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The LIGO Executive Committee Agenda for Monday February 11, 2002 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 1:00
Why are we doing this? Our current provider has done a fine job for many years. But Caltech has decided at the highest levels that the Institute can get a better deal by combining the entire Institute's purchasing power in one place to get the best discounts. Of the roughly $2 million per year in Caltech travel, LIGO is about 25% of the total and is by far the single biggest group doing Caltech travel. If we do not support this move, we undermine the possibility to make the best travel savings. I see no reason to withhold our support of this laudable goal. Caltech had a solicitation and Montrose Travel made the best case by far, according to the selection committee (Ed Jasnow served on this). In addition, I see several new and valuable services available to us. Web booking, excellent management reports on costs, potential savings, and on travel policy exceptions.
Therefore, I ask each of you to fill out the Traveler Profiles and start to use the Montrose capability.
I strongly urge that you make use of their web booking capability.
As part of this, the travel policy rules will be changed to align better with Caltech's emerging travel policies. I have asked Irene to defer to Travel Audit for rulings on permitted travel practices. This will evolve as we and Montrose and Caltech settle the policies and I will work with Ed and Irene to make LIGO-specific policy decisions. In the meantime, continue as you have been in making arrangements but do this through Montrose.
Remember, we are doing the public's business. We are to conserve public resources and travel in a thrifty and prudent manner. We have done well in this respect to date. We should continue to save those tax dollars at every opportunity.
Please direct any questions that you have to me and to Irene. Irene can provide the needed Montrose contact information.
GHS
laser telecon minutes in Adv. R&D section below
LIGO Operations--Administration
A Site Teleconference was held on Thursday, Frebruary 07, 2002. Discussion included the status FY 2002 costs-to-date, of NSF funding and the Cooperative Agreement, the establishment and budgeting of FY 2002 accounts, the FY 2002 Financial Reporting format, as well as the status of the construction at the two sites.
Budget status: we are spending at a rate of 65 percent of the Operations budget through January, but the first few months of the fiscal year are historically slow. Labor is running at about 80 percent of budget. It was noted that some procurements have been delayed because we have not yet received funding for FY 2002 from the NSF. NSF expressed the hope that the cooperative agreement would be approved by this weekend.
We have emphasized with the Contractor for the building at Livingston the importance of having the auditorium available for the LSC meeting in March. We also seek assurance that we will be able to efficiently work through any open punch list items. An action has been assigned to explore possible ways of providing power for laptops in the Livingston auditorium. An action has also been assigned to develop plans for 1) how the buildings are going to be populated, and 2) how the new building is going to be outfitted. It was noted that the total cost of furnishing the building is now in Operations, and yet to be determined is how much reserve will be available.
Question: will the audio/visual system in the auditorium at Livingston provide separate connections from the podium for each of the two projectors?
Excess property cubicles have been received in Livingston and appear to be in good condition.
A location has been proposed for the Weber Bar displays at Livingston. A location has not been finalized at Hanford. Everyone is reminded that display materials must be submitted to the University of Maryland for their review.
The list of current actions revised to reflect
the status of open actions assigned through February 07, 2001 may be found
at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
ACCOMPLISHMENTS
ACTIVITY
| 02/07/02 | Packages | Faxes |
| In | 44 | 44 |
| Out | 07 | 38 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
CONSTRUCTION:
SUPPORT
INFORMATION
The new format Roster is online. Click
the Staff Directory/Roster link at the top of the LIGO home page.
FROM Caltech Weekly Update February 4 - 10, 2002
- - -
VOICE MAIL INTERRUPTION - NOTICE TO CAMPUS
There will be no Caltech voice mail service from
11 p.m. Saturday, February 16 until 3 a.m. Sunday, February 17. During
this time, we will be adding more capacity to our voice mail system. There
should be no impact to existing messages, greetings and passwords. For
additional information, please contact Dawn Boyd, ATC Telecommunications
Office, ext. 3881. Details: http://atcaltech.caltech.edu/news/item.tcl?news_id=4975
Progress Period from 02.01 to 02.07
Accomplishments:
We are doing a standard Annual Report for the Construction Project as of the end of November. Started working on the report again. Work was interrupted by Audit questions and by need to review budgets. In particular, a review of the current status of the FY 2001 Advanced R&D costs and the budgets assigned for FY 2002 was overdue. An approach has been selected. We will be closing out most of the current Advanced R&D accounts for any more costs and transferring everyone over to the new accounts immediately. The exception will be the soft seismic studies.
The following change request has been submitted:
| CR-010012
Revision B |
WBS 1.4.4.1 | Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites | P. Lindquist |
Press for the latest Contingency Needs Projection.
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
No report this week.
----------------
LHO General
----------------
Most of the work was accomplished in the commissioning area. Please
see
Stan's report.
