There was an attempt to calibrate the sliders for the H1:SUS-ITMY_R0_OPTICALIGN_ P _OFFSET And also for Yaw.
Robert & Sheila were inside the vacuum chamber over by GV5 holding up a "Calibration sheet".
I was tasked to move the sliders back an forth.
H1:SUS-ITMY_R0_OPTICALIGN_P_OFFSET has a range from -410 to +410.
I set the ramp time to 10 seconds, and the stepsize to 880.
At 21:14 UTC I typed in the value to send the slider to -440.
I then took a singular step that took the slider from -440 to +440, and then took the slider back to -440 with a singular step.
This was repeated a few times.
I then changed the step size from 880 to 440 and set the slider to -220.
Then stepped from -220 to +220 with a singular step, and back to -220 again.
I then did a similar process again for H1:SUS-ITMY_R0_OPTICALIGN_Y_OFFSET which has a range from -610 to +610.
So the step size this time was 1220.
The slider was moved to -610 at 21:18 UTC.
The slider was then stepped over to +610 via a singular click of an arrow key. Then back down to -610 again with another click.
This was repeated once again.
The step size was then reduced to 610 , and the slider was moved to -305. We then stepped up from -305 to + 305 with a step.
the slider value was returned back to -305 and the process was repeated.
I assume that Robert was holding a laminated sheet of graphing paper that we could use as an absolute reference for this slider values to calibrate the beam movements.
Randy, Tyler, TJ,Oli,Corey, Mitch, Jim
Starting after lunch today, we launched on starting to disassemble the HAM1 passive stack. First we had to pull the L4Cs we installed IN the optical table. These proved difficult to remove, most of the screws could be removed with a long t-handle 3/16 allen key, but for the 2 vertical L4Cs on the +X side each one had one screw that was difficult to find a way to reach. Corey ended up removing the clamps from his, TJ painfully removed a final screw 1/8th a turn at a time. This took most of the afternoon.
While we chewed on that problem, we also tried pulling the pins holding the optical table to the mass stack. These also proved difficult, it seems like the pins may have been overtorqued. We ended up having to use a wiped down pair of vise grips to assist an awkwardly inserted screwdriver to break all 12 bolts free.
Once the L4Cs and optical table bolts were removed, pulling the table was simple: attach the lifting plate, pull up with the fork lift gently until the optical table popped free, then up and out of the chamber. The optical table is sitting on a pallet between HAM2 and HAM3, probably headed for recycling. Everything else is going to be bagged and tagged for somebody else's project.
Tomorrow we'll finish pulling the masses and support table.
TITLE: 04/09 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: HAM6 turbo work completed, BSC8 work progressed, and HAM1s passive stack was cleared off, the cabling was removed, and the passive stack's tabletop is on a pallet.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:35 | FAC | Nelly, Kim | LVEA | n | Tech clean (in at 14:20) | 17:58 |
14:36 | FAC | Randy | LVEA | n | Crane over YARM (in at 14:35) | 14:49 |
15:10 | VAC | Jordan | LVEA | n | Purge air checks | 15:23 |
16:07 | SLiC | Tony, Ibrahim, Sheila, Betsy, Robert | LVEA-BSC8 | n | BSC8, ITMY CP | 18:38 |
16:08 | ISC | Camilla, Elenna, Oli, Rahul | LVEA-HAM1 | n | HAM1 parts removal, Oli & Elenna out 18:30, Camilla 18:48 | 18:49 |
