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The LIGO Executive Committee Agenda for Monday August 5, 2002 will be:
(Meeting time: 10:30 am Pacific Time)
Open meeting 10:30 - 11:30
Special Items: PURCHASE OF DACs, STATUS OF PREPARATIONS FOR S1
From: Rainer Weiss <weiss@ligo.mit.edu>
to: LSC executive committee
from: R. Weiss July 31, 2002
concerning: Notes from the LSC Executive Committee meeting July 26,
2002
Report on the current state of the detectors prior
to S1 (R. Weiss)
-------------------------------------------------------------------
2km at Hanford is back in operation after repair
to MMT2 suspension wires
that were cut by laser beam heating. An atmospheric
exposure of about 6 hours cost
us about 2.5 weeks of pumping to reduce the water
load on the beam tube to 1 torr
liter/day (the water load permitted is 400 torr
liters total).
4km at Hanford is locking more robustly after
extensive work on driver electronics.
Common mode servo is being installed to reduce
the noise which is known to be
dominated by frequency fluctuations
4km at Livingston is being brought back into operation
after successful installation
of the two dimensional piezo-electric active
seismic control system (PEPI). The
system was installed outside the vacuum without
opening to air while maintaining
the mirror alignment.
Benno Willke and Ken Strain reported that GEO
has been running 16 hour uninterrupted
lock and may be able to operate at night unattended.
ITR 2003 Proposal preparation (Al Lazzarini)
-----------------------------------------------------------------
A coordinated proposal by the LSC (Penn State, Univ of Wisconsin@Milwaukee,
LIGO
Laboratory) is being prepared to ask for support for people at the
various LSC
computing centers. The proposal will include funds for 8 - 10 FTE and
address
LIGO science without a computer science component (the pattern of previous
computing proposals). Tom Lucatorto at the NSF is supportive and further
progress
may require the active campaigning of LIGO and LSC management.
Planning for the August LSC meeting
-----------------------------------
The idea of using the afternoon of the third day and all of the fourth
day
of the meeting for upper limit work was agreed. The technical development
groups have decided to meet more in plenary sessions to improve communications
between the groups and also to enable more experimenters to attend
the detector
characterization group meetings.
Information from the working group chairs
-----------------------------------------
Bruce Allen reported that the coupling of the source simulation researchers
and ASIS was not moving quickly and that we may need to reconsider
our strategy.
Benno Willke reported that the decision on the 180 watt laser design
for advanced
LIGO will not be made at the August meeting as planned. The groups
have not
made enough progress and there is no strong penalty in delaying the
decision.
The August meeting will be used to review the situation and set a new
decision
point.
Next LSC Executive Committee meeting
-------------------------------------
Tuesday August 20, 2002 at the LSC Executive Committee supper.
LIGO Operations--Administration
There was no site teleconference held on Thursday, August 01, 2002.
The list of current actions revised to reflect
the status of open actions assigned through July, 18, 2002 may be found
at ACTION
LIST.
From: Ed Chargois <chargois_e@ligo.caltech.edu>
>From: Linda Turner - turner@ligo.caltech.edu>
Web pages for the DCC give simple how-to's for document numbering, easy access to the latest on-line documents, and search capabilities for the DCC database. Take a look. . .
ACCOMPLISHMENTS
ACTIVITY
| WE 08/01/02 | Packages | Faxes |
| In | 46 | 27 |
| Out | 10 | 29 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
SUPPORT (Baldon, Torres, Lloyd, Tischler)
>Irene Baldon
Oracle will be upgraded to the 11i level and the system will be shutdown campus wide August 16-22 for the upgrade. For those of you contemplating a large purchase or have an invoice that will require payment during this time period, it is suggested that you submit your requisition(s)/invoice(s) no later than 5PM, Wednesday, August 15. Note that for emergency procurements, our group will have a block of numbers pre-assigned and will be able to prepare and order off-line. -pel]
>Rita Torres
Progress Period from 07.19 to 07.25
Progress Period from 07.26 to 08.01
Accomplishments:
The following change requests have been submitted:
| CR-010012
Revision B |
WBS 1.4.4.1 | Closeout Construction Budgets for Initial Computer Equipment Complement at the Sites | P. Lindquist |
| CR-020008 | WBS 1.1.4 | Purchase and Install Audio Visual Equipment in the New Hanford Auditorium | O. Matherny |
| CR-020009 | OPs | Digital Common Mode Servo to Mode Cleaner Path | D. Coyne |
| CR-020010 | OPs | Additional Funding for Low Frequency Seismic Isolation | P. Lindquist |
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
Work continues on completing the Livingston Observatory 2002 Safety Audit Report. The audit team has now reviewed the new and "old" safety audit action item status with G. Sanders. As a result of this meeting, a new draft of action item status and comments has been prepared and distributed (limited). In addition, an update of the LLO Visitor Information package is in-work.