---------------
Facility
---------------
A five ton crane was installed in the Staging Building. Electrical and
additional work on the building columns remain before the crane is
usable.
Commissioning activities: We tried alternative locking schemes for the recombined interferometer. It is possible to lock the recombined interferometer by locking the arms separately. This may aid in locking with high seismic noise. The ISC tables were prepared for recycling. This included a clean up of the optics, a documentation of table layouts and the debugging of the electro-optical shutters.
CDS: Rolf visiting LLO. Upgraded the Frame Builder LLOFb0 and the Frame
Broadcaster Tested and installed the new 2 omega I & Q board into 1X9.
Received boards back from Fiber Options for the cameras at the west end
station. Performed a custom board inventory - the list can be seen via
a hyperlink on the CSD
web page. Changed LLOFb1 to produce 16 sec frames. Upgraded all the
control room machines to Solaris 8. New Dataviewer version 6.0 installed.
New version of DTT also installed. Last week created an epics interface
to the DMT's BitTest program to look at PEM channels on MEDM screen. Setting
up the Ultra 60 as an upgrade to existing london. LLO2 cds server has been
setup but its not replaced LLO1. ATM switch rebooted on Thursday. (Chethan)
LDAS:
Installed DB2 products on sunbox1 to experiment with restoring backups
(does not work across platforms). Successfully restored on sunbox1 the
database backed up offline on metaserver. Successfully restored on sunbox1
the database backed up online on metaserver rolling forward to the end
of logs. Shipped 4 tapes with E7 data to MIT. Together with Shannon prepared
the inventory list of LDAS equipment at LLO. Repaired d2 metadevice on
gateway.Read DB2 SQL reference. Investigating the possibility of using
federated database configuration in LDAS.Updated the release of java 1.1.8
on metaserver and sunbox1 to be used with db2cc. (Igor Yakushin)
Testing an eight port serial card for controlling the various LDAS UPSs in the mass storage room. Results are looking promising so far. I hope to work on this more after the LSC is over and have something going quickly. Received the electronic license for QFS for the new "dataserver."(Shannon Roddy)
GC: Ordered some wireless access points and some wireless cards for
use in the new building during the LSC. Looking into a problem with one
of the linux machines here locking up for no apparent reason. This happens
to be the machine that Snort is running on. Trying to decide if it would
be worth while to remove the databases for the web site from of the
web server to a different machine and have a dedicated database server.
It would be beneficial in several ways, but would take some work on the
web pages. Ordered a laptop to replace an older one (~5 yrs. old) that
has died. Ordered a case with higher cooling capacity
for Igor's GC machine. It was having heat problems. Still working with
a company in Baton Rouge that may be able to provide us with a high speed
network to LSU.
Optics and Installation: Gary and Harry completed the installation of
the PSL acoustic enclosure, which required the installation of toggle clamps
to safely secure the table access plugs. Caution to registered Users! These
plugs are VERY heavy(~125#), and awkward. Do not attempt to remove them
without another person to assist you. We will post a reminder warning on
the plugs. A general cleanup of ISCT1 and 4 is ongoing, in anticipation
of resuming commissioning in a recycled state. EO shutters on ISCT-4 and
1 have also been reinstalled. Optical lever laser on MMT-3 died (old style)
and Gary replaced it with the iFLEX1000's supplied by Mike Zucker. Thanks
to Harry Overmaier for coming in Monday (his day off) to work on the ACAD
drawings of the ISC tables. (Jonathan Kern)
|
|
|
|
Installation&
Commissioning:
Livingston |
Other
Science/EngineeringActivities:
Issues/Concerns |
See also the Installation web page
Work continues to settle into operation at
6 W power into the modecleaner. The inital configuration used neutral
density filters in front of most detectors to give the same amount of light
as prior to the increase. We have now removed these from in front
of the SPOB and POB photodetectors, compensating for the increased optical
gain by turning down subsequent electronic gain. In doing this we
encountered a couple of faulty gain controls on the whitening filter boards,
and have repaired them.
Still trying to understand the locking behavior
of the 4 km interferometer. We have had a few extended locked sections
(including our current record of 36 minutes) but these are few and far
between. More typically, we get 10 second locks, with still no clear
indications of what causes it to lose lock. Early suspiscions about
limited range in the digital suspension coil drivers do not appear to be
the problem.
Corey and Ski made measurements of the digital suspension coil driver noise for all of the LVEA optics. We haven't had time to digest them all, but it looks like we will need to make some improvements.
Copying from the2 km we we tested all gain controls on the 4 km whitening filter boards. We found one step did not result in a gain change but a minor change to the EPICS database fixed that.
