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The LIGO Executive Committee Agenda for Monday March 11, 2003 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items: Status of S2,
Status of Upper Limits papers, Status of SEI prototype procuement
Task managers with budget remaining on Construction accounts have been requested to provide candidate lists of materials to be procured under the Construction Cooperative Agreement. These will be discussed during the Executive Committee Meeting on Monday, March 10, 2003. All Construction charges must be ready to be paid by June 30, 2003.
Ex Comm minutes next week
*** Construction Budget Issues ***
Task managers with budget remaining on Construction accounts have been requested to provide candidate lists of materials to be procured under the Construction Cooperative Agreement. These will be discussed during the Executive Committee Meeting on Monday, March 10, 2003. All Construction charges must be ready to be paid by June 30, 2003.
LIGO Weekly Site Telecon (Lindquist)
There was a site teleconferences held on Thursday, March 6, 2003. The following issues were among those discussed:
Livingston Storage Facility Inventory: A good list of the inventory in the storage building has been prepared. Ed Chargois will go to Livingston on Monday to identify with local staff the stuff to be excessed.
P-Card Procurements: LIGO is the only group on (or off) campus that has been authorized to acquire equipment on P-Cards. There is some concern regarding our ability to capture this material for the Caltech equipment lists. Ed Chargois has direct access to and is monitoring the P-Card database.
The expenditure type on fabrication accounts should always be "supplies allocable" regardless of whether the material is equipment >$5K or something else. This is a source of continued confusion. Means are being discussed to have all materials procured under fabrication accounts to automatically be identified as supplies allocable.
Ed Jasnow has an action (action 118) to discuss with with the P-Card
folks the need to update the documentation on the use of P-Cards.
LIGO is authorized to procure things using a P-Card that the rest of the
Campus has not been allowed to do. An list of exceptions needs to
be provided for the LIGO rules.
Petty Cash: A draft report has been prepared by Caltech Internal
Audit. It provides some recommendations, but lacks detail.
Ed Jasnow and Florence Kaufman, working with Fred Raab, have been given
the task (action 119) to prepare flow charts of the process for tracking
petty cash and to identify processes that Caltech should implement.
This improvement process will likely spill over into other control systems
that are not currently adequate.
Travel Reimbursement: Approximately 80 LIGO personnel have turned in the requested information needed to implement direct deposit of travel reimbursements. Roll out of the system by Finance has been deferred from April 1 to May 1 due to "software issues."
The list of current actions revised to reflect
the status of open actions assigned through March 6, 2003 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
| WE 03/06/03 | Packages | Faxes |
| In | 42 | 38 |
| Out | 13 | 45 |
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)
>Irene Baldon
Accomplishments:
Out of the office the 28th, 3rd, 4th, and 5th.
I have been working on setting up my upgraded PC. Installing software, network connections, etc.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
The Advanced LIGO Proposal has been submitted to the NSF and most of
the follow-up paperwork has been prepared and sent. The Office of
Sponsored Research is working with MIT to get a certification identifying
David Shoemaker as a Co-PI..
Change Request CR-030002 to adjust the FY 2003 operating
budgets to reflect actual staffing during the first quarter has been prepared.
We will update this request at the end of March to reflect a full six months
of expenditures. Meanwhile, we are reviewing the costs anticipated
for the remainder of the Construction Project (before June 30, 2003), and
a number of Change Requests will be prepared to close out the Cooperative
Agreement.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
No report this week.
Summary of S2 Science Run Activities at LIGO Hanford Observatory (compiled
by M. Landry)
---------------------------------------------------------------------------------------
Cumulative duty cycles of the two IFOs remain
stable, in the mid sixties. Efforts are
being made to understand the periods in which
we do not lock (sometimes long hours on
H1). Establishing the causes for long mean-times-to-lock
is seldom clear, and difficult
to distinguish from simple misalignment.
Tuesday saw the crash of the T3 disk system, LDAS, and the fb3 framebuilder.
G. Mendell
and D. Barker worked to restore the system within hours. The
loss of a significant
amount of DMT trend data means monitors will be rerun to recalculate
the trends. Some
3000s of full data was lost.
High winds returned Wednesday and Thursday, limiting duty cycles on
both IFOs. 2k MC
offsets were shown to be due to radiation pressure:
http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=03/04/2003&anchor_to_scroll_to=2003:03:04:19:04:20-daniel
New H1 lock record: forty-one hours.
S2: The interferometer runs well at night. We continue to have a duty factor of about 43%, dictated almost entirely by seismic noise. Wednesday night and early Thursday morning was the most sensitive run yet, due to a decrease in the low frequency noise. We were able to accumulate several hours of data with a SenseMon range of 1.2 Mpc. As this report is being prepared, we are recovering from a site-wide power outage of a few seconds due to a severe thunderstorm in the area. We are slowly restoring the operation of all of the computers and electronics on the site.
LDAS admin
1) Restored databases after the crash at LHO.
2) Applied patches to LDAS Solaris machines at LLO.
3) Received L700 tape robot today.
LDAS data analysis.
Studying sensitivity of Waveburst on S1 playground data by running
simulations with injected signal.
Igor Yakushin
GC: Fixed some print problems on the building controls computer. Installed some security patches on our mail server and several other machines in response to the new sendmail vulnerability. I still have a couple of machines to patch. Ordered a laptop for Chethan. Ordered a Matlab and compiler license for Chethan. Working on getting me listed as the contact name with Mathmatica and Matlab instead of Tom. I will also be the name on record for all of the licenses with Wolfram and Matlab. Working on some projector problems. We tried a new projector in the control room and the bulb blew after a few days. These projectors are not designed for continuous use, but I am concerned that the bulb blew after ~100 hours. However the display quality of the projectors seems to be superior to the LCD. Installed some wireless access points in the new building and in the auditorium. This should provide coverage to all of the office areas. Working with a contractor to get an audio conferencing device installed in the auditorium. This will provide the audio for any video-conferenced presentations for the LSC. Have a Canon rep that is supposed to send us a demo of a visualizer so that we can try it out during the LSC meeting. He has two models and I am not sure which one he will be able to send us. Doing lots of prep work fo rthe LSC meeting. Hooked up some of the network jacks in the new building. Discovered a problem with the sendmail configuration after the patch. I am still working on this issue. I believe that the mail server may now be acting as an open relay. This is not good and needs to be taken care of ASAP. Ordered a rack style cabinet to go in the auditorium. The delivery does not look good on this item though, so I may have to find another solution.
