Weekly Report for Week Ending April 11, 2002


 Exec. Comm. Agenda
Highlights
LSC
Administration
Hanford Observatory
Livingston Observatory
MIT
Caltech
Detector
40 Meter
TNI
LASTI
Data Analysis
LIGO II/Adv. R&D
Past Weekly Reports

The LIGO Executive Committee Agenda for Monday  April 15, 2002 will be:

 (Meeting time: 10:30 am Pacific Time)

Open meeting 10:30 - 11:30

  1. Announcements
  2. LSC Issues (Weiss)
  3. Comments on Weekly Report
  4. WBS 1 LIGO I Construction (Lindquist)
  5. WBS 2 LIGO Lab Operations
  6. WBS 3 and 4  Advanced R&D and LIGO II (Sanders)
Executive Committee only 11:30 - noon   Topics:
 

Special Items:


Special Announcements:


Weekly Report Highlights
 


LSC Issues (Weiss)


no report


LIGO I Construction/LIGO Laboratory Administration (Lindquist)



 

LIGO Operations--Administration



LIGO Weekly Site Telecon (Lindquist)

There was no Site Teleconference was held on Thursday, April 11, 2002.

The list of current actions revised to reflect the status of open actions assigned through March 28, 2001 may be found at ACTION LIST.


PROPERTY MANAGEMENT (Chargois)

From: Ed Chargois <chargois_e@ligo.caltech.edu>


DOCUMENT CONTROL CENTER (Turner, Mak)

>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

> From: Cleveland Mak <mak_c@ligo.caltech.edu>

ACTIVITY

Press here to access the DOCUMENT CONTROL CENTER WEB PAGE.


COST SCHEDULE CONTROL SYSTEMS (Cunningham, Brambila, Kaufman)

From: Esther Cunningham <esther@ligo.caltech.edu>

Press here for ACCOUNTS PAYABLE HISTORY DATA .

From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>

From: Florence Kaufman <fkaufman@ligo.caltech.edu>

SUBCONTRACTS MANAGEMENT (Petrac, Jasnow)

From: irena@ligo.caltech.edu (Irena Petrac)

From: Ed Jasnow <jasnow@ligo.caltech.edu>

CONSTRUCTION:

The Louisiana State Fire Marshal has accepted part of our appeal regarding handicapped access to the men's restroom adjacent to the auditorium in the Livingston Staging Building, but has denied the other part.  We will not have to change the commode partitions, but will have to re-arrange the urinals to provide greater handicapped access.  The revised drawings to cover this change were transmitted to Brunt Construction on Tuesday and they will prepare an estimate for this effort.  Additionally, the Fire Marshal requested a concrete pad at the receiving dock and an extra sidewalk around the side of the building.  Brunt has received change orders to acomplish this work.  The new building completion date is April 30, and they are on track to make that.

Chervenell Construction is re-working their schedule to try and compensate for the late delivery of materials on the Hanford OSB East Building.

OPERATIONS:

Both sites are preparing to support the first science run, now scheduled for June 29 through July 15.


SUPPORT (Baldon, Torres, Lloyd, Tischler)

 
>Irene Baldon >Dorothy Lloyd >Rita Torres >From: Ryan Tischler <rtischle@ligo.caltech.edu>

Advanced LIGO (Frey)

From: Thomas Frey <tfrey@ligo.caltech.edu>

Progress Period from 04.05 to 04.11

Accomplishments:

Schedule 04.12 to 04.18:

Reports (Lindquist)

I have still assembling a quarterly report for the Construction effort (end of February).  The goal remains to prepare a short report comparable to the old Monthly Reports without bothering the task managers.



Change Control/Contingency (Lindquist)

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-020002 WBS 1.3 (OPS) CDS Remote Control Room D. Coyne
CR-020003 WBS 1.3 (OPS) Fine Actuators for the LIvingston Input Test Masses D. Coyne

Press for the latest Contingency Needs Projection.


Human Resources (Akutagawa)

From: Cindy Akutagawa <cindy@ligo.caltech.edu>


Quality/Safety (Tyler)

>From: Bill Tyler <tyler@ligo.caltech.edu>

No report this week.
 


LIGO Hanford Observatory (LHO) Operations (Raab)


-------------------
FACILITIES
-------------------
There really is a new building coming up at the LIGO Hanford Observatory.
The picture shows the front entry in the making.


LIGO Livingston Observatory (LLO) Operations (Coles)


Interferometer: The mode cleaner wavefront sensors were checked and then calibrated. The wavefront sensors were then activated and they are now fully operational. The beam on ISCT4 (anti-symmetric port) was found to be elliptical and astigmatic. The culprit was a lens on the galilean telescope after the periscope for the anti-symmetric beam. The telescope was improved using a barrel lens mount. The beam was the adjusted to be collimated and not astigmatic. It was also found that the beam and the wave front sensor response look the same regardless of the EO shutter transmission level.  (Joe Kovalik)
 

CDS: Rusyl and I replaced the clock Driver boards. Got new firmware from the VPN box manufacturer this week. Installed it and fixed the broken VPN box. Fixed problems with the ASC freeze up couple of nights ago. Working on getting the disk to disk backup straightened out. Experiencing problems with disk getting full. Found a bug in the Mode Cleaner Auto Locker script. Added some buttons to reset the purple buttons on the LOS screens and the OPTLEV screens. Also added the epics records for the purple buttons in the saverestore.exclude list. Fixed a security bug on london found in ssh by Dave Barker.
(Chethan, Rusyl)

LDAS: Visited Caltech: made a presentation about DB2 features which we will be using soon (replication, federated system), talked to Kent, Stuart, Peter, Ed and Mary about how to proceed setting up replication for LDAS metadatabase and what experiments are needed to figure out the optimal configuration. (Igor)
 


Detector/Technical Support (Whitcomb, Coyne)


 
Commissioning:

Hanford
Livingston

Science & Engineering Support
See also the daily electronic logs for the installation and commissioning activities:

Hanford Detector Log

Livingston Detector Log

LHO COMMISSIONING

2km Commissioning

Stan Whicomb reporting

Concentration on the 4km has reduced the effort on the 2 km.Characterization

of the WFS continues, and the calibration factors for the optical levers have

been measured.

