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The LIGO Executive Committee Agenda for Monday November 11, 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:
no report
LIGO Operations--Administration
There was no site teleconference held on Thursday, November 7, 2002.
The list of current actions revised to reflect
the status of open actions assigned through October 31, 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
11/07/02 |
Packages | Faxes |
| In | 29 | 33 |
| Out | 10 | 15 |
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)
>Irene Baldon
Progress Period from 11.01 to 11.07
Accomplishments:
Weekly Advanced LIGO Project Controls meeting was not held this week.
Advanced LIGO MRE Proposal (Highest Priority)
Tested project being shipped to VA, to confirm compatibility.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
Nothing to report.
There are currently no open change requests to be considered
by the LIGO Chnage Control Board.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by M. Landry)
---------------------------------------------------------------------------------------
The Central Alaskan earthquake of Nov 3 (M7.9, 22:12:41UTC, triggering
3/4 of our optics'
watchdogs) appears to have not caused any major problems at LHO.
The 4k has resumed full
locking since that time, along with single-arm and PRM locks in the
2k.
Greg Mendell has moved LDAS from the staging building to its permanent
residence in the
new LHO building.
2K IFO (H2)
-----------
MC WFS stability was restored by ad hoc tweaking of the (previously
dependable) ASC output
matrix. Additionally, MCn damping loops were adjusted.
We might not be out of the mode
cleaner woods yet; MC_F remains a factor of 2 worse at frequencies
above 30Hz, compared to
reference spectra.
B. Kells is continuing visibility measurements using single arm locks.
4K IFO (H1)
-----------
Decided to pursue in parallel the re-establishing of full lock, with
investigations of
the ellipticity of the beam emanating from HAM4, noted last week.
A camera is being mounted
on the periscope to monitor the latter. Cleanup work on ISCT4
gave way to full locking
late this week.
The IFR frequency synthesizers which govern the 4k modulation frequencies
have been
synched to an SRS rubidium frequency standard. The rubidium unit
outputs 10MHz and shows
11 digit accuracy when measured with a time interval counter over 1s.
A noise budget for H1 can be found elogged at http://blue.ligo-wa.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=11/01/2002&anchor_to_scroll_to=2002:11:01:19:30:05-peterF
Misc commissioning (Matone):
Notched out 60Hz in the MC2 path in the Mode Cleaner, reducing the line
amplitude by a factor of 4. No impact on the RMS was observed.
Built a template file for the operators to use in order to monitor
one arm frequency noise.
DAQ
---
EDCU upgrade, EDCU on-a-Sun machine. Alaskan quake trends saved
to LDAS T3 system.
WFS testing: finished the electronics testing, closed one of the WFS2
feedback loops(the I phase) with power recycled Michelson to control the
RM. Released beta version of configuration tool to store/restore ifo channels.
Will try to integrate this new gui into the system. (Andri, Valera)
CDS Software:
a) Downloaded and installed EPICS version 3.14. Preparing myself for
the upcoming seminar on EPICS. One big advantage of using 3.14 is that
it supports sun solaris as IOC host. With EPICS IOC installed on sun we
can eliminate all the vxWorks controllers sitting in the Master storage
room.
b) Fixed the bug in the l1iool1 controller with the help of Chathen,
that the ADC 3113 is now being initialized properly. The controller stopped
scanning channel values after acquiring only one data.
c) Work in progress on fixing last minute problems on Tidal Servo
(Ash Khan)
LDAS admin:
1) Helped Erik in Keith's absence to diagnose and fix problem with
MIT's
LDAS: somebody turned LDAS debugging flag on that caused huge extra
output generated for each job.
2) Submitted 'Global use of LDAS metadatabase across LIGO and LSC sites'
technical note (LIGO-T020169-00-R) to DCC.
3) Together with Chethan fixed the problem with mounting minute-trend
data from fb0.
4) Mounted E7 and S1GEO data.
LDAS data analysis:
1) Continue working on Wave DSO.
(Igor)
GC
* Successfully evaluated and installed an anti virus solution
for our mail server. The product is very easy to install and
configure and it integrates well with our existing mail server
configuration. The product has anti SPAM features also.
* The above mentioned anti virus software has been stopping an
average of 4 viruses a day at our mail server in the first
three days of being installed.
* requested a quote on the fibers to install our new switches.
* Received the new switches from Foundry and started configuring
them.
* performed some maintenance on the mail aliases.
* researching upgrade options for Marcel.
