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The LIGO Executive Committee Agenda for Monday October 7, 2002 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Executive Committee only 11:30 - noon
Topics:
Special Items: IT Security Plan
no report
LIGO Operations--Administration
There was a site teleconference held on Thursday, September 27, 2002. The following issues were among those discussed:
The list of current actions
revised to reflect the status of open actions assigned through September
27, 2002 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
| For
Week Ending 09/26/02 |
Packages | Faxes |
| In | 34 | 34 |
| Out | 12 | 37 |
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)
CONSTRUCTION:
SUPPORT (Baldon, Torres, Lloyd, Tischler)
>Irene Baldon
Progress Period from 09.27 to 10.03
Accomplishments:
Weekly Advanced LIGO Project Controls meeting was not held this week.
Advanced LIGO MRE Proposal (Highest Priority)
Out of the office Friday the 4th and Monday the 7th.
See http://pmi2002.fusionproductions.com/ for conference details.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
The following change requests have been submitted:
| Open or Recent Change Requests
| |||
| CR-010012
Revision B |
WBS 1.4.4.1 | Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites | P. Lindquist |
| CR-020012 | OPs 1.6 | Additional Funds to Complete 40-Meter Facility Upgrade | A. Weinstein |
| CR-020015 | WBS 2.11, 3.11 OPS | Low Noise Dust Monitors (For Information Only) | D. Coyne |
I have distributed (via .pdf attachment to email) Change Request CR-020016
submitted by Otto Matherny for consideration during the Executive Committee
Meeting on Monday, October 7, 2002. The request is for $60,000 for
irrigation, erosion protection, and landscaping around the new Laboratory
building at Hanford. The amount requested is less than the amount
held for this purpose on the liens list for LIGO Construction.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
No report this week
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by F. Raab)
-------------------------------------------------------------------------------------
(see ilog for details - if it's not in the ilog, it didn't happen...)
2K IFO (H2)
-----------
Last week I reported that Jay had some reservations
about confusing signals from SM2 on H2. The following day, after straightening
out some DAQ problems, we were able to make a test for mechanical interference
with the suspension by measuring the pendulum modes of SM2 with no damping.
Instead of seeing the expected pitch, yaw and position resonances between
0.7-1.0 Hz, we saw a yaw resonance and new resonance at 1.8 and ~ 6 Hz.
The higher frequency resonances indicated large restoring forces in the
missing pitch and position modes, but the presence of the soft yaw mode
indicated that the optic was still suspended. We hypothesized that we probably
had a charge transfer hanging up the mass or the wire had jumped out of
its alignment notch. We guessed that this may have occurred by an excitation
of the optics table during the two-week period that the electronics were
being changed, leaving the optics undamped.
We began planning an entry into the HAM7 vacuum
chamber to make repairs. Staging took the first three days of this week
and we were ready to start repairs on Thursday morning. The hope was that
we had a charging problem and that the vent might discharge it as the pressure
in the chamber passed through the region of electric field instability.
However we were ready to enter the chamber if this did not work, and we
were ready to pull the suspension if we could not make repairs in the chamber.
Luckily the discharge did the trick. We began the vent at
8:35 am PDT and the optic came free at 8:36. By 9:10, we had completed
suspension tests and initiated a pumpdown shortly thereafter. Pressure
dropped rapidly and we were able tore-open the gate valves by the afternoon.
4K IFO (H1)
-----------
Francois Bondu, Luca Matone and Rick Savage continued to work on frequency
noise. They characterized the electronic gain for the two paths: the VCO
and MC2. A simulink model was then created to estimate open and closed
loop transfer functions. The measured 'effective' frequency stabilization
of the MC was found to agree well with the model.
Bill Kells worked on measurements of optical properties of H2.
No report due to hurricane. All is well though.
This week
has been spent answering questions and directing the welder
assembling
the first article HEPI actuator. Also generating a parts list and
ordering a
multitude of fasteners, o-rings and hydraulic fittings and
valves. The
threaded, mechanical process to restrain the diaphragm worked
fine, but
needs to be qualified in Stanford's test stand.We
expect to have
an actuator
completed this Thursday or Friday, and bring it to LLO for a
Helium leak
check first thing next week. Day by day progress this week can
be seen at
these sites.
http://emvogil-3.mit.edu/~jkern/ActuatorAssemblyOct1/index.htm
http://emvogil-3.mit.edu/~jkern/ActuatorAssemblyOct2/index.htm
Ken Mailand, Lee Cardenas
The LASTI pump station prototype is being revised to eliminate the possibility of any leaks. Shipping the pump station to MIT is delayed till about 10/28 (date TBR).