The installation of the fire suppression system in room 215, Synchrotron,
is nearing completion. Assuming there are no further delays or problems,
the final Pasadena Fire Department acceptance test will be completed before
the science run construction "cut-off" date (mid August).
Summary of Commissioning Activities at LIGO Hanford Observatory (compiled
by M. Landry)
--------------------------------------------------------------------
Full locking has resumed on both interferometers. The common
mode was resurrected on the
2k ifo yesterday, resulting in noise performance similar to that prior
to the vent, with
the exception at higher frequencies. Above 300Hz, noise was higher
as the EO shutter has
not been commissioned and less light is on the AS photodiode.
The 4k has at times
locked reliably with few dropouts, including an 8 hour stretch Wednesday
evening, but
at other points suffered from alignment shifts that have been traced
to MMT2 and
MMT3.
2k IFO investigations
---------------------
Relocking the interferometer highlighted several potential alignment
issues in the
2k. Straight reflection off first ITMX, then ITMY, differ by
10%. Straight
reflection off of the RM for full locking does not coincide with the
reflected maximum.
These and other observations have some worried about internal clipping;
investigations
are ongoing. Scattered light off of the core optics is being
measured.
4k IFO investigations
---------------------
MMT2/3 alignment instabilities may have a diurnal trend. However,
several flavours
of spontaneous misalignment (enough to unlock the ifo and keep it that
way) have been
noted: brief forays into never-never land, quasi-permanent shifts,
and diurnal drifts.
Mode cleaner characterization (part of the common mode push) continues.
More internal modes of test masses were measured; five modes
of the 4k ETMs.
FACILITIES
------------------
All the different trades are busy in the Laboratory Building, trying
to get it ready for
the LSC meeting.There is still lot of work to be done but hopefully
the auditorium and
the bathrooms together with the air conditioner will be functional
by the 18th of August.
CDS (Chethan)
Upgraded the old LLO CDS Server from Ultra 2 to E 220. Moved the files and two external disks from Ultra 2 to E220.
Upgrading the control room machines to 24 bit color mode. Installed
a CDS
machine for Ash. Working on setting redundant time server entries on
all control room machines.
GC (Shannon)
worked an issue on our web server that prevented users from secure
shelling to it.
Updating some files in the database for web pages.
Looking at tasks that need to be done over the next six months and
trying to schedule them in a reasonable form.
Preparing for the trip next week to Usenix and also Pasadena.
LDAS (Shannon)
Wrapping up the quotes for the VPN servers. I received one very
promising quote from Microway. I may settle on them as a vendor.
The
specs are below:
Item 1: 2.53GHz P4 Node
QTY: 8
Tyan S2099GNNR Motherboard with 845E Chipset and 533MHz FSB
2.53GHz Pentium 4 CPU with 512K Cache (mPGA-478) (Supports Northwood)
5 32-bit PCI Slots, AGP Pro50 (& AGP 4X), 6 USB 2.0 Ports
512MB DDR PC2100 Unbuffered (has 4 DIMM Sockets)
2U 19? Rackmount Chassis (3 Bays) with 300W Power Supply
40GB Ultra ATA/100 7200 RPM IDE Hard Disk Drive
Integrated ATI RAGE XL 8MB Video
Integrated Intel 82540 100/1000 GETH
Integrated Intel 82562 10/100 Ethernet
Integrated IDE RAID (0 & 1) ? Promise PDC20276 dual-channel ATA-133
3.5? Floppy Drive & Sony 52X IDE CDROM Drive
LDAS (Igor)
Finished writing LAL's part of correlation DSO. Started working on
LALWrapper's part of it.
* Investigating how to migrate data from DB2 7.1 to 7.2
This plan needs to be finalized ASAP so that appropriate priorities, travel plans, etc. can be made.
Dennis Coyne reporting for Jonathan Kern, Marcel Hammond
For the LASTI prototypes:
·Spring fabrication is proceeding well. Should have machined parts completed by a 8/12. Then heat treat, Ni plate, silver solder, spring test.
·Bellows are in production.
