The dome and east door of the BSC 3 chamber was removed and walking plates were placed on the work platform. These have not been installed because we have not located the C channel pieces that bolt to the walking plates so the C 3 cover can be secured to the walking plates. We also installed the permanent flooring in BSC 3 chamber. We installed the soft roof that was on the BSC 3 clean room onto the clean room over the cryo pump spool. The SEI soft roof "sock" is on the clean room over BSC 3.
HughR, HugoP,
Here is the current status of the aLIGO SEI work at Hanford. Everything in red is a change from last status. Everything in green is available.
· BSC1 - ITMY
o ISI + HEPI - Unlocked, Previously commissioned. Performance Spectra
· BSC2 - BS
o ISI + HEPI - Unlocked, Previously commissioned. Performance Spectra
· BSC3 - ITMX
o ISI : Chamber-Side testing complete. Report validated. Ready for cartridge install.
o HEPI : Locked. Model is running. Electronics ready for turn on.
· BSC9 - ETMX
o ISI : Locked. Chamber-Side testing complete. Report Validated. Cartridge installed.
Needs balancing
o HEPI : Unlocked, ongoing initial alignment.
· BSC10 - ETMY
o ISI : Currently installed in BSC6. Will be pulled out and installed in BSC10. Payload (SUS) will be moved then. Electronics are disconnected
o HEPI : Unlocked.
HAM 1
o HEPI: Locked (09/18/13) and vented.
Low priority testing
One L4C needs to be replaced: H2
One actuator is weak: V4 It is 20% weaker than its counterparts. Likely clogged. May require replacement further down the line.
· HAM2
o ISI: previously commissioned with HEPI locked (recent performance spectra - not calibrated in higher frequencies), currently unlocked, in vacuum
o HEPI - IPS position loops and alignment offsets installed - recent performance spectra
Unlocked 07/23
· HAM 3
o ISI: previously commissioned with HEPI locked (recent performance spectra - Calibrated), currently unlocked, in vacuum
Sensor correction installaton started.
New blend filters installed. aLigo Blend filters on all DOF but RX and RY. eLigo high roll off blend filters on RX and RY. Performance Spectra.
o HEPI - IPS position loops and alignment offsets installed - recent performance spectra
Unlocked 07/23
· HAM 4
o ISI: In chamber, Previously tested during assembly validation, currently locked, no suspension installed, in-vac cables not connected.
Electronics ready, in field cables ready, in-rack cables ready. Temporary STS cables
Model is running, and MEDM screens are available in the Sitemap.
o HEPI: Currently locked, to be commissioned
Electronics ready, in field cables ready, in-rack cables ready. Temporary STS cables
Model is running, and MEDM screens are available in the Sitemap.
· HAM 5
o ISI: In Chamber, Previously tested during assembly validation, currently locked, no suspension installed, in-vac cables not connected,
Chamber temporarily closed.
Electronics ready, in field cables ready, in-rack cables ready. Temporary STS cables
Model is running, and MEDM screens are available in the Sitemap.
o HEPI: Currently locked, to be commissioned
Electronics ready, in field cables ready, in-rack cables ready. Temporary STS cables
Model is running, and MEDM screens are available in the Sitemap.
· HAM 6
o ISI:
in chamber.
Unlocked, no SUS
Mechanical adjustments complete
Initial in-chamber testing complete, but not validated yet
o HEPI: Unlocked - Ongoing commissioning
· Guardian:
Transition scripts ready
Transition scripts work under guardian interpreter
alarm.txt files ready
snap files ready
WP#4183
To test the data content of the science frame (requested by Hugo) I have reconfigured h1nds0 to read only the science frames for the duration of this test. h1nds1 (which is the default NDS) is unchanged and continues to serve the full commissioning frames. When this test is completed I will revert h1nds0 back to commissioning frames.
