The air handler currently running had its bypass dampers open, so the airflow was bypassing the cooling coil and relying on outside air for space cooling. Because its dampers are manually set, it was not able to reach supply air setpoint. I manually closed the bypass damper which allowed airflow through the cooling coil again and the unit is now reaching supply air setpoint. This is the reason for the sudden drop in space temps in the trend.
Fri Feb 02 10:07:22 2024 INFO: Fill completed in 7min 18secs
FAMIS 26279
The Following Corner station Vibrometers have an increase at the same time:
H0:VAC-MR_FAN1_170_1_ACC_INCHSEC Has an Increase 24 hours ago and a decrease a few how
H0:VAC-MR_FAN1_170_2_ACC_INCHSEC
H0:VAC-MR_FAN4_170_1_ACC_INCHSEC
H0:VAC-MR_FAN6_170_1_ACC_INCHSEC
H0:VAC-MR_FAN6_170_2_ACC_INCHSEC
H0:VAC-MR_FAN2_170_1_ACC_INCHSEC looks to be zero but also had a big spike at the same time.
This event was coupled with an increase in LVEA temperature as well.
H0:VAC-EX_FAN1_570_1_ACC_INCHSEC also had an increase about 2 and a half days ago but it has since come back down.
Both MC2 and PR2 suspensions in HAM3 chamber are healthy as per the transfer function measurements I took this morning. Please see the plots attached below, the templates are stored at the following location,
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/MC2/SAGM1/Data
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_L_0p02to50Hz.xml
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_P_0p02to50Hz.xml
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_R_0p02to50Hz.xml
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_T_0p02to50Hz.xml
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_V_0p02to50Hz.xml
2024-02-02_1500_H1SUSMC2_M1_WhiteNoise_Y_0p02to50Hz.xml
MC2 T_dof (see page 4) has a small unwanted peak at around 4.1Hz which I suspect is due to the purge air in the Chamber. However it looks better when I took a second measurement as shown here. So nothing to worry.
/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PR2/SAGM1/Data
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_L_0p01to50Hz.xml
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_P_0p01to50Hz.xml
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_R_0p01to50Hz.xml
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_T_0p01to50Hz.xml
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_V_0p01to50Hz.xml
2024-02-02_1600_H1SUSPR2_M1_WhiteNoise_Y_0p01to50Hz.xml
Closes 26229, last done in alog 75568
Laser Status:
NPRO output power is 1.816W (nominal ~2W)
AMP1 output power is 67.86W (nominal ~70W)
AMP2 output power is 136.4W (nominal 135-140W)
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PMC:
It has been locked 12 days, 18 hr 31 minutes
Reflected power = 18.49W
Transmitted power = 108.3W
PowerSum = 126.8W
FSS:
It has been locked for 17 days 0 hr and 35 min
TPD[V] = 0.6663V
ISS:
The diffracted power is around 2.0%
Last saturation event was 17 days 1 hours and 7 minutes ago
Possible Issues:
PMC reflected power is high
FSS TPD is low
PMC power looks high, but I'm expecting this is not the biggest worry due to the state of the detector.
Closes 26506
Attached is the 3-month trend for the SUS HWWDs.
ETMX had a couple switches throughout the past rotation therefore no further action is needed.
Closes 26846
check_T240_centering.py
Averaging Mass Centering channels for 10 [sec] ...
2024-02-02 08:45:06.261973
There are 26 T240 proof masses out of range ( > 0.3 [V] )!