Site Issues: An order to stop work on the LLO staging building, as well as all other work on site, was hand delivered today by Ray Terral of the Livingston Parish Building Department to the site. Ed has been informed and has counseled us to continue work and he will consult with Sandy Pool. Craig Sauviac, the architect of the build out, has also been informed and a copy of the letter and marked up drawings delivered to him for his analysis. (Sibley)[ GHS note: After brief review, we have decided to stop work and to consult with the Livingston Parish Building Dept. re requirements to resume work under their new rules.]
Seismic Amelioration: Work on 3D digital content continues. I hope to
have a scheme that will illustrate the different beam piers by next week
(i.e. short tube-HEPI/MEPI or long tube-LIGO 1 for HAM and HEPI/MEPI or
LIGO 1.) This will make the search for the different configurations much
easier. I have also revisited efforts to summarize doubelstart counterwound
spring analysis. I took one SCI-Mon training shift last Friday and will
be taking two this week. I feel that this is important to help me familiarize
myself with the interferometer. Marcel
A design review is planned for early to mid April and will be announced soon.
This week I chased after bugs in the Name service,
Data tunnels and Data
quality monitor. I found an error in the handling
of buffers in the tunnel
code that may have resulted in the Tunnel stalling.
I also fixed a bug in
the script used to enter remote addresses into the
local name server
e.g. so the lock state in L1 is visible at LHO. I
also found and fixed
an error in the DataQual configuration file and then
fixed the PSLmon
program so (a) it was about 25% faster than before
to reduce the CP load,
and (b) made the glitch finding tool immune to the
loss of frames cause by
the heavier CP load with the corrected configuration file.
1) Continued work on using a PC in conjunction with
a VME crate to run the
suspensions on the 40m. We pretty much have a full
system running now and have
done some initial testing. It looks like on the VME
side, we can do all the I/O
plus data acquisition for 8 optics with one VME crate.
There is no longer a
distinction on the VME side of large or small optics,
so we can run all 40m lab
vertex optics with this one crate. The fact that the
VME crate also does handles
all the DAQ channels (sensor/coil readouts) eliminates
the need for a separate
DAQ VME crate.
On the PC side, it look like one 2.5GHz P4 box can
run all the control
algorithms for 5 optics and still get its output to
the VME unit in time. We ran
it is high as 6 optics, but I/O timing with the VME
unit became border line. We
have ordered a dual 2.8GHz Xeon processor unit, which
should be in late next
week. We hope to be able to run all the 40m
lab optics (10) with this one box.
In the course of the next week or two, we need to
do some finishing and clean up
work on the software. This includes getting all the
white/dewhite and
run/acquire switching in. We also want to use
this system to test if we can
trap ICS110B ADC channel hopping (by forcing it to
jump). If we can trap it in
some fashion, then this trap code would be also applied
to DAQ and watchdog
timer software.
2) After spending a lot of time concentrating on the
I/O for the suspensions,
have come across a number of ways to improve I/O in
the LSC system. Much of the
time was spent plodding thru the 300 page manual for
the VME I/O bridge chip
used on our VME processors and descriptions of its
hundreds of registers. In
short, we are now able to setup this VME I/O chip
to do most of the VME I/O at
that same time that the LSC filter processing is going
on. In this fashion, we
were able to drop the LSC overall cycle time to ~30usec
(reading in 24 sensor
channels, no GDS signals selected) and ~42usec (5
GDS excitation and 10 GDS TP
selected). With a little more work, I could probably
hide most of the GDS stuff
in the background as well.
Now that overall speed is up, I will add in the filter
banks, etc. for the 2
remaining AS photodiodes (for a total of 4). We will
then test on the 40m (at
least the VME with connections to DAQ and AWG) in
a couple of weeks.
3) Working with Jay to test the new DAC module from
Frequency Devices and the
Pentek module which was fixed to get rid of the DAC
glitches.
4) We shipped our RaidWeb disk drive unit to LHO to
replace theirs running on
the backup framebuilder (fb0). Their's had failed
and it became important for
recording trend data when the LDAS T3 system had problems
and we switched to fb0
as the primary framebuilder. These RaidWeb boxes haven't
proven to be very
reliable, so as a minimum, we should consider getting
something better for our
backup framebuilders.
Jay Heefner reporting
Frequency Devices DAC: The prototype module has been received from FDI and testing has been started. We should know if the module meets spec in a week or so.
Pentek DAC Glitches: A module has been returned from Pentek with the modifications made. Preliminary indications are that the fix may indeed eliminate the glitches.
RFI Upgrade: Two evaluation racks have been ordered from both Knurr and Equipto. They are scheduled for delivery to LLO in mid-April.
Sander Liu
Testing of the refurbished microseismic signal processor is complete. We are waiting for the STS-2 mating connector from Newark to replace the wrong one currently on the chassis.
The crystal parameters for a 14.75 MHz crystal were
measured. The
crystal will be installed into an oscillator, so that
I can resurrect a
resonant Pockels cell. The old NIM-based oscillator
was loaned out some
time ago.
A few minor additions were made
to the PSL Lab cross-connect to bring it
up to the current configuration at the observatories.
This will facilitate
testing of the intensity servo. Updates were
also made to the EPICS
records database.
The SPARC-20 in the PSL Lab was replaced with an Ultra-1.
Thanks to Larry
and Lisa for help in getting the workstation up and
running, as now we can
pull up the MEDM screens in the usual manner.
I toyed with a schematic for a high-power, low-noise,
normalized quadrant
photodetector.
AR coated aluminum baffles are being developed, as
an alternative to using black glass. The aluminum baffles will be mirror-polished
to obtain low-scattering comparable to the black glass baffles and will
have an absorptivity at normal incidence of 95 to >99%, depending upon
the chosen efficiency of the AR coating. The aluminum baffles will have
high thermal conductivity to dissipate the heat of the absorbed laser beam
into the HAM table.
I’ve been in contact with Doug @LHO on locations and other information, and Dave Reitze in Fl. Re. his beam dump. Gathering information on materials, vendors, and processes to complete this in the time available. The count is: 15 SOS baffles, 3 LOS baffles, 3 IO baffles [2 part ea.] and 3 beams for the reflected beam from an intentionally mis-aligned RM..
OTF Lab. (W. Bridge)
Contamination Cavity # 1
With a new test sample. CHEM-SOL Hydraulic fluid
We are taking ring down and beat frequency measurements everyday.
Liyuan is working on the graphs for absorption, ring down and thermal
lensing.
Absorption Test Measurement prototype is in STANDBY.
Scatterometer
We have recovered the function of the scatterometer. Laser beam
alignment has been completed.
