Robert, Sheila, Eric, Daniel D
Yesterday morning we were able to identify the source of the scatter in HAM7 as being SFI2, and notice that the beam is very off center on the polarizer on the ZM4 side of SFI2, B:P2.
We locked the OMC on a single bounce beam with 50W input to the IMC, and turned on the ISS second loop, and got 67mA DCPD sum. With the viewport on the HAM5 gate valve and a 1 Hz excitation of 1000 counts amplitude on ZM5 TEST, we could clearly see a fringe wrapping shelf at 140 Hz. We used a piece of black glass to block the beam and could see the scatter shelf go away when the black glass was after B:P2 and reappear when the black glass was before the rotator.
Robert got some photos of the location of the beam on B:P2, it is clearly off center and near the +Y edge of the polarizer aperture. We attempted to steer the ZMs to bring it close to the center, but we clipped the beam on the aperature attached to B:L2 before we could bring the beam close to centered. This indicates that this path was aligned with the beam poorly centered on the Faraday.
TITLE: 12/19 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: MAINTENANCE
Wind: 9mph Gusts, 5mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.45 μm/s
QUICK SUMMARY:
M. Todd, G. Vajente, L. Dartez
TITLE: 12/19 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
IFO is in IDLE for PLANNED ENGINEERING
Summary of activities today:
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 15:57 | SAF | LASER | LVEA | YES | LVEA is LASER HAZARD \u0d26\u0d4d\u0d26\u0d3f (\u2022O\u2022) | 10:51 |
| 15:46 | FAC | Tyler and Crane Tech | LVEA | Y | Crane upgrades south Bay | 18:33 |
| 15:59 | FAC | Kim, Nellie | LVEA | Y | Technical cleaning | 16:46 |
| 16:09 | FAC | TJ | LVEA | Y | Dust Monitor 10 Check | 16:46 |
| 17:22 | JAC | Masayuki | Optics Lab | N | JAC Work | 19:18 |
| 17:35 | FAC | Kim | MX | N | Technical Cleaning | 18:32 |
| 17:40 | SQZ | Sheila, Robert | LVEA | Y | Hunting for scattered light | 19:35 |
| 17:46 | PEM | Jim, Randy | LVEA | Y | PEM Support Tube Plate Check | 18:15 |
| 17:51 | SQZ | Eric, Daniel | LVEA | Y | Scattered light checks | 19:35 |
| 17:57 | TCS | Matt | Vac Prep Lab | N | Cheeta | 19:09 |
| 18:17 | SQZ | Jennie | LVEA | Y | HAM7 work | 18:30 |
| 18:29 | ISC | Betsy | Optics lab | N | Checks | 19:18 |
| 20:44 | ISC | Betsy | LVEA HAM1 | Y | Open light pipe, HAM1 work | 22:37 |
| 20:56 | FAC | Crane contractor | LVEA | Y | Crane inspections | 00:55 |
| 21:08 | SQZ | Daniel, Eric, Kar Meng | LVEA | Y | HAM 7 OPO | 00:03 |
| 21:09 | PCAL | Tony | PCAL | N | Transfer Meas. | 22:30 |
| 21:09 | Keita | LVEA | Y | Checking in with Betsy | 21:37 | |
| 21:15 | FAC | Randy | LVEA | Y | Checking on crane man | 21:42 |
| 21:17 | IAS | Jason | LVEA | Y | FARO Work BSC2 | 23:17 |
| 21:20 | IAS' | Ryan C | LVEA | Y | FARO BSC2 | 23:20 |
| 21:29 | TCS | Matt | Vac-Prep Lab | N | Cheeta\\ | 00:07 |
| 21:48 | PSL | Jean-Rene, Alicia | LVEA | Y | PSL Camera disconnect | 01:46 |
| 21:50 | ISC | Richard | LVEA | Y | Check on activities | 23:42 |
| 21:55 | Masayuki | LVEA | N | Beam dump assembly | 22:37 | |
| 22:03 | SQZ | Sheila | LVEA | Y | HAM7 OPO | 00:00 |
| 22:53 | Richard | LVEA | Y | Checking on activities | 23:41 | |
| 22:57 | FAC | Tyler | LVEA | Y | Crane upgrade wrap up | 23:09 |
| 23:09 | SUS | Rahul | LVEA | Y | HAM1 | 20:09 |
| 23:25 | FAC | Richard | LVEA | N | Checks | 00:07 |
| 23:28 | PCAL | Tony | PCAL Lab | N | Setting up a measurement | 22:28 |
| 23:37 | SEI | Jim | LVEA | Y | HAM2 HEPI | 00:06 |
| 00:07 | ISC | Keita | LVEA | Y | Opening Light Pipe | 02:07 |
| 00:24 | JAC | Jennie | Vac-Prep Lab | N | Putting stuff away | 01:24 |
| 00:35 | SQZ | Daniel, Eric | LVEA | N | HAM7 Work | 01:35 |
00:38 UTC Keita reports the PSL light pipe is closed and he took the IMC to offline.
