EY followed EX's lead and also came back to life this morning at 10:34 causing our second VACSTAT alarm for today. EY had been flatlined since yesterday 06:23, close to EX's time.
I restarted VACSTAT at 10:45 to clear the alarm.
10-32x0.375" SHCS that was blocking the access to one 1/4-20 screw was replaced with a low profile 10-32 SHCS.
"Issue 2" in alog 88862 was solved.
See picture, Mitch found a 10-32x0.5" SHCS with a low profile head. 0.5" seemed to be OK in that it's not too long, but we used two washers to make sure that the scrwe doesn't bottom out.
EOM crystal mounting practice part 2 (with a remote help from Michael)
Summary:
Laxen method test.
In alog 88862 we left the EOM module with the alumina piece mounted using Laxen method (no gap between the input side plate and the front plate, a big gap for the output side).
Shining flashlight into the iput or output aperture in the side plates is useful to see the gap between the electrode plate and the alumina piece, and we found that there was indeed a small gap only on one side (i.e. the "crystal" was pinched at the edge).
I loosened the screws for the face plate and repeated the mounting procedure, but this time being extra careful to tighten the screws by tinier amount (than my previous attempts) at a time while applying a gentle pressure from the top. As soon as I got much tighter than finger-tight, I stopped. This resulted in what was seemingly a good contact between the alumina and the electrode, no light visible between them.
See nogap.jpg, this is a representative picture of GOOD contact (even though I cannot prove that the contact is really plane-to-plane not just plane-to-one edge of the crystal).
Another picture gap.jpg is an example of BAD contact. It's hard to see but there's no gap at either edges closer to input/output faces, the gap is only in the middle. I don't have a good explanation for this.
Appert method tests.
We also tested Stephen's suggestion to make a gap on both sides of the front plate. This was trickier but doable by using two Allen keys. The third attachment (EOMassembly.jpg) shows the EOM placed on top of the EOM mount parts just for picture AFTER the alumina was mounted. During the mounting process, the face plate is facing down, and two allen keys will tighten two screws with green (or red) arrows in the picture with tiniest rotation at a time. Green, red, green, red, repeat it until it feels reasonably tight but much, much looser than you'll usually do for tight mechanical connection. After this was done, neither Matt nor I were able to undo the screws by finger.
We did this twice, both times no gap between the alumina and the board, and alumina didn't slip out.
Output side plate might be warped?
In the assembly picture, can you see that the gap between the face plate and the output side panel (right on the picture) is uneven, but the gap for the input (left on the picture) is fairly even? I don't think this is an optical illusion. This might be related to the reason why the crystal ALWAYS slips out when the face plate is tightened down to the output side plate, see my alog (88862). Quoting myself, "no matter what we did, the alumina piece (i.e. fake RTP for excercize) slid out of the assembly but only after tightening the screws". Maybe it's the output side plate.
Reflection measurement.
For each of the above three practices (one with Laxen method, two with Appert method), S11 coefficient was measured for all four ports.
What we found was that all four reflection dips were higher than they are supposed to be. According to Michael, alumina should give us similar results to RTP. I don't list results for all three sets (3x4=12 numbers) because numbers were pretty consistent across the sets, maybe give or take 10kHz or so.
| Nominal LHO/LLO (MHz) | 9.100230 / 9.099055 | 24.078360 / 24.078 | 45.50115 / 45.495275 | 118.30299/118.287715 |
| Measured (representative number) (MHz) | ~9.17 | ~24.10 | ~46.05 | ~119.8 |
In the attached pictures, green line is roughly where the center should be. 9.1 and 24.08 look reasonable to me. Not sure about 45.5MHz, it's 450kHz off. 118.3MHz is totally, totally off.
