Displaying reports 66441-66460 of 77195.Go to page Start 3319 3320 3321 3322 3323 3324 3325 3326 3327 End
Reports until 13:51, Saturday 29 March 2014
H1 SEI (SYS)
jameson.rollins@LIGO.ORG - posted 13:51, Saturday 29 March 2014 - last comment - 14:04, Saturday 29 March 2014(11077)
SEI guardian status update: BSC ISI guardians now running for BS, ITMX, ITMY, ETMX

BSC ISI guardians now running for BS, ITMX, ITMY, ETMX

After a lot struggle with the BSC ISIs this week, we finally have all commissioned BSCs under guardian control.

The BSC seismic stack is one of the more complicated systems we've deployed, as it currently consists of three nodes in a "managed" configuration: two separate nodes for each of the two ISI stages (e.g. ISI_ITMY_ST1, and ISI_ITMY_ST2), and a "chamber manager" (SEI_ITMY) that coordinates the activity of the two subordinate ISI stages.  USERAPPS location of the top level modules (and primary loaded library):

All single ISI stages share the exact same code, for each BSC stage as well the single HAM stage.  Here are the system graphs for the SEI manager and ISI stage 1:

The manager (left above) has three main requestable states: READY, DAMPED, ISOLATED.  The READY state puts both of the ISI stages in READY, the DAMPED state puts them both in DAMPED, and the ISOLATED state puts both into isolation levels that can be specified in the manager system description module (USERAPPS/isi/common/guardian/SEI_*.py).  At the moment all systems are using their default configuration, which is to operate the ISI stages in the HIGH_ISOLATED state, which corresponds to "lvl3" from the old "command" scripts.  This can't currently be changed on an individual BSC basis, due to a guardian core issue, but I'm working on it.

The degrees of freedom for which to restore cart bias offsets can also be specified on a per stage basis.  Note the ISI_ITMY_ST1 graph above has "RESTORE_ISO_CART_BIAS_*_RZ" states, and no corresponding states for the other degrees of freedom (X, Y, Z, RX, RY).  This indicates that we are restoring only RZ target cart bias offsets for this stage.

Notes about the BSC isolation procedure

There are a couple of important things to note about the current isolation procedure:

We had a lot of trouble dealing with the T240s in stage 1.  Their exterme sensitivity to pitch causes them to saturate if a large pitch cart bias offset is applied to the stage.  We there spend a lot of time trying to figure out how to gracefully bring them in and out of the loop, by reducing their gain and/or changing the blend filters during the isolation procedure.  All of theses things has problems, though:

This makes things very difficult if we need to hold pitch offsets on any of the ISIs.  It looks like we need to fix the synchronous switching of the T240 compensation filters before we can handle pitch cart bias offsets.

However, after speaking with the integration team, it seems that it's ok to operate temporarily in a mode where we only restore RZ cart biases.  Any needed pitch offsets can be held in the suspensions for now.  Therefore we do not need to change the T240 gains or blend filters during the isolation procedure.  This is good news, since it means we can run with the current guardian behavior.  Obviously this will have to be fixed down the line, as we will likely want to hold pitch offsets on the ETMs, but we have a workable solution for the moment.

Guardian BSC isolation configuration and procedure

With the above configuration we can successfully isolate the BSCs without touching the T240s or blend filters.  It seems to be fairly robust.

Important operator notes:

Notes about guardian SEI manager behavior

The SEI managers represent a new step for guardian, as their primary task is to control the state of other guardian nodes, which we haven't needed up to this point.  Getting their behavior robust has been quite tricky.  It necessitated a lot of work on the guardian built-in "manager" library, as well as a lot of experimentation with the SEI manager module itself.  The manager is designed to be fairly robust against commissioner noodling with it's subordinates, but that is also fairly tricky to get right in a robust and useful way.  Some things will need to be improved, but this is the behavior currently:

While things seem to working well at the moment, I certainly don't claim that all the bugs have excised.  If the manager does get hung in some state, resetting to the INIT state should clear everything, reset the ISIs, and get things back on track.