We have run a simple test to map the scattered beam from the coated
surface of the existing ETM.
We are continuing the work to fully have the system working because
we are missing some
equipment which we are looking for.
OTF Lab at Lauritsen ROOM 38
Cavity #3
The new test sample from Leander Lubricants
CHEM DRAW’ # HSF-75-2, Batch 12302001. (a synthetic, hydraulic fluid.)
with different additives. still pumping down.
We are taking ring down and beat frequency measurements every day.
Liyuan continues to graph absorption, ringdown and cavity thermal lensing
measurements.
Cavity #2 Test cavity
The chamber is pumping with new cleaned mirrors ~ 70ppm each.
RGA measurements, optical train set-up in progress.
New NPRO laser installed (M126-1064-700 S/N 414) and it is in operation.
Below is the latest sensitivity curve for the TNI, obtained with our newly tuned photodiodes and some moderate suppression of scattered light. (We were able to reduce the scattered light contribution, but we have not yet been able to eliminate it.)
Notice that NAC's noise floor has come down by quite a bit between 300 Hz and 10 kHz. Around 1 kHz the improvement is about a factor of five. The two arm cavities now have identical noise floors from 10 to 50 Hz, and from 300 Hz to about 20 kHz.
no report
Simulation and Modeling (Bhawal)
E2E Physics meeting
--------------------
We discussed the various peaks and bumps in current sensitivity curves
from all IFOs and their possible origins. The structure in the 90-100hz
range
originating from the WFS system and in the 20-25hz originating from
mich signal
were discussed at length. There was also discussion if errors in nspob
light measurement due to BS alignment adjustment could be the reason
behind some discrepancies in calibration.
SimLIGO Noise Curve
---------------------
(Matt) Working to understand the SimLIGO noise curve. Currently studying
the bilinear/non-linear coupling of noise to high frequencies
(greater
than 200Hz) that results from low frequency deviations of AS_Q
(typically generated by seismic motion). Also looking into DAC
and ADC
noise couplings in the presence of WFS and QPD alignment/centering
servos.
Code development and maintenance
---------------------------------
(Ed Maros) Helped Biplab with installing e2e on his laptop.
(Melody) Continued working on optimizing the modeler's functions analyzer.
Alfi
-----
(Bruce)
- Debugging new implementation of junctions.
LIGO Data Analysis System
Software Systems (Blackburn)
A new version of LDAS was pushed to the sites this week. LHO and LLO
are now
running version 0.6.20. We will later today be installing this version
on the
LDAS TEST and CIT systems. This version does not fix the frameAPI core
dump
issue, but it has an improved reliability in the mpiAPI (back to the
levels
seen in S1 of less than 1 failure in 10000). The diskcacheAPI should
be a
bit better in its performance also. The main motivation for installing
this
version at the sites was to overlap with the Solaris Operating System
Upgrade
requested by the LDAS Hardware Group so as to minimize the number of
times
and duration of down time for LDAS at the sites.
Unfortunately, the night before the scheduled upgrade, the LHO LDAS
system
suffered a major hardware failure. One of the most critical T3 RAID
boxes
crashed causing the loss of the LDAS database and the loss of metadata
for the
full complement of T3 RAID boxes at the sites. Fortunately we were
able to
recover the database but our 3 hour scheduled down time was stretched
out to
about 8 hours. In addition, the procedure used to restore the database
at the
sites required us to introduce an alias for the database to get everything
back to the state necessary to run jobs which use the database. Unfortunately,
this alias is not mapped into the user space of utility programs used
by our
database webpage generation tools so the webpages were not visible.
We have
now added a secondary (external to LDAS) application tool to generate
these
webpages until the database itself can be properly constructed without
the
new alias.
LDAS is now fully functional with the SAM/QFS tape storage system here
at
Caltech. It is now possible to issue job requests to LDAS which require
moving data off of tape first. This is all transparent to the user
with the
exception that it takes longer for jobs to run when requests require
reading
data off of tape. This experience has given us several ideas for ways
to fine
tune LDAS to better work with a tape storage unit (pre-staging of data
for
example), but the fact that it works is most obvious in our ability
to create
the RDS frames from the S2 raw frame data stored on tape!
We think we may now have finished the removal of all variable names
using the
reserved namespace of _* and *_t from LDAS and the objectspace C++
library.
As reported last week these are reserved for compiler variables and
should
not be part of user code. It is estimated that more than 500 files
in LDAS
had to be modified to make this change. Only time will tell if this
clears
up any long standing issues that have been difficult to fix in the
past.
We also think we have a clue about the source of the frameAPI core dumps.
On the LDAS-DEV system we have not seen these core dumps in roughly
4 weeks.
However, they happen regularly at MIT and on weekends at the sites.
We have
traced these failing systems to be related by the use of RDS frames
in jobs.
In addition, there is a strong tendency to have the same RDS opened
more
than once in these systems. This provides important clues in the part
of
code that needs to be reviewed in searching for the bug.
We have set up a tandem LDAS system using two test boxes to better simulate
the conditions associated with the core dumps in the frameAPI and provide
a
test platform for code experimentation in order to accelerate our search
for
the problem lines of code.
We are working on an asyncronous lamboot handler for the mpiAPI which
will
greatly reduce the time needed to start up LDAS on large clusters.
As with previous weeks, we have continued to support the science run
whenever
the need exists.
(Philip Charlton)
With Stuart's help, got the DSOrun web page up and running on the
ldas-jobs machine. Commenced producing reduced data sets for LLO and
LHO.
So far we have reduced 36 hours of LHO and 70 hours of LLO. The poor
rate
is due to a number of factors:
- slowness of getting data from tape
- processing time is more than real-time, especially for large
LHO files
- problems with the RDS script. It does not deal efficiently
with cases
when the output data files are already found to be in the output
directory. May need to update to Greg's new script.
Worked on problem of ",," vs. ",_," in output() action. These should
both have the same behaviour, but didn't. I tested Phil's fix on ldasbox1.
It fixes the problem but introduces a new one, since now it produces
two
identical result files, thus renaming the old one with .bak. (No changes
have been put into CVS yet).
Worked on memory leaks in datacon. Running a single script over many
hours on ldasbox1 seems to indicate that there is a leak in either
the
psd() action or in code which outputs the result of a psd().
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Received and installed permanent SAM-QFS (with 6000 tape slots = 1,200,000
MB) license
on ldas-archive.
