|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
The LIGO Executive Committee Agenda for Monday October 20, 2003 will be:
(Meeting time: 10:30 am Pacific Time)
STAFFING COMMITTEE MEETING
no report
LIGO Weekly Site Telecon (Lindquist)
A site teleconference was held on Thursday, October 16, 2003. The following were among the issues discussed:
Budgets - We are still comfortable with our estimate of $6 million for the carry-forward. FY 2003 costs being expensed in October are close to $1 million so far, but some of these items were on the list of items to be covered in the carry-forward..
University of Oregon - The University of Oregon has billed for more than is in their contact for R. Schofield. There appears to be some confusion here. This will be a priority item for Irena to straighten out when she returns.
Property - Ed Chargoiswill travel to Livingston to help with
the sale of the excess property..
The list of current actions revised to reflect
the status of open actions assigned through October 16, 2003 may be found
at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
ACCOMPLISHMENTS
(This report
reflects activity for the past month.)
Developed a phase II Statement of Work with George Stokes which includes three main areas that need consideration: 1) further system design, architecture, and maintenance enhancements; 2) automated processing of new electronically submitted documents; and 3) improved website search capabilities. This will be submitted to Phil by the end of the week.
| C | D | E | G |
| 6 records | 51 records | 8 records | 83 records |
| 8 files | 56 files | 10 files | 126 files |
| L | M | P | T |
| 5 records | 29 records | 7 records | 46 records |
| 9 files | 30 files | 9 files | 58 files |
The records represent the actual document submittals while the file numbers reflect that actual number of documents handled due to many submittals encompassing more than one document format. In total, the DCC processed 543 documents last month. This figure includes both electronic files and those documents received only as a hard copy.
ISSUES
Storage - We have accommodated the last large batch of documents and are down to piecemeal slots on the shelves as they correspond to category. I estimate that storage will be non-existant by the end of January. If all documents were processed that are currently in my office, there would be no place to file them. This is a large part of the encroachment problem seen in my office today.
Moving - Should there be a move for our group in the near future, we need at least a 3-4 week window to pack. This is no easy task and will require methodical preparation to ensure that the files remain intact and that piles currently stashed for processing can be carefully situated into a new environment. Also, if there are discussions regarding space allocations, the DCC needs additional space than what is the current allotment, including the subbasement area. The track files need to be relocated and there are problems with three of the stacks because of stripped wheels due to eight years of use. The manufacturer/company of these files is no longer in business, but I've located a company with similar equipment should there be interest in adding/replacing/repairing what we currently have.
ACTIVITY
| 10/16/03 | Packages | Faxes |
| In | 38 | 43 |
| Out | 9 | 37 |
Press here to access
the DOCUMENT CONTROL CENTER
WEB PAGE.
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, Lloyd, Tischler)
>Irene Baldon
(This report covers four working days, October 9-14).
ADVANCED LIGO (Cost Schedule
Control Systems) T. Frey
From: Thomas Frey <tfrey@ligo.caltech.edu>
For list of documents that
are being used to develop Adv. LIGO Cost and Schedule, see http://www.ligo.caltech.edu/~tfrey/Cost_MTG_082002/
Continued development of a proposal for implementing Primavera Project Planner Enterprise.
Progress Reporter - http://www.projwebsite.com/GroupServerP3e/en/ Login using Username: admin and Password: admin.
Static HTML Example - http://ligo.caltech.edu/~tfrey/SUS_WebProj/ (AdL Suspensions Only) NOTE: This is after importing and before any data corrections.
Static HTML Example - http://ligo.caltech.edu/~tfrey/DAQ_WebProj/ (AdL DAQ Only) NOTE: This is after making adjustments to the WBS so that it displays as expected.
Phone conferences with Carol regarding preparation for the SUS Workshop and input of codes.
Prepared reports for SUS meetings scheduled for the week of Oct. 13 - 17.
Attended meetings with SUS group regarding Project Management and Scope.
Prepared spreadsheet that compares SUS / US and SUS / UK key events as discussed at the meetings.
Started preparing resource analysis information for meeting with SUS Group on Friday AM.
PSL - No action items pending. Followed up with Peter and Benno has provided data. Peter has yet to review. Received update date for PSL with progress through 09.26.02.
AOS - Still need completed WBS dictionary and BOE.
IO - Still need completed WBS dictionary and BOE.
SUS - No action items pending.
SEI - No action items pending. Working with Larry to update SEI with progress through 09.26.02.
ISC - Still need completed WBS dictionary and BOE.
LDAS - No action required at this point in time.
INSTALL - No action items pending.
DAQ - No action required at this point in time.
PM - No action required at this point in time.
FAC - No action required at this point in time.
SUP - No action required at this point in time.
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
Have started a draft of a Final Report for Cooperative Agreement NSF
PHY-9210038, the cooperative agreement that covered construction, installation
and commissioning, and initial operations of the sites. This cooperative
agreement ended June 30, 2003. I have been able to dredge up information
from previously submitted documentation, specifically the annual reports,
the Advanced LIGO Proposal, the Procurement Plan for the LDAS Hardware,
etc. Have requested Albert's group to provide some additional information.
The target is to have a draft on the web page in time for the NSF Review,
November 17, 2003.
The following change requests are open.
| CR-030015 | FY 2003 Livingston Observatory Detector Maintenance Expenses (Increment) | R. Wooley | July 14, 2003 |
| CR-030016 | Hanford Facilities 2.2--Divide the Large Equipment Access to Facilitate Movement of Large Items (currently assigned to FY 2004 liens list) | J. Worden | July 31, 2003 |
Additionally we have received a request to add budget to the Louisiana
Facilities account to cover items moved there when the Construction Project
was closed. We will do this, but we are waiting for the final numbers
for FY 2003 so that we can address all of the Louisiana accounts.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled by M. Landry)
2K IFO
The H2 IFO posted its greatest
NS-NS inspiral range so far (444kpc).