Improvements in the noise of the recombined interferometer in the
100 Hz region have been made by:
The antisymmetric wavefront sensor does not give useful error signals in the recombined interferometer although it is known to function in the recycled interferometer. We are urging the interferometer modelers to establish if this is an intrinsic property of the sensor.
Upgraded FrameBuilder at LLO(LLOFB0) to write 16sec frame files;
DAQS controller code also updated. LHO and LLO DAQS should now be
the same, with the exception that LLOFB0 writes to its internal disk drives
and I believe the corresponding unit at LHO writes to Sun T3 drives using
QFS.
I have been working a lot on analytical calculations since Mathematica
is not dealing well with symbolic operations even giving the correct assumptions.
The results for the two by two model that takes into account scattered
light from one mode to another in the recycling cavity because of some
perturbations are put in a final form that is not difficult to interpret
at all and despite the complexities of the mid-steps the output is sensible
in each of its parts.
The study of the mismatch in the radii of curvature is going on and this requires a bit more of sophisticated evaluations because the Guoy phase is affected by this kind of perturbation.
Bill Kells
Continuing saga of the SB im balance phenomenon. More issues keep emerging!
Now we have determined that the MELODY code is not doing exactly what would
have been imagined. It can parametrically be restricted to only two modes,
making it nominally equivalent to the "Modal model". However there are
disagreements. Other issues being wraped up.
MCCMs and MCFMs were received from Wave Precision where they were
being repolished. They have been measured and have been shipped to
REO for coating. REO expects to deliver by the end of March.
Radius of curvature results obtained at CIT are longer than expected,
see http://www.ligo.caltech.edu/~gari/COCAsBuilt.htm
CIT metrology uses a flat reference and so can only measure the central
~25 mm diameter of the optic before running into the Nyquist limit.
These measurements are repeatable. The initial LIGO 1 mode cleaner
optics were not measured at CIT.
Wave Precision uses a test plate to measure the ROC, they report matching
to that test plate. This metrology should produce the same results
as were obtained for the initial LIGO 1 fabrication. The ROC is expected
to change after coating, so the mirrors will be measured again after being
returned from REO.
Lee Cardenas
Finally, after a very careful alignment the 2nd Contamination cavity
is performing properly. Now we can see modulation signal that we could
not see it before. We are in process to lock the cavity. The first
cavity, new mode match made and alignment completed but still can not get
a strong dip signal. A careful and precise alignment is in process.
Bill Kells
Working more intensely now in OTF to get contamination cavities locking,
This in anticipation (now fulfilled) of visit by Jordan to pass judgement
on what we are facing (that is puzzling symptoms that have not allowed
reliable locks so far). We have absorbed his comments (concurring that
things, alignment?, are not what they should be. Pursuing this more now...
Requirements were discussed with Rai Weiss. A draft statement of the isolation and damping requirements is in preparation for review by the group.
An analysis of the isolation performance of the hydraulic pre-isolation system was released by Brian Lantz, et. al. and is being reviewed by the group.
Joshua Phinney (MIT, grad student) reported on his transmission line analysis and testing for the hydraulics. He recommends use of an accumulator at the load end. The team is reviewing his analysis.
Performance testing of the initial version of the hydraulic actuator has been completed at Stanford. The performance is good, with a reduction of the ambient seismic noise to the noise floor of the displacement sensor (an optical shadow sensor), or a factor of 25. More loop gain is available for further reduction around 1 Hz. We hope to drive to the noise floor of an inductive displacement sensor (1e-9 m/rHz at 1 Hz)
Initial testing of the bellows breathing mode resonance for the new, modified bellows was higher (better), but not as high as hoped for. We may need to move ahead with the current bellows design for the LASTI prototype system, while in parallel exploring further improvements in the bellows design.
David Shoemaker reported on the status of selection of an electro-magnetic actuator (an alternate to the hydraulic actuator). The BEI actuator that was selected for the advanced LIGO stiff ETF prototype (a modification of a commercial off-the-shelf unit) looks promising.
WORK SPACE: A satisfactory area has been found in the CES building to set up the system, it will take 2 or 3 working days to prepare.
LAYOUT DRAWING: I have started a layout drawing of the location of the components on the granite base, and configuration of the plumbing.
MANIFOLDS: Station 1 and 2 and test load have not been started yet.
LONG TUBE RUN: Design of a method to assemble, support and isolate the 360 foot tubing run is in progress. Test taps at the 60 foot mark [shortest run] and 180 foot mark.
Additional parts and hardware have to be located and ordered. Final word on the accumulator, electronic pressure sensors, resistor configuration, and test load requirement from the Stanford group is hoped for soon, final layout and parts purchase require these components be defined.
An 80 MHz VCO and AOM were shipped out to LASTI. Prior to
shipping the maximum output power of the VCO was checked and was found
to be 2 W. This output power may have resulted in damage to the AOM,
which is only rated for 1.6 W. An internal attenuator was replaced
to limit the maximum output power to just over 1.3 W. The response
of the VCO to the RF amplifier AGC input was measured.
