TITLE: 10/10 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 158Mpc
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY: Currently Observing at 158Mpc and locked for 5 hours. A lot of time out of Observing today due to continued PSL troubleshooting and commissioning. Relocking after our one lockloss wasn't too bad.
LOG:
14:30 Observing and Locked for 4 hours
15:02 Out of Observing for Commissioning
15:29 Lockloss
16:24 Going through CHECK_MICH_FRINGES a second time, so decided to run an initial alignment only for PRC, MICH, and SRC
15:29 manual initial alignment done, relocking
16:39 Lockloss from LOCKING_ALS
16:49 IDLE for PSL power swap
17:45 Started relocking
17:51 Lockloss from ACQUIRE_DRMI_1F
18:42 NOMINAL_LOW_NOISE
20:25 Observing
21:45 Out of Observing to run calibration sweep
22:51 Observing
23:25 - 23:37 Trash truck onsite - tagging PEM, DetChar
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:17 | FAC | Tyler | n | Running well pump (started 14:55) | 19:11 | |
16:56 | PSL | RyanS, Fil, Fernando | LVEA | n | Swap power box | 17:18 |
16:56 | FAC | Tyler | YARM | n | Driving along YARM backside | 18:17 |
17:21 | PSL | RyanS, Fil | LVEA | n | Re-swap power | 17:47 |
19:14 | FAC | Tyler | n | Running well pump | 20:14 | |
19:16 | Sheila | LVEA | n | Plugging cable in | 19:25 | |
20:20 | Sheila | LVEA | n | Unplugging cable | 20:25 | |
21:24 | VAC | Fil, 1 VAC guy | YARM | n | Fixing solar panel | 22:47 |
The sum of the counts on the QPD IMC-IM4_TRANS_NSUM_OUT has been around 53W since July 2nd, 2024(attachment1). Before this, the nsum value was around 58W. On July 2nd, the PMC was swapped (78813), and so the pointing into the ifo changed. After the PMC change the IMC alignment was updated to realign the beam(78816), but the IM4 trans beam is still not hitting in the same place as it was before. As a result, the beam is very off in yaw when it hits the QPD, so yaw is currently at +0.98 so it's on the edge. You can also tell the beam is partially off the QPD because of how much change we see in the IM4 trans values as compared to before July 2nd.
WP 12136
One of the solar panels on Y2-8 was replaced. Panels provide power to a vacuum gauge inside the beamtube enclosure.
F. Clara, G. Moreno
TITLE: 10/10 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 155Mpc
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 9mph Gusts, 5mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.23 μm/s
QUICK SUMMARY:
IFO is in NLN and OBSERVING
Oli gave me the updates regarding fixes to the dolphin crash from yesterday.
Calibration measurement run after being locked for 3 hours
calibration monitor screenshot (accidently taken after going into NLN_CAL_MEAS)
Broadband 10/10 21:50 - 21:56UTC
File:
PCALY2DARM_BB/PCALY2DARM_BB_20241010T215057Z.xml
Simulines* 10/10 21:57 - 22:21UTC
*Simulines was run using the ini file settings_h1_20241005_lowerPcal.ini instead of the usual
settings_h1_newDARM_scaled_by_drivealign_20231221_factor_p1.ini, both of which are found in /ligo/groups/cal/H1/simulines_settings/newDARM_20231221/
Files:
DARMOLG_SS/DARMOLG_SS_20241010T215755Z.hdf5
PCALY2DARM_SS/PCALY2DARM_SS_20241010T215755Z.hdf5
SUSETMX_L1_SS/SUSETMX_L1_SS_20241010T215755Z.hdf5
SUSETMX_L2_SS/SUSETMX_L2_SS_20241010T215755Z.hdf5
SUSETMX_L3_SS/SUSETMX_L3_SS_20241010T215755Z.hdf5
R. Short, F. Clara, S. Dwyer
In the ongoing effort to diagnose the source of the glitches seen in the PSL, we decided to try moving the NeoLase control box in the PSL racks back to rack power, essentially undoing what was done in alog79593, and observe any changes in the glitch behavior. While H1 was unlocked during the commissioning window this morning, I shut down the PSL in a controlled manner (in order of ISS, FSS, PMC, AMP2, AMP1, NPRO), then Fil switched CB1 back to rack power, and I brought the system back up. When back in the control room, we very quickly noticed glitching in the NPRO output power channel as we've seen before, and after locking the RefCav, the FSS glitches also returned. Deciding this wasn't the solution we were looking for (and concluding it probably wouldn't have changed anything in the first place), I took the PSL down again for Fil to switch back to the bench-top power supply, then brough it back up all without issue. Fil also took the opportunity to install a longer cable for this power supply to reduce the trip hazard potential next to the PSL racks. This closes WP 12133.
