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The LIGO Executive Committee Agenda for Monday September 16, 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)
Field Change Orders/Contingency Liens/Change Requests5. WBS 2 LIGO Lab Operations
Administration (Lindquist)6.WBS 3 and 4 Advanced R&D and LIGO II (Sanders)
Sites (Raab, Coles, Shoemaker, Sanders)
Detector (Whitcomb, Coyne)
Campus Research Facilities (Weinstein (40 Meter), Libbrecht (TNI), Zucker(LASTI))
Data Analysis and Computing (Lazzarini)
Special Items:
No report.
There was a site teleconference held on Thursday, September 12, 2002. The following issues were among those discussed:
Budgets and Costs--The reports for the end of August have been posted on the Web. The projection for carry-forward into FY 2003 remains at approximately $3 million. This is the carry-forward for cash flow purposes. All of these funds have been budgeted for necessary items that remain to be purchased in the FY 2002 plan.
All reserve has been allocated to "planning packages" in the FY 2003 budget. These will be reported separately in the monthly reports that Florence prepares.
Equipment--Caltech Finance wants to modify the ORACLE systems to enable them to capture equipment data directly from their files instead of using E. Chargois' database. To do this, they will be modifying the description fields just a bit starting in FY 2003. E. Chargois has been given an action (#115) to prepare an EMAIL explaining the changes to the people affected (mostly Project Services people and the users of P-Cards).
Livingston Staging Building--A more definitive report was expected last week concerning causes and proposed corrective action for the HVAC problems. A draft has been received but was disappointing in content. It did not provide a substantive analysis of the causes of the problem and proposed action.
Hanford Laboratory Building--Construction is nearly complete. The flooring has not been installed in the lab areas because the underlying concrete has not fully cured. There are some additional punch list items. The fire Department must test the fire detection and suppression systems, but this cannot be done until after the O&M manuals have been received from the sub-, sub-, sub-vendors. Still expect to begin moving people in soon.
All Terrain Vehicle for Livingston--Procurement is in progress to be provided by a company in Baton Rouge. Delivery is expected two weeks after receipt of order.
Property--Ed Chargois has dicussed the available furniture with both Hanford and Livingston. Furniture should be at Hanford by October 1 including a conference table. Will be working on furniture for Livingston after Hanford shipment.
Use of Auditoriums by General Public--Ed Jasnow still has an action (#114) to prepare an email for NSF concerning the use of the auditorium by outside organizations and the notification of the DOE concerning the same.
The list of current actions revised to reflect
the status of open actions assigned through September 12, 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 09/12/02 | Packages | Faxes |
| In | 40 | 27 |
| Out | 13 | 40 |
From: Esther Cunningham <esther@ligo.caltech.edu>
Press here for ACCOUNTS PAYABLE HISTORY DATA .
From: "Brambila, Ruth" <Ruth.Brambila@caltech.edu>
From: irena@ligo.caltech.edu (Irena Petrac)
CONSTRUCTION:
SUPPORT (Baldon, Torres, Lloyd, Tischler)
>Irene Baldon
Weekly Advanced LIGO Project Controls meeting was not held this week.
Advanced LIGO MRE Proposal (Highest Priority)
Project Web Site for posting schedule and progress related data continues to be updated with the latest and greatest.
I feel that I am very close to a final version of the Annual Report and Request for FY 2003 Funding for LIGO Operations. This version addresses suggestions provided by Gary and includes sections on Hanford Outreach, Actual Costs, Proposed Staffing, LIGO Organization, and Planned Meetings. In addition, all "contingency" has been allocated to specific items or tasks in Planning Packages. I will distribute a .pdf version for final review and propose to begin entry into FastLane tomorrow.
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-020009 | OPs | Digital Common Mode Servo to Mode Cleaner Path | D. Coyne |
| CR-020011 | OPs | High Power Test in Suspended Interferometer (Gingin) | D. Coyne |
| CR-020012 | OPs | Additional Funds to Complete 40-Meter Facility Upgrade | A. Weinstein |
| CR-020013 | WBS 1.2 | Pentec VME Digital Signal Processing Boards | Withdrawn |
| CR-020014 | OPS, 5.14 | High Power Laser for Advanced Input Optics System | D. Coyne |
From: Cindy Akutagawa <cindy@ligo.caltech.edu>
No report this week.