The remains of the VCO originally shipped out to LASTI underwent an autopsy. It was found that the AGC input to the RF amplifier was not working and the LT1125 controlling the modulation level was faulty. I'm not sure how this may have happened but an AGC input voltage of greater than 5 V might be the culprit.
New bake oven- insulated blankets being made and attached to and
plumbing in process.
Small bake chamber(for small parts), rough pump oil leak has been fixed
and plumbing restored and it is under vacuum now, Baking in process .
New Dycor RGA, PC comparable has been installed and it is in use to
RGA scan the bake chambers.
RGA scan and graph of the baking has been sent for approval.
Received loaner 2Gbit/sec reflected memory boards, one for VME PMC
site and one for Sun PCI. We want to test them for use as the connection
between the DAQS controller and Framebuilder(s). This link is presently
a 262Mbit/sec link and is the limiting factor in the DAQS acquisition capacity(~10
MByte/sec actual throughput). The Hanford DAQS already runs at consistent
data rates of 9MByte/sec on this link, which does not allow much margin
for additional data channels. Alex is working on this test, primarily the
drivers needed on the Sun side of this link.
Revised drawings have been completed for addition of pole/zero module
and rev B sos coil drivers to the mode cleaner mirrors. Pole/Zero modules
are fab'd and being tested. SOS coil driver Rev B modules should be tested
by the end of the week. We should be ready to install and test the system
at LHO next week.
Lori is working the the CDS standard digital filter code. Code for
Pentiums is ready for test and EPICS interfaces for testing are about ready.
We should have some timing and test results by next week.
Despite promising published specs, a previously untested alternate
for the troubled EG&G/Perkin Elmer InGaAs PIN photodiodes did not pan
out. The JDS/Epitaxx ETX 2000 had junction capacitances of 200 pF (back
biased at 7V, meas. at 25 MHz), vs. 140 pF seen for recent ("bad") EGG/PE
diodes and 75 pF for our original batch of ("good") EGG/PE diodes. For
context, the signal-to-electronic noise ratio in our application goes roughly
like 1/(capacitance squared). It is not yet clear if we can recover
adequate SNR for the dark port by re-optimizing other circuit parameters
to suit the degraded diodes.
An additional EGG/PE QA problem, debonding of the die from the case in some of the diodes, is still under investigation by the manufacturer.
One mitigating factor may arise from the better-than-expected "darkness" of the dark port seen on the H2k. If this holds up on all three machines at full power, we may get away with relatively few super-quiet diodes (perhaps 4 per IFO, vs. 8 nominally anticipated).
Delivered one unit to LHO for spare. The one intended for LLO spare
has a high voltage power supply failure and is currently waiting for replacement
part. In the process of ordering parts to build three new ones for 40M.
Waiting for the LEMO connectors to start building the four new units
for the 40M
Preliminary design of the remote interface box is complete and schematic
will be circulate for peer review before starting PCB design next week.
The very nice and informative TAMA talks, describing the status
and achievements of the project to date, were accompanied by excellent
status reports from all the gravity wave detectors worldwide. Fred Raab
described the present status of the LIGO project, Harald Lück brought
us up to date on the GEO status, Matteo Barsuglia gave us an overview of
the VIRGO status and commissioning and David Blair highlighted the recent
successes and plans of the Asutralian consortium. I was invited to gave
a talk on the status and goals of the Collaborative (Network) Data Analysis
effort. I put special emphasis on the Network Data Analysis Server development
effort, in the light of the very recent decision of TAMA to support this
effort. I am working with their representative on the technical details.
I assembled and tested the my drift servo module for the second
tower, which is very close to completion. This servo is one of the LIGO
contributions to the project. We have near term plans to extend the capabilities
of the module (software extensions).
Noise reduction in the photothermal experiment continues. We discovered
that the mixer was underpowered, leading to bad PDH signals. We decreased
the power in the modulated beam from 50mW to approximately 2 mW, to
avoid
heating the Al mirror, clipping the signal in the electronics, and
scattered light contamination in other optical paths. We were
concerned
that there might be too much power in the sidebands for the
low-modulation-depth approximation of the PDH error signal to be valid,
so
we built a
higher-finesse (about 200) fixed length cavity from stock mirrors to
analyze this beam, and found that 2.7% of the light power of the modulated
beam is in the sidebands, with RF power to the EOM of 16.5 dBm.
We also
verified that the laser's fast input has a transfer function of 6.3
MHz/V
at low frequencies.
A good part of the week was also spent preparing for Thursday's TNI review.
