Weekly Report for Week Ending May 3, 2007


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

Past Weekly Reports


The LIGO Executive Committee Agenda for Monday, May 7, 2007 will be:

(Meeting time: 10:30 am Pacific Time)

1. Announcements

2. Programmatic (Marx)

  • End of April LIGO Operations Financial Review
  • Change Requests (see Below)

3. Comments on Weekly Report

4. LSC and Data Analysis (Reitze)

5. LIGO Lab Operations

  • Administration (Lindquist)
  • Sites (Raab, Giaime, Shoemaker)
  • Commissioning (Fritschel)
  • Optical and Mechanical (Coyne)
  • Control and Data Systems (Bork)
  • 40m (Weinstein)
  • TNI (Libbrecht)
  • LASTI (Ottaway)
  • Lab computing ( Anderson )
  • Data Analysis Group (Weinstein)
  • Instrument Science (Gustafson)

6. Enhancements (Zucker)

7. Advanced LIGO (Shoemaker)

8. Change Control Board/Technical Review Board Session as needed

  • Change Request CR070002 adjusts the budget to reflect actual hires in the first half of FY 2007 as well as corrections to actual payroll rates (salaries, raises, etc.) used in the FY2007 budget model.
  • Change Request CR070003 realigns budget for the Advanced LIGO Seismic Isolation effort.

Site and other Business Issues:

Special Items:


Special Announcements:


Weekly Report Highlights


LSC Issues (Reitze)

First, an update on two LSC papers observational papers:  the S4 all-sky burst paper was submitted to Classical and Quantum Gravity on Thursday; and the S3/S4 inspiral paper was posted on arXiv last week (http://arxiv.org/abs/0704.3368) and is waiting for comments from GWIC before submission to Phys. Rev. D.

In addition, a total of 37 LSC-related abstracts were submitted to the Amaldi meeting.  Special thanks goes out to the Publication and Presentation Committee for carefully vetting the abstracts before submission.

Finally, plans continue for the upcoming LSC-Virgo meeting.  Information and registration details can be found at https://pub3.ego-gw.it/lscvirgomay07/

LIGO Laboratory Administration (Lindquist)

STATUS OF LSC MOUs (Lloyd)


PROPERTY MANAGEMENT (Luna)

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

DOCUMENT CONTROL CENTER (Turner, Mak)

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

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

Update to Current Document Management System (Lindquist)

J. Giaime has prepared a web page for the committee with some instructions for accessing and running a copy of DocDB for evaluation purposes.  There is no meeting scheduled this week.

FINANCIAL SYSTEMS (Funaro, Brambila, Kaufman)

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

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

>From: Florence Kaufman <fkaufman>

SUBCONTRACTS MANAGEMENT (Jasnow, Salone)

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

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

PROPOSALS and REPORTS (Lindquist)

Material for the monthly report that we provide to the NSF is due.  I will provide an outline and a reminder of responsibilities.  I need this by Friday, May 11.

CHANGE CONTROL/CONTINGENCY MANAGEMENT (Lindquist)

HUMAN RESOURCES (Akutagawa)

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


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

Summary of S5 Activities at LIGO Hanford Observatory  (compiled by M. Landry)

The intererferometers achieved what are now typical and high duty cycles and ranges: H1 - 89% at ~15Mpc, and H2 - 90% at a newly restored, decent  range of ~7Mpc (see the "timing fanout" bullet below).

Some S5 highlights from the LHO elog are bulleted below:


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

DC readout work for eLIGO (Valera Frolov):

  • The output mode cleaner cavity (spare PMC cavity) was dither locked to the carrier light on the antisymmetric port with the interferometer locked at high power in FPRMI configuration. To achieve the stable locking and minimize the noise from the OMC length the bandwidth of the pushed to 350 Hz.
  • One quarter of the dark port light was directed to the OMC by taking the beam from one of the AS port detection diodes.
  • The offset of the order of several picometers was introduced into the differential arm degree of freedom to produce the linear coupling between the DARM and the power of the carrier light at the dark port.
  • After setting the relative gain and checking the loop shape between the DC and the RF photodetector sensing chains, the DARM control was handed off from the acquisition PD (ASPD5) to the DC PD on the OMC transmitted port.
  • After careful alignment of the OMC input beam with the ifo locked in high power state, the DARM noise at frequencies above the 200 Hz was mostly limited by the electronics noise of the DC photodetector (due to the LSC whitening limitation). The current DC readout noise is about factor of 50 above the S5 curve. The noise can be improved by modification of the DC PD circuit to match the LSC whitening input.
  • The next step is to verify the noise coupling to the dark port in the DC readout scheme including the laser frequency and amplitude noise and the oscillator phase and amplitude noise.