·Most machined parts of the hydraulic actuator are in machining; A few remaining parts are being detailed and will be released next week.
HEPI Pump Station/Distribution
Ken Mailand
·System
Operation: System being upgraded for tests and shipping to MIT.
·Test
Observations: Getting setup to do tests at all sensors with various accumulator
pressures.
·On-going:
A new pump mount adaptor has been designed to attach the existing motor
to the new screw style pump.
A new aluminum couplinghas been
modified or the existing pump, and new screw style pump.
A new Buna coupling spider material will be tried to smooth flow.
The motor pump adaptor will is being modified [opened] to allow air
flow thru coupling area.
The motor will be detached from the base and allowed to contact the
floor independent of the station plumbing brackets with the hope of further
isolation of vibrations from pump and motor.
New Base board is ready which is more secure than the current and of
a better material.
·Electronics
Sensors: Sensors are being electrically isolated from the piping.
·Manifold
[fluid distribution]: The manifolds [5] with their mounting bases are finished.
·Test:
Start tests 8-1 at several accumulator pressure settings to optimize the
operation of the pump isolation.
Determine which improvements or modifications might be made to improve
performance.
·Design
: A site installation version of the test pump station to be designed,
when final configuration is known. This would be more compact, have a mass
dampened mount base, and be in an isolation enclosure, to control temp
and exhaust vapor.
·Stanford: [information
needed from] A range of acceptable viscosities will guide us in the design,
re. the allowable temp rise of the oil in the system.
·MIT:
Sent motor data to Myron re. voltage and phases.The oil will ship with
the rest of the pump station. Distribution manifold drawings were sent
7-2 to MIT to show the configuration, and the attachment method. Need to
design and build a bypass resistor for MIT configuration.
·Shipping:
7-1-02 a shipping contractor visited CIT and looked at the requirements
for shipping the test pump station the MIT. A quote is in.A large box crate
is ready for shipping all items not on bases.
·Layout drawing: I have finished a scale plan view and partial elevation [acad 2D] layout drawing, of station component assembly.
- Working
on a code library for use by LSC/ASC/DCS to allow GDS to connect an
excitation
signal and three test points to every digital filter module. Since
large optics
DSC are not connected to the data acquisition network, the library
also includes
router software such that the ASC and/or small optics DSC front
ends can relay
GDS signals at the full 16KHz processing speed of the large
optics controllers.
I've been coordinating with Sigg to get the GDS test point
ordering and
numbering sorted out such that the test point manager and Arbitrary
Waveform Generator
(AWG) will interface properly.
- Epics Data
Collection Unit (EDCU) software has been ported to a Pentium and
tested here.We
hope to try this at LHO after S1 and see what the performance
improvements
might be over the present MIPS board EDCU.Since
it has a faster
CPU and more
memory than the presently installed MIPS board, plus a fast
ethernet connection,
it should get us closer to the desired 10000 channel
capability.
- AWG software ready for 40m lab.Alex is finishing up some testing.
With Gary
Sanders and Jay Heefner, conducted a site visit to the NRAO Green Bank
Radio Observatory in West Virginia. RFI and EMC engineers at the site were
open and helpful. MZ's questionable decision to kick off the meeting with
a bare-all horror show of LIGO's RFI blunders led to a full-blown trade
of dirty laundry from both sides, which was extremely productive. We got
significant useful guidance on RF interference mitigation and containment
"after the fact," as well as design and testing methods that contribute
to reduced interference for new designs.
One significant and immediate outcome is that numerous NRAO examples offer renewed hope that radiation from our digital infrastructure can be contained to some degree, rather than simply tolerated. The previous proposal (cf. LIGO-E020350-04) concentrated on passive defense of the analog front and back ends from radiated and conducted emissions; we'll now place higher priority on containment of these emissions at their sources wherever feasible (cf. LIGO-G020300-00). An integrated plan and cost estimate are in process.
Jay Heefner
·EMI: I have started to contact vendors regarding fully shielded eurocard and VME crates that could be used in any LIGO retrofit.
·Optical Lever Whitening: The optical lever whitening boards are still in fab and test. Hopefully the first units will be ready for shipment to LLO in the next week.
·Advanced LIGO DAC: We had a meeting with frequency devices regarding their DAC design and test results. Preliminary testing of a single channel prototype shows an output referred noise less than the required 100nV/rtHz. There were also clarifications and comments regarding their proposed VME interface. We will have another meeting next week to close the loop with them and following this meeting they will begin production of a full prototype module.