ETMX T240 1 DOF X/U = -0.316 [V]
ETMX T240 1 DOF Z/W = -0.369 [V]
ETMX T240 2 DOF X/U = -0.385 [V]
ETMX T240 2 DOF Z/W = -0.638 [V]
ETMX T240 3 DOF Y/V = -0.452 [V]
ITMX T240 1 DOF X/U = -1.323 [V]
ITMX T240 2 DOF X/U = -0.37 [V]
ITMX T240 2 DOF Z/W = -0.32 [V]
ITMX T240 3 DOF X/U = -1.367 [V]
ITMY T240 1 DOF Y/V = -0.319 [V]
ITMY T240 1 DOF Z/W = -0.475 [V]
ITMY T240 2 DOF Z/W = -0.609 [V]
ITMY T240 3 DOF X/U = -1.023 [V]
ITMY T240 3 DOF Y/V = -0.356 [V]
ITMY T240 3 DOF Z/W = -1.281 [V]
BS T240 1 DOF X/U = -0.487 [V]
BS T240 1 DOF Y/V = -0.697 [V]
BS T240 1 DOF Z/W = -0.384 [V]
BS T240 2 DOF X/U = -0.318 [V]
BS T240 2 DOF Y/V = -0.365 [V]
BS T240 2 DOF Z/W = -0.482 [V]
BS T240 3 DOF X/U = -0.629 [V]
BS T240 3 DOF Y/V = -0.589 [V]
BS T240 3 DOF Z/W = -0.932 [V]
HAM8 1 DOF X/U = -0.347 [V]
HAM8 1 DOF Z/W = -0.502 [V]
All other proof masses are within range ( < 0.3 [V] ):
ETMX T240 1 DOF Y/V = -0.214 [V]
ETMX T240 2 DOF Y/V = 0.02 [V]
ETMX T240 3 DOF X/U = -0.274 [V]
ETMX T240 3 DOF Z/W = -0.213 [V]
ETMY T240 1 DOF X/U = 0.16 [V]
ETMY T240 1 DOF Y/V = 0.184 [V]
ETMY T240 1 DOF Z/W = 0.247 [V]
ETMY T240 2 DOF X/U = -0.016 [V]
ETMY T240 2 DOF Y/V = 0.219 [V]
ETMY T240 2 DOF Z/W = 0.13 [V]
ETMY T240 3 DOF X/U = 0.269 [V]
ETMY T240 3 DOF Y/V = 0.194 [V]
ETMY T240 3 DOF Z/W = 0.194 [V]
ITMX T240 1 DOF Y/V = -0.197 [V]
ITMX T240 1 DOF Z/W = 0.016 [V]
ITMX T240 2 DOF Y/V = -0.233 [V]
ITMX T240 3 DOF Y/V = -0.252 [V]
ITMX T240 3 DOF Z/W = -0.209 [V]
ITMY T240 1 DOF X/U = -0.24 [V]
ITMY T240 2 DOF X/U = 0.034 [V]
ITMY T240 2 DOF Y/V = -0.095 [V]
HAM8 1 DOF Y/V = -0.278 [V]
check_sts_centering.py
Averaging Mass Centering channels for 10 [sec] ...
2024-02-02 08:46:20.259287
There are 2 STS proof masses out of range ( > 2.0 [V] )!
STS EY DOF X/U = -4.127 [V]
STS EY DOF Z/W = 2.843 [V]
All other proof masses are within range ( < 2.0 [V] ):
STS A DOF X/U = -0.667 [V]
STS A DOF Y/V = -0.734 [V]
STS A DOF Z/W = -0.517 [V]
STS B DOF X/U = 0.468 [V]
STS B DOF Y/V = 0.956 [V]
STS B DOF Z/W = -0.475 [V]
STS C DOF X/U = -0.666 [V]
STS C DOF Y/V = 0.932 [V]
STS C DOF Z/W = 0.325 [V]
STS EX DOF X/U = -0.148 [V]
STS EX DOF Y/V = 0.028 [V]
STS EX DOF Z/W = 0.065 [V]
STS EY DOF Y/V = 0.181 [V]
STS FC DOF X/U = 0.264 [V]
STS FC DOF Y/V = -0.947 [V]
STS FC DOF Z/W = 0.733 [V]
A new cds conda environment is available for testing.
Switch to the environment with 'conda activate cds-testing'.
Two workstations, cdsws27 and cdsws22 use cds-testing as the default environment. If you run in to trouble on these workstations, you can switch back to the production environment with 'conda activate cds'.
This environment includes two new programs from Gabriele: 'interactivefitting' and 'loopdesigner'.
It also includes a new release of diaggui and foton, version 4.0.3. This version has minor improvements and bug fixes.
foton now can suppress warnings for zeros in the right-hand plane. Pass -Z f as a command line argument or set the environment variable FOTON_WARN_RHP_ZEROS=false. The environment variable will also work with python-foton.
Difference cursors now work in diaggui plots.