As I wrote in the summary, I tried bending the coil windings for the 118MHz (bendandsqueeze.jpg) because it was the worst but also because it was the one with the loosest of all four coils (118MHzWinding.jpg), and it had a huge effect. With just a few rounds of bending/squeezing I was able to go down to 118.53MHz (afterbending_118MHz.jpg). I could have passed 118.3 and gone to the other side easily but I stopped there.
Just in case somebody else must do this, here's what I did to measure S11 (reflection coefficient).
If you go to the optics lab, everything is already set up like in the attached cartoon except that the dirty cable is removed from the coupler and placed on top of the optics table. You might still do the calibration again (because we turned off the analyzer at the end of the day and I cannot remember if the calibration results are kept in the analyzer). Remember that EOM is class A but your cables are dirty (even though we wiped the connectors of the dirty cable using q-tips and IPA). We're using one sacrificial SMA elbow that used to be class A to connect your dirty cable to the EOM.
Anyway, calibration. Set the frequency range to whatever you want but make sure that it covers the frequency range of main interest, like at least 9MHz to 125MHz or so while performing S11 calibration.
Connect the BNC of the dirty cable to the INPUT connector of the directional coupler, like in the attached cartoon.
Press "cal" button and select S11 calibration. Don't connect anything to the SMA of the dirty cable and press "Open" button. Next attach a hand-made short circuit plug to the dirty cable via BNC male to SMA female connector. Press "Short". Then connect a 50Ohm SMA terminator to the dirty cable via SMA barrel. Press "Load". Then press "Done".
Now you're done with calibration. Press "Measure" and make sure that you're measuring S11.
Clean the SMA with IPA and q-tip again. Connect the dirty cable to the elbow, and the elbow to the EOM. Set the frequency range to whatever you want. That's it.
At 10:11 the EX BT-Ionpump gauge came back to life, causing a VACSTAT ALARM. This gauge has been flat-lined since yesterday, 07:09 Fri23Jan2026.
Could be because today is a sunny day after a long period of cloudy weather (the EX_BT system is solar powered)?
At 10:18 I restarted VACSTAT to clear the alarm.
Sat Jan 24 10:10:15 2026 INFO: Fill completed in 10min 11secs
Jennie W, Sophie M, Sheila D,
First we checked that the MC mirrors top mass OSEMS matched their position at 00:00 UTC on December 19th. This was the last time when the IMC was locked in air after HEPI was locked on HAM2 before JAC install.
MC1 -678 mrad P, -1365 mrad Y.
Sheila and Sophie went to align in chamber using JAC_M3 (mirror right before JAC HAM1 output periscope) and JM2 (mirror right after JAC).
I looked with the beam card between the upper and lower periscope mirrors at the beam spot.
Sheila and Sophie walked the beam in pitch and the beam started to clip badly. They undid this and Sheila came to check the beam on the table and realised that it looked much dimmer than expected compared to the beam leaving the chamber.
She suggested it might be a ghost beam coming onto the table.
After lunch we checked this with the power metre and we had 40mW into HAM2 but 0.46 mW onto the bottom periscope mirror in IOT2L.
Sophie managed to unclip this mainly with pitch (in the JM2 basis) beam walking, with very slow changes on both mirrors in turn and checking the REFL output and the power onto the table we eventually got ~ 20mW, measured after the bottom periscope mirror.
We eventually made enough change that the beam was getting to both MC REFL WFS but not hitting the diodes.
Sophie did more beam walking in yaw on the two mirrors while looking at MC REFL PD and maximising the power on this. The power metre at the end of the day showed 23 mW just after the lower IOT2L periscope mirror but we were still not hitting the WFS PDs. The beam is low and right on MC REFL WFS B.
The workstation CDS conda environments will be updated by Saturday Jan 24. This is a major update that affects many conda packages. Many packages have been updated and some have been dropped.
Python is updated from python 3.10 to python 3.11. Yes, 3.11 is old already, but the CDS environment tracks the IGWN environment, and important packages have not been push beyond python 3.11.
