Weekly Report for Week Ending August 7, 2008


LSC

Administration

Hanford Observatory

Livingston Observatory

Optical & Mechanical

Controls and Data Systems

40 Meter Facility

TNI

LASTI

CIT Science Group

Laboratory Computing

Adv. LIGO Development & Project

Past Weekly Reports


There will be no meeting of the LIGO Executive Committee Monday, August 11, 2008. 
A Staffing Committee Meeting is scheduled that morning.

 

Calendar of future Executive Commitee Meetings


LSC Issues (Reitze)

No report provided.


LIGO Laboratory Administration (Lindquist)


STATUS OF LSC MOUs (Lloyd)

MOU
Attachments
Approved
ACIGA
ACF, DAT, LAS, OPS, OPT, OUT, SUS, Z
Andrews University
DAT, OPS, OUT, Z
Balearic Islands
DAT, Z
x
Carleton College
DAT, OPS, Z
x
Caltech Exper. Grav.-Physics Group
SUS, Z
x
Caltech Relativity Group
ACF, DAT, OPT, OUT, Z
x
Columbia University
DAT, OPS, OUT, Z
x
Embry-Riddle Aeronautical University
DAT, OPT, SUS, Z
Eotvos University
DAT, OPS, OUT, Z
Florida, University of
ACF, DAT, OPS, OPT, OUT, SUS, Z
x
GEO600
ACF, DAT, LAS, OPS, OPT, OUT, SUS, Z
x
Goddard Grav. Wave Astrophys.Group
DAT, OPS, Z
Hobart & William Smith Colleges
OPS, OPT, OUT, SUS, Z
x
Institute of Applied Physics
OPT, OUT, Z
IUCAA
DAT, Z
x
Louisiana State University
DAT, OPS, SUS, Z
x
Louisiana Tech University
DAT, OPS, OUT, Z
x
Maryland, University of
DAT, OPS, Z
x
Massachusetts at Amherst, University of
DAT, OPS, Z
x
Michigan Gravitational Wave Group
DAT, OPS, OUT, Z
x
Minnesota, University of
DAT, OPS, SUS, Z
x
Mississippi, Uiversity of
DAT, OPS, OUT, Z
x
Montana Grav. Wave Astronomy Group
DAT, Z
x
Moscow State University
Z
NAOJ-TAMA
ACF, Z
x
Northwestern University
ACF, DAT, Z
Oregon, University
DAT, OPS, OUT, Z
Pennsylvania State University
DAT, OPS, OUT, Z
Rochester, University of
DAT, Z
x
San Jose State University
ACF, Z
x
Sannio, University of at Benevento
DAT, OPT, Z
Sonoma State University
LAS, OUT, Z
Stanford University
ACF, LAS, OPS, OPT, OUT, SUS, Z
x
Syracuse University
DAT, OPS, OPT, Z
x
Texas, University of at Austin
DAT, OUT, Z
Texas, University of at
DAT, OPS, OPT, OUT, Z
Trinity University
OPT, OUT, Z
x
Washington State University
DAT, OPS, Z
x
Wisconsin at Milwaukee, University of
DAT, OPS, Z
 

PROPERTY MANAGEMENT (Luna)

>From: Rod Luna <rluna@ligo.caltech.edu>

DOCUMENT CONTROL CENTER (Turner, Mak)

>From: Linda Turner - turner@ligo.caltech.edu>

FINANCIAL SYSTEMS (Funaro, Oracion)

> From: "Funaro, Catherine" <Catherine.Funaro@caltech.edu>

> >From: Karl Oracion

SUBCONTRACTS MANAGEMENT (Jasnow, Salone)

>From: Rudy Arvizu <arvizu_r@ligo.caltech.edu>

>From: Gina Salone <gsalone@ligo.caltech.edu>

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

PROPOSALS and REPORTS (Lindquist)

CHANGE CONTROL/CONTINGENCY MANAGEMENT (Lindquist)

The following Change Requests were discussed during the meeting of the Executive Committee on August 4.  Approval was recommended.
In addition CR-080013 requesting additional budget for Advanced LIGO R&D accounts was distributed.  All recommendations were for approval.