This afternoon,
Ken and I, went on discussing the tasks needed to accomplish our goal.
As part of the tasks, I have finished pumping out all the mineral oil out of the reservoir. Tomorrow will empty the rest of the oil from the coils and blow it clean. The mechanical work can be accomplished easily but getting the parts needed is what will dictate the timing.
The features and configuration of a final pump station
design were discussed and agreed to at the last weekly meeting. This design
will be fleshed out for the upcoming PDR.
- Completed
installation of new Digital Suspension Control (DSC) and DSC related
software at
LLO.
- Working
on some DSC software change requests:
1)
Add four filter banks input of each optical lever (code ready to test)
2)
Allow multiple GDS EXC/TP per large optic (code ready to test)
3)
Display GDS EXC/TP names on monitor screens instead of numbers (code for
small optics
ready to test).
- Working
on a version of Dataviewer which replaces present 'xmgr' graphics
package with
'GRACE' graphics software.GRACE
is essentially an updated version
of xmgr.
Spent last
week at LLO doing repairs and testing of the DSC LOS coil drivers and measurements
of EMI backgrounds.
Rich Abbott reporting
1.Received
the boards to phase lock the individual capacitance position sensor modules
together.They are stuffed and being
shipped to Joe G. at LLO
2.Flavio
has distributed a preliminary list of requirements for the ISS to get the
ball rolling there.
3.Started
to develop noise filters to improve the interface between the electronics
and the pump motor controller on the hydraulic pump speed control servo.The
inverter used to power the motor is a significant source of EMI.
4.Mohana
has been working on the requirements for the timing system
5.This
week, Rich will be traveling to LASTI to help out there.
Mohana Mageswaran
I have finished
testing one of the Seismic interface module
chassis with
the corrections, and it will be shipped to MIT
tomorrow.
And I worked on the protel schematic of the Altera
FPGA variable
timing module. I am working on the requirements
document for
our new variable timing board.
Jay Heefner reporting
FPGA Timing
Board Prototype
===============================
- The schematics
for the prototype board have been completed and the board is being layed
out. Layout should be complete by Friday.
- Logic for
the FPGA has been developed and is awaiting prototype board for test.
Adv LIGO Suspensions
===============================
- System drawings
for the CIT and LASTI prototype have been completed.
-Design of
CIT supplied whitening and Anti-Alias modules has started.
DSC Upgrade
===============================
- Marked up schematics for DSC installation for each IFO have been generated and are being checked. Following check the as-built schematics will be issued.
Sander Liu
Shipped a set of micro-seismic signal processor (remote interface box + post processor) to LLO.
The
free-running length noise of the optically contacted
pre-modecleaner
was estimated by locking NPRO #259 to the pre-modecleaner.
This at least
represents an upper bound of what the length noise would be.
For frequencies
less than 1 kHz, a factor of 2 to 2.5 improvement was
observed.At
around 10 kHz, the length noise appeared the same as that for
an epoxied
pre-modecleaner.However the measurement
from 10 kHz and above
looks odd
because it's flat, suggesting some noise floor rather than the
true noise.Thus
far I have not been able to track down the source of the
noise floor.The
lowest body resonance observed is around 13 kHz compared
to the epoxied body's 10 kHz.
I have been
working on the requirements on the flat topped mirrors; I used
the map Garilynn
gave me for the surface of the beamsplitter in Ligo I, adapted
to the specifications
of the flat top mirror and looked for how bad the contrast
becomes for
different values of a multiplicative factor I put in front of the
distortion.
Most of the power is lost in the first excited modes and adjusting
the alignment
can compensate for most of the overall effect. For this reason I
am going through
some papers on the alignment control in order to follow what
the system
is supposed to do when the TEM10 and TEM01 are reflected back from
the resonator.
OTF Lab.
(Bridge)
Contamination
Cavity # 1
Cavity still
locked and continue taking ringdown measurements.
