Sheila, Ibrahim
PRMI locking waited a long while with high counts before going into MICH so Sheila changed the timer from 20 mins to 10 mins.
Lockloss seemingly due to ground motion instability. In the last 6 hours, the microseism increased by an order of magnitude.
PRG and ASC signals have been oscillating every few minutes since I started shift (and seismic was in micreoseism).
TITLE: 10/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 7mph Gusts, 4mph 3min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.50 μm/s
QUICK SUMMARY:
IFO is in NLN and OBSERVING as of 05:22 UTC
Range and wind are stable. Microseism is on the rise.
Plan is to stay OBSERVING
TITLE: 10/17 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Tony
SHIFT SUMMARY: Relocking and at MOVE_SPOTS. We were having a bit of a rough start trying to relock after the lockloss - for the first few minutes ALSX was buzzing weirdly, but then it went away on its own. I briefly checked the quad movements, and it looks like it may have been caused by ETMX Y moving to adjust the alignment. We then were having trouble locking DRMI or PRMI, so eventually I started an initial alignment and that helped a lot.
LOG:
23:30UTC Observing and have been Locked for 1 hour
23:49 Earthquake mode activated
23:50 Out of Observing to run ASC Hi Gains
23:59 GRB-Short E610763 https://gracedb.ligo.org/events/E610763/view/
00:09 Back into Observing after going back to nominal gains
00:09 Back to CALM
03:06 Lockloss https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=87534
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 23:32 | Jennie | JOAT | n | Putting away wipes | 23:35 |
Lockloss at 2025-10-17 03:06 UTC after over 4.5 hours Locked. Unsure of cause.
TITLE: 10/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY: The DARM fom struggled this morning as it wasn't getting data from GDS and sometimes nds2, ETMY beam spot adjustment alog87508, and we had to swap the ITMY L2 sat amp box alog87515. A PRM filter was also turned off alog87523, and I accepted some CDS calibration report related SDFs. After we relocked post sat amp swap there was a 1Hz ringup seen in ASC, but it calmed down.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 15:01 | FAC | Randy | Yarm beam tube | N | Beam tube inspection, mid to corner | 17:56 |
| 15:04 | FAC | Kim , Nellie | VAC prep lab | N | Tech clean | 15:31 |
| 18:19 | ISC | Jennie | Vac Prep lab | N | Looks for parts | 19:30 |
| 18:23 | FAC | Kim, Nellie | Receiving, then Mids | N | Tech clean and look for stuff | 18:49 |
| 18:25 | PSL | Keita | Optics lab | N | ISS array, Laser Safe | 19:43 |
| 18:32 | PSL | Rahul | Optics lab | N | Join Keita | 19:43 |
| 19:04 | FAC | Eric | Staging | N | Move boom lift to LeXi | 19:29 |
| 20:06 | EE | Fil | LVEA | N | ITMY L2 sat amp swap | 20:16 |
| 20:39 | FAC | Randy | Xarm | N | Beamtube calking | 22:10 |
| 21:06 | PSL | Jennie | Optics lab, Vac prep | N | Check for parts/tools/cleanliness, Laser Safe | 22:00 |
| 21:34 | SUS | Rahul | LVEA, near PSL | N | Grab parts | 21:47 |
| 21:45 | PSL | Keita | Optics lab | N | ISS array work | 23:09 |
TITLE: 10/16 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 13mph Gusts, 9mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.16 μm/s
QUICK SUMMARY:
Observing at 150 Mpc and have been Locked for 1 hour. Looks like everything is going well now.
J. Kissel
The ETMs have L2 to R0 "tracking" in longitudinal (in addition to pitch and roll "damping") L2 sensing to R0 actuation. It's referred to as "tracking" rather than "damping" because the open loop gain is greater than unity over a much broader frequency region, focusing around 0.1 Hz.
These, like the P and R damping, didn't change after the sat amp swaps.