For a full list of changes see https://git.ligo.org/cds/software/dtt/-/wikis/ChangeHistory
[Jonathan, Dave, Erik]
The portal for remote access to CDS, cdsssh, received an OS upgrade. Remote access to CDS was down during the upgrade and is now restored.
TITLE: 02/02 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 5mph Gusts, 4mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.71 μm/s
QUICK SUMMARY:
- HAM 3 work is completed, doors is slated to go back on later today
- HAM 7 beam spot work continues
- CDS/DMs ok
Mitchell, Betsy, Corey, Robert
Today I damped the MC baffles and took beamspot photos. More on this later. For now, I want to give some details about the unplanned baffle I installed.
While taking beam spot pictures I noticed an extremely bright retro-reflection seen by MC3. I had noticed this before (and also a similar glint for PRM). But this was the first time I was using the IR Illumintor and camera at this location. I use bracketing so that I could attempt to avoid saturation since the idea is to be quantitative. I had not previously realized how bright this reflection was – it completely saturated the pixels even with short exposures (see Fig. 1).
So, with creative help form Mitchell, Betsy and Corey, we baffled the glint. Figure 2 shows that the baffle is clamped to a HAM2 wall fixture and projects out about 2 cm from the wall to hide the glint surface from the MC3 beamspot.
In addition to the unplanned baffle 17 nozzle baffles were installed. Ten D2000285 type 11, and six D2000285 type 01.
Julian, Sheila, Vicky, Camilla. After today's alog 75677 ZM4 PSAMs offloading. WP11666
Started with ZM4 sliders at Pit -362, Yaw -273. Our beam off the OPOS was good, centered on both HAM7 QPDs with nsum 150 to 160.
The beam was off mainly in yaw, centered on irises by moving sliders to Pit -521, Yaw -1213. This was with PSAMS at 200V. There is still loads of range on the sliders, DAC counts up to 27,000 out of 500,000.
We watched the beam and ramped PSAMS from 200V to 0V over 30s, the beam may have moved slightly higher.
Leaving both ZM4 and ZM5 PSAMS at 0V for tomorrows work.
ZM4 has a 16bit DAC and hence we will need to mechanically relieve it in both pitch and yaw.
For the ZM4-5-6 alignment check after offloading PSAMS on ZM4 (75677) and ZM5 (75709) -- reminder that as-is, ZM6 is almost railed. Ideally none of ZM 4-5-6 are saturating.
So, before mechanically offloading ZM 4-5, can also check alignments with ZM6 sliders set ~0. For example, we brainstormed next steps like:
(i) use ZM5 sliders to center ZM4-5 alignment on HAM7 irises. SQZ beam should then naturally hit AS_C.
(ii) zero the ZM6 sliders, then use ZM4-5 sliders to recover the beam on AS_C. Then could offload if needed.
Summary:
OMC DCPD/QPDs/PZTs are good without caveat for the first time in LHO history.
OM2 heater and thermistors are good.
ASC-AS_C has a grounding issue which should be fixed in chamber at some point.
Didn't check grounding of the beam diverter and picos (confirmed that picos move, didn't test BDV).
For flange layout, see D1002877 (but note that LHO uses D6-F4 for OMCR diode, not D6-F6).
For in-air wiring, see D2200215 (OMC DCPD), D1300589 (OMC PZTs), D1002283 (OMC QPDs, OMCR DCPD also uses one channel of the QPD interface), D2000212 (T-SAMS heater/thermistor).
New OMC seems to have eliminated the source of headaches in the past.
The new OMC (1st attachment left) has a PEEK connector bracket on top of the OMC breadboard instead of an aluminum bracket (1st attachment right). In the past this aluminum bracket caused many, many headaches. Now that it's gone, OMC DCPD/QPD/PZT chain makes sense w/o caveat.
D6-F1 (DCPD/Preamp)
At the feedthgough, I disconnected the D6-F1 DB25 (for OMC DCPD/Preamp) and used a breakoutboard on the feedthrough to check grounding. No pin including pin13 (that is used for shield) is connected to the chamber. Pin 13 is only connected to signal GND pins of the in-vac preamp (pin 10/15/16/19/20/23).