* Exported all tapes and re-imported them in bar code order. Verified
that tapes that SAM reported as unused in fact had no data on
them (a
bug in the auditslot program causes a completely unused [no
header]
tape to show that it is 100% used). Dealt with media errors
and
unlabeled tapes that were reported during this process.
* Continued archiving of S2 data.
* Monitored SAM-QFS system while it was both archiving new S2 data and
staging back from tape data that was being requested by the
CIT system's
frameAPI.
* Determined the exact syntax/behavior of the SAM-QFS stage command
to be
used in the diskcacheAPI so that it could give a "hint" to the
SAM-QFS
software about which files would be needed shortly.
* Assisted in the recovery (primarily running samfsck and remounting)
of
the QFS filesystems at LHO after a T3 failure.
(Al Wilson)
* Got the graphing plug-in working in BB. But just one small problem,
it
generates tons of email!! So it is still a work in progress.
* Moved Moe (replacement for m90) into rm 602. M90 is still on-line
* Trying to get some beta software from 3ware. They tell me that it
will
allow monitoring of the raid assy from the command line. (we
will see)
* Had a V880 (dev system - Dataserver) with our old friend the memory
problem. Sun replaced 3 Dimm's They tell me that they
will have a FIN
soon.
(Stuart Anderson)
* Tested Solaris 9 kernel patch and found it to solve the slow NFS
performance from Linux NFS servers.
* Upgraded all of the LDAS Solaris servers at Caltech (except ldas-sw)
to the latest recommended patch cluster.
* Continuing to archive S2 data into SAM-QFS and monitor its performance
when it is overloaded with multiple read and write requests
with the
current configuration of only two tape drives. It has run very
well
under these circumstances.
* Rebuilding many of the desktop applications in /ldcg with the new
gcc-3.2.2 compiler to stay in synch with the compiler used by
the
current development release of LDAS (0.6.20).
MIT
---
(Keith Bayer)
* Moving/deleting data to make room for S1.
* Investigating LDR.
* Finishing up network troubleshooting diagnostics.
* Getting last quote for pc raid from Aztek computing.
* pc raid scsi timeouts apparently fixed (molex power cable loose).
Livingston
----------
(Igor Yakushin)
* Restored databases after the crash at LHO.
* Applied patches to LDAS Solaris machines at LLO.
* Received L700 tape robot today.
Hanford
-------
(Greg Mendell)
* A failure on a LDAS Sun t3 occurred just before 14:19 PST on Mar 04
2003. At this point fb3, DMT trends, and LDAS lost the
ability to access the LHO T3 disk cache. The
failure mode was that t3-26 froze -- a previously unseen and
unexpected failure. I tshoudl be noted that over the year-plus we have
ahd the T3 caches a number of drives have failed with no consequence. This
particular failure mode was pernicious in that an entire ARRAY of T3s froze
all at once. No server
could see the disks on this t3 (i.e. via ls, df, format). One
could not
ping or telnet to the T3 unit.
At first inspection all disk lights were green; however the RAID
controller board light "on line"
light on the back of T3 was amber. (A steady amber light indicates
the
controller is in the middle of a shutdown, reset, or reboot).
After
umounting disks from servers, the T3 was power cycled.
The disk lights
on disk 1 went off for a few seconds, while the "on line" light
changed to
green. The "on line" light then went amber again,
and disk 1's lights changed to
green. The T3 was power cycled a second time. This
time the "on line" stayed
green, but disk 6 started blinking its amber light, indicating
a disk failure. All other disks,
including disk 1, remained green. The T3 was reset, and it returned
to
this same state. A fru stat showed disk 6 was missing.
After 20 or so
minutes a fru stat finally showed a fault on disk 6. This is
what we had seen in past disk failures.
At this point the T3 was once again accessible. Mendell
ran fsck from metaserver on these
disks. while Dan Kozak (from Caltech) ran the qfs version of
fsck on other disks that had
the QFS metadata on T3-26. (Because the QFS metadata was
on T3-26, I/O on
all other 20-odd T3s failed when this single unit failed).
Unfortunately, some of the
directories undergoing I/O at the time of the failure were lost,
include
many of the DMT trends from the beginning of S2. Very
little raw data
was lost (and this was due to a prior, unrelated failure on
the CDS RAID box
attached to fb0, see below).
Sun replace the failed drive (drive 6) on T3-26 this morning
(03/06/03)
and suggested we apply firmware patch 109115. Sun believes
T3s have
been known to hang and show resets before this patch version.
However,
it was not clear from the syslogs that the T3 had tried to reset
at the
time of the failure. Also, we have had four or five previous
disk
failures on the T3s at LHO without incident. (These are RAID
5 units
that are designed to keep working with a single disk failure.)
Of course,
we will apply the firmware upgrade the next opportunity we have.
All the T3s were back up by Tue 04 2003 evening. The ldas
database had
to be restored at LHO (by Igor and Caltech). We also applied
planned
Solaris 9 patches to the LDAS Sun servers, and LDAS installed
a patched
version of its software. LDAS was backup by Wed 05 2003 evening.
* Notes on raw data lost:
When the T3 disks crashed fb3 lost its disk cache. It took
6.6711 hours
to get the disks back up, and fb3 was down during this time.
However,
fb0 uses independent disks, and kept on acquiring data and building
frames. Barker removed
fb3 from the state vector that determines science mode. Mendell
switched the
tapecontrol script to get its data from fb0 instead of fb3.
Thus, all the raw data
during science mode stretches has been recorded on tape.
This data will
appear at Caltech. However, fb0 overwrites its data every
13 hours, so
it is no longer on disk. Having recovered from fb0 the
missing data
from fb3's 6.6711 hours of downtime, the tapecontrol script
is once
again getting it data from fb3.
Dave Barker writes:
Summary of data available on fb0 and fb3:
fb0 only lost full frame data between:
Mar 4 14:42 H-R-730852928-16.gwf
Mar 4 15:38 H-R-730856272-16.gwf
[Note the reason for the missing fb0 frames is that it had its
own independent RAID
failure a day or so before the T3 failure andwe could
not write minute
trends. Dave tried to fix that when fb3 went down.
Thus, there is a 3344s
gap when both fb0 and fb3 were down and no frames could be created.]
fb3 lost full frame data between:
Mar 4 13:04 H-R-730847056-16.gwf
Mar 4 19:44 H-R-730871072-16.gwf
Lazzarini note: obviously this was a painful lesson
and we are studying the experience to guarantee this failure mode does
not get us a second time.
The planned upgrade to SAM-QFS and 6mo-12mo robotic
lookback at each site that will become avaialble shortly after S2 ends
should eliminate the risk to which we are presently exposed.