A complete list of changes in the new environment can be found here:
https://git.ligo.org/cds/packaging/cds-conda-distribution/-/wikis/Environments#version-2026-01-06-01
TITLE: 01/24 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Another productive day to wrap up the week.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| ---- | SAF | LVEA IS LASER HAZARD | LVEA | YES | LVEA IS LASER HAZARD | Ongoing |
| 15:50 | FAC | Nellie | FCES | N | Technical cleaning | 16:10 |
| 15:52 | FAC | Kim | LVEA | - | Technical cleaning | 17:09 |
| 16:10 | FAC | Nellie | EY | N | Technical cleaning | 17:00 |
| 16:43 | FAC | Randy | LVEA | - | Measuring on BSC2 platform | 17:43 |
| 17:00 | FAC | Nellie | MY | N | Technical cleaning | 18:04 |
| 17:34 | VAC | Jordan | LVEA | - | HAM7 viewport disassembly | 19:37 |
| 17:38 | SQZ | Kar Meng | LVEA | Y | Beam alignment on SQZT7 | 18:38 |
| 18:05 | JAC | Jennie, Marc | LVEA | - | Checking JAC PZT electronics | 18:21 |
| 18:22 | SQZ | Sheila | LVEA | Y | Check in w/ Kar Meng | 18:38 |
| 18:38 | VAC | Mitchell | LVEA | - | HAM7 viewport disassembly | 19:33 |
| 18:48 | JAC | Keita, Matt | Opt Lab | N | JAC EOM work | 21:09 |
| 19:16 | JAC | Sheila, Jennie, Sophie | LVEA | Y | JAC installation | 20:39 |
| 20:29 | PEM | Robert | LVEA | - | Laser vibrometry | 20:53 |
| 20:40 | SUS | Jeff | CR | N | OPO closeout transfer functions | 00:21 |
| 21:07 | PEM | Robert | LVEA | - | Laser vibrometry (lights off) | 21:32 |
| 21:33 | VAC | Jordan, Tony, Kar Meng | LVEA | - | HAM7 purge air tutorial | 21:53 |
| 21:57 | JAC | Sheila, Jennie, Sophie | LVEA | Y | JAC alignment | Ongoing |
| 22:20 | JAC | Keita, Matt | Opt Lab | N | JAC EOM work | Ongoing |
| 00:12 | PEM | Robert | LVEA | Y | Covering viewport HAM4 | 00:23 |
| 00:17 | SQZ | Kar Meng, Tony | LVEA | Y | HAM7 cleanup | Ongoing |
In prep for HAM7 closeout, the temporary viewport assembly was removed from the HAM5 relay tube port. RV-1 was closed, and the volume vented with viewport covers still installed, with dry N2. I monitored the corner pressure (PT-120B) during venting, to make sure there were no leaks through the gate valve. No change in pressure, so I continued with viewport removal.
Viewport was removed first, then the pump-out tee. The mitered spool piece and bellows assembly was installed on HAM5 side. Lines were marked across the relay tube assembly prior to removal, so the install orientation remained the same.
The ported spool piece will be installed next week during Laser Safe conditions. Bellows flanges were covered with foil for protection.
