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Reports until 14:00, Tuesday 01 July 2025
H1 SUS (DetChar, ISC, OpsInfo, SUS)
jeffrey.kissel@LIGO.ORG - posted 14:00, Tuesday 01 July 2025 (85474)
Note: Alignment Changes are *Apparent* Due to Top Mass SatAmp Changes
J. Kissel, O. Patane, F. Clara
ECR E2400330

Calling this out explicitly: 
    We have changed the OSEM PD satellite amplifiers on H1SUSPRM, H1SUSPR3, H1SUSBS, H1SUSSR3, and H1SUSSRM top masses; see LHO:85463
    We chose to implement ECR E2400330 by modifying spare chassis ahead of time, and installing those modified spares in place of the old chassis (which will become some other suspensions' "new" amps next week).
    Though the ECR only changes the whitening stage frequency response.
    However, because the old vs. new chasses have different set of other overall transimpedance gain determining components, the read-back for the OSEM PDs will likely change slightly.
    Thus, the OSEMs' recast as EULER basis signals will also change slightly, *looking* like an alignment change, even though the alignment of the physical suspension will NOT have changed.
    This won't be in any consistent direction, and the transimpedance gain is determined by components that have value at any value within the components' tolerance.

I attach two examples, H1SUSPR3 and H1SUSBS, of the levels we're talking about -- In the OSEM basis, it's 1-3 [urad], and same in the EULER basis. For the beam splitter, a physical change in alignment of that magnitude would be significant, hence me bringing it up explicitly.

So, the new normal for the following suspension alignment starts on 2025-07-01 12:30 UTC:
    H1SUSPRM
    H1SUSPR3
    H1SUSBS
    H1SUSSR3
    H1SUSSRM
We'll definitely have to re-run initial alignment after today's maintenance day, given that (unrelated)
    - we rebooted the entire electronics racks at EY to replace failing power supplies,
    - we rebooted the seih23
    - we adjusted the green camera alignment
H1 SUS (SUS)
corey.gray@LIGO.ORG - posted 09:46, Tuesday 01 July 2025 (85457)
SDF Diff Post-In-Lock SUS Measurement This Morning

This morning, while waiting for Maintenance, noticed that after the In-Lock SUS Measurement, we did not "automatically" return to Observing (which would only be a few min due imminent Maintenance).  Turns out there was an ITMx SDF Diff for (H1:SUS-ITMX_L3_LOCK_L_TRAMP, see attached). 

Since it was starting to get hectic in here leading up to Maintenance, I did not do anything about this SDF and kept H1 out of Observing.

Images attached to this report
H1 SUS (SEI, SUS)
edgard.bonilla@LIGO.ORG - posted 17:42, Monday 30 June 2025 - last comment - 14:41, Tuesday 01 July 2025(85446)
Created new OSEM estimator fits for SR3 Yaw

Ivey and Edgard,

We just finshed a fit of the Yaw-to-Yaw transfer functions for the OSEM estimator using the measurements that Oli took for SR3 last Tuesday [see LHO: 85288].

The fits were added to the Sus SVN and live inside '~/SusSVN/sus/trunk/HLTS/Common/FilterDesign/Estimator/fits_H1SR3_2025-06-30.mat' . They are already calibrated to work on the filter banks for the estimator and can be installed using 'make_SR3_yaw_model.m', which lives in the same folder [for reference, see LHO: 84041, where Oli got the fits running for a test].

Attached below are two pictures of the fits we made for the estimator.