[Daniel, Kar Meng, Eric, Sheila]
This afternoon, we continued with the realignment of the VIP after the VOPO swap. When we first started, we briefly lost the CLF input alignment between the fiber and the VOPO cavity. It turned out that the collimator was loose in the mount. We took out the collimator holder and noticed that the 2nd grub screw hadn't been tightened all the way. After fixing, we realigned the cavity till we could see a reasonably strong beam in transmission while the cavity was scanning.
We then began the painful process of aligning the weak transmitted beam through the various components in HAM 7. Using only the first steering mirror between the VOPO and SFI1 on the VIP, we managed to get the beam roughly aligned up to FC1. However, we couldn't quite figure out how to get the return beam from the filter cavity retroreflected through SFI1 again. We eventually decided to move FC1 a bit to get the beam back through SFI1, through SFI2, and onto the iris right before ZM4. We're thinking of doing the following to finish the alignment process:
Betsy, Rahul
We found that SUS JM1 had a faulty quadrupus cable, which we replaced it today. Next, I took OLC for both JM1 and JM3 in HAM1 chamber. I applied the offsets, gains and then centered the BOSEMs - and they look good. Next, I will start checking the health of the electronics chain and the suspension itself (i.e. by taking the transfer function measurements).
The offsets and gain for JM1 is recorded in this screenshot - accepted in the SDF (safe).
The offsets and gain for JM3 is recorded in this screenshot - accepted in the SDF (safe).
Oli, Rahul
We started damping both the suspensions - found that the voltmons were not working (Dave found that their gains were set to zero).
With voltmons ON, both the suspensions were damping fine - no overflows on this 28bit DAC.
Adding pictures of JM1 and JM3 I took today.
Tagging EPO for JM photos
For the upcoming ISS array swap, we plan to bypass the IMC, which is known to be a pain, but we need a stable beam for the array alignment.
Once the corner volume is vent, we use the QPD on the old array and IMC-IM4_TRANS as the initial reference for bypassing the IMC. Once IMC is bypassed, we will center REFL WFS BEFORE removing the old array and record the RM1/RM2 PIT and YAW. This way, even if we somehow suspect e.g. the pointing of the beam going to the IM4 moved after removing the old array, we can still restore the pointing by looking at the REFL WFSs in addition to IM4.
We measured the beam positions on these QPDs today even though we'll repeat this later.
