Patrick upgraded the EX HEPI Pump Controller system this week, which resulted in a name change for its EPICS channels and an EDC disconnect count of 276. For the long weekend I've added these missing channels to the edc_green_ioc which has greened up the EDC and removed the disconnect count alarm. Next Tuesday we will restart the DAQ with the latest H1EPICS_HEPIPUMPEX.ini file to trend the new channels.
-Flexures installed SN 21, SN 22, they have survived throughout the day (I haven't unlocked the CRS since moving to the table, but visually they look fine)
- I re-balanced the CRS so there is now a new distribution of masses on the proof mass
-The CRS is semi-bolted on the table, we haven't put any dog clamps down, but there is one place where the CRS can be bolted directly into the table
-Temperaraly put baffles on, on baffle SN 001 had to remove one of the bolts to fit it around a pre-existing optic on the table
-Fil, Mitchell and I got the out of vacuum fiber all cabled up, however, later in the day when we tested the laser power at each point of the chain, it looked like light wasn't making it through the fiber. We have been using this fiber for testing chamberside so if it's an issue with the fiber it started today.
-We turned on the laser briefly to look at the power at each point along the chain:
OUT OF LASER: 20.5mW
OUT OF VAC FIBER: 7um
Which means there's either a issue with the 27m out of vac fiber, or the connector between the laser and the fiber
The plan for Monday is to first switch out the connector and hope that was the issue. If that doesn't fix it, I'll look for another temperary fiber to use to at least get the HoQIs aligned and deal with the broken fiber later.
TITLE: 07/02 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
LVEA is Now Laser Hazard!
BSC2 Bolts are now on!
VAC team is getting ready to close up BSC2.
ITMS ISI's are balanced
ITMY Hardware watchdog trip immenant 19:09:00 UTC
ITMY Hardware watchdog trip 19:12:59 UTC
HEPI pump at EX alarmed after Fil told me he was gonna Fiddle around with it at EX.
Vacuum at EX was taken down by Fil's EX HEPI work the same way as yesterday's EY HEPI, VAC Power glitch issue.
CRS team is still inside HAM3.
End X is now Laser Safe again and the TCS team is heading back to the corner.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 15:20 | OPS | TJ | CR | n | Reservation test | 15:48 |
| 15:30 | JOT | Camilla | Prep LAB | n | Jack of all trades work | 16:30 |
| 15:31 | FAC | Kim | LVEA | N | Technical cleaning and resupply | 17:58 |
| 15:51 | PCAL | Tony | PCAL lab | y | checking on meas. | 15:51 |
| 16:02 | FAC | Tyler | PrepLab | N | Drilling Holes in the Jot Lab | 16:47 |
| 16:23 | CPS | Jim | LVEA HAM3 | N | CPS Install work | 20:08 |
| 16:47 | VAC | Gerardo | LVEA | N | Working on CP1 and other VAC stuff | 19:47 |
| 16:54 | VAC | Jordan & Travis | LVEA | n | taking down AUX carts from HAM1&2 Anualus | 17:28 |
| 16:56 | CHEETA | Camilla | PREP Lab | N | First contacting ZnSe | 17:58 |
| 16:59 | Safety | Mc Carthy + 3 | Roof | N | Firelook out and other Roof viewing. | 17:31 |
| 17:02 | CRS | Shoshana | LVEA HAM3 | N | Installing CRS | 20:08 |
| 17:13 | SEI | Jim | LVEA | N | BSC1 and 3 New balance! | 20:13 |
| 17:17 | PEM | Robert, Shrey, Carlos | End X | N | PEM work | 18:58 |
| 17:47 | IFO | Betsy | LVEA | n | Coordinating with crews on the LVEA floor & walk about | 00:09 |
| 18:07 | BCS | TJ | LVEA | N | balanceing the BSCs | 20:31 |
| 18:55 | TCS | Camilla | PREP Lab | N | First contact ZnSe | 19:09 |
| 20:07 | VAC | Jordan & Gerardo | LVEA HAM2 | N | Checking View ports. | 21:07 |
| 20:15 | VAC | Travis | LVEA | N | BSC2 dome Bolts! | 22:41 |
| 20:15 | CPS | Mitchell | LVEA HAM3 | N | Installing CPS | 20:48 |
| 20:19 | EE | Fil | EX | N | HEPI Beckhoff | 22:19 |
| 20:29 | PEM | Robert | LVEA HAM3 | N | Baffling work | 00:39 |
| 20:35 | PEM | Ibriham | LVEA | N | Cleaning up first contact | 21:57 |
| 21:08 | SUS | Rahul | Output arm | N | Measurements on ZM5 | 21:59 |
| 21:11 | OMC | Disha & Keita | LVEA HAM6 | N | making measurements. | 22:00 |
| 21:15 | Cheeta | Camilla | Prep lab | N | First contacting | 23:15 |