The templates to take this data lives here:
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAGR0/Data
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_L.xml
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMX/SAGR0/Data
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_L.xml
J. Kissel, S. Dwyer, E. Capote We recently re-discovered that H1SUSPRM M3 DRIVEALIGN matrix has an L2P filter ON with gain of -1.36 that was designed in 2014 (see LHO:9589). Unsure of its function/performance with the modern IFO, we wanted to test turning it OFF. We turned it OFF (by ramping the gain in that bank to 0.0 with a 10 sec ramp time) at the end of the most recent lock stretch, with the IFO in nominal low noise (just after Elenna's calibration push; LHO:87520). Namely the IFO was suffering from a failed H1 SUS ITMY PUM sat amp, and we knew we needed to replace it, so we were looking for "useful" ways to break the lock. Turning off the H1 SUS PRM M3 DRIVEALIGN L2P filter, at first superficial glance, has no impact on the IFO excpet for reducing the M3 pitch drive from +/- 300 to +/- 2 (Euler Basis) DAC Counts. For more in-depth analysis, - 2025-10-16 18:45 UTC the problems with the ITMY satamp started - 2025-10-16 19:54 UTC we turned off the PRM M3 L2P filter, and - 2025-10-16 20:02 UTC I caused the IFO lock loss by inverting the polarity on IN2 of the IMC common mode board. So, we should have a good 5 minutes of time right before vs. right after to compare ISC ASDs. We also tried this next lock acquisition with the filter OFF, to see if it's still needed for lock acquisition. PRMI isn't locking after 10 minutes of trying (*after* going through MICH fringes), though we did NOT run an initial alignment prior to this lock attempt and the AS port does look a little splotchy. Turned it back on 2025-10-16 20:39:44 UTC, but pretty quickly decided to run initial alignment instead (by 2025-10-16 20:42:57 UTC). We'll leave it ON and test more / again some other day; we'd rather get back to observing.
Turned off again at 21:15:30 UTC. SDF.
I don't see any difference in ISC signals (PRC2, PRCL, MICH ASC, REFL SERVO) from this change.
We made it through our second attempt at DRMI locking with the usual amount of difficulty. It's not obvious to me how this filter could impact our DRMI locking, since it's a length-to-pitch decoupler and the impact to locking should be in length only. DRMI ASC engaged with no issues.
Observe
18:45 UTC While Jim was running a measurement on ISI HAM5, SUS ITMY started to flash its' red Rocker Switch Death on L2 and report that its' L2 OSEMs were in fault, we also noticed there's a big new line at ~92Hz. Jeff turned off feedback from L2. It looks like it could be a sat amp issue, the L2 sat amp was upgraded this past Tuesday alog87469. Jeff is starting to work on characterizing a sat amp box in the EE shop to swap in.
We would need a lockloss to swap this component.
We are going to try to go back into Observing for a bit until we can fix it or lose lock.
19:31 UTC Observing
FYI -- we went into observing with the ITMY PUM sat amp OSEM PD's still dead. We turned OFF the ITMY L2 (PUM) to R0 "damping" feedback loop, so the failed sensors *should* not have any impact on the IFO. However, an obvious, loud ~92-93 Hz feature remained new and glaringly obvious in the DARM sensitivity.
@DetChar / @CW Group Probably best to just veto this observation stretch, unless we -- in the future -- find some amazingly exceptional event.
2025-10-16 19:31 UTC to 19:54 UTC.
ITMY L2 (PUM) Sat Amp S1100148 installed on 10/14/2025. Replaced on 10/16/2024 with S1100080.