Liyuan has
accomplished in setting up the new lab view PC version program for the
Ringdown measurements.
Scatterometer
Motivated
for the new measurements for GEO we have switched all our efforts to
reviving the
Scatterometer ASAP.Even though,GEO
later decided to have the measurements done by
Waveprecision,
We still went ahead in our efforts, and as a result, we recovered the
function of
theX-YAxis
base plate that holds theETM .We
encounter a small situation as the Y-axis motion can go forwards but can't
go backwards.We solved thissituation
temporary by making the changes in the program.Liyuan
is still debugging the program.
We have tested
the motors in both X-Y directions loaded with 44 Kg. of weight that we
increased
the weights
in small amounts until we reached our desired weight.The
heaviest ETM Sapphire weights
40 Kg.The
others( ITM, BS, FM, PRM, SRM, MC1-MC3 ) are less.
I have looked
into the base plate to make the changes so it can hold different ETM diameters.
So far, I
decided to make a new base with adjustable legs to accommodate the desired
diameters.
punch some
holes to reduce the weight on the new plate etc.All
these efforts are in progress.
New OTF
Lab at Lauritsen ROOM 38
Cavity #3
Reference Cavity still pumping down. Optical train ready.
Continue taking
RGA measurements.
Cavity #2
Test cavity
This cavity
still pumping, optical train installation in progress.
Continue taking
RGA measurements. I am still looking for a new roughing pump.
The old one
will be repaired eventually.
The New OTF
lab. is ready for operation.We'll
continue the works.
no report
LASTI (Coyne, Harry, Kern, MacInnis, McKenzie, Mason, Mittleman,
Ottaway, Rollins, Shoemaker, Zucker)
=============================================================
VACUUM SYSTEM (Zucker, MacInnis)
Still at 1 atm for MEPI testing
PSL (Jamie R, Kirk M, Mike Z and Dave O)
Jamie completed design and layout for his 300 mA photodetector for
intensity noise studies. Kirk is measuring and modeling the prototype
fast FSS card.
MEPI/HEPI DESIGN, FABRICATION AND INSTALLATION (Mason, MacInnis, Coyne)
MEPI Installation
Several of the Kamam position sensors were damaged during setup and
had
to be replaced. We believe the damage was caused during the calibration
when the flag touched the sensors. We now calibrate over a shorter
distance and none have been damaged.
HEPI Design and Installation
We spoke with several suppliers to install plumbing for hydraulic lines
from the pump room into the high bay. We are planning on 1" dia
stainless tubing from the pump to the large manifold tig
welded the entire way. They will also run 1/2" dia stainless tube up
to
each of the 4 small manifolds on the top of the piers. VCO fittings
will
be placed on the small manifolds so that
they can be blanked off and the line can be helium leak checked.
HEPI/LASTI Fabrication (Hammond/Kern)
This week has been spent answering questions and directing the welder
assembling the first article HEPI actuator. Also generating a parts
list
and ordering a multitude of fasteners, o-rings and hydraulic fittings
and valves. The threaded, mechanical process to restrain the diaphragm
worked fine, but needs to be qualified in Stanford's test stand.
We
expect to have an actuator completed this Thursday or Friday, and bring
it to LLO for a Helium leak check first thing next week. Day by day
progress this week can be seen at these sites (hurricane permitting).
http://emvogil-3.mit.edu/~jkern/ActuatorAssemblyOct1/index.htm
http://emvogil-3.mit.edu/~jkern/ActuatorAssemblyOct2/index.htm
EPI MODEL DEVELOPMENT, TESTING & SIMULATION (Coyne, Ottaway &
Mittleman)
MEPI/Ham Characterization update
We now have four fully instrumented HAM piers. A number
of the new
position sensors did not work after being installed; these were
replaced and everything works.
#MZ note: now understood
as an assembly/calibration problem,
resolved.
Professor Nayfeh and two of his graduate students, Lei and Osamah, were
in last week characterizing the external support structure. There
have
identified and characterized a number of modes, and plan to return
next
week for follow up work.
The DSpace system identification has begun, with some preliminary
results.
Today we found that the piers were not completely free, some stops
were
just touching the suspended mass, one actuator might have been in
contact with it coil. How this affects the previous measurements
remains to be seen.
#MZ note: this problem was
mechanical interference with one
of the motion stops; it
has now also been resolved.