Data Analysis Activities (Lazzarini)
Weinstein:
- Continuing to study hardware burst injections.
- Continuing to study the effect of HPF, whitening, and
base-band filtering in datacond.
- Monitoring S2 online burst searches.
- Compiling a list of systematic errors associated with
the S1 untriggered burst analysis.
Mendell:
I've been busy with S2 scimon shifts and working on hardware failures.
However, I hope to start generating SFTs with the knownpulsardemod
DSO
soon.
Kaice Reilly:
Last Friday I finished the time-frequency CC maps.
I have begun to make the CC maps an optional part of the
upper limit analysis. Joe and I spent some time discussing
the next step. We, as well as others have concluded that
it will be interesting to look at a difference of the CC value
and the expected value or a ratio of the two. It is prohibitive
(time-wise) to generate a full map of this difference or ratio, so
I will most likely only do it for one job. We assume that this
will be ok because the CC maps indicate that the processes
are "constant" over the S1 run. I have been reading through
the LAL wrapper documentation and the relevant papers
in order to get a better understanding of the details involved
in the stochastic data analysis.
Yakushin:
Studying sensitivity of Waveburst on S1 playground data by running
simulations with injected signal.
General Computing (Wallace)
MIT:
(Keith)
-Troubleshooting Tania's desktop (memory errors)
-Troubleshooting Erik's desktop (hdd errors)
-Setting up a new user (Jon Allen) on gc and spare laptop
-Spec-ing out new laptop for Jon Allen
-Patched sendmail on all gc computers
Livingston:
(Shannon)
-Fixed some print problems on the building controls computer.
-Installed some security patches on our mail server and several other
machines in response to the new sendmail vulnerability. I still
have a
couple of machines to patch.
-Ordered a laptop for Chethan. Ordered a Matlab and compiler
license for
Chethan.
-Working on getting me listed as the contact name with Mathmatica and
Matlab instead of Tom. I will also be the name on record for
all of the
licenses with Wolfram and Matlab.
-Working on some projector problems. We tried a new projector
in the
control room and the bulb blew after a few days. These projectors
are
not designed for continuous use, but I am concerned that the bulb blew
after ~100 hours. However the display quality of the projectors
seems
to be superior to the LCD.
-Installed some wireless access points in the new building and in the
auditorium. This should provide coverage to all of the office
areas.
-Working with a contractor to get an audio conferencing device installed
in the auditorium. This will provide the audio for any video
conferenced presentations for the LSC.
-Have a Canon rep that is supposed to send us a demo of a visualizer
so
that we can try it out during the LSC meeting. He has two models
and I
am not sure which one he will be able to send us.
-Doing lots of prep work fo rthe LSC meeting.
-Hooked up some of the network jacks in the new building.
-Discovered a problem with the sendmail configuration after the patch.
I
am still working on this issue. I believe that the mail server
may now
be acting as an open relay. This is not good and needs to be
taken care
of ASAP.
-Ordered a rack style cabinet to go in the auditorium. The delivery
does
not look good on this item though, so I may have to find another solution.
Hanford:
(Christine)
Nothing to report.
CIT:
(Mike)
-Pulled out some temporary mini switches in the third floor closet
and
swapped them out with a replacement edge switch for Larry.
-Cleaned up a laptop for the loaner pool and have it ready for the
next
prominent user.
-Setup for a meeting using the new VRVS software 3.0 that is recommended
by VRVS technical support group to their updated software for VRVS.
I did
this but came across multiple problems and couldn't get the audio or
video
due to runtime errors and other unknown OS errors. I did get the video
to
work, but had to run the audio on our backup computer. I need to work
on
this some more to be ready for the next meeting.
-Reloaded Thomas Frey's computer that was running win98 that was having
multiple software problems that I corrected until I could have the
time to
update his computer to 2000 Pro & a hardware upgrade. This operation
is
complete and is back up in his office.
-Had a lot of tech support that included email, networking & printing
issues; plus loading additional software for some users.
-Pictor, I had to update the flex LM license server for Ansys software.
Amaldi, I compacted the database.
(Veronica)
- LSC website: continuous updates of the March meeting webpage as the
new
information arrives. Generated and posted an expanded and printable
version of the agenda.
Rewrote and posted pages for the spokesperson voting. Updated Talks
page.
- LIGO website: extensive work on videos of Rita Colwell's presentation
at
AAAS. The original files were encoded using a codec that was missing
from
the libraries of both RealPlayer and QuickTime, so no playback was
possible. Downloaded the codec and compressed the three videos for
3
various bandwidths each to ensure easy access. The videos are now posted
with the rest of AAAS presentations. Investigated a possible problem
with Rai Weiss' file (it appears to be on the user's end).
Working with George and Linda on modifications to the DCC database;
the
backend changes will include a new layer for restricted-access documents
for various workgroups.
Working with Digital Media Center on digitising LIGO VHS tapes; tested
the
newly encoded batch on our camcorder.
Posted various updates throughout the website.
- CaJAGWR website: recorded and compressed the talk by Braginsky. Working
on the smil combo of video and synchronized visuals. Posted updates
at the
website.
- Planning for redesign of the Advanced LIGO website.
(Lisa)
- Patched a sendmail exploit on acrux and becrux.
- Installed licensed copies of RAV milter on acrux and becrux.
Began
looking at ways to customize RAV to do better spam blocking.
Currently, it is
catching about 500 spams/day.
- Finished the inventory of active sun workstations and servers.
- Did a full system dump of canopus.
- Did monthly backups.
- Contacted opengroup about a quote for motif. Opened a discussion
with
ITS about purchasing a caltech site license for motif.
(Larry)
-Plenty of procurement related items. The Foundry maintenance contract
renewal has to be retransmitted. Helped a number of people on getting
quotes for different systems and related equipment.
Lisa is working the Motif issue. The edu site license appears to be
the
way to go at this time.
Received the licenses for RAV which Lisa now has installed.
Received the licenses for the Calcium calendar tool. Checking out
additional functionality for that tool. Our site license allows unlimited
users but it can only be installed on one server.
-Helped out the DCC on a few items. Requests for additional functionality
is being checked into.
-Worked a number of security items.
Most of the mail servers on the project have had the necessary patches
installed. Lisa was able to get the CIT servers patched with limited
down
time.
Updated virus-scan on a couple of PC's and cleaned up a couple of
machines.
Ten+ sites a day are being added to the e-mail block list.