IFO configuration:
Arrow ("->") means before and after the REFL centering servo (DC1 and DC2) was turned ON:
| PSL-ISS_SECONDLOOP_QPD | IMC-IM4_TRANS | ASC-REFL_A_DC | ASC-REFL_B_DC | SUS-RM1-M1_DAMP INMON | SUS-RM1-M1_DAMP INMON | |
| PIT | -0.814 | 0.366 | -0.884 -> 0 | -0.995 -> 0 | 293 -> 168 | -363 -> 68 |
| YAW | 0.655 | -0.146 | 0.590 -> 0 | 0.220 -> 0 | -176 -> -214 | 277 -> -70 |
Septum cover is left OFF but the PSL light pipe was closed after this. REFL centering was turned off but I didn't bother to offload the ASC output to RM sliders.
REFL WFS nubmers as of now are not super meaningful as we'll still have to lock HAM2 down, which potentially change the relative alignment between HAM1 and HAM2. (But it's good that the beam is still hitting REFL WFSs after HAM1 was locked down even though Jim noted that the ISI position of HAM1 is not good. )
I'll open the light pipe tomorrow and quickly repeat the measurement after Jim locks down HAM2 HEPI.
Jim locked HAM2 HEPI today. I opened the PSL light pipe and locked IMC, and the beam was already reasonable on REFL WFSs without centering servo.
I'm convinced at this point that Jim does a good job that the angle change won't be large enough to lose the beam in HAM1 even after Jim locks down HAM2 in air. We will very likely find the beam on REFL WFSs after bypassing the IMC using ISS array QPD and IM4 trans.
As before, "->" means before and after the refl centering was turned ON.
| ASC-REFL_A_DC | ASC-REFL_B_DC | SUS-RM1_M1_DAMP INMON | SUS-RM2_M1_DAMP INMON | |
| PIT | 0 -> 0 | -0.39 -> 0 | 190 -> 174 | 108 -> 14 |
| YAW | 0 -> 0 | 0.07 -> 0 | -210 -> -214 | -69 -> -59 |
After this,
Closes FAMIS 27648, last checked in alog 88314
Trends look fine!
Betsy, Fil, Rahul
Today we kicked started the installation activities in HAM1 chamber for the Jitter Attenuation Cavity (JAC). Given below are the things we placed on the ISI table - they are all roughly positioned and dog clamped.
1. Tip Tilt JM1 - now connected to electronics chain, having some issues with the bosem adc counts etc, will continue looking into it.
2. Tip Tilt JM3 - now connected to the electronics chain, bosem centered, will proceed for health checks once the chassis and electronics chain looks okay.
3. The two periscopes for the JAC, Type 121 and 132 - assembly report posted by Jennie - 88574.
4. Some optics on Siskiyou mount were also added to the table.
I am attaching pictures which shows the above mentioned things added to the table - and for comparison a picture showing before any addition was (here) made.
Fil also performed group loop checks on JM1 and JM3 and did not find any issues with them.
EPO-Tagging for JAC installation
[Jason, Betsy, Masayuki]
Two arises are installed into HAM1 chamber. They will be used as the alignment reference for new PSL modematching lens installation.
Next step: move to the PSL and install the new mode-matching lens, likely tomorrow. This will break the IMC mode matching; IMC relocking will not be possible until the JAC installation is completed.
(Jordan, Travis, Gerardo)
The relay tube connecting HAM5 and HAM7 was removed. We had a few snags while removing it, for some reason the space between bellows is tight, perhaps due to the difference between pressure states, one chamber is under vacuum the other is not.
After the tube was out, the viewport was installed on a short assembly, the viewport and the entire assembly was leak checked and no leaks were found. He background a the leak detector remained at 1.0x10-10 torr*l/sec during the leak testing.
System is currently being pumped down via a small turbo plus an aux cart.
EPO-Tagging for Relay Tube removal
[Eric, Daniel, Karmeng]
We transferred the OPO from LVEA to optics lab, uncovered the lids and everything looks good.
Touch the mirror mounts and mirrors, no failure except for M3, which swivels off the mount, only part of the glue holding the mirror on the mount.
EPO-Tagging for cool photos of OPO.
TITLE: 12/04 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
After CDS & H1-Locking work of yesterday, today we transitioned to starting prep work for the upcoming vent of HAM7.
