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Reports until 16:34, Tuesday 16 September 2025
LHO General
thomas.shaffer@LIGO.ORG - posted 16:34, Tuesday 16 September 2025 - last comment - 12:44, Wednesday 17 September 2025(86969)
Ops Day Shift Start

TITLE: 09/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Lots of work today to understand our troubled IFO as well as some maintenance items. We perhaps have narrowed down the change from the power outage and have changed the input power into the PMC to bring us back to a similar place. We have run an initial alignment, which probably could have run automated, and we are now going through PRMI/DRMI for a second time. I accepted some SDFs in safe before we started locking, see screenshots attached.

BRSY was rung up during some work at EY today, and doesn't seem to be damping. I've contacted Jim, but we will keep an eye on it.


LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:36 SYS Randy, Mitchell, Chris EY n Craning spiral staircase out 16:36
14:58 FAC Contractor (C&E) Vertex n Fire hydrant repair in vertex area near FCBTE 20:19
15:11 CDS Ken LVEA n HAM5/6 cable tray install 19:04
15:17 FAC Nelly LVEA n Tech clean 16:40
15:33 SPI Jeff Opt Lab n Parts 15:38
15:34 - Jennie, parents LVEA n Tour 16:11
15:35 CDS Fil LVEA LOCAL IOT2 table enclosure lights 15:59
15:38 VAC Janos, Travis MY n Pump work 19:22
15:45 ISC Camilla Opt Lab n Grab equipment 15:50
15:46 ISC Camilla, Sheila LVEA LOCAL IOT2 table checks 17:09
15:46 PSL Jason, Ryan S PSL enc YES PSL FSS adjustment 18:54
15:56 PEM Ryan C LVEA n Dropping off dust monitor testing equipment for the PSL team 15:58
16:00 SUS Ryan C EX n SUS charge meas. 17:59
16:15 SEI Jim LVEA n Replace CPS card for HAM3 17:09
16:41 FAC Nelly PSL enc YES Tech clean 16:46
16:41 SYS Betsy LVEA n Mega clean room sock meas. and check on status of work 16:55
16:52 ISC Elenna LVEA n Unplugged SR785 and other test equipment 16:52
17:24 FAC Nelly EX n Tech clean 17:58
17:32 VAC Gerardo, Jordan LVEA n AIP check at HAM6 17:38
17:33 FAC Tyler Mids n 3IFO checks 18:33
17:59 FAC Nelly HAM Shack n Tech clean 18:34
19:59 CDS Marc MY n Grabbing a chassis 21:36
20:20 PSL Jason, Ryan S PSL enc YES Table test 21:55
20:27 VAC' Gerardo, Camilla LVEA n Lookng for viewport covers 20:46
20:46 VAC Gerardo LVEA n HAM6 AIP 20:48
20:54 PCAL Francisco PCAL lab Local PCAL lab work 21:21
22:28 - Oli LVEA n Sweep 22:49
Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 12:44, Wednesday 17 September 2025 (86990)

Interestingly we saw a slight rise in the iop duo-tones for all four EY front ends which coincide with the spiral-staircase craining.

Plot shows all four IOP DUOTONE channels, AC2 power strip current usage and building lights. Seqence is

07:51 lights on

08:04 duo tone rise

09:13 duo tone starts dropping, AC2 less noisy

09:32 lights out

Images attached to this comment
H1 GRD (OpsInfo)
thomas.shaffer@LIGO.ORG - posted 16:33, Tuesday 16 September 2025 (86975)
Added a decorator to H1_MANAGER that will kill the lock if IMC_REFL gets too high

On the night of Sept 10 the IMC REFL power slowly increased all night. To avoid this happening in the future, we decided to have H1_MANAGER check this and kill the lock before calling someone. This is the first instance in guardian, that I'm aware of, that we intentially kill the lock.