All WFS
d.o.f. have been
engaged, although this application degrades spob and arm powers.
Work on debugging the WFS
and adding the QPDs continues. ASI problems were debugged.
Power was increased
into the
IFO.
Bill Kells visited LHO and worked on 2k scatterometer
measurements. Initial findings include that
the predominant mechanism for scatter is from discrete point scatterers,
likely coating imperfections
or contamination on the optic, and, the newly replaced ITMX shows far
less scatter than the old
(replaced) test mass. High-resolution beam spot images are given
here.
4K IFO
As the 4k has been frozen, it has mostly been left to lock in full
or acquire++ modes. Fundamental
violin modes remain apparently high, perhaps three
times thermal excitation. New calibrations are
being performed (to ensure we've not introduced too much systematic
error since S2 and the
violins are in fact simply thermally excited).
---------------------------------------------------------------------
Interferometer commissioning:
--------------------------------------------------------------------
Continued commissioning and stabilization work in preparation for S3.
We
have made about a thousandfold improvement over the excess
noise reported this time last week but are still stumped by a
persistent broadband excess, holding us
about a decade off the previous best sensitivity. Tests have eliminated
numerous candidate mechanisms (see Rana's nice <A HREF="http://www.ligo-la.caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/15/2003&anchor_to_scroll_to=2003:10:15:14:48:55-rana"
TARGET="_top">summary</A>).
At present attention is focused on anomalous behavior of the signals
derived from the beamsplitter pickoff (POB) which control the minor
degrees of freedom (Michelson and recycling cavity lengths),
and on an observed but unexplained discrepancy in the gain of the
common-mode wavelength control additive offset (AO) path.
Some other highlights:
o in the process of commissioning the new atomic clock timing system
we
noticed a failed GPS clock module at the Y end and replaced it
o the new ISS was tweaked up to improve reliability and fault recovery
o a failed mirror mount adjustment micrometer was replaced on the PSL/IO
final output periscope
o an F2P filter was added to MC2 to match those on the core optics and
tested
o the thermal controller on the PSL reference cavity was updated to
an
improved revision like those at LHO
o the ETM tidal offload servo continued to suffer from bugs which caused
unlocking; these may have been fixed, or at least temporarily swept
under the rug.
o A nasty bug was found in the end station EPICS processors causing
timing hiccups every 64 seconds; it was eventually fixed by swapping
in
a different type of processor.
o The control room remodeling is largely finished, with new projectors,
operator and scimon workstations, and fixed displays for data
figures of merit.
Safety/security (Riesen)
---------------------------------------------------------------------
Completed weekly IR scan on the PSL and the 4 IOT/ISC tables, Found
no
errant beams.
Found no safety concerns on the weekly site tour.
Continuing work on the LLO Laser SOP.
Re-established Laser Safety System control computer access;
there are now 3 access levels on the LSS;
a) Read only. Allows minimum access in controlling the system (without
operator log-in).
b) Operator Control. Allows Operators (after operator log-in)
to control
the LSS for daily functions.
c) Administration. Has full function capabilities including program
modification.
The man door between the large equipment airlock and the LVEA is now
alarmable to the control room.
General Computing (Roddy)
---------------------------------------------------------------------
Spent some time making sure that we are fully recovered from last weeks
disk crash.
Received the server that was ordered for Jonathan as the PDM Works
server.Spent a couple hours setting it up. The next morning the
power
supply blew. ASA is working on getting me a replacement.
Spent much of the night last night working on LDAP. I finally
got it
working with SSL so that the entire session is encrypted. This
is for
Solaris only so far, but I feel confident in deploying it at this point.
I will repeat the process again and document all of the needed
steps.
Expecting the new RAID disk server from ASA today or tomorrow.
As soon
as it gets here I will start working on it and burn it in. Afterwards
I
will begin moving GC files to it.
LLO Seismic retrofit (Kern)
---------------------------------------------------------------------
Our last large contract has been received by
the vendor, and all of the
machine and fabrication work can now be termed
'in progress'. Chips are
really falling on the floor. The machine
shop manufacturing complete
sets of parts for 12 actuators by November 14
is on schedule, meaning we
will be able to begin the welded assembly before
December begins. The
Parker valve test manifold is back in the shop
for manufacture and
installation of sleeve bushings in the plug valve
bores. The new
configuration control software (PDMWorks) for
the SEI effort is
installed and serving us well. We're pleased
with its functions and
learning to operate within it's constraints.
This is just what it is
intended to do.
CDS networks (Parameswariah)
---------------------------------------------------------------------
Finishing up on work needed to be done before E10/S3.
Completed a initial check of the automatic Daily Summary plot program
-
ROBO-PLOTTER. This will complement the ROBO-SCIMON and run during S3.
Worked with Rolf last week to fix the End Station front end problems.
We found the CPU load hiccuped evry 62-66 seconds periodically.
Traced the problem to mv162 epics processor. Fixed the problem by putting
in a baja. Cause of problem still needs to be understood.
Added all the requested channels to the master.config file. This has
now
added 2400 channels to the frames. I still have to estimate the disk
space
available for S3 with this change. Even though the thinking is that
this
addition is equivalent to adding 2 16KHz channels, this is only true
for
full-frames. For trends this is equivalent to adding 2400 channels.
Installed the Refl port half wave plate with the help of Ash and
Rupal.
Moved the autoburt snapshots for the previous 3 years to a backup disk
on
control4.