TODO for SEI guardian

Images attached to this report
Comments related to this report
jameson.rollins@LIGO.ORG - 14:04, Saturday 29 March 2014 (11086)

Note, the following code version number are applicable to the above configuration:

  • guardian: svn r878
  • cdsutils: svn r211
  • USERAPPS/isi/common/guardian: svn r7619
LHO VE
kyle.ryan@LIGO.ORG - posted 10:15, Saturday 29 March 2014 (11085)
Kyle on site for rough pumping of Y-end -> Should be here several hours -> Will make aLOG entry when leaving


			
			
H1 ISC (CDS, SYS)
jeffrey.kissel@LIGO.ORG - posted 19:21, Friday 28 March 2014 - last comment - 11:56, Monday 31 March 2014(11083)
ALS Electro-optical Control Schematic
A. Staley, S. Dwyer, J. Kissel 

After speaking with Sheila and Alexa, trying to understand the spectrum in LHO aLOG 11026, I realized that -- because of so much unexpected excess noise -- the current ALS setup has diverged significantly from the baseline plan. As such, we've worked together to create a diagram that is to-the-best-of-(my)-knowledge accurate, and makes sure to show how every control signal gets around to its actuators, including passes through digital land. The only things I did not include were the demodulator boards between the REFL diodes (ARM REFL, MC REFL, and the two green XARM and YARM REFLs) and lame things like whitening, AA, and AI chassis that facilitate getting in-and-out of digital land.

In particular, I draw your attention to the unorthodox and new features that were not part of the original design plan:
(1) The PRM is misaligned. This way we can use IFO REFL red diode signal (after normalizing / linearizing it with the red arm cavity trans) to measure the arm and offload at low frequency to the CARM board in the second input. This is unorthodox because normally we would feed REFL straight to the CARM board in all analog and retain the large bandwidth, but because the noise is so large, it must be linearized in the front-end (the only place the Arm TRANS signal exists), and fed out one of the corner station LSC DACs. Note that this configuration is just a special technique for these particular series of measurements and is not designed to become a normal part of the lock acquisition scheme.

(2) The Voltage Controlled Oscillator (VCO) actuated, Phase-Locking Loop (PLL) that's wrapped around the corner-station COMM and DIFF Phase-Frequency Discriminators (PFD) are used to reduce the noise enough to keep the PFD in the linear, phase detecting mode (check out pgs 6-8 of the AD9901 datasheet -- it's a really nice explanation of how it works).

(3) Before the hand-off, there's another temporary step which is to use the Beckhoff system ("Slow ADC" in the diagram) to feed directly to the PSL VCO (again at low frequency) to reduce the noise enough for the COMM hand-off to work. 

This is most certainly an impressively complicated system!

Note that this diagram has been committed into the noisebudget repo here:
${NBSVN}/trunk/HIFO/Common/
and I imagine will become an "as built" DCC document in the glorious future when everything is working beautifully.
Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 11:56, Monday 31 March 2014 (11096)
Comments and my replies on the diagram from Bram, to be added/fixed later:

You are missing the Fiber Distribution Box, which shifts the laser frequency by -160 MHz before it gets shipped to the end-stations to compensate for the PSL AOM. The lasers at the end-station are then locked at the + (X-end?) and - (Y-end?) 40 MHz around the ‘0’.
Ah, yes. I had debated putting the distribution box in there, and decided against it for clarity because I forgot the important frequency shift feature.
See D1200136 for details or Figure for in T1000555 for schematical diagram.

Also, the F and S in the ‘servo’ block diagrams, is the S beckhoff? 
No -- the "F" and "S" are the "Fast" and "Slow" paths of what has been traditionally called a "common mode" board everywhere -- I was trying to start a clarifying revolution with this diagram...

The lasers in the end-station get the slow temp control directly from the beckhoff from the demos error signal monitor.

