Displaying reports 501-520 of 79139.Go to page Start 22 23 24 25 26 27 28 29 30 End
Reports until 22:01, Thursday 31 October 2024
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 22:01, Thursday 31 October 2024 (80986)
OPS Eve Shift Summary

TITLE: 11/01 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 152Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:

IFO is in NLN and OBSERVING since 02:36 UTC

Mostly a quiet and uneventful shift, with the exception of the squeezer failing to lock for abbout 50 mins (until we lost lock - Lockloss Alog 80985). Vicky reverted some changes to SQZ that were made today (comment alog 80984) I accepted those SDF changes (attached).

Microseism is still high and rising, but doesn't seem to be too much of an issue.


LOG:

None

 

Images attached to this report
H1 ISC (Lockloss)
ibrahim.abouelfettouh@LIGO.ORG - posted 20:06, Thursday 31 October 2024 (80985)
Lockloss 01:06 UTC

Lockloss while troubleshooting SQZer not locking (before going into OBSERVING). No IMC tags on the Lockloss Tool.

H1 PSL
jenne.driggers@LIGO.ORG - posted 17:21, Thursday 31 October 2024 (80983)
Attempt at swapping in spare PSL TTFSS boxes, reverted to original

[Jenne and Betsy in PSL enclosure; Jason logged in remotely; Marc, Fil, Rick, Fernando as EE support; consults with Daniel]

At today's commissioning meeting, we decided that one candidate thing to try to help mitigate the lockloss-causing glitches would be to swap in one of the spare TTFSS boxes.  We also noted that if it was going to happen, it had to happen today, or wait until Mon/Tues next week.  So, we tried swapping in a new FSS box.  We were unable to lock the RefCav with either spare without significant oscillations, so ended up putting back in the original box, and that's how we'll leave things at least for the weekend.

Each time we changed out a box, we followed the steps 1-5 of our work permit 12182 (listed also below).  In particular, before unplugging the 37 pin connector on the back, we had one of the support folks turn off the high voltage in the mezzanine of the CER (I think it is a pair of Kepcos, one +150V, one -150V).  Then, once we had the 37 pin connector secured in the new box, one of the support folks went back to the mezzanine and turned back on the high voltage. 

For both spares, the autolocker was able to find a ref cav resonance and hold it there.  However, even with both the FAST and COMMON gain sliders set to the minimum values of -10dB we saw significant oscillation of the loop.  An idea I had later (have not yet checked with anyone else to see if it's crazy or not) is to try one of the spare boxes, but with an attenuator on one of the cables, to see if it really is just a loop gain thing, or if there is something else going on. This could potentially be tried next week.

We first tried the 'blue box' spare, since it is supposed to be the same (including form factor) as the in-service unit.  We noted that this box has had trouble in the past, but Marc said he'd taken a look and made some fixes, so it should work.  Since that one caused oscillations and had previously been known to be challenging to work with, we tried also the 'silver box' spare, which I think has also been referred to as 'Rev-C'. 

The silver box spare is a different form factor and different front/back panel than the blue box style, but it's supposed to be a drop-in replacement.  There is no space to mount the water-cooled cold block, so if we had left the silver box TTFSS in place, we were just going to leave the cold block hanging around on top of the box, but not mounted to anything.  Also, on the blue boxes, there is a SLOW output on the back panel that goes to a RAMP IN on the front panel.  However, on the silver box that SLOW output is on the front panel, and it needs to be connected to the FAST OUT2 also on the front panel.  Finally, the spigot labeled "PC" on the blue boxes is labeled "EOM" on the silver box.  To install the silver box, you'll also need 2 adapters to go from TNC (on the silver box) to BNC (what the cables are, and what the blue box is), so bring those into the PSL enclosure with you. 

 


Steps from the work permit submitted by Jason:


1)Unlock FSS RefCav.
2)Turn off High Voltage power supply in CER mezzanine.
3)Enter PSL enclosure and disconnect in-service TTFSS box.
4)Install spare TTFSS, hooking the same cables to the same ports on the TTFSS box; turn HV supply back ON.
5)Try to lock RefCav.