Inside the chamber on the in-vac preamp, the DB25 shell is connected to the preamp body (which is isolated from the ISI via PEEK spacer). At first DB25 shell and the preamp body was shorted to the ISI table, but this turns out to be via 3MHz cable ultimately connected to the in-air chassis. As soon as both of the 3MHz cables were discunnected from the in-air chassis, preamp body as well as the DB25 shell weren't conducting to the ISI table any more.
D6-F1 and 3MHz connection.
D6-F2 (PZT)
Disconnected D6-F2 (PZTs) at the feedthrough, used a breakout board. Discharged the PZTs. Measured capacitance: HZ PZT (pin1-14) was 373nF, LV PZT (pin2-15) 392nF, these include in-chamber cables. Nominally these are 380nF and the measured numbers are good.
Pin 13 is not connected to any pins nor the chamber. No short circuiting between LV and HV path.
Restored D6-F2 connection.
D6-F3 (QPDs)
Disconnected D6-F3 (OMC QPDs) at the feedthrough, used a breakout board.
Pin 13 is not connected to any pins nor chamber. Diode connection from QPD1 anode 1/2/3/4 (pin 15/2/14/1) to QPD1 cathode (pin 16). Diode connection from QPD2 anode 1/2/3/4 (pin 18/5/17/4) to QPD cathode (pin 19). No connection from QPD1 to QPD2 and vice versa.
Restored D6-F3.
OMCR diode is good
Disconnected D6-F4 to check. Pin 13 is not connected to chamber nor any pins. Restored D6-F4.
ASC-AS_C has a grounding issue
Disconnected D6-F5 to check. Pin 13 is connected to the chamber. Restored D6-F5.
T-SAMS heater/thermistors are good
Disconnected D6-F9 to check.
Pin 13 is not connected to chamber nor any pins.
Pin 1-14 (heater) is 104 Ohm, which is good.
Pin 11-24 (thermistor 2) and pin 12-25 were both 11.7kOhm, sounds about right. No cross-connection between thermistor 1 and 2.
Things that weren't checked
Will check grounding:
Pico (checked that both WFSA and B pico moved).
WFS (DC).
Suspensions. Will leave it to Fil.
Won't recheck grounding:
Beam diverter (will check that it moves). Known in-chamber grounding, this was dealt with in air in the past, no reason it changed.
WFS (RF, interface). Coax, no reason to worry.
DCPD 3MHz. Coax, no reason to worry.
Tagging with EPO for OMC mass comparison.
Added later: WFS (DC), Picos, and Fast Shutter are good.
D6-F7 (pico):
See D1100326 for pin connections. Disconnected the DB25 at the feedthrough and used a breakout board.
No pin (incl. pin 13) is connected to the chamber ground. Pin 13 is not connected to any other pins.
WFSA and WFSB DC:
See D1300467 for pin connections. These are on D3-2C1 and 2C2, but they're almost impossible to access, so I disconnected the DB15 from the front panel of the WFS interface, attached DB15 breakout board to the cable and checked. (Note that they use special DB25-DB15 cable to make a connection between the feedthrough and the interface.)
For both of the cables, DB15 connector shell is only connected to pin 14 and 15 (signal ground for in-vac WFS board), not connected to the rack ground.
Fast Shutter:
See D1400225 for pin connections. This is on D3-3 but it's almost impossible to access, so I disabled the HV for the FS driver, disconnected the 6-pin HV connector from the front panel and checked the connection betweein the cable pins.
No pin is connected to the rack ground. No cross connection between positive drive, negative drive and continuity check pins.
Today's activities: - EX pumpdown continues. The pressure is in the mid-E-7s already, after ~37 hours of pumping. - EX was also leak checked: the newly installed 12" blank on BSC5; the new RGA angle valve; and the dismounted and re-mounted 3 viewports were leak-checked, and all passed nicely: see it more in-detail in the comments - At EX the last thing to do is the RGA bakeout, which will be started on next Monday - From BSC8 all the 12" 3IFO feedthroughs were removed, and they were replaced with blanks (5 pcs. of them). The removal of the particularly awkwardly placed 16.5" feedthroughs has been started (there are 3 of them). - The purge air dew point was measured in the LVEA, and found satisfactory (~-42 deg C) - see more in-detail in the comments
Helium leak detector was connected to the foreline of the main turbopump at EX, and five new flanges (listed above) were sprayed with helium. No helium signature observed above the leak detector background of ~4E-10 Torr-l/s. Foreline was switched back to the local scroll pump to continue pumpdown.