Note
from Coyne: Hope to have an internal
discussion this Monday (Peter Fritschel, Mike Zucker, Jay Heefner, myself)
to discuss the issues associated with pursuing this VME design as is, or
attempting to add requirements (read more up-front cost and time) to have
Frequency Devices make a system that may be more EMI/EMC compliant. This
topic should be discussed at the executive meeting on Monday as well, before
direction is given to Frequency Devices.
·Timing Module: The design of the new FPGA timing module has been started. In an interesting side note, the simulator was used to develop the circuit used for multiple DAC output pulses using circuitry already on the existing board. This fix was tested on the board and works nicely.
Rich Abbott reporting
Preparing
to ship all the hardware for the LASTI pre-isolator system.Items
to include, +/- 10 amp driver chassis, L4C interface box, cables, connectors
and test procedures and documentation.
The transfer
functions for all the laser-supplied intensity-related
actuators
have been measured.It seems that
some minor electronic
modifications
have been made to the NPRO design as this particular laser is
a quieter
than the others at 60 Hz.However
the noise around the 10 kHz
region seems
to have degraded a little, with the presence of a small comb.
I have been
chasing up components that we do not have in stock for
the experimental VCO.All the footprints for the PCB have been checked
This week
I have continued preparation for S1. I updated some DMT
documentation,
making sure that the monitor list web page was complete. I
have also
been working on a major revision to the name server and its
client interface
to support tunneling to monitors on the CDS network and
reduce the potential for name entries to be changed accidentally.
The WYKO interferometer
has developed an Astigmatism of roughly 5 nm along the X direction.This
astigmatism does not show up in our large optic measurements from last
May, it has developed some time since then.The
most probable explanation is that something has moved as the instrument
has been switched in and out of zoom, while measuring the smaller 40 m
optics.I have contacted Veeco to
see if we can correct the situation.
In the meanwhile,
recall that all of our specifications deal with power and astigmatism as
a separate specification from the rms surface error.True
astigmatism can be observed directly by rotation of the part.We
do this because it is well known that instrument astigmatism can be difficult
to calibrate correctly, and the astigmatism of individual parts can be
easily measured by the rotation technique.
The two LIGO1 Beamsplitters were received from REO after coating.
OTF Lab.
Contamination
Cavity # 1 with glycerin still running. Terminating this week. The change
in absorption << 1ppm/month
Will repeat
the mineral oil contamination tests.
New Lab at
RSE
Cavity #3
Reference Cavity still pumping down.RGA
scan taken and the sum of masses
(amu:41,43,53,55
& 57 ~ 7E-12 torr.It is considered
clean cavity.
The optics
has been installed and aligned and waiting to be aligned into the cavity.
Cavity #2
Test cavity
This cavity
is pumping now.After I haverefurbished
the one I got before.
We brought
most of the equipment needed here at RSE from OTF Lab.
OTF Lab
The refurbished
100mw NPRO S/N 267 Laser from Lightwave is running now on the new optical
table
used for the
transmission test setup.This morning
we(Helena,Liyuan and I) have tested and measured the transmission of some
partially transmitted mirrors and beam splitters from REO.We
encounter some situation
as these mirrors
are all wedged and throws the transmitted beam away from the small area
of the GaAs chip photodetector.So
alignment had be done one after another one.What
we need is a bigger chip and i am looking into(cost ~$875)Overall,
We willmake the upgrading necessary
to comply with the needs now that we have different mirrors to be measured.
I am assembling
and refurbishing another vacuum pump unit that it is needed to pump the
cavity#1 which has the glycerin sample after this test is done this week.Cavity
needs to be baked then.
I have received
this afternoon the Laser warning sign from LHO and assembling is in progress.
Misc...task accomplished, machining parts, placed orders
no report
no report
Simulation and Modeling (Bhawal)
E2E weekly Physics meeting
-------------------------------
We discussed about measurement of angular motion of mirrors. First,
Virginio explained measurements of transfer functions from Ground noise
to
stack and mirrors done by Fred Raab in April-May. Sany Yoshida gave
a talk on
"Can't we monitor HAM table motion by OSEM sensors?" and presented
the work
on this by him and his students at LLO.
SimLIGO
-----------
(Matt) Rebuilt ISC detection sub-system in SimLIGO to allow for inclusion
of
wave-front-sensors with correct optical paths. Constructed digital
ASC
system. Next to come is parameter setting for ASC hardware
and software
enroute to full alignment control.