No report this week.
Detector Installation: Following the conclusion of S1 running and post-run injections, the interferometer was shut down for installation work on Tuesday morning. At present, the SOS and LOS racks in the LVEA have been completely replaced, and LOS DSC replacement at the Y-end is in progress. The work is progresssing very rapidly owing to the fine job Rus, Mike Fyfee, Ken Watts, and Gary Traylor did modifying boards, building new racks and crossovers, and making new cables in advance so that everything would be ready. (Rus, Mike, Ken, Gary, Peter King, Jay, Ash) We are preparing a detailed plan for commissioning activities following behind the DSC installation work.
HEPI / MEPI / LASTI:
(Hammond): The machined springs were received by MIT and installed. I have completed the gross characterization of the springs and the spring constant was within 4.5% of the FEA model and the each spring was within +/- 1.3% of the mean spring constant. At my request, Rusyl Wooley took a look at the data acquisition system of the spring tester in hopes to get a better resolution on the force readout. In conversation with Ken Watts, they suggested that we install a field isolator to convert the signal level to a more appropriate range. This will be investigated further in the not to distant future. Harry Overmeir has been installing mechanical hardware for the GS-13 pods which include the mounting feet and the locking mechanism. Those efforts are going reasonably well and should have the units ready to be shipped to Stanford to be fit into the ETF Prototype within 2-3 weeks. I have started installing the plumbing into the digital HEPI models to be installed at LASTI so that we may determine which plumbing routes would be the most efficient.
(Kern): At Stanford this week working on calibration and characterization methods for the Parker differential proportional servo valves used for controlling the hydraulic actuators. Working together has led us to a cleared understanding of what is required of the calibration process, and we've reducing the number of steps and simplified the existing procedure. Rich Duder, an application engineer with Parker visited the Stanford lab this morning to help us prepare a spec which we might ask Parker to perform. Gathering up 'busted' valves and returning them to Parker for overhaul. Checking fits on the Pods in the ETF. Prepared 2 additional purchase requisitions for MIT/LASTI and sent the machine shop's first invoice for completed parts onto MIT for payment. Met with Brian and Corwin to go over assembly issues of the welded actuator. Word from the machine shop is that all parts (excepting tripod) ought to be completed this week. Issued PR for additional load cells for the LASTI BSC, as well as 4 more BSC machined springs from Digital Machine.
Optics/Laser Safety (Kern): Gerry, Katrina and I have evolved a procedure to make sure visitors and staff can receive a new or replacement laser safety card as long as one of the three of us is in Livingston.
CDS (Chethan): Ash and I are working on getting the Pentiums and the aux processor for the Digital Suspension control in the LVEA going. Sorted out problems with some license issues on sun workshop software. Tried to increase the memory on the LLOFB2 frame builder to 3GB form 1Gb but ran into problems. Contacted Sun for tech support but our warranty has expired on this machine and we might have to get a time and materials service contract. Trying to fix the problem in-house if possible. Investigating the discrepancy identified by LDAS identified in one of the data files written by LLOfb2 on LDAS T3 disks.
GC (Shannon):
Other: Two bids were received for construction of the office and lab partitions in the new building. Tree harvesting continues very close to the LVEA and to the Y end station.
Pump station system tests are finished. A motor speed control circuit is being tested and should be complete by week of 9-23. The pump station and the manifold will then ship to MIT for installation at LASTI. The pump station has yet to be redesigned to a final ‘tight’ package. Assembly and test of the hydraulic actuator appears to be on track for a late Oct deliver to LASTI for installation.
Electro-Magnetic External Pre-Isolator (MEPI)
The new machined springs have been installed on the HAM MEPI prototype.
The fit and alignment was excellent; much better than the coil springs.
A problem with 220V AC power wiring to the MEPI rack was discovered but
only after some damage to the coil driver and sensor conditioning boards.