Daniel Sigg has measured the amplitude fluctuations on the drive to the phase

modulator.It pretty much meets specs.

4-k Commissioning

Stan Whicomb reporting

Locking continues to be amazingly good at times, frustratingly bad at others.

During one of the good locking times we got a first calibrated noise spectrum

in the recycled mode.The sensitivity reaches its best at about 700 Hz, at

about 2e-16 m/rHzThis is about an order of magnitude better than its E7

sensitivity, but still about an order of magnitude poorer than the 2 km.

The dewhitening filters have been tested.Some quick coding by Rolf fixed a

minor problem with the digital suspension dewhitening filters and they seem

to be functioning properly.Although we have not had the opportunity to test

them with the full interferometer, we have successfully engaged them (single

stage only) on single arm locks.

The main thrust at LHO this week has been to get the common mode servo

working on the 4 km.The board has been installed and cabled up.Transfer

functions have been measured, a number of capacitors removed, and then

remeasured.The gain stages have been tested and a couple of fixes made.

Luca Matone has measured the gains in the various paths and is ready to try

to engage the loop.

LLO COMMISSIONING

Rai Weiss reporting

Operation and noise studies of the interferometer:

* Recycled lock has been made more robust, the system will almost

survive the train. Lock loss is primarily due to beam motion

at the symmetric port (symmetric motions) rather than loss of 

contrast at the antisymmetric port due to antisymmetric motions 

of the cavity optic axes, as was the case for the unrecycled 

recombined interferometer.

* Contrast defect (1-c) has been measured as 1.2 x 10^-3 and the

sideband buildup in the power recycled Michelson is a factor of

4

* The common mode servo has been exciting the vertical bounce mode

of MC2 which has limited the gain in this loop.

* The 1/f^3 noise at 100 Hz still persists.

Wavefront sensors: A concerted effort has been made to understand the

problems in the wavefronts sensors. Careful measurements of the focus 

in the Guoy phase telescope have been made. A significant problem

may have been found in astigmatism in a reducing telescope that

has distorted the wavefront. The electro-optic shutter is

no longer the dominant source of wavefront error.

Scatterometers: Work is continuing to install the scatterometers

to measure the changes in mirror coating surfaces with time.

SCIENCE & ENGINEERING SUPPORT

Seismic Retrofit

Dennis Coyne reporting

Documentation for the Conceptual Design Review has been prepared and posted temporarily here (until it is processed and posted in the DCC archive). A revised schedule is also posted the the same web page. We have slipped schedule to the point where there is little or no margin left in the schedule supporting an installation at LLO Jan 2003.

Rich with help from Peter has prepared electronics system layout/wiring including: Hydraulic Pump noise reduction servo, Geophone interface, Position sensor interface, STS interface and valve driver specifics among others. Rich also prepared initial schematics for the L4C field interface and has been in communication with Peter F. to develop the required topologies.

Expect to have received the EPI coil springs and initiate stiffness and strength testing this week.

New machined spring (stiffness test sample only) is expected within a week.

AID testing with multiple degrees-of-freedom started this week, after receiving additional electronics. Have achieved 5 DOF damping so far.

CDS Software

Rolf Bork reporting

- Hongyu has finished up the new EDCU software; ready to ship to Hanford.

- Alex and Khan working on updating digital suspension code to incorporate new 

filter module; target for completion is May 1.

- Lori and I working on updating LSC code with new filter modules; will test at 

Hanford next week.

CDS Hardware

Jay Heefner

Pentek Differential Driver/Receivers

The schematics for all four boards are complete and the board layout for one 

board is complete. The other three boards will be completed after the software 

for the new LHO 4K system is complete. Probably next week. In the meantime 

another driver/receiver part has been found by Rich. If we can get the parts we 

may redesign the boards to use them. The part is lower noise and much higher 

bandwidth. It is also fully differential in and out.

Jay Heefner

LHO 4K New SUS Software

The database records and state code for the new suspension code are ~80% 

complete. Operator screens for all of the filter modules (213 module and 2130 

filters) have been built.

Flavio Nocera

Finished with the design and schematics for the ISS. He is doing a final review prior to laying out the boards.

Ben Abbott

The ISS DC photodiode design has changed one last(?) time, to include a new differential driver, and new connector choice to better interface with Flavio's board.The pcb file should go to the board house sometime in the next day or two.

Mohana

Variable delay timing board have been getting stuffed and I will test the

first two boards when they are ready. I have also got a test procedure ready

for this board to give it for production. I wrote a test procedure for one of

Rich's PD Interface Board.

Sander Liu

Micro-Seismic Signal Processor -

Remote interface box's PCB is on order. They should be here sometime this week.