Control room suns are now mostly in and I have been checking to make
sure
they all have the same environments/paths. Updated the video database
and
software for the new projectors and monitors.
Detector Commissioning, High Power Testing (Amin)
---------------------------------------------------------------------
WFS 2: The WFS 2 sensor at LLO has been dissuaded from its obstinate
ways.
Following Rich Abbott's repairs to the detector head, the WFS team
found that the headaches of a dynamic I-phase resulted from four LEMO
backshells not being secured. Once Rich Abbott torqued the backshells,
the I-phases of all three segments with respect to the number two
segment were stationary and easily cancelled in the digital phase
settings. WFS 2 is now ready for running.
ISCT 1 Redesign: All equipment and optics have been prepared for Daniel
Sigg's arrival at LLO. ISCT 1's new half-wave plate controller
has been
installed and tested thanks to Chethan and Ash's assistance.
RM Camera Installation: Prior to the vent, we noted some
operators and scientists wanted a camera looking at the recycling
mirror. Mike Fyffe and I installed the camera on BSC3's new viewport
only to find a dimensional problem. The camera housing being used
partially occludes the view of the RM. Unfortunately we do not have
a
housing that sits 45 degrees offset to viewport axis. Such a
housing
would grant a camera full view of the RM.
High Power Laser Facility (HPLF): The HPLF's first high power laser
is
expected to arrive this week. Our vendor has informed us that this
lower
power laser may be kept until the arrival of the 100 W device. The
SOP
governing the lab is one day from final delivery and review by both
UF-LIGO and LLO.
CDS software (Khan)
---------------------------------------------------------------------
Detector commissioning, modeling and data analysis (Franzen)
---------------------------------------------------------------------
1) Weili Ken and I tested the new MC2 f2p filter installed by Brian
O'Reilly.
2) The S2 RDS107 frame data necessary for my WaveMon veto analysis was
mounted to alvar. Veto triggers are now being produced.
3) Amber Lynn Bullington at Stanford discussed the AdLIGO MC class of
Melody with me. She is planning to release a new, more realistic
version within short. This is good since the UF IOO group needs the
model very much.
LDAS (Zucker for Yakushin)
---------------------------------------------------------------------
Igor is busy installing the final pre-run version of LDAS and
updating the main frame builder FB2.
Dennis Coyne
Held a kick-off meeting with our two Quiet Hydraulics Consultants (Rich Duder and Stephen Osder) at Stanford Univ. Dan DeBra, Brian Lantz and Corwin Hardham prepared talks on the HEPI system with concentration on the quiet (laminar flow) aspects of the system. A follow up meeting is scheduled for next Wed at LASTI. The consultants will see the full scale prototype and we'll review plans for, and questions and issues associated with, the fluid distribution and pump station designs.
Jonathan Kern
Ken Mailand
This week I have been working to identify channels for use as epoch vetosfor the burst analysis. I have also been preparing to install DMT software for the E10 run.
- Working on getting the remote control room (RCR)
machine at Caltech up to date. We
downloaded the EPICS 'gateway' software from Argonne
and got it running on both
the LHO and 40m lab gateway machines. With this software,
EPICS programs, such
as MEDM, run on your local machine and makes connections
to the gateways to
send/receive EPICS data. In the past, it was required
to log into a gateway and
bring MEDM screens back on an X window. Besides running
much faster in this data
only mode, the gateway software provides added security
(set to default of read
only) and reduces loading on EPICS front end processors
(never makes more than
one connection to a front end regardless of number
of clients). We will continue
testing today, and, if it seems stable, we will add
a gateway to LLO.
We are also in the process of updating the other tools
on the RCR today.
- Spent last week at LLO trying to find problems with
end station controller
(ran late and had periodic errors). Turned out to
be a strange problem with some
up our EPICS cpus holding up the VME bus (up to 15usec)
at a fairly periodic
rate of every 64-66 sec. We replaced these Motorola
processor boards with MIPS
processor boards and the problem was fixed. (See LLO
elog for more details).
- Working on getting the LSC operational at the 40m
lab. Since layout is
different than sites, code changes will take about a week.
During the weekend we installed the hardware
components of the new atomic clock based timing system at LLO. The mass
storage room (MSR) houses the CsIII clock and the Master Clock Assembly
of the optical fiber based distribution system. Time is transferred via
single-mode fibers to the LVEA and the Mid/End stations, where it is compared
to the GPS time. Every component of the MSR assembly is installed, tested
and running.
The Time Code Translators (TCT), timing comparators
and related cabling are installed in the LVEA and the two end stations.
These installations are tested and running fine.
The basic communication to the 162s(EPICS) is
not tested as it would require more installations and software changes,
as there are slight differences between LLO and LHO. It is not clear whether
the changes can be safely finished before E10. The lack of communication
will prohibit us from recording the timing difference second trends during
S3.
The LVEA setup indicates a stable ~0.5 us difference
between the Cs time and the PEM GPS time.
The X end stations shows a stable ~2+20 us difference
between the Cs time and the GPS time. It is consistent with the delay we
expect due to the fiber delays (~5ns/m).
The Y end station measurement unfortunately
indicates wild and periodic variations
of the time lag between LIGO’s GPS 1PPS and the CsIII
clock’s 1PPS. I observed the same behavior using the EX hardware and the
CsIII clock at EY. Therefore it was very likely that the either the GPS
receiver or the fan-out board was misbehaving. Replacing the GPS board
fixed the problem. Now the Y end stations shows a stable ~1.2+20 us difference
between the Cs time and the GPS time. It is consistent with the delay we
expect due to the fiber delays.