The beckhoff links are a little confusing, maybe make a little color legend?
H1 SUS
arnaud.pele@LIGO.ORG - posted 18:58, Friday 28 March 2014 (11082)
ETMY M0 and R0 TF running overnight

started at ~18:50 will run for 8 hours.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:43, Friday 28 March 2014 (11072)
ALS WFS better beam quality

Yesterday I went to end X to investigate the beam shape for the ALS WFS.  (This is to follow up the measurements we made in alog 10774)

First I tried changing the alingment of the reaction chain, this didn't make a difference.  Then I tried changing the TMS QPD offsets.  This moves the lock point of the input alingment loops, changing the alingment of the green beam as it goes through TMS.  This certaintly changes the beam quality on the WFS, screenshots of several different offsets are attached.  In the end I left the offsets at ALS-X_IP_ANG_PIT at -50, ALS-X_IP_POS_PIT at 150. 

I am not sure why changing these offsets makes such a difference in the beam quality. 

This moved the QPD A by 0.07 counts and QPD B by 0.04 counts.  Pablo and I redid the pointing of TMS to the baffle PDs, but it hadn't changed more than the normal change between ISI trips.  However, switching these offsets does move the beamspot on ISCT1, I moved PR3 by 0.9urad in pitch to bring the spot back.  

After realinging the arm, we re checked the phasing of the WFS. We did this by putting an exictation on LSC-X_EXTRA_AO_1_EXC at 50Hz and looking at the signals of the individual segments, which seems fine.  This is saved in /home/sheila.dwyer/ALS?HIFOX/WFS/WFS_PhaseDTT_March282014.xml

Then we started the sensing matrix measurement in Alexa's alog 11073

Non-image files attached to this report
H1 SUS
arnaud.pele@LIGO.ORG - posted 18:39, Friday 28 March 2014 - last comment - 18:41, Friday 28 March 2014(11067)
ETMX UIM filter tested

This week, I tested the ETMX UIM P2P and Y2Y filters (described in alog 10912). The results are showing that filters are working as expected giving a single pendulum transfer function falling at 1/f^2 after the resonnance (f=0.45Hz for pitch, f=0.6Hz for yaw). Also the coupling between pitch and yaw is small (~5%) so unless this is too much, there's no need for diagonalization for UIM.

Attached pdf are showing P2P P2Y (first pdf) Y2Y Y2P (second pdf) transfer functions with/without the filter.

Left to do for next week :

ETMX : Long decoupling on UIM/PUM

ETMY

ITMX/ITMY

Non-image files attached to this report
Comments related to this report
arnaud.pele@LIGO.ORG - 18:41, Friday 28 March 2014 (11080)

sorry for the 90degrees rotated pdfs ! couldn't find a way to rotate and save them.

H1 SEI
hugh.radkins@LIGO.ORG - posted 18:03, Friday 28 March 2014 (11078)
WHAM4 SEI--HEPI MEDM Populated & Safe snapped--Measurement Underway

I got the medms populated so the cartesian location values are now valid.  These initial values today are the 'Aligned' numbers.  They will probably be a little different after these range of motion/linearity tests complete and the stress of the system are further released/shaken out.

LHO VE
kyle.ryan@LIGO.ORG - posted 17:55, Friday 28 March 2014 (11076)
Pre-pumpdown activities at Y-end
Removed iLIGO RGA hardware from BSC10 and installed 10" blank in its place*installed ESD interlock gauge and 4.5"-2.75" zero-length reducer on BSC10*Installed 2.5" aLIGO RGA isolation valve and 10"-4.5" zero-length reducer on BSC6 (remaining aLIGO RGA components to be installed later) 

"Bumped" dial indicator cluster on BSC10's NE support tube -> readings from these dial indicators can be considered "bogus" as a result 

Running QDP80 overnight but couldn't start Turbo pump as its foreline pirani gauge isn't working now(?) -> I'll fix this gauge tomorrow while rough pumping the Y-end with the QDP80.
H1 ISC
alexan.staley@LIGO.ORG - posted 17:48, Friday 28 March 2014 (11073)
WFS Comissioning

(Alexa, Daniel, Sheila)

We measured the WFS sensing matrix for both PIT and YAW. The matrices were computed by exciting ITMX/ETMX PIT/YAW at 1.5Hz with 0.3 amplitude, and looking at the WFS transfer function. The results can be found in the following DTTs saved in /ligo/home/sheila.dwyer/ALS/HIFOX/WFS/:

Inverting the results gives...