This takes place in the form of a decorator in the Low_Noise state of H1_MANAGER. The threshold is currently set to 35, and if it goes above then the node will kill the lock and move ISC_LOCK to IDLE before going to ASSISTANCE_REQUIRED itself.

We tested it while not in low noise with an offset in IMC_REFL and the decorator moved to the Relocking state of H1_MANAGER.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:32, Tuesday 16 September 2025 (86971)
Tues EVE Ops Transition

TITLE: 09/16 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 12mph Gusts, 7mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY:

Site Power Outage recovery continues (with H1 down, but it was  up last night/18hrs ago for almost 3hrs).  Saw H1 locking DRMI as I walked in but it lost lock...but it looks like this was intentional---running Guardian tests to return for being able to have Owl Shift calls.

BRSy is NOT In USE (It's been noisy since around the beginning of Maintenance today)---TJ says it might get a Beckhoff reboot in the morning.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:24, Tuesday 16 September 2025 (86974)
added flag to CARM_5_PM for after_power_outage changes

We have been doing some things by hand to lock recently.  I've put a flag in CARM_5_PM to do these. 

This will take the TR_CARM offset to -52 (instead of the caclulated offset), waits, then increases the TR_CARM to 2.1, then sets the offset to -56, increases the DHARD P gain to -30 and Y to -40, and increases the input matrix element for REFLAIR 27 I to PRCL by a factor of 1.6. 

Of these things, I think that the DHARD gain increases should probably be a good thing that we would want to keep in the long run.  The PRCL gain we plan to check early in the locking sequence. 

H1 PSL
jason.oberling@LIGO.ORG - posted 16:12, Tuesday 16 September 2025 - last comment - 16:53, Tuesday 16 September 2025(86972)
PSL FSS RefCav On-Table Tune Up (WP 12796)

R. Short, J. Oberling

Today we tuned up the RefCav alignment for the PSL FSS, since the TPD had been doing its usual wander and also had a drop after last week's power outage.  As usual, we began with a power budget:

The AOM signle pass diffraction is lower than usual, so we adjusted the AOM alignment to improve it.  While we were doing this we kept seeing small drops in the AOM output that we couldn't recover with alignment, which was making us think that we were walking the alignment off.  Turns out the PMC transmission was slightly dropping.  We remeasured the power incident on the AOM and sure enough, it had dropped a little, to 265.1 mW.  The diffraction efficiency looked good, so we stopped moving the AOM and moved on with adjusting M21 to improve the double pass diffraction (always have to adjust this mirror if the AOM is moved).  The results:

There was no clipping through the EOM, but we adjusted it to better center the beam through the input and output apertures.

In recovering the RefCav, we decided to check beam alignment on the transmission PD, so I set up a LEMO splitter so we could see the DC voltage on a voltmeter.  The RefCav locked without much issue, and Ryan tweaked the beam alignment with the picomotor mirrrors.  Interestingly, the TPD voltage in MEDM did not match the voltage read by the voltmeter, so a recalibration there was necessary.  The TPD readings were not close to each other, at all, so we trended back to see the last time the TPD was calibrated.  Turns out this was at original PSL install in 2012, it hasn't been updated since.  Well then.  Alignment tweaking results:

The negative sign is normal on these PDs from AEI, as they were designed to output a negative voltage; the sign gets flipped in the MEDM filter module.  I tweaked the beam alignment on the TPD, which increased the voltmeter voltage to -0.535 V, so it was decently aligned already.  We recalibrated the MEDM reading to match the voltmeter, and updated the offset to cancel out the small dark offset observed when the TPD was blocked.  Results:

We then aligned the beam onto the RFPD and measured the RefCav visibility:

We were done in the enclosure at this point, so we exited and returned the enclosure to Science Mode.  Outside, we set up a network analyzer to measure the FSS TF.  With a common gain of 14 the FSS UGF was ~380 kHz.  We increased the common gain to 15 and the UGF was 445.6 kHz.  This is closer to where we generally like it, so we left the common gain at 15 (this can be reverted should there be an issue).  Ryan has a picture of the TF that he'll post as a comment to this alog.  With the lower, but now correct, TPD in MEDM, a couple of guardian thresholds required updating.  The TPD light on the Ops Overview screen now comes on if the TPD is less than 0.4 V and the "FSS Transmission Low" warning in DIAG_MAIN now comes on when the TPD is less than 0.3 V.  We'll monitor this over the coming days/weeks and adjust as needed.  This closes WP 12796.