Electronics troubleshooting after this electrical problem continues. We
hope to recover and begin system identification and attempts as SISO control
next week. Prof. Samir Nayfeh from the MIT ME department and two of his
students will perform a modal survey of the HAM support structure and assist
in the dSpace based system identification next week.
CDS Hardware
A "PAPR" (Power Air Purifying Respirator--a breathing mask with battery-powered blower) system was ordered and received; this will be modified and combined with a fabricated belt-mounted silica gel cannister as the first step in attempting to reduce the moisture added to the chambers (from exhalation) when entry is required. Other steps include a means to reduce perspiration moisture and to reduce the moisture added by migrating room air. A vest with "phase change" cooling inserts was ordered and received; these inserts deliver a constant 58F sink for up to 3 hours. Our current plan is to be ready with simple equipment for the next required entry to see what improvement can be achieved in a shorter pumpdown time.
PSL
A new 60 degree beam combiner/splitter arrived. On inspection it appeared to work as advertised. The split beams haven't been checked out for beam distortion though.
Sideband Imager
(Keisuke Go, Nergis M, Dave O, Blair)
Two problems have been identified as limiting its performance. One is
the stability of the relative stability of the two lasers. This will be
solved by phase locking the lasers together. The other problem is the galvo
scan out system. This will be solved with impproved labview code.
OTF Lab:
Contamination Cavity # 1--Cavity still locked and continue taking ringdown
measurements. Liyuan is still working on the lab view program for
the new OTF Lab
New Lab at RSE:
Cavity #3 Reference Cavity still pumping down. Optical train ready.
Taking RGA measurements.
Cavity #2 Test cavity--This cavity still pumping, optical train installation in progress. Taking RGA measurements.
I have requested from Rick Savage ( LHO ) the previous lab view card NI AT- MIO-16XE-10 that we had at PSL. Rick has responded and he will send the whole lab view set up including a PC as soon as he receives approval from Fred Raab.
Laser warning signal, Walls, and Curtain are all installed and completed. (It needs Garilynn's approval, as the LIGO/CIT laser safety officer). I am gathering all the hardware needed for the lab.
Misc... tasks, placed some orders for the PSL Lab. Optical items sent to LLO for the new PMC.
Optical sensing (Smith):
1. We rotated our pre-beamsplitter Faraday Isolator and moved the half-wave plate to produce p-polarized light going into the beamsplitter. Before, the light had been polarized at 45°, which resulted in a loss of power going into the cavities.
2. We equalized light power between NAC and SAC by replacing our unpolarized beamsplitter with one designed for p-polarization.
3. We verified that 1 and 2, along with changes to the NAC photodetector, resolved the discrepancy between the NAC and SAC error signals.
4. We built new, low-noise electronics for rapid lock acquisition, along with lower-noise summing junctions than SR560's can provide. Successfully tested these in both SAC and NAC. We can lock during the day now, with ~10 seconds acquisition time under favorable conditions.
5. We measured Q's of modes of arm cavity mirrors. They were all over the map.
6. We measured individual noise sources, including shot noise, electronic noise, laser amplitude noise, and detector current noise (dark current). We failed to measure OSEM controller noise because, at our measurement port, the corresponding voltage we looked at was less than 4nV/ˆHz.
7. We tested the transfer function of a broadband Pockels cell for secondary calibration. Found (too late) that responses are not even expected to conform to factory spec! If we want the Pockels cell calibration path to work, we will have to calibrate the Pockels cell itself before we install it in the TNI.
8. We recalibrated the mirror transfer function M, based on the PZT response in the NPRO. Our original (rough) estimate was 1.0µm/V at dc. Our new, more accurate value came out to be 0.63µm/V at dc. This lowers all of our previous noise estimates by 40%.
9. We inserted collimating lenses on the output beams of both NAC and SAC inside the chamber to tighten up the beams.
10. Upon reassembling the instrument and taking a noise curve, we found that the noise had come up by two orders of magnitude compared with our best previous spectrum. One order of magnitude was due to electronic crosstalk between two of our custom servo boxes, and that was easily eliminated. That leaves us one order of magnitude above our old noise floor. We are currently investigating what this excess noise might be.