Minutes are being prepared (LIGO-M-080321-00-P) and will be distributed.

HUMAN RESOURCES (Akutagawa)

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


Quality/Safety (Tyler)

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


LIGO Hanford Observatory (LHO) and Interferometer Operations (Raab)

LHO Outreach (D. Ingram)


LIGO Livingston Observatory (LLO) and Interferometer Operations (Giaime)

Enhanced LIGO Installation and Commissioning (Valera Frolov):

Safety & Security (Rich Riesen):

Outreach (Deborah Muhammad):

LIGO computing and network security (Roddy)

Reported under General Computing, see below

General computing and LDAS admin (Giardina)

Reported under General Computing, see below

Reported under LDAS System Administration, see below

Data analysis & computing (Yakushin)

Storage/Condor/LDAS admin:

Reported under LDAS System Administration, see below

Data analysis:

Reported under Data Analysis activities, see below


Mechanical and Optical Systems (Coyne)

See Advanced LIGO


Controls and Data Systems (Bork)

See Advanced LIGO


40-Meter Interferometer (Adhikari)

  • After the earthquake, we've been working on recovering the interferometer. We vented the 40m vacuum system on Monday. The venting went fine. We inspected suspicious optics, ITMX, SRM and PRM. Apparently, the vent freed the ITMX, which seemed to be stuck somewhere before the vent. SRM's side magnet fell off and was stuck to the LR magnet. We picked it up and moved the side OSEM to the other side where another magnet was intact.
  • We used the laser for the absolute length measurement (see below) as a reference and aligned the ITMX, ITMY, BS and SRM.
  • The PRM magnets are all there and the mirror is not touching anywhere. But the mirror is tilted in pitch a lot. The wire seems to be in the grooves of the stand-off, although the farther side is difficult to see. We suspected the wire is shifted a bit on the bottom of the mirror. We lifted the mirror very gently using the bottom earthquake stops to relieve the tension of the wire and pushed the mirror on the face using another earthquake stop screw to make the mirror upright. Then the bottom earthquake stops were slowly lowered so that the mirror sits on the wire again. By repeating this many times, we hoped that the mirror comes back to upright position. So far we were able to change the angle, but the PRM is still not perfectly upright.
  • The absolute length measurement of the Y-arm cavity was done by Koji. The FSR and the length of the Y-arm are measured to be:
    f_FSR = 3878678 Hz +/- 30 Hz
    L_yarm = 38.6462 m +/- 0.0003 m

    He also found a split in the resonant frequencies of TEM01 and TEM10 modes. These techniques should allow use to measure the length of the recycling cavities as well as get the astigmatism of the COC.
  • Joe has been trying to use Gstreamer for compressing the data from the GigE cameras to avoid the saturation of the network.
  • The MZ for the fiber noise measurement is reconstructed with better mounts. Testing an AOM for the noise cancellation experiment.

Thermal Noise Interferometer (Black)


LASTI (Mittleman)

BSC-ISI

Quad Prototype

Fiber Pulling-Welding


CIT Science Group (Weinstein)

___________________

Antony Searle:

___________________

Drew Keppel:

___________________

Kent Blackburn for the Grid R&D Team:

GRID APPLICATION DEVELOPMENT

OPEN SCIENCE GRID INTEGRATION & VALIDATION TESTBEDS

GRID MANAGEMENT

___________________

Amber L. Stuver:

___________________

Kipp Cannon:

___________________

Joseph Betzwieser:

___________________

Anand Sengupta:

___________________

Igor Yakushin:

___________________

Chad Hanna:

___________________

Gregory Mendell:

___________________

Pinkesh Patel:

___________________

Diego Fazi:

Christina Torres:


Laboratory Computing (Anderson)

(Compiled this week by Kozak)

LDAS Software Systems (Maros)

LDAS System Administration (Anderson)

(Kozak reporting for Anderson)

Caltech

(Dan Kozak)