16:13 | CDS | Fil, Marc, Corey | Opt Lab | n | HAM1 cable prep, corey out @ 1800UTC | 19:42 |
16:24 | Property | Christina | Mids | n | Pelican case check | 16:44 |
16:39 | SEI | Jim & Mitch | LVEA | N | HEPI actuators disconnect cont | 18:44 |
16:41 | VAC | Travis, Melina, Jordan | LVEA | N | HAM6 turbo | 19:13 |
16:42 | SPI | Jeff, Josh | Optics lab | N | SPI pickoff install prep | 19:01 |
17:08 | IAS | Jason | LVEA | N | FARO temperature troubleshooting | 17:47 |
17:21 | OPS | TJ | LVEA | N | Check for tooling | 18:31 |
17:58 | OPS | Jennie, Matt+2 | LVEA | N | TOur for new fellows | 18:20 |
17:59 | FAC | Nelly | MidY | N | Tech clean | 18:54 |
18:24 | FAC | Richard | LVEA | N | Safety checks | 18:36 |
18:54 | FAC | Nelly | MidX | N | Tech clean | 19:27 |
19:05 | SPI | Jeff, Josh | Optics lab | LOCAL | SPI work | 19:34 |
19:38 | ISC | Camilla, Rahul | LVEA | N | HAM1 parts removal, Rahul out 20:42 | 20:54 |
19:43 | ISC | Elenna | LVEA | N | Grab drawing by HAM1 | 19:47 |
19:43 | ISC | Tj | LVEA | N | HAM1 work, platform stair removal | 23:26 |
19:49 | FAC | Randy | LVEA | N | HAM1 work, forklifting | 22:00 |
19:59 | CDS | Dave | MidX | N | Wind sensor, midy and ends after for various fixes | 20:51 |
20:09 | ISC | Corey | LVEA | N | HAM1 work | 23:25 |
20:11 | FAC | Richard | LVEA | N | Checks/Walkthrough, in and out | 21:04 |
20:23 | OPS | Oli | LVEA | N | Wrap bag and tag | 23:26 |
20:23 | ISC | Mitch, Jim | LVEA | N | HAM1 passive stack, Mitch out 23:20 | 23:26 |
20:44 | VAC | Jordan, Melina | LVEA | N | HAM6 turbo work | 22:33 |
20:47 | EE | Fil, Marc | Optics Lab | Local | Measurements | ? |
21:02 | ISC | Ibrahim, Robert, Sheila | LVEA | N | BSC8 ITMY work | 22:28 |
21:09 | ISC | Betsy | LVEA | N | Join BSC8 ITMY crew | 22:36 |
21:24 | FAC | Richard | LVEA | N | Steel toe shoe count | 22:01 |
22:13 | FAC | Tyler | LVEA | N | CHeck out HAM1 progress | 22:28 |
22:25 | FAC | Richard | LVEA | N | Safety checks | 22:50 |
22:29 | FAC | Tyler | LVEA | N | Quick check | 23:20 |
Ibrahim, Tony, Betsy, Sheila, Robert
We tried adjusting the pitch of CPY to overlap the optical lever beam spot from the arm cavity side of CPY with the spot from the AR side of ITMY, but the PUM-level inter-chain earthquake stops limited our pitch adjustment. The figure shows that we reduced the distance between the spots we were trying to overlap by a factor of 0.56. If we are going to leave it this way, we should back off a little from this setting.
Travis, Melina, Jordan
Per the updated HAM6 VE drawing (D0901823), we moved the HAM6 turbopump and pump out spool from the top D7 flange to the -Y door BF3 port. The 12"CF ->10" CF adapter, gate valve, pump out spool and turbo pump were removed and replaced with a single 12"CF blank on the D7 flange. We also replaced the turbo with a 500 l/s Leybold maglev turbo compatible with the SS500 pump carts.
The turbo assembly (with GV closed) was pumped down and helium leak checked. Each joint sprayed with a 5s dwell of He, no signal observed above the leak detector background of 3.6E-10 Torr-l/s. Remaining chamberside flanges will be He leak checked during corner pumpdown.
Nice work, guys! Looks great!
Rahul, Elenna, Oli, TJ, Camilla, Jim, Betsy. WP12419
Following yesterday's work 83820, this morning we removed all remaining ISC components on HAM1. Rahul removed RM1, RM2 and the SEI 10kg weights (bolts are in foil pouches with the weights).