However, there was more CDS work today which was related to ISC Slow Controls....but in the middle of this...
There was a 90min power outage on site!!
LOG:
Recovery milestones:
22:02 Power back-up
22:04 CDS / GC seeing what's on/functional, then bring infrastructure back up
22:10 VAC team starts Kebelco to support the ar pressure that's keeping the cornerstation gate valves for closing
22:13 Phones are back
22:17 LHO GC Internet's back
22:25 GC wifi back up, alog and CDS back up
22:40 RyanS, Jason, Patick got PSL beckoff back up
22:55 VAC in LVEA/FCES back up
22:57 CDS back up (only controls)
23:27 PSL computer back
00:14 Safety interlock is back
00:14 HV and ALSY on at EY
00:35 opslogin0 back up
00:37 CS HV back up
00:53 CS HEPI pump station controller back up
01:05 CO2X and CO2Y back up
01:10 HV and ALSY on at EY
01:22 PSL is alive
Note: EY 24MHz oscillator had to be power cycled to resync
Casualties:
- lost ADC on seiH16
- 18V power supply failure at EY in SUS rack
Log:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 22:32 | VAC | Gerardo | MX, EX, MY, EY | n | Bringing back VAC computers | 23:41 |
| 23:32 | VAC | Jordan | LVEA, FCES | n | Bringing back VAC computers | 22:55 |
| 22:54 | PSL | RyanS, Jason | LVEA | n | Turning PSL chiller back on | 23:27 |
| 23:03 | VAC | Jordan | LVEA | n | Checking out VAC computer | 23:41 |
| 23:56 | SAF | Richard | EY | n | Looking at safety system | 00:25 |
| 00:02 | JAC | Jennie | JOAT, OpticsLab | n | Putting components on table | 01:24 |
| 00:19 | SAF | TJ | EX | n | Turning on HV and ALSX | 00:49 |
| 00:38 | TCS | RyanC | LVEA | n | Turning CO2 lasers back on | 01:06 |
| 01:03 | EE | Marc | CER | n | Power cycling io chassis | 01:14 |
| 01:06 | PSL | RyanS, Jason | LVEA | n | Checking makeup air for PSL | 01:10 |
| 01:07 | JAC | Jennie | LVEA | n | Grabbing parts | 01:14 |
| 01:08 | beckhoff | patrick | cr | - | BRSx recovery | 02:20 |
| 01:08 | sei | jim | EX.EY | - | HEPI pump station recovery | 01:58 |
| 01:25 | SEI | Patrick | EX | n | BRSX troubleshooting | 01:54 |
| 01:27 | EE | Marc | EX | n | Looking at RF sources | 02:09 |
| 02:00 | EE | Fil | EY | n | Power cycling SUSEY | 02:19 |
| 02:09 | VAC | Gerardo | MX | N | Troubleshooting VAC computer | 02:27 |
| 02:12 | EE | Marc | CER | N | Checking power supplies | 02:16 |
Since Oli's alog, I tried to keep a rough outline of the goings-on:
Marc and Fil went down to EY to replace the failed power supply, which brought life back to the EY frondends.
Dave noticed several models across site had timing errors, so he restarted them.
Gerardo continued to torubleshoot VAC computers at the mid-stations.
Once CDS boots were finished, I brought all suspension Guardians to either ALIGNED or MISALIGNED so that they're damped overnight.
I started to recover some of the Guardian nodes that didn't come up initially. When TJ started the Guardian service earlier, it took a very long time, but most of the nodes came up and he put them into good states for the night. The ones that didn't come up (still white on the GRD overview screen) I've been able to revive with a 'guardctrl restart' command, but I can only do a couple at a time or else the process times out. Even this way, the nodes take several minutes to come online. I got through many of the dead nodes, but I did not finish as I am very tired.