Inter connect cables design is now complete. Will start to build them in the field soon.

Post Processor PCB design is done. In the process of double checking the design before ordering them.

Since chassis design will take about a week and manufacturing by outside vendor will take another four to five, we plan to build the first set using stock chassis and send to the field as "Prototype" for the Science test. The unit will be retro-fit later when the chassis arrive.

PSL

Peter King

Using the power adjust actuator as the frequency actuator,

NPRO #259 was locked to the reference cavity.A number of measurements

suggest that this actuator is at least equal to the fast actuator.One

interesting thing to note is that when locked to the reference cavity,

adjusting the slow actuator by many tens of millivolts does not break the

lock.If this were to be done with the fast actuator, a 20 mV change in

the slow actuator voltage would be enough to break lock.The power

actuator coefficient is approximately 4.5 MHz/V.

Whether or not the use of this actuator results in some intensity noise

increase will hopefully be determined by a set of measurements to be

performed later this week.

A small circuit, that is the summation stage for the VCO, is currently

being tested.

Optical modeling

Bill Kells

Have spent most of this period preparing for presentation to e2e (Weds mtg) on results

of SB imbalance studies. The whole subject is now resonably consistant and summarizable. Many detailed

discussions with e2e gurus on the specifics (limits of modal model, sufficient state space, etc).

Erika D’Ambrosio

Mirror maps:

there are some features in the results obtained by Ken 

that are quite similar to the ones I got a couple of years ago. 

The most important thing is that the requirements for the imperfections 

become stricter. This can be explained with the analogy of what happens 

to the "longitudinal portion" of the electric field:

a higher Finesse squeezes the allowable "delta l". 

When the "transverse-dependant" part is taken into account something similar 

is expected to happen. I had also played around with the maps to see "where" 

the same imperfections were damaging the interferometer performance more.

SB Imbalance:

the SU(2) model for the study of the sideband imbalance is considered 

wrapped up and several comparisons with "special cases" have been done 

using simulation tools (Melody and FFT-code).

However some more runs are in order for some more "general" cases 

that have not been studied as part of the previous efforts for validating 

Melody so I tried to run the FFT-code on the CACR computers in order to 

save time and I had the bad surprise that my job was rejected because of 

allocation problems; it seems that "ligo-opt" has no allocation anymore 

and I don't quite understand what is going on about that.

Anyway this will not stop me and I can always copy all my directories 

to some other fast machine that "ligo-opt" is allowed to use as soon as 

I find out who may have these informations.

EOM Shutter Characterization

Peter F., Ryan and Dave O.

To support wave front sensor characterization at LLO the phase front

distortion of an EO shutter (identical one to that used on the ISC

tables at the sites) was measured. The measurement was done using a

Shack-Hartmann sensor and a HeNe probe beam. Two EOMs were measured, the

first gave good clear results, the wave front distortion was around 30nm

across the diameter of the probe beam (~5 mm). The second EOM we measured

gave very poor results, we were plagued with secondary reflections and a

very poor transmission for HeNe of less than 50%. Suggesting that the

coatings are on different shutters are quite different.

Improved Phase Camera Work

Nergis, Go and Dave O.

The aim of this project is to build on and improve existing phase camera

techniques (by Rana Adhikari and others) to be able to spatially 

profile a single sideband using a

heterodyne technique. This will be an additional diagnostic in trying to

determine the cause of the "badness" of SPOB. At the moment we are trying

to detect the beam note between two NPRO lasers.

Optical Contamination Cavity

Lee Cardenas, Liyuan Zhang and Bill Kells

Contamination cavity #2, Liyuan and I, are continuing taking data of ring down and beat frequency everyday.

We have a ring down situation that Liyuan and I are trying to understand.Our measurements show a longer decay time for both cavities.Cavity #1 the ringdown is 49us and previously was 36us. the transmitted power is only 7 mw with an input power of 110mw.(This is one of the situation that we try to understand, alignment is TEMoo, and mode match is accurate same for cavity #2)

Cavity #2 the ringdown is 33us and previously 24us.The transmitted power is ~78mw with an input of 120mw.

We have taken ring down measurements both cavities with four different photodiodesavailable,and all of them give us basically the same numbers with a variation of ~ 3us. Finally we found one home made old photodiode labeled 'Ringdown Photodiode Detector' (hopefully it is that one mentioned in lab notebook and in paper), so we measured the ringdown with it for the two cavities,basically, the Ringdown photodiode gives the same results as that of other photodiode, so there is certainly something else changed now. Following Jordan's suggestion, we checked the effect of the fitting parameters and found the variation of the ringdown is in range of ~2 us provided the fitting is good.

If we think the last mentioned result (~36 us) , in cavity #2 and results with different photodiodes

showsan average of ~ 33us.thenresults of cavity #2 are consistent, so maybe we could go ahead to set up the sample test.

Bill Kells comments are as follows:

The ringdown times you have measured are accurate. The mirrors in cavity 1

are higher in reflectivity than cavity 2; they were done in a separate

coating run. I believe the transmissions are: cavity 2, 70 ppm; cavity 1,

50 ppm So I have to conclude that the transmission of cavity 1 is low for some

other reason. Maybe polarization of the input light or something like that?

Or a servo oscillation? 

We did double check the polarization for both cavities and they are correct ( the 1/4 wave plate checks)

We are dedicating station #2 to production running with

contaminants (first samples preped this week). Station #1 reserved

for ongoing analysis of measurement resolution, sensitivity, stability.