* made a couple changes to the firewall configuration at LLO.
* Looking into another VPN software solution I learned about
yesterday. It looks interesting and may provide some
solutions for Livingston.
(Shannon)
HEPI / LASTI
Hydro-tested Hyspan's un-annealed bellows last weekend. We brought
the pressure to 150psi, stopping and venting the system every 10 psi. Within
our ability to measure these rolled structures it behave elastically and
always returned to its relaxed state. We were limited to 150psi by a hand
pump so ordered a higher pressure replacement. On Monday with the new pump
the bellows yielded rather suddenly at 210psi. When it did, the pressure
went down into the low 100s. Additional pumping just continued to swell
and yield it more with the pressure going up to about ~150 and then back
down to the low 100s. We didn't continue much past that point so as not
to destroy any evidence on how it failed. It looks like the valley of the
convolution yielded in tension. It seems to have started from the middle.
This is the first time the bellows have been stressed to failure, which
we find is about ~3x the system's operating pressure. Good news. Ameriflex,
the manufacturer of the replacement bellows is still on schedule to ship
this week. We are ready to assemble 2 this weekend, which looks good to
get them to MIT next week. The last 2 springs have been received from the
shop, characterized at LLO and delivered to MIT. L4C mounts are in the
shop and should be finished by Nov 15. (Hammond,Kern)
ETF / Advanced LIGO pod bases
Completed the design of a simplified GS-13 mount and sent to Joe Giaime
for review, production in the LSU Physics shop. (Hammond,Kern)
Optics / Laser
Worked with Rai, Gary and Harry to locate and setup a test fixture
to measured the wavefront distortion introduced by our large metal/glass
seal viewports. This is to determine if they would be suitable to replace
the small COS viewports at the symmetric, and AS ports. (Kern)
Hydro-tested
Hyspan's un-annealed bellows last weekend.We
brought the
pressure to
150psi, stopping and venting the system every 10 psi.
Within our
ability to measure these rolled structures it behaved
elastically
and always returned to its relaxed state. We were limited to
150psi by
a hand pump so ordered a higher pressure replacement. On
Monday with
the new pump the bellows yielded rather suddenly at 210psi.
When it did,
the pressure went down into the low 100s.Additional
pumping just
continued to swell and yield it more with the pressure
going up to
about ~150 and then back down to the low 100s.We
didn't
continue much
past that point so as not to destroy any evidence on how
it failed.It
looks like the valley of the convolution yielded in
tension.It
seems to have started from the middle.This
is the first
time the bellows
have been stressed to failure, which we find is about
~3x the system's
operating pressure.Good news.
Ameriflex,
the manufacturer of the replacement bellows is still on schedule to ship
this week.We
are ready to assemble 2 this weekend, which looks good to
get them to
MIT next week.The last 2 springs
have been received from
the shop,
characterized at LLO and delivered to MIT.L4C
mounts are in
the shop and should be finished by Nov 15.
Ken Mailand
All pump station
related components have been shipped to LASTI MIT, except the pressure
sensor read out box and cables, due out 11-7.
Pump Station
arrived safely at MIT. On going communication with Ken Masonre.the
re-assembly of the pump station at MIT,
arrangements
for facilities, staging,and tools.
Due to some concern regarding the flammability of an Alcohol / Glycerin mixture, a safety review and approval is in process before deciding the fluid to use at LASTI.
- Alex and
I continued work on an EDCU capable of the 16Hz update rate
and 20000+
channels.We tried several schemes,
which worked at Caltech,
but did not
work at LHO.Main problem seemed
to be the reflected memory
load, which
is maxed out until we receive the new 2Gbit/sec boards.
Today, we
installed yet another scheme.This
one uses a Sun as the EDCU
with a private
5588 network connection to the DAQ controller to get
around the
main network bottleneck.So far,
this scheme appears to be
working.We
are running with ~7000 channels and the EDCU is updating
this info
to the controller at about 80-90Hz.Note
that just making the
EDCU run at
16Hz does not mean that all EPICS channels will in fact have
16Hz resolution,
as the data from the front end EPICS systems are not
now running
at 16Hz.We will continue to run
this system thru the night
and check
that it is stable.
- Moved up
(to LHO) Lori's code, which makes a sorted list of all active
GDS signals.This
is a separate EPICS sequencer which gets the GDS info
from the LSC/ASC/DSC
to compile its list.This code is
running on the
ASC epics
processor.This list now appears
on the LHO overview screen.