Comments related to this report
ryan.short@LIGO.ORG - 16:53, Tuesday 16 September 2025 (86977)

FSS transfer function attached with a UGF of 445.6kHz (measured at -10dB as the TTFSS box always is).

Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 15:50, Tuesday 16 September 2025 (86970)
LVEA was Swept

LVEA was swept and everything looks good

H1 PSL
daniel.sigg@LIGO.ORG - posted 14:32, Tuesday 16 September 2025 - last comment - 16:12, Tuesday 16 September 2025(86966)
Thermal Effect on PSL High Power Path

Jason Ryan Jenne Daniel

We reduced the PSL power after the amplifier and before the AOM by a factor of 2.3. We then re-adjusted the power into the IMC to get back to 2W. This reduced the IMC reflected light power by ~2.7. This seems to strongly indicate that we have a heating issue in the path from the PMC to the polarizer. The following tests were run:

  1. Normal PSL setup (first screen shot)
  2. PMC input power reduced: the power was reduced with the waveplate before the ISS EOM (which is before the PMC)
  3. EOM input power reduced: the power was reduced with the waveplate between the PMC and the EOM
  4. Same as above but with enough power to lock th einterferometer at full power. The maximum IMC input power is now 70W.
  Normal PSL
setup

PMC inp
power
reduced

EOM inp
power
reduced
EOM inp
power
reduced
EOM power (W) 115 50.8 49.6 87
IMC input power (W) 2.01 2.05 2.02 2.04
IMC REFL power (mW) 1.10 0.405 0.49 0.64

 

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 14:50, Tuesday 16 September 2025 (86967)
  • During this time with reduced power in the PMC, PMC refl was 12.93 W and PMC trans was 44.86W  (28.8% is the ratio), with PSL air conditioner on.
  • Today, with normal power in the PMC,PMC refl is 24.6W,  trans is 103.7W (23.8% reflected) with the air conditioner on  trans is 104.48 (23%)
  • After the 14 hour, 60W lock where we saw degredation in the IMC visibility, the PMC refl was 24.7W trans was 104.9W, (23.5%)
  • Immediately after the power outage, PMC refl is 26.7W, while trans is 103.1W, (25.9%), then things improved (maybe when Ryan moved pico's) to 23.3%
  • before the power outage, the PMC refl was 24.0W, trans was 105.7W (22.7%)
  • The PMC refl has been slowly increasing for a while, Feb 26 2025 it was 22.2W, with 106.6 W trans (20.8%)

Attaching a trend showing that the PMC refl has been increasing gradually since Feb, and that there was a jump at the time of the power outage. 

When the power into the PMC was low, the mode matching was worse, this is probably expected due to thermal lensing in the PMC. 

Images attached to this comment
sheila.dwyer@LIGO.ORG - 16:12, Tuesday 16 September 2025 (86973)

Elenna, Sheila

Before the power outage, IM4 trans was 93% of the IMC input power.  Yesterday, we had 90% of IMC input power at IM4 trans.  Today after lowering the power through the EOM, we have 91%.

H1 DetChar (IOO)
elenna.capote@LIGO.ORG - posted 14:31, Tuesday 16 September 2025 (86968)
Glitch problem seems solved with 1/2 power on IMC REFL

The summary page finally created the omicron glitch plot for last night's 3 hours of lock. On Friday we halved the power on the IMC refl diode. Last night we locked for three hours. Here is the glitch rate from last night, which can be compared to our 10 hour lock just after the power outage which had a significantly increased glitch rate.. As a reference, here is what the glitch rate looked like a few days before the power outage. It appears the glitch rate is back to the normal level.