For now I set the fiber delay for the end stations
to the generic 20.00us, to be consistent with the LHO setup. We plan to
measure the precise fiber delays after S3, as the distribution system is
capable of subtracting it with 5 ns accuracy.
I would like to thank Mike Fyffe, Rupal and Andri for their help during the installation and testing.
Rich Abbott reporting
- Completed tests of first article VME crates from
Dawn. We found several deficiencies in the gasketing that should be easy
for Dawn to correct. Once they have addressed the issues the next batch
of 5 crates will be shipped to LLO.
- Tested a VME crate from AP Labs. The crate did not
perform very well. We have informed the manufacturer.
- Tested another EMI rack from Knurr. This rack is
produced in Europe and the performance was comparable to our Equipto racks.
A quote for price and delivery has been requested.
After approximately 12 months of being exposed to
the open surrounds of
the PSL Lab, the pair of optically contacted flats
was inspected. The
contact was still good. After inspection, the
bond was deliberately broken
and the flats were contacted together again.
Working with Dave Ottaway on the design of the CO2 laser imaging optics for thermal compensation of the HR side of the 4K ITM mirrors.
I will review with Bob Taylor the complete list of
cleaned baffles, mounts, and hardware, sort, and prepare for shipping to
LLO and LHO.
OTF Lab. (W. Bridge)
Contamination Cavity # 1
This cavity is going into a new optical alignment
because the people who worked in the lab to
install the water cooling bumped into the mode match
lens.We are recovering this cavity.
Absorption Test Measurement prototypein
standby
We have received the new 30 watts laser and took it
down to OTF Lab.
We have wired the Laser and the power supply already
and attached the water cooling.
I am now working on the SOP for this laser so we can
turn it ON.
New bench for the new laser is under fabrication.
Scatterometer system: A new and complete scan for
the HR and AR surface Reflectance and transmission for the 2ITM04-C (Inner
test mass mirror) is in progress.Complete
plot and results will be released by Dr. Zhang.
The new base to house the larger Sapphire mirrors
is completed and it will be installed next week.
There is some modification that it needs to be done
on the old base.
OTF Lab at Lauritsen ROOM 38
Cavity #3: We have recovered the old results and the
chamber is pumping now and we are taking ring down and beat
frequency measurements every day as well as new RGA
measurements .
We will introduce a new test simple of solder joints.Kester
SN63Pb37 solder vacuum cleaned with RGA results.
Cavity #2 Test cavity in STANDBY.
Since our last report we have made considerable progress in enhancing
the modulation depth, and hence the discriminant, in the TNI arm cavities.
By phase locking two separate function generators, we are able to deliver
all of the power from one unit straight to the Pockels cell, with the other
output going to the local oscillator. Not only does this boost the modulation
depth, it also allows us to do away with the NIM phase shifter and limiter
we had been using.
While we are able to boost the modulation depth, and while we see an
analogous increase in the discriminant, we still do not observe any dramatic
reduction in the noise floor. With the much-higher discriminant, the electronic
noise at the output of the mixer appears to no longer be large enough to
account for our noise floor. This noise is, as before, flat from a few
hundred Hz up to 100 kHz, and its level is about 1e-18 m/rHz. Neither
a theoretical prediction for the shot noise nor an experimental measurement
of it appears to be high enough to account for this noise floor.
On the photothermal experiment, we have measured the loss in the cavity
and compared it with the mirror absorption as measured by the photothermal
response. Assuming the bulk value for Sapphire's thermal expansion coefficient,
the two values for the absorption agree within experimental errors. Put
another way, if we use the cavity-loss measurement to obtain the absorption,
we can then measure the substrate thermal expansion coefficient and obtain
a number consistent with the tabulated value.
no report
---------------------------------------------------------
LIGO Data Analysis and Computing (Anderson for Lazzarini)
---------------------------------------------------------
------------------------------
LDAS Software Team (Blackburn)
------------------------------
The 0.8.0 release of LDAS is in great shape and expected to go out tomorrow
without a hitch. Over 100 problem reports have been closed out in the
past
few weeks and of those identified as critical and/or important for
the S3
run, only one will remain in a non-closed state for this release. This
will
allow for running the new release of LDAS during the E10 run this weekend.
Changes to the frameCPP dictionary class to removed the Standard Template
Library's String class and replace it with a more stable thread safe
version
of our own design has resulted in no core dumps in the frameAPI even
when
optimized with inlining options since last Friday. An exception specification
bug caused an unrelated core dump but has been fixed.
The sites have new database tables configured specifically for E10.
These
were setup under the old Solaris database server and that is the dataabase
environment that LDAS will use during E10. The plan is to create a
new S3
set of database tables under the new Linux servers for S3 once the
Solaris
databases can be migrated between the two platforms post-E10.
We have repeated our suite of regression tests on the LDAS pre-release
three
times this week and will repeat one final time on the final tagged
release
this Friday.
One of the newest regression tests confirming data integraty out of
the
frameAPI was run since last Friday night without any instances of data
corruption out of the nearly 100,000 repeats of the test.
We updated the known pulsar search scripts and short Fourier Transform
search scripts per recommendations from the LSC developers. We are
waiting
for updated instructions for the inspiral and power to allow us to
begin
testing against the latest LAL and LALwrapper releases.
The documentation changes this week will continue until close of business
today. After that, the official LDAS version will be tagged in CVS
and
the release built over night.
-----------------
E2E team (Bhawal)
-----------------
QND lecture
----------------
Kentaro Somiya of Univ. of Tokyo was visiting the 40m group. He gave
an
informal lecture of QND to a few people around. This was a nice introduction
to understand what is necessary to implement this physics in e2e simulation.