LASTI (Bayer, Fritschel, Harry, MacInnis, Mason,
Miller, Mittleman, Ottaway, Rollins, Shoemaker, Zucker)
=======================================================================
VACUUM ENVELOPE:
We had a visit from Steve Foster, Pfeiffer Vacuum's product manager
for mass spectrometers. He showed us workarounds for some of
the more
annoying bugs in our QMS421 RGA software, and we're now getting
higher dynamic range by defeating the programmers' intent. High AMU
partial pressures in LASTI remain excellent, but we're still
puzzling over the air
signature.
We began staging to relocate the pump system further
from the BSC at the next vent cycle.
HYDRAULIC ACTUATORS:
Hosted a successful visit by Dennis Coyne, Gerry Stapfer, Brian Lantz,
and Joe Giaime to work technical and programmatic issues for the LLO
pre-isolator retrofit.
The need was identified for a broad characterization of BSC stack and
support pier modes and reactances to plan the pre-isolator control
dynamics. This will be carried out over the next 4 weeks in LASTI.
A
suite of at least 12 acceleration/velocity sensors is required to
support this test. We're trying to recall accelerometers, seismometers
and geophones which have been dispersed to other sites, but haven't
succeeded in locating everything yet.
PLEA: if you know of vibration
excitation or monitoring equipment
in your lab which might
be "on loan" from another site (for
example, MIT) please email
Mike Z. and/or the party responsible
for that equipment so we'll
know where it is.
On the mechanical pre-isolator design Ken reports:
Completed several design modifications resulting from the meetings
held
at MIT over the past week. The following design changes were made:
1. Springs were moved inboard of the pier to allow for easier access
to
actuators.
2. The housing asembly was modified so that it could be used in either
a
RH or LH orientation.
3. The housing assembly was modified to use either hydraulic actuators
or the BEI electromagnetic actuator.
CDS/DAQ/GDS:
No problems to report.
PSL:
Replacement AOM and driver were received from Peter King at Caltech
and installed successfully.
The PMC modematching has been optimized; the power transmitted though
cavity is 8W for 9.7 W incident on it. The reflection dip was measured
and found to be 11.5%. The reflected light was analysed by studying
the
power found in the higher order modes. It was concluded that the
majority of the residual light on reflection is caused by a poor
spatial mode in the horizontal plane (earlier measured to be M^2=1.3)
This probably cannot be improved by improved modematching outside the
MOPA, and only a realignment of the laser head is likely to fix it.
#MZ
note: further realignment is not a priority, as the
transmitted
power is already more than adequate.
Simulation and Modeling (Bhawal)
Modal Model (Hiro,Biplab,Matt)
------------------------------
The effect of the change of the input beam basis was studied. At least
to the first order,
the phase change due to the curvature mismatch cancels out the change
of the guoy phase.
Due to this cancelation, the cavity length change predicted by e2e
before turned out to
be incorrect, and will be much smaller. Further calculation and the
implementation in e2e
is in progress.
LIGO I simulation system
--------------------------
(Matt) I built the LSC analog electronic sub-system, largely taken
from Luca's updated
model. I am currently building the LSC digital system.
Code development and maintenance
---------------------------------
(Biplab) A discrepancy in transfer functions from L+ mode to Asymmetric
Q signal
observed by Luca could be solved by taking into account very little
time-differences
among various partial beams bouncing back and forth inside the recycling
cavity.
A few lines are added in the recycling summation cavity module.
(Ed Maros)
- Updated build instructions for e2e software
- Created release of e2e software 1.7.4
- Installed and created run script for alfi5
Alfi
----
(Bruce)
- Beta release of Alfi5 completed.
- Debugging newer parser elements (like #quote).
(Melody)
- Released an alpha version of alfi5 (Java version).
LIGO Data Analysis System
Software Systems (Blackburn)
The LDAS startup procedures have been modified to run each API under
a
unique directory. This is to avoid clobbering core files in ill behaved
software and will facilitate debugging efforts. Additionally, the nightly
builds of LDAS are now using -no_in_lining to provide better source
level
debugging information. This speeds up build times but has caused code
to
run 3 or 4 times slower.
The abortJob malfunction that was discovered in the E7 run has finally
been tracked down and fixed. A similar coding bug which existed in
the
lightWeightAPI was also fixed, though it was not the source of any
issues
discovered in the E7 run.
The controlMonitorAPI now support monitoring database insertions and
queries. Filters are available to look at individual users and a plotting
package is integrated to allow graphing usage of database over time.
The LAL modification to the wrapperAPI to support generation of a list
of channel names and providing a comment to the search codes continues.
The
skeleton changes are in place but the lexical parser being integrated
from
other sources fails at runtime. This should be fixed in a couple of
days.
Also the requested modification to provided more timing statistics
is now
in place and working. Information is stored in the log files. The other
open request for a -userTag passed by the search codes is now available.