We received hydraulic fluid samples from the seismic retrofit effort (mineral oil and Glycerin). The test bars which will be used as a substrate for the contaminant will be done baking Friday.

DMT

John Zweizig

This week I started writing the infrastructure software for DMT alarm

system. I have also modified the Frame writer to work with the next

version of FrameCPP and Fixed some bugs in Histogram2.


40 Meter Interferometer (Weinstein)



 



Thermal Noise Interferometer (Libbrecht)


no report


LASTI (Zucker)


LASTI (MacInnis, Mason, Mittleman, Ottaway, Rollins, Shoemaker, Zucker)
=======================================================================

Vacuum envelope:

Took RGA baseline and backfilled 4/4 to begin second round of stack
impedance characterization. RGA showed trace hydrocarbon signature, possibly
been due to extended Cambridge air exposure in first testing round.
Setting
up monitor to watch suspect molecular weights in subsequent pumpdowns to
distinguish diffusion vs. desorption time dependencies.

Myron is investigating compressed air cleaner/drier systems to reduce
our
dependence on bottled N2 seal gas for the pumps and possibly to provide
minimal clean purge capability.  Also ordered
a new bootscrubber (prior borrowed unit was recalled by owners).

BSC stack sharacterization for EPI design (Rich, Myron):

In the last week
and a  half we vented LASTI, opened up the BSC and
reinstrumented the stack internally with 4 Hz IDE geophones and
Wilcoxon 731A accelerometers.  We also added two new external sensors (L22-D
geophones, 2Hz) so we can now measure all 6 degrees of freedom on the
support structure.  We've taken 4 over night data runs; the ground noise
is much quieter, usually allowing us to run with high sensor gain.
Plan to complete these measurements and then repeat with the external
shakers oriented horizontally to probe translation and yaw.

External Pre-Isolator Design (Ken):

The welded support structure and the majority of machined parts have
been ordered for the hydraulic pre-isolator. The final quote for the
large machined foot is due today. The lead time for this part is 5-6
weeks.

Improvements have been made to the electro magnetic isolator to improve
cooling, reduce the overall mass of the actuator, and improved
positioning of the geophones. The welded support structure has been
ordered and the large machined foot final quote is due today.
Fabrication drawings for the mounts and actuator parts need to be
completed.

A fixture is currently being designed which will hold the crossbeam
during installation and provide  +/- 5mm course positioning of the
seismic load.

External Pre-Isolator EM Actuator Option (MZ for DHS):

Tested force constant and magnetic crosstalk from BEI magnetic forcer
to L4C geophone as a function of
geometry. Setting up to measure induced thermal gradients next.

PSL (Jamie and Dave):

Work continues to attempt to understand why our new FSS board does not
meet the performance expected due to its high electrical bandwidth. A
different alignment strategy actually worsened the performance. We have
ordered a new broadband EOM to determine whether the EOM is the limiting
factor. Preliminary modelling of the system using simulink has not
revealed any glaring errors.


Data Analysis and Computing (Lazzarini)


-----------------------
E2E MODELING (Biplab)
-----------------------

E2E Physics meeting
------------------------
In Wednesday's Physics meeting, Bill Kells gave a talk on some aspects of the
sideband imbalance problem and we had a long discussion on application and
limitation of modal model.

LIGO I simulation system
--------------------------
(Matt) Debugged seismic/stack model, final validation is underway. I also began
 work on testing the LSC system in anticipation of locking the IFO.

(Biplab) Did validation tests for seismic/stack model.

DAC noise model (Hiro, Matt)
----------------------------
The modeling of a DAC noise was completed. This is based on the following assumption.
When the digital value is changed, each bit takes some time to flip, and the observed
analog value is the weighted average of all intermediate values. E.g., when the value
changes from -1 to 0, there is an intermediate state 01111111, i.e., only the sign bit
is flipped, and this is a huge number. For 16 bit system, even the average time of the
bit flipping is O(1 nano seconds), this can introduce a noise of the order of 10 when
the sign of the value changes. The glitch when the sign changes is roughly proportional
to (bit flip time) / (measurement time) * 2^(number of bits).
We are going to validate this model by comparing the prediction with real measurements.

Code development and maintenance
---------------------------------
(Biplab) Validation of recent guoy-phase and mismatch related changes in code.

Alfi
----
(Melody)
 - Fixed more PRs for alfi5.  Currently working on resolving more popup menu
   issues and enhancing the settings value editor.

(Ed Maros)
 Continued to work on Makefile.am files for JAlfi

---------------------------
Hardware Systems (Anderson)
---------------------------

Caltech
-------
(Dan Kozak)

* Continued HPSS migration from Redwoods/3590s to 9940s.

* More HPSS user directory reconfiguration and account maintenance.

* Helped Greg Mendell at Hanford with Qlogic HBA firmware, T3 pSOS
  upgrades and FC switch firmware upgrades.

* Finally swapped out flaky Sun Ultra 10 for a spare LIGO Ultra 10.
  Still working to get StorageTek to make good on replacing the machine.

* LIGO SAN testbed:

        SAM-QFS still not working, but substantial progress made
        towards identifying the problem (it's not ACSLS but the SAM
        device tree).  Working with Lance at LSC/Sun to resolve the
        issue.

(Al Wilson)

* Trying to get tripwire working on a Solaris box. The web site has code for
  Linux. But no open source for Solaris. Still searching.