SimLIGO study
-----------------
Xiao Xu, sophomore, has started working with us, who has worked
as a
SURF student this summer.
He runs SimLIGO under different conditions and studies the effects.
His
first tasks are
(1) sensitivity degradation by the existence of radiation pressure
-
when locked, no degradation
(2) stability and performance degradation when the input beam
tilts
(3) stability and performance degradation when the cavity axes
have
offset with respect to beam axes
WFS
------
(Biplab) Effects of differential heating in arms on WFS signals were
studied
and some of the effects like sign-flip and changes in magnitude
that had
been recorded in experiments were observed in simulation. To
explain the
effects that could not be seen in e2e simulation, we decided
to use FFT
model.
The experiments at LHO are related to heating from an initial
cold state to
a medium-hot state whereas, due to the limited number of modes
in e2e,
the e2e results become quantitatively more accurate as the interferometer
approaches the final hot state.
Code development and maintenance
----------------------------------
AdLib code:
(Melody and Hiro) worked to make the new FUNC module using C++ compiler
work properly. The new FUNC module code is compiled, if necessary,
after
boxes
are loaded, and dynamically linked and used when needed. For
a FUNC with a
complex code, the speed gain is over 10. This method of using
dynamic linking
of C++ codes could change the concept of modules dramatically
and could make
the e2e system very flexible.
Several issues were found in a hard way. One is the setting of
stack
pointers. When a function in a shared library is called, the
stack pointer is
not properly set in a certain situation and the argument passing
failed. A
work around was found : at the top of the function body, insert
an
unnecessary
instruction to force the compiler to set the stack pointer and
place actual
body of the code.
A few code structure changes were necessary to use shared libraries
on
the fly. A new generic support was added so that modules can
request the
modeler to call certain functions just before the time loop starts.
Together
with initialize_before_run() function calls, the use of macros,
settings in
par files, data_in modules can change in the near future for
more clean
environments.
(Melody) Finished code reorganization for the framework to do the on-the-fly
compiling & dynamic linking. Tested the code base using
multiple and boxes
primitives. Continuing with code modifications to extend
FUNC_X to VxV
primitives and enabling backward compatibility to previously
created box
files.
Propagator module:
(Hiro) Yoshida and Tiffany found that a propagator primitive could
change the
amplitude of fields which should not happen. This was caused
by an
interpolation algorithm used in the module when the time step
was not exactly
the one way travel time of the field through cavity. The interpolation
has
been changed to apply to the amplitude and the phase, instead
of the real and
imaginary part. This reduced the unwanted effect by 1000. The
effect is
O(10^-14) and is very small, but the existence of this needs
to be kept in
mind when we are dealing with a wide dynamic range problems.
Fortunately, for
LIGO I, this fix did not affect the sensitivity curve.
Alfi
--------
(Bruce) Completed edit window initialization fix (PR 431).
-----------------------------------
Data Analysis Activities (Anderson)
-----------------------------------
(Shawhan)
* Went through the latest draft of the S1 burst paper.
* Worked with Kaice Reilly and Gaby Gonzalez to catalog time intervals
during the S2 run when calibration information is not available, which
turns
out to be the first and last partial minute of most locked segments.
These intervals will be flagged and incorporated into the
<a href="http://tenaya.physics.lsa.umich.edu/~keithr/S2DQ/S2seglists.html">
Segment Data Quality Repository</a>. Also, the current algorithm
in LAL
actually looks for calibration info one minute later than it "should",
and
the consensus is to revise this algorithm.
* Fixed conlog to construct its index correctly even when Epics controllers
have badly wrong system clocks.
* Verified that the frame files now being written at the sites contain
the
correct detector geometry information, the appropriate excitation channels,
and the slow channels which keep track of Epics timing discrepancies.
* Working on a new control-room tool called 'beacon' which continuously
compares the current control settings against an established configuration,
e.g. "science mode". This is to help avoid variances in the control
settings from one locked segment to the next, which happened some during
S2.
Hopefully, this tool should be ready for use beginning tomorrow afternoon.
(Creighton)
* Tracking down bugs in LAL 3.0.
(Weinstein)
* Prepared final (?) draft of S1 burst paper
* Working on hardware burst injection waveforms for S3.
-------------------------------------
LDAS System Administration (Anderson)
-------------------------------------
Caltech
-------
(Dan Kozak)
* Migration from 9940A to 9940B format tapes finished (several hundred
tapes).
* Continued to copy E7 data from HPSS (until HPSS went down on Wednesday).
* Worked with Sun to try to fix problem with part of /archive disappearing.
Following Sun's directions, reset 3510's FC ports to "point
to point only"
and upgraded FC swith firmware. So far, we've had no reoccurences.
* Received tapes from LHO and LLO with MDC data on them and incorporated
these into /archive. Some LHO data appears not to have
made it to tape.
Am pursuing the cause of/fix for this problem.
* Submitted problem reports to Sun about archiving continuing after
a disk
disappears from a SAM-QFS filesystem and some data not making
it to tape
(when moving data from LHO to CIT).
* Finished copying RDS from IDE-RAID into SAM-QFS at LLO.
(Al Wilson)
* Continue installing RH9 on desktop machines
* Fine tuning of BB on ldas-archive/dataserver
* Added sendmail fixes to cfdef
* Replaced motherboard in node210/cit Unit is running burntest
now.
* Used Ben's fix to reset the port 11 on blade 12 on the switch in cit.
(Stuart Anderson)
* Coordinate system upgrade tasks associated with LDAS S3 release
scheduled for Fri (Oct 17).
* Worked with Larry Wallace to order replacement motherboards for
all of the IDE-RAID systems we have to increase system stability.