J. Kissel, R. Short Trying to chase down the issues Ryan Crouch was seeing in his attempt at health check TF measurements of the OPOS (88851), I found that there were no OSEMINF OFFSETs and GAINs to compensate for the OSEM sensors' "open light" current (OLC). Trending back, this suspension has hasn't had OLC compensating OFFSETs or GAINs since we migrated it from HAM6 to HAM7 circa 2021. However, there are TFs in the measurement library (list ${SusSVN}/sus/trunk/OPOS/Common/MatlabTools/plotallopos_tfs.m) in 2022, documented and compared to matlab model in LHO:64275, and they look great. This sadly makes sense, as the former open light current compensating gains were close to 1.0, and the "centering" offset to make the "flag is centered within the range of the OSEM sensor" equal to 0 doesn't really matter for a driven transfer function or ASD, since these both don't care what the DC value of the sensor is, as long that sensor doesn't saturate during the measurement (i.e. the raw ADC counts are somehwere around +15000 [ADC ct]). There's several reports -- over the years as HAM7 has been occasionally open -- how incredibly inaccessible the AOSEMs are within the suspension, and thus every attempt to gather new open light current values are thwarted by "we don't have time for that" or "I tried and it'll require interfering with way too much other stuff." Examples of this are the 2021 attempt by Keita / Camilla (LHO:59939) and last week's undocumented attempt by Rahul (while he was in HAM7 to relieve the yaw offset on ZM4; LHO:88788). Even worse, prior to the move to HAM7, during the installation in HAM6 circa Feb 2018 (LHO:40727) the new OSEMs AOSEMs saturated the ADC at olc = +32768 [ADC ct], so we installed relatively meaningless compensating OFFSETs and GAINs of -olc/2 = -16384 [ct] and 30000/olc = 0.916 [ct/ct], for all but one -- the V3 sensor which was set to -15481 [ct] and 0.973 [ct/ct]. In Apr 2018, we found that the V2 AOSEM's flexi-circuit V2 OFFSET and GAIN was changed to -14553 [ct] 1.031 [ct/ct] in Apr 2018 (see LHO:41468, LHO:41470 and LHO:41503. So this has been left as wrong for 5 years. And really, prior to that, inaccurate. Citing me from 2021 -- the OPOS is using the same AOSEMs and sat-amps as it did while it lived in HAM6, the only difference in the open light current will be from the cable length difference between HAM6 to SUS-R4 and HAM7 to SUS-R4, which I suspect is negligible. So let's at least restore the "inaccurate." But in short, assuming no LED light lumin decay, I think the "correct" values -- and the values that I've now re-installed -- are OSEM OFFSET GAIN H1 -16384 0.916 H2 -16384 0.916 H3 -16384 0.916 V1 -16384 0.916 V2 -14553 1.0307 V3 -15481 0.973 These have been accepted in the SAFE and OBSERVE.snaps So, the question that now remains whether the AOSEM LEDs have decayed significantly, but that -- as we every suspension we ever try to assess -- is horribly confused by alignment shifts (intended or not), making it essentially impossible to assess. The OPOS is no different. The flags physical relationship to the OSEM sensor / LED is wherever they are, with the chamber in-air at the moment. Comparing the last relatively pre-chaos period to now, 2025-12-04 NOW Under UHV In-air H1 7904 8488 H2 8831 7431 H3 8482 3106 V1 14934 14088 V2 13534 11864 V3 12618 9824 In between the "reference" times above, there have been a series of major alignment shifts of the suspension (see last attached), as reported by the OSEM ADCs, for the following reasons: 2025-12-04 18:03 UTC H567 Mega-clean room turned on, causes all the OSEMs to drift over ~7 days. 2025-12-04 20:23 UTC Site Power Outage, brief outage, but 2025-12-10 00:46 UTC HAM7 Door pulled off 2025-12-10 18:50 UTC OPOS locked down in prep for removal of OPO cavity for crystal swap 2025-12-12 23:41 UTC Removal of OPO cavity for crystal swap 2026-01-20 21:34 UTC OPO is reinstalled, OPOS is unlocked 2026-01-21 19:02 UTC On-platform adjustment of optics, reasonable to expect alignment shifts 2026-01-22 22:15 UTC More on-platform optic adjustments, reasonable to expect alignment shifts All this makes it tough to say what the "right" position of the OSEMs should be, and whether e.g. having a raw OSEM count of 3000 [ADC ct] on the H3 OSEM is "acceptable." Acknowledging that there's very little range on the H3 OSEM right now, I'll try reducing the excitation amplitude. However, while we have the chamber open, I recommend re-centering the AOSEMs. Other "interesting" aLOG references. 