Main things still to do for recovery: (off the top of my head)
EPO-tagging for power outage
[Joan-Rene Merou, Alicia Calafat, Sheila Dwyer, Jenne Driggers] We have entered the LVEA and went to the Beer garden. There, we first turned off the Low Voltage ITM ESD Driver D1600092, first the 15V switch and then the medium voltage switch. In order to turn it on again, it should be reconnected in the opposite order. With the voltage request set to 0 and chassis powered off, we have unplugged the SHV cables going to the chamber and plugged into Robert's ground boxes, which we used to ground to the rack which is grounded to the chamber. This has been done at both drivers (See attached photos). Afterwards, we have changed the code at /opt/rtcds/userapps/release/isc/h1/guardian/ISC_LOCK.py in order that the LOWNOISE_COIL_DRIVERS will go to LOWNOISE_ESD_ETMY instead of TRANSITION_FROM_ETMX. This has been done by changing lines 6670 and 6674, moving the ", 15" step from line 6670 to 6674. Finally, we communicated the change to the operator and loaded the guardian.
It appears that the grounding did not decrease the amplitude of the combs. As seen in the attached figure, the relative amplitude of the first harmonics of the combs remains mostly the same before and after the change on November 13th.
EPO-Tagging for photo of ESD work
Related: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=87729
We disconnected everything from the ISS array installation spare unit S1202965 and stored it in the ISS array cabinet in the vac prep area next to the OSB optics lab. See the first 8 pictures.
The incomplete spare ISS array assy originally removed from LLO HAM2 (S1202966) was moved to a shelf under the work table right next to the clean loom in the optics lab (see the 9th picture). Note that one PD was pulled from that and was transplanted to our installation spare S1202965.
Metadata for both 2965 and 2966 were updated.
ISS second array parts inventory https://dcc.ligo.org/E2500191 is being updated.
Rahul and I cleared the optics table so Josh and Jeff can do their SPI work.
Optics mounts and things were put in the blue cabinet. Mirrors, PBS and lenses were put back into labeled containers and in the cabinet in front of the door to the change area.
Butterfly module laser, the LD driver and TEC controller were put back in the gray plastic bin. There was no space in the cabinets/shelves so it's put under the optics table closer to the flow bench area.
Single channel PZT drivers were put back in the cabinet on the northwest wall in the optics lab. Two channel PZT driver, oscilloscopes, a function generator and DC supplies went back to the EE shop.
OnTrack QPD preamp, its dedicated power transformer, LIGO's LCD interface for QPD and its power supply were put in a corner of one of the bottom shelf of the cabinet on the southwest wall.
Thorlabs M2 profiler and a special lens kit for that were given to Tony who stored them in the Pcal lab.
aLIGO PSL ISS PD array spare parts inventory E2500191 was updated.
I was baffled to find that I haven't made an alog about it, so here it is. These as well as other alogs written by Jennie, Rahul or myself in since May-ish 2025 will be added to https://dcc.ligo.org/LIGO-T2500077.
Multiple PDs were moved so that there's no huge outlier in the position of the PDs relative to the beam. When Mayank and Siva were here, we used to do this using an IR camera to see the beam spot position. However, since then we have found that the PD output itself to search for the edge of the active area is easier.
After the adjustments were made, the beam going into the ISS array was scanned vertically as well as horizontally while the PD outputs were recorded. See the first attachment. There are two noteworthy points.
1. PDs "look" much narrower in YAW than in PIT due to 45 degrees AOI only in YAW.
Relative alignment matters more for YAW because of this.
2. YAW scan shows the second peak for most of PDs but only in one direction.
This was observed in Mayank/Siva data too but it wasn't understood back then. This is the design feature. The PDs are behind an array plate like in the second attachment (the plate itself is https://dcc.ligo.org/D1300322). Red lines show the nominal beam lines and they're pretty close to one side of the conical bores on the plate. Pink and blue arrows represent the shifted beam in YAW.