* Prepped rack in the test system for future T3's moved T3's into the rack
  for the CIT system

* Setup and installed Big Brother (BB) on the ldas-lho systems.
  Gathering files for remote administration of BB

(Stuart Anderson)

* Upgraded the CIT, TEST, and DEV LDAS systems to use openssh-3.1p1 for
  security reasons.

* Thinking about network topology issues to support inter-site database
  communication for advanced LDAS configurations.

* Installed additional UPS in LDAS-CIT system.

* Ordered initial datacon server for LDAS-CIT system.

MIT
---
(Keith Bayer)

* Finished reading E7 data back from tape.

* Trouble-shot Foundry switch problems.

* Investigated firewire to Linux for large cheap data repository
  for ldas-pcdev1.mit.edu (user request).

* Installed 100BT card on DMT machine (eventually to hook up to SF880)

Livingston
----------
(Igor Yakushin)

* Visited Caltech: made a presentation about DB2 features which we
  will be using soon (replication, federated system), talked to Kent,
  Stuart, Peter, Ed and Mary about how to proceed setting up replication
  for LDAS metadatabase and what experiments are needed to figure out the
  optimal configuration.

Hanford
-------
(Greg Mendell)

* Patched and updated firmware on the T3s, fiber channels switches,
  and fiber channel HBAs on the LHO LDAS network.  Coordinated with Dave
  Barker to simultaneously update fiber channel HBA firmware on the fb3
  framebuilder.  No updates were made to fb0 or the T3s that it uses.

* Worked with Igor and Julien to get a reduced data set onto tape and
  sent to MIT.  This is still in progress.

-------------------------------------
LDAS software development (Blackburn)
-------------------------------------

A significant effort has gone into testing LDAS this week. The code base
is still developing as we are feverishly adding the final features from
the target list of to-dos. Testing has revealed that database functionality
and the internal data format transmission through sockets are working as
expected. The ability to handle frames is working for time domain data that
is stored in the frames. There are still some issues with handling frequency
series data stored in frames which was discovered during testing. Testing has
also revealed a problem with collecting data objects for a single job at
the dataConditionAPI. This bug results in a "bad symbol" error and was
last calculated to occur in 3-5% of the jobs. Another problem with the
pre-release system was just discovered today. The nightly test script that
sends through a dataPipeline search job ever 30 seconds triggered a failure
mode at around 11PM for which all subsequent jobs failed to start up on
the Beowulf. We are not sure why the suddenly started to fail but we are
looking into it. LATE NOTE: This was do to a new objectSpace library being
pushed on the system by rsync last night.

We have begun some integrity testing of reduced data algorithms including
downsampling in the frame API. Need to verify that the data in the reduced
frames is correct and that all the channels required by the LSC can be
handled.

Added a "getResampleDelay" action to the dataConditionAPI to be used in
concert with shift() as demonstrated below in the example:

    y = resample(x, p, q, z);
    offset = getResampleDelay(z);
    yy = shift(y, offset, order);

This gives back a time-series yy starting at the same time as the original
x.
The interpolation() action was also renamed to shift() to better represent
its purpose. This shift() action has new tests at the unit and API level.
The resample() action has new unit tests which are performed during the
LDAS build. The final bit of redundant code has now been moved from the
dataConditionAPI subdirectory into the filters library subdirectory. Also
the windows class now has a new UDT wrapper.

The proper handling of detector geometry data stored in the frames has
now been fully tested and confirmed to work form input to output in all
dataPipeline jobs.

GUILD has been revised to handle the new frame cache index format in
the development version of LDAS, and to improve the utility which
watches the jobs running on an LDAS system.

The new diskCacheAPI is now working per its design requirements. This
is the first phase in a 3 part design of the diskCacheAPI so future
changes will occur starting with a migration to C++ cache trees and
the use of binary objects to store cache information. To date all
LDAS commands tested have worked with the new diskCacheAPI. This is
a significant step forward in our preparation for the next release.

Fine tuning and minor tweeks have occurred in all APIs this week as
we work towards increasing the robustness of this release. I suspect
that we will be able to have a similar success rate as with the E7
release but probably not much better...There has been a 10% growth
in the LDAS code base since the E7 release.

We held an internal database workshop this week here at Caltech for
LDAS to learn about and discuss the technologies available to use
through IBMs DB2 database software. Central topics covered were
database backups and recoveries, database replication, and database
federation. Igor will begin to prototype a model that will eventually
combine all of these aspects for LDAS and LIGO to use in its next step
up toward database management for the collaboration.

---------------------------
General Computing (Wallace)
---------------------------

MIT:
(Keith)
-Ordered more IP addresses from MIT for LIGO use.
-Ordered new low-cost printer for 11x17 prints
-Added 2nd graphics card to conf room pc (connect to projector)
-Fixed problem w/ VRVS software running on W2K
-Rebuilding old mailserver machine

Livingston:
(Shannon)
-Received the FORE equipment from Caltech.
-Still doing some recovery work from the LSC meeting.
-Working on resolving some network issues.
-Installed Norton Anti virus management console.

Hanford:
(Christine)
- Out sick most of this week.
- Finishing up with new PCs.
- Put a new battery in a laptop.
- Created a new user account, provide user support and CDS support.

(Larry)
-Working with Christine and Richard on getting more bandwidth to the WAN. The
connection using NoaNet appears to be a positive direction to go. PNNL has made
the switch to NoaNet and appears to be happy with the change.
We have a number of logistical issues to work out and will be getting LIGO
management involved in the next few weeks to help resolve a few issues but as of
now things are looking pretty good.

