Displaying reports 9281-9300 of 84071.Go to page Start 461 462 463 464 465 466 467 468 469 End
Reports until 06:12, Tuesday 09 April 2024
H1 CDS
david.barker@LIGO.ORG - posted 06:12, Tuesday 09 April 2024 - last comment - 10:48, Wednesday 10 April 2024(77040)
h1omc0 channel hop caused dolphin glitch of SUS and LSC

Oli, Erik, Dave:

Around 04:30 this morning a ADC channel hop on h1iopomc0 caused all of the omc0 models to stop running, and also caused a corner station Dolphin glitch which DACKILLED h1susb123, h1sush34, h1sush56 and h1lsc0.

Comments related to this report
david.barker@LIGO.ORG - 06:14, Tuesday 09 April 2024 (77041)

h1omc0 dmesg:

[Tue Apr  9 04:34:05 2024] rts_cpu_isolator: LIGO code is done, calling regular shutdown code
[Tue Apr  9 04:34:05 2024] h1iopomc0: ERROR - A channel hop error has been detected, waiting for an exit signal.
[Tue Apr  9 04:34:05 2024] h1omcpi: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
[Tue Apr  9 04:34:05 2024] h1omc: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
 

david.barker@LIGO.ORG - 06:22, Tuesday 09 April 2024 (77042)

Initially I thought this was an IO Chassis issue, so we power cycled h1omc0 rather than a restart all of its models (my confusion was because this front end only has one Adnaco, and is running the low-noise ADC). This brought h1omc0 back up and running.

We restarted the models on h1lsc0, which cleared the DACKILL.

Oli put the SUS and SEI for BSC1,2,3 and HAM3,4,5,6 into safe, I SWWD bypassed the SEI IOPs  and we restarted the models on h1susb123, h1sush34, h1sush56. All came back with no problems.

I cleared the SWWDs, did a DIAG_RESET and cleared the DAQ CRCs.

Handing over to Oli for IFO recovery.

david.barker@LIGO.ORG - 06:35, Tuesday 09 April 2024 (77043)

CDS Overview after DIAG_RESET run on all front ends:

Images attached to this comment
david.barker@LIGO.ORG - 06:39, Tuesday 09 April 2024 (77045)

Time of OMC crash:

04:32:45 PDT

11:32:45 UTC

1396697583 GPS

david.barker@LIGO.ORG - 10:48, Wednesday 10 April 2024 (77089)
H1 General (CDS)
ryan.crouch@LIGO.ORG - posted 23:59, Monday 08 April 2024 - last comment - 05:29, Tuesday 09 April 2024(77036)
OPS Monday eve shift summary

TITLE: 04/09 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 134Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:
LOG: We stayed locked the whole shift, almost 11 hours as of 07:00UTC. Rode through a 6.0.

The range has been lower tonight, it got a little worse after the SQZer relocked itself. Low frequency noise was esp high.

I noticed in the last hour or so of the shift that there were 3 FEs with CRC errors, H1IOPSUSH2B, H1SUSIM, AND H1SUSHTTS (Tagging CDS)

Comments related to this report
keith.thorne@LIGO.ORG - 05:29, Tuesday 09 April 2024 (77038)
Those are three processes from the same computer (H1SUSH2B).  There is only a single data packet sent from each front-end to the DAQ.

I might be more concerned about the red indicators on many front-ends on the CPU overview screen
H1 General
ryan.crouch@LIGO.ORG - posted 20:05, Monday 08 April 2024 - last comment - 10:33, Tuesday 09 April 2024(77034)
OPS Monday eve shift update

We've been locked for 6:50, range is lower tonight

A 6.0 from Indonesia rolled through around 00:38 UTC

Comments related to this report
ryan.crouch@LIGO.ORG - 21:23, Monday 08 April 2024 (77037)SQZ

SQZer lost lock and dropped us from observing at 04:22, will return once it relocks. Back into observing at 04:26UTC

camilla.compton@LIGO.ORG - 10:33, Tuesday 09 April 2024 (77054)SQZ

This lockloss was due to the OPO PZT running out of range @40V, plot. There's already a checker in SQZ_MANGER to relock when IFOs unlocked and OPO PZT1 is below 50V but it was at 70V when the IFO locked.