CDS Computing (Lisa Bogue):

  • spent most of the week working on LDAP.
  • supported the blind injection project.
  • working on orders for new equipment.

LLO Science Outreach (John Thacker):

  • Planned, Developed and Delivered two programs for school visits (1 Middle School; 1 High School)
  • Hosted the LA Math/Science Partnership Workshop on the evening of May 2nd. Dinner, tour of control room, Einstein's Messenger viewing and Exhibit Play were the program components for the 21 attendees. The 21 attendees represent the science curriculum leadership at various parish school systems and may prove helpful to our efforts to expand our reach.
  • Held the LIGO SEC Directorate F2F meeting and addressed procedures for closing the current grant, developing ideas for the Next Phase and establishing bylaws for governance of the partnership.
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 (Weinstein)

Thermal Noise Interferometer (Black)

While waiting for our mirrors with aperiodic coatings, we have decided to go ahead and measure the thermal noise at two other spots  on the existing mirrors. Ilaria has designed a scheme for doing that, with input from Riccardo, and she has started on this experiment.

LASTI (Mittelman)

Friday, 4 May was David Ottaway's last day with LIGO. We wish him well as he returns to Australia. Responsibility for the oversight of the LASTI facility has been taken on by Rich Mittelman.

CIT Science Group (Weinstein)

________________________
Patrick Sutton:

I've spent most of the past week on LSC-PP duties and making MDC frames for the GRB070201 analysis.

GRB070201:

  • Finished production and testing of the sine-Gaussian and white-noise-burst MDC frames for the GRB070201 analysis, using X-Pipeline simulation codes.
  • Wrote summary document of the preliminary X-Pipeline results for GRB070201 analysis, as requested by Marka.

Other:

  • Reviewed Mukherjee's paper on glitch classification for GWDAW proceedings.
  • Handled review of BNS review paper by Anderson and Creighton.
  • Data analysis meeting.
  • LSC-PP telecon.
  • Bursts telecon.
________________________
Igor Yakushin:

Running coherent waveburst trigger production and sine-gaussian simulations on the first year of S5 in preparation for the LSC and Amaldi7 meetings. The networks currently used are: H1H2, L1H1, L1H2, L1H1H2. We shall probably also use some networks that include GEO, at least L1H1H2G1.

________________________
Gregory Mendell:

Not much to report for the last week, but I will be getting back to work on the S4 PowerFlux/StackSlide/Hough paper soon, as well as completing some work for the pulgroup to be presented at Amaldi this summer.

________________________
Eirini Messaritaki:
  • I have been spending most of my time finishing up and debugging the code that performs the null stream test for H1-H2 for the inspiral analyses.
  • I have been working with the people involved in the follow-up project.
  • I have been working with Vibha on her SURF project proposal.
________________________
Kent Blackburn:

OPEN SCIENCE GRID APPLICATION DEVELOPMENT

  • Successfully ran NanoHipe at 7 different OSG sites
  • Run NanoHipe on the FNAL_GPFARM site successfully on the FNAL_FERMIGRID  site it failed
  • Conducted error analysis of Failure on FERMIGRID with help from Steven Timm at Fermilab
  • Started full Hipe at Milwaukee's OSG site.
  • Inspection of results of NanoHipe run on GPFARM
  • Getting familiar with TWiki, editing on TWiki
  • Reading Condor online material in preparation for Condor Week 2007
  • Attending Condor Week 2007 in Madison Wisconsin.