 

The first attachment shows the Suspoint Y to M1 DAMP Y fit. We made sure to fit the asymptotic behavior as well as we could, which ends up being 0.95x10^{-3} um/nm (5% lower than expected from the OSEM calibration). The zpk for this fit is

    'zpk([-0.024+20.407i,-0.024-20.407i,-0.044+11.493i,-0.044-11.493i,0,0],[-0.067+21.278i,-0.067-21.278i,-0.095+14.443i,-0.095-14.443i,-0.07+6.405i,-0.07-6.405i],-0.001)'

 

The second attachment shows the M1 drive Y to M1 DAMP Y fit. We kept the same poles that we had for the other fit, but manually fit the zeros and gain to make a good match. The zpk for this fit is

'zpk([-0.051+8.326i,-0.051-8.326i,-0.011+19.259i,-0.011-19.259i],[-0.067+21.278i,-0.067-21.278i,-0.095+14.443i,-0.095-14.443i,-0.07+6.405i,-0.07-6.405i],12.096)'

Hopefully Oli and co. will have time to test this soon!

Images attached to this report
Comments related to this report
oli.patane@LIGO.ORG - 14:41, Tuesday 01 July 2025 (85477)

The new filters have been loaded in. Here are the matlab plots for the fits for SUSPOINT_Y_2GAP and for EST_MODL_DRV_Y_2GAP.

Images attached to this comment
H1 SUS (SUS)
anthony.sanchez@LIGO.ORG - posted 17:59, Tuesday 24 June 2025 (85311)
Weekly In-Lock SUS Charge Measurement

Famis 28411 Weekly In-Lock SUS Charge Measurement.

This command is very useful to determine if the SUS charge measurements ran in the last week:
ls /opt/rtcds/userapps/release/sus/common/scripts/quad/InLockChargeMeasurements/rec_LHO  -lt | head -n 6

 

Coherence for bias_drive_bias_off is 0.06426009151210332, which is below the threshold of 0.1. Skipping this measurement
Cannot calculate beta/beta2 because some measurements failed or have insufficient coherence!
Cannot calculate alpha/gamma because some measurements failed or have insufficient coherence!
Something went wrong with analysis, skipping ITMX_13_Hz_1434811847

Images attached to this report
H1 SUS (SUS)
ryan.crouch@LIGO.ORG - posted 10:53, Tuesday 24 June 2025 (85274)
OPLEV charge measurements, ETMX, ETMY

There were some light end station VAC pump checks/disassemblies but they didn't seem to affect the measurements, the error bars are much better/smaller than the last time when it was windy out.

ETMY's charge is high (>50V) on half of the quadrants, it appears stable if we discount the previous bad measurement.

ETMX's charge is hovering within +/-10V of 50V except for LR_P, it also appears stable ignoring the previous measurement.

Images attached to this report
X1 SUS (SUS)
rahul.kumar@LIGO.ORG - posted 16:37, Monday 16 June 2025 (85097)
2nd round of B&K measurements of HRTS mounted on BBSS structure in staging building

Ibrahim, Rahul

The first round of B&K test results for BBSS & HRTS were posted in LHO alog 84654 . Now were are presenting the second round of test results after making the following improvements on BBSS - (a) added four side dampers (D1101299), two on each side, (b) two lower structure Y-brace strut - D1900589. Please see figure (IMG_2926) for reference. We have also removed the four optical posts which were earlier attached to the HRTS. Finally we attached four Vibration Absorbers (D1002424) to BBSS.

The B&K test results are attached below as a pdf document. We have taken 9 measurements with different boundary conditions, each of which is explained below. For each case the tri-axis accelerometer was mounted on the BBSS frame (marked as position P1 or P2 here) - X axis is along the longitudinal side of the BBSS, Y axis is the vertical and Z is transverse. For HRTS, it's shown in page 9 of the pdf document.

Test 1a (see page 2): case - BBSS (without HRTS) and no side dampers or Y-brace attached to BBSS, Accelerometer position P1.

Test 1b (see page 3): case - BBSS & HRTS and no side dampers or Y-brace attached to BBSS, Accelerometer position P1.

Next ,side dampers and Y-brace attached.

Test 2a (see page 5): case - BBSS & HRTS with side dampers and Y-brace attached to BBSS (No Vibration Absorbers), Accelerometer position P1. Hammer hits on the center of the structure.