YAW input sensing matrix:

-2.294    -3.155

0.529     -2.604

PIT input sensing matrix:

-0.494    -0.239

0.302    -0.489

These values are in microradians; however the factor of 1e-3 is taken care of in the gain of the filter module. We also adjusted the signs as follows:

Under this configuration, with all four DOFs engaged (DOF 1,2 P,Y) the WFS_A/B_I_YAW/PIT_OUTMON all converge to zero. The lock appears to be stable with a transmission betweeen 950 to 1050 counts. Futher investigation needs to be done...

H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 17:35, Friday 28 March 2014 (11074)
TCS CO2X laser install - leaking laser housing, issue with flow meter, chiller settings, Beckhoff

Aidan. Dave H. Greg G. Thomas V.

We have, basically, finished installing all the electronics and cabling on the TCSX table. There are a few outstanding issues (summarized in the attached PDF). The ones that are preventing us from turning on the laser are listed below.

  1. For some reason, the flow meter is not outputting a sense current (current proportional to the measured flow). This means that the CO2 controller, D1200745, is registering low flow and preventing the laser from being turned on. We're not sure if this is a faulty connection at the terminal block in the meter or if there is a deeper problem. We will continue investigating on Monday. The connections are shown in photo 1.
  2. The TCS Beckhoff unit is, apparently, running but is not connecting to EPICS. We need to be able to access the software on/off switch to turn the laser on.
  3. We don't currently have the viewport IR sensor that plugs into the CO2 laser controller, D1200745. We can bypass this input by changing a jumper on the board.

We hope to address all these early on Monday to get the laser running to check the output power.

Chiller settings:

We adjusted the bypass valve on the back of the TCSX chiller to achieve the following settings (to mimic what's at LLO)

Flow rate: 3.4GPM

Pressure: 60.5PSI

Laser housing leak.

The replacement laser installed on the TCSX table also has a slow leak from the laser housing (in the same place as the first one) - about 1 drip every 5 minutes. We will check the output power of this laser before we pull it. See photos 3 & 4

Images attached to this report
Non-image files attached to this report
H1 SEI
sheila.dwyer@LIGO.ORG - posted 16:55, Friday 28 March 2014 - last comment - 11:45, Monday 31 March 2014(11070)
HAM3 ISI trip

This trip happened around the time of a beckhoff restart.  A beckhoff restart causes a crash of the IMC guardian, which causes it to stop.  Its not clear to me why this should cause MC2 to get a large signal, but it seems to.  This causes a cascade of trips.  Even though I don't know why this happends, creating a safe state in the IMC guardian so that it handels missing channels better could help with the problem. 

Another solution is to have the SUS WDs not trip HEPI.  Can we get that fix soon?

HAM2 also tripped at the same time, Jeff and Hugh brought that back. 

Images attached to this report
Comments related to this report
jameson.rollins@LIGO.ORG - 17:54, Friday 28 March 2014 (11075)

To be clear, IMC guardian did not "crash" in this particular situation.  The guardian responded exactly as it's currently programmed to respond, which is to go into ERROR when it looses communication with any of the channels it's monitoring.  I want to distinguish and ERROR condition, which is something that guardian handles, to a "crash", which means that the guardian process died unexpectedly.