(Phil Ehrens)

MIT

(Fred Donovan)

Livingston

(Igor Yakushin)

Hanford

(Gregory Mendell)

General Computing (Wallace)

MIT

(Fred)

Livingston

(Dwayne)

Hanford

(Larry)

(Mike)

Caltech

(Veronica)

(Christian)

(Melody)

(Mike)

(Larry)


Advanced LIGO and Supporting R&D (Shoemaker)

Advanced LIGO Management

Advanced LIGO Systems

Dennis Coyne <coyne@ligo.caltech.edu>, Peter Fritschel <pf@ligo.mit.edu>, Calum Torrie<ctorrie@ligo.caltech.edu>

AdL Project-Funded Activities

Design Reviews:
    For a list of reviews, see the main AdL wiki page

Procurement Reviews:


Technical Review Board (TRB)
:
    see the TRB log

Vacuum Review Board (VRB):


Configuration Control:

Design:

Interfaces:

Modeling and Simulation

From: Hiroaki Yamamoto hiro@ligo.caltech.edu

 

 

Static IFO simulation (Hiro)

----------------------------------------------

 

Hiro starts to calculate various quantities to help the COC design finalized, which includes the choice of the beam size in the Michelson cavity and the loss due to the BS curvature.

 

 

Hiro has modified SIS further to help Bill's analysis.

 

 

Hiro sent  to Hans about the documentation and the binary code of SIS. Hans is going to help Bill to update the PI calculation using SIS.

 

 

Melody started working on the parser code of SIS to correctly parse functions with vector parameters.

 

 

Mechanical Simulation for advanced LIGO (Sany and SLU team)

-----------------------------------------------------------------------------------------

 

Made substantial progress in length and frequency control servos in our e2e modeling of the AdvLIGO IMC. By adjusting zeros and poles of the length and frequency control filters, succeeded in getting rid of the bump that we used to have in the MC transmitted light’s frequency noise spectrum near the cross over frequency. As compared with the previous best result, the frequency noise is an order of magnitude lower in the frequency range of 200 – 1000 Hz. The frequency noise spectrum still shows some structures corresponding to the triple suspended optic’s resonance near 1 Hz, which seems to be further improved by properly increasing the length control gain. With PSL frequency noise of 2e-3 Hz/rtHz incident to the IMC (dc to 1000 Hz), the frequency noise on the IMC’s transmitted light starts to go down around 50 Hz, reaching 1e-4 Hz/rtHz level around 800 Hz. Further study on the IMC frequency noise is under way. 

 

Facilities Modifications and Preparations

            From: John Worden worden_j@ligo-wa.caltech.edu

Nothing to report this week.

Seismic Isolation

From: Ken Mason kmason@ligo.mit.edu

HAM Crossbeam Design
Sending final drawings for LASTI prototype Crossbeams to machine shop on Friday. Still working on remaining details: L-4C clamps, Support Tube clamps, HEPI Caging assemblies, etc. ~ Andy S.

BSC ISI Design
Making further changes to the AdLIGO BSC LARGE actuator assembly models so that these can be tested at LASTI with fewer changed pieces. e.g. designing some adapter plates so that we can try the design changes on the actuator brackets without changing the large, expensive stage 0 post and bridge that these brackets will ultimately attach to. Hope to be making drawings for these models by next week so that these prototype parts can be quoted then ordered before the end of August.

The SMALL actuator assemblies are stalled at the concept model stage--- without the models from PSI for the small actuators themselves the surrounding brackets can't be dimensioned or have holes added, etc. Still in contact with PSI about getting these small actuators moving. ~Stephany F.

SEI Project Activities
Quotes for the HEPI actuators are due today.  ~Ken M.

Suspensions

From Janeen Romie and Norna Robertson
  (romie_j@ligo-la.caltech.edu, nroberts@ligo.caltech.edu)

 

*Operations Work *

 

HAM Suspensions for Advanced & Enhanced LIGO

 

 

OMC. The LHO OMC SUS team has made transfer function measurements (posted on the LHO elog) with the metal bench, and these compare well with the MATLAB model.  They have now installed the the ISC glass bench and after aligning will take more transfer functions to check everything OK before installation.