Today's dew point measurement in the LVEA attached, -42.2degC at the output tube prior to in-chamber activities
Not a complete & thorough photo close out since we only had one door removed for HAM3, but tried to take as many photos as possible (last photos I have were from 2017 for HAM3!). Here's the link on Box:
Here is a folder with photos and videos of IMC Baffle work from Jan 31, 2024 (with Tony, Mitch, Robert, and Corey):
Camille (CIT), Austin , Rahul
This morning we went to HAM7 chamber and changed the preload on ZM4 (P-SAMS) suspension as per the document E2300463_V1. This changed the RoC of ZM4 mirror without the PZT actuation. Given below are the details of our work - Camille will add pictures later on.
- After setting ZM4 into SAFE state we locked all three stages of the suspension. We had already taken healthy TF measurements before starting our work.
- The bottom mass cable was disconnected and carefully re-routed so that it stays away from the fixture plate.
- four add-on masses (basically 1/4-20 screws with washers) attached to the bottom mass was then removed.
- bottom mass Fixture plate (D2100121) was attached to the structure using six 8-32 screws.
- The bottom mass (already locked using EQ stops) was then further clamped using four 1/4-20 screws through the fixture plate. We had to adjust the height of the bottom mass to the align the threads with the holes on the fixture plate.
- Once the bottom mass was securely clamped, we removed the three set screws on the preloader.
- Using a torque wrench we increased the preload on the bottom mass by ~29 in.lb. (Total preload from torque after increase was 75 in.lb).
- We then followed all the above steps backwards (i.e set screws, add on mass put back, fixture plate removed, cable re-connected and the suspension set free).
- Once all done, we started damping the suspension and checked for any BOSEM flag changes - looked all fine.
- We took the transfer function measurements and ZM4 looked healthy.
Hence we took all the tools out and put the curtains back on HAM7 chamber.
Next, we will go into laser hazard with SQZ team and check for any changes in beam alignment and make adjustments as required.
1st image: PSAMS locked in place with EQ stops. 2nd image: PSAMS locked with bottom mass fixture plate. 3rd image: Removal of set screws. 4th image: Preload adjustment with torque wrench. 5th image: Preload adjustment with torque wrench. 6th image: Torque wrench dial with the blue needle showing the total torque on the preloader (75 in lbs.)
Excellent!
ZM5 offloaded as well, see LHO alog 75709.
J. Oberling, R. Crouch, T. Guidry
Update on FARO progress so far. Warning, incoming wall of text.
There have been issues accurately aligning to the LHO global coordinate system to the accuracy necessary for IAS work, specifically in getting good alignment to the global Z axis. This is somewhat of a repeat of the struggles when prepping the FARO for the FCT (Filter Cavity Tube) install work; while we were able to get an alignment good enough to be well within the FCT installation tolerances, the tolerances for optic alignment are more stringent (+/-1.0 mm positional tolerance) so we have to get a better alignment to our global coordinate system. To date we have worked in 2 areas: aligning to the global coordinate system, and accurately moving the FARO around the West Bay. For reference, monument name and coordinate information can be found on the DCC at D1100291.