Here's my guess for the sequence of events:

  1. Beckhoff action somehow caused one of the PSL channels (H1:PSL-PERISCOPE_A_DC_ERROR_FLAG) to momentarily disappear.
  2. IMC guardian, which is monitoring the above channel, goes into ERROR when said channel disappears
  3. Around this time, the IMC looses lock, presumably for the same reason the PSL channels disappeared.  Since the IMC guardian is in ERROR and no longer monitoring the IMC situation, it doesn't shut off the feedback to MC2.
  4. Large control signals into MC2 cause it to trip.  A typical watchdog cascade causes everthing from here to Walla Walla to trip.

It's possible guardian could be made slightly more robust against loss of some of it's channels, but that only helps up to a point.  Eventually guardian has to drop into some error condition if it can't talk to whatever it's trying to control.  It could try to move everything to some sort of safe state, but that only works if it can talk to the front-ends to actually change their state.

daniel.sigg@LIGO.ORG - 09:30, Saturday 29 March 2014 (11084)

A Beckhoff restart also causes the IMC servo board to be reset, as well as all whitening for photodiodes, wavefront sensors and QPDs. I assume that the resulting transient caused the MC to trip. It would be interesting to know, if this is due the length or alignment system. Is it the initial transient or a run-away integrator? In either case this should not result in a trip. A better action would be to simply turn off the ISC inputs.

arnaud.pele@LIGO.ORG - 11:45, Monday 31 March 2014 (11094)

After taking a look at the time of WD trips, it seems like HAM3 ISI trips before MC2, see green plot vs red plot (the X axis is the number of seconds after gps=1080083200)

Images attached to this comment
H1 SEI (INS)
hugh.radkins@LIGO.ORG - posted 16:54, Friday 28 March 2014 (11071)
WHAM4 SEI--HEPI Status--HEPI is Unlocked

Please mind the signs here at HAM4, there is an Optic suspended here.  Commissioning to commence shortly.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:35, Friday 28 March 2014 (11069)
Ops Summary
Day Shift Summary
LVEA Laser Safe

Apollo - Bolting dome on BSC10, working on view ports at End-Y
Mitch – Check ACB at End-Y
Hugh – Working on HAM5 HEPI
Richard – Y-Arm TCS cabling

08:35 Mitch – Going to End-Y
08:53 Dave – LVEA working on TCS cabling
09:00 Justin – Moving laser barriers around the HAM4 TCS table area
09:18 Andres – Working on dog clamp shelves next to HAM2
09:20 Hugh & Jim – Working on HAM5 HEPI 
09:29 Betsy & Margo – Going to End-Y for BSC10 closeout
11:26 Filiberto – Going to Mid-Y to pick up TCS panels
13:00 Justin – Transition LVEA to laser hazard
13:20 Dave & Thomas – Turning on TCS chillers
14:00 Filiberto – Going to End-Y to check ACB feed through
14:05 Andres – Working on dog clamps shelves next to HAM2
15:30 Jax – Briefly transitioning End-Y to laser hazard to make a PZT check
15:36 Michael – Going to End-Y to check chamber close status 


H1 General
sheila.dwyer@LIGO.ORG - posted 16:22, Friday 28 March 2014 (11068)
EY picomotors disabled

At Richard's request I disabled the End Y picomotors, so that they will not be used durring the pumpdown.

H1 ISC
jaclyn.sanders@LIGO.ORG - posted 15:15, Friday 28 March 2014 (11066)
ISCTEY handoff
I’ve been more or less solely responsible for commissioning ISCTEY at the end station, and the scope of the project has proven to be slightly larger than the amount of time I have left this trip. This is a summary of what’s left to do to finish commissioning the table. I’ve updated the Blue Team Punchlist to put these onto an “Active Tasks” sheet. 
 
PLL beatnote finding
 
The power and polarization of the fiber light has been drifting. As of yesterday, less than 40uW of power was making it to the table. Last week when Alexa and I first measured, we were getting more like 70uW. The polarization drifts over time, as expected and adjustable by the polarization controller. At the moment, the polarization monitor PD is aligned, but after aligning the PLL path, check to make sure this is still the case; it wasn’t aligned the other day, leading me to assume that the polarization was good when there was actually ~80% of the fiber power missing the polarization PD entirely.
 