If it locks:

6)Measure TF to set common gain for ~500kHz UGF.
7)Measure crossover (use SR785, take a spectrum of IN1 port, crossover is at ~20kHz), set Fast gain to minimize hump in spectrum.

If it will not lock, then follow the same steps above to re-install the in-service TTFSS box.

H1 General
oli.patane@LIGO.ORG - posted 16:42, Thursday 31 October 2024 (80982)
Ops Day Shift End

TITLE: 10/31 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY: Currently relocking and at DARM_TO_RF. Spent most of the day unlocked, with two locklosses and multiple hours of downtime while trying to figure out the FSS issues. Relocking since that work finished has gone great so far.
A couple minutes after Jenne and Betsy left the PSL laser room(and maybe also antetroom), we did notice the FSS PZT have the huge oscillations for about two minutes(attachment), similar to those we had been seeing on the backup FSS boxes(probably alog to come). Jenne is not sure what that means in the case of this FSS box, but mentioned that it might have been due to turning off the air conditioning or something else related to them being in there.
LOG:

14:30 Close to end of an initial alignment
14:40 Initial alignment done, relocking
15:25 NOMINAL_LOW_NOISE
15:32 Observing

16:01 Dropping Observing for Commissioning

16:22 Lockloss
    17:17 Took to DOWN and started manual initial alignment due to DRMI being bad and PRMI ASC having trouble
    17:31 manual IA done, started relocking
18:13 NOMINAL_LOW_NOISE

18:35 Lockloss from little earthquake+low CARM gain actuation range
    18:38 Started an initial alignment
    FSS unlocked due to measurement cable being plugged in and was unlocked for an hour
    20:05 FSS relocked, started manual initial alignment for PRC, MICH, SRC
    20:21 Left manual initial alignment for IDLE for PSL FSS box swap
    22:59 PSL incursion done, started an initial alignment
    23:17 Initial alignment done, relocking                                                                                                                                                                                                                                               

Start Time System Name Location Lazer_Haz Task Time End
15:28 FAC Karen OptLab/VacPrep n Tech clean 15:50
16:02 PEM Robert LVEA n Setting up for injections 16:20
16:28 PSL Sheila, Vicky LVEA n Setting up for measurements 16:37
17:01 FAC Karen WoodShop n Tech clean 18:02
18:41 PSL Jenne, Sheila, Vicky LVEA n Connecting cable for FSS transfer functions 18:59
20:02 ISI Jim HAM Shack n Move measurement equipment 20:40
20:36 PSL Betsy, Jenne PSL Encl y(local) Swapping FSS box 22:58
20:39 EE Fil, Rick, Daniel, Fernando CER, LVEA n Turning off HV, looking at PSL rack layout (Fil out 21:13), Rick out 22:12
20:59   Richard LVEA n Looking at PSL light pipes 21:15
21:03 FAC Tyler CER n Investigating burning smell 21:07
21:16 EE Fil LVEA n Looking at SQZ racks 21:56
21:22 EE Rick, Fil CER n Turn HV back on 21:25
21:48 EE Fil LVEA n Taking other FSS box out to PSL 22:29
21:58 EE Marc LVEA n Helping with FSS box 22:14
21:58   Rick CER n Turning off high voltage 22:12
22:16 EE Rick, Marc CER n Turning HV back on 22:21
22:35 EE Rick, Fil CER n Turnign off HV 22:54
Images attached to this report
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 16:02, Thursday 31 October 2024 (80981)
OPS Eve Shift Start

TITLE: 10/31 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: Oli
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 18mph Gusts, 14mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.80 μm/s
QUICK SUMMARY:

IFO is LOCKING and recovering from CORRECTIVE MAINTENANCE.

To solve some of the PSL/IMC issues, IFO went into maintenance in order to swap out the FSS box. Unfortunately, both spares had PZT oscillations so we had to revert the swap. Attempting to get observing through the weekend until further potential action.

H1 SQZ (GRD)
camilla.compton@LIGO.ORG - posted 15:42, Thursday 31 October 2024 (80980)
ISC_LOCK now takes SQZ_MANAGER to DOWN

Vicky was concerned that the SQZ_SHG stays trying and failing to lock even when the IMC is unlocked. Driving the PZTs unnecessarily and maybe injecting excess light into the fibers.