Global Coordinate System Alignment
To start, we began by following our WIP procedure for global coordinate alignment. Part of this is to refine said procedure, since I quickly threw this document together (almost 2 years ago now) after a phone call with PolyWorks tech support; we now have a red lined copy that I will use to update the WIP procedure. Due to line of sight issues and monument shape (BTVE monuments are domes, not flat; direct line of sight to PSI-6 is blocked) we use a sphere fit rod to probe the monuments (place the point of the rod in the monument punch and trace out a sphere as best we can while keeping the rod point firmly in the punch (the monument punch limits how much of a sphere we can trace, and therefore the accuracy of Polyworks' sphere fit); the Polyworks software then fits the data to a sphere). In this way we can enter the coordinates of our alignment monuments as the center point of a sphere, then use the sphere fit rod to probe the monument (useful for ones that are out of direct line of sight, like PSI-6, or ones that are not flat, like BTVE-1). We have 2 sizes of sphere fit rod, a 3" and a 5". We first used the 5" rod, as it's the same we used for FCT install setup, and the results of that alignment are shown in the 1st picture. As can be seen, not very good (one can ignore the diameter measurement on this picture and all the ones that follow, the error there is a result of the limited sphere shape we can trace with the sphere fit rod; PolyWorks told us back in 2022 that the alignment algorithms do no consider this data, only X, Y, and Z). We then used the 3" rod and repeated the alignment procedure, results shown in the 2nd picture. This is seemingly a good bit better, but the issues arise when we then try to measure a known monument. Unfortunately, due to a lack of known monuments in the LVEA West Bay, we don't have any independent monuments we can measure against that have an associated Z axis coordinate, so we have to use the same monuments we use to perform the alignment (i.e. BTVE-1, PSI-1, PSI-2, and PSI-6). In addition, we can't use PSI-6 (located in the biergarten), because the SUS electronics rack closest to WBSC2 sits directly over it and blocks direct line of sight (we can see it when using a sphere fit rod, but not with a regular SMR nest). When looking at the 3 available monuments we have, the FARO reports their coordinates as ~1.5mm higher than our documentation says they are; this is consistent across all 3 monuments, indicating a systemic error somewhere (or maybe the documentation is wrong?). X and Y are accurate to <0.1 mm across all monuments measured.
This launched us on trying to find this 1.5mm error. The first thing we tried is reading up on PolyWorks' alignment algorithms to see if there's something in the setup we're missing (PolyWorks' included reference guide is a wealth of information on the software). From this we learned that the alignment algorithms are updateable after the fact (including adding and removing alignment features/monuments), and the software will then apply that update across all alignments in the project. This includes adding and removing alignment targets on the fly, and changing how the routine considers the available data (weighting different monuments over others, which axes to use, etc.). Part of our alignment procedure is to first align to X, Y, and axis tilt, then perform another alignment routine to align to the Z axis. We noticed that the portion of the alignment routine that aligns to X, Y, and tilt was also considering Z, when it shouldn't be; the portion that aligned to Z was considering X and Y when it shouldn't be. We can make these corrections on the fly, without having to re-measure anything, so we did. The update changed the X and Y axis deviations, but caused no change in the Z axis deviations; the results of this correction are shown in the 3rd picture. The X deviation for PSI-2 got a little worse but improved for the other 3 monuments, Y is practically the same across all 4, and Z was unchanged as expected. But we still see the +1.5mm Z axis error when directly measuring these monuments (X and Y remain accurate to <0.1mm).
The next thing we considered is the difference between the monument surface and the monument punch. The sphere fit rod measures to the point of the rod, which sits at the bottom of the punch while we use it to probe the monument location. However, the Z axis coordinate for these monuments is registered to the surface of the monument, not the bottom of the punch. Therefore in this setup the FARO is actually measuring the bottom of the punch, which then adds error to the coordinate system alignment. Using our Center Punch Nest (an SMR nest with an included punch for marking monuments, abbreviated CPN from here on out) and a depth gauge we measured the difference between the monument surface and the bottom of the punch for each of our 4 alignment monuments (the punch portion of the nest only depresses as far as the punch can go, so we can measure the difference between the surface and the monument punch based on how far the nest punch can travel). The results, assuming the surface of the monument is 0:
This means that when we use a sphere fit rod to probe these monuments we have to correct the global coordinate by the above amounts so we're measuring the correct point on the monument. For example, the global Z axis coordiante for BTVE-1 is -1057.2mm, but when using a sphere fit rod we need to enter the corrected coordinate of -1058.0mm (-1057.2 - 0.8) into PolyWorks.