Images attached to this comment
H1 ISC (SQZ)
jennifer.wright@LIGO.ORG - posted 17:04, Monday 08 April 2024 (77033)
Tuning CAM2 YAW offset makes build-ups better

Jennie W, Sheila, Ryan Short

 

After tuning the CAM1 PIT offset this morning and optimising the A2L gains after that, I tuned down the CAM2 YAW offset just before we went into observing. I chose this direction based on the overnight tests Camilla and I did. In the attached picture the cursor shows where the optimum offset is that improves the circulating arm powers. At each stage I had to wait about 2 minutes for the camera servo to bring the error point (IN1 channel) to the set-point.

The optimum value which increased the build-ups by about 6kW (OFFSET = -422) was set in the guardian (via updating the CAM YAW2 offset in userapps/isc/h1/guardian/lscparams.py) and accepted and monitored in SDF. I loaded the ISC_LOCK and CAMERA_SERVO guardians and made the SDF changes before we went into observing. We still need to optimise the A2L gains to match this change so the noise might not be better.

For reference I include a more comprehensive ndscope with all the channels I was monitoring as we did this.

Images attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 16:50, Monday 08 April 2024 (77030)
Tuninng A2L gains

Jennie W, Sheila

We wanted to inject into individual optics to optimise A2L gains today.

This was because we worried that the CHARD and DHARD injections we made on Friday to evaluate our ITM yaw A2L gains mean that we are moving our ETMs to cancel out the noise on our ITMs.

We injected into the channels of the form H1:SUS_{ETMX,ITMX,ITMY}_L2_LOCK_{Y,P}_EXC.

Today we tuned ETMX Y2L, ITMX P2L, ITMY P2L.

The green traces were measured with the new better value and the blue shows the reference value before injecting. We managed to get gains which decreased the transfer function of that test mass motion to DARM. Although it can be seen from the plots of coherence that the coherence was very small for our injections which might imply that there was some non-linear coupling at the frequencies we injected at.

The starting values are in this image and we changed them to these values.
 

This means we have finished retuning the camera servo that keeps the spot on the beam splitter constant (CAM1).

We need to retune the camera offsets for servo 2 which moves ITMX and ETMX to keep the spot on ETMX, and then retune the ETMX A2L gains for this new value.

We also still need to retune the camera offsets for servo 3 which moves ITMY and ETMY to keep the spot on  ETMY, and then retune the ETMY A2L gains for this new value.

Images attached to this report
H1 SQZ
eric.oelker@LIGO.ORG - posted 16:49, Monday 08 April 2024 (77029)
Alternate SCRL Detuning worse for SQZ -> Nominal settings restored

Naoki, Eric

Based on the FIS measurements in 77023, we thought that it was worth taking a look at the FDS for H1:LSC-SRCL_OFFSET1 = -275.  Unfortunately, we are unable to see any improvement in DARM relative to our nominal SRCL detuning.  We tried two SQZ angles chosen to optimize for mid-band and high freq squeezing respectively.  We did not have time to try tweaking the FC detuning, but we don't think it makes sense for this to be a FC detuning issue alone.  We were concerned that we might be fooling ourselves since the ifo had come unlocked early in the afternoon, so we checked the FIS trace again and it looked identical to earlier in the day.

We have reverted back to H1:LSC-SRCL_OFFSET1 = -175 for the observing period.

We have realized that our approach of optimizing the FIS spectrum for high frequency squeezing and looking for flatness was error prone.  We erroniously assumed that a reduction in low frequency RPN was desireable because it resulted in a flatter spectrum in the mid band and chose H1:LSC-SRCL_OFFSET1 = -275 accordingly.  In fact, we were adding an undesireable frequency dependent rotation with an unoptimal SRCL detuning which was rotating our injected squeezing away from driving RPN at low frequencies.    In the future, we will optimizing FIS for mid-band squeezing and attempt to tune the SRCL offset to flatten out the spectra at high and low frequencies (ie, eliminate any v-shape in the mid-band optimized FIS spetra).

New Datasets (all for H1:LSC-SRCL_OFFSET1 = -275) :

 

 

 

Images attached to this report
LHO General
jonathan.hanks@LIGO.ORG - posted 16:34, Monday 08 April 2024 (77032)
WP 11790 2fa system updated
As WP 11790 I updated the OS and 2fa software on 2fa.ligo-wa.caltech.edu.  I ended up doing upgrade here before doing the work at LLO.
H1 ISC (SQZ)
jennifer.wright@LIGO.ORG - posted 16:30, Monday 08 April 2024 (77031)
No SQZ Measurements

Jennie W, Sheila

Camilla grabbed some NO SQZ time this morning and I compared it to our O4a measurement of NO SQZ time.