We edited ISC_LOCK's DOWN to now take SQZ_MANAGER to DOWN and then ISC_LOCK's READY (had to main a main state) to take SQZ_MANAGER to FDS_READY_IFO in.  Previously requested SQZ_MANAGER to FDS_READY_IFO in DOWN.

Also edited SQZ_MANGER's DOWN to take SQZ_SHG and SQZ_PMC to DOWN. Reloaded all guardian. Previously didn't touch them.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 15:26, Thursday 31 October 2024 (80979)
IMC OLG measured

Vicky and I plugged in the 785 to the IMC common mode board.   The first attachment was taken while Oli was trying to lock DRMI, with 10W into the IMC for CHECK_MICH_FRINGES, ugf just over 4kHz.  The second attachment was taken at full lock, nominal low noise, a nearly 80kHz UGF.  This is somewhat higher than in March 76753

Non-image files attached to this report
H1 General
oli.patane@LIGO.ORG - posted 13:44, Thursday 31 October 2024 (80978)
Ops DAY Midshift Status

Detector is currently in IDLE while the FSS box gets swapped in an effort to solve our PSL/FSS issues.

H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 13:43, Thursday 31 October 2024 (80977)
Lockloss

Lockloss @ 10/31 18:35UTC due to small earthquake, high microseism, and low CARM actuation range(80969)

LHO VE
david.barker@LIGO.ORG - posted 10:26, Thursday 31 October 2024 (80971)
Thu CP1 Fill

Thu Oct 31 10:07:19 2024 INFO: Fill completed in 7min 16secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 SQZ
victoriaa.xu@LIGO.ORG - posted 10:18, Thursday 31 October 2024 - last comment - 18:31, Thursday 31 October 2024(80970)
Re-enabled FC beam spot control

We re-enabled FC beam spot control, by enabling inputs to the H1:SQZ-FC_ASC_INJ_ANG_{P,Y} filter banks. Seemed to just work (see attached screenshot) - moves ZM3 to control the spot on the green QPD in filter cavity transmission (SQZ-FC_TRANS_A on SQZT8). Have not yet checked the centering, last done in May 2024 (see 77942 , 6927669374 , 73777).

QPD offsets are set in the FC_ASC_INMATRIX filter banks, last column and row.

I set the flag in sqzparams.py (use_fc_beamspot_control = True), and reloaded SQZ_FC guardian so it will be used in the next locks.

Images attached to this report
Comments related to this report
victoriaa.xu@LIGO.ORG - 18:31, Thursday 31 October 2024 (80984)OpsInfo

Disabled FC beam spot control (use_fc_beamspot_control = False) and loaded SQZ_FC guardian. We can try that again later, beam should be closer to centered now.

FC had a hard time locking in this past lock (ending ~0100 UTC), so that lock didn't have squeezing injected. We first used sliders to set ZMs2-3 and FC1-2 back according to M1_DAMP_{P/Y}_INMONs, to a time during the last lock. FC alignment was still bad with slides set back (bad green tem00 trans, green vco not catching the lock stably).

Then see the attached scope for the QPD alignment that worked. Overall what we should have done: 1) bringing SQZ_MANAGER through DOWN first (I think that fixed something). 2) Setting ZM3+FC1 according to RLF QPDs in HAM7, then set FC2 according to green trans QPD (FC_QPD_TRANS_A) on SQZT8. Biggest move was moving FC2 Y by about +20 on the slider, which is a really big change for this one. With setting SUS back based on top mass osems, then green FC_REFL looked bad, and FC couldn't hand off the IR lock successfully. With the alignment looking good on all QPD's, the FC alignment looks stable (both FC_GR_TRANS and FC_GR_REFL), and I think FC should lock next time.

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 10:18, Thursday 31 October 2024 - last comment - 13:30, Friday 01 November 2024(80969)
CARM gain redistributed again, now limiting range of frequency actuation

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.

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 13:30, Friday 01 November 2024 (80995)

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.