MEPI model
Dave finished the MASS/Spring constant matrices, and they should
be
installed in the MEPI model quite soon.
Simulation and Modeling (Bhawal)
E2E Physics meeting
-------------------------
Matt and Biplab discussed about the WFS outputs of SimLIGO and why
some
outputs for modes of pitch are different from outputs for corresponding
modes of yaw. Hiro and Matt then discussed about the implementation
of
merged box files which may speed up the modeler runs.
SimLIGO
---------
(Matt & Biplab) Continued debugging of WFS in SimLIGO. Apart from
RM (Rec Mir)
mislaignment (common) mode, all other modes generate correct signals.
However, in Han2k runs, all including the RM mode generate correct
outputs.
From various tests and our current understanding, it seems to be a
problem somewhere in data-handling part of SimLIGO or the extraneous
matlab files used to look at the data.
Code development and maintenance
----------------------------------
(Hiro) Modeler Code: Working with Melody to support the merged box
file.
File caching support is implemented in a similar way for the merged
box
file and standard box files. These modifications will simplify and
speed
up the use of e2e. Various other low level modifications are going
on
to support the next version of SimLIGO.
(Biplab) Another bug in misalignment calculations for summation cavities
was traced out.
Alfi
-----
(Bruce)
- Cleaned up and modified event code for cut and paste implementation.
- Continued implementation of cut and paste.
(Melody)
- Continued work on the automated tester for alfi5.
- Finished first version of exporting modeler files from alfi5.
LIGO Data Analysis System
Software Systems (Blackburn)
Dedicated ldas user accounts were created for testing each of the different
search strategies that are looped throug each night. This should allow
test
rates that exceed the current throttle limit for individual users (one
job
per second). Hard to beleive that LDAS is approaching this level of
job
submission with 95+ percent succcess rates.
The new frameCPP is approaching the 90% complete mark. This has allowed
it
to be integrated into LDAS. The frameAPI, dataConditionAPI and eventMonitorAPI
have all undergone some changes to support the new frame specification.
We are
currently able to run jobs through with this new frameCPP, though a
complete
investigation of the validity of the data products has not been finished.
The
preliminary results are seeing some minor differences in the data products.
We
are currently looking into these to see if they are numerical precision
or
indications of some bug in the new frameCPP its usage in LDAS. One
of these
tests which has been completed does indicate that the correct data
is making
it way from the frameAPI through the dataConditionAPI and into the
wrapperAPI
for simple data types.
Several problem reports associated with shutdown and startup of LDAS
APIs have
been addressed this week. In addition, several problem reports in the
data-
ConditionAPI have been closed out this week.
A big bug in the controlMonitorAPI server was discovered this week which
caused
requests to add or modify LDAS user accounts through the Secure Web
Server to
fail.
Some of the excessive logging in the metaDataAPI has been suppressed
which
should help to increase database request performance by a few percent.
The performance of the diskCacheAPI was improved by a factor of a thousand
for
the larger directories currently exported by the new RAID disk servers.
This
fix was identified when it was discovered that the frames listed from
large
directories was not in a sorted order as expected.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* SAM-QFS: Imported the tapes that had been erroneously exported so
the copy
of S1
data to IDE-RAID could continue. Did a tape catalog changeover
to simulate
moving tapes from a site to CIT. Copied files to
IDE-RAID
that had been missed due to their tapes not being imported
earlier.
Started work on sanity check scripts to make sure the
SAM-QFS
configuration is writing data to tape in the way that
we want.
(Al Wilson)
* Started the LDAS upgrade to RedHat 7.3
* Updated the Kickstart file for RH7.3. Have a local copy of the
disk
image, when out of the beta stage I will post it on the ldas-sw
machine
* Updated the rpmsync files for RH7.3. The new files are ldas
and node.
Same names as before but different RPM's Note that there is
still a
listing for Beowulf. This will be removed in the near future.
And a file
for workstation was updated, but not tested.
* Overhauled the cfdef files. Old copies are still left on the system.
There will be 3 classes of machines ldas, node, workstation.
Besides
removing obsolete files, updating site specific files, the def
tree has
been pruned.
* Updated the ldas-dev system to RH7.3. Looks like it survived the storm.
