Yesterday we went back to the higher range CARM configuration, in which the fast/IMC locklosses first appeared 80938. Overnight we had two observing locklosses tagged with the IMC, neither of which had glitches visible in the FSS fast mon channel, 1414411965 (1st attached screenshot), and 1414381791.
This morning I changed the gains by 6 dB in the other direction, so we further limit the range available to the frequency actuator. (CARM sliders and ndscope) Our microseism is around 5um/second right now, slightly above the 90th percentile, but there was no wind and no earthquakes this morning. At times the IMC splitmon was reaching -8V, it's range is +/- 10V so this is about as far as we can go in this direction, and might be kind of marginal.
We've since had one lockloss 1414426971, this is tagged as commissioning because we were in commissioning time at the moment, but no one was actively doing anything at the time so this wasn't caused by commissioners. There was a glitch in the FSS fast mon for this lockloss, although it was below the threshold for the tag to be applied, and around the time of that glitch the drive to the ISS AOM becomes noisy. We were not saturating the IMC splitmon at the time of the lockloss so that doesn't seem to be the cause.
I've removed this, so now we will be back to the gains we've been with for the last several weeks, and most of O4.
Lockloss @ 10/31 16:01 UTC after almost an hour locked
18:13 Just got to NLN, staying out of Observing for Commissioning
All models on h1seih45 glitched at 07:09:46 PDT (14:09:46 UTC). This appears to have broken the lock and caused guardian to start an initial alignment.
Symptoms are:
The models appeared to have resumed normal operation following the glitch, no restarts were needed. At the time of writing H1 is locked with a range of 160MPc.
At the time of the glitch we had been relocking and at TRANSITION_FROM_ETMX. There seem to have been no issues at all from this - the initial alignment was automatically started after trying to relock took us into CHECK_MICH_FRINGES for the third time during the relock period, and went smoothly and without issue.
HAM4 and HAM5 GS13 signals following the glitch:
There are 8 Dolphin IPC channels which are sent by h1seih45 models (h1isiham4 and h1isiham5). They are all received by h1seiproc on h1oaf0. h1seiproc runs at 4kHz.
All 8 receive channels saw 4096 errors at the time of the glitch.
rcv model type snd host snd model ipc channel
h1seiproc PCIE h1seih45 h1isiham4 H1:ISI-HAM4_CPS_X_IPC_OUT
h1seiproc PCIE h1seih45 h1isiham4 H1:ISI-HAM4_CPS_Y_IPC_OUT
h1seiproc PCIE h1seih45 h1isiham4 H1:ISI-HAM4_SUSPOINT_SR2_L_OUT_IPC
h1seiproc PCIE h1seih45 h1isiham5 H1:ISI-HAM5_CPS_X_IPC_OUT
h1seiproc PCIE h1seih45 h1isiham5 H1:ISI-HAM5_CPS_Y_IPC_OUT
h1seiproc PCIE h1seih45 h1isiham5 H1:ISI-HAM5_SUSPOINT_OFI_L_OUT_IPC
h1seiproc PCIE h1seih45 h1isiham5 H1:ISI-HAM5_SUSPOINT_SR3_L_OUT_IPC
h1seiproc PCIE h1seih45 h1isiham5 H1:ISI-HAM5_SUSPOINT_SRM_L_OUT_IPC
TITLE: 10/31 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 5mph Gusts, 3mph 3min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.47 μm/s
QUICK SUMMARY:
Looks like we just finished an initial alignment and are starting to relock
H1 called for assistance at 13:13 UTC when SRM watchdogs tripped during the SRC alignment steps of initial alignment. After resetting the WDs, I just let Guardian try SRC align again, but SRM tripped during ACQUIRE_SRY. I reset the WDs again and took ALIGN_IFO to DOWN to manually align SRM a bit (didn't get too much improvement on the AS_A fringing, but some), and had Guardian try again. This time, there were no issues, and initial alignment finished without issue.
H1 is currently relocking and just got through DRMI.
TITLE: 10/31 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: Currently relocking, but we've had a few lock losses after DRMI and one at engage_asc_for_full_ifo. We've just made it past that point again.
Lockloss 0349
Averaging Mass Centering channels for 10 [sec] ...