2022-08-02 LHO:64275 Post HAM7 install health checks in Feb, May, and Aug 2022 show a reasonable, and coherent set of TFs that match the model. Even without OFFSETs or GAINs. 2021-10-27 LHO:60422 Bug identified in OPOS OSEM2EUL/EUL2OSEM basis change matrices. Identified, but never implemented. 2021-09-17 LHO:59939 Attempt to measure open light currents after installation into HAM7, but inaccessibility of H3/V3 OSEMs thwarted effort. 2021-08-26 LHO:59741 OPOS Lands in HAM7 2021-08-17 LHO:59752 OPOS Front-end Infrastructure Migrated from HAM6 (h1susopo) to HAM7 (h1sussqzin) 2021-08-17 LHO:59652 h1susopo model is brought down for above migration to new model -- HERE'S WHERE OPOS OLC OFFSETs and GAINs were lost. 2018-02-26 LHO:40727 Generic 16384 ct OFFSETs and 0.916 GAINs installed because new AOSEMs saturated the ADC during open light. 2018-04-17 LHO:41470 V2 OSEM replaced, new OSEM has non-saturating OLC values
FAMIS 39748
Laser Status:
NPRO output power is 1.835W
AMP1 output power is 70.39W
AMP2 output power is 139.0W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 14 days, 20 hr 48 minutes
Reflected power = 26.68W
Transmitted power = 104.1W
PowerSum = 130.8W
FSS:
It has been locked for 8 days 2 hr and 16 min
TPD[V] = 0.3187V
ISS:
The diffracted power is around 4.0%
Last saturation event was 0 days 0 hours and 0 minutes ago
Possible Issues:
PMC reflected power is high
FSS TPD is low
Both RLF_QPDs A and B are centered on both PIT and YAW, at low seed launch power (2.3)
The CLF transmission PD on SQZT7 was centered.
Fri Jan 23 10:09:29 2026 INFO: Fill completed in 9min 25secs
Note I am using a new format for the trend plot which reduces the number of log divisions on the top plot's y-axis.
The problem: during the winter months the TCs start with a positive temp, dropping to around -70C when LN2 is flowing. To show the TCs along with the discharge line pressure and LLCV on the same plot the TC signals are inverted and then all are ploted logarithmically. This means the baseline (positive)temps are now negative which is not shown on a log plot, and when crossing zero they force many divisions in the autoscaled log axis.
The solution: I modified cp1 overfill IOC to serve modified TC[A,B] channels with max temp limits. Max temp is currently -12.3C, settable in the configuration file. Any temp greater that -12.3 is kept at this value for the channels H1:VAC-CP1_OVERFILL_TC_[A,B]_TEMP_PLOT_DEGC
We have identified two mechanical issues with the JAC EOM and its mount.
Issue 1. Crystal isn't captured in the EOM assembly when we install it in a certain way, but installing it in another way to capture it might (or might not) put overly strong force on the crystal.
No I haven't dropped the real crystal, I did drop alumina piece with the same outer dimensions as the RTP crystal while testing the installation procedure.
It's probably hard for you to understand this issue if you're not familiar with the EOM assembly (D2500130) and the assembly/test procedure (google doc), look at my super-simplified cartoon (ideal.png).
EOM comprises the face plate, RTP crystal and everything else. Everything else is already assembled. The task is to sandwich the RTP between the electrode board (which is a part of "everything else") and the face plate. You'll put the face plate on a table, put RTP on top of the face plate, carefully lower everything else until the board touches the RTP along its entire length, and you bolt the face plate to the side panels. Simple.
It can be much different from that if the board is not orthogonal to the side panels, look at the second attachment. Here, the board is crooked, the distance to the face plate on the output side is smaller than on the input side (this cartoon).