Node15 looks like the only casualty. There is one problem still
need to
be worked out, the nodes on the dev system hang on boot without
an
keyboard plugged in. This is new with the upgrade.
(Stuart Anderson)
* Finished retrieving LHO S1 data from SAM-QFS and copying to IDE-RAID.
The average transfer rate was an impressive 27MB/s.
* Working on installing complete LDAS systems on each of the new LDAS
server farm dual-CPU systems.
MIT
---
(Keith Bayer)
* Installed several firmware version of 3ware card (7.5.2 took)
rebuilt raid on datawulf
Hanford
-------
(Greg Mendell)
1) Four beowulf nodes have experienced problems since purchase: node25,
node29, node32, and node48. All have since past
the burntest, after
repairs, and have run over a week without problems.
I have added
node25, node29, and node48 back into the list of nodes
available to LDAS
at LHO. Node32 did initially crash again during
the burntest, but
subsequently passed. However, I plan to do additional
testing of this
node.
2) Sorted out issues with raw S1 data sent to Caltech and RDS data sent
to UWM. It seems some problem occurred with 3 tapes
sent to Caltech and
1 tape sent to UWM. The UWM problem occurred for
a small amount of
data, and this data was transfered over the internet to
UWM from disk at
LHO. Igor and I will check the tapes sent to Caltech,
and replicate
them from data on disk if the tapes are unreadable.
Data Analysis Activities (Lazzarini)
Mendell:
1) Generated a playground set of 64 second LIGO S1 H2 SFTs on two 5.69
hr GPS intervals: 714150032 to 714170512 and 714886656 to 714907136.
This is to investigate issues of windowing, filtering, and padding,
as
well as nonstationarity of the noise during SFT generation. The
shorter
time SFTs can also be used to test code being developed to search for
periodic signals from neutron stars in binaries.
2) Assisted the PULG group in preparation for the lsc-wide telecon on
Fri Oct 4, 2002.
Weinstein:
- Continued to run LDAS jobs on S1 playground data
with burst simulations, injecting gaussians, sine-gaussians,
and ZMs.
- Discussed issues regarding the time dependence of calibration,
relevant for burst group work, with Patrick and LSUG.
Shawhan:
* Working with Keith Riles and Vladimir Dergachev at Michigan on plans
for
a new, multi-platform trend-data viewer.
MIT:
Continuing investigations on S1 playground data with Bursts
DSOs (Laura, Stefan, SHourov, Erik) and vetoes (Stefan, Shourov)
in preparation of the weekend analysis meeting. Alan made
available (software) injection data that Laura started parsing.
Lazzarini;
Together with Mike Landry and David Shoemaker, I set up a new web site
(temporarily located in my directory) that will become the source of
"official" sensitivity
curves (with DCC numbers) for people to use in talks, publications,
etc. The site includes
links to the ASCII data files from which the graphics were created.
See
http://www.ligo.caltech.edu/~lazz/distribution/LSC_Data/
General Computing (Wallace)
Lazzarini: Iterated on the IT security plan with a number of people
across all LIGO sites
MIT:
(Keith)
-Reinstalled win2k on XP box for DSpace utility (R Middleman)
-Helped setup linux box for Tania
-Ordered software / harddrives / printer supplies
Livingston:
(Tom)
-Monday afternoon: Finally finished recovering from hurricane Isidore.
-Tuesday morning: Began preparing for hurricane Lili.
(Shannon)
-Recovered from Isidore storm.
-Prepared for hurricane Lili.
-Went over a number of logistical issues with Larry.
-Setup a couple of PC's including a laptop for Mark.
Hanford:
(Christine)
- Upgraded fortress, the LSC sandbox computer, to Solaris 8.
It's still
behind all the other computers on upgrades because the Solaris 9
drivers are not available yet for the ATM card. The upgrade to
8 at
least means that it is now compatible with the DMT computers.
Had to
install new drivers for the ATM card and external scsi raid system.
Still waiting to hear from Sun for new drivers for the internal raid
system. Also installed the latest version of SSH 3.2.0.
- Setup a new PC for a new operator. Cleaned off personal files
and
upgraded an old laptop that is being handed down from the old owner
to a
new owner.
- Fixed some problems with the daemon config file for the latest version
of SSH.
CIT:
(Mike)
-Reloaded Irene's and Ryans computer from win98 to 2000 PRO.