CIT:
(Mike)
-Finish putting together the backup Ghost Server and swapped out the old
one; this is now up and running.
-Loaded a new Laptop with special Engineering software for Janeen and Calum.
-Loading a PC to upgrade a user who is scheduled for an upgrade. On
this computer I had to add and replace hardware in order to get this PC
running correctly.
-Loaded Matlab for Norna R.; this installation took some time for the first two
installations did not work and had to completely uninstall and clear out
the registry and delete the Matlab directory in order to get this software
installed. This is now installed and seems to be running correctly.
-A Printer 4500, was having problems with paper jams; I did everything I could
but had no luck and had to call a tech to correct this problem. This turned
out to be one of the rollers were out of line from where the transfer kit
is located.
-Lisa has the PHP webserver up and running and has asked me to update all PC
information. I have been going around getting an updated list for all PC's that
includes IP numbers and MAC addresses, property tags and to whom they are
assigned; this is going to take sometime, I have started this and will continue
to update list as I work on the different PC's.
-Due to the limited amount of disk space I added an additional hard disk to
this server.

(Lisa)
- Finished up monthly backups
- Helped Larry put in a temporary kvm switch in the server room
- Setup a mailman mailing list "commissioning" for David shoemaker
- Working on a problem with the vacation program on the mail server.  It had 2
issues: 1) the new version of sendmail requires an /etc/shells entry and 2) the
new version of sendmail uses Berkeley DB with the vacation program.  This
portion of it is not yet fixed.
- Did some work on a prototype of a web-based inventory system for general
computing.
- Deleted and reinstalled the development environment on vega.
- Worked with Gary and ITS to get the ligo.org domain name properly hosted.
- Working on Cadence licensing issues with ITS.

(Veronica)
- LIGO website: the LSC transparencies keep coming in. I am posting them
as they arrive.
-Most time was spent on writing and testing various layouts of the new LIGO
Science Links webpage. Made several versions with different navigation
layouts to see which one is easier to use.
-Posted updates to the LIGO website (Fellowships, Elba Conference,
Internal BBoard).
-Met with Donna regarding the maintenance of the LIGO Visitors webpages.
- CaJAGWR: compressed the video of last week's talk by Massimo Tinto.
Video and the viewgraphs will be posted after the final security clearance
by JPL. Updated the seminars page.

(Larry)
-Worked with Lisa in getting the KVM switch swapped out in the server room.
Will be ordering a new one this week and the backup switch will be swapped out
when the new one arrives.
-Worked a couple of server and web issues.

-----------------------------------
Data Analysis Activities (Anderson)
-----------------------------------

* David Chin reported there were bugs in his clean locked segments,
  invalidating the SFTs I have generated.

* Since new release of ldas needs to be pushed to the sites next week,
  I will need to update the knownpulsardemod DSO to run under the latest
  releases of lal, lalwrapper and ldas.  Once this is done I will
  regenerate the SFTs at the sites.  The plan will be have this completed
  within two weeks from today.
(Greg)

* I have figured out how to build Masahiro & Daniel's Event Analysis
  Tool for distribution as a LIGOtools package on Solaris and Linux, but
  my testing of the Tool has found some apparent memory usage
  inconsistencies which are still being tracked down.

* Participated in a workshop about grid-computing security mechanisms
  using digital certificates, which is a technology being considered for
  use by LIGO for remote data analysis using LDAS, etc.

* Participated in discussions with Igor and others about strategies
  for federating the various LDAS databases and/or replicating data from
  one database to another.

* Worked with Veronica to improve the "Science Links" web page which
  is replacing the old Research Bulletin Boards web page.
(Shawhan)
 


LIGO II/Advanced R&D (Sanders)


For adv LIGO:

Bill Kells
Have completed a basic analysis of CR matching into
a (AdL) double cavity. The result is rather universal
thanks to the ~"degeneracy" (actually effective anit-degeneracy)
of the first (RC) cavity. As often the case, the result seems
simple in hindsight. Will be summarizing in write-up.
 

From: Helena Armandula <ahelena@ligo.caltech.edu>

Advanced LIGO Coatings
Received Ta2O5 / Al2O3 coated substrates from MLD. The coated parts will be evaluated for absorption and mechanical loss.

Advanced LIGO Suspensions
Received 4 polished substrates made from high density glass (# 24935 from Viox).
The parts will be used to evaluate silicate bonds.
 

From: Janeen Hazel Romie <romie_j@ligo.caltech.edu>

40m Suspensions
The three mode cleaner suspensions are in the chambers.
AdLIGO Suspensions
Calum, Norna and I are working on the MC suspension assembly. I'm looking into increasing the MC structure height to accomodate an optical table to beam height of 5.5", which is the same as the SOS beam height.

I received the LEDs and photodiodes for the sensor/actuators for the controls prototypes.

Working on a drawing template for Solidworks and AutoCAD for all AdLIGO drawings.

Working on combining the Solidworks files for the MC suspension assembly and the HAM chamber assembly, with the optical table moved to its lower (-315mm) position, to check for height clearances.
 

From: ctorrie <ctorrie@ligo.caltech.edu>
Mode Cleaner Suspension

Both CIT and GEO people (NAR, currently visiting Caltech, and colleagues at
Glasgow) are working on MC suspension design. We plan to have a drawing
review on Monday, April 22nd at 9:30am pacific. At that time, we'll go
over the mode cleaner design parameters and the drawings themselves. I am
taking  the drawing package to GEO when I visit in May.