Test 2b (see page 6): case - BBSS & HRTS with side dampers and Y-brace attached to BBSS (No Vibration Absorbers), Accelerometer position P2. Hammer hits on the center of the structure.

Test 3 (see page 7): case - BBSS & HRTS with side dampers and Y-brace attached to BBSS (No Vibration Absorbers), Accelerometer position P1. Hammer hits on the side of the structure (left or right).

Test 4 (see page 8): case - BBSS & HRTS with side dampers and Y-brace attached to BBSS (No Vibration Absorbers), Accelerometer position P2. Hammer hits on the side of the structure (left or right).

Test 5 (see page 9): case - BBSS & HRTS with side dampers and Y-brace attached to BBSS (No Vibration Absorbers), Accelerometer attached to HRTS. Hammer hits on HRTS.

Next ,side dampers Y-brace and Vibration Absorbers attached.

Test 6a (see page 11): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the center of the structure (X axis or longitudinal direction).

Test 6b (see page 12): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the center of the structure (Y axis or vertical direction).

Test 6c (see page 13): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the center of the structure (Z axis or transverse direction).

Test 7a (see page 14): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the side of the structure (X axis or longitudinal direction).

Test 7b (see page 15): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the side of the structure (Y axis or vertical direction).

Test 7c (see page 16): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P1. Hammer hits on the side of the structure (Z axis or transverse direction).

Test 8a (see page 17): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the center of the structure (X axis or longitudinal direction).

Test 8b (see page 18): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the center of the structure (Y axis or vertical direction).

Test 8c (see page 19): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the center of the structure (Z axis or transverse direction).

Test 9a (see page 20): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the side of the structure (X axis or longitudinal direction).

Test 9b (see page 21): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the side of the structure (Y axis or vertical direction).

Test 9c (see page 22): case - BBSS & HRTS with side dampers, Y-brace attached to BBSS and Vibration Absorbers, Accelerometer position P2. Hammer hits on the side of the structure (Z axis or transverse direction).

 

The raw data (.csv files) generated by the B&K software are stored at the following location,

/ligo/home/rahul.kumar/Desktop/scripts/bnk_csv_files

Images attached to this report
Non-image files attached to this report
H1 General (ISC, OpsInfo, SEI, SUS)
elenna.capote@LIGO.ORG - posted 15:40, Monday 16 June 2025 - last comment - 17:03, Monday 16 June 2025(85092)
Safe SDF reconciliation

In preparation for the RCG upgrade, we are using the relocking time to reconcile SDF differences in the SAFE file.

Here are some of mine:

I have also determined that the unmonitored channel diffs in the LSC, ASC, and OMC models are guardian controlled values and do not need to be saved.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 15:29, Monday 16 June 2025 (85094)

Not accepting or reverting the h1sqz, h1ascsqzfc, or slow controls cs_sqz sdfs, attached. As these have the same observe and safe files.

Images attached to this comment
camilla.compton@LIGO.ORG - 15:35, Monday 16 June 2025 (85095)

Accepted  H1:TCS-ETMX_RH_SET{LOWER,UPPER}DRIVECURRENT as  ndscope-ing shows they are normally at this value.

Images attached to this comment
elenna.capote@LIGO.ORG - 17:00, Monday 16 June 2025 (85103)

Some of these SDFs may have then led to diffs in the OBSERVE state. I have reverted the roll mode tRamp, and accepted the OSC gains in the CAL CS model.

Images attached to this comment
oli.patane@LIGO.ORG - 17:03, Monday 16 June 2025 (85104)

I updated the OPTICALIGN OFFSETs for each suspension that we use those sliders on. I tried using my update_sus_safesnap.py script at first, but even though it's worked one other time in that past, it was not working anytime I tried using it on more than one suspension at a time (it seems like it was only doing one out of each suspension group). I ended up being able to get them all updated anyway eventually. I'm attaching all their sdfs and will be working on fixing the script. Note that a couple of the ETM/TMS values might not match thesetpoint exactly due to the screenshots happening during relocking and after they had moved a bit with the WFS

Images attached to this comment
H1 SUS (SUS)
corey.gray@LIGO.ORG - posted 02:32, Saturday 14 June 2025 (85041)
ITMx MODE13

Before going back to bed, wanted to check violins, and noticed that ITMx MODE13 was ringing up again.  I'm guessing the settings RyanC had going were not being used.  So, I put in what RyanC had 2hrs ago for the last lock, and within 2min, it quickly damped out the rung up MODE13.