11. We got started looking for non-Gaussian events. We set up a system to take data continuously and analyze it on the fly. So far, we have taken only one, fifteen-minute data stream and found no non-Gaussian events.
12. We found a good deal of beam cross-talk in the photo-thermal experiment
was coming from mirror birefringence. We greatly reduced this problem
with better polarization management, and now this experiment is working
well. Photo-thermal data taken with an aluminum mirror agrees well
with
theory.
VACUUM SYSTEM (Zucker, Macinnis):
At 1 atm all week.
PSL (Jamie R, Kirk M, Mike Z and Dave O):
We have settled on the design of a photo detector capable of observing shot noise at high power and very low frequencies. Initial noise characterization by a quick breadboard mock-up suggests that the noise is where we expect.
A visiting student from ANU (Kirk McKenzie) has agreed to complete the characterization and optimization of the new high bandwidth servo. This will serve as a tutorial introduction to the LIGO frequency stabilization/mode cleaner/common mode control technology, which he will explore further when the test cavity is back under vacuum.
HEPI / MEPI / LASTI (Kern, Hammond):
At Stanford this week working on calibration and characterization methods
for the Parker differential proportional servo valves used for controlling
the hydraulic actuators. Working together has led us to a cleared
understanding of what is required of the calibration process, and we've
reducing the number of steps and simplified the existing procedure.
Rich Duder, an application engineer with Parker visited the Stanford lab
this morning to help us prepare a spec which we might ask Parker to perform.
Gathering up 'busted' valves and returning them to Parker for overhaul.
Checking fits on the Pods in the ETF. Prepared 2 additional purchase
requisitions for
MIT/LASTI and sent the machine shop's first invoice for completed parts
onto MIT for payment. Met with Brian and Corwin to go over assembly issues
of the welded actuator. Word from the machine shop is that all parts
(excepting tripod) ought to be completed this week. Issued PR for
additional load cells for the LASTI BSC, as well as 4 more BSC machined
springs from Digital Machine.
MEPI INSTALLATION (Mason, MacInnis, Coyne):
The mechanical installation of the electromagnetic pre-isolator has been completed.
#MZ LOOKING GOOD, GUYS! READY FOR A TEST DRIVE.
The bent coil springs were replaced with the newer machined springs made of maraging steel. Installation was much easier as the new machined springs were straight and fit in with no side loading on the stack. The electromagnetic actuator coils and position sensors were centered. There still remains an axial and lateral displacement in the stack which was caused by attempting to accommodate the old springs. Our feeling is that it will not affect our tests so we are proceeding with powering up the system. We will return later and set the stack in its original position using the coarse actuation system.
MEPI MODELING & DYNAMICAL TESTING (Mittleman, Coyne, Ottaway):
Dave has finished converting the hytec stack model to a stack-plus-support table model, which has now been incorporated into the Simulink model.
The electronics to drive the MEPI are all in place and currently undergoing a debugging process. We hope to be able to start comparing the plant and model by the end of the week.
Simulation and Modeling (Bhawal)
Physics meeting
Matt reported his progress in developing the new E2E field model. We discussed about thick-mirror code, change in beam-basis, proper implementation of guoy phase etc.
Outreach collaboration
Hiro helped Sany Yoshida to prepare the NSF proposal for his research at SLU, including his students. Some preparatory work was done at LLO during the summer season by Sany and his student Raghu.
Code development and maintenance
(Hiro) The simulation code is reorganized because no C++ code is needed to be shared with Alfi. Also changes and modifications are made to make it work under gcc 3.1.
(Biplab) A few modifications were done in triangular summation cavity code to conform it with last week's change in parts related to misalignment matrix calculations. Tested results by comparing with primitive version, found another bug. A few more tests are needed before I commit.
(Matt) Continued development of new E2E field model.