Images attached to this report
H1 SQZ
camilla.compton@LIGO.ORG - posted 14:31, Tuesday 16 September 2025 (86965)
SQZ to OMC scan, Similar result to August: 2.97 vs 2.17%.

Camilla

Followed setup instructions from 80010, last done in 86445. Increased to 75mW injected in the SEED beam, we had 1mW on OPO_IR_PD_DC. Have counts of ~60 and 66 on ASC-AS_A and B and 7e-4 on ASC-OMC-A and B NSUMs all similar to the August 19th measurement. To turn on the OMC ASC, H1:OMC-ASC_MASTERGAIN to 0.02. Took H1:OMC-PZT2_OFFSET goes down to -50 to start and then ran a template /sqz/h1/Templates/dtt/OMC_SCANS/ Sept16_2025_PSAMS_OMC_scan_coldOM2.xml  ref 35,36.

PSAMS settings at nominal ZM4/ZM5 6.0V / -0/4V. Measured mode mismatch of TEM02 of 2.975%. In August 86445, this was only 2.174% however in that measurement, the OMC ASC has been left off so there would have been more in the misalignment peaks.

ZM4/5 PSAMs TEM00 TEM02
Mismatch*
(% of TEM02)
6.0V / -0/4V 0.5375 0.01648 2.975%

*calculated with TEM02 / (TEM00 + TEM02)

Images attached to this report
H1 SUS (SUS)
ryan.crouch@LIGO.ORG - posted 12:02, Tuesday 16 September 2025 (86958)
ETMX OPLEV charge measurement

I tried to get a better measurement of the ETMX charge per its OPLEVs this morning, I started with a higher gain on the ESD_OUTPUT filters than the last time (0.75 instead of 0.5, 1 worked until recently). This measurement had pretty low coherence like last week so I ctrl+c and increased the drive_amp by 20%. This measurement was a little better but still not as good as I would like it, and as we have had in the past, so I restarted it again with another 20% increase in drive_amp, I ran 3 measurements with this configuration. The prelimary processing looked decent but the full processing revealed pretty large error bars still.

This measurement is better than last weeks, but there is still room for improvement. I brought the drive_amp up from 11000 to 20600 with ESD_OUTPUT gains of 0.75 and I still wasn't saturating so I still have more room to push to improve the measurements and increase the coherence.

Images attached to this report
H1 ISC (IOO)
elenna.capote@LIGO.ORG - posted 11:18, Tuesday 16 September 2025 (86964)
Comparing all powers before and after power outage

Here is a side by side of powers at the ports before and after the power outage. This is using last night's lock at 2 hours 55 minutes after the end of the max power, versus a lock before the power outage at 2 hours 55 minutes from max power.

Quantity Now Then Ratio (now/then)
IM4 trans (W on PRM) 56.5 56.0 1.008
PRG (W/W) 49.5 49.6 0.997
LSC POP A (mW on diode) 31.76 31.58 1.006
LSC REFL A (mW on diode) 7.64 7.59 1.006
OMC REFL (mW?) 684.2 698.0 0.980
X arm circ (kW) 379.4 376.2 1.008
Y arm circ (kW) 379.9 375.8 1.01
AS_C (W into HAM6) 0.680 0.695 0.978
kappa_c 0.967 0.988 0.979
f_c (Hz) 446.5 445.5  

It seems like the input power, POP, LSC REFL and circulating power numbers hang together. The OMC refl, as AS_C numbers also hang together. Sheila and I discussed that we would expect if the arm power increased the kappa c would increase, but it appears that arm power increased but kappa c decreased following the OMC refl and AS_C values.