I'm tagging DetChar since this separate power supply was noted to have helped reduce a 9.5Hz comb seen in DARM, but I'll reiterate that functionally nothing here has changed and CB1 remains on its own power supply.
I ran the noise budget injections for frequency noise, input jitter (both pitch and yaw) and PRCL. All injections were run with CARM on one sensor (REFL B). The cable for the frequency injection is still plugged in as of this alog, but I reset the gains and switches so we are back on two CARM sensors and the injection switch is set to OFF.
All injections are saved in the usual /ligo/gitcommon/NoiseBudget/aligoNB/aligoNB/H1/couplings folder under Frequency_excitation.xml, IMC_PZT_[P/Y]_inj.xml, and PRCL_excitation.xml.
I realized an intensity noise injection might be interesting, but when I went to run the template for the ISS excitation, I was unable to see an excitation. I think there's a cable that must be plugged in to do this? I am not sure.
*********Edit************
Ryan S. sent me a message with this alog that has notes about how intensity noise injections should be taken. Through this conversation, I realized that I had misread the instructions in the template. I toggled an excitation switch on the ISS second loop screen, when I should have instead set the excitation gain to 1.
I was allowed another chance to run the intensity injections, and I was able to do so, using the low, middle, and high frequency injection templates in the couplings folder.
Also, the Input jitter injections have in the past been limited to 900 Hz, because the IMC WFS channels are DQed at 2048 Hz. However, the live IMC channels are at 16 kHz, so I edited the IMC injection templates to run up to 7 kHz, and use the live channels instead of the DQ channels. That allowed the measurements to run above 900 Hz. However, the current injections are band-limited to only 1 or 2 kHz. I think we can widen the injection band to measure jitter up to 7 kHz. I was unable to make those changes because we had to go back to observing, so this is future to-do item. I also updated the noise budget code to read in the live traces instead of the DQ traces.
Unfortunately, in my rush to run these injections, I forgot to transition over to one CARM sensor, so both the intensity and jitter measurements that are saved are with CARM on REFL A and B.
I ran an updated noise budget using these new measurements, plus whatever previous measurements were taken by Camilla in this alog. Reminder: the whole noise budget is now being run using median averaging.
I used a sqz time from last night where the range was around 165 Mpc, starting at GPS 1412603869. Camilla and Sheila took a no-sqz data set today starting at 1412607778. Both data sets are 600 seconds long. I created a new entry in gps_reference_times.yml called "LHO_O4b_Oct" with these times.
To run the budget:
>conda activate aligoNB
>python /ligo/gitcommon/NoiseBudget/aligoNB/production_code/H1/lho_darm_noisebudget.py
all plots found in /ligo/gitcommon/NoiseBudget/aligoNB/out/H1/lho_darm_noisebudget/
I made one significant edit to the code, which is that I decided to separate the laser and input jitter traces on the main DARM noise budget. That means that the laser trace is now only a sum of frequency noise and intensity noise. Input beam jitter is now a trace that combines the pitch and yaw measurements from the IMC WFS. Now, due to my changes in the jitter injections detailed above, these jitter injections extend above 900 Hz. To reiterate: the injections are still only band-limited around 2 kHz, which means that there could be unmeasured jitter noise above 2 kHz that was not captured by this measurement.
One reason I wanted to separate these traces is partly because it appears there has been a significant change in the frequency noise. Compared to the last frequency noise measurement, the frequency noise above 1 kHz has dropped by a factor of 10. The last time a frequency noise injection was taken was on July 11, right before the OFI vent, alog 79037. After the OFI vent, Camilla noticed that the noise floor around 10 kHz appeared to have reduced, as well as the HOM peak heights, alog 76794. She posted a follow-up comment on that log today noting that the IFO to OMC mode matching could have an effect on those peaks. This could possibly be related to the decrease in frequency noise. Meanwhile, the frequency noise below 100 Hz seems to be about the same as the July measurement. One significant feature in the high frequency portion of the spectrum is a large peak just above 5 kHz. I have a vague memory that this is approximately where a first order mode peak should be, but I am not sure.
There is no significant change in the intensity noise from July, except that there is also a large peak in the intensity noise just above 5 kHz. Gabriele and I talked about this briefly; we think this might be gain peaking in the ISS, but its hard to tell from alog measurements if that's possible. We think that peak is unlikely to be from the CARM loop. We mentioned the ISS theory to Ryan S. on the off-chance it is related to the current PSL struggles.
The other significant change in the noise budget is the change in the LSC noise. The LSC noise has reduced relative to the last noise budget measurement, alog 80215, which was expected from the PRCL feedforward implementation. Looking directly at the LSC subbudget, PRCL has been reduced by a factor of 10, just as predicted from the FF performance. Now, the overall LSC noise contribution is dominated by noise from MICH. Between 10-20 Hz, we might be able to win a little more with a better MICH feedforward, however that is a very difficult region to fit because of various high Q features (reminder alog).