2024-10-30 14:34:04.266740
There are 14 T240 proof masses out of range ( > 0.3 [V] )!
ETMX T240 2 DOF X/U = -0.755 [V]
ETMX T240 2 DOF Y/V = -0.707 [V]
ETMX T240 2 DOF Z/W = -0.473 [V]
ITMX T240 1 DOF X/U = -1.549 [V]
ITMX T240 1 DOF Y/V = 0.328 [V]
ITMX T240 1 DOF Z/W = 0.452 [V]
ITMX T240 3 DOF X/U = -1.611 [V]
ITMY T240 3 DOF X/U = -0.797 [V]
ITMY T240 3 DOF Z/W = -1.997 [V]
BS T240 1 DOF Y/V = -0.404 [V]
BS T240 3 DOF Y/V = -0.317 [V]
BS T240 3 DOF Z/W = -0.502 [V]
HAM8 1 DOF Y/V = -0.436 [V]
HAM8 1 DOF Z/W = -0.758 [V]
All other proof masses are within range ( < 0.3 [V] ):
ETMX T240 1 DOF X/U = -0.04 [V]
ETMX T240 1 DOF Y/V = -0.066 [V]
ETMX T240 1 DOF Z/W = -0.098 [V]
ETMX T240 3 DOF X/U = -0.055 [V]
ETMX T240 3 DOF Y/V = -0.111 [V]
ETMX T240 3 DOF Z/W = -0.058 [V]
ETMY T240 1 DOF X/U = 0.015 [V]
ETMY T240 1 DOF Y/V = 0.136 [V]
ETMY T240 1 DOF Z/W = 0.192 [V]
ETMY T240 2 DOF X/U = -0.069 [V]
ETMY T240 2 DOF Y/V = 0.187 [V]
ETMY T240 2 DOF Z/W = 0.029 [V]
ETMY T240 3 DOF X/U = 0.206 [V]
ETMY T240 3 DOF Y/V = 0.04 [V]
ETMY T240 3 DOF Z/W = 0.128 [V]
ITMX T240 2 DOF X/U = 0.129 [V]
ITMX T240 2 DOF Y/V = 0.265 [V]
ITMX T240 2 DOF Z/W = 0.229 [V]
ITMX T240 3 DOF Y/V = 0.124 [V]
ITMX T240 3 DOF Z/W = 0.102 [V]
ITMY T240 1 DOF X/U = 0.083 [V]
ITMY T240 1 DOF Y/V = 0.084 [V]
ITMY T240 1 DOF Z/W = -0.063 [V]
ITMY T240 2 DOF X/U = 0.05 [V]
ITMY T240 2 DOF Y/V = 0.182 [V]
ITMY T240 2 DOF Z/W = 0.1 [V]
ITMY T240 3 DOF Y/V = 0.072 [V]
BS T240 1 DOF X/U = -0.174 [V]
BS T240 1 DOF Z/W = 0.082 [V]
BS T240 2 DOF X/U = -0.099 [V]
BS T240 2 DOF Y/V = 0.002 [V]
BS T240 2 DOF Z/W = -0.126 [V]
BS T240 3 DOF X/U = -0.213 [V]
HAM8 1 DOF X/U = -0.286 [V]
IMC tag on this one, ending a 1 hr 48min lock.
Following instructions from alog76751 and from Sheila herself, I ran the CARM olg python script located in /ligo/gitcommon/psl_measurements/. Sheila had already hooked up the SR785 at the PSL racks earlier in the day while we were relocking, so it was easy enough for me to check that we could connect to it through GPIB (checked with ipython like Craig did in alog64204), then run the commands listed in alog76751. After I ran it, I then went out into the LVEA and unplugged and turned off the SR785, as well as the LVEA lights.
Since this plot is saved as a pdf, its hard to say exactly what the UGF is, but it looks around 17kHz just as it has been, consistent with 76751 & 76448 but a little higher than 70920 and 65676 and 67584.
TITLE: 10/31 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Earthquake
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 14mph Gusts, 9mph 3min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.49 μm/s
QUICK SUMMARY: After the earthquake we started an initial alignment, in which Oli only had to adjust IM4. Now while locking PRMI, the POP90 signal isn't as high has before the earthquake when locked. Trending the PRs, PR2 is a little bit off in Y from before, so I've tried to keep PRC1 on and move PR2 slowly toward its old position while PRM followed. I'm not too sure this is helping at all though. Once this is done I'll try more DRMI.