Alfi
(Melody)
Software Systems (Blackburn)
The final summary for the use of LDAS during the Science Run for LHO,
LLO and MIT is in:
Interval: 08/23/02 12:00:00 PDT - 09/10/02 12:00:00 PDT
|
User Command
|
|
|
||||
|
Submitted
|
Failed
|
Percent
|
Submitted
|
Failed
|
Percent
|
|
|
createRDS
|
18538
|
187
|
1.0
|
18413
|
42
|
0.2
|
|
dataPipeline
|
28744
|
1866
|
6.5
|
8095
|
1044
|
13
|
|
inspiral
|
13076
|
873
|
6.4
|
2464
|
482
|
19
|
|
power
|
5417
|
106
|
2.0
|
2003
|
7
|
0.4
|
|
slope
|
4829
|
387
|
8.0
|
1885
|
354
|
19
|
|
tfcluster
|
4787
|
495
|
10
|
1739
|
197
|
11
|
|
getMetaData
|
18115
|
26
|
0.1
|
8653
|
111
|
1.3
|
|
putMetaData
|
33646
|
12
|
0.1
|
12497
|
15
|
0.1
|
|
All Jobs
|
99094
|
2098
|
2.1
|
47576
|
1215
|
2.6
|
|
User Command
|
|
||
|
Submitted
|
Failed
|
Percent
|
|
|
createRDS
|
58974
|
64
|
0.1
|
|
dataPipeline
|
2031
|
634
|
31
|
|
inspiral
|
0
|
0
|
-
|
|
power
|
167
|
15
|
9.0
|
|
slope
|
215
|
22
|
10
|
|
tfcluster
|
560
|
27
|
4.8
|
|
getMetaData
|
94
|
0
|
0
|
|
putMetaData
|
0
|
0
|
-
|
|
All Jobs
|
61171
|
699
|
1.1
|
Looking at the details for the failures reveals that the dominant
cause of job failure was missing frames, accounting for roughly 50% of
the failed jobs. Segmentation faults in the LALwrapper DSOs accounted for
about 45 % of the job failures and too many triggers being sent to
the database, the power outage accounting for most of the remaining 5%.
The
number of jobs that failed do to internal errors in LDAS software was very
small (order a few).
Work continued this week on the new frameCPP I/O library to read and write version 6 frames. An empty test frame with a "Table of Contents" was shared with VIRGO to validate against the version 6 frameLIB I/O library developed in C. Several new standalone utilities are also being developed for dumping the dictionary, data, and table of contents. A version {3,4,5} to version 6 converter application is also in development.
A new series of test scripts was developed for trying out the new dataStandalone and putStandAlone user commands against each of the DSO search codes. This is still being polished up but in working. The controlMonitorAPI has a new least squares fit routine and now plots a histogram of the number of jobs vs number of nodes allocated. Log plots are planned for the next release as is support for LDAS account based access to monitoring functions.
A bug was found in the asynchronous communications between the wrapperAPI's master process and the mpiAPI. This has now been fixed. Will also be implementing a new data domain type of "NONE" to compliment the existing time, frequency and time-frequency domains. This has been discussed in the LSUG meeting and has majority approval of the software change board. An issue in the diskCacheAPI came up at the sites after the Science Run from August frames co-existing with science run frames the minor bug in the diskCacheAPI has been fixed and the August frames moved. Some progress has been made on getting LDAS to run on Solaris 9 platforms on a test system. So far simple inspiral jobs work as do database jobs. Similar progress is being made towards running LDAS on Linux 7.3 platforms. No effort has yet gone into porting LDAS to GCC 3.1.x though.
Hardware Systems (Anderson)
(Dan Kozak)
Received over 30 tapes with S1 RDS data. Injection of data onto PC RAID on LDAS is currently paused due to hardware errors of the unit. Laura has been working on fall back scenarios to bring S1 playground data at MIT on Frame v4 format. Some of that data are at MIT. Tania is setting up running the stochastic DSO on the S1. She reports a misbehaving of the DSO when a specific DB partition is used. Stefan is catching up on S1 data analysis issue now that he's back from Europe. Burst Analysis Meeting (=BAM) #1 starts next Friday at MIT and will go over the weekend.