Just as in the previous noise budget, there is a large amount of unaccounted-for noise. The noise budget code uses a quantum model that Sheila and Vicky have been working on extensively, but I am not sure of the status, and how much of that noise could be affected by adjustments to the model. Many of the noisy low frequency peaks also appear very broad on the timescale of the noise budget plot. We could try running over a longer period of time to better resolve those peaks.
Between 100-500 Hz there are regions where the sum of known noises is actually larger than the measured noise. I think this is because the input jitter projections are made using CAL DELTA L, but the overall noise budget is run on CALIB CLEAN where we are running a jitter subtraction.
I believe these couplings were pushed to aligoNB repo in commit bcdd729e.
I reran the jitter noise injections, trying to increase the excitation about 2 kHz to better see the high frequency jitter noise. The results were moderately successful; we could probably push even harder. The results indicate that jitter noise is with a factor of 2-3 of DARM above 1 kHz.
I have attached the updated DARM noise budget and input jitter budget. I'm also attaching the ASC budget (no change expected) just because I forgot to attach it in the previous post.
Currently in Locked and in Commissioning. We are taking an extra hour for commissioning past the normal schedule, so we should be getting back to Observing around 20:10UTC.
20:25 Observing
Oli, Ryan S, Sheila, Camilla
This morning we didn't go through SDF_REVERT as I had a pending sdf change so we went to CHECK_SDF whihc skips SDF_REVERT. We then had the ETMX suspensions model saturating, tracked this down via cds overview of h1susetmx and ETMX L3 DAC screens to be the L3 bias saturating.
We found that the nominal ETMX_L3_LOCK_BIAS_OFFSET value (saved in sdf) is -8.9 but ISC_LOCK PREP_FOR_LOCKING sets this to -9.3 (saturates DAC). Can see them arguing in the attached plot.
A to-do would be to remove this control from ISC_LOCK but Sheila said this isn't simple as other gains need to be adjusted too. Can look at doing this is the future.
Thu Oct 10 10:10:59 2024 INFO: Fill completed in 10min 55secs
Non-optimal fill, TC-A went to -200C (unusual in autumn), TC-B only went to -115C. Early trip because TC-A started at -75C, but pressure spike indicates a good fill.
Jordan discovered the TCs were completely iced over.
Sheila, Camilla
15:02:40-15:13:00UTC - Took No Squeezing time. IFO had been in NLN for 4h30m.
Checked NLG (0.1178/0.00872) = 13.5. Adjusted OPO temperature.
After our no SQZ time, once in FDS, we let the IFO ASC converge and then turned it off, cleared histories in SQZ-ASC filter banks and ran scan sqz alignment. We never checked these were the same in 80506. Lost lock before scan sqz alignment could finish running.
Ibrahim This alog is a summary of all the BBSS drift data we have, and what observations informed which next steps. The embedded table below shows each "regime", which is a span of data collection after a mechanical adjustment. I have then linked pictures of each regime's available OSEM readouts. In the case of BOSEMs, we've only had clean readings with working electronics for regimes 8, 9, 10. We briefly had a broken sat-amp box for regime 5 so we do have some readings. Either way, I don't believe these show significant drift. At the end, I also have attached an overview of the two main adjustment types over the course of the time we've been dealing with this issue. First is blade tip adjustment and second is added weight (grams) distribution adjustment (which also has a graphic for each config). I will add Transfer Functions later (IFO is misbehaving on EVE shift and want to get something out!). They are located on X1 under: /ligo/svncommon/SusSVN/sus/trunk/BBSS/X1/BS/SAGM1/Results and are dated. With limited further ado: Overview: Blade Tip Height Changes:Blade Tip Height Changes: Regime 1:
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Regime 2:
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Regime 3:
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Regime 4:
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Regime 5:
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Regime 5 PUM BOSEMs (Broken Sat Amp):
Regime 6:
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Regime 7:
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Added Weight Distribution Changes: Regime 8:
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Regime 9:
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Regime 10:
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Regime 8, 9, 10 (Weight Changes) PUM BOSEMs:
Added Weight Distribution Config Graphic: In reply Added Weight Changes Zoomed Out:
Blade Tip Height Changes and Initial Drift Zoomed Out:
Lockloss @ 10/10 15:29UTC during Commisioning
Seems that the IMC lost lock here (correctly tagged "IMC" by the lockloss tool, see short-term trend), but I'm not convinced in this case it was due to the FSS. The last FSS glitch happened ~4 seconds before the IMC lost lock and there weren't many happening frequently before that (see longer-term trend).