-Loaded a new PC for with 2000 PRO.
-Tested new data drops that we ran to Gary Sanders office all is good.
-User Support;
That included loading additional software and troubleshooting
software/hardware glitches.
(Bruce Sears)
- General Ilog Maintenance:
(0.25 days)
- Added users.
- Fixed some incorrect log entries.
(Veronica)
- LIGO website: continued working on the Press & Media website.
Posting
editing/updates as they arrive.
Working on one of DCC database script modifications.
Posted updates to several pages (Fellowships, etc).
- Project Science website: tested a newer version of the website.
Incorporated some of the new graphics into the current layout.
- LSC website: updated MOUs pages.
- CaJAGWR website: posted various updates.
(Lisa)
- Working on integrating the sun crypto accelerator into becrux.
This is quite
complex because the card has its own openssl libraries that have to
be compiled
into the applications.
- Resolved a problem with the html configuration of the mailman archive
pages.
Internet explorer has a known bug displaying default URL's. I
also did some
more work with the perl filters for the archives.
- Worked on some wireless bandwidth problems on the 6th floor of Millikan.
Also
did maintenance on all of the access point configurations.
- Put in an order with the telephone office to convert the first two
lines of
the 800 number to ISDN.
(Larry)
- It appears that there are no more Maxtor 160GB 5200 rpm drives left
at a
reasonable price. Spent some time looking for them and so far no luck.
Working on a couple of laptop and Sunblade purchases.
The order for the GigE equipment to be installed at Livingston is in
the
procurement cycle.
- Cleaned up a couple of network issues. So far nothing major, mostly
workstations needing to be reset.
- Worked with Donna, Mike and Lisa on setting up a network and computers
for a
small conference being held here at Caltech. Assisting the users in
changing
their configurations for use on the network went smoothly in most cases.
- Worked a number of e-mail issues. Everything from user configuration,
updating
aliases, blocking and unblocking hosts to helping get needed information
for the
different mailing groups to update their lists.
- Checked out the power in the computer room and so far things are
looking good.
Also replaced the battery in one of the UPS units.
- Finally, got to spend some time working on the VRVS system. So far
the concept
of getting the presentations to broadcast directly on the VRVS broadcast
does
work but the resolution is poor. Now looking at some equipment that
may improve
the resolution on computer to computer capture system.
- Still working on various documents.
- Did some more trouble shooting for the DCC and a couple of other
PC
webservers.
From: ctorrie <ctorrie@ligo.caltech.edu>
Advanced LIGO
SUS
Mode Cleaner
I have been working on some optimisations for the mode cleaner prototype these week. These include a winch adjustment similar to that being currently used in LIGO I and pitch adjustment similar to the design used on the upmost mass in the MIT quadruple pendulum.
With the help of Russell Jones we have been looking at a 2x2 array eddy current damper for the Caltech triple pendulum. Drawings for a prototype version of this should be ready this week. There is a still a lot of work to do here before a set of arrays could be tested on the pendulum.
The library of clamps used to balance the blades have proved to be a success and the plan is to extend this set to 3.0 and 3.5 degree.
Mike Plissi and I have been keeping in touch this week and hope to continue work on investigating the set of cantilever blades that was started during his visit.
Recycling Mirror
We have made an introduction to the Recycling Mirror drafting in so
far as we have set up a space on the SUS 3D TeamWorks page and held introductory
discussions with the designers and draftsmen in Glasgow about what is required.
(The modelling, carried out by Phil Willems, is nearing a stage that
drafting and detailed design work can begin)
Synchrotron Lab
A drill press is being installed this week and some other material
removed in order to give us more room. Temporary storage units and a preparation
and checking table are ready to be moved in. The carpentry shop have already
been to measured up for the installation of shelves, lighting and some
tool storage.
From: Peter King <pking@ligo.caltech.edu>
2.1 Engineering and R&D
The free-running length noise of the optically contacted
pre-modecleaner was estimated by locking NPRO #259 to the pre-modecleaner.
This at least represents an upper bound of what the length noise would
be.