(Sheila, Alexa)
532nm power:
@ laser = 52mW
@ M11 = 32.5mW
We inserted a dichroic mirror after M11 in the green path and found the transmitted 532nm light to be 32.1mW and the reflected 1064nm light to be .54mW
I've created a large OSEM overview medm screen, accessible from the sitemap under the CDS tag. It shows all the OSEMS which are currently in the DAQ system.
It can only be displayed on a high resolution iMAC screen (e.g. control room workstations).
(Sheila, Alexa)
See D1201448 for reference.
We inserted ALS-L1 (ROC=75mm), which we had temporarily removed. Then, with the Mode Master (silicon detector), we spent the day mode matching the telescope along the green path (ALS-L6 and ALS-L7), which were placed for the OAT configuration and not the nominal configuration.
First, we examined the beam profile with the table in the OAT configuration and the mode master 28.5inches from ALS-M11. Image 'OneArmTextEndX' portrays the result. We subsequently removed ALS-L6 (ROC=-100mm) from the path and took another beam profile with the mode master in the same position. Image 'OneArmNoLens' portrays the resullt. We used this data to determine the seed waist of the beam. This seed waist matched that of the optical layout. We proceeded to create an "a la mode" matlab script to determine the proper positions of L6 and L7 with the target waist size of 2.2mm at 184.6inch from M11. Note: the target wasit size was determined via T1200200; the location was determined by measuring the distance from the TransMon secondary mirror to the chamber viewport (TransMon layout (D0902163, D1201457) and assuming the TransMon chamber was 2ft from the ALS table. We determined that L7 was 7inch from M10 and that L6 was 37inch from L7. This gave us a 99% overlap.
In this nominal configuration, we placed the mode master 660mm from M11 (we wanted to better stablize the MM). We noticed that the MM kept giving different results. Images 'ISCEXMM660mm2M11...' are snaptshots of four runs of the beam profile with everything in the exact same position. We were a bit unsure why the MM kept giving such different results. The waist size seemed close enough to 2.2mm; however, the location was drasitically off. We concluded for the day in this puzzled state...(more work tomorrow)
I have also attached the matlab script.
We realized that the MM has a diveregence minimum of .25mr, meanwhlie our beam has a divergence of around .18mr. This could explain the bad M^2 and the strange waist projections. However, using the waist measured at the MM lens (x_waist ~ 4.5mm, y_waist ~ 5.4mm), and the target waist of 2.2mm at 184.6 inches, the overlap for x was 99% and for y was 95.5%. I have attached the updated MatLab script.
(Note: the Rayleigh range is 28m)
We have concluded ISCTEX ready to be moved to EX.
The dust monitor software has been moved to met_one_227b_comp_ctrl-1.0.0 for device support and dust_met_one_227b_comp_ctrl-1.0.0 for the IOCs. The targets in /ligo/lho/h0/target were backed up to /ligo/lho/h0/target_archive and updated. The sitemap has been updated to link to modified medm screens. The primary change is that the software now controls the timing and puts the dust monitor into 'standby mode' between samples. The sample time and hold time durations can be set from EPICS. I also added code to attempt to reconnect on TCP/IP disconnects. The IOCs are running in 'screen' on a new virtual machine that Cyrus created, h0epics. I updated the H0EDCU_DUST.ini file to remove the MODE, TEMP and RELHUM channels and add ACTSAMPLETIME, HOLDTIMEMON, SAMPLETIMEMON, STATE and ISENABLED channels. Dave has rebooted the DAQ and these changes are now in place. Each dust monitor location is now enabled/disabled by toggling the on/off switch on the medm screens. I tried to update the alarm configuration file to use the ISENABLED channels to mask the dust monitors that are not running, but could not seem to get this to work. The wiki pages have been updated. This should complete WP 4172.