Everything has been placed on a rack in the HAM1 cleanroom, labeled photo attached. The beamdumps are ordered as shown, BD17 and 18 are the largest plates (BD naming convention in D1000313 v17 Cartoon). Which pan each optic is in has been added to the D1000313 googledoc along with any optic serial numbers that could be read, our current working copy of the document is attached.
After lunch, TJ removed the platforms/stairs around HAM1 and Rahul, Jim and I removed all the ISC and SUS cables. All DB-25s were stored in foil in the ISC components rack (bottom shelf) and the RF cables have been given to Fil for rework.
Adding a picture of the HAM1 table after all the components were removed.
Tagging EPO for pic.
Wed Apr 09 10:11:18 2025 INFO: Fill completed in 11min 14secs
J. Kissel, B. Lantz, E. Bonilla, O. Patane Very alarmed but how *apparently* different the in-air vs. in-vac TFs for H1SUSSR3 were -- see original plots in LHO:83818, and alarmed commentary in LHO:83819 -- Brian suggested "are you *sure* you've plotted the same DOF to DOF comparison on some of these plots?" He was right. I re-exported both the 2024-08-01 in-air transfer function set and 2024-08-08 in-vacuum set from the DTT templates. The in-air TF's exported text files showed a diff with what was in the svn on the L, T, V, and Y drives. So, all the TFs that were "very interesting" in the above mentioned commentary were "very interesting" because they were comparing apples to oranges, and treating that orange as an apple. So, here, I attach the same comparison for SR3, but with the fixed in-air data set. D R I V E D O F L T V R P Y L -- meh nd meh eand YI R T meh -- meh eand meh meh E S V YI YI -- YI nd YI P R YI eand YI -- YI meh D O P eand VI YI meh -- meh F Y YI nd meh nd nd -- Recall the legend is VI = Very Interesting (and unmodeled); very different between vac and air. esVI = Modeled, but Still Very Interesting; very different between vac and air YI = Yes, Interesting. DC response magnitude is a bit different between vac and air, but not by much and all the resonances show up at roughly the same magnitude. meh = The resonant structure is different in magnitude, but probably just a difference in measurement coherence eand = The cross coupling is expected, and not different between air and vac. nd = Not Different (and unmodeled). The cross-coupling is there, but it doesn't change from air to vac. Thankfully, - there are WAY less "very interesting," only the T to P (page 22) remains. - the matrix is more symmetric, and - the changes between air and vac are LOT less dramatic. We'll continue to discuss.
Morning dry air skid checks, water pump, kobelco, drying towers all nominal.
Dew point measurement at YBM in prep for BSC1/8 work, -42C
Starting around 22:13 Tue08apr2025 the MX weather station wind speed anemometer stopped recording. The other MX sensors, for example outside temperature, continue to run.
Attachment shows wind speed and temp for EX top row, and for MX bottom row.
Literally minutes after I made this alog, unbeknownst to me, it fixed itself. I drove to MX this afternoon and visually confirmed the paddles were turning and appared to be unrestricted. The freeze between 10pm Tue and 9am Wed is still a mystery.
TITLE: 04/09 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: MAINTENANCE
Wind: 4mph Gusts, 2mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.21 μm/s
QUICK SUMMARY:
Plans for today:
Today's activities:
J. Oberling, R. Crouch
Today we took pre-deinstall measurements of the position of the optical table surface of the WHAM1 passive stack. The plan was to use the FARO to measure the coordinates of several bolt holes, using a threaded nest that locates the Spherically Mounted Retroreflector (SMR) precisely over the bolt hole, on both the +Y and -Y side of the chamber. This, unfortunately, did not happen in full due to the untimely death of the FARO's climate sensor (or the FARO's ability to read the climate sensor, we're hoping for the former). The FARO cannot function without this sensor as it relies on accurate measurements of the air temperature, relative humidity, and air pressure to feed into a model of the refractive index of air, which it needs to accurately calculate the SMR distance from the FARO. We did manage to get a few points measured before the sensor died. I've reached out to FARO tech support about getting a new climate sensor and should hear back from them tomorrow (they usually replay in 1 business day).
