Thomas et.al. on the GEO PPARC Proposal input.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Alessandro
Accelerometer paper ready at 75%
Virginio
Both theoretical and measurement MGAS papers ready at 80%
Szabi
IP paper 50-60% done.
Akiteru
I have been working on details to finalize our work.
Here is a to-do list for next few weeks, apart from desk works:
- implement inertial damping
- improve the optical lever: remove laser and PD from the vacuum tank,
replace them with better ones.
- repair broken electronics, particularly coil drivers
- replace coil driver for the end mirror to a lower noise version
- implement dc alignment on the suspension platform
- implement low freq longitudinal control on the IP and the sus platform
- confirm beam centering scheme for the end mirror
I have been working on the inertial damping and the optical lever this
moment. Some of the rest has been prepared already.
After these small tasks, I will take (hopefully final) measurements
in air and vacuum.
Eric
Made first microdensitometry measurements of MoRuB samples I have done
more extensive analysis into the x-ray images on Matlab (including 3-d
imaging and histograms) as well as taken a microscope picture. This
has led to concerns about background noise making it impossible to detect
surface variation. I contacted the film manufacturer and am waiting
for a response about how to what resolution the film is accurate.
I also plan on somehow averaging the image in order to clearly see the
general surface trends, as well as attempting to minimize background noise.
Writing my initial SURF progress report.
Hareem
Splatting more samples of MoRuB-16, MoRuB-18 presents annealing fragility.
Tried new CuBe splatting anvil heads, maybe the wrong material, tend
to stick to film. Working on AuSi brazing alloy, obtained not uniform
melt. Miniarc melter broken and repaired.
Aso
Preparing talk for next LIGO seminar. Still calculating flexures
under stress and finding it tough.
Mike
Finally a good and repetitive TTO measurement on a standard Ni sample.
Now proceeding to Vitralloys and Glasmet.
Heat capacity holder finished by machine shop. Preparing cabling
for heat capacity measurement.
Kelin
Reconditioned position sensitive photo diode puck. Found mismatch
between laser and photodiode sensitivity, buying matching pair.
Purchased mechanics for room temperature Q-measurement setup.
Ric Hareem Eric
X-rated!
Got safety training for X-ray use.
Ric
Fixed some more problem in creep measurement on June 6th,
For additional information about this report, contact sanders@ligo.caltech.edu