General Computing (Wallace)
MIT:
(Keith)
Core Optics
(From: GariLynn Billingsley <Billingsley_G@ligo.caltech.edu>)
Crystal systems has had one more successful boule growth making the ratio 2/5, they are now proceeding to work on 20" boules for another customer, though of course the technology is applicable to our efforts as well. They have been doing some developmental work with core drilling of large pieces and are now ready to proceed with processing our order. This pushes the estimated delivery out to mid-November. However, Insaco is known to be conservative in their processing estimates, so there is still some room for optimism.
Insaco has completed (ahead of their estimate) the edge polish of the ITM for Gin Gin, I am waiting on a quote from Wave precision for full polish. I still need to know if there are special requirements for the back side of the Gin Gin ETM. I have gone ahead and assumed there are not, and am asking for l/10 polish.
We have had some exploratory conversations about using "flat topped beams" for Advanced LIGO. I am generating possible errors for these surfaces; Kip's group will use these to explore the tolerance of the system to errors on the mirrors. You can see the ideal profile at http://www.ligo.caltech.edu/~gari/LIGOIII/FlatTopProfile.JPG The vertical scale is waves, horizontal scale is millimeters.
CSIRO believes they could easily produce the surfaces to within 50 nm, they have a ~50% confidence that they could produce the surfaces to within 10nm using ion beam etching.
Another avenue to explore is the use of corrective coating, or creative masking during the coating process. in LIGO1 we found that the coatings were uniform to within ~0.5% Peak to Valley or about 50nm for a high reflector. This bump was at a radius of 100mm and was caused by masking errors. The coating mask is commonly modeled then tweaked for best performance. One could imagine using a mask that allowed much more material (~5% in the Flat top case) to be deposited at the edge, or perhaps using some combination of a polished sphere and a coating which is thicker in the center.
Once we have a tolerance established we will be speaking to our coating and polishing vendors about the possibility of demonstrating this technology.
Coating Thermal Noise Experiment (Gregg Harry):
(From: Michael Zucker <zucker_m@ligo.mit.edu>)
We received the sample from Wave Precision coated with tantala/alumina. However, they forgot to put the mask on while coating so we didn't have a region to weld to free of coating. We tried hanging it anyway and the coating near the weld was visibly changed along the edge. We don't have any Q's from it yet.
We do have some data on the silica/tantala sample coated at MLD and annealed to 450 C. However, its coating near the weld was also visibly affected, similar to the WP tantala/alumina.
| phi_bf-x | 1.7 x 10-4 |
| phi_2bf-1 | 1.8 x 10-4 |
| phi_2bf-2 | 1.9 x 10-4 |
This is very similar to what we were seeing on the SMA samples. I am waiting for confirmation of these numbers from the other samples. It is conceivable that the small damage on the coating isn't enough to effect the loss and we might be able to get usable data on the WP samples.
We will hang the niobia/silica sample from MLD next.
Adv LIGO Core Optics:
(Erika D’Ambrosio)
I am back on mathematical computations for the flat topped beam that has been proposed as a choice for reducing thermoelastic noise. I am going through some optimization for the driving beam considering the constraints we have settled.
Adv LIGO Mode Cleaner Suspension Prototype
Advanced LIGO Suspensions
(From: Janeen Romie <romie_j@ligo.caltech.edu>)
Yesterday, Calum and Mike Plissi assembled the mode cleaner controls prototype triple pendulum. It was an exciting milestone. Click on the link - Triple Pendulum Pictures for photos and links to the Solidworks model. Use password "geo600" to see the Solidworks web page with Internet Explorer. Calum and Mike started with an assembled top mass and walked us through the use of the wire jigs and the balancing process. Mark Barton, Helena, Betsy Bland, Mike Smith and I were watching and assisting.
Blade characterization is continuing. The small and large MC blades have had their thicknesses measured down their lengths. This data will be logged into an Excel spreadsheet for blade analysis. This analysis will aid in modeling future blade designs. Half of the small blades have had their deflections measured and noted. We measure the deflection of the blades unloaded and under two different loads. The other half will be measured tomorrow. All of the large blades have had their deflections measured.
The hybrid osem coils are in the oven for their hot bake. Bob Taylor is soldering the boards and will begin assembly tomorrow or Friday. He's still assembling the LIGO I osems for global control. Helena has assembled the large magnet flag assemblies for the local control hybrid osems. The LIGO I magnet assemblies are also complete.