* Tracked down the last LDAS server order (3 8-way Sun V880's) for S3,
and found that they are scheduled to ship Thurs Oct 16.
MIT
---
(Keith Bayer)
* Installed FC-AL card in 280R.
* Installed metaserver 1U unit into rack and am configuring it now.
* Moving data off of pcraid#3 in prep to swap motherboard.
Hanford
-------
(Ben Johnson)
* The disk2disk full frame copy script appears to be working robustly
at
both Observatories. I am presently working on the error handler/monitor
script, to further ease administration.
* Cut short the MDC run to 11:00 PDT Oct 16, in order to patch the FC
switch, reconfigure the 3510 RAID array, and turn on striping
for
/samraw and /samrds.
* diskcacheAPI stopped seeing new data on Friday Oct. 10, I had to
rebuild the frame cache in order to get LDAS to see new raw
frames.
* I updated the sendmail configuration on the ldas-jobs box, Oct. 15.
* The new linux metaserver has been re-partitioned so that hda and hdb
now have identical partition tables.
---------------------------
General Computing (Wallace)
---------------------------
MIT:
(Keith)
-Fixed desktop PC that wouldn't post with 3rd set of ram
(bad initial ram and bad replacement ram)
-Installed / replaced hdd in Dell laptop
-Investigating old penguin computing node that won't turn on
-Removing / shifting old users on gc filesystem to free up disk space
-Ordered software
-Obtained MIT site-license for Adobe 6.0
-Walking around to windows computers to force users to patch their
nodes
Livingston:
(Shannon)
-Spent some time making sure that we are fully recovered from last
weeks
disk crash.
-Received the server that was ordered for Jonathan as the PDM Works
server.Spent a couple hours setting it up. The next morning the
power
supply blew. ASA is working on getting me a replacement.
-Spent much of the night last night working on LDAP. I finally
got it
working with SSL so that the entire session is encrypted. This
is for
Solaris only so far, but I feel confident in deploying it at this
point. I will repeat the process again and document all of the
needed
steps.
-Expecting the new RAID disk server from ASA today or tomorrow.
As soon
as it gets here I will start working on it and burn it in. Afterwards
I
will begin moving GC files to it.
Hanford:
(Christine)
- A lot of user account activity this week. I added some users
to
additional groups, had to create several new user accounts, reset the
password on a few accounts and added several users to the lho-all e-mail
alias.
- Started investigating wireless access points and nat routers for
the
LSC meeting network setup.
- Helped get a new long-term visitor setup with a computer and place
to
sit.
- We are still being probed by hackers. I have blocked ping to
all
computers on the site, so the hackers started sending messages
requesting the address mask, another ICMP protocol message type.
I have
blocked that at the firewall and now the hackers are sending HTTP
messages. I am still working on a way to block the hacker HTTP
traffic
without blocking legitimate HTTP traffic.
- Spent some time in training for my upcoming S3 operator shifts.
- Spent time working on upgrades to my laser power and refl transmission
software for both here and at LLO.
CIT:
(Veronica)
- LIGO website: Set up and monitored VRVS for the last seminar; posted
the
presentation at the seminars webpage. Reworked a webpage for the 'Next
Seminar' announcement at the LIGO homepage.
Worked with Kip in providing him with a high-resolution image of a
Hanford
aerial shot. Kip decided to use a negative to generate a printer-quality
image.
Repointed the links fro the old PAC url to the new one. Posting updates
to
the Undergraduate Projects'03 page, internal bulletin board and fellowships
pages. Updated the roster database.
Met with other GC members to discuss a proposed makeover of the DCC
architecture. We agreed that the new system needs some further fine-tuning
but is an overall improvement. Continue working with George Stokes
on the
DCC issue.
Per a request from Larry, looking into web cameras with higher resolution
for VRVS. The last seminar was a successful test of a combined VRVS/VNC
setup and can be used for future seminars/meetings.
- LSC webiste: Posting daily updates to the website for the November
meeting, as well as updates to other parts of the LSC website.
- CaJAGWR website: Updated the seminars schedule webpage. Compressed
the
video of the last talk and transferred it to the streaming media server.
It is now posted along with the visuals. Provided user support.
(Mike)
-Reloaded a laptop that came back from travel that seemed to be having
problems with the operating system. It seems to be okay for now.
-loaded Linda Turner's old laptop that has been assigned to the loaner
pool. Mohanna is going to be using this laptop which she has requested
that
I load additional engineering software.
-Loaded and configured a NT 2000 Server for PDM/WORKS (this is for
Calum
Torrie) testing purposes.
-Loaded some additional software on Calum Torrie's workstation.
-Worked on a Hardware issue on our ghost server. This was a hard drive
failure that has lost multiple ghost images; I have tried to restore
them
with multiple tools that I have, but had no success. I have a lot of
ghosting to catch up on to get these images back on the server through
out
the weeks ahead.
-Problems with my office workstation. This seems like a hardware failure.
The cpu fan went out and now I my computer continues to crash. I will
have
called Dell and they are claiming that it is a software problem. They
have
asked me to reload this computer from scratch and if it happens again
then
call them back.
- Reload Millikan's conference room PC that is a dual boot computer.
The
windows OS ended up getting corrupted. I am reloading the windows side
once
again.
-I worked on VRVS setting up and testing multiple configurations that
included testing the share option in VRVS and also running VNC
concurrently. Then I tried to run VRVS on one computer then on an
additional computer I ran VNC transmitting the guest speakers talk.
The
problem we are having with the video conferencing is you can not read
the
guest speakers talk from the VRVS camera. This is why we are trying
many
different configurations to transmit a quality presentation. Larry
and I
will be trying a few more configurations using some additional peripherals.