I have NOT made a change/updated lscparams.

NEW Settings

ITMx MODE13:  FM1 + FM4 + FM10 + gain = -0.2

OLD Settings:

ITMx MODE13:  FM1 + FM2 + FM4 + FM10 + gain = 0.0

OK, going back to bed.  Sleep...we'll see.

H1 General
ryan.crouch@LIGO.ORG - posted 22:06, Friday 13 June 2025 - last comment - 23:49, Friday 13 June 2025(85028)
OPS Friday EVE shift summary

TITLE: 06/14 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Aquisition
INCOMING OPERATOR: Corey
SHIFT SUMMARY: A quaternary of issues, environmental (wind and an earthquake), hardware, and software it seems. The new DAMP_BOUNCE_ROLL seems to be killing it everytime it engages so I've commented it out.
LOG:                                       

Start Time System Name Location Lazer_Haz Task Time End
15:22 FAC LVEA is LASER HAZARD LVEA YES LVEA is LASER HAZARD \u0d26\u0d4d\u0d26\u0d3f(\u239a_\u239a) 05:18
00:46 OMC Keita LVEA Y Investigate OMC PZT 00:56
Images attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 22:50, Friday 13 June 2025 (85036)

I checked the screenshots when I got home and saw that we had been sitting in DAMP_BOUNCE_ROLL for ~20 minutes with the state completed, so I hopped on and requested it to move on to NLN, I'm not sure why H1_MANAGER wasn't moving it on as the REQUEST was set to NLN as it should have been.

ryan.crouch@LIGO.ORG - 23:49, Friday 13 June 2025 (85037)SUS

ITMX13 decided it didn't want to damp again, so I had to find some new settings. FM1 + FM4 + FM10 G = -0.2 seems to be working. I've set its gain to zero in lscparams in the meantime and reloaded the node.

H1 AOS (DetChar, SUS)
kiet.pham@LIGO.ORG - posted 16:28, Friday 13 June 2025 - last comment - 12:45, Tuesday 17 June 2025(85026)
Violin mode contaimination near 500Hz: possible mixxing between the 2nd harmonic (near 1500 Hz) and the 1st harmonic (near 1000 Hz)

Kiet and Sheila,

Following up on the investigation posted in aLOG 84136, we examined the impact of higher-order violin mode harmonics on the contamination region.

We found that subtracting the violin peaks near 1000 Hz (1st harmonic) from those near 1500 Hz (2nd harmonic) results in frequency differences that align with many of the narrow lines observed in the contamination region around 500 Hz.

Violin peaks that we used (using O4a+b run average spectra)

F_n1 = {1008.69472,1008.81764, 1007.99944,1005.10319,1005.40083} Hz 
F_n2 = {1472.77958,1466.18903,1465.59417,1468.58861, 1465.02333, 1486.36153, 1485.76708} Hz 

Out of the 35 possible difference pairs (one from each set), 27 matched known lines in the contamination region to within 1/1800 Hz (~0.56 mHz)—most within 0.1 mHz. Considering that each region actually contains >30 peaks, the number of matching pairs likely increases significantly, helping explain the dense forest of lines in the comtaimination region.

Next steps:

The Fscan run average data are available here (interactive plots): 

Fundamental region (500 Hz): 

1st harmonic region (1000 Hz): 

2nd harmonic region (1500 Hz): 

Comments related to this report
kiet.pham@LIGO.ORG - 12:45, Tuesday 17 June 2025 (85127)DetChar, SUS

Adding plot comparing the PSDs before and after getting rid of the peaks that can be indentified by this method.