- Later this
week, we will try out the GRACE version of the dataviewer
at LHO.
- I'm at LHO
thru next Wednesday, primarily to track down reported
problems.
-
Today, we found that the noise reported on the nPtrr signal for the
LHO2k was
caused the QPDX input cable shield being tied to ground at the
chassis.Not
sure why this caused the noise and will investigate
further tomorrow.
-
Added a diagnostic into the LSC code at Peter's request.The
code
now monitors
the LSC ADC inputs and reports the number of times a
channel is
saturated (> +/- 32000 counts) during a 1 second period.
This info
is fed to EPICS channels which are then being recorded by the
DAQ.
-
Starting work on finding the "channel hopping" problem with ICS110B
ADC modules.Spoke
with the factory, and they say that the SYNC WORD
capability
is partially incorporated in these B models.(We
want to use
the SYNC WORD,
as it is supposed to be output prior to the first ADC
channel such
that our code can determine which channel we are reading
out as all
ADC channels are read from the same memory location on the
ADC board). The
"partial" implementation on the "B" models means that
the SYNC WORD
will
not read back exactly as it is written.Instead,
it
is some encrypted
form of this, and the ICS rep wasn't quite sure what
this incryption
was.So, we are going to try and
get this SYNC WORD to
come out at
all and then try to decipher the encrytion.
-
This week, also want to look closer at LHO timing issues.As
a
start, the
DMT TimeMon tool is now running at LHO. I also want to repeat
some of the
test that were run at LLO, as well as add a few more timing
diagnostics into digital servo software.
EMC Upgrade:
prepared web materials and graphics for 11/22 review and corresponded with
outside reviewers to clarify program scope and review logistics.
ISS requirements:
discussed and closed remaining open issues with recent draft, revision
should be turned over to RTRB today for blessing. Re: schedule, we reached
a consensus that rushing the new ISS in time for installation prior to
S2 was not worthwhile. Current IFO noise would not be directly impacted,
and continued prototype testing on the 40m (Flavio and Ben) promises a
significantly improved final ISS product with a few more weeks' investment.
LOS coil readout
filter requirements: incorporated recent improvements in 25-35 Hz L1 and
H1 noise to relax dynamic reserve requirement.Also
relaxed input noise spec in view of intrinsic thermal noise in coil driver
outputs.Expected RTRB Friday or
Monday.
Mohana Mageswaran
I have tested 6 more of the Variable Delay Timing Boards with the changes. And I also wrapped up Rich's Pump Servo Controller (for the seismic retrofit hydraulic actuator) and shipped it to MIT on Tuesday. I am collecting the information for our New Common Mode Servo.
Jay Heefner reporting
FPGA Timing
Board
- The requirements
document is complete and out for review.
- The configuration
device board that automatically reprograms the FPGA on power up was received,
installed and tested successfully. Prototype testing of the FPGA prototype
board contintues.
Adv LIGO SUS
and LIGO Anti-Image
- The first Rev C Anti-Image board was stuffed and tested successfully. Nine more are being fabricated. A total of 4 are needed for the adv LIGO MC prototype, but the other 6 will be available for testing in the interferometers.
Jamie is studying
the issues of saturation of PDs to get to our goal of 300mA of photo-current.
Kirk is looking into the limits of our new FSS board, with the aim of improving
its robustness to environmentally produced perturbations.
Go and Blair
have impoved the scan time to 0.1 S and have increased the resolution to
10000 pixels. Dave and Go will be going to LLO to work with Andri in measuring
the wavefront properties of the beams exiting the interferometer starting
the week of the Nov 18th.
More details from Go: The sideband camera measures the complete spatial profile of a low level optical field in the presence of a much larger field at a different frequency by scanning with a pair of galvanometers.We have successfully demonstrated the sideband camera and obtained the images of spatial variation in the amplitude and phase of the first and second order sidebands which are respectively 25dB and 50dB smaller than the carrier. For the past few weeks Blair Connelly (senior thesis student) and I increased the number of scanning points to have a better spatial resolution and also increased the scanning speed up to 10Hz.
I worked on
the comparison between perturbation theory and modal model: for one cavity
if the input beam is an eigenvector of the round-trip propagator what is
reflected back is its conjugate. I convinced myself this is related with
time-reversal.
I also understood the use of left and right eigenvectors in perturbation theory (they would be the same if the round-trip propagator were Hermitian) that are biorthogonal and I reproduced my results from perturbation theory, by using the formalism of modal model.
OTF Lab.