TITLE: 10/30 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Earthquake
INCOMING OPERATOR: TJ
SHIFT SUMMARY: Trying to relock after the huge earthquake off the coast of Oregon knocked us down. Currently at PRMI_ASC and TJ is trying to touch up PRMI.
LOG:
14:30 In tail end of an initial alignment
14:33 Initial alignment done, relocking
15:26 NOMINAL_LOW_NOISE
15:26 Observing
15:49 Out of Observing to adjust CARM gain
- Trying to recreate FSS glitches
15:50 Back into Observing
16:09 Lockloss
16:10 Initial alignment
- SRC wouldn't lock and SRM tripped twice
16:37 Took us to DOWN and just started relocking
- Lockloss from LOCKING_ARMS_GREEN
- Lockloss from ACQUIRE_DRMI_1F
- IMC took 15 minutes to relock. Relocked after I took it to OFFLINE for a few minutes
17:55 NOMINAL_LOW_NOISE
17:58 Observing
18:00 Out of Observing for PSL makeup air check
18:32 Back to Observing
20:17 Lockloss due to earthquake
Tripped:
- ISI HAM{2,3,4,5,7,8}, BS, {E,I}TM{X,Y}
- SUS PR2, PR3, SR2, SRM, IM4, OFI, TMSY
21:45 Starting initial alignment
- Could not get XARM IR due to the IMs having drifted during the earthquake. I trended them back with driftmon and adjusted sliders until they were back to where they were before the earthquake.
22:36 Initial alignment finished, relocking
- Lockloss from PRMI_ASC x2
- Lockloss from LOCKING_ARMS_GREEN
- Lockloss from FIND_IR
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:57 | FAC | Karen | OptLab, VacPrep | n | Tech clean | 15:25 |
16:52 | VAC | Janos | Mid/Ends | n | Checking receiving areas | 17:18 |
17:06 | FAC | Tyler, contractor | Mids | n | In chiller yards, mech rooms | 19:39 |
18:01 | PEM | Robert | LVEA | n | Checking PSL makeup air | 18:32 |
18:01 | PSL | Jenne | LVEA | n | Spectrum of FSS output | 18:32 |
18:29 | FAC | Kim | H2 | n | Tech clean | 18:43 |
Reran all O4b locklosses on the locklost tool with the most up to date code, which includes the "IMC" tag.
I used the lockloss tool data since the emergency OFI vent (back online ~23rd August) until today and did some excel wizardry (attached) to make the two attached plots, showing the number of locklosses per day tagged with IMC and without tag IMC. I made this plots for just locklosses from Observing and all NLN locklosses (can include commissioning/maintenance times), including:
Attaching plots from zooming in on a few locklosses:
Time | Tags | Zoom Plot | Wide Plot |
2024-10-31 12:12:26.993164 UTC (IMC) | OBSERVE IMC REFINED | annotated plot | plot |
2024-10-30 12:16:33.504883 UTC (IMC) | OBSERVE IMC REFINED | annotated plot | plot |
2024-10-30 16:09:21.548828 UTC (Normal) | OBSERVE REFINED OMC_DCPD | N/A | annotated plot |
The 10-31 zoom plot notes the framerates of the channels: ASC, REFL and NPRO_PWR are 2kHz and GS13 is 4kHz, the others are 16kHz.
Since September 18th we've had 21 locklosses from NLN tagged as FSS_OSCILLATION, of these 20 also had the IMC tag. Since September 12th, we've had 49 locklosses from NLN tagged IMC, so roughly 40% of these IMC locklosses have the FSS oscillation tag, since the NPRO was swapped we don't have any tagged with FSS_OSCILLATION.
(Reminder, the FSS_OSCILLATION tag is an old tag, intended for a different problem, but it tags times where the FSS fast mon goes above a treshold.)
Updated plot attached of NLN locklosses tagged with and without the IMC tag.