Images attached to this comment
H1 General
ryan.crouch@LIGO.ORG - posted 16:03, Friday 13 June 2025 - last comment - 18:51, Friday 13 June 2025(85020)
OPS Friday EVE shift start

TITLE: 06/13 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 17mph Gusts, 11mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.12 μm/s
QUICK SUMMARY:

Images attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 18:51, Friday 13 June 2025 (85031)SUS

We've lost lock at POWER_10Ws twice in a row, within a 5 seconds of entering the state. I'm worried of how rung up the violins will be now, as they looked large right before the 2nd lockloss. I'm going to stop at CHECK_VIOLINS on my way up now. Both locklosses tag ADS_EXCURSION

H1 GRD (ISC, OpsInfo, SUS)
corey.gray@LIGO.ORG - posted 02:19, Friday 13 June 2025 - last comment - 08:21, Friday 13 June 2025(85010)
OWL Shift Wake Up Due To SDF Diffs for LSC & SUSETMY---REVERTED & Back To Observing

Received phone call at 1:20amPDT.

Saw that H1 was at NLN, and ready to go to Observing, but could not due to SDF Diffs for LSC & SUSETMY (see attached screenshot):

1) LSC

I was not familiar with these channels, so I went through the exercise of trying to find their medm, but for the life of me I could not get there!  The closest I got was LSC Overview / IMC-MCL Filter Bank, but they were not on that medm.  (probably spent 30min looking everywhere and in between with no luck).   Looked at these channels in ndscope & these channels were at their nominals for the last lock.  Also looked in the alog, and only saw SDF entries for them from 2019 & 2020.  Ultimately, I just decided to do a REVERT (and luckily, H1 did not lose lock).

2) SUSETMY

Then H1 automatically went back to Observe.

Maybe Guardian, for some reason took these channels to these settings?  At any rate, going to try to go back to sleep since it has been an hour already (hopefully this does not happen for the next lock!).

Images attached to this report
Comments related to this report
ryan.short@LIGO.ORG - 08:21, Friday 13 June 2025 (85012)ISC, OpsInfo

These MCL trigger thresholds come from the IMC_LOCK Guardian and are set in the 'DOWN' and 'MOVE_TO_OFFLINE' states.

In 'DOWN', the trigger ON and trigger OFF thresholds are set at 1300 and 200, respectively, for the IMC to prepare to lock as seen in the setpoints from Corey's screenshot.

In 'MOVE_TO_OFFLINE', the trigger ON and trigger OFF thresholds are set at 100 and 90, respectively (for <4W input), as seen in the EPICS values from Corey's screenshot.

So, it would seem that after the lower thresholds were set when taking the IMC offline sometime recently, they were incorrectly accepted in SDF. I'll accept them as the correct values in the OBSERVE.snap table once H1 is back up to low noise, as I expect they'll show up as a difference again.

H1 General (Lockloss)
ibrahim.abouelfettouh@LIGO.ORG - posted 14:42, Thursday 12 June 2025 - last comment - 16:52, Thursday 12 June 2025(85004)
Lockloss 20:16 UTC

Lost lock due to the ETM Glitch while commissioning.

Comments related to this report
oli.patane@LIGO.ORG - 16:52, Thursday 12 June 2025 (85006)ISC, SUS

2025-06-12 23:39 UTC Back to Observing

Accepted sdfs for SUSPROC (filter for Roll modes) and for LSC (IMC-MCL_FM_TRIG thresholds) to get into Observing. Control room at the time didn't know who changed the MCL thresholds, so I just accepted them.