Both samples are roughly ten minutes.

DTT template is saved in /ligo/home/jennifer.wright/Documents/Noise_DARM/20240408_DARM_comp_sqz_no_sqz2.xml

The grey is O4a and red is today.

It can be seen that the 50-500Hz excess noise seems to be gone and we are doing better than O4a between 10 and 40 Hz and above 800 Hz.

We want to tackle the bump of lines around 25 Hz which may come from modes of the triple suspension.

Images attached to this report
LHO General
ryan.short@LIGO.ORG - posted 16:06, Monday 08 April 2024 (77022)
Ops Day Shift Summary

TITLE: 04/08 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1:
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY: Mostly quiet day with good commissioning opportunities and only one lockloss.

H1 has now been locked for almost 3 hours.

LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:26 SQZ Camilla, Eric CR - No SQZ time 15:52
17:04 FAC Kim MX - Technical cleaning 17:47
17:11 FAC Chris MX - Picking up cable trays 18:24
21:10 SQZ Julian, Camilla Opt Lab Local SHG work Ongoing
H1 General
ryan.crouch@LIGO.ORG - posted 15:57, Monday 08 April 2024 - last comment - 16:06, Monday 08 April 2024(77027)
OPS Monday eve shift start

TITLE: 04/08 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 12mph Gusts, 10mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.20 μm/s
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 16:06, Monday 08 April 2024 (77028)

Into Observing at 23:06UTC

H1 SQZ
camilla.compton@LIGO.ORG - posted 12:49, Monday 08 April 2024 - last comment - 18:35, Monday 08 April 2024(77023)
SQZ and SRCL tuning Measurements

Eric, Sheila, Jennie, Naoki, Camilla

Aiming to repeat 68814 O4a FIS SQZ, SCRL offset data set. Nominal H1:LSC-SRCL1_OFFSET = -175, previously looked at in 74373.

Measured NLG =16.86  (following 76542). Adjusted OPO temperature 31.481 to 31.470.
PZT1 is locked around 70V, which isn't our favorite place, we're seen SQZ is better when it locks at nearer 100V.

Using data from our PSAMS scan 76986, we're set ZM4 to 8.8V (175 offset), leaving ZM5 with -0/7V (100 offset). Reran alignment scripts following 76986. Accepted PSAMs sdf, and alignment sliders.

For FIS took SQZ_MANGER to AUTO to stop ISC_LOCK bringing it to FDS.

PSAMs at 8.8/-0.7

  • 15:23:30 - 15:42:00UTC  No SQZ time
  • 16:04:45 - 16:10:00UTC FDS SQZ
  • 16:13:00 - 16:21:30UTC FIS SRCL1_OFFSET -175, SCAN_SQZANG tuned to 350Hz: 193deg CLF Phase
  • 16:30:20 - 16:36:00UTC FIS SRCL1_OFFSET -225,  hand tuned SQZ angle to 2kHz: 208deg CLF Phase
  • 16:39:00 - 16:45:00UTC FIS SRCL1_OFFSET -275,  hand tuned SQZ angle to 2kHz: 212deg CLF Phase
  • 16:49:00 - 16:54:30UTC FIS SRCL1_OFFSET -325,  hand tuned SQZ angle to 2kHz: 217deg CLF Phase
  • 16:57:30 - 17:04:00UTC FIS SRCL1_OFFSET -375,  hand tuned SQZ angle to 2kHz: 223deg CLF Phase
  • 17:07:00 - 17:12:30UTC FIS SRCL1_OFFSET -425,  hand tuned SQZ angle to 2kHz: 228deg CLF Phase
  • 17:13:10 - 17:18:30UTC  No SQZ time (to check for SRCL offset causing technical noise but DARM looks the same as previous)
  • 17:25:30 - 17:31:30UTC FIS SRCL1_OFFSET -175, hand tuned SQZ angle to 2kHz: 192deg CLF Phase
  • 17:35:00 - 17:41:00UTC FIS SRCL1_OFFSET -125, hand tuned SQZ angle to 2kHz: 186deg CLF Phase
  • 17:43:00 - 17:48:30UTC FIS SRCL1_OFFSET -75, hand tuned SQZ angle to 2kHz: 168deg CLF Phase

Data with different angles (+/-10deg from SQZ and ASQZ, and +/- midsqz aimed to match no SQZ level) with SRCL1_OFFSET -175. Plot attached.