(Bridge)
Contamination
Cavity # 1operating continuously.
Cavity with
test sample 65 % Glycerin and 35% Ethyl.
We continue
taking ringdown and beat frequency measurements every day.
Initial results
(9 days) show no change in loss.
New OTF
Lab at Lauritsen ROOM 38
Cavity #3
Reference Cavity still pumping down. Optical train ready.
We moved this
cavity to the side.Beam visibility
still low ~ 65% so we decided to open the cavity
and change
the mirrors.
Cavity #2
Test cavity
WE prepared
this cavity very good.Alignment
is very good as we have a beam visibility ~ 90%.
This cavity
will be our reference cavity instead of Cavity #3.
Continue taking
RGA measurements.In preparation
to have the cavity locked.
We are preparing
and installing all the electronics necessary to take ringdown measurements.
We are arranging
the whole lab as installing new power strips, bringing Metro racks, cabling
arrangements, etc...etc..
Preliminary
results for errant laser beams in the LIGO 4K IFO indicate that a 3 deg
half-angle cone of rays emanating from either the IOO steering mirror (SM)
or MMT1 mirror, caused by the earthquake stops being set 1 mm from the
mirror, will flood the MC2 and MMT2 towers with errant beams; Also, a similar
source of rays emanating from MMT2 will flood the MC1, MC3, MMT3, MMT1,
and SM towers with errant beams that might damage the COC suspension wires,
OSEM's,and/or electronic cables.
A Gaussian beam profile will be superimposed on the errant ray locations to indicate the power density at the target COC suspension towers.
Held a meeting
on Tuesday on the earthquake stop redesign effort. Doug Cook and I are
working on the prototype designs for the SOS. Mark Barton will head the
testing of the prototypes here at Caltech in a vacuum chamber in the OTF
with an SOS structure and osems borrowed from the 40m and (hopefully) a
dummy mass from LHO. The SOS and osems will be cleaned and baked after
testing and delivered back to the So. Annex. I'm working on expanding and
quantifying the redesign requirements document with Dennis Coyne.
Performed FEA on SOS and MMT2 beam blocking baffle and have found that the baffle does not negatively affect the resonances.
Activated alumina beads were received in three sizes: 1/8", 3/16", and 1/4". The 3/16" beads were loaded in the cannister and the cannister/full mask combination was tested for pressure drop/air flow, which just met the required 4 scfm for safety. This was breathing-tested for one hour with periodic exhaust humidity measurements, from which calculations indicate that field use in LIGO BSC chambers with dry air purge should reduce the moisture added to the environment by exhaling from approx. 4.8 g/hr to 0.45 g/hr per worker. This is not the only source, however, and the other moisture sources are more difficult to estimate and to control with low expenditures: purge gas moisture content, moist room air migration, and worker perspiration. The full mask setup will be sent to a site for evaluation, and may be tried during a required entry for effectiveness.
no report
LASTI (Coyne, Forbes, Hammond, Kern, Mason, MacInnis, McKenzie, Mittleman,
Ottaway, Rankin, Rollins, Shoemaker, Zucker)
---------------------------------------------------------------------
PSL (McKenzie, Rollins, Ottaway)
-------------------------------------------
Jamie is studying the issues of saturation of PDs to get to our goal
of
300mA of photo-current. Kirk is looking into the limits of our new
FSS
board, with the aim of improving its robustness to environmentally
produced perturbations.
EPI design and installation (Mason, MacInnis, Rankin, Forbes)
-----------------------------------------------------
The first HEPI housing assembly was installed on BSC0 with no major
problems. We have started installation of the second assembly.
Bill Forbes (CSR machinist) has been working in our shop with Myron
on
last-minute clearance and fit mods to the HEPI housings.
The plumbing of the hydraulic lines is approximately 80% completed.
We
have recieved the pump system from Caltech and moved it into the lab.
Ken Mailand is scheduled to arrive next week to install it.
We have recieved the first hydraulic actuator from LLO. This actuator
is not usable, but it is being used to check the fit in both the
horizontal and vertical axis and to start planning installation
procedures.
MEPI Characterization and Test (Ottaway, Coyne, Mittleman)
----------------------------------------------------------------------
We have started to design and close modal damping loops on the HAM
platform.
Our first try worked well at suppressing the lowest horizontal modes
(see
http://emvogil-3.mit.edu/ilog/pub/ilog.cgi?group=lasti&date_to_view=11/01/2002&a
nchor_to_scroll_to=2002:11:01:17:41:53-ottaway).