H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 09:24, Thursday 31 October 2024 - last comment - 11:14, Thursday 31 October 2024(80966)
Lockloss

Lockloss @ 10/31 16:01 UTC after almost an hour locked

Comments related to this report
oli.patane@LIGO.ORG - 11:14, Thursday 31 October 2024 (80974)

18:13 Just got to NLN, staying out of Observing for Commissioning

H1 CDS
david.barker@LIGO.ORG - posted 08:46, Thursday 31 October 2024 - last comment - 09:52, Thursday 31 October 2024(80962)
h1seih45 glitch 07:09:46 Thu 31oct2024 PDT

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.

Comments related to this report
oli.patane@LIGO.ORG - 08:59, Thursday 31 October 2024 (80963)

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.

david.barker@LIGO.ORG - 09:16, Thursday 31 October 2024 (80964)

HAM4 and HAM5 GS13 signals following the glitch:

Images attached to this comment
david.barker@LIGO.ORG - 09:41, Thursday 31 October 2024 (80967)
david.barker@LIGO.ORG - 09:52, Thursday 31 October 2024 (80968)

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
 

H1 General (ISC, Lockloss, PSL)
camilla.compton@LIGO.ORG - posted 16:34, Wednesday 30 October 2024 - last comment - 09:28, Monday 11 November 2024(80951)
IMC tagged Locklosses

Reran all O4b locklosses on the locklost tool with the most up to date code, which includes the "IMC" tag.

The locklooss tool tags "IMC" if the IMC looses lock within 50ms of the AS_A channel seeing the lockloss (example plots in 80561).
Note that we don't know that the IMC is causing the lockloss but we are sure that this lockloss is different from the typical lockloss where the IMC loses lock ~250ms after the IFO (seen by AS-port).
Vicky, Sheila and I did some trending this morning and found no conclusions of whats causing the locklosses, we checked that the fast shutter itself isn't causing the lockloss (via HAM6 SEI GS13's) and it seem like in the milliseconds of the lockloss, the AS power decreases and excess power goes to the REFL port.

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:

Images attached to this report
Non-image files attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:49, Thursday 31 October 2024 (80965)ISC, Lockloss

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.

  • In the "NORMAL" lockloss (nearly 100% of locklosses since O4a and O4b before OFI vent):
    • The arm signals (ASC_AS_A/C) increase over 10's ms as the REFL signal decreases.
    • ~250ms later the PSL channels change and the IMC looses lock. 
  • In the "IMC" lockloss (25% of locklosses since OFI vent):
    • The arm signals (ASC_AS_A/C) suddenly (<0.5ms) decrease as the REFL signal increases.
    • At the same time the PSL signals change.
    • <10 ms later the IMC looses lock.
Images attached to this comment
sheila.dwyer@LIGO.ORG - 11:31, Thursday 31 October 2024 (80975)

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.)

camilla.compton@LIGO.ORG - 09:28, Monday 11 November 2024 (81191)

Updated plot attached of NLN locklosses tagged with and without the IMC tag. 

Images attached to this comment
X1 DTS
joshua.freed@LIGO.ORG - posted 13:27, Wednesday 30 October 2024 - last comment - 11:12, Thursday 31 October 2024(80923)
SPI, First step of characterizing double mixer

J. Freed

I followed Step 1 of the double mixer test plan in T2400327 under "1. Characterize frequency references." 

PNSPIDACTestStand.pdf Shows the results in dBc/Hz. And PNSPIDACTestStandrad.pdf shows the result in rad/sqrt(Hz).

Besides the 80MHz standard reference there were 2 devices under test, the IFR 2023A and the SRS SG382. These two devices went under 3 tests involving different combinations of

1. Timing to a 10MHz frequency standard produced by the 80MHz Standard. (Time Standard)

2. PLL locking to a different 80MHz frequency ref through the tune in port. (Lock)

During this process it was assumed that the 80MHz standard and the added 80MHz ref would have a simmilar noise profile as they come from a simmialar OCXO.

A 4th test was added to the Time Standard/No Lock test which used the SR785s internal high pass filter (-3dB at 0.16Hz) to remove some of the DC components from the test. This is because the results of the initial test were inconclusive as the noise floor of the SR785 was too high. The noise floor was too high because there was a DC signal that caused the input range of the SR785 to be about 20dB. The high pass filter, removed the DC signal, lowering the noise floor at the cost of signals below about 0.2Hz not being accurate. We believe this is caused by the fact that while the PLL locking can be controled (tries to lock signals to destructivly interfere so to lower output power for Phase noise tests), there was no control by the Time Standard on phase differences between oscilators. As Time Standard/ No lock, showed the best results above 0.06Hz and is closest to the SPI set up design, this fact may be important when doing futher tests.