Our frequency noise and contrast defect (measured at the OMC) are lower than they ever have been in O4 (contrast defect, frequency noise). As a part of trying to track down what may have caused this reduction, I tracked the coherence of DARM with the LSC REFL A RIN, using that as a witness to frequency noise, as it was used in OAF for online frequency noise cleaning in O4a (source: 72276 and poking around the OAF screens).
I tried to pick times that were a few hours into the lock to avoid thermalization confusion. I also used only observing data.
There are a couple ideas about what could have caused this improvement. A short list:
These are the times I used. All of these times were at the same 60 W input power from the PSL:
Dec 10 2023: O4a time, no WFS offset in use, EY ring heater set to 1 W (1386244818)
Apr 11 2024: O4b time, before the OFI problems, WFS offset in use, EY ring heater set to 1 W (1396950886)
Jul 10 2024: O4b time, just before OFI repair vent, WFS offset in use, EY ring heater set to 1 W (1404656647)
Sept 14 2024: O4b, after OFI repair, WFS offset in use, EY ring heater set to 1 W (1410432000)
Sept 20 2024: O4b, after OFI repair, WFS offset set OFF, EY ring heater set to 1 W (1410855190)
Oct 22 2024: O4b, after OFI repair, WFS offset set OFF, EY ring heater set to 1.1 W (1413635762)
Here are some notes for the comparison of these times:
All of these O4 times show less coherence than the O4a time. Based on this data, it seems like the WFS offset did have an impact on the frequency noise. It also seems like the various vents with output port changes could affect the frequency noise, but the overall beam alignment in the arms could have changed during the vent. For example, we did adjust the camera offsets/ADS gains during the vent commissioning times. The change in frequency noise during the OFI problems (between April and July) could have a similar source, since we had to change a lot of alignment during that time. I'm not sure if any arm alignment was significantly changed though. Finally, it seems like this small ring heater change had no effect on the frequency noise.
Just a quick look at how the input jitter coherence has changed with these changes as well. For estimating input jitter, we generally use the IMC WFS A DC pitch and yaw channels, both for the noise budget and for jitter cleaning.
I used the exact same times as the freqeuency noise traces for ease, and I matched the colors too for easy comparison. Note: I used coherence with a channel that has no jitter subtraction to also avoid confusion.
This first plot compares the jitter coherence with DARM from all the times across the whole band in pitch and yaw. It's a bit hard to read. To make this easier, I'll break down the trace comparisons:
The most interesting point here (in my opinion) is that the improvement in frequency noise from the brown trace to the pink trace, that is, when we turned off the WFS offset, is opposite to the effect on the jitter noise. We've seen this before: improvements to frequency noise worsen jitter coupling and vice versa. I still don't understand that mechanism.
These are saved in the same template as the frequency noise plot: /ligo/home/elenna.capote/freq_noise_coherence_compare.xml
Daniel rightfully pointed out to me that REFL A RIN is a better measure of intensity noise than frequency noise. In the process of thinking about this, I realized that we found that PRCL had some offset present that increased DARM coherence to LSC REFL RIN. We first fixed this by applying a digital offset, and then Sheila rephased POP9 which had the same effect of reducing the coupling to REFL RIN and increasing power in the PRC. The digital offset was applied to PRCL from March 30 to May 6, and then again applied from Sept 16 until Sheila rephased POP 9 on Sept 23.
Since the PRCL offset/POP9 rephasing effects the coherence of DARM and REFL RIN, and to better ensure I am capturing frequency noise, I reran these measurements using coherence with the REFL SERVO CTRL channel.
Figure 1 We see similar improvement and worsening between O4a, Apr 12 O4b and Jun 10 O4b. Then, the three traces after the OFI vent show the same coherence, Figure 2. This indicates that the improvement between the brown (Sept 14) and pink (Sept 20) trace in the REFL RIN plot (original alog) is likely due to the changes in PRCL and not due to changes in frequency noise. In fact, the frequency noise coherence since the vent for these three times looks about the same.
This leads to the conclusion that the something about the OFI vent itself changed the frequency noise. We might be able to attribute it to an alignment change, but my sense is that whatever alignment change that occurred is small compared to the significant change in the output mode matching. I still don't full see how this then couples back to frequency noise, but it's worth some thinking and modeling.