Janeen and I met with Dennis Coyne and Ken Mailand to discuss a
standard drawing template for AdLIGO AutoCAD and Solidworks drawings.
Janeen will make up a template and distribute this week.

Janeen and I met with Norna, Phil, Mark Barton and Harry Ward to discuss the electronics for the Mode Cleaner and other suspensions. Specific numbers off for each suspension were discussed.

We have started to look at the Recycling Mirror design parameters.
____________________________________________________
From: David Shoemaker <dhs@ligo.mit.edu>
Subject: SWG: monthly reports

=======================================================

no reports from the seismic isolation people; please see
http://www.ligo.caltech.edu/~coyne/seismic_upgrade/design_review/seismic_upgrade.htm
for adequate documentation of their activities over the last few months!

================================

SWG progress Report for the Syracuse Group
submitted 10 April 2002 by Peter Saulson
Annealing chamber
Our annealing chamber for long vertical samples
is almost ready. We took delivery of a glass insert,
with plumbing for clean gas flow. After a few small
modifications, we should be ready to start annealing
fibers and rods.

Search for excess noise in anelastic apparatus
Scott Kittelberger has been analyzing time series
of noise from various sections of his electronics using
the same procedures as if he were measuring step function
responses. He is trying to track down the source of the
excess scatter in his measurements. There are hints that
the problem may be in his pre-amplifier of differential
amplifier.

Violin mode monitor
Andri Gretarsson has now taken all of the data for his
thesis (by construction, as he has now moved to LLO to
start his postdoc.) He took long undisturbed data sets
on his stressed tungsten wire at several different stresses.
He also measured ringdown Q's from driven motion, to compare with
Q at the Brownian level. (They agreed, until very large motions were
used. Apparently the clamps at the wire ends changed their properties
after a large drive.) Shortly before leaving for Louisiana, Andri
installed a fine silica fiber, and took noise data on its violin modes.
Andri defends his thesis at the end of May.

Personnel note
Steve Penn has accepted a faculty position at Hobart and
William Smith Colleges in Geneva, NY, to start this fall. He'll
be setting up a lab to do SWG-related research. Until that's ready,
he'll continue to do some research work in Syracuse. (Hobart is about
a 1 hour drive away.)
 

=================

10th April 2002
Suspensions Report from Norna Robertson covering GEO Glasgow and NAR at
Caltech.

A. Materials
1) Measurements on coating losses (to be reported by Sheila Rowan for
Stanford/Glasgow)
2) Bonding to heavy glass (E Elliffe).
4 different samples have been tested :
VIOX leaded glass V1656, density 3.84 g/cc
VIOX bismuth glass V1586, density 4.20 g/cc
VIOX leaded glass 24935, density 6.77 g/cc
VIOX bismuth glass 19911, density 7.23 g/cc
A silica ear was bonded to one of each sample (see attached picture).
Three of the four samples showed high bond strength, stronger than
silica to silica
bonds previously tested and some done at the same time as the heavy
glass samples, under the same conditions. The weakest bond was to the
highest density 7.23g/cc sample. From subsequent measurements it was
found that the higher density glass samples (6.77 and 7.23 g/cc) were
not flat but convex. All of the
samples showed rounding off at the edges (approx 2 mm ring) Some
staining was also visible on surface of the higher density samples. It
was surprising the 6.77 g/cc sample bonded so well given its shape. It
appears that the polishing technique particularly for the higher density
glasses needs some attention.

http://www.ligo.caltech.edu/~dhs/SWG/heavyglass.JPG

Key to picture. Top left V1656, top right 19911, bottom left 24935,
bottom right V1586. In top right sample the ~2 mm rounded off ring round
the edge can clearly be
seen.

B. Other Suspension Matters
1) Continuing work on design of modecleaner prototype for LASTI,
including mechanical drawings, and general design work for blade tests
(R Jones, A Grant, E Elliffe, G Cagnoli + CIT, JR, NAR at Caltech)
2) Continuing work on design and costings of mechanical parts (coil
former, holder etc) for local control for prototypes at Caltech and
LASTI (R Jones, E Elliffe + CIT Caltech)
(see Caltech report for further details of 1) and 2))

========================

Phil Willems

Fused silica suspensions:
-------------------------
Nothing to report.
Silicate Bonding:
-----------------
We have begun learning to use an atomic force microscope located on campus to
measure silicate bond interfaces. This could be a powerful tool to study creep.
It will also allow us to study the surfaces of differently-prepared fused silica
resonator samples provided to us by Boris Lunin.
Electrostatic charging of test masses:
--------------------------------------
We have begun plans to install cosmic ray detectors around the Moscow pendulum Q
chamber to better understand the charging events they see.