COC phasemap
-----------------
(Hiro) Software tools were developed to prepare a phasemap of COC to
be used
to calculate the mode decomposition when fields interact with
optics.
Code development and maintenance
----------------------------------
(Hiro) The code of the simulation engine are improved to simplify the
construction of SimLIGO.
(Ed Maros) Worked on installation at LLO
Alfi
-----
(Bruce)
- Cleaning up event processing code in MemberNodeWidget in order
to make the
widgets resizable, and later to be able to move ports
on the external view
of a node.
(Melody)
- Working on the automated tester for alfi5.
- Implemented several print features in alfi5. Users can now
print using
the scale that is displayed or use the 'fit to page' print
feature.
LIGO Data Analysis System
Software Systems (Philip Charlton for Kent Blackburn)
-This week we have continued final testing and preparation
for the next release of LDAS to be used in S1. The system
has been exercised with a variety of user jobs based on
the expected usage during and after the science run.
These include jobs that use the available LAL DSO's
for inspirals, bursts, tfclusters, slope detection,
stochastic background and known pulsars, and also the
new user commands for creation of reduced frames.
Throughput of the system has been substantially improved,
although it is still possible for the job queue to fill
up to its maximum allowed value if jobs are submitted too
quickly.
-A bug in the diskcache API has been found that occasionally causes
the API to use up large amounts of CPU when a request is made for
frames that don't exist in the disk cache. This is being investigated.
-The new user command "createRDS " for creation of reduced
data sets has been profiled and tested on the local CIT systems
and at LHO. On an unloaded system the time taken to produce
reduced frames is around 0.5 * real time, while under realistic load
conditions the time taken is about 0.85 * real time.
-Some minor fixes were made to the control and monitor application
interface and documentation.
-Background development has continued for support of Version 5 frames
and C++ routines for more efficient frame concatenation.
-Routine nightly testing of LDAS is showing a somewhat reduced failure
rate. No failures out of 5800 jobs were reported overnight
at ldas-dev and ldas-cit, while a failure rate of 0.06% was reported
at MIT.
Data Analysis Activities (Wallace)
CIT:
(Creighton)
This week I have been writing a program for generic coherent
multi-detector GW signal simulation and injection.
Hanford:
Livingston:
(Yakushin)
* Finished writing LAL's part of correlation DSO. Started working on
LALWrapper's part of it.
* Investigating how to migrate data from DB2 7.1 to 7.2
MIT:
(Katsavounidis)
Work is continuing on finishing up the E7 analysis
looking for bursts. Stefan and Laura have worked
on specific items that were raised by the bursts group
during the conference calls over the last 2-3 weeks.
More specifically:
o implemented code to deal with a vetoing scheme where
the response of the gravitational channel is taken
into account. This was motivated by the use of the
MICH_CTRL in H2 as a veto for the E7 bursts analysis.
Code is in place and functional but needs testing.
Several subtle issues still need to be understood
w/r/t to this vetoing scheme (Stefan).
o analyzed entire E7 (coincidence) data set for vetoes.
Roughly 100,000 veto triggers per instrument per
veto channel were generated. Entries were temp written
to the MIT_TEST database but will be soon moved to
their definitive location on MIT_E7 (Stefan).
o performed a detailed analysis of vetoes and efficiencies
for the slope DSO (Laura). In addition, following discussion
at Tuesday's bursts call, investigated a re-analysis of
the TFCluster E7 (playground) data after splitting the
events in three separate bands. This is work in progress.
(Laura, Jacob- Jacob is a summer undergrad student).
o produced various additional supporting plots for E7 playground
analysis already reported (Stefan, Laura, Erik).
Beyond E7-related activity, Stefan looked at the low noise
LLO data collected in mid July. He presented his findings at
the commissioning conference call last Monday.
He performed a TFCLUSTER-based burst search on that data.
Several modes were seen ringing down over the first
~5min of the lock while there were still some broad-band
glitches visible similar to the E7-PSL ones but ~ 20x weaker.
Hanford:
(Greg)
1) Worked with LDAS to debug the new prereleased version of LDAS when
requesting SFT data for the knownpulsardemod DSO. The metadata
about
the input frequency series and the start time the data were generated
from were getting set incorrectly, but this has been fixed. Updated
my
scripts to work with the new prerelease of LDAS; more work is needed
along these lines, but scripts for test cases work. These scripts were
sent to Isaac to made part of the standard LDAS tests.