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=87469
J. Kissel This past Tuesday (Oct 14 2025), we upgraded the L2 (PUM) OSEM PD Sat Amps to improve their whitening filter, per ECR E2400330; see LHO:87469. These QUAD L2 PUM OSEMs (in which the flags are on the QUADs main chain PUM, and the LED & PD are on the reaction chain PUM [aka the "PenRe"]) are used in feedback. This "damping" of a "3.3" Hz reaction chain resonance is different ITMs and ETMs (ITM Install = LHO:65728; ETMs Install = LHO:68012 --- commissioning of both = LHO:68200); the ITM has resonances at 3.28 / 3.31 Hz and the ETM has modes at 3.18 Hz / 3.42 Hz. Because the improved sat amps come with better compensation of the whitening filter frequency response, we know that the frequency dependent gain on each channel -- especially around 3.3 Hz may change by as much as ~10%. In the aLOG (and comments collection) I report (a) That we *did* see a change in the open loop gain TFs of these loops, but (after ~2 days of observing since the upgrade) the IFO doesn't seem to mind the changes. (b) We were able to get better coherence on the open loop gain TFs in the 0.1 to 10 Hz region because of the sat amp whitening improvement (c) A comparison between all four QUAD's PITCH and YAW damping, so that we might understand them better and potentially improve them. In this main aLOG I show the comparison between the PITCH and ROLL open loop gain TFs and loop suppression for all four QUADs. Rushed commentary: - The surprising thing to me is that we're getting gain peaking and/or some suppression of other modes below 1 Hz, which I'm confident was not the design intent. - Even though the filters and EPICs gains are the same for EX and EY, ETMX has a lot more open loop gain below 1 Hz. - Also though the ETM loop suppression is about the same on these 3.18 / 3.42 Hz, the ITM loops have pretty different amount of gain peaking. - I'm guessing we *don't* want this much sharp gain peaking just *off* the "3.3" Hz mode.
Here's the EPICs configurations, gains, and frequency response for L2DAMP filters. In foton, I added a temporary filter that multiplied in the EPICs gain in use (including the sign) for plotting/comparison purposes. As shown, the ITM filter and overall gain design is identical between ITMX and ITMY, and the ETM filter design and overall gain is identical between ETMX and ETMY.
ITMX Before vs. After Sat Amp Swap Open Loop Gain and Loop Suppression plots for PITCH and ROLL.
As advertised -- no substantial change. The overall magnitude of PITCH open loop gain dropped by 18% between 0.5 and 3 Hz, but I suspect this is actually a clean-up of the compensation or frequency dependent calibration rather than a "real" gain drop. Since this all happens below the intended functional frequency, there's little to no change in functional loop suppression, save a little bit *less* gain peaking at 3.3 Hz.
The templates for taking this this before vs. after data lives in
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMX/SAGR0/Data/
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P.xml
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R.xml
and to make the comparison in the main aLOG entry, I exported the results to
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMX/SAGR0/Data/
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_OpenLoopGain_tf.txt
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSITMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_OpenLoopGain_tf.txt
ITMY Before vs. After Sat Amp Swap Open Loop Gain and Loop Suppression plots for PITCH and ROLL.
Even less change than ITMX -- arguably none at all to within the precision [i.e. coherence] of the measurement.
The templates for taking this this before vs. after data lives in
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGR0/Data/
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P.xml
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R.xml
and to make the comparison in the main aLOG entry, I exported the results to
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGR0/Data/
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_OpenLoopGain_tf.txt
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSITMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_OpenLoopGain_tf.txt
ETMX Before vs. After Sat Amp Swap Open Loop Gain and Loop Suppression plots for PITCH and ROLL.
Arguably no change -- and the measurement coherence is better *after* in the 0.5 to 5 Hz band because of the improved whitening on the L2 OSEM PDs.
The templates for taking this this before vs. after data lives in
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMX/SAGR0/Data/
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P.xml
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R.xml
and to make the comparison in the main aLOG entry, I exported the results to
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMX/SAGR0/Data/
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_OpenLoopGain_tf.txt
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSETMX_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_OpenLoopGain_tf.txt
ETMY Before vs. After Sat Amp Swap Open Loop Gain and Loop Suppression plots for PITCH and ROLL.
Similar to ETMX -- arguably no change at all in open loop gain or loop suppression to within the measurement precision i.e. coherence.
The templates for taking this this before vs. after data lives in
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAGR0/Data/
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P.xml
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R.xml
and to make the comparison in the main aLOG entry, I exported the results to
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAGR0/Data/
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_P_OpenLoopGain_tf.txt
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_LoopSuppression_tf.txt
2025-10-14_1830UTC_H1SUSETMY_R0_WhiteNoise_0p02to50Hz_L2DAMP_OLGTF_R_OpenLoopGain_tf.txt
Summary: Since we have made many changes to DRMI over the last few weeks and locking is much slower than it was, I started trying to restore us to the old configuration which worked pretty well. We have locked DRMI 6 times since, none of the acquisitions have taken longer than 8 minutes. (see second attachment)
Lesson for the future:
We should be much more careful about making changes to DRMI acquisition, and look at locking statistics to evaluate whatever we do.