For reference, the BBPD on the table has never been exposed to the shorted power cable, so any problems with it are not related to having been powered incorrectly. Also, remember to adjust the nominal power on the TMS green QPDs after optimizing the beatnote.
 
Analog video feedthrough
 
The analog video power cable is not connected because the feedthrough was filed out at some point, so the cable can’t be attached with screws. The two solutions proposed are epoxying the cable to the feedthrough or making a proper part. Either way, you will need to remove the feedthrough, fish the cable out of the table, install the cable, then replace the feedthrough. I have passed custody of this project on to Dick.
 
Wavefront sensing
 
The WFS paths are installed and nominally aligned, and the picomotor mirrors have been tested. The legacy WFS interface is in place at the EY field rack, but it is not cabled. Cables will need to be installed and the electronics will need to undergo the usual testing. The WFS on the table had good RF response in the EE shop but still need to be tested on-table. The return beam shape and quality also needs to be measured on these WFS paths.
 
Faraday mount
 
From the first beam measurement, it appears that the 532 path has some clipping. A new mount for the second Faraday isolator has been left on the bottom left corner of the table. This mount needs to be swapped in, and the beam needs to be realigned to the TMS using the irises on the table. Please check the iris position first, I placed them fairly well but I haven’t checked their positioning recently. The return path will also need to be realigned to the LSC RFPD and the wavefront sensors. 
 
HWS pickoff
 
The Hartmann sensor path will need a pickoff from the return beam. I received the beam sampler from Aidan today, but the wrong mounts were sent from Caltech. Once we receive open mounts, this optic needs to be installed between the second pico mirror and the first iris, and the beam aligned to the irises to return to the TMS. Thomas has custody of the beam samplers and the less-than-optimal mounts.

H1 SUS
betsy.weaver@LIGO.ORG - posted 14:31, Friday 28 March 2014 - last comment - 13:08, Monday 31 March 2014(11064)
EY closeout

Margot and I performed all of BSC10 closeout tasks listed in my previous alog regarding this closeout.  We pulled the FC from the ETMy optic a little after 11am, and the door was going on at ~1:30.  It took "so long" (ha) because we ended up having to spend some extra time calling in the troops about one of the ISC viewports having what appeared to be a scratch on it's inside surface.  More details to come as needed.

Comments related to this report
betsy.weaver@LIGO.ORG - 18:44, Friday 28 March 2014 (11081)

Here are some further pictures of the ACB swing back and the FirstContact spray cone attachment to the HR side of the ETMy QUAD structure from yesterday.  Yes, the cone protrudes into the baffle.  Yes, Margot still was able to fit her head and an arm with the spray bottle in the cone.

The last picture shows the placement of the horizontal wafer and verticle 1" witness optic in the center of the chamber, placed today just before the door went on the chamber.

Images attached to this comment
margot.phelps@LIGO.ORG - 13:08, Monday 31 March 2014 (11097)
Notes and dcc numbers for Contamination Control Samples (ones that came out and ones that went in) to WBSC10 before doors went on:
1. Vertical 1’’ optics on QUAD: T1400246 (SN1195) out and T1400247 (SN 262) in. 
2. Vertical 1’’ optic under quad: T1400248 (SN261) placed at end of closeout.
3. Vertical wafer on quad: T1400249 attached to quad under HR of ETM.
4. Horizontal wafer on floor under quad:T1400250 placed at end of closeout.
5. Horizontal 1’’ optic: T1400251 was left on beam tube floor between BSC10 and BSC6. Looking up SN/history. Didn’t take it out, because we had no clean optic containers handy.
6. 24’’ PET swipe sample taken in tube near purge today close to end of closeout. Labeled, and taken to PET microscope area. 
H1 SUS
betsy.weaver@LIGO.ORG - posted 19:27, Thursday 27 March 2014 - last comment - 18:38, Friday 28 March 2014(11049)
ETMy First Contact Applied

This morning, SEI, TMS, and SUS gave a cursory "approval" of their systems in order to proceed with chamber close-out tasks.  So, after lunch, Margot and I applied First Contact to the ETMy-HR surface which will be pulled just before closing the door tomorrow.  The order of events this afternoon (and late morning in order to catch the alog up):

Jim locked the ISI and put final touches on chamber feedthru cable routing.