For frequencies less than 1 kHz, a factor of 2 to 2.5 improvement was
observed. At around 10 kHz, the length noise appeared the same
as that for
an epoxied pre-modecleaner. However the measurement from 10 kHz
and above
looks odd because it's flat, suggesting some noise floor rather than
the
true noise. Thus far I have not been able to track down the source
of the
noise floor. The lowest body resonance observed is around 13
kHz compared
to the epoxied body's 10 kHz.
2.2 AdLIGO PSL
Ivo Zawischa released another set of laser selection
criteria with
some minor changes. It looks like locking a pre-modecleaner style
cavity
to the candidate high power laser may not be convenient because of
issues
to deal with a suitable Pockels cell. This is the selection criteria
proposed to measure the beam quality of the 100-W laser. Updates
might be
discussed at the next Lasers Working Group telecon.
From: Janeen Romie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Worked on budgets and viewgraphs for the Tech. Review 10/8.
Working on Norna's questions for her PPARC meeting.
Working on mode cleaner tasks and setting up the lab with Calum.
From: "Mark Barton" <mbarton@ligo.caltech.edu>
This week I finished coding and debugging a set of
control system
models that I had been working on and published them on my models page.
There's on with a full LIGO-I-style diagonalizing controller, a simpler
one where the control signal for each actuator is derived from the
colocated sensor, and an eddy current version. All have detailed
modelling of sensor and actuator geometry, and, where relevant, the
ADC
and DAC converters.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Barbara and Maddalena leaving, back in Pisa.
Alessandro
Managed to low temperature braze over Ni-P electrode-less layer using
appropriate etchant and flux. The use of sputtering seems now superfluous.
Working on how to deposit thin, uniform and well localized layers.
Now we can think about building real structures.
Stoyan
Tested the new splat pistons. They do not work properly, apparently
the stems are too magnetic and the piston recoil before generating good
cooling. Need more thinking.
Running low on splat heads, ordered new alumina precipitation hardened
copper.
Working on simplified 2D flex joint model, finding problems.
Massimo, Mario (Pisa)
Finished LVDTs for new stress strain fixture, sending to Caltech
Maddalena, Barbara, Stoyan, …..
Splatting to generate more samples replacing the ones used in testing.
The splatter has grown unreliable. Riccardo tuned splatter mechanics which
now is more reliably and effectively producing glassy samples.
Barbara
Investigated on the two peaks identified in the DTA data before it
became unreliable. Confirmed precipitation of crystallites out of the alloy
on X-ray scattering of samples baked at temperatures (700, 750 and 930oC)
below, between and above the two peaks. Observed growth and narrowing of
the peaks for longer and hotter bakes. However some crystallisation was
observed even for oven temperatures lower than the first DTA peak. Realised
that the oven heating elements (white hot) directly irradiate the MoRuB
film sample and heat it up by black body radiation well above the nominal
oven temperature. Need to repeat measurements while shielding the samples
from the resistors black body radiation or eliminate the problem in some
other way.
Hareem
Still working on DTA tuning.
Maddalena, Allison
Found that Vickers hardness grows up to 16%, then flattens out. Observed
in literature that above 16% the fracture toughness decreases. The MoRuB
at 16-17% is the obvious working point for flex joints.
Three explanations proposed by Bill about the hardness growth followed
by the plateau.
1) there is not enough Boron to force full crystallization below 16%.
If true some crystallites should be present in MoRuB 14 and 15. The presence
of softer crystals would explain the lower hardness at low B concentration.
This possibility was rapidly ruled out by x-ray scan of the samples that
showed absence of crystals, well below the percent.
2) Boron is progressively filling the interstices between Mo and Ru
impeding interstice collapse under stress and rendering the glass stiffer
for growing B concentrations. Above 16% the excess of Boron would form
precipitates in the glassy matrix thus being ineffective in rendering the
material tougher, but introducing progressive fragility.
3) Same as before, but at B concentrations above 16%, after saturating
the interstices, a different stochyometry, Boron rich, glass would form
and make a sort of froth. The majority of MoRuB16 glass would be responsible
for the saturated hardness, while the froth of the second glass would be
at the source of the fragility.
Both theories are equivalent from the user point of view and indicate
the same optimal B concentration. It would be interesting though to distinguish
between the two.
Allison will repeat and confirm Barbara measurements in the following
weeks.
Xavier
Analysing heat conductivity data.
More work on flex joint shapes.
For additional information about this report, contact sanders@ligo.caltech.edu