TJ Massinger pointed out that there is a page that already displays times, ISC_LOCK summary. If you scroll to the bottom and click on the state LOCK_DRMI_1F [101] you can see a list of the locking attempts and their duration. Craig and I used this data to make the histograms in the second attachment. We were locking much more quickly in Sept 9-12 than in the first days of October, and after making the changes tonight the times are closer to what we had in mid September although the distribution will probably not be as good.
I think our approach going forward should be to wait a few days after making a change, and get several tens of locking attempts for statistics before we make a change. If we compare the locking statistics before and after the change, and they are better, we can go ahead try another change if we want to then.
Details:
I compared changes in the DRMI acquisition settings for LSC using conlog. The two times are used are Sept 12 2018 at 21:43 (1220823832), this was a week when we remember DRMI locking quickly and looking back at the data confirms that it was locking quickly. Now DRMI locking is consuming a lot of time, and we have made many changes and aren't sure which of the changes made are the problem.
| Sept 12 | Oct 4th | changes made tonight | |
| POP18 when locked | 145 | 179 (alignment onto diode) | |
| MICH trigg +FM trig on | 40 (27% of locked) | 40 (22% of locked level) | 48 (27%) |
| SRCL trigger on level | 40 (27%) | 30 (17%) | 48 (27%) |
| SRCL trig + FM trig off | 15 (10%) | 5 (3%) | 18 (10%) |
| MICH trigger threshold off | 15 (10%) | 5 (3%) | 18 (10%) |
| REFL9I to PRCL matrix | 3.5 | 2.2 | 3.5 |
| PRCL gain | 12 | 8 | 12 (ACQUIRE) |
| REFL9I to SRCL | -5.508 | -1.8(44318) | not changed |
| MICH FM trig wait | 0.1 | 0.2 | 0.1 added to guardian |
| PRCL FM trig wait | 0.2 | 0.3 | 0.2 added to guardian |
| REFLair RF45 phase R | 82 | 97 | not changed |
| Refl air RF9 phase R | -21 | -23 | not changed |
| SRCL FM1 | was triggered, +6dB, 0.2 second ramp | no longer triggered, +106 dB to cancel -100dB in FM2 | reluctant to change |
I was reluctant to make changes to SRCL FM1 because that is the filter that has twice given huge and inexplicable outputs when we modified it.
Things I haven't done which could be done (after collecting some stats about this state, if we want to try to get closer to Sept):
The values of POP18 refered to above at H1:LSC-POPAIR_B_RF18_I_ERR_DQ. The channel used in the trigger matrix is actaully normalized.
On the Oct 4th, 2018 time above, the normalized channel was 82. This means that in the above table, for the good locking time the MICH + SRCL trigger was at 49% of the locked build ups.
Tony, Ibrahim, Sheila
Referencing 44348, Ibrahim and I went back to Sept 12 2018, and found a time when PRMI locked in 3 minutes. At that time, the MICH trigger level was 6, and based on the minute trend max the MICH TRIF channel was around 70, 9% of the max value. In locked DRMI, the trigger channel was 70, and the trigger level was 40, so 57% of the locked value, and the trigger matrix had a value of 1.
On March 31st, 2025 I changed the trigger matrix from 1 to 2 for PRMI and DRMI 83655, at that time the locked value on POPAIR 18 NORM was only 32 perhaps because the diode was misalinged, the trigger threshold was 37, so with the factor of 2 the trigger was still 43% of the locked value for DRMI. After the vent where ISCT1 was moved and realinged, POP 18 NORM has been back at around 70 counts when DRMI was locked.
We removed the factor of 2 from the input matrix, and loaded the DRMI guardian. After this we have had one short PRMI lock, where we can see that something is moving a lot and PRMI is not well aligned.