Summary
We were able to get measurements of 3 bolt holes, all in the furthest -Y line of bolt holes, and an old IAS monument from aLIGO install before the FARO's climate sensor died. The results are listed below under the Results heading. The most interesting thing here is there appears to be an error in WHAM1 placement in the x-axis, as the bolt holes we measured are all ~37.25 mm too far in the -X direction from nominal. We also set a scale on the wall across from the -Y door of the WHAM1 chamber that is registered to the current elevation of the optical table; placing an autolevel so it sights 150.0 mm on this scale (sighting the side of the scale with the 0.5 mm tick marks) places that autolevel 150.0 mm above the surface of the passive stack's optical table.
Details
We started on the -Y side of the WHAM1 chamber. The FARO was set with a good view of its alignment monuments and the passive stack's optical table. We ran through the startup checks and calibrations without much issue (we did see a return of the odd 'ADM Checks Failing' error, which had been absent for about 1 month, but it immediately went away and didn't come back when we performed a Go Home operation). FARO monuments F-CS026 through F-CS035, inclusive, were used to align the FARO to the LHO LVEA local coordinate system; the 2 standard deviation device position uncertainty after this alignment was 0.016 mm (PolyWorks does 100 Monte Carlo simulations of the device position). This complete, we started measuring.
First, as a quick test of the alignment we took a look at old IAS monument LV24. This monument was used to align the WHAM2 ISI during aLIGO install, and its nominal X,Y coordinates are [-20122.0, -3050.7] mm (there is no z-axis coordinate as we were not setting these in Z back then, a separate set of wall marks was used for z-axis alignment). The results are shown in the 1st attached picture; again, ignore the z-axis results as I had to enter something for the nominal or PolyWorks wouldn't accept the entry, so I rounded to the closest whole number (this isn't even the surface of the monument, it's the point 2" above it where the SMR was, due to use of the Hubbs Center Punch Nest (which has a 2" vertical offset when using a 1.5" SMR)). Knowing how we had to set these older monuments, since I'm one of the people that set them, I'm not entirely surprised by the X and Y deviations. The monuments we set for aLIGO install (the LV monuments) were placed w.r.t. a set of monuments used to align iLIGO, which themselves were placed w.r.t. the monuments used to install the vacuum equipment during facility construction (the PSI monuments), which themselves were placed w.r.t. the BTVE monuments which define the interface between the arm beam tubes and the LVEA vacuum equipment, which we then found errors in their coordinates during our alignment of the FARO during the O4a/b commisioning break in 2024. Not at all surprised that errors could have stacked up without notice over all of those monuments set off of monuments set off of monuments set off of... Also, take note of the x-axis coordinate of this monument, this will be important later.
We then set about taking measurements of the passive stack optical table. To map the bolt holes we measured we used an XY cartesian basis, assuming the bolt hole in the -X/-Y corner was the origin. We then proceeded to increment the number by the bolt hole (not distance), following the same XY axis layout used for the IFO. Using this scheme the bolt holes for the table corners were marked as:
We were able to get measurements for bolt holes (0,0), (14,0), and (25,0). We were in the process of measuring bolt hole (36,0) (the +X/-Y corner bolt hole) when the FARO's climate sensor died.