HEPI Fabrication (Kern, Hammond)
----------------------------------------------------------------------
Hydro-tested Hyspan's un-annealed bellows last weekend. We brought
the
pressure to 150psi, stopping and venting the system every 10 psi.
Within our ability to measure these rolled structures it behave
elastically and always returned to its relaxed state. We were limited
to
150psi by a hand pump so ordered a higher pressure replacement. On
Monday with the new pump the bellows yielded rather suddenly at 210psi.
When it did, the pressure went down into the low 100s. Additional
pumping just continued to swell and yield it more with the pressure
going up to about ~150 and then back down to the low 100s. We
didn't
continue much past that point so as not to destroy any evidence on
how
it failed. It looks like the valley of the convolution yielded
in
tension. It seems to have started from the middle. This
is the first
time the bellows have been stressed to failure, which we find is about
~3x the system's operating pressure. Good news. Ameriflex,
the
manufacturer of the replacement bellows is still on schedule to ship
this week. We are ready to assemble 2 this weekend, which looks
good to
get them to MIT next week. The last 2 springs have been received
from
the shop, characterized at LLO and delivered to MIT. L4C mounts
are in
the shop and should be finished by Nov 15.
Simulation and Modeling ( Yamamoto )
* e2e weekly meeting
Virginio, Matt and Hiro discussed about the simulation of the mechanical
motion of the mirror. Topics include
(1) use of the accelerometer on top of the pier to study the effect
of
the huge noise at LLO (train, logging),
(2) direct measurement of the table top motion using OESM, optical lever,
FP cavity,
(3) props and cons of using the ground motion vs pier top motion.
* LLO model
Virginio and Hiro are working to set up the simulation to study the
huge noise at LLO. Sany Yoshida made measurements of seismic correlations
at LLO LVEA, which shows fairly complication pattern. Sany analyzed
it
and has a model for it. This will be useful for this simulation work.
The
first approach will be to record the time series of 6 stack motions
using accelerometers for the duration of the train passing and logging
activities - including several seconds of silent period - to simulate
the
locked state and the lock break with different stack model to set the
requirements of the improving the SUS at LLO.
* LHO model
Luca wants to have a model to simulate the MC. He is going to prepare
a
SimLink model to identify the system to be modeled. This is useful
for
LLO modeling as well, in order to simulate the seismic effect to the
lock
and noise level. This model is consisted of 3 suspended mirrors, with
LSC
around. This will not be used integrated with the rest of the COC simulation,
because the band widths of these two subsystems are too different,
and the
simulation can be very slow if they are to be simulated together. Rather,
this model will be used to study the frequency noise induced by MC.
* field model
The cavity response again frequency noise is not quite well implemented
in the summation cavity formulation (fast simulation). The issue was
found in the PRM model, but the same issue seems to exit in FP model.
Hiro is calculating the approximation used in the fast simulation module
to make it work properly.
Matt's new field model - continued.
* documentation
Hiro has updated the primitive reference manual, and is revising the
introductory document.
* GUI development
Bruce Sears
- Cut and paste implementation completed
- Fixing node naming bug
- Checking all menus to make sure options make sense
Melody Araya
- Continuing work on the modeler to read the revised file format
and implement discussed optimizations.
Ed Maros, Bruce Sears
- Started to work to separate JAlfi (GUI part of e2e) package
from
the simulation code package. GUI and simulation
software are updated
at a different pace, and this separation allows
more timely update
and distribution with less hassle.
LIGO Data Analysis System
Software Systems ( Blackburn )
Completed successfully two rounds of full system testing in preparation
for the LDAS 0.5.0 beta release. These tests identified over a dozen
bugs
which have all been fixed now and we are about to start our last round
of
system testing for this release. UWM has asked that we postpone the
date
of the release for a couple of days to give them a chance to work with
the pre-release version. If they identify no issues, then we expect
to
have the release on Monday. If they do find issues we will weigh the
schedule cost vs benefits to determine the next best release date.
We did discover a new thread issue in the GCC standard template file
this week. This one is can occur when multiple thread are attempting
to open or close a file at the same time. This is a very raw bug and
only shows up under extreme load. It is hope that this will be fixed
in the next GCC release. LDAS plans to migrate over to the new GCC
in
the next development/release cycle.
The performance of LDAS has been slightly reduced in this release as
a result of the new frameCPP. The problem is in the inherited memory
management from the standard library. We will be implementing our own
memory management to resolve this performance issue in the next release.