2) Worked extensively with my SURF student this past week to understand
the distribution of the maximum likelihood estimator we use to search
for periodic signals with amplitude and phase modulation. We can now
derive from first principles all the basic distributions and produce
these distributions numerically with his test code and matlab. We also
wrote code to fit histograms of the data to a model of the distribution.
We find discrepancies between our calculations and numerical results,
and some published theories about the distribution. We are working
to
sort this out. We have also found discrepancies between his code
and
code in LAL. These appear to be do to a few minor bugs in LAL, and
we
will be contacting the authors of this code to get these bugs fixed.
LDAS Hardware Systems (Mendell)
(Greg Mendell)
1) The two ASA beowulf node computers that I sent for repair were
returned with new motherboards and memory. However, one of these
now
has a problem with its network interface, the other hung during a 3
day
burntest. I have contacted ASA about this, and I am running some further
tests.
2) I've made measurements to make drawings of the new LDAS room, as
part
of plans to move LDAS into the new building at LHO at the end of
September or early October.
3) Provide the usually assistance to LSC scientist and graduate
students, this week from U Oregon, U Mich, and WSU requesting
information about data and running LDAS jobs.
(Dan Kozak)
HPSS: migration off of Redwoods halted until CACR gets some more 9940
tapes. Worked on migration of small files off of 3590 tapes.
This
being a good opportunity to catch violations of policy (people using
HPSS for system backups mainly), I'm keeping a close eye on it.
Managed to delete ~68,000 small files during this process this week,
which helps the ever growing namespace problem.
Took delivery of 1050 LIGO 9940 tapes and set up summer student Mik
Garvey to label them and put them in the silo.
Worked on getting a quote from Sun/LSC for our real (non-eval) SAM-QFS
license.
Worked on setting up SAM-QFS to put files on tape in such a way that
we'll be able to ship tapes from the sites and import them into the
CalTech system.
(Igor Yakushin)
* Finished writing LAL's part of correlation DSO. Started working on
LALWrapper's part of it.
* Investigating how to migrate data from DB2 7.1 to 7.2
(Shannon Roddy)
Wrapping up the quotes for the VPN servers. I received one very
promising quote from Microway. I may settle on them as a vendor.
The
specs are below:
Item 1: 2.53GHz P4 Node
QTY: 8
Tyan S2099GNNR Motherboard with 845E Chipset and 533MHz FSB
2.53GHz Pentium 4 CPU with 512K Cache (mPGA-478) (Supports Northwood)
5 32-bit PCI Slots, AGP Pro50 (& AGP 4X), 6 USB 2.0 Ports
512MB DDR PC2100 Unbuffered (has 4 DIMM Sockets)
2U 19 Rackmount Chassis (3 Bays) with 300W Power Supply
40GB Ultra ATA/100 7200 RPM IDE Hard Disk Drive
Integrated ATI RAGE XL 8MB Video
Integrated Intel 82540 100/1000 GETH
Integrated Intel 82562 10/100 Ethernet
Integrated IDE RAID (0 & 1)
(Keith Bayer)
removed old data on SF880 internal raid unit
Loaded lownoise data from LLO onto internal raid unit
installed o/s's on PC Raid Unit
configured RAID cards on PC Raid Unit
running benchmark tests on unit
(Al Wilson)
Working on the kickstart 7.3 release
Ordered parts for the new terabyte raid systems
Did a power down test at millikan, even though campus maintenance did
not
kill the power.
Tested the backup tape system
General Computing (Wallace)
MIT:
(Keith)
-Pulled pellinore.mit.edu off network after discovering hack
reinstalled o/s and patched machine.
-Installed patched version of openssl on solaris servers.
-Installed software on virtual control room computers.
Livingston:
(Shannon)
-Worked an issue on our web server that prevented users from secure
shelling to it.
-Updating some files in the database for web pages.
-Looking at tasks that need to be done over the next six months and
trying to schedule them in a reasonable form.
-Preparing for the trip next week to Usenix and also Pasadena.
Hanford:
(Christine)
- The LHO network will be down Tuesday, Aug. 6 at about 10 a.m. PT
for
one-half to one hour. We will be upgrading the WAN network from
T1 to
10 Mb ethernet (about 6.5 times faster than T1). I will announce
this
again before it happens.
- The LHO email/web server was moved to a new IP address on Mon. July
29. This was necessary as part of the WAN bandwidth upgrade.
Caltech
modified their DNS tables with the new IP address. The name of
the
server stays the same. Everything went very smoothly, only a
few e-mail
problems have cropped up over the last few days and all those have
been
fixed. Thanks to Larry for coordinating everything with Caltech
ITS.