To get the coordinates for the bolt holes I used the .EASM file for WHAM1 with the passive stack configuration located at D0901821-v4. From the assembly, using eDrawings, I was able to get coordinates w.r.t. the chamber origin for the bolt holes we measured. Those were then added to the coordinates for the WHAM1 chamber, in the LVEA local coordinate system, to get nominal coordinates for the bolt holes. I also had to add 25.4 mm to the z-axis coordinates to account for the 1" offset of the nest we were using for the SMR; the center of the SMR sits 1" above the point being measured, so I needed to manually add that offset to the nominal z-axis coordinate of the bolt hole. For reference, according to D0901821 the global coordinates for WHAM1 are [-22692.0, 0.0, 0.0] mm; when converted to the LVEA local coordinate system (removing the 619.5 µrad downward tilt of the X-arm) this becomes [-22692.0, 0.0, +14.1]. The measurement results are shown in the 2nd attached picture. Notice those x-axis deviations? Remember the measurement we made of LV24? Clearly the FARO alignment is not 37 mm off, as the measurement of LV24 showed, so something is definitely up with the x-axis coordinate of the WHAM1 chamber (error in chamber placement? aLIGO WHAM1 is the iLIGO WHAM2 chamber, moved from its old location next to WHAM3).
Results
We can do some analysis of the numbers we have, although limited since we only have 3 points in a line. This really only applies to the furthest -Y line of bolt holes on the table, since we weren't able to get measurements of the +Y side to get a more full picture of where the table is sitting, but it's something. Position tolerances at install in 2012 were +/-3.0 mm in all axes.
I do want to note that D0901821-v4 claims the table surface should be -187.8 mm in LVEA local coordinates (-201.9 mm in global), but this is not the number we used when installing the passive stack in 2012. In 2012 we used -185.9 mm local (-200.0 mm global), as can be seen in D0901821-v2. To compare our measurements to the install numbers I changed the nominal z-axis coordinate to match that of our install target (-185.9 + 25.4 mm SMR offset = -160.5 mm) and the results are shown in the final attached picture.
Wall Scale Registered to Current Table Surface Elevation
To finish, we set a scale on the -Y wall directly Crane East of the WHAM1 chamber and registered it to the current elevation of the passive stack's optical table. To do this we used a scale provided by Jim (the scale was in inches, with 0.01" tick marks) and an autolevel. We set the autolevel at a fixed elevation on the -Y side of the chamber. The scale was then placed at each corner of the optical table, starting with the -X/+Y corner, and the autolevel was used to sight the scale; only the scale was moved, the autolevel was fixed (rotated only to follow the scale, but not moved otherwise). We then averaged the 4 scale readings to get the table elevation, set the autolevel to this reading with the scale back at our starting point (we actually didn't have to move it, thankfully), and then set a scale on the wall using the autolevel. The 4 scale readings:
The average of the 4 readings is 5.9", and since the autolevel was already sighting 5.9" on our starting point at the -X/+Y corner we left it there. This may seem high, but we had to have the autolevel high enough that we could see over the various components mounted to the table surface. We then turned the autolevel and set a scale on the wall. This scale was in mm (since that's what we had), but this worked out OK. 5.9" is ~149.9 mm (149.86 mm to be exact), so we set the wall scale so it read ~149.9 mm when sighted through the autolevel. So a 150.0 mm reading on this scale (sighting the side with the 0.5 mm tick marks) is ~150.0 mm above the current position of the passive stack's optical table.
This closes LHO WP 12442.
TJ O'Hanlon informed me via email that there indeed was an error in the x-axis coordinate at both LHO and LLO, due to the thickness of the septum between HAM1 and HAM2 not being taken into account, which had not been propagated to all of the SYS mechanical layout drawings (and some of the CAD files as well). I had completely forgotten about this, and explains why we had moved the WHAM1 passive stack monument LV25 further in the -X direction some time back in 2012; the first attached picture shows this (the clear cut out next to the existing monument was the old position of LV25 before we moved it). I went spelunking through my old 2012 emails to find some communication about this, but all I could find was an email chain re: LLO setting the LHAM6 support tubes and not being able to get them in the proper y-axis position. Dennis replied that this was due to the septum thickness and would apply to HAM1 and HAM6 at both sites, and that he would update E1200625 with the correct coordinates for all involved chambers. From E1200625 the x-axis coordinate of WHAM1 should be -22726.7 mm, so I have updated the PolyWorks project with this new, correct coordinate; this is shown in the 2nd attached picture.