| 21:17 | Safe tea | Richard Gerardo | LVEA | N | Checking on some safety Items. | 21:27 |
| 21:22 | SEI | TJ & Jim | LVEA BSC3 | N | Balancing ISI's and shaking SUS ITMX | 23:22 |
| 21:28 | CPS | Mitchell | LVEA HAM3 | N | Installing CPS | 23:20 |
| 22:36 | VAC | Jordan & Gerado | LVEA | N | Setting up annulus pump | 22:41 |
| 22:37 | TCS | Camilia Madie | EX | yes | Working on Hartmann | 00:42 |
| 22:57 | CRS | Shoshana | LVEA | n | quick in and out to push buttons | 23:12 |
| 23:08 | VAC | Jordan | LVEA | N | Parts hunt | 23:14 |
| 23:36 | CRS | Shoshana | LVEA | Yes | CRS work | 00:36 |
The bolts for the BSC2 dome were torqued. The annulus system is being pumped by a small turbo and the tiny pump station which is up on the E-module.
While I was up there, I also replaced a gasket and torqued a 4.5" blank on the gauge adapter ports metal-to-metal. The blank was very gappy, so we wanted to eliminate the possibllity of any leaks. See pics for before and after. Yet another flange that will need to be leak tested.
I took a transfer function measurement yesterday in the early afternoon actuating in P and plotted P2P and P2Y to see the state of our P2Y cross coupling. It looks like swapping out the F3 QOSEM a couple days ago resulted in a bit less P to Y cross coupling? I will be having another go at P to Y measurements (as well as Y to P) once BSC2 is quiet, but results as of now seem to indicate that the P to Y cross coupling has gone down by an order of magnitude since last week.
We will mostly be focusing on the P to Y plots
The last P2Y comparison we did (in green) was from measurements taken on 06/25/2026 (90753). Between that measurement and the second measurement (in blue) taken July 1st at 19:47 UTC, the only change we had made was swapping out the F3 QOSEM since the coil pins were grounding to the chamber (90834). Comparing these two measurements, even if we just look at the frequencies where the coherence is good for the second measurement, it seems that the second measurement is over an order of magnitude lower than it was last week (same excitation and amplitude).
Then we went in and aligned QOSEMs in the afternoon, and afterwards (July 1st at 23:51 UTC) I took another measurement with 10 averages instead of the previous 5 to try and get better coherence, but the coherence ended up worse in most places. I'm not exactly sure why this is the case here. Having trouble with coherence is partially a sign that there is just less cross coupling, but also it would obviously be good to have better coherence. The few places where the coherence is okay though seems to corroborate with the magnitude of the second measurement. The P to P TFs for all three measurements still match and look great.
This morning Tyler secured the two CHETA tables to their frames with corner brackets and #10 self tapping screws, as LLO did in 80840. Two brackets on each table, perpendicular to each other. Photo attached.
The brackets are slotted so the height of the table can be adjusted if needed.
(Randy, Jordan, Travis, Jake, Owen, Gerardo)
Late entry, activities took place yestereday. Installation was a bit harder than anticipated.
Stuck walking plate
We removed a couple of the walking plates, then when trying to remove the third plate, it got stuck, the plate was wedged between 3 hard places and the chamber, we used a pry bar to get it unstuck and out of there.
Bad Inner O-ring
We inspected both of the BSC O-rings, outer and inner, the outer O-ring is in good condition, however the inner O-ring was not, it had chaffing/scuffing on several locations and of large lengths along the sealing surface, and since it was not going to seal we decided to remove it. When removing the O-ring, it left strings of O-ring behind on the sealing surface, and after completely removing the O-ring it was time for elbow grease (only compatible vacuum grease) and lab q-tips to the rescue that Jordan found, with IPA and lots of rubbing and a Travis hack, we manage to clear the debris left behind. A new O-ring was installed without issues and it stayed put to set the dome on.