Images attached to this comment
H1 General (SUS)
anthony.sanchez@LIGO.ORG - posted 08:02, Thursday 12 June 2025 - last comment - 09:14, Thursday 12 June 2025(84991)
Thursday morning Ops shift start

TITLE: 06/12 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 144Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 6mph Gusts, 4mph 3min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.11 μm/s
QUICK SUMMARY:

H1 is still locked and has been for 5 hours and 45 minutes.
But the DCPDs are diverging again, Like there is some sort of Roll mode ring up again.
Turns out its the Same Roll mode from yesterday. I applied the same gain from yesterday to the roll mode and it has turned around immediately. I have accepted this as an SDF Diff so we can stay observing.
GRB-Short E573164 @ 1454 UTC stand down

it has been requested of me to run the PSAMS script if we were still locked this morning. Camilla just walked and I her and I will start working on PSAMs when the Stand Down ends.

 

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:14, Thursday 12 June 2025 (84993)

Dropped out of Observing for Commissioning at 15:51UTC. Optimistic plan for commissioning time today:

  • [Camilla] PSAMS Scan, aim to make SQZ better over all frequencies
  • [Robert] Remove VP covers and photo, aim to evaluate CPY move
  • [Elenna] LSC FF edits to avoid ETM Roll Mode ring up
  • [Robert] HAM1 Shaker, other PEM injections.
  • [Kevin] 10kHz ADF Injections, aim to understand HOMs
  • [Sheila+OPS] OMC alignment checks
  • [Kevin] SQZ ADF sweep, aim to understand SQZ/IFO
  • [Camilla,Sheila] SQZ data set, aim to understand SQZ
  • [Sheila,Elenna,Jennie] Noise Budget injections, aim to see Jitter, Intensity and ASC contributions.
X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 15:38, Tuesday 10 June 2025 (84942)
BBSS Transportation (Container, Support Plate and Lifting Bar) Tested

Randy, Ibrahim

Today, Randy an I fit checked the BBSS Structure Support Plate (D2500013) and the Lifting Bar Assembly (D1100802) for the BBSS. 

Overall, everything fit. See pictures below. Some relevant notes:

Images attached to this report
H1 ISC
camilla.compton@LIGO.ORG - posted 10:34, Tuesday 10 June 2025 - last comment - 16:59, Wednesday 25 June 2025(84922)
Noticed BS PIT Moved while locking and then drifts in NLN: not new, happened end of O3b but not 1 year ago.

Sheila, Elenna, Camilla

Sheila was questioning if something is drifting for us to need an initial alignment after the majority of relocks. Elenna and I noticed that BS PIT moves a lot both while powering up /moving spots and while in NLN. Unsure from the BS alignment inputs plot what's causing this.

This was also happening before the break (see below) but the operators were similarly needing more regular initial alignments before the break too.  1 year ago this was not happening, plot.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 12:44, Tuesday 10 June 2025 (84929)

These large BS PIT changes began 5th to 6th July 2024 (plot). This is the day shift from the time that the first lock like this happened 5th July 2024 19:26UTC (12:26PT): 78877 at the time we were doing PR2 spot moves. There also was a SUS computer restart 78892 but that appeared to be a day after this started happening.

Images attached to this comment
camilla.compton@LIGO.ORG - 09:45, Wednesday 11 June 2025 (84966)ISC, SUS

Sheila, Camilla

This reminded Sheila of when we were heating a SUS in the past and causing the bottom mass to pitch and the ASC to move the top mass to counteract this. Then after lockloss, the bottom mass would slowly go back to it's nominal position.

We do see this on the BS since the PR2 move, see attached (top 2 left plots). See in the green bottom mass oplev trace, when the ASC is turned off on lockloss, the BS moves quickly and then slowly moves again over the next ~30 minutes, do not see simular things on PR3. Attached is the same plot before the PR2 move. And below is a list of other PR2 positions we tried, all the other positions have also made this BS drift. The total PR2 move since the good place is ~3500urad in Yaw.