-So far at the security conference copywrite issues has been one of
the
hot topics. The Gov't is taking the lead in a number of items but they
are
also working closely with industry and global partners. Global network
security has become a high priority.
----------------
The Advanced
LIGO Proposal was submitted to the NSF; the proposal will be posted soon
to the LIGO Web Page. The system proposed follows very closely the baseline
with which we have been working, including 3 interferometers (two in
Seismic
Isolation
Busy with
pre-isolator work
Suspension
DHS
note: this week we have the Suspensions Working Group report which amplifies
considerably on the Suspensions report.
From:
Jay Heefner <jay@ligo.caltech.edu>
Adv
LIGO SUS
===================================
-
Drawings for the RM prototype test stand have been started and should be
complete by next Friday.
From:
"Mark Barton" <mbarton@ligo.caltech.edu>
The
last few days I've been at LLO working shifts for S2, but before
that
I investigated two last-ditch strategies to salvage some of the
magnetized
stainless steel OSEM coil formers. initially
we hoped that the
magnetism
might be from EDM machining which typically only affects an
extremely
shallow layer that can be taken off with electropolishing.
Stefano
of Riccardo's group has been doing such
work so I liaised with
him
about treating a test sample. Unfortunately we later concluded that
most
of the magnetisation was produced by extreme
heating from a blunt
conventional
drill that was used to make the central cavity (after
removing
the circuit boards one can see scorching and scoring). We tried
having
the hole enlarged with a sharp tool, which made a noticeable
improvement
but not enough.
From: JaneenRomie
<romie_j@ligo.caltech.edu>
AdLIGO
Suspensions
We've
been working on validating Dennis's mass budgets (seismic payloads), submitted
to all prior to the Systems meeting on 2/27, in support of the seismic
RFQ. This work is ongoing. Larry Jones is providing some much-welcome support.
I've
just redlined the mode cleaner RFQ and will get it to Gina and Ruth tomorrow
morning. I need to change the parts quantities in the Excel spreadsheet
and make some more changes before giving it to them to include in the RFQ.
The
recycling mirror suspension design is progressing well, due to Michael Perreur-Lloyd
hard work. We had a meeting Monday and this morning about this design.
We will be increasing the footprint from 300mm x 400mm to 300 x 480. Due
to the small clearance under the RM optic, we are considering petitioning
for a beam height increase.
Luke
has sent us his AutoCAD AdLIGO input optics
layout so we may review it and compare it to Dennis's layout from 2/27.
I
have proposed to the suspension group that we postpone the mid-April LASTI
MC prototype practice installation. Other
tasks have higher priority, such as the LIGO 1 earthquake stop redesign,
the review of the seismic payloads and the pre-isolator work.Rather
than spending time cataloging, cleaning, baking and assembling mode cleaner
parts, this will allow us to take time to work on improving the reliability
of the hybrid osem design. It will also
allow us time to look at ways to stiffen up the MC structure design. To
support this, Caroline Cantley will be
visiting Caltech April 8-16.
We
spoke with Russell Jones about the hybrid osems
this morning. He talked to his vendor and hopes to get a quote for the
rework sometime soon.
We
have a meeting with Linda Turner tomorrow to talk about our configuration
management needs, hopes and dreams. I'll provide a matrix of the software
compatibilities that I know of at this piont.
Gin Gin
LIGO
1 Earthquake Stops
Doug
and I are going out for quotes for the components of earthquake stop design
that Mark Barton is currently testing. Mark feels confident that with a
bit more testing that the design will meet the requirements. We hope to
have a review at the end of March.
From: ctorrie
<ctorrie@ligo.caltech.edu>
Advanced
LIGO
MC
Hybrid
OSEMS made from aluminium and then anodised
are being considered as an alternative to using 300 series stainless. At
the same time we have been looking into annealing the 300 series stainless.
RM
Mike
Lloyd and I have been working on the 3D layout of the masses with a structure
for the recycling mirror suspension.
http://www.ligo.caltech.edu/~ctorrie/RM/RMsuspension.html
Work
has continued on the modelling of various
aspects of the design with help from Norna
and Caroline and Mike Plissi in Glasgow
and LukeWilliams
at the
Virtual
Conference room and file sharing
Working
with Linda Turner and Veronica, Mike Lloyd, Janeen
and I have held a couple of meetings to discuss the various options that
are available on the market place for file exchange and virtual conferencing
and how all of this could be linked to an updated DCC in the future.
From:
Helena Armandula <ahelena@ligo.caltech.edu>
Silicate
bonding
The
SF4 / Fused silica bond (SF4-5) loaded in shear with 10.5kg broke apart
after ~12 days. There was glass pulled on spots around the edge, however,
there was not signs of bonding over the rest of the surface.
A
new bond (SF4-9) has been loaded with 10.5 kg. This bond was made with
newly bought sodium silicate solution; it has been loaded for
5 hr.at this writing (Wed. 5th)
The
SF4 / fused silica bond (SF4-1) being pulled with 26kg (tension) is still
holding. It has been under continuous tension for ~47 days and at one point
it was heated to 33 degrees C for 24 hr. There was
not signs of stress with the increase in temperature.
SUSPENSION
WORKING GROUP REPORTS
SWG
Update for HWS (Steve Penn)
------------------------------
Coating
work:I had a minor delay this month
because the
suspension/isolation
system (bob/fiber chain) had to be replaced because it
had
been damaged.This is now complete
and the annealed alumina/silica
sample
is installed.I plan to take data
on this sample on Thursday and
Friday
before I leave for LLO.Hopefully
I will have results by the
telecon.
Also
after a protracted LSC review (9 weeks) our coating paper was finally
returned
to us.It has now been submitted
to Classical and Quantum Gravity.
Anyone
wishing a preprintcan
email me (penn@hws.edu) or grab a preprint
(low
quality graphics) from arXiv (http://arXiv.org/abs/gr-qc/0302093)
Silica
work:Our original annealed fiber
sample has now been repeatedly
measured
and we have confirmed the high Q of 200 million.A
second sample
has
been annealed and is currently being measured.I
hope to have
preliminary
results by the telecon.Unfortunately
a mishap has occurred in
this
experiment as well.The quartz furnace
tube in which the annealing is
performed
has been damaged.It will require
repair before the next fiber
sample
can be annealed.
I
have also completed and submitted a CRDF grant proposal with Boris Lunin
of
collaboration
on experiments on loss in silica.Lunin
has done extensive
work
on annealing, temperature dependence, surface preparation, and surface
loss.I
think he will be an asset for the silica program. He is also quite
excited
about our recent annealing work.
Classes
and conferences have eaten up all the rest of my time.