Tyler suggested we also check the local difference in the Z axis between our alignment monuments, using BTVE-1 as the origin. We have a local coordinate survey from the late 90s for the PSI and BTVE monuments in the LVEA (the last time this was done); this data is available at D970210 in the file Rogers_LHO_PSIMonumentsAs-Built.pdf on page 2, and again in D1100291 in the file LHO_PSI_Monument_Z_Corr_MEZ220406a.xlsx, in Column C. We used the FARO to check this, using a blank project so the FARO was not aligned to our global coordinate system. Setup again in the West Bay in the same position we've been using to probe our alignment monuments, we oriented the FARO to local gravity (the FARO levels and then orients itself to the local gravity at its current location), then used an SMR with our CPN set over each monument punch to measure the difference in Z for each monument (deltaZPSI-X = ZBTVE - ZPSI-X); we're essentially using the FARO as an autolevel to perform a differential height survey. Since we don't have direct line of sight to PSI-6 we set the CPN roughly inline with PSI-6 in X but set against the SUS rack so the FARO can see it (roughly 300mm +Y from the monument); this put the SMR on the vinyl floor, which we measured to be ~2mm thick using a set of calipers. This could add some error, as we're not directly over PSI-6 and therefore cannot account for any height difference between our location and the monument (such as variations in the surface height of the concrete), but it's the best we have given our line of sight restrictions (the West Bay is crowded, but it's the only place where we have a collection of monuments with a registered Z axis coordinate). Results and deltaZ from the old Rogers survey, all units in mm:
| Rogers As-Built Survey, 1997 | FARO, 2024 | Difference between Rogers/FARO | |
| deltaZPSI-1 | -826.3 | -825.1 | +1.2 |
| deltaZPSI-2 | -827.5 | -826.4 | +1.1 |
| deltaZPSI-6 | -822.4 | -821.0 | +1.4 |
So the FARO indicates that the Rogers As-Built survey from 1997 was not correct, so we adjusted the global Z axis coordinates for our 3 PSI monuments using the above FARO data. We then further adjusted the Z axis coordinates using the difference between the punch depth and the monument surface. This gives us the following global Z axis coordinates for our alignment monuments, all units in mm:
| New global Z using FARO height | Global Z for bottom of monument punch | |
| BTVE-1 | -1057.2 (unchanged) | -1058.0 |
| PSI-1 | -1880.8 | -1881.9 |
| PSI-2 | -1877.7 | -1878.4 |
| PSI-6 | -1876.2 | -1876.8 |
We then used these new global Z axis coordinates for the bottom of the monument punch to align the FARO to our global coordinate system, results shown in the 4th picture. We created points based on the global Z of the monuments themselves, and performed a Build/Inspect operation to get our deviations in X, Y, and Z (again using the CPN to place the SMR over the monument punch; the CPN registers to the monument surface); these results are shown in the final picture. As can be seen, the reported X and Y axis measurements are good to better than 0.05mm, but we still have some significant error in Z. It's much better than the ~1.5mm we were seeing previously, but nowhere near as good as X and Y.
We also noticed from the FARO's position that we could see height monument 903 (information in T1100187); this height mark is registered to the local LVEA coordinate system, and is on a metal post. Using a autolevel we placed a temporary magnetic SMR nest in line with the height mark. From this we could get X and Y coordinates for a spot very close, but not exactly on, the height mark (X is right on it, but Y is roughly 1" +Y). With these X and Y coordinates we can transform the registered local Z coordinate to a global one (see T0900340) and compare to what the FARO says (the ~1" offset in Y is not an issue, as the Y axis tilt is very small at 12.5µrad, which causes a 0.3µm error in the global Z (yes, that's micrometers)). We did this very quickly with a cell phone calculator, and did not get a screenshot or picture of the results (my fault), but the FARO thinks that height mark 903 is ~4.2mm higher than we would expect after converting its local Z to a global Z. We have no other height marks we can place a nest by to do this same measurement, so we currently have no way to know if this error is in the height mark itself or something with the FARO (or a combo of the 2). Will have to move the FARO around (which we can do accurately, see next section) to find something else to look at.
What's causing this error? At this point in time we are not sure. Some thoughts:
Moving FARO
We were able to move the FARO into the biergarten area using a collection of glued nests (set during FCT install) and magnetic nests. This was done independently of our gloabl coordinate alignment work. We were aligned to our global coordinate system (although we're still questioning the accuracy), but only looking at how accurately we could move the FARO (device target deviations between moves and device positional uncertainty at each location), which does not depend on being accurately aligned to any set coordinate system. When doing a move you want a minimum of 3 targets, but PolyWorks support has repeatedly told us that you really want at least 6. While the software will use 3, using 6 or more greatly increases the accuracy of the move. We were able to use roughly 8 targets to move into the biergarten area and back out near the Test Stand. In total we did 3 device moves for a total of 4 device positions: position 1 at our intial setup point, position 2 closer to the FCT to have better line of sight into the biergarten, position 3 in the biergarten area but outside of the cleanroom, and position 4 back in the West Bay near the test stand. The largest target deviation we saw between device positions was ~0.2mm. In addition, PolyWorks has a routine to calculate the positional uncertainty of the FARO. This routine reported a positional uncertainty of <0.05mm for each device position, indicating that we can accuratly move the FARO around. This was good to confirm, as we're going to have to move the FARO around the LVEA to find other monuments with known global Z axis coordinates to test our global coordinate system alignment.