  • Different time May 21st to 24th 2024:
    • BS Oplev Drift
    • Plot shows 30urad M1 drift
    • PR2 Alignment Sliders P: 1435, Y: 1130
  • Pre July 5th 2024:
    • No BS Oplev Drift
    • Plot shows 5urad M1 drift
    • PR2 Alignment Sliders P: 1565, Y: 3210
  • July 5th 2024 to 6th Feb 2025:
    • BS Oplev Drift
    • Plot shows 50urad M1 drift
    • PR2 Alignment Sliders P: 1535, Y: 2785
  • 6th Feb 2025 to 10th Feb 2025:
    • BS Oplev Drift
    • Plot shows 30urad M1 drift
    • PR2 Alignment Sliders P: 1480, Y: 1195
  • 10th Feb 2025 to now:
    • BS Oplev Drift
    • Plot shows 30-40urad M1 drift
    • PR2 Alignment Sliders P: 1430, Y: -245

To avoid this heating and BS drift, we should move back towards a PR2 YAW of closer to 3200. But, we moved PR2 to avoid the spot clipping on the scrapper baffle, e.g.  77631, 80319, 82722, 82641.

Images attached to this comment
jenne.driggers@LIGO.ORG - 14:38, Thursday 12 June 2025 (85002)

I did a bit of alog archaeology to re-remember what we'd done in the past.

  • In August of 2015, we found that we were struggling with PR3 pitch alignment jumping, then cooling down upon lockloss.  Alog 20268 talks about the implementation of the lock loss compensation, which first appeared in ISC_DRMI guardian in rev 11228.
  • At some point (I didn't dig to find out when precisely), we also implemented the same filters for BS pitch.
  • By Jan 2020, both BS and PRM had the soft ASC turn-off.
  • In Jan 2020, ISC_DRMI rev 20905 we removed this soft ASC turn-off for both PR3 and BS.  The referenced alog 54709 notes that we shouldn't need those anymore, since we had installed wire heating baffles, to prevent the wires from being illuminated and heating up.
  • We haven't had the soft turn-off filters in use since 2020, about 3 months before the end of O3b.  This may be why Camilla saw that we were seeing BS drift at the end of O3b.
  • Perhaps our alignment during O4, until we moved the PR spots in May 2024, was such that we weren't susceptible to this wire heating.
  • I don't think PR3 is seeing the same kind of trouble that it did back in 2015 upon lockloss, so I think its wire heating baffles are working as designed, so no need to make any changes to the PR3 controls.
  • Sheila made the point that because we unclipped some of the +Y side of the beam (without moving the spot on the BS), maybe there is a bit more light that is illuminating the barrel of the BS or getting to the wires.  Or, something?  Without having looked at the actual drawings, I could imagine that the wire heating baffles are working better on PR3 than they are on the BS, because we hit PR3 much closer to normal incidence, whereas with the BS the light could be sneaking around the baffles.  Robert thinks that light could get inside the cage baffle and reflect around and be hitting and heating the wires.
  • All of this seems to say that we should re-implement the soft ASC turn-off for the BS. I had a quick look at the 1/e time for the BS to move after lockloss (it's about 241 seconds), and the 1/e time for the filters (about 240 seconds, despite my quoting in alog 54706 that they were 25 min filters (2*pis are hard!)

To put back the soft turn-off of the BS ASC, I think we need to:

  • Disable the BS M1 ASC lockloss trigger.  Jeff reminded me that this would foil my plans, since it turns off the ASC signals to the EUL2OSEM matrix.  This will mean that neither the Pit nor the Yaw BS M1 signals will be shut off by the lockloss trigger.  To disable, we'll need to set H1:SUS-BS_M1_TRIG_ASC_ENABLE to zero (which means that the ASC signals will always be passed to the EUL2OSEM matrix).  I don't think this is in guardian anywhere, so we should only need to change it and then accept in safe and observe snap files.
  • Change ISC_DRMI around line 66 such that BS pit gain is not set to zero.  Also, have it turn off FM1 in addition to turning off the input.
  • Change ISC_DRMI around line 141 to not hit the BS pit RSET button.