Most effected by this performance degradation is the creation of RDS
Frames. We will probably have a 25% slow down in the production time.
It was not possible to get a working compression module into this release
of the frameCPP I/O library. It will be added in the next release.
This pre-release of LDAS has now been successfully exercised in the
context of the GriPhyN demonstration for the Super Computing 2002
conference next week. Everything is working very nicely and we even
got
a preview of the graphical viewer on the milky way which will be used
to
identify points on the sky for which a directed pulsar search has been
made.
Hardware Systems ( Anderson )
Caltech ( Al Wilson & Stuart Anderson )
* Installing RH7.3 on the desktop/workstations at CIT/millikan.
* Updating web page for KS instructions.
* Continued discussions with CACR and ITS regarding future Caltech
Internet2 network connectivity.
* Successfully tested Apache-2.x on LDAS gateway machine.
* Supported RedHat 7.3 upgrade of desktop LDAS machines.
* Investigating Linux IDE-RAID NFS server performance.
Livingston ( Igor Yakushin )
* Helped Erik in Keith's absence to diagnose and fix problem with MIT's
LDAS: somebody turned LDAS debugging flag on that caused huge
extra
output generated for each job.
* Submitted 'Global use of LDAS metadatabase across LIGO and LSC sites'
technical note (LIGO-T020169-00-R) to DCC.
* Together with Chethan fixed the problem with mounting minute-trend
data from fb0.
* Mounted E7 and S1GEO data.
Hanford ( Greg Mendell )
* LDAS was successfully moved from the staging building to the new
building at LHO, Nov 2 - Nov 7. The entire system has
been brought up,
the framebuilders are once again using the T3s for their disk
space, and
the LDAS servers are once again serving S1 data to fortress.
The LDAS
APIs were brought up briefly and test jobs were run. Thus, everything
was shown to work as before the move.
* LDAS is currently down again for an upgrade of the Linux OS to Redhat
7.3.
This means S1 data is currently available again at LHO from
fb3 in the
control room and from fortress, but it will be another day or
so until LDAS
is back up to run jobs.
Data Analysis Activities
MIT ( Katsavounidis )
Stefan:
Here is a short summary of what I was working on:
- I produced a bunch of sanity check plots for both streams
of veto triggers, including deadtime and rate vs
time and segments,
Amplitude, Duration and time between triggers histograms.
All is done for both playground and full S1.
- I started with scatter plots of AS_Q vs REFL_I for H1, using
TFCLUSTER triggers for the full S1. The same thing
for slope and
L1 remains to be done.
The page http://emvogil-3.mit.edu/~sballmer/S1san/diagnostic.html
contains link to all of the above.
Laura:
Defined an epoch veto for the S1 triple coincidence analysis, based
on
band limited RMS (6 min averages).
Extended the burst pipeline macros to calculate the background in triple
coincidences.
Produced plots and summary tables for the playground analysis. Continued
work on efficiency calculation through simulation.
Pushed the whole triple coincidence set through the pipeline. Now
wrapping up the results.
Ran tfcluster over the 3 hour GEO playground, with two threshold
settings and parsed the triggers into ASCII files for the GEO veto
analysis.
Caltech ( Weinstein )
- Generated lots of plots of S1 burst efficiency
for detector network, averaged over
source directions and polarizations.
Caltech ( Shawhan )
* Worked on veto optimization and other aspects of the inspiral upper
limit
analysis using S1 data.
LHO ( Mendell )
1) Worked with the PULG group to solve a round-off error problem in
LALDemod. A fix for this, along with several other minor
changes to the
code, was checked into the LAL CVS repository last night
by Xavier
Siemens. Also worked on preliminary results as part of
our preparing a
report of our progress with the S1 data. See the PULG
web page,
http://www.lsc-group.phys.uwm.edu/pulgroup/, and the S1
investigations
link (which is password protected).
2) Coding to use the calibration data in the knownpulsardemod DSO was
completed and checked into the LALWrapper cvs repository.
LLO ( Yakushin )
1) Continue working on Wave DSO.
General Computing ( Wallace )
MIT:
(Keith)
Attending LISA conference.
Livingston:
(Shannon)
-Successfully evaluated and installed an anti virus solution
for our mail server. The product is very easy to install
and
configure and it integrates well with our existing mail server
configuration. The product has anti SPAM features also.
The above mentioned anti virus software has been stopping an
average of 4 viruses a day at our mail server in the first
three days of being installed.