Suppose that I choose to make the face plate contact with the output side plate, and bolt the face plate down. The face plate is squared up relative to the side plate, not the board, and the "everything else" part will rotate away from the face plate (or face plate rotates away from everything else) and RTP is free to move. I think this is what happened consistently (10 or so trials) in the lab today, no matter what we did, the alumina piece (i.e. fake RTP for excercize) slid out of the assembly but only after tightening the screws.
On the other hand, if I choose to make the face plate contact with the input side plate (notsoideal.png), the rotation will be in the opposite direction, the face plate is not reqlly squared up but will put a pressure on the RTP, securely captureing it. After switching the side where the face panel contacts in the lab, the alumina piece (fake RTP) never dropped (3 trials so not much statistics but 3/3 success is much better than 10/10 failure).
The problems are that we don't have any control over how much force is applied to the crystal. Moreover, in our "successful" trials, the board might not be touching the alumina piece along its entire length. Look at the picture, this is after the last (3rd) "successful" attempt with the alumina piece still in, the board and the face plate are not parallel with each other, we might be pinching the alumina thing at the corner closest to the output side. Not sure if it's always like this but it's likely.
Stephen and Michael suggest that instead of bolting the face plate firmly to the input side, there could be a gap on each side, the face plate is supported by the tension of the screws, making sure that the face is parallel to the board. I'm not necessarily a fan of the idea but we'll try.
Issue 2. One of the bolts for the EOM base is blocked by another screw head.
See the last picture. One 1/4-20 screw cannot be tightened because the 10-32 bolt head just above that blocks access. We might replace the offending bolt with 10-32x0.375" pan head screw AND use the ball head Allen key for 1/4-20, that might work.
Other issues.
We can move the mount in PIT/ROLL and YAW, but somehow it's very difficult to cause pure PIT motion, it always couples to ROLL.
When we use set screws to tilt the base and then back them off, the mount won't return to the original position, I have to push down the pivot plate toward the base plate firmly, then there's a metal clicking sound and the mount goes back. This might be related to the fact that, as of now, the dowel pin (part #14 of the assembly drawing) is a REALLY tight fit for the pivot plate as of now.
Finally, the cable strain relief post could not be set at a desired angle using the supplied slotted washer (the only difference I was able to make is either bad angle or 180 degrees off of the bad angle). But using other washers on top of the slotted one(s) I was able to manage good-ish angle.
Another potential mechanical issue (?).
One of the roll adjustment set screw (8-32 oval point) is riding on top of the shallow groove that is 0.125" wide and 0.02" deep in the base plate. Depending on the YAW adjustment, the round tip of the screw might sit on the edge of the groove, making things unstable. FYI the standard diameter of 8-32 screw is 0.164" so it's wider than the recess, I don't know the exact profile of the oval point but the YAW adjustment range of this mount is smaller than it seemed at first to me.
If the groove is just a visual aid, maybe it can be shortened such that it won't interfere with the set screw.
I couldn't take a good picture of this, if I can I'll post it later.
Jennie W, Jenne D, Masayuki N
Today Jenne and I went into HAM1 and onto IOT2L.
Our first priority was to check the input alignment to the JAC after alignment efforts yesterday to check we were not locking to a HOM mode. We locked the JAC with a power of 0.1 on the TRANS_A_LF_OUT channel.
I checked after lens JAC_L3 which is right before the steering mirror into the HAM1 output periscope. Here the beam looked like a 10 mode (two lobes in the horizontal axis). Further upstream (just after JAC cavity this was not obvious due to the beam size.
We used the steering mirror between the input periscope and JAC + the PSL periscope PZT mirror to improve the alignment. To do this we changed yaw in the closer mirror and pitch in the PSL PZT mirror as the input periscope switches the P and Y around.
We recovered a value of 0.22 on TRANS_A_LF_OUT which matches with the values we got on friday the last time we had a good TM00 lock on the JAC cavity.
After this Jenne went to the table to look at the beam we found yesterday which is at the edge of the MC REFL periscope mirrors in yaw and clips on the BS1 optic.