--------------------------
CIT
Suspension Report
[This
is a condensed form of an e-mail I sent out 3/4 that most of you have seen w.r.t.
the AdLIGO suspension testing schedule.]
For
the last few months, we've been pursuing the goal of sending a mode cleaner
suspension
to LASTI for a practice installation in the second week of April. In
reviewing
the activities here at CIT required to meet that schedule, we've realized
that
we will have to let other tasks slip.In
considering the work required to meet the priorities Dennis provided, I've
concluded, and I think a number of us here at CIT agree, that the April
LASTI visit must be postponed.
The
LASTI MC cannot be tested in a pre-isolated chamber until the seismic group
has completed their testing, which Dennis and David assess will be, optimistically,
early May.
Rather
than spending time cataloging, cleaning, baking and assembling mode cleaner
parts,
this will allow us to take time to work on improving the reliability of
the
hybridosem
design. It will also allow us time to look at ways to
stiffen
up the MC structure design.
---
Caroline Cantley
has confirmed that she will join us in mid-April here at CIT. We look forward
to her visit.
The
recycling mirror suspension design is progressing well, due to Michael Perreur-Lloyd
hard work. We will be increasing the footprint from 300mm x 400mm to 300
x 480. Due to the small clearance under the RM optic, we are considering
petitioning for a beam height increase.
In
testing the local control damping of the MC prototype, it's been discovered
that the 316 stainless osem heads are magnetic.
We've discovered that the wire EDM process used to fabricate the heads
magnetizes the heads, and that occasionally the stock itself is partially
magnetic. Russell Jones is looking into having the heads re-worked to increase
radii (to decrease the chance of sawing through the Kapton
insulation) and then having the heads annealed. As an alternative, we're
hoping to get provisional approval from the vacuum review board to use
an anodized aluminum head.
--------------------------------------
Sheila
Rowan
At
Stanford:
We
talked to Pierre Khuri-Yakub (faculty member
in Ginzton lab.) re measuring some mechanical
properties of the dielectric coating of the witness samples which Roger
has for optical absorption measurements He thinks this is do-able. It seems
there are various ways to do the experiment: either
the water-tank method, a pulsed laser technique or bonding some
transducers on the back of the sample.He
will talk to one of his research associates and get back to us with what
they feel would be the easiest method.
A
draft is almost complete on the thermoelastic damping from coatings. Briefly,
it suggests that this is a loss mechanism whose magnitude can be significant forboth
interpretation of Q measurements and modelling
of thermal noise. The size of the effect can be different for the same
coating on different substrates (ie on sapphire
or silica)
From
Peter Sneddon/David Crooks in
Measurements
made of two samples with 30 layers Silica/Alumina coatings.These
(averaged)
give a coating loss of (2.10 +/- 0.62) x 10^-4.This
is slightly
better
than Silica/Tantala..
Measurements
made of one silica sample with 30 layers of Silica/Tantala
coating where the Tantala has been doped.This
gave (1.50 +/- 0.74) x 10^-4. (This number is in rough
agreement
with Gregg who got around 1.6 x 10^-4, at least for three of his
modes.)
Sapphire
work (both uncoated and coated) now resumes.
---------------------------------------------
Silicate
bonding (HelenaArmandula)
The
SF4 / Fused silica bond (SF4-5) loaded in shear with 10.5kg broke apart
after ~12 days. There was glass pulled on spots around the edge, however,
there was not signs of bonding over the rest of the surface.
--------------------------------------
Coatings
(Gregg Harry)
Measured
the two lowest (butterfly) modes of a thin sapphire coating
sample.The
Q's are in agreement with thermoelastic damping at 1.5
million.Other
than testing thermoelastic damping, we probably won't get
much
out of these uncoated sapphire, but the Q's seem high enough to see a
clear
change when a coating is applied.I
am struggling to find a few
higher
modes, but this sample will be ready when we resume coating.
-------------------------------------------
Suspensions
Report from GEO600
Caroline
A. Cantley
A.MATERIALS
See
separate report from Sheila Rowan.
B.OTHER
SUSPENSION MATTERS
B.1.
The
UK Advanced LIGO proposal was submitted to the UK Particle Physics and
Astronomy Research Council (PPARC) in June 2002 (GEO600 Glasgow plus Rutherford
Appleton Laboratory and
B.2.Monolithic
Suspensions in GEO600
The
two mirrors in the central area and the beam splitter were installed in
the detector in December 2002. Violin mode frequencies and Qs are currently
under measurement.
(GEO600
team).
B.3.Cantilever
Blades
A
number of cantilever blades have been tested and the deflection results
compared with an ANSYS model of the blade. The experimentally measured
deflection and the model agree to within a few percent. Further blades
will be manufactured, using the acquired information from these tests,
with an additional lapping process to achieve a uniform thickness along
the length of the blade. Mike Plissi has
been liasing with the
(M.Plissi,
C. Torrie (Caltech), M.P.Lloyd,R.Jones, E.Elliffe)
B.4.Suspension
Wires & Blade Clamp Design
Measurements
of the tensile strength of wires used in suspensions with different designs
of wire clamps are ongoing. These will be used to determine the clamp design
that allows the closest approach to the theoretical maximum breaking stress
for a particular wire used in a suspension.
(M.P.
Lloyd, R. Jones, C. Torrie (Caltech),
B.5.Analogue
Electronics for LASTI
Production
is continuing. The second complete set is ready to be tested and shipped.
We
are awaiting confirmation that the first set is working as predicted before
shipping
this next set.
(D.I.
Robertson, H. Ward).
B.6.
Recycling Mirror Suspension
The
design of the recycling mirror prototype is well underway. The cantilever
blades for this suspension have been designed and the pendulum mass and
mass geometries are being finalised. Calculation
of the deflection (bending) of the upper mass due to loading of the cantilever
blades is also underway.
Mike Perreur-Lloyd
is currently visiting Caltech and is assisting in engineering activities
associated with the design of the upper, intermediate and test mass assemblies.
This includes creation of a 3D layout of the suspension, design of the
associated structure and catchers, checking that all components can be
integrated within the footprint of 400mm x 300mm, interfacing of the suspension
with the support structure and creation of engineering drawings for component
manufacture.
(N.A.
Robertson (Stanford), C. Torrie/J. Romie
(Caltech), M. Perreur-Lloyd,
B.7.
Mass Budgets for Advanced LIGO Suspension Prototypes
The
mass budgets are being reviewed, in particular with respect to the interface
with the isolation systems.
(N.A.