The cycle of develop, test, fix, develop... continues with the new
diskCacheAPI/frameAPI upgrades to LDAS. Most things are once again
working
but there is still some irregular behavior that is being tracked down
and
fixed.
Guild was modified so that it displays estimates of data volume and
execution time when requesting frame data.
Continuing to work on resampling/linear filtering in the new "filters"
library. The library has now been created in CVS and was in last night's
build (although omitting one file by mistake broke the build). Directories
src, test, doc, doc/html have all been added including the Perceps-generated
documentation (at some point Ed will need to add graphics to the software
layout diagrams for the library)
Added EXTENSIVE testing to LinFilt and have started doing so for
Resample. New testing aggressively verifies linear filtering in the
following way: a continuous data stream is first filtered "as a whole"
and then broken up into three components which are filtered separately.
The results from both are compared for an exact match. Every possible
way of partitioning the continuous data stream is tried eg. for a length
10 input we filter 3 segments with lengths 1, 1, 8 then 1, 2, 7 then
1, 3,
6 and so on.
Planning to do similar testing for Resample. An issue which came to
light today is that Resample produces significantly different results
than
Matlab, which may be intentional but I don't know at this point. This
discrepancy is present in the existing dataconAPI Resample class.
Hardware Systems (Anderson)
Caltech
-------
(Dan Kozak)
* Finished splitting up the large directories in the LIGO HPSS archive.
* HPSS migration from 3590s to 9940s continues and has been somewhat
automated (there have been a lot of unrelated HPSS problems since I
started running the new script, so it's hard to tell how well it's
going to work long term, but I'm optimistic).
* Fixed various breakages in HPSS (deleted core files, restarted servers,
added tapes to storage classes) including a big "restart the whole
thing" one just this morning.
* The Ultra 10 has been working fine with the LIGO supplied memory.
Still
waiting on StorageTek to make good on coming up with some replacement
memory.
* 10 (electronic) QFS licenses obtained for Caltech machines.
(Al Wilson)
* We have a working BigBrother setup on the ldas-test system. It will
be the
template for other LDAS installations. It will migrate to the other
Caltech
system by the end of the week. In two weeks it will be running on all
of the
LDAS installations.
* Still have not given up on a simplified Kickstart configuration. I
am
meeting with the Redhat guru at CACR. I will get this one yet.
* There are now cabinets at Millikan and at Synchrotron for LDAS books
and for spare parts, start using them.
(Stuart Anderson)
* Finished archiving all of the E7 data into the LIGO archive at Caltech.
* Reworked the LDAS HPSS web page catalog generating script to handle
the
large number of files (~370,000) more efficiently, i.e., now
able to update
in less than 24hours which is useful since the contents are
updated
daily.
MIT
---
(Keith Bayer)
* Received permanent QFS license.
* Received UPS stand-alone unit.
* Received E7 "playground data" tapes from Hanford and Livingston.
* Loaded Livingston tapes.
* Loading Hanford tapes.
* Moving ldas-sundev1 back to LDAS lab.
Livingston
----------
(Igor Yakushin)
* Installed DB2 products on sunbox1 to experiment with restoring backups
(does not work across platforms).
* Successfully restored on sunbox1 the database backed up offline on metaserver.
* Successfully restored on sunbox1 the database backed up online
on metaserver rolling forward to the end of logs.
* Shipped 4 tapes with E7 data to MIT.
* Together with Shannon prepared the inventory list of LDAS equipment at LLO.
* Repaired d2 metadevice on gateway.
* Read DB2 SQL reference.
* Investigating the possibility of using federated database configuration in LDAS.
* Updated the release of java 1.1.8 on metaserver and sunbox1 to be
used with db2cc.
(Shannon Roddy)
* Testing an eight port serial card for controlling the various
LDAS UPSs in the mass storage room. Results are looking promising
so
far. I hope to work on this more after the LSC is over and have
something going quickly.
* Received the electronic license for QFS for the new "dataserver."
Hanford
-------
(Greg Mendell)
* The data for the time intervals listed in the files PlayH1noH2L1.txt,
PlayH2noL1.txt, and PlayL1noH1H2.txt at
http://www.phys.lsu.edu/faculty/gonzalez/E7Segments/ has been sent
to
LDAS MIT on tape.
* Most of the last week has been spent writing and debugging a script
to control LDAS jobs to produce SFTs. The script is basically
ready to
go, once locked an clean segments are identified, and certain issues
involving the quality channel are worked out.
Data Analysis Activities (Lazzarini)
General Computing (Wallace)
MIT:
(Keith)
-Salvaged/refurbished/butchered/swapped PC's around labs
-Hooked up networking to NW22
NW17-tp<->SC<->SMA--to NW22---SMA<->SC<->switch
-Continued to install MU6 on Sun machines
-Installed o/s on new dell for conference room
-Installed video conf software on new dell
Livingston:
(Shannon)
-Ordered some wireless access points and some wireless cards for use
in the new building during the LSC.