 

 

Large Triple prototype. We are starting to receive quotes for the large triple blade and wire clamps, needed to characterize the blades. We hope to initiate procurement this week. The drawing tree and parts list are complete. A few parts still need drawings and most need some changes. There is still some work to be done on EQ stop design for the back faces of the intermediate and test masses.  We are also considering using cam-type OSEM adjustment fixtures ( similar to those developed for the BOSEMs).

 

 

Small triple. We are working on further preliminary design review documentation.

 

 

BSC Suspensions for Advanced LIGO

Work continue towards the monolithic build at LASTI now scheduled for September.

 

 

Brett Shapiro has updated his document on quad balancing and alignment procedure and circulated for comments.

 

 

Doug Cook is researching a device to measure the gap between the ETM/ITM and the reaction mass.

 

 

*Project-funded activities*

Work has begun on the RFQ for the SEI and SUS mechanical test stands for the sites. Ken Mason has finished updating the drawings and Betsy has begun organizing the statement of work. We need one BSC-style mechanical test stand for the quad training at LLO in November. The rest of the test stands (quantity 5 total) are not needed until next year.

 

 

Work has begun on OSEM value engineering. Focus is on whether the head/former needs to be plated alumina, or whether it can be changed to metal. Also, focusing on whether the components should be changed to the LED & photodiode that the Birmingham OSEM use. A number of other issues have been identified for value analysis.

 

 

Work has begun on organizing the RFQ for the quad production assembly tooling. We are still awaiting RAL updates of the top stage tooling, which is scheduled to be completed this week.

Core Optics

From: GariLynn Billingsley Billingsley_G@ligo.caltech.edu

Project
Heraeus and Corning orders have gone out, both are under review at the vendors, we expect signature this month. 

We are planning to release documents for final design review in the coming week.


Development
We have fairly conclusive evidence that the highest grade fused silica from Corning contains inclusions, too small for their inspection to capture, that contribute to high scattering, up to 2000ppm in spots.  While that material may be used for transmitting control signals we recommend that it not be used in loss sensitive applications, ie. in transmission, as part of a resonant cavity, or in transmission in a loss sensitive beam train. 

Until formally written, the results can be found here:  http://www.ligo.caltech.edu/%7Elzhang/esw03/esw03_ars_sum_2.pdf  This is a summary of data taken on a septum window Corning grade 0AA.   As a system check we measured a 1" piece of the same material and found it to be reasonable. Other zones in the septum window also measured at expected values.  In light of the upcoming Advanced LIGO IOO procurements, a piece of Heraeus 311 SV (40m BS spare) T080185-00 (currently in DCC out.)  We were only able to measure a 5mm x 40mm line, but found it to be uniform and low.

The tooling and compensation plate for LASTI are at Navitar for gold ESD coating and barrel coating.  Their quoted delivery time is four weeks from this point. 

QED has finished one iteration of MRF on the re-finished pathfinder.  They have their surface measurement IFO out for repair, but are not projecting a schedule slip.

Tinsley pathfinder has been delivered from Coastline to ASML, it is currently in soak for initial metrology.  First look puts the ROC very close to the desired finish, this means little removal of material.  Quite encouraging.  The Tinsley metrology review is scheduled for August 21 at Tinsley.  Tinsley is currently projecting a 11 day slip.

We have approval to go ahead with a coating experiment where three different polish techniques are coated in the same run.  We hope this will shed light on the contribution of polish to scatter.

Auxiliary Optics

From:   Michael Smith smith@ligo.caltech.edu

ADLIGO

Work under Project budget

Work under Operations budget
SLC
Mike has revised the concept for baffling of the wide angle scattered light from the ITM and ETM. He proposes a cylindrical baffle close to the COC HR surface and against the Arm Cavity back surface. Without the cylinder in place, the wide angle scattered light onto the BSC chamber and manifold walls, assuming 10 ppm Lambertian scattering loss from the COC surface, exceeds the AOS requirement.