Jim did the hard work and I did the brain thing. We could only get our level rod to just past half way to the west side from the East door and Jim was really stretching. We found the vertical level runout from the East side to the center portion of the table to be about 0.047" or about 2.4mm over the whole table. May have been good enough (per comm RAbbott) but you're talking about SEI & HCR here. We weren't about to be satisfied. The elevation was about 1/64" low and that is close enough. So to level the table we moved one stack of 20kg 2x2" (diagonally NW to SE) to get our calibration. We then move 10kg 24" ultimately to put us very level. I redlined a pdf and added this to the DCC, D1200524, to show the as-built of the masses. Final position: -200.45mm Gz level to +-0.1mm over the span of the Optical Table per D1200524. Attached is my log book page for this survey. The numbers there are in local elevations. At HAM1 subtract the 14.1mm vertical offset to get to the Gz: -186.35-14.1 = -200.45mm
PeterK and RickS We intended to make weekly PSL performance assessment measurements this morning, but we found that the FSS had not locked since about 4 PM yesterday afternoon. After 6 hours of so of investigating, we found that there was a mouse in the RF distribution rack (one that likes Swiss chocolate!). It seems that the 80 MHz RF distribution is being reconfigured. After restoring the RF drive to the VCO and FSS AOM, the FSS locked right up, the ISS locked, and the system appears on cursory inspection to be operating as expected.
Both HAM2 and HAM3 chambers are now fully controlled (HEPI+ISI).
Those chambers feature:
- Standardized ISI damping loops (defined in: SeiSVN/seismic/HAM-ISI/H1/
- Standardized ISI blend filters (SeiSVN/seismic/HAM-ISI/Complementary_Filters_HAM_ISI/HAM-ISI_Generic_Comp_Filters.mat)
- Hybrid aLigo/eLigo blend filters are available (SeiSVN/seismic/HAM-ISI/Common/Blend_filters/Filters_HAM_ISI_Blend_Hybrid_24_Jul_2013.mat)
- All 3 levels of ISI isolation loops (UGF=10Hz, 25Hz, 35Hz - LHO aLog # 5355). Performance is mostly limited by the blend filters. Level 2 controllers give similar amount of isolation as Level 3. Level 2 controllers are prefferred for now - ISI Perfomance can be found in LHO aLog #7414
- HEPI position blend filters (IPS signals are multiplied by 1, L4C signals are multiplied by 0)
- HEPI position loops. UUG = 2 Hz. Should be set to 5Hz soon. HEPI position loops performance plots, and controllers, can be found in LHO aLog #8037.
Trun on Process:
Prepare:
Damp ISI:
Turn on HEPI:
Engage the isolation loops, on the ISI
I took performance spectra on the ISI, in air, earlier this week.
HEPI was running with 2Hz UUG IPS position loops. The ISI had Level 3 isolation loops running, with the hybrid aLigo + eLigo on RX/RY blend.
Performance plots are attached for reference.
Betsy, Travis
This afternoon, we connected the 5 ETMx SUS cables and the ringheater cable to the inside of the feedthru flange. We then had issues with signal faults. We investigated and found the out-of vac cables not plugged in well at the outside of the feedthru. Apon fixing, all looked well with the signals. The suspension is still not fully suspended although we pulled out all of the extra teflon stopping brackets and prepped it for full unlock after SEI is done float/balance, after IAS is done figuring out where to put us.
Note - Yesterday (Oct 16) we discovered that we had incorrectly pugged the cables into the internal side of the feedthru. This was due to the fact that the cable connectors were mounted in the table bracket slightly incorrectly. We remedied this yesterday.