Between IFR and SRS, the SRS showed better phase noise performance below 7kHz. While IFR showed better performance above 7kHz. As such, SRS shows more promise in SPIs phase noise range of interest 0-4096Hz.

 

 

Non-image files attached to this report
Comments related to this report
joshua.freed@LIGO.ORG - 11:12, Thursday 31 October 2024 (80972)

After a talk with Jeff what is really important to show is the TIme Standard/Lock which is the 80 MHz OCXO, IFR and SRS which we believe is most represntative of phase noise

These are, one at a time, locked to another 80 MHz REF OCXO. In this it was assumed that the 80 MHz OCXO and the 80 MHz REF OCXO would produce the same phase noise, as such contribute equally to the output phase noise. As such the output was manually halved to represent the only the 80 MHz OCXO. As stated before these measurments also had a Time Standard (sometimes called time sync) where the 80 MHz OCXO is synced to the site's 1PPS. And the IFR and SRS have a 10MHz signal time standard signal that was produced by the 80 MHz OCXO divided by 8 and sent into the back of the devices.

PNSPIDACTestStandrad(sync_lockOnly).pdf Shows only the results of the Time Standard/Lock, which we believe to be the most represntative of the phasenoise of these devices. 

Since it was assumed that the two OCXOs would have the same phase noise, this also makes our noise limit equal the OCXO. As such, it can be seen from this graph that we are at the noise limit in measuring the phase noise of the IFR and SRS between 0.1Hz-10Hz. 

Non-image files attached to this comment
H1 PSL
sheila.dwyer@LIGO.ORG - posted 11:22, Monday 28 October 2024 - last comment - 11:20, Thursday 31 October 2024(80902)
comarison of new and old PSL glitches

Continuing on from Jenne's observation that there are still glitches in the new NPRO, I've tried to make a plot we can use to compare the glitch rate in the new and old NPROs, using the NPRO_PWR channel instead of the FSS channel which isn't available for the new NPRO. 

I've used a 3 hour stretch of observing time for the old NPRO, and a three hour stretch before the time when Jenne made a plot in 80837.  The ISS is not on for the new NPRO time, which is probably why the intensity is flcutuating and making it harder to see the small steps in power that are the glitches we are looking for.  In the second panel, I've plotted the data high passed with a 0.05 Hz butterworth, this helps to show the glitches, although not perfectly (in either case).  Based on this, the glitches look to be happening at a roughly similar rate, although somewhat less with the new NPRO.

This script in in sheila.dwyer/DutyCycle)4/dutycycleplots/PSL_glitches.py

Images attached to this report
Comments related to this report
brian.lantz@LIGO.ORG - 16:04, Monday 28 October 2024 (80906)
sheila.dwyer@LIGO.ORG - 11:42, Monday 28 October 2024 (80903)

Attaching another plot, showing that comparing our old NPRO to LLO during an observing stretch that started at midnight UTC time on Oct7th, LLO has no similar glitches.

Images attached to this comment
sheila.dwyer@LIGO.ORG - 14:26, Tuesday 29 October 2024 (80921)

Here's the same plot, but using a time from last night when the PSL environmental controls were off.  There are still gltiches, but fewer.

Images attached to this comment
victoriaa.xu@LIGO.ORG - 14:23, Wednesday 30 October 2024 (80947)

These plot tiles show runs of Sheila's code looking for PSL power glitches on several days before / after the suspect date around Sept 12.

There's not a clear correlation between the glitches and locklosses. While maybe there's more glitches after Sept 12 (bottom row), the glitches don't consistently correlate with locklosses? Sept 14 is a good example of this: lots of glitches, the IFO stays locked through many of them.

2nd plot here shows overnight again with the swapped new laser. There are still glitches (though potentially less). 