Dome installation
The easy part, setting the dome on top of the chamber went on with no issues, currently the dome has a total of 6 bolts, we will get back to it as soon as we can.
T1200131 Grounding and Shielding at LIGO
D2300383 SUS BSC2 HAM3 HAM4 (susb2h34) System Wiring Diagrams
A summary of closeout activities for BSC2 and HAM3:
BBSS OSEM Cable
TOP F1, F2 BS_081
TOP F3, SD BS_082
TOP LF, RT BS_083
Middle UL, LL, UR, LR BS_084
Bottom UL, LL, UR, LR BS_384
Issue: Pin 10 on cable BS_082 grounded to chamber ground, QOSEM replaced alog 90834.
PR2 OSEM Cable
TOP F3, LF, RT, SD HAM3_003
Middle UL, LL, UR, LR HAM3_025
Bottom UL, LL, UR, LR HAM3_026
Issue: Pin 13 on cable HAM3_025 grounded to chamber ground. Found cable shield grounding to backshell of air-cable on feedthrough side. Cable jacket had pulled back. Reassembled the backshell. As precaution cable HAM3_026 was also reassembled.
MC2 OSEM Cable
TOP F1, F2, F3, LF HAM3_001
TOP RT, SD / PR2 F1, F2 HAM3_002
Middle UL, LL, UR, LR HAM3_019
Bottom UL, LL, UR, LR HAM3_020
Issue: Cables 19 and 20 had pin 13 grounded to chamber ground. Jim was able to move cables inside chamber to clear shorts. Old style cables with the shield protruding out.
All cable issues resolved. All pins are isolated from chamber ground and pin13 is tied to backshell.
ECR E2200043
A RIB2401D relay was installed at EY for monitoring the HEPI reservoir level on 7/1/2026. The same scheme is used in the corner station. The RIB2401D relay is enabled by the reservoir level sensor. The outputs of the RIB2401D will be used to enable the motor control panel and status readback signal of the level sensor. The EL1094 terminal was replaced with EL1004.
While installing the new RIB2401D relay we glitched the 24V. This caused the Vacuum Beckhoff computer to reboot. See alog 90866.
D. Barker, F. Clara, P. Thomas, J. Vanosky
Same work completed at EX. Vacuum Beckhoff computer glitched, same as EY.
[Jim, Shoshana]
Yesterday when I went to put the cover on the CRS to get it ready to move to the clean area right next to HAM3, I noticed one of the flexures (SN 15) was broken [picture attached]. It's unclear how this flexure broke as it had been locked since last Wednesday (?), and it is strange that only one flexure broke.
We decided that it would be better to install a new pair of flexures and re-suspend next to the chamber rather than in the temporary clean room to reduce the risk of them breaking again. So today we wheeled the table the CRS is on to the space next to HAM3 and I re-suspended the CRS there and roughly balanced it.
Following the procedure outlined in E2600210 and work permit 13356, we moved the CRS to the table and lined everything up so that the CRS baseplate can be bolted directly to the table in one spot.
We installed the fiber feedthrough, and dealt with all the cabling (fiber and DB25) that required Jim to be physically inside the chamber and we'll install the rest of the cable clamps which we can reach from outside the chamber tomorrow and finish connecting all the cables and dog clamping the CRS down (hopefully)
[Betsy, Oli, Ibrahim, Elenna, with online help from Arnaud, Marie and Gabriele]
Today we began by attempting to follow the same steps that LLO did to decouple pitch and yaw, as described in 81817. To summarize, they applied a length offset and adjusted coil driver gains to ensure the same amount of motion is sensed on M0 F2 and F3 oseminfs.
Betsy and I immediately found that following that same process was not going to work. As a reminder, Ibrahim and Oli swapped the F3 osem yesterday due to ground loops, 90838. To get straight to the point, here are some results:
Arnaud notes that overall this is an improvement, because last week the P2Y cross coupling was much worse, roughly 1x pitch to 2x yaw. The overall numbers are different depending on which sensor you trust. However, Betsy and I think that the top mass drive versus sensed motion (master outs versus oseminfs) should be relatively straightforward. It seems like we have a mechanical imbalance on the suspension. However, the improvement that has occured was only due to swapping an osem, which seems electrical.
Oli will revisit the derivation of the osem2eul/eul2osem matrices. We also plan to recheck the suspension transfer functions to see if the P2Y coupling is reduced.