Apollo+Joe+Gerardo had a viewport party at the BSC10/6 area.

Margot and I locked the lowest masses of the ETMy QUAD.  Then we,

Secured the ACB locking bracket and used the wedge to swing it back and prop it into place.  See notes on this in attached alog.

Attached the FC QUAD cone to the structure and sprayed FC (standard 3 coats) on the HR surface.

Removed the cone from the suspension.  Finished FC layer reinforcement.

Removed the wedge from the ACB and restored it's nominal hanging position. Removed the ACB locking bracket screws.

Started stowing all left over bags of "junk" left outside of the chamber door on various table surfaces by SUS and every other team that visited this last month.  If you're missing something (and you noticed), I took ownership of it.

Jim arrived and unlocked the ISI.  The ETMy QUAD will remain locked during dome replacement.

Apollo started gearing up to remove walking plates from upstairs and crane the dome on the chamber.

 

Tomorrow's to-do list which Margot and I will do until the last step:

Inspect insides of viewports.

Adjust ACB to check magnet gap which may or may not have shifted slightly due to the swing back from today.

Clean the chamber, vacuum, etc.

Take final PCL swipes.

Blow various other optic surfaces.  Or not.

Swap in final 1" witness optic on QUAD structure.

Check/Remove all tools.

Remove ETMy-HR with N2 blow.

Set and lock all 64 QUAD EQ stops and nuts, accounting for buoyancy.

Set QUAD BOSEMs to account for buoyancy.

Quick QUAD health check with DTT TFs.

Lay final witness plates.

Exit chamber.

Finish stowing everything around door and move it out of the way.

Put door on.

Comments related to this report
betsy.weaver@LIGO.ORG - 20:10, Thursday 27 March 2014 (11050)

So, when we went to swing back the ACB and stuff the wedge into place, the wedge could not be inserted in the gap all of the way due to interference with the round balance weight attached on top of the baffle.  We pushed the wedge in ~2/3 of the way which gave us ~2/3 more working area than we had with out swinging it back at all.  Good enough.  (Removing the round weight would have cause the balance of the ACB to be out of alignment so that wasn't an option.)  Also, even though the locking bracket was engaded which provided some support to the down tube of the ACB, the ACB was still a bit "rickety" during this maneuver.

betsy.weaver@LIGO.ORG - 18:38, Friday 28 March 2014 (11079)

The first picture below is of the ACB wedge not quite installed as far in as it could.  This meant that the screw holes to secure the wedge in place could not be engaged.  ACB engineers must have anticipated this so they provided us with a "safety" chain which one could tie up "somewhere" such that the wedge doesn't come flying out at you if you bump the baffle while it's up.  The chain was of limited length, so they best Margot and I could do was wind it around the post loosely a few times.  Note, the wedge seemed wedged in well enough that it didn't budge when we did happen to bump the baffle a bit here and there with the cone work.

 

Also note, the ACB did not hang the same way after we restored it.  Mitchell had to make some minor tweeks to the balance today in order to recover the correct gap setting for the magnets (specifically 0.09 inches! - Really?  Not 0.08" or 0.1", but 0.09", huh!?  Seems a bit tight given the grossness of both the swing back application and the shear size of the baffle... but what do I in SUS know.)  In the end, as usual the ACB comes with in a few mm of the QUAD structure at the head of one of it's screws (see 2nd picture with red circle around it).

Images attached to this comment
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