- Provided the usual types of user support and worked on several
procurement issues.
CIT:
(Veronica)
- LIGO website: Recorded two SURF lectures and compressed them for
streaming, currently in RealMedia format. Experimenting with QuickTime
video editing.
-Together with Gary and Linda, met with a consultant regarding possible
software upgrades for the DCC. Discussed with Larry the needs and possible
solutions.
-MIT reported a problem with image loading; trying to pinpoint the
problem, tested the pages in question on various platforms/settings.
The
problem turned out to be at the user end and is now resolved.
Mike and I looked into a glitch that caused a webserver malfunction
on pherkab. A license expiration date turned out to be the problem.
Posted several web updates.
- LSC website: updated the LSC August meeting page. Posted a bulk of
MOUs, progress reports, and talks to be presented. Working with Rita
and
Irena on updating some LSC-related pages.
- CaJAGWR website: posted a new membership information.
- LDAS website: the latest hardware diagrams are now installed; the
pointers will be active by the end of the day today.
(Lisa)
- Did monthly backups.
- Showed Mick how to replace a fan in an ultra10.
- Pulled the Cadence disk off of sadal and disabled the cadence automount.
- Ran XSun patches on algol and rastaban to try and fix an xlock problem.
It
appears that Solaris 8 has been having chronic xlock troubles (see
patch
106852).
- Installed a java web-mail package but the authentication mechanism
keeps
failing. I'm pretty sure there is an unrelated piece of software missing
but
the documentation for the package is pretty poor.
- Updated the 115 and 125 wireless access points with a new access
list.
- Wrote a script to automate updating the sendmail access list.
(Mike)
-Worked some Networking issues on the second floor of West
Bridge; it turned out to be some bad cabling. This problem is corrected
and
I enabled a couple extra ethernet ports to get some other cabling issues
squared away.
-Upgraded Calum's PC to service pack 4 on his Solid Works installation
and this
became an issue with interacting Solid Works files from education and
commercial version when he did this. I tried to uninstall service pack
4,
but had no luck. I was forced to uninstall Solid Works and then reinstalled
with only loading service packs 2&3, this has the Solid Works group
back up
and running.
-Reworked the Bridge VRVS, which was having audio transmission (MIC).
This
is back up and running.
-Working a Sony LapTop that was owned by Alan Weinstein. This computer
keeps on freezing and it is looking more like a motherboard problem.
I
called Sony about this LapTop and it is out of warrantee.
-Finished loading two Laptops to give to Ed to send to Hanford Wendy
gave me a hand with this.
-Worked on multiple workstations that included cleaning up viruses,
hardware issues and loading software. I ended up having to bring two
of
these computers to my office to work on. I finished these computers
up and
have them back in Synchrotron.
-Trouble shooting Jim's computer for we are trying to upgrade his computer
to 2000 but this computer is having some hardware and software issues.
We are reloading another computer to swap him out.
-Worked on printers up on the 3rd floor of W/B, Millikan and Bridge
Annex that included paper jams and changing out a replacement drum
and
toner cartridges.
-Wendy and I have been working on upgrading users from win98 to 2000
Professional this is including getting current ghost images of user
computers then upgrading computers, which include flashing bios and
adding
additional memory. So far this has seems to be working out okay,
the only
problems that we have come across is that you must uninstall Norton
AntiVirus and PCARD then reinstall. We have just started working this
project; our goal is to have everyone on the same 2000 platform (hardware
permitting) to take advantage of security features plus this seems
to be a
much more stable operating system than win98 as long as current service
packs are loaded which we take care of. If those of you are going on
vacation please backup your personal files to your home accounts just
to be
safe. You never know about computers for they are sometimes temperamental
and refuse to cooperate. Just a safety precaution! I will contact all
users
before I attempt to upgrade their computers we already have a great
percentage of our users already running win2000 and all software is
compatible. If there is a problem with this, please contact either
Larry or
myself and we will hold off on the upgrade of your computer.
(Mick)
-Worked on documentation for luna build
-Loaded 2 laptops
-Installed new fan in Ultra 10
-Performed root partition dumps for primary servers; importantly,
first
dump for luna since rebuild on Blade1000
(Christian)
-Working on documentation for Larry.
-Spent time learning the h/w setup on PC's.
-Labeling cables and computers at various locations.