ADLIGO
OPTLEV
Tara, Giovanni, and Zach are continuing to refine their intensity noise measurements of a free-space HeNe beam on a benchtop hitting a quad photodiode.
Robert Schofield is continuing to measure the angular noise characteristics of the LVEA floor and the optical lever piers at LHO.

ETM TEL SUS
Virginio has a preliminary model for the ETM Telescope Suspension, using the masses and moments of inertia given him by Chris.

ELIGO
SLC
Luke completed the installation of the HAM5 baffle at LHO.
Ken completed the installation of both manifold baffles at LHO. He is revising the installation procedure slightly and will communicate that to Gary at LLO.
The Staff at LLO installed the ETM baffles.

Input Optics

From: Rodica Martin <rmartin@phys.ufl.edu>
 

ELIGO Commissioning:

 

Measured FSS AOM double pass diffraction efficiency (61%). Completed FSS beam path.

Reference cavity moved to the new location on the PSL table and locked again.

Started optimizing reference cavity visibility (75%). - Antonio

 

Preparing for LLO IO vent - Kate

 

Modulator preparatory work and PSL work - Volker

 

Advanced LIGO:

 

We have been looking at the beam splitter flatness and allowable tolerance in the recycling cavity - Muzammil

A brief study can be found at:

http://lhocds.ligo-wa.caltech.edu:8000/advligo/Recycling_Cavity_Geometry?action=AttachFile&do=get&target=flatnessBS.pdf

 

Finished aligo mach-zehnder EOM design, finishing aligo in vac-mirror blank drawings - Luke

 

Prestabilized Laser

From: Peter King pking@ligo.caltech.edu

Operations

==========

    In talking with an engineer at Ophir about their L50A-SH calorimeter,

they mentioned that the calorimeter is not meant to be exposed to a high

power laser beam for long periods of time, ie overnight.  The accuracy of

the calorimeter falls as the temperature of the calorimeter increases

beyond 75 degC.  Typically a stable reading is achieved after 2 minutes.

 

Project

=======

    Another draft of the preliminary design document was released amongst

the working group.  We are still aiming for a mid-August release of the

final version.

 

Some investigation is being carried to figure out why the 4k laser at LHO

tripped out.  Whether the chiller tripped and caused the laser to go, or

vice versa.  One scenario raised by Christian Veltkamp (LZH) is that the

mains voltage dipped below some level causing the NPRO power supply to go

out, which turn cascaded to the 35-W laser going.  The jury is still out.

 

CDS

            From: Rolf Bork rolf@ligo.caltech.edu

- The majority of DAQ PDR documents have been posted to the AdvLigo CDS Wiki. One more remains to be posted, the Software Development Plan, which Vern should have done soon. Some comments/questions starting to come in from the review committee and others.

- More work on the ELigo DAQ system installed at LHO, which employs the basic designs proposed for AdvLigo. Primary focus this week was to get all of the GDS TP/EXC working through the new NDS servers. This now all seems to work, with proper connections to DTT and Dataviewer. Tomorrow, the initial Ligo FrameBuilder (running in parallel with the new system) will get updated software such that both old and new DAQ can get data properly from the new ISI/OMC computers (byte swapping issue between existing Solaris FrameBuilder and new x86 based systems).

- Timing: Work continues on the slave modules, with hardware/software being added to provide the dual tone generator.

- Continuing to design/order components for the 40m lab upgrade as the AdvLigo controls prototype.

- Adding new features to the realtime code generator in support of various ELigo/AdvLigo application development activities:

   - Ability to read a separate coefficient file for FIR filters (used in HEPI/ISI).

   - Ability to turn on/off filters within a filter module from within the user application (previously just thru EPICS).

   - Bit to word and word to bit parts to help reduce the user logic necessary to drive binary in/out modules and the new filter controls.

   - Device driver to interface the new 32bit binary output module.


For additional information about this report, contact Albert Lazzarini