Last week's measurement showing worse P2Y coupling than in this alog: 90739
ndscope-test can now show "scatter" plots.
Plot one channel against others. Each plot can have one channel giving the X value, and any number of channels giving Y values. The plot will show one trace per Y value channel using the color of that channel.
Create a scatter plot from the command line by running "ndscope-test --scatter <x-channel> <y-channel-1> <y-channel-2> ..."
Create a scatter plot from a time domain plot.
1. Right click to get the pop up menu.
2. Select configure channels.
3. Select at least two of the channel names in the window with Control + click or Shift + click. The first selected channel is always the X channel
4. Press the Add Scatter Plot button at the bottom of the screen.
5. Press the OK button.
The timespan of the traces matches the time span of the traditional time-domain plots. Pan and zoom a time domain plot to
change how much is shown on the scatter plot.
WARNING: This is a development release.
There may be bugs.
Some bits are not working for scatter plots. For example, the configure channels window does not appear for these plots.
Some needed interface is not yet included. There's no way to change the X channel for a scatter plot yet, other than to
open a new window and add the new X channel to the command line. Scatter plots cannot be saved to or configured in yaml files. Many more bits aren't done.
Thank you Erik, this is going to be a useful feature for the CRS commissioning.
I tested it with the following channels and confirmed that it works well (looking back in time when the CRS was online) :
ndscope-test --scatter H1:ISI-HAM3_CRSRY_HOQI1_QUAD1_OUT_DQ H1:ISI-HAM3_CRSRY_HOQI1_QUAD2_OUT_DQ
The only feature request that I have is to set the X-Y to the same dimensions (or force the figure to be a square). In our application, we are evaluating how circular is the scatter plot, so having the X-Y different dimensions distorts the circle to an ellipse. For the same reasons, we would always set both axis limits to the same values, so having a way to do this quickly would be helpful.
(Jordan, Gerardo)
We inspected the 5 viewports on the west door of HAM2.
We found on viewport A1F4 the typical smudge or print left by first contact the print appears to be on the inside, but not the vacuum side (this VP has two windwos). We also noted a scratch on the outside window (not under vacuum), around 1 O'clock and about 3/4" away from the edge, we contacted Keita who was walking by the area and we asked him if the location of the smude/scratch were on the path of beam, no they are not. BTW, VP4 is a high quality wedged viewport, a double window, type D1101714.
Then on A1F2 ZV-800 viewport we noted some scratches, something was dancing on the window, since it appears as a single scratch with multiple turns. This viewport was removed and replaced with a spare ZV-800 type. SN of new unit is 0098, old scratched and full of particulate viewport serial number 63.
All other viewports nothing to report, A1F1, A1F3, A1F5.
(Jordan, Gerardo)
Both viewports were removed to get a closer look on the bench, both have several scratches on both surfaces (vacuum side and air side), we are trying to quantify the defects. More on the inspection on the next couple of days. Locations of viewports are A2F1 and A2F4. The rest of the ports have blanks.
Pictures of the A2F1 (ZV800 SN 80 Uncoated) and A2F4 (ZV-800 SN81 Uncoated) viewports on HAM2 for reference. Full inspection report will be made and posted to the DCC now that the viewports are removed. We are evaluating potential replacements.
Jennie W, Jeff K, Josh F, TJ S,
Summary: SPI interferometers aligned, shroud installed successfully. One stray beam and possible clipping on shroud to investigate/deal with but otherwise all problems were solved. Obligatory success photo taken by Josh.
Today we:
More details regarding the baffle installation:
When placing the below table baffle brackets, there was a ballast mass baffle (D1700262) that was blocking the angle bracket for the furthest -Y bracket. The bracket could not slide under the ballast mass baffle (bmb), so we decided to move the bmb in the +Y direction a few inches and I had to loosen the baffle panel within the feet to slide it up a few mm and then reclamp. This allowed the bracket to slide under the baffle just to the side of the feet, but the move partially exposed a corner of the shiny ballast mass stack.
The lower baffle shroud that covers the breadboard needed the fiber spools to be moved. We moved them over one set of bolt holes, but they are quite close to chamber edge, I'd guess around 1/2". Jeff then centered the two aperatures to the SPI beam, and we called it good. We still need to B&K the whole area.