-This week I had a lot of onsite user support that included software
&
printing issues.
(Lisa)
- Worked with Stuart to try and get a mail configuration for their
servers that
would properly masquerade e-mail from their cronjobs (using submit.cf).
- Updated apache and openssl on castor. That server had php compiled
with
openssl, but the new version of php was not compiling properly.
I am waiting
for a more stable release of php to come out.
- Demo'd a bayesian spam filter called dspam. I could not get
it properly
working on becrux. It would need to be compiled on acrux.
I'm going to look at
other packages before returning to this one.
- Began testing a package called CanIt for spam/virus filtering.
Right now I'm
not too happy with their support. They don't provide binaries
for solaris 8, so
I have to compile all their code myself.
- Dealt with a mailserver outage.
- Addressed a problem with a user who dumped 10Gb of data into a home
account
thereby filling up the disk and preventing others from working.
Folks, if you
need a big chunk of disk space, please talk to someone in GC.
We can
accommodate your needs if you let us know what they are.
(Larry)
-This has been a busy week with procurement issues. Mainly, trying
to get
invoices so I can get my P-card account reconciled.
-Assisted Mike on a number of PC related issues. The problems covered
h/w, s/w
and user implementation.
-Worked with the DCC on a number if issues including trouble shooting
the
upgrade of the s/w they are using.
-Working with Christine, Shannon and Ed C. with some of the logistical
issues
for the different meetings that are coming up.
-Worked with Mike and Veronica on the VRVS and VNC setup. We still
have a number
of items to investigate but so far things are looking better.
-We have moved over to the campus GigE backbone. I have been able to
spend a
little time monitoring the new installation. So far no major problems.
Still
have a number of performance checks to run.
-Touched on a number of projects which include: Updating the remote
control
room, Calcium Calendar tool and options, new servers for the 40M, new
sandbox
units for Hiro's group.
-Resolved a couple of hiccups with the servers.
-General assistance for the user community.
(Bruce Sears)
* Systems Work:
(0.5 days)
- Evaluated eNote for general LIGO use.
- More admin work on the JAWG Ilog.
Planning for and participating in the Advanced LIGO Suspensions Alignment
Workshop. Received two quotes for the RM blades.
We will review them at the weekly meeting Tuesday.
From: "Mark Barton" <maaku@attglobal.net>
This week I did some new impulse-response
tests on the LASTI MC
prototype. In these tests all 14 OSEMS were installed and being monitored
by the dSpace (as opposed to just the
6 on the top mass of the previous
tests). I participated in the AdvLIGO
SUS Workshop at Caltech and rewrote
several pages of
issues that people had. I also did a Mathematica
model of a LIGO-I style
two-wire pendulum to provide results for comparison with a test case
that
Virginio is using to debug MSE.
With ShallySaraf,
of Stanford, a short low-finesse triangular cavity was
fabricated. Right now the assembly is curing; hopefully the cavity
will be
ready for testing on Friday or Monday. Assembling such a short
cavity
presented some problems with the fittings used..
FROM THE CORE OPTICS WORKING GROUP TELECON:
Status reports for the CO Working Groups,
Meeting with JM Mackowski
took place at Caltech on October 6. Details in last
week’s report.
Garilynn: Sapphire Status
Nothing significant to report…
.
Bill Kells: Scatter
measurements in LIGO I
Hi Res beam spot images.
Have made a detailed study of the video beam spot images
on 2k optics under full
lock illumination: TMs (from
HR side); FMx (from HR side); BS (from split
side); and
RM (from AR side, HAM 9 video VP).
All of these were from BSC ports except for the
ETMs which were viewed from
the [short] spool positions (this to get as
normal as possible face view
to eliminate depth of focus problems). This allowed detailed
magnified views with minimum
optical zoom. In all cases a 75mm f1.4 video camera lens
was used with the addition
of an auxillary 2x magnifying lens (and
in some cases for the
frame grabber analysis two
2x lenses). The normal Watekccd
video camera was used
(also the Sony handy cams
were tried, with "super night vision" but had inferior S/N).
Typical images (with single 2x mag)
are attatched. A survey (just eyeballing
the images)
reveals:
1. The characteristic "globular cluster" of point defects
dominates the images as a whole.
However it is visually clear that the interstitials
between points is quite dark. It is this
background level (presumably
from inherent surface/coating "microroughness") that
motivated these studies. We
analyze the images to extract this (see below) by utilizing the
Spiricon frame grabber.
2. MOST of the optics have
additional flaw patterns: particularly bright point defects;
gouges; near verticle
streak patterns (cleaning?). These are exemplified in that attached
images.
3. For optics where the
beam is 45 deg. incident, the point pattern distinctively
"scintillates" with a bright/dark
frequency of 1-2 Hz. The ratio of bright/dark can be
dramatic: ~10x. The cluster
pattern does not uniformly pulsate, so that the integrated
scatter is very closely constant.
For instance it has been accurately established that scatter
(from all these optics) into
the integrating scatterometer detector is
precisely correlated in
time with NPTRX/Y). The scintillation
is clearly associated with the residual optics
motions. By driving the RM
(LSC ext.) this can be greatly accentuated. A third plot
(attached) shows a spectrum
response (the GDS_TEST_22 channel is the scatterometer
output while aimed at FMx
from BSC7 illuminator port) to the RM being driven
longitudinally at 0.6 Hz (260
units). The reference traces are for no excitation. An
upconversion
series is clearly evident. The fact that this series is absent in the NPTRX
trace is probable indication
of the scintillation "grating" noise. Whether this might be an
actual noise source in detection
is not clear.