** LVEA has been laser safe throughout the day ** Praxair delivered to CP8 this morning. The CP8 value on the HOVE overview screen remained near 104 through the lunch hour and now sits at 101. ** Roofers have worked all day on the LVEA roof except for a period this afternoon when the storm was active. ** See John's entry about water leaks in the LVEA this afternoon because of the storm. ** Alexa and Sheila have worked in the HAM6 bay through the day. ** Betsy entered the chamber at EX late this morning. The ETMX speedometer needles on SUS_OSEM_OVERVIEW are now active. ** The cartridge is bagged on the LVEA test stand. ** Lots of dust alarms through the day at a number of locations. In most cases the alarms correlated with human activity in the affected areas. We saw alarms this afternoon from the beer garden dust monitor (5) near 30,000 and it wasn't clear from the cameras if there was activity near BSC3 that was the cause. Patrick is checking the area to see if there might be a water leak nearby. ** The EX dust monitor went white this afternoon. Filiberto was in the VEA; he tightened the cable on the rack side and the monitor turned back on. ** Rick has been working on the ref cav this afternoon
Dan saw the same problems on h1ldasgw0 as he saw on h1ldasgw1 a few weeks ago. He upgraded solaris and rebooted to fix the QFS file system. h1fw0 got into a stuck state, unable to unmount or remount the NFS file system, I had to reboot it using the front panel reset button (it got stuck rebooting too). Unfortunately I accidentally restarted the DAQ in the process.
The data gap on h1fw0 is:
Oct 8 13:44
Oct 8 15:17
h1fw1 was running the entire time, except for the DAQ restart.
(Rich, Stefan) We installed jumpers in the coil drivers (D1100117) to permanently enable input on/off switch and the run switch. The affected the following coil driver serial numbers: S1106044 (RM1), S1200612 (RM2), S1106043 (OM1), S1200608 (OM2), S1200614 (OM3) For proper operation H1:ASC-RM2_BIO_M1_STATEREQ needs to be set to 2, and the anti-dewhitening filters need to be in FM6 of the H1:ASC-RM?_M1_COILOUTF_?? filter modules. (FM1 is reserved for the sim-dewhitenig filter.)
Jason, Tyler and I measured the BSC9 chamber longitudinal position from the face of the gate valve (GV19) nearest to the termination slab and compared it to the drawing position call outs. We found the chamber to be 6.01mm further north than the drawing perfect position. We set a new monument on our offset line perpendicular to BTVE-8 and measured longitudinal positions for EX-B1 ,EX-T3, IAM-17. So far first error found is BX-B1 has a positive error 19.5mm +X which caries over to EX-T2 which we are using to shoot the ETMx from When we finish up with the BSC9 chamber centerline we will know more.
Roofing was interrupted this afternoon when a sudden thunderstorm came through. The crew covered what they could before scrambling off the roof. Some water managed to get into the building - primarily along two open edges and a few other locations at screw holes. The worst hit area was the return air plenum at the north west inside corner of the building. The weather has cleared and the roofers should be able to lay membrane material down for the night in case we get more rain.
If you need rain in your garden just start working on your roof! Or wash your car.
(Keita, Stefan) We noticed that the feed-back gains of RM2 were the opposite of RM1. So went through all 6 tip-tilts that we have at LHO, and determined their magnet polarity: As viewed from behind (incl magnetic pole facing backward): Default: UL: N, UR: S LL: S, LR: N The following serial numbers are conform with that: 009 (bad wire), 002, 033, 004, 022 (RM1) Serial number 024 (RM2) is different: UL: S, UR: N LL: N, LR: S For now we flipped the digital coil gains of RM2 to account for that.
Venting completed at ~2:45 pm. The purge valve on the X manifold has been dialed back until a door can be removed.
[Jeff B, Stuart A] After a few power glitches etc, the triple test-stand was in need of some attention prior to hooking-up OMC suspensions for Phase 1b testing. Logging in remotely, I noticed that the incorrect model was running, x1sushxts27 instead of x1sushxts05, so I re-started the *05 model. I then BURT restored the safe snapshot (/opt/rtcds3/tst/x1/userapps/release/sus/x1/burtfiles/20130911_x1sushxts05_OMC.snap) I had already previously taken of the OMC configuration (see LHO aLOG entry 7728 for further details). The triple test-stand should now be ready to accept OMCS for testing.