=================================

Janeen Romie
 

AdLIGO Suspensions Summary
CIT and GEO people (NAR, currently visiting Caltech, and colleagues at
Glasgow) are working on MC suspension design. We plan to have a drawing
review on Monday, April 22nd at 9:30am pacific. At that time, we'll go
over the mode cleaner design parameters and the drawings themselves. Calum
will be bringing the drawing package with him to GEO in May.
We are also looking at the RM design parameters.
CIT and GEO people are also working on the electronics design, whose
hardware is required for the controls prototypes. NAR has been considering
overall gains in local control for required settling times, and
corresponding sensor noise levels. Harry Ward is working on the
analog/front-end electronics and LIGO Lab will be working on the digital
electronics. To that end, we will be purchasing a dSPACE system for
controls development and testing. For the controls prototypes, it has been
decided that local control will be accomplished by a hybrid LIGO1/GEO
co-located sensor/actuator with the LIGO1 sensor and the GEO
actuator/magnet pair. Global control actuation will be accomplished by
using LIGO1 "osem" units with magnets on the penultimate mass and the
test mass. The sensors in the units can be used for diagnostics.
Calum and Janeen met with Dennis Coyne and Ken Mailand to discuss a
standard drawing template for AdLIGO AutoCAD and Solidworks drawings.
Janeen will make up a template and distribute this week. We will publish
these templates, upon agreement.

==========================

Rich Mittleman

MIT QUAD PENDULUM

Following Calum Torries calculations the masses on the reaction chain
have been trimmed. Mass has been removed from the bottom mass and added to
the top mass. This should correct the under damped pitch modes which have
been previously observed. The under damping of these modes has been
attributed to a greater than expected vertical distance between the center
of mass and the break off at the end of the blades springs on the two
middle masses. This is a result of the blade springs having a slightly
smaller spring constant than expected. The chain will be reinstrumented
and remeasured in the near future.
The discrepancy between the model and the measured two high frequency
modes, bounce at 29.3Hz and roll and 21.4Hz has been resolved.
The optimal damping level has been found and all of the low frequency
modes (<6Hz) damp well except for the previously mentioned pitch modes.

BSC Stack Characterization

The MIT BSC has been instrumented with 20 sensors (3 different types of
geophones and 1 type of accelerometer) and 4 shakers. The shakers and the
ambient ground motion we are characterizing the response of the LIGO-I
stack and support. The included plots
http://www.ligo.caltech.edu/~dhs/SWG/ExtZtoGeoXYZ.jpg
http://www.ligo.caltech.edu/~dhs/SWG/VDrivetoGeolXYZ.jpg
http://www.ligo.caltech.edu/~dhs/SWG/VDrivetoWilXYZ.jpg
http://www.ligo.caltech.edu/~dhs/SWG/VDrivetoWilangle.jpg

are only one step past raw and are
very preliminary.

==========================

Sheila Rowan

Report from Glasgow/Stanford on Q related work:
Since LSC, experimental measurements focused on investigation of any time dependence of Q of coated samples. Preliminary results suggest may see some degradation of Q with time - still under investigation.
Two Al2O3/Ta2O5 coated silica samples from MLD next in line to be measured as part of the main coating loss program.

After discussions at LSC, calculations of ("standard") thermo-elastic damping in
thin flexing samples of sapphire revisited re: using thin coating samples
- still looks to be at a significant level.

=====================
Helena Armandula

Heavy glass
Received four polished 1/2"dia. substrates made from Viox # 24935. This is a high lead glass with 6.77 gm/cc density.
The company that polished it, J.L Wood, had a very hard time keeping the glass from staining.
The substrates will be silicate bonded to fused silica to test bond strength.

=====================

Gregg Harry

We have been finishing up Q measurements on the
silica/tantala coated samples. We measured the
drumhead mode of sample 3, which is coated with 30
layers of silica/tantala in even proportion. The
Q was 424,000. We also measured the drumhead mode
of sample 4, coated with 2 layers of silica/tantala
in even proportion. The Q was 6.4 million. These
values give coating phi's of 1.7 10^-4 for sample 3
and 1.9 10^-4 for sample 4, which are a little high
compared to other modes. We are continuing to make
measurements on sample 4.
We have finished the FEA modeling and calculation of
the energy in the coating for all measured modes. For
both the butterfly modes and the drumhead, the ratio
of energy in the coating to the substrate increased
by 5 percent from the values presented at the LSC
meeting. This means the predicted coating phi dropped
to around 1.5 10^-4 from 1.7 10^-4 presented at LSC.
This makes it closer to the value 1.0 10^-4 measured
on the even silica/tantala sample coated by REO.
Using the final values from the FEA we find phi values
for silica and tantala; phisio2 = -0.26 +/- 0.43 10^-4,
phita2o5 = 2.3 +/- 0.15 10^-4.
We are in possession of a 30 layer alumina/tantala  sample
coated at MLD in Oregon. It will be the next sample
we measure.

====================

Mark Barton

I've been doing validation on the thermal noise code. In fact I hadn't
been calculating it right and in the process of correcting it I got a
good education in the physics of dissipation dilution which it might be
of interest to summarize. The general principle is that the net restoring
force can be broken down into two components: (i) that due to first order
dimension changes in elastic objects and (ii) that due to changing the
mechanical advantage between elastic objects under constant stress and
the output. Only the first component contributes to the net loss, but
early versions of my code did not take this into account. The fix was to
calculate the elasticity matrix for stage 0 of the calculation twice, the
second time setting all the static forces and tensions to zero, and to
apply the loss angle multipliers only to the tension-free elasticities.
The fix has been tested on a toy model of a simple pendulum and has been
validated against analytical predictions. The corrected toy and quad
models can be downloaded from <http://www.ligo.caltech.edu/~mbarton/
SUSmodels/>. The fix for the triple model will be straightforward but I
haven't gotten to it yet. The quad model is now more or less feature
complete. The only thing remaining to be done is to put in better values
of some of the more obscure blade parameters, but it can be used as-is to
study most things connected with the 24 low-frequency modes.
 


For additional information about this report, contact sanders@ligo.caltech.edu