Camilla made the good point that we probably don't want to implement this and then have the first trial of it be overnight.  Maybe I'll put it in sometime Monday (when we again have commissioning time), and if we lose lock we can check that it did all the right things.

jenne.driggers@LIGO.ORG - 09:57, Monday 16 June 2025 (85075)

I've now implemented this soft let-go of BS pit in the ISC_DRMI guardian, and loaded.  We'll be able to watch it throughout the day today, including while we're commissioning, so hopefully we'll be able to see it work properly at least once (eg, from a DRMI lockloss).

jenne.driggers@LIGO.ORG - 17:16, Monday 16 June 2025 (85106)

This 'slow let-go' mode for BS pitch certainly makes the behavior of the BS pit oplev qualitatively different. 

In the attached plots, the sharp spike up and decay down behavior around -8 hours is how it had been looking for a long time (as Camilla notes in previous logs in this thread).  Around -2 hours we lost lock from NomLowNoise, and while we do get a glitch upon lockloss, the BS doesn't seem to move quite as much, and is mostly flattened out after a shorter amount of time.  I also note that this time (-2 hours ago) we didn't need to do an initial alignment (which was done at the -8 hours ago time).  However, as Jeff pointed out, we held at DOWN for a while to reconcile SDFs, it's not quite a fair comparison. 

We'll see how things go, but there's at least a chance that this will help reduce the need for initial alignments.  If needed, we can try to tweak the time constant of the 'soft let-go' to further make the optical lever signal stay more overall flat.

The SUSBS SDF safe.snap file is saved with FM1 off, so that it won't get turned back on in SDF revert.  The PREP_PRMI_ASC and PREP_DRMI_ASC states both re-enable FM1 - I may need to go through and ensure it's on for MICH initial alignment.

Images attached to this comment
jenne.driggers@LIGO.ORG - 16:59, Wednesday 25 June 2025 (85344)

RyanS, Jenne

We've looked at a couple of times that the BS has been let go of slowly, and it seems like the cooldown time is usually about 17 minutes until it's basically done and at where it wants to be for the next acquisition of DRMI.  Attached is one such example.

Alternatively, a day or so ago Tony had to do an initial alignment.  On that day, it seemed like the BS took much longer to get to its quiescent spot.  I'm not yet sure why the behavior is different sometimes.

Tony is working on taking a look at our average reacquisition time, which will help tell us whether we should make another change to further improve the time it takes to get the BS to where it wants to be for acquisition.

Images attached to this comment
H1 General
anthony.sanchez@LIGO.ORG - posted 07:42, Tuesday 10 June 2025 - last comment - 12:36, Wednesday 11 June 2025(84914)
Tuesday Ops Day Shift - A Light Maintenance Day.


TITLE: 06/10 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 4mph Gusts, 1mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.18 μm/s
QUICK SUMMARY:
H1 was in IDLE when I arrived.
I will start trying to lock now.
 

Comments related to this report
ryan.crouch@LIGO.ORG - 12:41, Tuesday 10 June 2025 (84931)SUS

I've changed the sign of the damping gain for ITMX 13 in lscparams from +0.2 to -0.2 after seeing it damp correctly in 2 lock stretches. The VIOLIN_DAMPING GRD could use a reload to see this change.

rahul.kumar@LIGO.ORG - 12:36, Wednesday 11 June 2025 (84979)

I have loaded the violin damping guardian, since the setting RyanC found still works.

X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 15:56, Monday 09 June 2025 - last comment - 16:31, Monday 09 June 2025(84904)
BBSS Vibration Absorber Installed

Ibrahim, Rahul

Rahul and I installed the BBSS Vibration Absorbers. We then took more B&K measurements and Rahul is analyzing them. Pictures attached.

Images attached to this report
Comments related to this report
rahul.kumar@LIGO.ORG - 16:31, Monday 09 June 2025 (84910)SUS

The above are D1002424, FM/BS config. (see page 2 of the document, top right figure for reference). 

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