OPEN SCIENCE GRID INTEGRATION TESTBED

  • Documented on the OSG Twiki, an addenda to installing and configuring the ws-gram interface in OSG 0.6.0 that captures configuration information required to increase the robustness of the interface when >200 jobs are submitted in a short interval.
  • Configured syslog-ng to send gatekeeper, gridftp and Globus container logs to a logging repository at UChicago as part of a testbed on a central logging facility for OSG.
  • Successfully used srmcp to transfer 64 gravitational-wave files to the UCSD Storage Resource Manager.
  • Attended DASWG, ITB, LIGO-Pegasus and VTB telecoms.

OPEN SCIENCE GRID MANAGEMENT

  • Attended OSG Executive and Finance Board Meetings at Fermilab last week.
  • Reviewed changes to University of Chicago Statement of Work to get through their office of sponsored research.
  • Reviewed new Statement of Work from NCSA with the OSG which precipitated out of IOWA PI transitioning to a new position at NCSA.
  • Discussed plans to begin running h(t) based HIPE analysis on the Open Science Grid with Steve Fairhurst.
  • Provided the list of OSG milestones affiliated with LIGO that Kent Blackburn, Warren Anderson and Doug Olson (LBNL) are carrying as the "owners" to the LSC Computer Committee.

Laboratory Computing (Anderson)

LDAS Software Systems (Maros)

After much investigation, it has been theorized that the diskcacheAPI has issues with frame files of two second lengths. The theory is being tested by creating a unit test to simulate the condition.

After generating a mail storm, the logscan utility was modified to write out email state to state file so as to throttle mail messages even when there are many restarts of APIs. The new code has been shown to work properly.

The two TCL commands, getFrameCache and getFrameFiles, have been modified to execute within a C++ thread.

An issue was discovered with the weekend testing where the managerAPI would continuously reboot APIs. The garbageCollect routine is being investigated to better understand the problem.

System testing was done using version 1.8.533 of the software. Several of the RDSVerify tests failed because of gaps detected in the frame sets. Because of the use of an active mount point, /archive, lsync is unable to get to a stable point and generate a cache dump file.

LDAS System Administration (Anderson)

Caltech

(Erik Espinoza)

MIT

(Fred Donovan)

Livingston

(Igor Yakushin)

(Dwayne Giardina)

Hanford

(Greg Mendell)

General Computing (Wallace)

MIT

(Fred)

Livingston

(Dwayne)

Hanford

(Christine)

(Shannon)

CIT

(Bruce Sears)

(Veronica)

(Christian)

(Larry)

Advanced LIGO and Supporting R&D (Shoemaker)

Advanced LIGO Systems

Modeling and Simulation

From: Hiroaki Yamamoto hiro@ligo.caltech.edu

e2e weekly meeting

The MC stimulation to study the frequency noise induced by the MC of avdLIGO has been discussed. 

The main topics were : (1) which observable signal is to be used to compare with the requirement set by PF and (2) if the simulation setup includes all necessary physics elements properly, including the laser frequency broadening ~4kHz.

AdvLIGO LSC/ASC design using FP arm model with quad suspension (Osamu)

For lock acquisition of AdLIGO arm cavity, I am investigating the fast speed mirror motion (~0.5um/s) with stronger ESD force (450uN). A special method is necessary to damp the mirror speed without using the error signal because ringing happens for too fast mirror motion and error signal is useless anymore. The "gudelock" algorithm predicts the mirror motion and speed, but the prediction of speed is not so accurate for fast motion. Gain adjustment which is used to estimate the mirror speed can compensate the error of mirror speed, but optimal gain depends on the mirror speed itself. I introduced a speed dependent compensation for the predicted speed since e2e can know the mirror speed directly. Then mirror can be locked from very low speed up to 0.5um/s. Experimentally this compensation equation can be estimated from two transmitted light peaks.

Static IFO simulation (Hiro)

Hello-Vinet formulation of the thermal effect on a mirror has been implemented and validated. Sign of Saint-Venant correction for the surface deformation seems to be incorrect in the original Hello-Vinet paper. Phil calculated the surface deformation by suing FEM and the code in the simulation matches with this result.