Just did an 8 hour trend of the fiber power monitor channels for REF and MEAS channels (left two plots) and the optical lever QPDs (right two plots) to check whether we expect variations on the order of ~2V on the QPDslike we saw on Thursday before and after baffle installation.
From this trend the power appears to drift more than this for two hours after unshuttering the laser (around 15:56 UTC), but once it reaches a steady state both QPDs were only drifting by 1V and the fiber power input monitor PDs by 1V or less.
Conclusion: I think we would have seen a dramatic power drop on Thursday when we installed the shroud, that I would expeact to have been much larger than the trends I saw today.
Note mentioned in the summary of activities in the main entry -- per LHO:90667, we re-installed all the ballast or balance mass discussed during this 2026-06-18 day's session. See attached "after" picture.
Here's another picture of the SPI breadboard on HAM3 prior to the baffle installation. Photo credit is ?? maybe Jeff?
New diode housing is ASSY-D2000246-S2100827 the D2000384-S2100908 Photodiode Assembly was not installed, instead the original one was used.
Below is the analysis for data taken on the FC path: between ZM1 and ZM2 and between ZM2 and ZM3, with Nanoscan, see Camilla's log 90573. As a reminder, ZM1 are flat optics, ZM2 is a PSAM with variable curvature, FC1 HR side is flat, AR side is curved with RoC ~1m.
The data suggest that the OPO mode is slightly different from O4 OPO, and also strongly suggest a new optimal ZM2 PSAM voltage can be found within the range.
We measured the beam profile at 5 different points after ZM1 with A:L2 lens at its nominal 0 position (sled that the lens lives on is flush to its translation stage on both front and back edges). At the last point with A:L2 at 0, we realized it would be pertinent to measure beam profiles for the two extremities of the A:L2 translation stage: -13 mm, which is closer to ZM1 by 13 mm and +17 mm, which is 17 mm further from ZM1. We then proceeded to take 5 measurements (again downstream from ZM1) for each of these lens positions. The nanoscan screenshots for each measurement are attached in the .zip folder.
The attached gif shows the beam waist position estimation extracted from the beam profile scans downstream ZM1, for all three A:L2 positions. The "target" and "O4 x/y" come from Keita's log 59515. The overlap plot attached shows the field overlap in percentage for all three A:L2 positions, with target and O4 beam parameters. With A:L2@0, the overlaps are above 99%, which bodes well for the FC mode matching prospects. There could potentially be a better mode matching solution to the "target" or "O4" for A:L2 between 0 pos and -13mm pos. However, the following measurements betwen ZM2 and ZM3 suggest fine-tuning of A:L2 position will not be necessary.
We also measured beam profile between ZM2 and ZM3 for three different points, setting ZM2 PSAM voltage to 4 different values at each point. The "nominal" O4 strain gauge (S.G.) for ZM2 has been 3.15 V, which corresponds to ~ 60 or 90 V pzt supply voltage depending on which direction one scans from. The edges of the psam range are 0 V and 196 V, which corresponds to ~1.2-1.3 V and ~6.04 V S.G. respectively. In the interest of more uniform sampling of the available psam curvatures, we also chose to sample 4.5 V S.G. (~120 V or 150 V).
This table shows experimental data mapped to radii of curvature of the ZM2 mirror, using Camille's E2100298. The exact PZT strain gauge/ PZT supply voltage that gives a certain RoC is affected by the hysteresis curve i.e. sweep direction.
| Strain Gauge (V) | PZT Supply Voltage (V) | RoC (m) with increasing scan | RoC (m) with decreasing scan |
| 1.3 V | 0 | 0.8211 | 0.82202 |
| 6.0x V | 196 | 0.8911 | 0.89114 |
| 3.1x V | 60 (d) or 90 (i) V | 0.8523 | 0.85025 |
| 4.4x V | 120 or 150 V | 0.87534 | 0.87242 |
Attached gif for propagation between FC1 and ZM2 show esimated beam parameters for all four SG cases: 1.3, 3.1x, 4.4x and 6.0x V. The exact values for the strain gauge varied from one beam profile position to the next, however it should be good enough to tell if we have enough range on ZM2 or not.