  • 17:59:30 - 18:04:30UTC FIS SRCL1_OFFSET -175, 192deg CLF Phase
  • 18:05:30 - 18:10:30UTC FIS SRCL1_OFFSET -175, 182deg CLF Phase
  • 18:11:20 - 18:16:30UTC FIS SRCL1_OFFSET -175, 202deg CLF Phase
  • 18:18:30 - 18:23:30UTC FIAS SRCL1_OFFSET -175, (neg sign) 108deg CLF Phase
  • 18:24:35 - 18:29:40UTC FIAS SRCL1_OFFSET -175, (neg sign) 98deg CLF Phase
  • 18:30:00 - 18:35:00UTC FIAS SRCL1_OFFSET -175, (neg sign) 118deg CLF Phase
  • 18:41:00 - 18:46:00UTC FIMS SRCL1_OFFSET -175, 140deg CLF Phase (-Mid SQZ aimed to match no SQZ level)
  • 18:55:00 - 19:00:00UTC FIMS SRCL1_OFFSET -175, 220deg CLF Phase (+Mid SQZ aimed to match no SQZ level)

Data with different angles (+/-10deg from SQZ and ASQZ) with SRCL1_OFFSET -275.

  • 19:10:30 - 19:15:30UTC FIS SRCL1_OFFSET -275, 207deg CLF Phase
  • 19:16:00 - 19:21:00UTC FIS SRCL1_OFFSET -275, 197deg CLF Phase
  • 19:21:30 - 19:24:00 [glitch] 19:24:35 - 19:27:40UTC FIS SRCL1_OFFSET -275, 217deg CLF Phase
  • Lockloss before completing data set
Images attached to this report
Comments related to this report
eric.oelker@LIGO.ORG - 13:53, Monday 08 April 2024 (77026)

Additional plots for data above:

  • SRCL_TUNE_FIS_2.png:  This shows how FIS changes as a function of SRCL detuning (-175 is our current nominal value).  We see that when increasing the SRCL detuning, we initially see significant improvement at lower frequencies with a slight rise in midband.
  • SRCL_TUNE_FIS_3.png:  This shows how FIS changes as we change the SRCL detuning in the other direction.  Everythihng appears to get worse.

Note:  As a sanity check, we took another NoSQZ trace at H1:LSC-SRCL1_OFFSET = -= -425 and saw that it looked idential to NoSQZ at H1:LSC-SRCL1_OFFSET = -175. 

After looking at this scan, we were wondering if H1:LSC-SRCL1_OFFSET = -275 might be a more optimal operating point than H1:LSC-SRCL1_OFFSET = -175.  We decided to do a few more FIS measurements at the two candidate operating points:

  • FIS_SRCL_neg175.png (Attached above in Camilla's post): shows FIS, FIAS and FIMid Squeezing and nearby squeezing angles for a H1:LSC-SRCL1_OFFSET = -175
  • VARY_SQZANG_SRCL_275 shows FIS and +/- 10 degrees for H1:LSC-SRCL1_OFFSET = -275.  Unfortunately we lost lock before taking the remaining points.

After rethermalizing, we plan to look at FDS at H1:LSC-SRCL1_OFFSET = -275 and perhaps tweak the filter cavity a bit to see if this SRCL detuning is better or worse in terms of range. 

Images attached to this comment
eric.oelker@LIGO.ORG - 18:35, Monday 08 April 2024 (77035)

An alternate version of one of the plot from the original post. A few intetrmediate traces are removed and replaced w reference FDS and No SQZ traces.  

Images attached to this comment
H1 ISC (ISC)
jennifer.wright@LIGO.ORG - posted 11:59, Monday 08 April 2024 (77025)
Optimising Build-ups with CAM PIT OFFSET

Sheila, Jennie W

 

Sheila and I changed H1:ASC-CAM_PIT1_OFFSET down and went through a point which increased the build-ups in the arms.

She has added this camera offset to guardian.

CAM1 is the servo which moves the PRM to keep the spot constant on the beamsplitter.

See Sheila's pic showing where the best offset is.

We are planning to optimise the A2L gains for each ITM and ETM after this.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:22, Monday 08 April 2024 (77024)
Mon CP1 Fill

Mon Apr 08 10:08:37 2024 INFO: Fill completed in 8min 34secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 08:29, Monday 08 April 2024 (77021)
PSL 10-Day Trends

FAMIS 20023

The PSL was taken down 6 days ago for a Beckhoff update (alog76879), which is seen on several trends.

After that, the PMC seems to have locked with lower transmission by almost 1W.

Images attached to this report
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