Images attached to this report
H1 ISC
camilla.compton@LIGO.ORG - posted 10:43, Tuesday 16 September 2025 (86962)
Beam Profiles Taken of MC REFL on IOT2L

Sheila, Elenna, Camilla. WP#12797 . IOT2L layout D1300357

We took the PSL input power down to ~100mW, locked out the rotation stage and then used the nano scan to take some beam profiles in the IMC REFL path on IOT2L. Elenna and Sheila also moved a beamdump to fully block the MC REFL rejected beam that was getting on the MC REFL camera. 

Location D4 Sigma A1 Horizontal (um) D4 Sigma A2 Vertical (um) D4 Sigma A1 at 45deg (um) D4 Sigma A2 at 45deg (um)
A: Profiler 11 3/4" upstream of IO_MCR_BS1 4685 4240 4345 4450
B: Profiler 10 1/16" downstream of IO_MCR_BS1 (7" + 1 1/4" + 1 13/16") 4678 4647 4605 47921
C: Profiler 14 1/2" downstream of IO_MCR_BS1 (7" + 1 1/4" + 6 1/4") 4800 4807 4784 4676

By eye the beam looked gaussian and the numbers show it is mainly symmetric. Maybe last measurements where when the WFS were being installed in 2013 6439

For positions B and C, we added a temporary steering mirror between IO_MCR_M7 and IO_MCR_L2. Distance between IO_MCR_BS1 and IO_MCR_M7 = 7"; Distance bewtween IO_MCR_M7 = 7" and temporary steering mirror = 1 1/4". 

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:14, Tuesday 16 September 2025 (86960)
Tue CP1 Fill

Tue Sep 16 10:07:25 2025 INFO: Fill completed in 7min 21secs

 

Images attached to this report
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 22:21, Monday 15 September 2025 - last comment - 10:18, Tuesday 16 September 2025(86954)
OPS Eve Shift Summary

Literally everyone (to name who I know/can recall would be unfair)

TITLE: 09/16 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: IDLE
INCOMING OPERATOR: NONE
SHIFT SUMMARY:

IFO is in IDLE and DOWN for CORRECTIVE MAINTENANCE  buuuuut IFO was OBSERVING for ~1 hr.

Lockloss was intentional in order to avoid potential harmful lockloses and issues throughout the night. We actually got to NLN and OBSERVING though!

It's not exactly over yet - because we have only been locked for 2 hours. Problems may be there and dormant. Nevertheless, we got here from a outrageous outage recovery and a nasty ISC/Lock reacquisition that took 5 days to get back into observing.

The main things:

How we got to NLN:

Alog 86951 summarizes the lock acquisition. We just sat there for a bit at OMC_WHITENING as violins fell (and continued to)

After NLN:

LOG:

None

 

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 10:18, Tuesday 16 September 2025 (86961)

Just want to add some notes about a few of these SDFs

In this alog I accepted the TCS SIM and OAF jitter SDFs incorrectly. The safe restore had restored old values and I mixed up the "set point" and "epics value" columns here (a mistake I have made before and will likely make again). I should have reverted these values last week instead of accepting them.

Luckily, I was able to look back at Matt's TCS sim changes and I have the script that set the jitter cleaning coeffs, so I was able to reset the values and sdf them in safe. Now they are correctly SDFed in observe as well.

H1 CAL (CAL)
ibrahim.abouelfettouh@LIGO.ORG - posted 22:20, Monday 15 September 2025 - last comment - 11:07, Tuesday 16 September 2025(86955)
Post Outage Thermalized NLN BroadBand Calibration

Start Time: 1442034629

End Time: 1442034940

 

2025-09-15 22:15:22,374 bb measurement complete.
2025-09-15 22:15:22,375 bb output: /ligo/groups/cal/H1/measurements/PCALY2DARM_BB/PCALY2DARM_BB_20250916T051011Z.xml
2025-09-15 22:15:22,375 all measurements complete

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 11:07, Tuesday 16 September 2025 (86963)

Here is the pcal broadband compared to the broadband taken after we pushed the calibration on 8/28. Overall looks ok.