-Looking into a problem with one of the linux machines here locking
up for no
apparent reason. This happens to be the machine that Snort is running
on.
Trying to decide if it would be worth while to remove the databases
for the web
site from of the web server to a different machine and have a dedicated
database
server. It would be beneficial in several ways, but would take some
work on the web pages.
-Ordered a laptop to replace an older one (~5yrs. old) that has died.
-Ordered a case with higher cooling capacity for Igor's GC machine.
It was
having heat problems.
-Still working with a company in Baton Rouge that may be able to provide
us with
a high speed network to LSU.
Hanford:
(Christine)
- Set-up a new Win 2k PC.
- Provided user support for various problems.
CIT:
(Veronica)
- LIGO website: posted updates to various parts. Working with Larry
and
Mike on troubleshooting of the Amaldi NT server where the Elba GWADW
webpages and Amaldi99 Proceedings reside. Mike has set up a temporary
backup server until the old one is fully restored. Posted the new LIGO
roster. Edited and posted the LSC March meeting announcement; rewrote
the
registration form. Looking into the setup of the meeting's transparencies
webpage.
- LDAS: Working my way through the CVS manual and LDAS website directory
tree.
- Project Science Jan 18-19 workshop: Added minor changes to the database
of contact names.
- CaJAGWR: posted the new seminars schedule. Posted a pointer to Luis
Lehner's talk (pdf and animation's). Compressed and installed the video
of
Luis's talk. Contacted about the availability of 155 Arms lecture hall
for
CaJAGWR and LIGO seminars.
(Lisa)
- Replaced castor with betelgeuse for Phil Willems
- Larry put the new mail server in place. Mike and I worked on
the little user
glitches that followed -- mostly deleting secure shell host keys.
- I spent a lot of time refining the mailman set up. We have
a pretty good set
of defaults and a policy in place, but I haven't yet finished the documentation.
(Mike)
-Restored a couple of PC's that had been infected with a virus. The
units needed
complete rebuilds.
-Worked on the cleanup of ssh for the users needing to tunnel their
Eudora with
e-mail. The fix was to delete the SSH hostkey for the machine they
were
tunneling in to.
-Updated and cleaned up a couple of units for the users.
-The Amaldi server went down over the weekend, due to a hardware failure.
Contacted HPC, it turns out the power supply was corrupted this was
replaced but when I brought the server up it was running real sluggish,
HPC
brought out another motherboard, but this still has not fixed the problem.
I have loaded a temporary server to get the Elba2002 and Amaldi99 websites
back up, until I get the original server back into service.
-Auditor from ITS.CALTECH came by to check our security permissions
on the
NTSRV's; he went over a lot the security issues, that he looks for
as far
as tightening down your shared permissions, this is still a on going
process and will report the out come when this is completed.
(Larry)
-Resolved the licensing issues with SDRC. We still have Master Series
7 up and
running and did not have to upgrade to the latest version of the application.
This would have been a time consuming task for the end users to have
to update
all of their data bases.
-Placed a number of orders for PC's. A couple for the 40M and a couple
for other
users. Checked on the orders with DELL that were placed last month
and they are
having a problem getting one of the components, so those units will
not ship
until the end of February.
-Worked with Mike on the Amaldi server. He's got it under control.
Though I had
to reset the pherkab server which is the same type of h/w being used
for the
Amaldi server. We will be keeping an eye on it.
-Worked out a few more issues on the e-mail server with Lisa. Also,
some work
with her on the MailMan logistics and policy. That should be a pretty
good tool
once it is on-line.
-Worked a number of network issues. We've a FORE edge switch that has
gone out
and working on getting it replaced.
The Foundry FE met with us this last week, to start working out the
logistics on
the installation of the GigE backbone and equipment. Ordered four more
edge
switches, two of the units ordered, were because of Marconi not planning
on
supporting the FORE edge equipment.
-Worked on policy and procedure documentation for GC and the over all
LIGO
procedures the gang of 5 +1 is working on.
LSC LASERS WORKING GROUP
Minutes of telecon Feb 7 th 2002:
participants: morning call: Peter Veitch, Jesper Munch, Maik Frede,
Martina Brendel, Ralf
Wilhelm, Carsten Fallnich, Michèle Heurs, Benno Willke
evening call: Ralf Wilhelm, Michèle Heurs , Rick Savage, Peter
King, Benno
Willke
1) updates
Adelaide:
- variation of pump power out of the different diodes was reduced to
below 5% by
adjusting the angle under which the fibre leaves the SMA connector,
it is not clear if the
strong dependence of the power on the angle was there from the beginning
or developed
over time
- after putting the pumping fibres at one side of the slab back into
position (close to the
slab, no waveguide that allows spreading out the pump distribution
in the horizontal
direction while keeping it confined in the vertical) the negative lens
still was there
(checked with a Mach-Zehnder)
- when putting the wave guide back in, the negative
lens disappeared !!!