Next Steps
Outstanding progress, agree the discrepancies are puzzling. I might suggest picking up the factory scribe lines on BSC, manifold and gate valve large flanges, if you can see them (might need a water hose level between the sides to correct for clocking). True, these will have cumulative installation error (spec potentially ± 2mm radially, though recall none that bad). And they could just as well be referred to faulty historic survey (!) But, at the end of the day, we may want to just follow the chambers anyway, wherever they have wandered...
Yesterday, Ryan and I went out and tried a couple of things. First, I used the 3" sphere fit rod to probe the monuments in a test of how much probing technique could potentially change the alignment results. Turns out, a good bit. We changed nothing in our alignment procedure except I probed the alignment monuments using the 3" sphere fit rod while Ryan drove the computer. The results of the alignment routine and the subsequent Build/Inspect on our monuments are shown in the first two pictures. As can be seen, a good bit different from our previous attempt with Ryan probing the monuments. While not surprising, this shows that probing technique with the sphere fit rod potentially has a large effect on the accuracy of the alignment.
We next repeated this process, except we changed monuments PSI-1 and PSI-2 from spheres to points. We can only do this for these 2 monuments, as the top of BTVE-1 is dome shaped and we do not have direct line of sight to PSI-6. We had to offset the Z axis coordinate for PSI-1 and PSI-2 by +50.8mm to account for the CPN we used to probe these monuments, hence the diffferent Z axis coordinates (the software does not automatically compensate for the nest offset when doing a simple probe operation, but it does do this compensation with a Build/Inspect operation). Nothing else in the process changed. Results are shown in the final 2 pictures. As can be seen, some alignment deviations became worse and some became better, but the Build/Inspect results were all better across the board (but still not within the aLIGO monument placement tolerance of +/- 0.2mm).
What does this mean? As stated previously, due to the lack of known monuments in the West Bay and lack of line of sight to other known monuments we currently can't tell if this error is in the FARO setup or in our monument coordinates. But what this does tell me is that we need to get away from using the sphere fit rods as much as we can. This won't be possible for BTVE-1 due to its dome shape, but I think we can do this for PSI-6. The PolyWorks alignment routines are updatable on the fly and after the fact (meaning we can add an alignment monument to the routine after we've already performed said alignment routine). From reading the reference guide, it seems to me that we could use BTVE-1, PSI-1, and PSI-2 to do an initial alignment to the global coordinate system, move the FARO to a location with direct line of sight to PSI-6, then probe PSI-6 as a point instead of a sphere and add it to the alignment routine; it's our hope that this allows us to get a more accurate shot at PSI-6 and therefore a better alignment to our global coordiante system. This is the next thing we want to test, and will also look into Mike's suggestion of the chamber door flange scribes (these can be a little difficult, as the blue HEPI support piers make the line of sight to these scribes pretty narrow). The ultimate goal here is to get a good alignment for the FARO and then map out the LVEA monuments, adding more where and when we need to; the hope is that we can then use those monuments to align the FARO from anywhere in the LVEA without having to constantly resort to this intial alignment routine (and therefore getting away from using the sphere fit rods entirely).
Another potential issue we noticed, is there is now a running clean room next to our FARO setup, set over the mechanical test stand (to be used, I think, for sorting 3IFO SUS parts from a large ISI storage container into individual SUS storage containers). Proper coordination was done in advance and we didn't expect this to be an issue, but this week we have had problems probing monument PSI-6 that we did not have in the prior 2 weeks. While it's not confirmed the clean room is the cause, air temperature gradients and air currents can affect the accuracy of the FARO so this could also be influencing our results. Will also try doing these alignment tests with the clean room off and see if we get better results.