Images attached to this comment
Non-image files attached to this comment
sheila.dwyer@LIGO.ORG - 15:21, Wednesday 30 October 2024 (80948)

The PSL-PWR_NPRO_OUT_DQ channel seems to not be connected at LLO, which explains why the comparison plot a few comments above makes it look like L1 PSL is so much quieter than H1.

victoriaa.xu@LIGO.ORG - 11:20, Thursday 31 October 2024 (80973)

Adding screenshot of the NPRO power glitches over the past day. There are still glitches with the new laser -- not all glitches correspond to locklosses, but some do.

Images attached to this comment
H1 SQZ (DetChar, OpsInfo)
camilla.compton@LIGO.ORG - posted 16:18, Monday 21 October 2024 - last comment - 12:38, Thursday 31 October 2024(80801)
SQZ angle servo using ADF turned on

Sheila, Vicky, Camilla

We have turned back on the SQZ angle servo using the ADF at 322Hz. Last briefly tried while testing ADS alignment in ADS in 80194.  Turned on ADF and used 'python setADF.py -f 322'. Then set H1:SQZ-ADF_OMC_TRANS_PHASE to get H1:SQZ-ADF_OMC_TRANS_SQZ_ANG close to zero and checked by stepping the SQZ angle that there is a zero crossing in the ADF measured SQZ angle, plot attached.

The servo adjusts the SQZ angle (H1:SQZ-CLF_REFL_RF6_PHASE_PHASEDEG) via keeping the ADF measured angle (H1:SQZ-ADF_OMC_TRANS_SQZ_ANG) at zero. Setpoint can be adjusted using the ADF phase (H1:SQZ-ADF_OMC_TRANS_PHASE).

Tagging Detchar:  ADF is now on at 322Hz. It was turned all the way off in 79573 by Alan. We can adjust the frequency 50-500Hz if there is a better place for a line.

Note to operators: if you want to run SCAN_SQZANG, the ADF servo will now overwrite the sqz angle. So BEFORE going back to FREQ_DEP_SQZ  you'll want to tweak H1:SQZ-ADF_OMC_TRANS_PHASE (via sqz overview > ADF) to make H1:SQZ-ADF_OMC_TRANS_SQZ_ANG close to zero. Or you can tweak H1:SQZ-ADF_OMC_TRANS_PHASE (via sqz overview > ADF) until the SQZ BLRMs/ DARM is best.

If this ADF servo works well, it should stop the need for running SCAN_SQZ_ANG as often or we can built this into SCAN_SQZ_ANG.
Images attached to this report
Comments related to this report
victoriaa.xu@LIGO.ORG - 13:08, Tuesday 22 October 2024 (80821)

Trends of the ADF servo stabilizing the SQZ angle overnight. Looks good: the ADF SQZ ANGLE servo can hold the maximum squeezing level throughout the lock! Last night was running with the ADF SQZ angle servo + SQZ-IFO AS42 ASC together.

In the first lock of the screenshot, the ADF SQZ ANGLE servo is not yet running, and the squeezing level drifts quite a bit (~0.5-1 dB in ~2 hours, and ends up un-optimal). In the last 2 locks, the ADF SQZ ANGLE servo is running and successfully stabilizes the SQZ angle, though the 2 locks from last night stabilize at different SQZ angles (weird?). Note SQZ ASC is running in both of these locks, so it seems like ASC + ADF SQZ ANG servo work well when used together.

Naoki looked at sqz trends with/without the ADF servo before in LHO:75000. Looking at sqz trends for yesterday, the ADF servo stabilized the SQZ angle in the first ~25 minutes. Then over the first ~2 hours, the ADF servo needed to move the CLF_RF6 demod phase by 5-10 degrees to hold the SQZ angle stable. This implies something like, the optimal injected squeezing angle changed by about 2-5 degrees during IFO thermalization.

Also noting a reference to LHO:77292, where Naoki does an On/Off test with the ADF line at 322 Hz.

Images attached to this comment
camilla.compton@LIGO.ORG - 12:38, Thursday 31 October 2024 (80976)

Checked against the 68139 list, can see that 322Hz is a good frequency for CW. We will look at trying to add this ADF line to the _CLEAN or _NOLINES subtractions. 

Displaying reports 501-520 of 79139.Go to page Start 22 23 24 25 26 27 28 29 30 End