- assembly of the laser head will continue the next days (fibres on
the other side back into
position) and new result on the output power vs pump power are expected
next week
LZH
- modelling continued, oscillator with two rods was modelled, results:
for 100W pump
power per rod the output power was 85W with an estimated M^2 of 1.1,
increasing the
pump power up to 250W per rod reduced the output power to 70W with
M^2 = 1.5, when
aberrations in the model were turned of (no temperature dependence
of dn/dT and of heat
conductivity) the output power was above 200W
- validation of the model will start once the rods are coated (coating
is done by IBS coater
in house)
- 20 diodes are delivered (each 30W), 10 are mounted characterized
and temperature
stabilized, no variation of the output power when moving the fibre
around was observed
Caltech-Stanford
- delivery of Lightwave amplifier is expected next week
- no info on the 100W project
2) schedule
- it was decided to shift the decision on “which
high power stage design to choose” by a
couple of month, depending on the progress of
the different groups this milestone will be
scheduled (latest fall LSC meeting)
From Peter King:
AdLIGO PSL
The amplifier ordered from
Lightwave Electronics to boost the
output power of the 10-W laser to 20 W, is expected to be shipped next
week. Stanford have arranged with Lightwave Electronics to have a graduate
student, most likely Shally Saraf, work with them in increasing the
power
of 10-W laser S/N #104 to 20 W by increasing both the NPRO pump diode
current and the power amplifier pump diode current.
From Janeen Romie:
AdLIGO Suspensions
Working on the RM suspension layout.
Still working on the budget with Thomas, et.al.
From Rich Abbott:
4. Worked out a repair plan for the manufacturing defect on the Cap.
Pos. Sensors.
5. Finished (with the testing done by Dave Grimmett) the test of voice
coil driver.
From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>
Subject: Weekly Report - Billingsley
Sapphire homogeneity:
Goodrich reports 14nm rms single pass homogeneity of the 250mm sapphire
substrate. This was accomplished by computer controlled polishing,
which uses a small rotating tool to remove material on side 2 of the substrate.
Aaron Turner, their CCP expert believes that they could do better if they
went to another polishing cycle. He will send an estimate of the
possible improvement and cost for another run, along with data from the
current run.
We have received 4 m-axis sapphire substrates intended for coating loss
investigations. These are 3" x 1" pieces. All show inhomogeneity
on the order 10nmrms. For one polarization the measurement
is entirely dominated by a ~10 nm rms ring pattern on surface 2 of each
optic. I have not been able to explicitly subtract this pattern,
so cannot tell the level of inhomogeneity with the optic in that orientation.
In the other orientation the inhomogeneity is clearly visible with features
typically at the 10 nm level. Typical results are posted at:
http://www.ligo.caltech.edu/~gari/Supporting/3x1m-axis-homog.html
These are much lower levels of inhomogeneity than we have seen in m-axis
material, begging the question: Is there really any difference between
A and M? The only way to tell for sure may be to turn one of our
pieces into a cube so that we can measure the same bulk along each axis.
Mark Felt has left Crystal Systems, our new contact is Chandra Khattak.
From: Mark Barton <mbarton@ligo.caltech.edu>
This week I got the export to Simulink working for
my Mathematica
model. It runs rather more slowly than the pure Matlab model in the
time
domain simulation but is still quite useable, and the frequency domain
analyses are not significantly different. And the slowness is due to
the
new physics (the high frequency modes of the springs) which is the
point
of the new model in any case.
From: Helena Armandula <ahelena@ligo.caltech.edu>
Advanced LIGO Coating Development - Low Absorption Coatings
Received substrates from MLD coated with Nb2O5 / SiO2. The substrates
were baked in sets of 3's at 300, 350 and 400 degrees C.
Sent the parts to Stanford.
Vlad is finishing calibration on the system; he should be able to start
the measurements shortly.
From: Janeen Hazel Romie <romie_j@ligo.caltech.edu>
AdLIGO Suspensions
Working on the RM suspension layout.
Still working on the budget with Thomas, et.al.
40m
A box of 40m TM suspension parts have been sent to LHO for cleaning
and baking. Another box will be sent in a week. The last machined parts
(which are waiting for custom material) will be done in 4 weeks.
Todd Etzel is working on making sensor/actuator heads and hopes to
assemble a majority of the 40m heads by the end of next week. They will
need to be cleaned and baked after that.
For additional information about this report, contact sanders@ligo.caltech.edu