David Robertson from GEO reported Tuesday that the GEO portion of the osem electronics shall not be delivered until after the first week of October. At this point, that is certainly our long pole. We can perform form and fit with the osems but that's all. Mark Barton has taken the Norna/Simulink suspension model and has been modeling the sensor/actuator system in dSPACE as a prelude to developing the controller. He modularized it so that the simulated plant is separated from the controller. The aim of this is to replace the simulated portion with real sensor data from the dSPACE system when ready. He will post his model at Mark's Model Page this afternoon.
Tomorrow, I'll get together with Larry Jones and Mike Zucker and get in an order for the in-vacuum cabling. We'll also check on baked feedthrough connector spares that may be available for borrowing from Livingston, with the assumption that replacements will be ordered and processed.
Calum and I are working on quick drawing changes so parts may be reworked and optimized. We're still waiting for the structure stiffeners and the magnet fixture for the LIGO I osems. The second structure is due to be finished on Monday the 16th. The second set of metal test masses are due any day. I still need to design a few small installation fixtures.
Dennis had reported that a positive schedule forecast would allow use to use the LASTI vacuum chamber around the first of the year. The chamber is now being used for seismic retrofit testing and cannot be used simultaneously because the optical table needs to be changed.
Advanced LIGO Suspensions:
(From: ctorrie <ctorrie@ligo.caltech.edu> )
Mike Plissi, Janeen Romie and I assembled a triple pendulum assisted by Helena and Phil Willems on Friday of last week. On Tuesday we repeated the process of assembly with Mark, Betsy, Helena, Mike, Janeen and I present. Some pictures can be seen at the following link, hopefully more of better quality will appear when the student photographer starts next week. http://www.ligo.caltech.edu/~ctorrie/ligotriple.html
SolidWorks
Also available at the above link is an animated assembly of the triple
pendulum and structure. The password is "geo600."
Blades
With the help of Mike Plissi and Janeen we have been spending a lot
of time characterising the blades. This information will be used to fine
tune the choice of parameters for future designs.
Electronics:
(Jay Heefner)
GEO will send us schematics of their modules by 9/13. Once we have them we can complete the system and whitening/dewhitening designs. We are shooting to have electronics available by the first of October. This should be possible if other priorities, like the DSC upgrade do not interfere.
40m Suspensions:
(From: Janeen Romie <romie_j@ligo.caltech.edu>)
Betsy and Helena have started the work on the BS optic. They have also
started work on one of the test mass suspensions. Steve Vass has been observing.
Prestabilized Laser (PSL):
(From: Peter King <pking@ligo.caltech.edu>)
After a boot up test of the VME modules last week, a 3123 and a 4116 failed. These were replaced and successfully passed the boot stage. For some reason I don't understand why the Motorola IOC timed out whilst attempting to load the vxWorks kernel. Booting up the VME crate with the Motorola and testing of the 21.5 MHz photodetector are the only two remaining tasks to be performed before shipping the items to Hannover.
Software:
(From: "Mark Barton" <mbarton@ligo.caltech.edu> )
I finished a big chunk of the Simulink/dSpace programming for the mode cleaner prototype test. The Simulink model of the pendulum and controls used to design the system was fairly high-level and didn't attempt to model the sensors and actuators in any detail, so I fleshed it out considerably, adding blocks representing the sensors and actuators, the geometry of their deployment and their driver electronics. I also modularized it so that it will be easy to swap out the simulated plant and replace it with inputs and outputs to the physical pendulum when the electronics arrives. A lot of the more detailed simulation will be made redundant at that time but it will be useful in the interim because we want to try designing a simpler, pure-SISO controller. The existing controller design assumes that the six sensor inputs have been magically diagonalized to measures of x/y/z/yaw/pitch/roll, and contrariwise for the outputs
Advanced LIGO Coatings
(From: Helena Armandula <ahelena@ligo.caltech.edu>)
Low Frequency Seismic Isolation:
(From: Hareem Tariq <htariq@ligo.caltech.edu>)
Stefano:
For additional information about this report, contact sanders@ligo.caltech.edu