Images attached to this comment
H1 PSL (OpsInfo)
jason.oberling@LIGO.ORG - posted 17:07, Monday 15 September 2025 - last comment - 09:17, Tuesday 16 September 2025(86949)
PSL Inspection After Power Outage

J. Oberling, K. Kawabe

This afternoon we went into the PSL enclosure to inspect things after last week's power outage.  We concentrated on the IOO side of the PSL table, downstream of the PMC.  Our results:

We did a visual inspection with both the IR viewer and the IR-sensitive Nikon camera and did not find any obvious signs of damage on any of the optical surfaces we had access to; the only ones we couldn't see were the crystal surfaces inside the ISC EOM, we could see everything else.  I looked at the optics between Amp2 and the PMC and everything there looked normal, no signs of anything amiss.

While the beam was not perfectly centered on every optic, we saw no clipping anywhere in the beam path.  The irises after the bottom periscope mirror were not well centered, but they've been that way for a while so we didn't have a good reference for assessing alignment in that path (these irises were set after the O4 PSL upgrade, but there have been a couple of alignment shifts since then and the irises were not reset).  For reference, the beam is in the -X direction on the HWP in the power control rotation stage and in the -Z direction (but centered horizontally) on the PZT mirror after the power control stage.  We do have a good alignment reference on the ALS path (picked off through mirror IO_MB_M2, the mirror just before the ISC EOM), as those were set as part of the HAM1 realignment during this year's vent.  By my eye the first iris looked a tiny bit off in yaw (-Y direction) and pitch (+Z direction), while the second iris looked perfectly centered.  We found this odd, so Keita used the IR-sensitive camera to get a better angle on both irises and took some pictures.  With the better angle the beam looked well centered in yaw and maybe a little off in pitch (+Z direction) on that first iris, so I think my eye was influenced by the angle from which I was viewing the iris.  The second iris still looked very well centered.  Edit to add: Since the ALS path alignment looks good, to me this signals that there was not an appreciable alignment shift as a result of the change in PMC temperature.  If the PMC was the source of the alignment shift we would see it in both the main IFO and ALS paths.  If there is a misalignment in the main IFO path, its source is not the PMC.  Upon further reflection, a more accurate statement is:  If the PMC is the source of an alignment shift, the shift is too small to be seen on the PSL table (but not necessarily too small to be seen by the IMC).

The other spot of note is the entrance aperture for the ISC EOM.  It's really bright so it's hard to make a definitive determination, but it could be argued there's a very slight misalignment going into the ISC EOM.  I couldn't make anything out with the IR viewer, but Keita's picture shows the typical ring around the aperture a little brighter on the left side versus the right.  Despite this, there is no clipping in the beam, as we set up a WinCAM beam profiler to check.

The WinCAM was set behind IO_AB_L4, which is the lens immediately behind the bottom periscope mirror (this is the path that goes to the IMC_IN PD).  The attached picture shows what the beam looks like there.  No signs of clipping in the beam, so it's clearing all the apertures in the beam path.  I recall doing a similar measurement at this spot several years ago, but a quick alog search yields nothing.  I'll do a deeper dive tomorrow and add a comment should I find anything.

So to summarize, we saw no signs of damage to any visible optical surfaces.  We saw no clear evidence of a misalignment in the beam; the ALS path looks good, and nothing in the main IFO path looks suspicious outside of the ISC EOM entrance aperture (a lack of good alignment irises makes this a little difficult to assess; once we get the IFO back to a good alignment we should reset those irises).  We saw no clipping in the beam.

Keita has many pictures that he will post as a comment to this log.

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 09:17, Tuesday 16 September 2025 (86952)

For PSL table layout, see https://dcc.ligo.org/D1300348/.