H1 requested assistance around 11pm PT due to the SQZ filter cavity not being able to lock. Based on previous alogs, it sounds like there was some SQZ issues earlier today, but there's no mention as to what exactly. Looking at the FC green camera it was clearly trying to lock with a pitch misalingment, so I adjusted FC2 and maximized H1:SQZ-FC_TRANS_C_LF_OUTPUT. This seemed to help, but then after it would find IR it would lose lock. I'm not sure why, but we just lost lock (0720UTC) so I guess I'll see if it happens again when we get back.
Relocking was automatic but again the SQZ FC couldn't tranistion to IR. Vicky came to rescue and was able to get it working. Something I should have seen earlier is that there was a dolphin crash, so the ZMs were way off from their nominal position. Notes from Vicky:
Accepted SDFs for SQZ ZMs/FC2 and LSC-LOCKIN_OSC_FREQ
Sheila, Camilla
Trending back what happened last night:
To avoid this in future:
Tagging OpsInfo: if you run SCAN_SQZ_ALIGN and don't like it, you'll need to trend back ZM4/6 optical align sliders as they aren't in sdf. Also you need to turn off SQZ ASC before running scan_sqz_alignment, updated instructions in wiki. <- added this the the guardian.
While looking at this we also decided to remove SQZ_FC state LOCKED (nominal is IR_LOCKED we don't see a need for a state that can be GREEN_LOCKED or IR_LOCKED).
Sheila, Camilla.
New SQZ ASC using AS42 signals with feedback to ZM4 and ZM6 tested and implemented. We still need to watch that this can keep a good SQZ alignment during thermalization. In O4a we used a SQZ ASC with ZM5/6, we have not had a SQZ ASC for the majority of O4b.
Prep to improve SQZ:
Testing ASC from 80373:
In the first 20 minutes of the lock, the SQZ ASC appears to be working well, plot.
Note to operator team: if the squeezing gets really bad, you should be able to use the SQZ Overview > IFO ASC (black linked button) > "!graceful clear history" script to turn off the SQZ ASC. Then change /opt/rtcds/userapps/release/sqz/h1/guardian/sqzparams.py use_ifo_as42_asc to False and go though NO_SQZEEZING then FREQ_DEP_SQUEEZING in SQZ_MANAGER and accept the sdfs for not using SQZ ASC. If SQZ still looks bad, put ZM4/6 osems (H1:SUS-ZM4/6_M1_DAMP_P/Y_INMON) back to when squeezing was last good and if needed run scan sqz alignment and scan sqz angle with SQZ_MANAGER.
Sheila moved the "0.01:0" integrators from the ASC_POS/ANG_P/Y filters into the ZM4/5/6_M1_LOCK_P/Y filter banks.
This will allow us to more easily adjust the ASC gains and to use the guardian ZM offload states. We turned them on on ZM4/6. Edited OFFLOAD_SQZ_ASC to offload for ZM4,5,6. And tested by putting an offset on ZM4. We put ZM4/6 back to positions they were in in lock via the osesms. SDFs for filters accepted. I removed the "!offload AS42" button from the SQZ > IFO ASC screen (liked to sqz/h1/scripts/ASC/offload_IFO_AS42_ASC.py) as it caused a lockloss yesterday.
Oli tested the SQZ_MANAGER OFFLOAD_SQZ_ASC guardian state today and it worked well. We still need to make the state request-able.
ASC now turns off before SCAN_SQZANG_FDS/FIS and SCAN_ALIGNMENT_FDS/FIS. It wil check if the ASC is on via H1:SQZ-ASC_WFS_SWITCH and turn the asc off before scanning alignment or angle.
We changed the paths so that to get from SCAN_SQZANG_FDS/FIS and SCAN_ALIGNMENT_FDS/FIS back to squeezing, the guardian will go though SQZ_ASC_FDS/FIS to turn back on ASC afterwards.
Plot attached showing that the Higher Order Modes around 10.4 to 10.6kHz are in a similar position during ER16 (blue) that they were at the end of O4a (yellow).
This is expected as we have not changed the TCS system (CO2 and RH settings the same). Unsure why in the last long (2024/03/28) they are larger, the noise floor changes with SQZ but wouldn't expect the peaks to change much.
Vicky, Camilla. Attached plot has comparisons of No SQZ times, the noise floor at 10kHz seems to have decreased since O4a. Using times in Jennie's 76516 show similar noise floors.
Late alog: After the Emergency vent and OFI crystal swap in July/August, in late August we saw that the two HOM peaks had moved into a single peak. Plot: Blue = pre vent in July, Brown and green = Post vent in August.
Dan Brown made the quick model attached showing that the IFO to OMC mismatch does have an impact on the height of those peaks. From Dan: The plot looks at mode mismatch change and how laser frequency to DCPD coupling scales with it. If changing the OFI has modified the mode-matching or more likely just reduced HOM scattering then seeing smaller peaks could be due to that.