If the beam is shifted too much "to the right" on the figure (i.e. pink), the beam is blocked by the plate, but if the shift is "to the left" (i.e. blue) the beam is not blocked. It turns out that it's possible that the beam grazes along the bore, and when that happens, a part of the broad specular reflection hits the diode.
See the third attachment, this was shot when PD1 (the rightmost in the picture) was showing the second peak while PD2 didn't.
(Note that the v2 plate which we use is an improvement over the v1 that actually blocked the beam when the beam is correctly aligned. However, there's no reason things are designed this way.)
We used a PZT-driven mirror to modulate the beam position, which was measured by the array QPD connected to ON-TRAK OT-301 preamp as explained in this document in T2500077 (though it is misidentified as OT-310).
See the fourth attachment where relatively good (small/acceptable) coupling was obtained. The numbers measured this time VS April 2025 (Mayank/Siva numbers) VS February 2016 (T1600063-V2) are listed below. All in all, horizontal coupling was better in April but vertical is better now. Both now and Apr/2025 are better than Feb/2016.
| PD number |
Horizontal [RIN/m] |
Vertical [RIN/m] |
||||
| Now |
Apr/2025 (phase NA) |
Feb/2016 (phase NA) |
Now |
Apr/2025 (phase NA) |
Feb/2016 (phase NA) |
|
|
1 |
6.9 | 0.8 | 20 | -0.77 | 34.1 | 11 |
| 2 | 7.1 | 2.7 | 83 | 5.1 | 2 | 25 |
| 3 | 8.2 | 5.5 | 59 | 2.2 | 4.4 | 80 |
| 4 | 8.8 | 2.3 | 33 | 0.30 | 1.1 | 21 |
| 5 | -19 | 5.1 | 22 | 11 | 12.3 | 56 |
| 6 | -14 | 12.9 | 67 | 16 | 30.4 | 44 |
| 7 | -18 | 10.2 | 27 | 2.9 | 42.7 | 51 |
| 8 | -19 | 5.3 | 11 | 12 | 52.1 | 54 |
Phase of the jitter coupling: You can mix and match to potentially lower jitter coupling further.
Only in "Now" column, the coupling is expressed as signed numbers as we measured the phase of the array PD output relative to the QPD output. Absolute phase is not that important but relative phase between the array PDs is important. The phase is not uniform across all diodes when the beam is well aligned. This means that you can potentially mix and match PDs to further minimize the jitter coupling.
Using the example of this particular measurement, if you choose PD1/2/3/4 as the in-loop PD, the jitter coupling of the combined signal is roughly mean(6.9,7.1,8.2,8.8)=7.8 RIN/m horizontally and mean(-0.77, 5.1, 2.2, 0.3) = 1.7.
However, if you choose PD1/3/4/7 (in analog land), the coupling is reduced to mean(6.9, 8.2, 8.8, -18)=1.5 horizontally and mean(-0.77, 2.2, 0.3, 2.9)=1.2.
You don't pre-determine the combination now, you should tune the alignment and measure the coupling in chamber to decide if you want a different combination than 1/2/3/4.
Note, when monotonically scanning the beam position in YAW (or PIT) edge to edge of PDs, some PDs showed more than one phase flips. When the beam is apparently clipped at the edge (thus the coupling is huge), all diodes show the same phase as expected. But that's not necessarily the case when the beam is well aligned as you saw above.The reason of the sign flips when the beam is far from the edge of the PD is unknown but there should be something like particulates on the PD surface.
The QPD was physically moved so the beam is very close to the center of the QPD. This can be used as a reference in chamber when aligning the beam to the ISS array.
After this, we manually scanned the beam horizontally and measured the QPD output. See the 5th attachment, vertical axis is directly comparable to the normalized PIT/YAW of the CDS QPD module, assuming that the beam size on the QPD in the lab is close enough to the real beam in chamber (which it should be).
EPO-tagging for ISS Array work