4. More detailed studies of 2kBS(face
view) ant ETMy (short spool view) were
conducted by Spiricon
frame grabber. These two optics showed the the
least additional
flaws (point 2 above) A full
analysis of this will be forthcoming. The object was to
determine what fraction the
"globular cluster" point scattering contributes to the total
scatter (loss). The strategy
was to grab two images, one sharply in focus, and a second
with the image strongly defocused
(via the 75mm lens focus ring). Then the level of
interstitial minima (focused
image) could be compared with the mean level of the
"smoothed" defocused image
(which presumably has the same Net scatter). This scheme
works but is technically limited.
The focused image still has some significant point
spread function (thus limiting
the depth of interstitial minima). The defocused images
suffer from coherent light
"speckle" patterning (never become completely smooth).
However it is clear from extensive image disection
that the scatter from the globular
cluster substantially dominates
the scatter, at least by a factor ~3 over any diffuse
background. This must be taken
as only a lower limit.
See image at:
http://apex.ligo-wa.caltech.edu/ilog/pub/groups/detector/logs/2003/images/10/13/BillK-
1066074717.pdf
Elog entry link:
http://apex.ligowa.
caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/13/2003&anchor_to_
scroll_to=2003:
the previous image was of
ITMx HR (GBnote: newly installed) face shot
at 45 deg from
the video camera
in both that defocus, side
to side is evident due to the depth of field.
See image at
http://apex.ligo-wa.caltech.edu/ilog/pub/groups/detector/logs/2003/images/10/13/BillK-
1066074954.pdf
E- log entry link:
http://apex.ligowa.
caltech.edu/ilog/pub/ilog.cgi?group=detector&date_to_view=10/13/2003&anchor_to_
scroll_to=2003:
Ju Li/David Blair: High
Optical Power Test Facility Project Summary (
Thermal lensing simulations:
Even with the compensation plate,
thermal lensing correction for Gingin Test 3 remains a
challenge.
The compensation plate restores the original power recycling cavity modes
but
cannot
change the ‘hot’ arm cavity modes. So we can expect a serious mode mismatch
between
the laser modes and the hot arm cavity modes. Due to this mode mismatch
the
carrier
power circulating in the FP arms will be divided by 2.
Solution investigated:
- Heating ring to change the radius of curvature of
the ETM, not practical for
Gingin (required too much radiative
power).
- Dynamic mode matching, seems to be a promising solution
but difficult to
engineer.
- Change the ‘cold’ mirror radius curvature to include
the possible thermal
expansion. I don’t recommend
this solution.
The Mach-Zender interferometer
using to test the compensation plate is having a major
hardware upgrade (new optics).
Gingin High Power Facility update
The last few items are installed in the laser hut,
which will make it ready to be cleaned
down next week. Then the installation
of the laser will start. This will be a 500mW laser
initially, to be replaced
by the 10W laser. The pre- mode cleaner will be installed
consequently, from which point
the mode matching for the 80 m cavity will be set up. A
10 MHz phase modulator is installed to provide the
RF sidebands for locking the laser to
the cavity.
Group meetings for integrating the local control and
the global control are instigated.
More attention is needed for a smooth operation of
the local control of the isolator
system. Initially the LIGO
SOS will be used for damping the test mass motion. In the
case when the residual test
mass motion is to large, DC to ~20Hz feedback to the LIGO
SOS will be applied.
Baking of the central tank will take place early next
week. This will take up the next 5 to
6 weeks. In the mean time, the cleaning and baking
of the isolator part will be started. A
large portable clean room
assembly tent is under construction which is used to cover the
open tank when the isolators
are installed. John Jacobs is in contact (or will be soon) to
ask for LIGO technicians to
come over to help installing the LIGO SOS.
Materials report from
At
in each of the modes of the samples used to calculate coating losses;
shear plays no part in the coating thermoelastic damping so we need
this
information to calculate the thermoelastic damping correctly. We
are now in the process of gathering this data for the 3" x 1" and
3"x 0.1" silica discs.
Gregg and David Crooks have been comparing their respective codes used
to calculate 'Intrinsic' thermal noise and thermoelastic coating noise.
After initial discrepancies the two codes now essentially agree, with
one or two points of difference only remaining.
EoinElliffe has
been running some FE models to check the effect of
including the finite size of the test mass on expected coating thermal
noise and we are comparing results from this with the calculated thermal
noise for a half infinite test mass.
RE: recent discussions with JMM on plans for future plans for coating
runs - the following is extracted from Greggs
summary of discussions:
> > 2 - We tentatively agreed that he will provide two small
> > coater runs of monolayer coatings, one each of silica and
> > tantala. We agreed on a canonical
thickness of 2 microns.
> > He (the vendor) felt any thicker would seriously distort the
> properties of
> > the layer. We will check to see if this thickness will work
> > for Q, absorption etc measurments.
Sheila checked with Ira Wygant - the
Stanford student making
measurements of coating young's modulus - whether this would be a
suitable thickness, currently his setup is optimised
at 5 micron
thickness and sensitivity drops signficantly
for a 2 micron coating.
From: Eric Black <black_e@ligo.caltech.edu>
Here is a description of our photothermal experiment. We have finished a paper on it, including how we extract both the thermal expansion coefficient and thermal conductivity of a coating. Link to a copy at my website is
http://www.ligo.caltech.edu/~blacke/0310194.pdf
SUSPENSION
Attending the SUS conference. Set up an autocollimator demo for aligning
the Triple suspension prototype. Preparing slides
and a presentation to describe the initial alignment of the LIGO1 IFO using
the
PHOTON DRIVE R&D
Awaiting replacement of the 500 mW laser.
For additional information about this report, contact sanders@ligo.caltech.edu