From this I can now say that the -Y row of holes on the WHAM1 passive stack's optical table are ~2.56 mm too far in the -X direction. If we were to use the FARO to survey monument LV25 my guess is that would explain the 2.5 mm error, seeing as how nearby LV24 was also ~2.0 mm too far in -X direction. As stated in the main alog this difference doesn't exactly surprise me given the "monuments placed off of monuments placed off of monuments" situation we have here. The FARO was aligned to our X and Y axes using monuments PSI-1, PSI-2, PSI-6, and BTVE-1, so any error between these 1st and 2nd generation monuments and the 4th generation LV monuments will be measured by the FARO.
While I was at it I went ahead and applied the required transform for local to global coordinates. This is done by creating a new coordinate system and applying the requisite tilt of both the X and Y axes. The tilt must be entered in degrees and for the opposite axis. This is because our, for example, y-axis tilt angle w.r.t. local gravity is a rotation of the x-axis. Since PolyWorks works off of axis rotation, we enter the y-axis angle as an x-axis tilt (same for the x-axis angle). To get PolyWorks to correctly calculate the transform matrix both values should be entered as positive numbers (I'm not entirely sure why). The values to enter:
The calculated transform matrix is shown in the 4th attached picture, which properly matches Table 10 in T980044 (note, the numbers in the transform matrix are in radians, even though I had to enter the rotations in degrees). To confirm this was correct I manually calculated the correct global z-axis coordinate using the formula in Section 2.3 of T0900340 for each bolt hole; the results were the same between my calculation and PolyWorks'. The final picture shows the bolt hole survey in the LHO global coordinate frame.
This morning, we added dial indicators to the ends of the support tubes to monitor the support tube locations on the -X side. We had to remove a cable tray to get room to do this under the chamber. They are protected under the chamber, but there is a bunch of loose cabling on that side that could bump my set up. Unfortunately, we don't have access to the northside. Not quite sure how to track the support tube ends on the +X side when we float HEPI yet.
While Betsy and crew were pulling parts in chamber, Mitch and I were disconnecting actuators at the piers. Vertical actuators are quite difficult, access is very tight, going to be hard reconnecting them. Horizontal actuators are a lot easier, but we are adding .100" shims and bolts to protect the bellows and IPS, we lost a couple shims inside one of the actuators and it was a struggle to fish them out. We are adding wires to the shims going forward to prevent that mishap. We'll get the other 2 actuators tomorrow. So far dial indicators show we are still in the same spot as before disconnecting the actuators.
All 4 actuators are disconnected now, we'll move to passive stack de-install after lunch. Dial indicators we have move .002", but that could very well just be drift in my set up.
[Betsy, Camilla, Elenna, Oli]
We cleared half of the HAM1 table today on the +y side. This cleared optics on the ALS and POP paths, and the first part of the optics on the REFL path. We carefully labeled each component, and Oli logged component and cable names with serial numbers. Betsy laid the components in clean pans lined with cleanroom cloths. The cables are still attached to the feedthroughs and were left lying at the bottom of the chamber.
Attached photos show cleared side of the table.
Before removing components, we reviewed the table layout after Ibrahim and TJ noticed some discrepancies between the solidworks drawing and the optic locations as depicted in Corey's pictures from yesterday. We confirmed that there are some dispcrepancies between the two. TJ has a more detailed report.
Before we started, Betsy and I replaced the septum plate VP cover we had removed yesterday 83798.
Layout before: D1000313-v15
Added photo of myself, Betsy, Melina and Elenna before the HAM1 ISC removal work started.