Robertson (Stanford), C. Torrie/J. Romie(Caltech),
M. Plissi,
B.8.
Hybrid OSEMS
Development
of the Hybrid OSEMS is continuing. Currently a detailed investigation is
underway as to the cause of the slight magnetism of the 316 austenitic
stainless steel coil formers.
(R.
Jones, C. Torrie/J. Romie
(Caltech))
B.9.
Ribbon Pendulum Q Measurements
A
four-week test was conducted to measure the Q of a ribbon pendulum (400g
mass; 30cm long; 1.2mm x 0.12mm ribbon, Suprasil
2). The measured pendulum Q was 8.8e8. However this result has to be confirmed
since it must be checked that the pendulum is not being significantly driven
by seismic noise.
(G. Cagnoli,
A. Heptonstall, K. Strain)
----------------------------------
Sapphire
Q measurements, bonds (Phil Willems)
Dan
Busby and I have finished our set of measurements on the clear 40kg sapphire and
sent it on to Gari.While
it would have been good to collect more data for more
modes, there are other demands on this sapphire before the downselect,
and the poor barrel polish
of the sapphire sets limits on the utility of further tests.In
particular, while it would be nice to set limits on the anisotropy of sapphire
losses, we would need vastly more data on vastly more modes to separate the
polish and anisotropy contributions with any certainty.
I
think there would be great value in repolishing
this sapphire to remove all
surface
scratches and the chip in the edge and repeating the Q measurements sometime
in the future.
Nevertheless,
the best Q measured for this sapphire is 2.0e8, for a radial
antisymmetric
mode.This meets the Advanced LIGO
requirements.The scatter of the
other measured Q's is in reasonable agreement with a lossy
barrel contribution given the
uncertainties typical in these experiments.
We
have data for one attempt at suspending the pink sapphire.The
best Q so far is
1.8e8, for the same mode as for the clear sapphire.Other
Q's are within the scatter
of the measured values of the clear sapphire, most worse, one better.
We
expect to complete our tests on the pink sapphire before the LSC meeting.
A
new bond (SF4-9) has been loaded with 10.5 kg. This bond was made with
newly bought sodium silicate solution; it has been loaded for
5 hr.at this writing (Wed. 5th)
The
SF4 / fused silica bond (SF4-1) being pulled with 26kg (tension) is still
holding. It has been under continuous tension for ~47 days and at one point
it was heated to 33 degrees C for 24 hr. There was
not signs of stress with the increase in temperature.
-------------------------------------------
Glassy
Metals etc. (RiccardoDeSalvo)
Mainly
a lot of work on brazing the MoRuB to its
mechanical substrate.
We
were fooled into believing to be close to success by a strange wetting
of AuSn,our braze
of choice.We built an oxygen free
glove box to mitigate the effect of the thin surface oxyde
on MoRuB.We
de-oxyde the surface and dip it in the
braze in Argon atmosphere.We
made several brazings and initially obtained
what looked like good wetting of MoRuB.We
also made some samples for Q-factor measurements Francesco C..But
we always had bad adhesion strength in the stress strain tests, and the
Q- factor measurements were all low (in the thousands when our break even
point with fused silica is 10,000), and strongly dependent on the measurement
mode.
This
is particularly maddening when tests on other glasses,
that can be produced in thicker layers, yield good levels of Q-factors
and indicate that MoRuB should be at least
above 30,000, well above our break even point.
Finally
Stefano found out that AuSn wets the MoRuB
somewhat like scotch tape wets glass, possibly by Van derWaalls
forces, and, although it sticks some, it can peel off easily.This
is totally unexpected from a braze (if it
wets it normally holds well) and worrisome.Could
be a show stopper, or send us all the way back to sputtering.
Finally
Stefano found that in the glove box AgSnTi
braze (Ti .5% is added to neutralize the oxides) not only wets MoRuB
reliably, but it seems that it sticks there as a
braze should do.He is investigating
if the improvement comes from the Ti that breaks the residual oxyde
or from the different affinity of the alloy to the MoRuB
surface.He has several ideas, he
is preparing a setup to make brazes under pressure and testing AuSnTi.A
worry is that AgSn is much softer than AuSn,
and it may introduce much more dissipation.
To
be mentioned also that we (Eric) are trying new formulas for MoRuB
that may make its production much more easy
and allow MoRuB in thick layers.
Also
we made cryogenic thermal conductivity measurements on both sapphire and
pure alumi
--------------------------------
Prestabilized
Laser
Preparing
for the power head downselect at the upcoming LSC meeting
Input
Optics
Nothing
to report.
Core
Optics
Full-sized
sapphire substrates in mechanical characterization (see above)
Auxiliary
Optics
Following
experiments at GEO-600 in performing ROC correction by ring heating of
reflective face.
Dave Ottaway is developing a model for
this configuration, which may be useful for Adv LIGO.
Interferometer
Sensing and Controls
Nothing
to report
Data
Acquisition, Diagnostics, Network & Supervisory Control
Nothing
to report.
Other
Laboratory R&D
From:RiccardoDeSalvodesalvo@ligo.caltech.edu
Allyson:
Measuring
SEM photos of indentations data.
Eric,Hareem:
Retuning splatter and splatting.
Eric:
Making new melts of MoRuB of several recipes.Lots
of work in melting and splatting.
Stefano:
Optimized the oxygen free glove box, made several brazings
and obtained good wetting of MoRuB.Initially
encouraging, but always bad adhesion strength.Finally
found that AuSn wets the MoRuB
but just as scotch tape wets glass, it can peel off easily.This
is totally unexpected and worrisome.Could
be a show stopper.Finally
found that AgSnTi braze (Ti .5% to neutralize
the oxides) not only wets MoRuB, but it
seems that it sticks there as a braze should
do.Investigating, after all the deceptions
we are very cautious, but this seems to do.Interested
to discover if it is the Ti to break the residual oxyde
or the different affinity of the alloy.Preparing
a setup to make brazes under pressure and testing AuSnTi.Also AgSn
is much softer, if it turns out to be the only solution, it may introduce
much more dissipation.
Building
the new stress-strain testing machine.Making
tests with the old machine.
Riccardo:
Maintenance and improvement of machines.
Francesco
Cordero: Made more measurements on MoRuB
samples.The samples with machined
off braze are even worse than before.Real
problems with the braze.Is
this a show stopper?
Alessandro:
Working with the Ultra-Sound mill. Adapted the Diamond loadedvitralloy
to the Ultrasound machine head, tests will follow.
For additional information about this report, contact sanders@ligo.caltech.edu