-Requested a quote on the fibers to install our new switches.
-Received the new switches from Foundry and started configuring
them.
-Performed some maintenance on the mail aliases.
-Researching upgrade options for Marcel.
-Made a couple changes to the firewall configuration at LLO.
-Looking into another VPN software solution I learned about
yesterday. It looks interesting and may provide some
solutions for Livingston.
Hanford:
(Christine)
- Called the repair person in to fix one of the printers.
- Created a new user account for an LSC member. Changed the password
on
another.
- Various user support.
- Worked on web Sys. Admin. documentation.
CIT:
(Mike)
-Reloaded Phil Lindquist laptop from win98 to 2000 pro.
-Finished up loading a laptop with GC software for loaner pool plus
setup
user configurations to loan out to Helena.
-Still trying to finish up working on the Synchrotron workstation.
-Had to work on security issues this week this included locking down
servers due unknown users trying to access the Security Accounts
Manager.
It looks like I have this situation under control.
-This week I had a lot of user support that included software/virus
problems
that were infecting the network.
-Went around getting some of the MAC addresses from PC's to update the
General Computing IP database. This to make tracking infected/illegal
use of computers much more easier to track down. I still have
many
more computers to attend too.
(Lisa)
Attending LISA conference.
(Bruce Sears)
-Ilog Maintenance and Upgrade: 3.5 days
- Next and Previous Log buttons now respond more appropriately
when the adjacent day has no entries.
- Alphabetized user list in search feature.
- Added Most Current Log button, useful for rarely used logs.
- Init no longer creates a blank day's log, but asks for an
initial entry. Blank days will no longer appear in the
log.
- Cleaned out entries which were blank or only tests of ilog.
- Added the possibility of background images for each log to
make them easier to differentiate between.
- Distributing new update of ilog to MIT, LHO, and LLO.
(Veronica)
- LIGO website: most time was spent working on the Aspen Winter Conference
webpages. Posting updates to the LIGO website. Collecting my
own stock
photography to keep for future use in graphics generation.
- CaJAGWR website: arranged with the ITS to have a virtual host name
cajagwr.caltech.edu. Recorded and compressed a video of last
seminar. The
video is now posted along with the viewgraphs. Updated the roster
and the
seminars pages.
- LSC website: worked with the LSC roster database to see how it can
be
modified to allow expanded searches. Sill a work in progress.
- Project Science website: posting last-minute updates as they arrive.
- GNATS: looking into Szabi's request of updating the database.
(Larry)
-Ran down a few more procurement issues. SUN has extended their matching
grant program. The replacement batteries for the UPS have arrived
and tracking
down the new UPS that was ordered at the same time.
-Continuing the server upgrades. The progress has been slow with all
of
the interruptions the past few weeks. I was able to resolve a
number of
configuration issues.
-Worked with Mike on chasing down infected machines and getting MAC
addresses
put in the database.
-Performed a number of network tests. Mostly between CIT and the Observatories.
Things have improved a little but are still not as good as they
were a month
ago.
-Added a few more user accounts and modified a number of accounts.
-Went of the RAV e-mail anti-virus program with Shannon. It looks like
it will
be a good solution. Livingston will be implementing it full scale
and CIT will
start running its testing of the program next week.
-Went over some of the logistics with Shannon for the GigE network installation
at Livingston. After going over a number of items on his present
network the
new system looks to be a major improvement for their setup.
-Assisted DCC on various items.
-Working with Ed C. to get some more of the old equipment turned over
to
Caltech.
From: "Mark Barton" <mbarton@ligo.caltech.edu>
This week I continued working with the reconfigured interferometric
position sensor. Basically I'm back where I was a week ago, getting
fringes from the Michelson using a laser test source, except I've
completely redone the mountings to make some components more secure
and
add more degrees of freedom of adjustability. As a result the fringes
are
much more stable and I'm in a better position to get it working with
the
internal LED source.
From: Larry Jones <ljones@ligo.caltech.edu>
Advanced SEI
The SolidWorks files from HPD's contract to design and fab the SEI structure
for testing in Stanford's ETF chamber have been input to the DCC as D020525.
This includes a Zip file of the over 400 drawings (2D drawings, 3D parts
and 3D assemblies) and a .pdf file to show (most of) the hardware in general.
The DCC also now has hard copies of the nearly 100 2D drawings.