I started changing the tilt of the beam through HAM2 by changing the pitch of the mirror right before the HAM1 output periscope. This did not really change the beam position so we moved to a further away mirror (JM2) to translate the beam.
During this process we also became unable to lock the JAC using the guardian. More details at the end.
After some iteration we were able to see a beam on the MC REFL PD but have not been able to walk the beam to see any signals on the MC REFL WFS orflashing from the IMC on the MC TRANS PD.
After a break we went to the control room and did some checking of the MC sus alignments. We found problems with the alignment of MC3 - Dave and Ollie debugged this.
Jenne then did some walking of the MC mirrors and by moving MC1 she could get a larger signal on MC REFL. We might be able to use this tomorrow by moving MC1 to this 'wrong' ( ie. not consistent with the nominal IMC alignment before JAC was installed) place and walking MC1 back while changing the in-vac fixed mirrors in HAM1 to reover the beam on MC REFL PD.
During the day an electronics chassis was swapped that does the whitening for the TRANS PD A. The signal stopped getting to the diode so Daniel gave us the go-ahead to bypass this - this might need to be fixed properly at some point, it is level 10 on the rack closest to HAM1, next to the PSL enclosure. I took put IN3 and OUT 3 cables and connected them with a TNC connector.
This afternoon and evening we tried to trouble-shoot the JAC locking.
There was also an incorrect gain that got reset by the model restart for h1lsc earlier today but fixing this (JAC_DITHER_PD_IN gain was set to 200 and should be 4) did not allow us to lock.
After changing the servo gain in the dither lock Jenne noticed that this had no effect on the lock level/noise on the TRANS PD.
After checking with Masayuki the problem seems to be that the fast channel to drive the PZT is not connected somehow at the racks but the Beckhoff controller can be used to drive the PZT - will consult with Daniel/Marc tomorrow.
This morning Marc and I switched back to the old PZT chassis that was swapped out yesterday. Now the PZT feedback works in CDS so we can lock JAC.
[Sheila, Karmeng]
We offloaded the saturation on ZM4 and ZM6 while maintaining the alignment to HAM6 QPDs.
Power budget: we measured 0.75mW at the OPO output, after SFI1, and after thin film polarizer. The power dropped to 0.74mW after BM3. And further to 0.71mW at the viewport/SQZT7 periscope and HD.
Scanned the IR and green transmission of the OPO, the green transmision (orange trace) will need further adjustmnet.
We spent most of yesterday and this morning recovering from the alignment shift that resulted from unlocking the VIP.
Yesterday Ryan Short joined us and we worked on the path from the VIP to FC. We now have the osems of FC1 and ZM2 (and ZM1yaw) back as they were in O4, and the beam centered on the iris right after ZM3. The beam should be aligned to the filter cavity since it is retroreflecting off FC1 and FC1 should be pointing to FC2. Since we only have the -Y door removed, we can't easily check the centering on ZM2 with a card; we set the alignment of ZM2 to match what it was in O4 and since the beam is centered on the ZM3 iris it should be at the position on ZM2 that it was in O4 (centered we believe). We also had to spend some time to make sure that none of the suspensions were close to saturation. While doing this we adjusted the pointing off the VIP using A:M1 and A:M2 (see VIP layout), which is why we had to readjust the co-alingment today, we also used A:M3.
This morning I made the final adjustments to get the beam centered on the ZM3 iris, and adjusted B:M4 to center the spot on the Z:M4 iris, and first iris on SQZT7, then also adjusted Zm4 and ZM5 to get the beam well centered on the SQZT7 irises. Kar Meng and I sent the beam into HAM6 and we were able to run centering servos to adjust ZM4 + ZM5 to center AS_A and AS_B, but this saturated ZM4. We then walked the beam using B:M4 so that it was a little high on the ZM4 iris (KarMeng has a photo 88859 to estimate how above center), but no suspensions are close to saturation.