  • Picture 1 and 2: PMC input coupler shows some scattering on the front surface as well as HR surface but nothing unusual. Same thing for the output coupler. (The output coupler clamp plate receives a ghost beam, Jason remembers that this was always the case.)
  • Picture 3, 4 and 5: HWP (IO-MB-HWP1) and the polarizer for the manual power adjustment, the splitter for EOM-ALS: Not centered but far from clipping.
  • Picture 6 and 7: EOM input looks a bit off-centered in YAW to the left, but not extraordinarily so. Pictured from different viewing positions to make sure that this is not some kind of photograph artifact.
  • Picture 8: EOM output. Hard to say anything except that you can see a ghost beam on the EOM case to the right of the output aperture in this picture.
  • Picture 9: Lenses look OK. Note that you see three spots in L1 but the two are actually EOM output and the ghost beam on the EOM case seen through the lens.
  • Picture 10: Corner mirror (IO-MB_M3) in front of the motorized HWP rotator.
  • Picture 11: Motorized HWP rotator. Some scattered light (?) is hitting the mount. 
  • No picture for TFPs, they were very hard to photograph, but the first TFP looked OK when viewed using the IR viewer.
  • Picture 12 shows the steering mirror below the first TFP that receives the rejected light.
  • Very hard to picture any scattered light from the periscope mirrors when the power was set to 2W. Which already tells us that there's no scattering/clipping at 1% or even 0.1% level (on these optics).
  • Could not take a picture of the PZT mirror, very hard to have a good view of the mirror surface.
  • Picture 13 and 14: These are between the L2 lens and the corner mirror, IRIS1 is close to L2 and IRIS2 is about a foot downstream. Both look pretty good, if anything the beam might be a bit high on IRIS1.
  • Picture 15: This is an iris right behind the lens for the bottom periscope mirror transmission (IO_AB_L4).  (Update later. It looks like an iris between the PZT mirror and the bottom periscope mirror though that doesn't change the conclusion.) It's off-centered, but Jason thinks that this iris was set a long, long, long time ago and cannot be trusted.
  • Picture 16: Wincam was placed between the iris pictured above and IO_AB_BS1.
    • The distance from the downstream face of the lens holder of IO_AB_L4 and the front of the the attenuator stack was measured to be 76.5mm.
    • The Wincam sensor to the front of the stack is known to be 72.3mm.
    • The post holder for Wincam was left on the table so people can put Wincam in the same position later if necessary.

 

Images attached to this comment
H1 SEI
jim.warner@LIGO.ORG - posted 13:23, Thursday 11 September 2025 - last comment - 09:53, Tuesday 16 September 2025(86859)
HAM3 H2 CPS is noisy, has been for a while

I don't really think this is related to the poor range, but it seems that one of the cps on HAM3 has excess high frequency noise and has been noisy for a while.

First image is 30+ day trends of the 65-100hz nad 130-200hz blrms for the HAM3 cps. Something happened  about 30 days ago that cause the H2 cps to get noisy at higher frequency.

Second image are rz location trends for all the HAM ISI for the last day around the power outage. HAM3 shows more rz noise after the power outage.

Last image are asds comparing HAM2 and HAM3 horizontal CPS. HAM3 H2 shows much more noise above 200hz.

Since finding this, I've tried power cycling the CPS on HAM3 and reseating the card, but that so far has not fixed the noise. Since this has been going for a while, I will wait until maintenance to try to either fix or replace the card for this CPS.

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jim.warner@LIGO.ORG - 09:53, Tuesday 16 September 2025 (86959)

I've replaced the noisy cps, and adjusted the cps setpoint to maintain the global yaw alignment, meaning I looked at the free hanging (iso loops off) position before and after the swap and changed the RZ setpoint  so the delta between the isolated and freehanging position for RZ was the same with the new sensor. New sensor doesn't show either the glitching or high frequency noise that the old sensor had. I also changed the X and Y set points, but those only changed a few microns and should not affect IFO alignment.

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