The simulation code is being developed to simulate a coupled cavity, which will be used for the comparison of the choice of the recycling cavity, stable or unstable.

Modeler - e2e simulation engine, ALFI : e2e front end (Hiro, Bruce, Melody)

Hiro provided support for Matt and Lisa to use the e2e dual recycled fast simulation module to study the adv.LIGO lock acquisition.

Melody and Bruce worked on the front end of UserDefinedPrimitive module support. This is almost done, and, at Bruce's next visit of Caltech, a release candidate will be built.

Mechanical Simulation for advanced LIGO (Sany and SLU team)

Continued the e2e modeling of AdvLIGO Input Mode Cleaner. Measured length sensing control open loop transfer function. Following Osamu's suggestion, the transfer function was measured in the following way. To keep the Mod Cleaner cavity locked, both the frequency and length sensing control loops were engaged. An excitation (disturbance) signal was injected after the splitting point of the length sensing and frequency sensing controls. The resultant open loop transfer function indicates that the length sensing control has too high gain at the high frequency region, and the crossover frequency is lower than 10 Hz. To fix the problem, redesigning of the length sensing control filter is under planning.  

CDS Prestabilized Laser

From: Peter King <pking@ligo.caltech.edu>

I'm hoping that we can organise a meeting with the Beckhoff Automation programmer here in Hannover.  Then we can go over how to do the communications between EPICS and TwinCAT.

A fan in the air handling system at LZH died, putting work on the laser on hold.  This is a cautionary step to protect the laser rods.

Rolf and Alex have successfully updated the digital controls system here. We are about to try and put the diagnostic breadboard under control.

Control and Data Systems

From: Jay Heefner <jay@ligo.caltech.edu>
AEI PSL Work

AdL SUS

Enhanced LIGO OMC SUS

Tip-Tilt equipment for ANU

AdL PSL

AdL ISI

Seismic Isolation

From: Ken Mason kmason@ligo.mit.edu

BSC Seismic Isolation Assembly and Test

HAM seismic Isolation Design

Suspensions

From: Norna Robertson <nroberts@ligo.caltech.edu>

From: k mailand kmailand@ligo.caltech.edu

Core Optic

From: Helena Armandula ahelena@ligo.caltech.edu

Advanced LIGO Coatings

LASTI   - LMA report

Auxiliary Optics

From: Michael Smith smith@ligo.caltech.edu

SLC
Arm Cavity Baffle

I modeled the BRDF and reflectivity of black glass analytically, and used that information to determine more accurately the scattering requirements for the arm cavity baffle. A reflectivity <0.001 is required, and a BRDF <0.01. These are both met with black glass. Furthermore, I analyzed the scattering and reflectivity properties of a truncated "conical" (an octagonal representation of a cone) beam baffle/trap for the arm cavity baffle. Such a design has BRDF <0.01 and R < 1E-5.

Elliptical Cavity Baffle

There is also a potential scattering problem associated with the elliptical baffle. Approximately 3 W is incident on the periphery of the elliptical baffle from the ITM direction. This light will scatter from the baffle directly back toward the ETM and subsequently re-scatter and enter the IFO mode. Also, some of this light will reflect from the baffle, hit the vacuum wall, scatter back toward the baffle, reflect from the baffle, and follow a return path which will get it down to the ETM where it can scatter into the mode. This scattering imposes a similar requirement on the elliptical baffle reflectivity and BRDF as does the Arm Cavity Baffle.

I made a conceptual model of a truncated "conical" elliptical baffle/trap using SW.

INTERNAL REVIEW

In the process of cleaning up some last minute AOS cost details.

Input Optics

From: David tanner@phys.ufl.edu

Guido Mueller:

Luke Williams:

Wan Wu:

Rodica Martin:

Antonio Lucianetti:

David Tanner:


For additional information about this report, contact Albert Lazzarini or Phil Lindquist

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For additional information about this report, contact Albert Lazzarini or Phil Lindquist

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Rodica Martin:

Antonio Lucianetti:

David Tanner:


For additional information about this report, contact Albert Lazzarini or Phil Lindquist


For additional information about this report, contact Albert Lazzarini or Phil Lindquist