From: Peter King <pking@ligo.caltech.edu>
2.2 AdvLIGO PSL
The hardware for the technology exchange with the University of Hannover
has been assembled and the VME crate was installed. The hardware
rack is
installed next to the optical table. At the moment we are experiencing
a
number of computer related problems, network related issues, and the
compilation of the vxWorks kernel amongst other things.
From: ctorrie <ctorrie@ligo.caltech.edu>
AdLIGO Suspensions
Mode Cleaner
Helena and I continued to work on the assembly of the 2 prototype suspensions last week.
Again this week we have been taking a lot of photographs this week and these can be seen at http://www.ligo.caltech.edu/~ctorrie/ligotriple.html, and by clicking on the recent diary dates.
Height adapters and the catcher for the metal masses were delivered
at the start of this week. CES is reworking the structures
and some associated parts. They are projected to be completed tomorrow
afternoon. The Physics Shop is due to start work on other reworks associated
with the endstops and global OSEMs.
Mike Perreur-Lloyd is now at Caltech for ~1 month from U of Glasgow . Amoung other things we will work on detailed design of the recycling mirror suspension.
So far we have been spending time this week looking at Bills of material,
drawing trees and the ability to copy drawings, and there associated files,
using SOLIDWORKS Explorer as well as reviewing engineering drawing templates
created in Glasgow.
We have also started assembly of the local control coils and there
associated parts.
From: Janeen Romie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Working on mode cleaner design tasks. Height adapters were delivered
last week. CES is reworking the structures and some associated parts. They
are projected to be completed tomorrow afternoon.
Jay is planning to deliver the electronics for the MC prototype at
the end of this week. Mark Barton is ready to hook up the GEO analog electronics
with Jay's digital components and the dSPACE system.
Working with the suspension group on determining the maximum quad pendulum suspension length. This information is needed for the seismic prototype RFP, due near the end of November.
Magnets for the suspension prototypes have been found.
Mike Perreur-Lloyd has joined us for 5 weeks. It is with pleasure that
we welcome him to Caltech and thank him for his support of the suspension
design efforts.
From: Riccardo DeSalvo <desalvo@ligo.caltech.edu>
Akiteru
Repaired all vacuum leaks.
When started realigning interferometer found that the North mirror
was dropped and was seating inside the recoil mass. It had just slipped
from the standoffs.
The damage was tracked back to an accident during vacuuming (opened
gate valve with pressure on other side) that sent the mirrors to swing
wildly.
Remounted mirror in situ but did not perfectly recovered the alignment.
Mirror realigned by tilting the intermediate mass. May be sufficient to
complete the measurements.
LATEST NEWS:
The 3m cavity is now back on line, and it has been locked for a few
hours in air this afternoon. There was no natural lock loss. The duration
is only limited for our operation for characterization.
I will try to operate it in vacuum soon, without the inertial damping.
With luck, the towers won't drift too much.
For the damping, probably I will have to re-diagonalize the front tower
we have made so many nasty tricks to recover the mirror misalignment there.
akiteru
I have managed to lock the cavity in vacuum this afternoon. The result
did not get improved very spectacularly below 10 Hz as I wished, but it
made the error signal spectrum much smoother at higher frequencies. Will
try to test the damping in vacuum tomorrow.
akiteru
Alessandro Riccardo
In Pisa checked out that peeled off MoRuB film has no detectable layer
of Ni, it peeled off cleanly. Although chemical deposition is probably
good enough for most developmental tests, we will need to use sputtering
for more intimate bonding
Stoyan
Ansys, installed modal analysis of hook + strings and simplified geometry,
trouble with long strings because of number of nodes.
Revalving splatter.
Starting the new oven, checked out 3 10-8 l/s leak, OK to go starting
first run soon.
Maddalena, Barbara
Submitted final reports.
Hareem
Repaired leak in DTA, adjusting thermal settings and recalibrating.
Allyson
Vickers hardness measurements systematically lower than Maddalenas,
but with similar trend. Trying to make reliable measurements. Repeated
one measurement with Xavier and Stoyan, and found different averages. Need
more work to find a more repetitible technique. Some improvement by measuring
flat to flat instead of tip to tip and with better lighting, but still
need to work more.
Xavier
Cryo setup, calibrating the power reading of the heting shoes with
external amperometers.
Found a stable excitation current, quantifying stability.
Charles
Working on Stress gauge and LVDTs
Achieved 3 g resolution over 30 Kg range
0.2 micron resolution over 1 mm max excursion.
Cutting samples and electro-polishing
For additional information about this report, contact sanders@ligo.caltech.edu