(Wendy)
-Loaded laptops and PCs with win2k and all software with Mike
-Upgraded a few machines to win2k from win98
-Helped users do random computer stuff, such as trying to troubleshoot
programs and installing new ink cartridge for printer
-Ghosted a few machines
(Larry)
-Spent a deal of time going over financial/procurement issues. Florance
is
working on setting up a training session for those involved in the
procurement
process. This session will cover some of the details to help us put
in the
correct information on the paperwork.
-Working out the details on the SUN maintenance renewal. Renewed the
maintenance
on the CISCO router. Purchased a number of supply items that we have
depleted
over the past few months.
-Purchased another 8 port GigE blade for the Foundry switch. This should
allow
us to have all the major servers on a GigE backbone. Next FY we will
work on
getting the PC based servers on the GigE backbone.
-Spent a deal of time working on machines with viruses. A few visitors
did not
have a Anti-Virus pkg. on their machine and are now having to rebuild
their
machine. Fortunately, we've been able to recover their data.
Spent time recovering data for the PC's and others that had inadvertently
lost
their data for other reasons.
-Worked a number of e-mail issues. Also, we've added a large number
of addresses
to be blocked by the access list. We are really getting a number of
spams. The
campus as a whole is getting inundated with this type of e-mail.
-Worked a number of hardware issues. Did some recabling of the computer
room.
Working on some VRVS enhancements.
From: Mark Barton <mbarton@ligo.caltech.edu>
This week I've been doing a literature search of
suspension-related
material in support of a forthcoming paper on LIGO I suspensions by
Fred
Raab and me.
From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>
Goodrich reports that the microroughness measured on the large m-axis sapphire piece after compensating polish was 55 angstroms. Our goal for the LIGO TMs is that the microroughness be less than 5 angstroms, the requirement is that it be less than 10 angstroms. Goodrich has indicated that they could pursue better microroughness using a separate slurry, however there is concern that the bubbles which break through the surface of this piece will chip and cause more sleeks in the surface. They suggest that they could work on another piece to demonstrate improved microroughness. The trade-off is that as you re-polish for a smoother surface, it may compromise the compensated wavefront.
I think they do need to demonstrate the ability to achieve the compensation
and microroughness concurrently. I have found that the piece, when originally
delivered from Wave Precision had a microroughness of 0.54 angstroms rms,
with one or two peaks at 2 angstroms. A repolish with a second slurry
should be possible.
From: Michael Smith <smith@ligo.caltech.edu>
40 METER IFO
IFO Mode Matching Telescope:
A final design for a remotely focusable, vacuum compatible, off-axis
telescope is in process. Quotations for the parabolic mirrors have been
received. A specification for the parabolic mirrors is being written in
preparation for placing a purchase order.
Quad Photodiode Mounting Pedestal
The parts for insulated mounting pedestals for the quad photodiode
boxes have been received. New mounting holes will be drilled in the boxes
to accommodate the pedestals.
Optics Parts List
Purchase orders are being prepared for most of the opto-mechanical
parts for the AP1, AP2, ITM PO, BS PO, ETM PO, and SPS ISC beams and sensing
table optical trains.
ADVANCED LIGO
Photon Actuation:
Costing data for an experimental task to evaluate the performance of
a photon actuation scheme is being prepared; the experiment would take
place during the summer of 2003 and involve several SURF students. A simple
performance analysis is being made to assess the feasibility of the photon
actuation scheme.
From: Gregg Harry <gharry@ligo.mit.edu>
We finished measuring mechanical Q for 5 modes on the SMA/Virgo coated
sample that is 3/4 silica and 1/4 tantala. Based on our previous
measurements and the theory developed from it, we could calculate
an expected Q for this sample. These measurements then serve
as a check
on our understanding of coating loss to date. Qualitatively,
we expected
the Q to be higher than when the coating was even, as we had found
that
tantala was the lossier component. This was true for all the
modes.
Quantitatively, one of the modes gave an answer for the tantala phi,
2.4
+/- 0.4 X 10^-4, that agreed with the previous values. All the
other
modes gave phi values on the high side of this, but all were within
2
sigma.
We have now hung the MLD coated sample with equal amounts of silica
and
tantala. This will serve as a test of the effect of the coating
process
(including annealing) on the coating loss. Previous measurements
on an
MLD coated sample gave much worse loss for an alumina/tantala than
had
been seen from a different coating vendor.
For additional information about this report, contact sanders@ligo.caltech.edu