The gif switches between different SG values once every 2 second, the lefthand plot is useful in looking at the beam divergence near FC1 while the righthand plot is a zoom-in around the beam waist. Looking at the estimated beam waist position for 1.3 V and 3.1x V cases switching across the "FC x/y waist", "VOPO target waist", ''O4 x/y waist", we can guess there could be a better mode matching solution between these two SG values. "FC x/y waist" comes from the Finesse eigenmode solution for the FC path (thanks Kevin Kuns!), target and O4 values are the same from the above-mentioned Keita log, assuming ZM2 curvature to be 0.85025 m (3.15V SG), and the following distances between the optics: A:M3 --> ZM1: 158.2 mm, ZM1--> ZM2: 1498.625 mm, ZM2 --> ZM3: 1821.497 mm, ZM3--> FC1: 1000.261 mm. Camilla extracted these distance values from D1900365-v1.
Knowing the applied PZT voltage and the corresponding RoC, we can use the measurements at 3.1x V and 1.3 V to estimate the mode matching we would obtain if we swept the RoC between that of these strain gauge values. The attached FC mode matching projection plot is computed by taking beam parameter estimated from the beam size measurements for 3.1x V, propagates the beam back to ZM2, unapplies the estimated RoC (decreasing RoC value was used informed by data, indicated in bold in the above table), then reapplies the RoC between these two values, after the overlap with the FC eigenmode is calculated. This projection suggests that mode-matching points with >99% overlap for both x and y axes are accessible. Clearly, there is varying astigmatism with strain gauge setting, see beam profile plots where 3.1x and 6.0x V shows beams with smaller astig. than the other two points. Since the PSAM characterization data gives only a single RoC number rather than separate x/y effective curvatures, the projection should be interpreted as approximate. In practice, the final optimization should be done empirically.
The effect of the astigmatism is also apparent in this defocus vs beam size at FC1 plot that shows mode matching contours. The calculation is made at the FC1.p2.o plane in Finesse.
The beam width data kindly tabulated by Camilla, the R(V) data from Camille's dcc E2100298, and the analysis code .py are attached, in the .zip. Fair warning, the analysis code also makes a bunch of plots I find useful to look at but another user may find irritating :)
Code for the data points upstream of ZM2 attached. The measured beam widths and their corresponding position are listed in the script. The real raw data with the screenshots from the beam profiler UI is attached to the main log.
I wanted to try to get an idea of what sort of astigmatism we're seeing on the FC path. I was able to get good fits of Begum's data right after ZM1. This indicates that the astigmatism coming right off of the VIP looks quite good ( 99.9 +/- 0.1% overlap between X and Y). Plots of the fits are attached for each lens position.
I wasn't able to get particularly convincing fits of the data after ZM2. The points are several Rayliegh ranges away from the waist and I found that the fits were quite sensitive. I could get answers anywhere between 98%-100% mode overlap between X and Y depending on what parameters I used in a la mode for the seed waist. Someone might be able to do a more sophistocated fit of the data, but I think one would want to measure closer to the waist to better constrain the fit and get a more precise estimate of the astigmatism added by ZM2.
I've been reading through the design document about the FC path and ZM2. One thing imay be important to note when making projections about the correct strain gauge setting for ZM2: According to the design document the mode matching is quite sensitive to the exact value of the FC1 AR surface ROC. One might find that, if we change our assumption about the ROC for S2 of FC1, our target strain gauge setting for ZM2 changes significantly. In fact, the discussion makes it sound like most of the point of having ZM2 be adjustable was to compensate for our uncertainty in the ROC of S2 for FC1.
See LIGO-T1900649 and the discussion on Page 18 as well as Figure 10.
A note on the FC1 ROC sensitivity question: a scalar FC1 ROC sweep alone would be only partially informative, because the projection also depends on the FC-path distances and the voltage-dependent x/y astigmatism of ZM2 (see plots for the mode space and projected overlap with eigenmode from the original log). This is why the original log interpreted the projection as approximate and stated that the final optimization should be done empirically.
The more meaningful check right now is therefore a return-beam measurement between ZM1 and ZM2 while stepping the ZM2 strain-gauge setting. This can be done by placing a beam splitter between ZM1 and ZM2 and matching the return beam to the input beam by varying ZM2 curvature.
The modeling exercise could be a nice little real life vs model analysis later on.
We did use the long 27m patch fiber for chamberside testing, and it worked well.
There is an other 5m PM fiber on the cart nearby you can use to verify if it's a problem with the connector or the fiber itself.
I would also inspect the fiber ferrules of the long fiber with a fiber microscope to check for damages.