Ryan Crouch ran OPO health checks, 88851, but wants to retake them with purge air turned down.
After lunch we readjsuted the co-alignment of the green and IR (photos in 88859), and re-alinged the seed beam onto the RLF QPDs, which was needed because of the shift when unlocking the VIP. With the seed beam we saturate the QPDs so we will need to revisit this and center using the CLF. We then took photos of various things in chamber as Kar Meng has added in 88859.
After all this we took one last peak at the beam going into HAM6, it was well centered on the AS_A, AS_B, and AS_C with our final alignment for about 30 seconds at 22:29:45, as shown in Kar Meng's screenshot. This means that we are done using the viewport.
Things left to do in HAM7:
The pump scan looks good ok the scope. The distortion from ndscope scan is most probably due to the filtering of ADC.
We have intalled the POP periscope stiffener.
Some dog clamps in the REFL path as well as the cable bracket for PM1 were relocated to accomodate. 1st and 2nd picture are "before" photo. 3rd one is after PM1 cable bracket relocation but before installing the stiffener. There are also three "after" photos showing how things look on the table.
POP beam clearance:
I took the picture of the bottom periscope mirror through dichroic (HR for IR, transmission for green) to see the beam clearance. In the first such photo (POP_beam_clearance.jpg), the camera is close to the center of the dichroic and the short stiffener beam is close to the edge of the optic but not occulting the mirror, so we're OK. Just to make sure that we're absolutely safe, I moved the camera closer to the -Y edge (right on the picture) of the dichroic (POP_beam_clearance_extreme.jpg) and it still looks OK.
If it's hard to understand what was done, look at the annotated photo (the last attachment After_stiffener_installed_annotated.jpg), the cellphone camera was inserted to "Camera" position.
REFL beam path:
I confirmed that the long stiffener beam doesn't interfere with the motion of the REFL beam diverter. Also, when the REFL beam diverter is open, I looked into the last steering mirror for the REFL air path from the viewport position to make sure that the short stiffener beam won't occult the REFL path.
Some hiccups:
We used D2500433 -11 variant S/N 4 and -1 variant S/N1 even though page 11 of T2500339 suggests it should be -10 and -2 variant, respectively. We didn't have -10 variant, and -2 variant was absolutely too short.
B&K
We performed B&K hammer measurements before/after the stiffener installation for POP periscope. Before, there was a 70Hz-ish peak. After, it was pushed higher up in frequency. The transducer was attached to the ISI table and Jim hammered the top of the periscope.
Likewise we did B&K test for the input periscope of the JAC even though it was not absolutely necessary.
We haven't done B&K for the JAC output periscope because it's not even fully clamped down (we will move it).
Jim will post the data.
Unused stiffener parts are in my office for now.
Tagging EPO for photos.
These are the measurements we got with the B&K of the POP periscope before and after adding the stiffener. For the POP periscope, we mounted the accel to the table, right at the foot of the periscope, and did the impacts at the top of the post. The accelerometer was mounted with the sensors Z aligned vertically, the Y axis was roughly parallel to the edge of the ISI, so it was mostly pointing along the IFO X arm. First and second images are impacts in the IFO X and Y dofs, you can pretty clearly see the 70hz post resonance. Third, fourth and fifth images are with the accelerometer in the same spot after adding the stiffener, it seems the mode has successfully been moved much higher to around 170hz. This should allow me to increase the ugf and loop gain quite a bit, to be more like the other ISI. I'll verify with tfs on the ISI after the vent.
Last 3 images are B&K measurements of the JAC periscope, accel for these measurements was mounted on the edge of the table, with x,y,z sensor dofs aligned to the IFO x,y,z dofs. This also looks pretty good, first features are over 200hz.
Attached zip contains the csv data exports of each of the measurements. Names indicate the direction of the hit with the hammer, relative to IFO x,y,z conventions.
As per Jeff's request we took osme zoomed out photos of the periscope today.